෺ཧ‫ࣨڭ‬೥࣍ใࠂॻ
ฏ੒̎̑೥౓

̎̌̍̐೥݄̏
‫۝‬भେֶେֶӃཧֶ‫ڀݚ‬Ӄ෺ཧֶ෦໳

໨࣍

͸͡Ίʹ

1

ฏ੒̎̑೥౓ͷ‫ڀݚ‬ςʔϚͱ੒Ռ
ૉཻࢠཧ࿦

2

ཧ࿦֩෺ཧ

12

Ӊ஦෺ཧཧ࿦

39

ૉཻࢠ࣮‫ݧ‬54‫ݧ࣮֩ࢠݪ‬

79

෺ੑཧ࿦

93

౷‫ܭ‬෺ཧֶ

102‫ڽ‬ॖ‫ܥ‬ཧ࿦

109

࣓ੑ෺ཧֶ

113

ྔࢠඍগ෺ੑ

122‫ݻ‬ମిࢠ෺ੑ

126

௿࣍‫ࢠిݩ‬෺ੑ

132ෳࡶ෺ੑ‫ૅج‬

136

ෳࡶྲྀମ

153

٬һ‫ڭ‬त

161‫ڭ‬৬һҰཡ

162

֤छҕһҰཡ

163

෺ཧֶ‫ࣨڭ‬ஊ࿩ձ

164෺ཧֶ‫ࣨڭ‬ਫ༵໦༵ஊ࿩ձ

166

෺ੑ‫ૅج‬࿦ίϩΩϡ΢Ϝ

168‫۝‬େ‫֩ࢠݪ‬ηϛφʔ

170

ඇৗ‫ࢣߨۈ‬Ұཡ

172֎ࠃਓ‫ऀڀݚ‬౳डೖ‫ه‬࿥173‫ڭ‬ҭ՝ఔҕһձ‫׆‬ಈใࠂ

174෺ཧֶ෦໳ϑΝΧϧςΟ· σϕϩοϓϝϯτใࠂ

175ೖֶऀ਺ͱଔ‫਺ऀۀ‬176

ब৬ · ਐֶ৘‫گ‬177ମ‫ݧ‬ೖֶ · ެ։ߨ࠲ใࠂ

178

ࣾձ‫׆‬ಈߩ‫ݙ‬ใࠂ

180ࡣࡌࡵ࡟
ᮏሗ࿌᭩ࡣ≀⌮ᩍᐊ࡜ྛ◊✲ᐊࡢ㸰㸮㸯㸱ᖺᗘࡢάືグ㘓ࢆࡲ࡜ࡵࡓࡶࡢ࡛ࡍࠋࡇࡇ࡛ࡣࠊ
≀⌮ᩍᐊ඲య࡟㛵ࢃࡿࡇ࡜ࢆ⡆༢࡟ሗ࿌࠸ࡓࡋࡲࡍࠋ
ࡲࡎᩍဨࡢ␗ື࡟ࡘ࠸࡚ሗ࿌ࡋࡲࡍࠋ㸲᭶࡟ᮌᮧ㸦ᓫ㸧ᩍᤵ࡜᳃⏣ᩍᤵࡀ╔௵ࡋࡲࡋࡓࠋࡉ
ࡽ࡟㸷᭶࡟ࡣ㕥ᮌᩍᤵ࡜኱すຓᩍࠊ㸯㸮᭶࡟ࡣᑠ㔝ຓᩍ࡜ᮎཎຓᩍࡀ╔௵ࡋࡲࡋࡓࠋ㸲᭶࡟ඛ➃⣲⢏Ꮚ≀⌮◊✲ࢭࣥࢱ࣮࡟╔௵ࡋࡓྜྷᒸ෸ᩍᤵ㸦≀⌮Ꮫ㒊㛛ຓᩍ࠿ࡽ᪼௵㸧࡜㡢㔝ຓᩍࡣࠊ≀⌮ᩍᐊࡢ୍ဨ࡜ࡋ࡚ࡶάືࡋ࡚࠸ࡲࡍ㸦⌮Ꮫᗓ࣭⌮Ꮫ㒊ᢸᙜ㸧ࠋࡲࡓࠊᇶᖿᩍ⫱㝔ࡢ኱Ἑෆ෸ᩍᤵࡶ㸯㸯᭶࠿ࡽ⌮Ꮫᗓᢸᙜ࡟࡞ࡾࡲࡋࡓࠋࡑࡢ୍᪉࡛ࠊὸ㔝ຓᩍࡀᖺᗘᮎ࡟⚟஭኱Ꮫ෸ᩍᤵ࡟㌿ฟࡉࢀࡲࡋࡓࠋ
ᣍ⪸ே஦࡟ࡼࡾ╔௵ࡋࡓᮌᮧ㸦ᓫ㸧ᩍᤵࡣ╔௵᪩ࠎᇶ┙◊✲ 6 ࢆ⋓ᚓࡋ࡚୺ᖿᩍᤵ࡜࡞ࡾࠊ
ࠕ㔞Ꮚࢼࣀࢫࣆࣥ≀ᛶ◊✲ࢭࣥࢱ࣮ࠖࢆタ⨨ࡍࡿࡇ࡜࡟࡞ࡾࡲࡋࡓ㸦㸰㸮㸯㸲ᖺᗘ࠿ࡽ㸧ࠋྠ୺ᖿᩍᤵࡣ㸰㸮㸯㸱ᖺࡢ᪥ᮏᏛ⾡᣺⯆఍㈹ࡶཷ㈹ࡉࢀ࡚࠾ࡾࠊ௒ᚋࡢ≀ᛶ≀⌮Ꮫㅮᗙࡢ୺ᰕ
࡜ࡋ࡚ࡢά㌍ࡀᮇᚅࡉࢀࡲࡍࠋ
⌮Ꮫ◊✲㝔ࡢ୰࡛≀⌮Ꮫ㒊㛛ࡔࡅࡀ㸰㸮㸮㸷ᖺᗘ࠿ࡽຓᩍࡢ௵ᮇไࢆ᥇⏝ࡋ࡚࠾ࡾࠊ㸰㸮㸯㸰ᖺᗘࡲ࡛࡟᥇⏝ࡋࡓ᪉ࡣ᭱ึࡢ௵ᮇࡀࡃࡿ㸯ᖺ๓࠿ࡽ෌௵ᑂᰝࢆ⾜࡞࠺ࡇ࡜࡟࡞ࡗ࡚࠸ࡲ
ࡍ㸦㸳ᖺ௵ᮇ࣭෌௵㸯ᅇ㸧ࠋ௒ᖺᗘࡣึࡵ࡚㸲ྡࡢຓᩍࡢ෌௵ᑂᰝࢆ⾜࠸ࠊࡳ࡞ࡉࢇ㧗࠸ホ౯࡛෌௵ࡀㄆࡵࡽࢀࡲࡋࡓࠋ࡞࠾ࠊປാዎ⣙ἲࡢᨵṇࢆཷࡅ࡚ࠊ௒ᖺᗘ᥇⏝ࡉࢀࡓຓᩍࡢ௵ᮇ
ࡣ㸳ᖺ࣭෌௵୙ྍ࡟࡞ࡾࡲࡋࡓࠋࡋ࠿ࡋࠊࡑࡢᚋປാዎ⣙ἲࡢ≉౛ᨵṇἲ᱌ࡀㄆࡵࡽࢀࡓࡇ
࡜࠿ࡽࠊຓᩍࡢ௵ᮇไࢆࡶ࠺୍ᗘぢ┤ࡍࡇ࡜࡟࡞ࡿ࡛ࡋࡻ࠺ࠋ
⚾ࡀ஑ᕞ኱Ꮫ࡟╔௵ࡋ࡚࠿ࡽ㸱ᖺ࡟࡞ࡾࡲࡍࠋࡑࡢ㛫࡟࠿࡞ࡾࡢᩍဨࡀධࢀ᭰ࢃࡾࠊㅮᗙ࣭
◊✲ᐊࡢᵓᡂࡶ኱ࡁࡃኚ໬ࡋ࡚ࡁࡲࡋࡓࠋ㸰㸮㸯㸲ᖺᗘ࠿ࡽᇶᖿᩍ⫱㝔ࡀᮏ᱁ⓗ࡟ືࡁฟࡋ
ࡲࡍࠋࡑࡋ࡚ࠊ᮶ᖺኟ࡟ࡣࠊ⌮Ꮫ◊✲㝔ࡀఀ㒔࢟ࣕࣥࣃࢫ࡬⛣㌿ࡋࡲࡍࠋࡇࡢࡼ࠺࡞⃭ືࡢ᫬ᮇ࡟࠶ࡾࡲࡍࡀࠊ◊✲࣭ᩍ⫱ࡢ㉁ࢆࡉࡽ࡟㧗ࡵ࡚࠸ࡃࡼ࠺ࠊ≀⌮ᩍᐊ඲య࡛ບࢇ࡛࠸ࡁࡓ
࠸࡜⪃࠼࡚࠾ࡾࡲࡍࠋ
≀⌮ᩍᐊࡢ᝟ሗࡣࠊ࢙࢘ࣈࢧ࢖ࢺ࡟ࡶࡈࡊ࠸ࡲࡍࡢ࡛ࠊేࡏ࡚ࡈぴࡃࡔࡉ࠸ࠋ
KWWSZZZSK\VN\XVKXXDFMS㸰㸮㸯㸲ᖺ㸱᭶≀⌮Ꮫ㒊㛛 㒊㛛㛗 ᕝ㉺Ύ௨ૉཻࢠཧ࿦
‫ߏࣨڀݚ‬੒һ‫ڭװج( ࢘߃ాݪ‬ҭӃ) ‫ڭ‬तླ໦ത ‫ڭ‬तେՏ಺๛ (‫ڭװج‬ҭӃ) ।‫ڭ‬तԞଜ݈Ұ ॿ‫ڭ‬ େֶӃ ത࢜՝ఔ ‫ٱ‬อ޾‫و‬

٢ຊҰੈ

຀໺޿थ

ਫ‫୓ޱ‬໵

ߴ‫ژڮ‬େ

෢ాେయ େֶӃ म࢜՝ఔ ‫ྒྷాݪ‬ฏ
৿ຊޫࢁ‫࢘ݡޱ‬ถຊོ༟ ֶ෦ ଔ‫ڀݚۀ‬ੜ 
஛ቌஐ೭

౻ࢁᠳ೫

౻ࢁ༏Ұ

Ҫ্‫ࡾݚ‬

খౡ݈ଠ࿠ (‫ڭװج‬ҭӃ) ๚໰‫ ऀڀݚ‬‫ٱ‬อത࢙

ాඌपҰ࿠ (‫ڭװج‬ҭӃ)๛ాจ඙୲౰त‫ۀ‬
෺ཧֶ‫ૅج‬ԋश (Ԟଜ݈Ұ)ɺղੳྗֶɾಉԋश (‫࢘߃ాݪ‬ɾԞଜ݈Ұ)ɺྔࢠྗֶ II (‫ݪ‬ా߃࢘)ɺૉཻࢠ෺ཧֶ (ླ໦ത)ɺ෺ཧֶಛผ‫ ڀݚ‬IɾII (Ԟଜ݈Ұ)ɺ৔ͷྔࢠ࿦ (‫ాݪ‬߃࢘)ɺM1 θϛφʔϧ (‫)࢘߃ాݪ‬‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ
௒‫ݭ‬ཧ࿦ʹஔ͚ΔΞϋϩϊϑϘʔϜ์ࣹ (େՏ಺๛)௒‫ݭ‬ཧ࿦ͷίϯύΫτԽʹΑΔελϯμʔυϞσϧͷߏ੒Ͱ͸ɺ͠͹͠͹σΟεΫϦʔτରশੑ͕෇ਵ͢Δɻ࠷ۙͷ Banks–Seiberg ʹΑΔٞ࿦ʹΑΕ͹ɺͦ͏ͨ͠σΟεΫϦʔτରশੑ͸ήʔδԽ͞Ε͍ͯΔඞཁ͕͋Δɻͦͷ৔߹ɺؔ࿈ͯ͠Ӊ஦ඥ͕ੜ੒͞
Εॳ‫ظ‬Ӊ஦ͷίϯύΫτԽͷ৘ใΛर͍ग़ͤΔՄೳੑ͕͋Δ͜ͱΛΞϋϩϊϑϘʔϜޮՌΛ༻͍ͯࣔͨ͠ɻ‫ࡏݱ‬ͷ‫؍‬ଌ݁ՌΛ༻͍Δͱɺ͋ΔछͷίϯύΫτԽ͸‫͞ڐ‬Εͳ͍ࣄΛࣔͨ͠ɻ

2

R-ΞΫγΦϯͱӉ஦࿦త੍‫( ݶ‬େՏ಺๛)४҆ఆঢ়ଶΛ༻͍ͨ௒ରশੑͷഁΕͷϞσϧ͸ɺۙ೥஫໨͞Ε͍ͯΔɻϞσϧͷߏ੒Λ༰қʹ͢Δ͏͑ʹɺ‫Ͱ఺࣌ݱ‬ͷίϥΠμʔͷ࣮‫݁ݧ‬Ռͱ΋ໃ६͠ͳ͍ɻ௒ରশੑͷϞσϧʹಛ༗ͷ R ରশੑʹண໨͠ɺͦͷഁΕʹ൐͏ιϦτϯ͕४҆ఆঢ়ଶͷण໋ʹඇৗʹॏཁͰ͋Δ͜ͱΛࢦఠ͠ɺ‫ط‬ଘͷϞσϧʹؔͯ͠ͷ੍‫ݶ‬Λ෇͚ͨɻ௒ରশੑͷഁΕͷ mirage mediation ʹ͓͚Δ Next-to-Minimal SupersymmetricStandard Model (NMSSM) ͷ‫ݱ‬৅࿦తղੳ (Ԟଜ݈Ұɺ຀໺޿थ)LHC ࣮‫ ͍͓ͯʹݧ‬125GeV ͷ࣭ྔΛ࣋ͬͨ Higgs ཻࢠΒ͖͠৽ཻࢠ͕ൃ‫͞ݟ‬ΕͨɻҰํͰ௒ରশཻࢠͷஹީ͸‫ݟ‬ΒΕͣɺͦͷ࣭ྔԼ‫ݶ‬͸ 1TeV Λӽ͑࢝Ίͨɻ͜ͷΑ͏ͳঢ়‫گ‬Λ౿·͑ɺLHC ͷ݁ՌΛࣗવʹઆ໌Ͱ͖Δ໛‫ܕ‬ͷߏஙΛ໨ඪʹ‫ڀݚ‬Λߦͬͨɻࡢ೥౓ʹҾ͖ଓ͖ TeV scale mirage mediation ʹ͓͍ͯ MSSM ʹҰॏ߲৔Λಋೖͨ͠ NMSSM
Λߟ࡯ͨ͠ɻࡢ೥౓ͷ‫͍͓ͯʹڀݚ‬ɺHiggs ཻࢠͷ࣭ྔΛ‫؍‬ଌ͞Ε͍ͯΔ 125GeV ·Ͱ্͛Δ͜ͱ͕ग़དྷΔࣄɺNMSSM ೋॏ߲ͱҰॏ߲ͷؒͷࠞ߹͕ࣗಈతʹ཈੍͞ΕΔ
͜ͱ͕਺஋‫ࢉܭ‬ͷ݁Ռ͔Β໌Β͔ʹͳ͍͕ͬͯͨɺࠞ߹ͷ཈੍ͷ෺ཧతͳഎ‫͕ܠ‬શ͘ཧղ͞Ε͍ͯͳ͔ͬͨɻຊ೥౓ͷ‫ʹڀݚ‬ΑΓɺTeV scale mirage mediation ʹ͓͍ͯ͸

NMSSM ໛‫͕͋ܕ‬Δ‫Ͱݶۃ‬εέʔϧม‫ʹ׵‬ର͢ΔෆมੑΛ΋͓ͬͯΓɺώοάε৔͕ਅۭ‫ظ‬଴஋Λ࣋ͭ͜ͱʹΑΓ͜ͷෆมੑ͕ഁΕΔ͜ͱ͕ཧղ͞Εͨɻͭ·Γɺώοάεཻࢠ͸͜ͷରশੑʹରٖͯ͠ೆ෦ΰʔϧυετʔϯ৔ͱͯ͠ৼΔ෣͏ͨΊҰॏ߲ͱͷࠞ߹͸εέʔϧม‫׵‬Λ໌ࣔతʹഁΔখ͞ͳύϥϝʔλʹΑΓ཈੍͞ΕΔɻ͜ͷࠞ߹ͷ཈੍ͷͨΊඪ४ཧ࿦‫ܕ‬ͷώοάεཻࢠҎ֎ͷεΧϥʔཻࢠ͸ 200GeV ఔ౓ҎԼͱ͍ܰʹ΋ؔΘΒͣ LHC ͔ΒӅ͞Ε͓ͨΓɺࠃࡍϦχΞίϥΠμʔ (ILC) ʹΑΔਫ਼ີଌఆͷ֨޷ͷඪతͱͳΔɻຊ‫ڀݚ‬੒Ռ͸ࡢ೥౓ͷ੒Ռͱ‫ࡏݱʹڞ‬࿦จʹ·ͱΊ͓ͯΓɺग़
൛·Ͱͷ࠷ऴஈ֊ʹ͋Δɻ

TeV εέʔϧϛϥʔδϡഔհ໛‫΁ܕ‬ͷ LHC ʹΑΔ௚઀୳ࡧ͔Βͷ੍‫( ݶ‬Ԟଜ݈Ұɺࢁ‫)࢘ݡޱ‬

TeV scale mirage ഔհ໛‫ܕ‬͸ॏ͍௒ରশཻࢠͱ͍ܰώοάεཻࢠΛগͳ͍ඍௐ੔ʹΑΓ࣮‫ݱ‬ग़དྷΔ‫ر‬༗ͳ௒ରশੑͷഁΕͷഔհ‫͋Ͱߏػ‬Δ͕ɺLHC ͷ௚઀୳ࡧ࣮‫ʹݧ‬ΑΓͲͷఔ౓੍‫͞ݶ‬Ε͍ͯΔ͔Λௐ΂ͨྫ͸ະͩͳ͍ɻຊ೥౓͸·ͣख࢝Ίͱͯ͠‫ ʹط‬ATLASάϧʔϓʹΑΓൃද͞Ε͍ͯΔ৽ཻࢠ୳ࡧͷղੳ݁ՌΛ༻͍ͯ໛‫ܕ‬ͷ੍‫ݶ‬Λ‫ٻ‬Ίͨɻղੳ͸ MadGraph Λ༻͍ͯ਺஋తʹ TeV scale mirage ഔհ໛‫ܕ‬ͷ௒ରশཻࢠΛ‫ؚ‬ΉΠϕϯτΛੜ੒͠ɺATLAS άϧʔϓʹΑͬͯߦΘΕͨ missing transverse momentum ͱϚϧνδΣοτ͋Δ͍͸ࡾຊҎ্ͷ b δΣοτΛཁ‫ͨ͠ٻ‬ղੳͱશ͘ಉ͡ΧοτΛ͔͚ͯ
ੜ͖࢒ΔΠϕϯτ਺Λௐ΂ͨɻ͜ͷղੳʹΑΓɺୈҰɺୈೋੈ୅ͷεΫΥʔΫ͕ୈࡾੈ

3୅ͱॖୀͨ͠໛‫͍͓ͯʹܕ‬͸‫ʹط‬άϧΠʔϊ࣭ྔͷԼ‫ ͕ݶ‬2.2–2.3TeV ·Ͱདྷ͍ͯΔ͜
ͱ͕෼͔ͬͨɻ͜Ε͸ిऑରশੑͷඍௐ੔ύϥϝʔλͱͯ͠͸ 5%ఔ౓ͱͳΔɻୈҰɺୈೋੈ୅ΛάϧΠʔϊͱॖୀͤͨ͞໛‫͍͓ͯʹܕ‬͸άϧΠʔϊ࣭ྔͷ੍‫ݶ‬͸ 1.6TeV ఔ౓Ͱ͋Γɺ·ͩ 10%ఔ౓ͷඍௐ੔ύϥϝʔλ͕‫͞ڐ‬Ε͍ͯΔ͜ͱ͕෼͔ͬͨɻ͍ͣΕͷ৔߹΋ϚϧνδΣοτ͕‫ݶ੍͍ڧ‬Λ༩͍͑ͯΔɻ

Holographic cold nuclear matter and neutron star (‫ٱ‬อ޾‫)و‬ήʔδ/ॏྗରԠ͸ʢ֨ࢠ৔ͷཧ࿦ʹΑΔ਺஋‫ࢉܭ‬Λআ͍ͯ͸ɺʣ΄΅།Ұͷɺઁಈ࿦ʹཔΒͳ͍ήʔδ৔ͷཧ࿦ͷղੳखஈͰ͋ΔɻͦͷͨΊ͜ΕΛ༻͍ͨඇઁಈతͳ‫ܥ‬ɺಛʹ֨ࢠ৔ͷཧ࿦ͷ਺஋‫Ͱࢉܭ‬͸ѻ͍͕ඇৗʹࠔ೉ͱͳΔ༗‫ݶ‬ԽֶϙςϯγϟϧΛ࣋ͬͨ‫߹݁ڧ‬ͷ௿ΤωϧΪʔྖҬ QCD ͳͲɺͷղੳ͸ಛʹ‫ڵ‬ຯਂ͍‫ڀݚ‬ର৅Ͱ͋Δɻզʑ͸ञҪɾਿຊ໛‫ ͏͍ͱܕ‬QCD ʹൺֱత͍ۙੑ࣭Λࣔ͢ήʔδ/ॏྗରԠͷ໛‫رʹܕ‬ബΨεۙࣅΛద༻͢Δ͜ͱͰ༗‫ݶ‬ԽֶϙςϯγϟϧΛ࣋ͭήʔδཧ࿦ͷ༗‫ݶ‬όϦΦϯີ౓૬΁ͷ૬సҠΛൃ‫ͨ͠ݟ‬ɻ·ͨɺͦͷۙࣅͷԼͰ༗‫ݶ‬όϦΦϯີ౓૬Ͱͷঢ়ଶํఔࣜΛ‫ٻ‬ΊɺͦΕΛ༻͍ͯதੑࢠ੕ͷ࣭ྔͱ൒‫ܘ‬Λ༧‫͢ݴ‬Δํ๏ΛఏҊͨ͠ɻ͜ͷํ๏ʹΑΓࣔࠦ͞Εͨதੑࢠ੕ͷ࣭ྔ͸࣮ࡍͷ਺஋ΑΓ΋ඇৗʹখ͘͞‫ੵݟ‬΋ΒΕͨɻ͜Ε͸ಋೖͨ͠‫ر‬ബΨεۙࣅ΋ҰҼͰ͋Δ͕ɺࠜຊతʹ͸໛‫ݱʹܕ‬ΕΔόϦΦϯؒͷੱྗϙςϯγϟϧͷऑ͔͞Βདྷ͍ͯΔͱߟ͑ΒΕΔͨΊ‫ߦݱ‬ͷ໛‫Ͱܕ‬͸ద੾ʹ‫࣮ݱ‬ͷதੑࢠ੕ͷ෺ཧΛද͢͜ͱ͸ࠔ೉Ͱ͋Δ͜ͱ͕෼͔ͬͨɻ
֨ࢠήʔδཧ࿦ʹ͓͚ΔΤωϧΪʔӡಈྔςϯιϧͷ৽͍͠ߏ੒๏ͱͦΕΛ༻͍ͨSU (3) ήʔδཧ࿦ͷ೤ྗֶྔͷଌఆ (ླ໦ത)֨ࢠήʔδཧ࿦͸ήʔδ৔ཧ࿦ͷඇઁಈ࿦తఆࣜԽͱͯ͠࠷΋Α͘ཧղ͞Ε͍ͯΔ΋ͷͰɺ͜Ε·Ͱྔࢠ৭ྗֶ΁ͷԠ༻ʹ͓͍ͯಛʹେ͖ͳ੒ՌΛ͋͛ͯདྷͨɻ֨ࢠήʔδཧ࿦͸ήʔδରশੑΛ‫ʹີݫ‬อͭ఺ʹͦͷಛ௃͕͋Δ͕ɺҰํͰͦͷ֨ࢠߏ଄͸ฒਐɺճసͳͲͷ͍ΘΏΔۭ࣌ରশੑΛյͯ͠͠·͏ɻ͜ͷ͜ͱ͸ɺۭ࣌ฒਐʹରԠͨ͠ωʔλʔΧϨϯτͰ͋ΔΤωϧΪʔӡಈྔςϯιϧɺ·ͨͦΕʹ෇ਵͨ͠෺ཧྔΛ֨ࢠήʔδཧ࿦ʹ͓͍ͯఆٛ͢Δࡍʹ໰୊ͱͳΔɻզʑ͸ɺۙ೥֨ࢠήʔδཧ࿦ͷผͷจ຺Ͱಋೖ͞Εͨ Yang–Mills gradient ﬂow ͱ͍͏ख๏Λར༻͢Δ͜ͱͰɺ࿈ଓ‫Ͱݶۃ‬ࣗಈతʹอଘ͢Δɺਖ਼͘͠‫֨ن‬Խ͞ΕͨΤωϧΪʔӡಈྔςϯιϧΛ֨ࢠήʔδཧ࿦ʹ͓͍ͯߏ੒Ͱ͖Δ͜ͱΛࢦఠͨ͠ɻ͞Βʹɺ͜ͷߏ੒๏ͷҰͭͷԠ༻ͱͯ͠ɺϞϯςΧϧϩγϛϡϨʔγϣϯΛ༻͍༗‫ݶ‬Թ౓ SU (3) ήʔδཧ࿦ͷ೤ྗֶྔʢΤωϧΪʔີ౓ɺѹྗɺΤϯτϩϐʔີ౓ͳͲʣΛਫ਼౓Αܾ͘ఆͰ͖Δ͜ͱΛࣔͨ͠ɻ͜ͷํ๏͸ैདྷͷํ๏ʹൺ΂ඇઁಈ࿦తͳ‫܁‬ΓࠐΈΛඞཁͱ͠ͳ͍఺ʹಛ௃͕͋Γɺࠓ‫͞ޙ‬ΒͳΔԠ༻͕‫ظ‬଴͞ΕΔɻ

4ϑΣϧϛΦϯΛ‫ؚ‬Μͩ֨ࢠήʔδཧ࿦ʹ͓͚ΔΤωϧΪʔӡಈྔςϯιϧͷ৽͍͠ߏ੒๏ (ླ໦തɺ຀໺޿थʣ
ήʔδཧ࿦ͷඇઁಈ࿦తఆࣜԽͰ͋Δ֨ࢠήʔδཧ࿦͸ɺͦͷߏ଄্ɺۭ࣌ରশੑʢฒ
ਐɺճసɺίϯϑΥʔϚϧɺ௒ରশੑͳͲʣͱ‫ۃ‬Ίͯ૬ੑ͕ѱ͘ɺ͜ͷ͜ͱ͕ۭ࣌ରশ
ੑʹରԠͨ͠ωʔλʔΧϨϯτ΍ͦΕʹ෇ਵͨ͠෺ཧྔΛ֨ࢠήʔδཧ࿦Ͱఆٛ͢Δ
ࡍͷ໰୊ͱͳΔɻ࠷ۙླ໦͸ɺฒਐରশੑΛ‫ʹີݫ‬อ͕ͭઁಈ࿦తʹͷΈఆٛ͞ΕΔ࣍‫ݩ‬ਖ਼ଇԽͰͷෳ߹ԋࢉࢠͱɺฒਐରশੑ͸յ͕͢ඇઁಈ࿦త‫͕ࢉܭ‬Մೳͳ֨ࢠਖ਼ଇ
ԽͰͷෳ߹ԋࢉࢠΛɺYang–Mills gradient ﬂow ͱ͍͏֓೦Λഔհʹؔ܎͚ͮΔͱ͍͏ΞΠσΞΛΤωϧΪʔӡಈྔςϯιϧʹద༻ͨ͠ɻ͜ͷ͜ͱͰɺ࿈ଓ‫ࣗͰݶۃ‬ಈతʹอଘ͢Δɺਖ਼͘͠‫֨ن‬Խ͞ΕͨΤωϧΪʔӡಈྔςϯιϧ͕֨ࢠήʔδཧ࿦ʹରͯ͠ߏ੒͞ΕΔɻ͜ͷߏ੒ʹ͸ gradient ﬂow ʹै͏৔ͷԋࢉࢠͷ‫܁‬ΓࠐΈΛઁಈ࿦ͷ௿࣍ͰධՁ͢Δඞཁ͕͋Δ͕ɺͦͷ‫ࢉܭ‬͸७ήʔδཧ࿦ʹ͓͍͔࣮ͯ͠ߦ͞Ε͍ͯͳ͔ͬ
ͨɻ͜ͷ‫Ͱڀݚ‬͸ɺ͜ͷ‫ࢉܭ‬ΛϑΣϧϛΦϯΛ‫ؚ‬ΉҰൠͷϕΫτϧ‫ܕ‬ήʔδཧ࿦Ͱ࣮ߦ͠ɺ֨ࢠήʔδཧ࿦ʹ͓͚ΔΤωϧΪʔӡಈྔςϯιϧΛ gradient ﬂow Ͱ༩͑Δ۩
ମతදࣜΛಘͨɻࠓ‫ޙ‬ɺྔࢠ৭ྗֶ΍ଟϑϨʔόʔήʔδཧ࿦ͳͲʹ͓͚Δۭ࣌ରশੑʹؔ࿈ͨ͠ඇઁಈ࿦త෺ཧʹରͯ͠ɺ͜ͷߏ੒๏͕޿͘Ԡ༻͞ΕΔͱ‫ظ‬଴͍ͯ͠Δɻ
ඇઁಈ࿦త‫܁‬ΓࠐΈ‫ࢄࢠ֩ࢠ֩ͮ͘جʹ܈‬ཚͷղੳ (‫)࢘߃ాݪ‬௿ΤωϧΪʔͷ֩ࢠ‫ܥ‬ͷ૬‫༻࡞ޓ‬͸ɺ֩ࢠ‫ܥ‬༗ޮ৔ཧ࿦ʹΑͬͯ‫ه‬ड़͞ΕΔɻ͜ͷ༗ޮ৔ཧ࿦Ͱ͸ɺS ೾ͷ૬‫༻࡞ޓ‬Λද͢ԋࢉࢠͷ݁߹ఆ਺ʹඇઁಈ࿦త‫ݻ‬ఆ఺͕ଘࡏ͢Δ
͜ͱ͕஌ΒΕ͍ͯΔɻͦΕΏ͑ɺͦͷղੳతͳ‫͍͓ͯʹࢉܭ‬΋ɺ͜ͷඇઁಈ࿦తͳੑ
࣭Λ൓өͤ͞Δඞཁ͕͋Δɻզʑ͸ hybrid regularization ͱ‫ݺ‬͹ΕΔɺύΠΦϯͷަ‫׵‬ͷ૬‫઀ͱ༻࡞ޓ‬৮૬‫༻࡞ޓ‬Λ۠ผ͢Δ‫ํࢉܭ‬๏Λ։ൃ͠ɺͦΕΛ༻͍ͯ֩ࢠ֩ࢠࢄཚ
ͷҐ૬ͷͣΕΛɺNNLO ͷΦʔμʔ·Ͱղੳతʹ‫ͨ͠ࢉܭ‬ɻͦͷදࣜʹ‫·ؚ‬ΕΔ݁߹
ఆ਺Λɺ࣮‫ݧ‬஋ʹ ﬁt ͢Δ͜ͱͰܾఆͨ͠ɻઌߦ‫͍͓ͯʹڀݚ‬͸ɺ͜ͷΑ͏ͳऔΓѻ͍͕༗ޮ৔ཧ࿦ͱͯ͠ͷऩଋੑͷഁ୼Λ΋ͨΒ͢͜ͱ͕ࣔ͞Ε͕ͨɺզʑ͸ઌߦ‫ʹڀݚ‬
͓͚Δ໰୊఺Λࢦఠ͠ɺഁ୼͕ੜ͡ͳ͍͜ͱΛࣔͨ͠ɻP ೾ঢ়ଶʹ͋Δ 2 ͭͷϑΣϧϛΦϯͱɺ࣭ྔͷҟͳΔ 3 ൪໨ͷཻࢠ͔ΒͳΔ‫͚͓ʹܥ‬Δଋറঢ়ଶͱ Eﬁmov ޮՌͷ‫܁‬ΓࠐΈ‫ʹ܈‬ΑΔղੳ (‫࢘߃ాݪ‬ɺ٢ຊҰੈ)Eﬁmov ޮՌͱ͸ɺ2 ମࢄཚͷࢄཚ௕͕ແ‫ݶ‬େͷ‫Ͱݶۃ‬ɺ3 ମͷଋറঢ়ଶ͕ɺྡ͋͏ 2 ͭͷଋറঢ়ଶͷଋറΤωϧΪʔ͕ҰఆͷൺΛ࣋ͬͯແ‫ݱݸݶ‬ΕΔͱ͍͏‫ݱ‬৅Ͱ͋Δɻඇઁ
ಈ࿦త༗ޮ৔ཧ࿦ͷ‫܁‬ΓࠐΈ‫ʹ܈‬ΑΔղੳ͸ɺEﬁmov ޮՌͷΑ͏ͳ‫ݱ‬৅ʹ৔ͷྔࢠ࿦తઆ໌Λ༩͑Δ఺Ͱඇৗʹ‫ڵ‬ຯਂ͍ɻ༗ޮ৔ཧ࿦Λ༻͍ͨઌߦ‫Ͱڀݚ‬͸ɺ͢΂ͯ dimer5ͱ͔ dimeron ͱ‫ݺ‬͹ΕΔ 2 ཻࢠͷ఻೻Λ͋ΒΘ͢ิॿ৔͕༻͍ΒΕ͖ͯͨɻզʑͷલͷ࿦จͰ͸ɺ3 ͭͷಉछϘιϯ‫ʹܥ‬ରͯ͠ɺิॿ৔Λ༻͍ͳ͍ఆࣜԽΛߦͳ͍ɺઌߦ‫ݚ‬‫Ͱڀ‬ͷ‫ޡ‬ΓΛਖ਼͢ͱͱ΋ʹɺEﬁmov ޮՌ͕༗ޮ৔ཧ࿦ͷ௿࣍ͷ߲ʹର͢Δඇઁಈ࿦త
‫܁‬ΓࠐΈ‫܈‬ͷϦϛοταΠΫϧͱͯ͠‫ݱ‬ΕΔ͜ͱΛࣔͨ͠ɻ͜ΕΛ 2 ͭͷϑΣϧϛΦ
ϯͱɺ࣭ྔͷҟͳΔୈ 3 ͷཻࢠ͔ΒͳΔ 3 ମ‫ʹܥ‬ద༻͢Δ‫ڀݚ‬Λߦͳͬͨɻ͜ͷ‫Ͱܥ‬͸ɺ࣭ྔൺʹΑͬͯɺ༷ʑͳঢ়ଶ͕‫ݱ‬Εͯ͘Δ͜ͱ͕஌ΒΕ͍ͯΔ͕ɺզʑͷ‫Ͱڀݚ‬͸ɺͦͷྟքൺ͕ઌߦ‫ͱڀݚ‬͸ҧ͍ͬͯΔ͜ͱΛࣔͨ͠ɻզʑͷ஋͕ਖ਼͚͠Ε͹ɺ͢Ͱʹ࣮‫ݧ‬తʹ‫؍‬ଌՄೳ͔΋஌Εͳ͍ɻӡಈྔґଘ෼෍ؔ਺Λ༻͍ͨϨϓτϯ਺ੜ੒ͷղੳ (ਫ‫୓ޱ‬໵)‫؍‬ଌʹ‫͔࡯ߟ͍ͨͮج‬Βɺ‫ࡏݱ‬ͷӉ஦͸όϦΦϯ਺ඇରশͳঢ়‫͋ʹگ‬Δͱߟ͑ΒΕ͍ͯΔɻͳͥ͜ͷΑ͏ͳঢ়‫͞ݱ࣮͕گ‬Ε͔ͨΛઆ໌ՄೳͳϞσϧͷ 1 ͭͱͯ͠ɺ“ϨϓτδΣωγε” ͕ઌߦ‫ߟ͍͓ͯʹڀݚ‬Ҋ͞Ε͍ͯΔɻ͜ͷϞσϧ͸ɺ‫ࡏݱ‬ଘࡏ͕֬ೝ͞Ε͍ͯΔχϡʔτϦϊ͕ϚϤϥφཻࢠͰ͋ΔͱͷલఏΛஔ͘͜ͱʹΑΓɺͦͷ࣭ྔ͕খ͍͞ཧ༝Λઆ໌ՄೳͰ͋Δͱ͍͏ಛ௃΋‫ؚ‬ΜͰ͓Γɺཧ࿦తʹ͸ඇৗʹ༗๬ࢹ͞Εͯ
͍Δɻࡢ೥౓ͷ‫಺ڀݚ‬༰͸ɺϨϓτδΣωγεͷγφϦΦʹ͓͚ΔඇฏߧաఔͷɺϘϧπϚϯํఔࣜʹ‫ͮ͘ج‬ղੳͰ͋Δɻಉ༷ͷ‫ڀݚ‬͸ɺ͜Ε·Ͱʹ΋ଞͷଟ͘ͷ‫ऀڀݚ‬ʹΑͬͯҝ͞Ε͖͍ͯͯΔɻ͔͠͠ͳ͕Βɺଟ͘ͷઌߦ‫Ͱڀݚ‬͸ɺ෼෍ؔ਺͕೤ฏߧ
࣌ͷ෼෍ؔ਺ʹൺྫ͢Δͱ͍͏ඇࣗ໌ͳԾఆ͕༻͍ΒΕ͍ͯΔɻ͔֬ʹͦͷΑ͏ͳԾఆΛ༻͍ΔͱɺϘϧπϚϯํఔ͕ࣜղੳతʹ୯७ͳ‫ʹܗ‬ม‫͖Ͱܗ‬ɺ਺஋తʹղ͖қ͍‫ͳʹܗ‬ΔͷͰ͋Δ͕ɺԾఆͷ෺ཧతͳࠜ‫ڌ‬͸ͳ͍ɻͦͷΑ͏ͳղੳํ๏ͱ͸ରরతʹɺຊ‫͍͓ͯʹڀݚ‬͸ɺ෼෍ؔ਺ͷӡಈྔґଘੑ͸े෼ʹߟྀ͞Ε͍ͯΔɻ‫ࡏݱ‬͸ɺϘϧπϚϯํఔࣜͷিಥ߲ʹ৽ͨʹࢄཚաఔͷ‫د‬༩Λ‫ؚ‬ΊɺͦΕΒ͕Ϩϓτϯ਺ඇରশͷ࣌ؒൃలʹͲͷΑ͏ͳӨ‫ڹ‬Λ‫͔͢΅ٴ‬Λઌͱಉ༷෼෍ؔ਺ͷӡಈྔґଘੑΛߟྀͯ͠
ߦ͍ͬͯΔɻൃද࿦จ ‫ݪ‬ஶ࿦จ 
Discrete gauge symmetry and Aharonov–Bohm radiation in string theory:
Yutaka Ookouchi,
Journal of High Energy Physics, 1401 (2014) 049

6

More on cosmological constraints on spontaneous R-symmetry breaking models:
Yuta Hamada, Kohei Kamada, Tatsuo Kobayashi, Yutaka Ookouchi,
Journal of Cosmology and Astrophysics, P01 (2014) 024
Holographic cold nuclear matter and neutron star:Kazuo Ghoroku, Kouki Kubo, Motoi Tachibana, Fumihiko Toyoda,
International Journal of Modern Physics A, 29 (2014) 1450060
Thermodynamics of SU (3) Gauge Theory from Gradient Flow:
Masayuki Asakawa, Tetsuo Hatsuda, Etsuko Itou, Masakiyo Kitazawa, Hiroshi Suzuki,
arXiv:1312.7492
Lattice energy–momentum tensor from the Yang–Mills gradient ﬂow—inclusion offermion ﬁelds:
Hiroki Makino, Hiroshi Suzuki,
arXiv:1403.4772, to appear in Progress of Theoretical and Experimental Physics
Convergent perturbative nuclear eﬀective ﬁeld theory:
Koji Harada, Hirofumi Kubo, Tatsuya Sakaeda, Yuki Yamamoto,arXiv:1311.3063

Proceedings
Converging low energy expansion of nucleon-nucleon scattering based on the Wilsonian
renormalization group:
H. Kubo, K. Harada, T. Sakaeda, Y. Yamamoto,
PoS Hadron2013 (2014) 143. (Proceedings, 15th International Conference on Hadron
Spectroscopy (Hadron 2013) : Nara, Japan, November 4–8, 2013)ߨԋ ւ֎Ͱͷߨԋ 
Phenomenology of NMSSM in TeV scale mirage mediation:
Tatsuo Kobayashi, Hiroki Makino, Ken-ichi Okumura and Takashi Shimomura,7

19th International Symposium on Particles, Strings, and Cosmology
TeV scale Mirage Mediation with Vector-like Quark:
Hiroki Makino, Takahiro Nakamura, Ken-ichi Okumura,
Summer Institute 2013, 20 August 2013, Jirisan National Park, Korea ࠃ಺Ͱͷߨԋ 
Aharonov-Bohm radiation in string theory:େՏ಺๛ηϛφʔߨԋɺ2013 ೥ 12 ݄ 17 ೔ɺେࡕࢢཱେֶ

Aharonov-Bohm radiation in string theory:େՏ಺๛ηϛφʔߨԋɺ2014 ೥ 1 ݄ 8 ೔ɺ‫౎ژ‬େֶཧֶ෦
௒ରশཧ࿦ͷ‫ͱࡏݱ‬ະདྷ:Ԟଜ݈ҰՃ଎‫ث‬ɾ෺ཧ߹ಉ ILC Նͷ߹॓ 2013෦෼తʹॖୀͨ͠௒ରশ໛‫΁ܕ‬ͷ LHC ͔Βͷ੍‫ݶ‬:Ԟଜ݈Ұɺ຀໺޿थɺࢁ‫࢘ݡޱ‬ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձɺ2013 ೥ 11 ݄ 30 ೔ɺ‫ཹٱ‬ถ޻‫ۀ‬େֶ

Holographic cold nuclear matter as dilute instanton gas:‫ٱ‬อ޾‫و‬೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɺ2013 ೥ 9 ݄ 20 ೔ɺߴ஌େֶே૔Ωϟϯύε
ߴ࣍‫ݩ‬ήʔδ৔ʹΑΔ E6 ରশੑͷࣗൃతͳഁΕͱେ౷Ұ໛‫ܕ‬:খౡ݈ଠ࿠ɺ஛Ӭ࿨యɺࢁԼහ࢙
೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ2014 ೥ 3 ݄ 28 ೔ɺ౦ւେֶভೆΩϟϯύε

Energy–momentum tensor from the Yang–Mills gradient ﬂow:ླ໦ത೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɺ2013 ೥ 9 ݄ 22 ೔ɺߴ஌େֶே૔Ωϟϯύε

8

Yang–Mills gradient ﬂow ʹΑΔ֨ࢠ্ͷΤωϧΪʔӡಈྔςϯιϧ:ླ໦ത‫ڀݚ‬ձʮ཭ࢄతख๏ʹΑΔ৔ͱۭ࣌ͷμΠφϛΫεʯɺ2013 ೥ 9 ݄ 27 ೔ɺߴΤωϧΪʔՃ଎‫ߏػڀݚث‬Lattice energy-momentum tensor from the Yang–Mills gradient ﬂow:ླ໦ത
ୈ 3 ճ‫ૅجࢉܭ‬Պֶ࿈‫( ఺ڌܞ‬JICFuS) ηϛφʔɺ2013 ೥ 10 ݄ 16 ೔ɺେࡕେֶཧֶ෦

Lattice energy–momentum tensor from the Yang–Mills gradient ﬂow:ླ໦ത‫ૅجࢉܭ‬Պֶ࿈‫( ఺ڌܞ‬JICFuS) ‫ڀݚ‬ձʮLattice QCD at ﬁnite temperature and den-sityʯɺ2014 ೥ 1 ݄ 22 ೔ɺߴΤωϧΪʔՃ଎‫ߏػڀݚث‬֩ࢠ‫ܥ‬༗ޮ৔ཧ࿦ͷ‫܁‬ΓࠐΈ‫Ͱ܈‬Կ͕Θ͔Δ͔:‫࢘߃ాݪ‬

RCNP/‫۝‬େ‫ڀݚ‬ձʮϋυϩϯ෺ཧͱ‫֩ࢠݪ‬෺ཧͷΫϩεΦʔόʔʯɺ2013 ೥ 9 ݄ 4 ೔–6೔ɺ‫۝‬भେֶ

Vector-like quark Λಋೖͨ͠ TeV εέʔϧ Mirage Mediation:຀໺޿थɺ஥ଜਸେɺԞଜ݈Ұୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձɺ2013 ೥ 11 ݄ 30 ೔ɺ‫ཹٱ‬ถ޻‫ۀ‬େֶॖୀͨ͠௒ରশ໛‫΁ܕ‬ͷ LHC ͔Βͷ੍‫ݶ‬:ࢁ‫࢘ݡޱ‬‫ऀࡾ֩ࢠݪ‬एखՆͷֶߍɺ2013 ೥ 8 ݄ 5 ೔ิॿ৔Λ༻͍ͳ͍ Wilson ྲྀ͘Γ͜Έ‫ʹ܈‬ΑΔ mass imbalanced fermion ‫ܥ‬ͷղੳ:‫࢘߃ాݪ‬ɺ‫ٱ‬อത࢙ɺ˓٢ຊҰੈ೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɺ2013 ೥ 9 ݄ 23 ೔ɺߴ஌େֶே૔Ωϟϯύε

Nonperturbative RG in nonrelativistic mass imbalanced fermionic system without auxiliary ﬁelds:‫࢘߃ాݪ‬ɺ˓٢ຊҰੈ

9೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ2014 ೥ 3 ݄ 30 ೔ɺ౦ւେֶভೆΩϟϯύε

֎෦ࢿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ Պֶ‫ڀݚ‬අิॿۚɺएख Bਅۭͷ҆ఆੑͱཻ͍ܰࢠ͔Βͷ‫ݭ‬ཧ࿦΁ͷ੍‫ݶ‬‫ڀݚ‬୅දऀɿେՏ಺๛
Պֶ‫ڀݚ‬අิॿۚɺ৽ֶज़ྖҬ (‫ྖڀݚ‬ҬఏҊ‫)ܕ‬χϡʔτϦϊͰ୳Δૉཻࢠͷ‫ͱݯى‬Ӊ஦ͷߏ଄‫ڀݚ‬୅දऀɿ๺໺ཾҰ࿠‫ڀݚ‬෼୲ऀɿେՏ಺๛
Պֶ‫ڀݚ‬අิॿۚɺ೔ຊֶज़ৼ‫ڵ‬ձಛผ‫ڀݚ‬һՊ‫ݚ‬අ‫ڀݚ‬୅දऀɿ‫ٱ‬อ޾‫و‬Պֶ‫ڀݚ‬අิॿۚɺ‫ج‬൫ C (Ұൠ)௒ରশੑཧ࿦ͷඇઁಈ࿦తఆࣜԽͱ਺஋γϛϡϨʔγϣϯ‫ڀݚ‬୅දऀɿླ໦ത

ଞେֶͰͷ‫ڭͱڀݚ‬ҭԞଜ݈Ұɿ৽ׁେֶͰूதߨٛΛߦͬͨɻ2014 ೥ 1 ݄ 14 ೔͔Β 1 ݄ 16 ೔·Ͱɻߨٛ୊໨͸ʮώοάεཻࢠͱ௒ରশੑʯ
‫࢘߃ాݪ‬ɿࣛࣇౡେֶͰूதߨٛΛߦͬͨɻ2014 ೥ 10 ݄ 14–15 ೔͓Αͼ 11 ݄ 18–19೔ɻߨٛ୊໨͸ʮ૬ର࿦ʯ

ֶ෦̐೥ੜଔ‫ڀݚۀ‬஛ቌஐ೭ɿ(ࢦಋ‫ڭ‬һɺԞଜ݈Ұ)ɿޫԁਲ਼ήʔδʹ‫͍ͨͮج‬௒‫ݭ‬ཧ࿦ͷཧղ

10౻ࢁᠳ೫ɿ(ࢦಋ‫ڭ‬һɺԞଜ݈Ұ)ɿޫԁਲ਼ήʔδʹ‫͍ͨͮج‬௒‫ݭ‬ཧ࿦ͷཧղ౻ࢁ༏Ұɿ(ࢦಋ‫ڭ‬һɺԞଜ݈Ұ)ɿޫԁਲ਼ήʔδʹ‫͍ͨͮج‬௒‫ݭ‬ཧ࿦ͷཧղम࢜࿦จ‫ྒྷాݪ‬ฏɿ(ࢦಋ‫ڭ‬һɺ‫)࢘߃ాݪ‬ɿ‫ڞ‬ม‫܁‬ΓࠐΈՄೳॏྗཧ࿦ʹ͓͚Δઁಈల։දࣔͱ

Arnowitte–Deser–Misner ෼ղදࣔͱͷ੔߹ੑʹ͍ͭͯࢁ‫࢘ݡޱ‬ɿ(ࢦಋ‫ڭ‬һɺླ໦തɾԞଜ݈Ұ)ɿTeV εέʔϧϛϥʔδϡഔհ໛‫΁ܕ‬ͷ LHC
ʹΑΔ௚઀୳ࡧ͔Βͷ੍‫ݶ‬ത࢜࿦จ‫ٱ‬อ޾‫و‬ɿ(ࢦಋ‫ڭ‬һɺ‫)࢘߃ాݪ‬ɿNovel examples of the application of gauge/gravity

dualityʢήʔδॏྗରԠͷద༻ͷ৽͍͠ྫʣ
٢ຊҰੈɿ(ࢦಋ‫ڭ‬һɺ‫)࢘߃ాݪ‬ɿWilsonian renormalization group analysis of nonrel-

ativistic three-body systems without introducing auxiliary ﬁeldsʢิॿ৔Λ༻͍ͳ͍ඇ
૬ର࿦త 3 ମ‫ܥ‬ͷ Wilson ྲྀ͘Γ͜Έ‫܈‬Λ༻͍ͨղੳʣ
ֶ֎Ͱͷֶձ‫׆‬ಈࠃࡍ‫ڀݚ‬ձʮBeyond the Standard Model 2014ʯɺ2014 ೥ 3 ݄ 3 ೔–3 ݄ 7 ೔ɺߴΤωϧΪʔՃ଎‫( ߏػڀݚث‬KEK)ɺੈ࿩ਓ (େՏ಺๛)‫ڀݚݚج‬ձʮૉཻࢠ෺ཧֶͷਐల 2013ʯɺ2013 ೥ 8 ݄ 3 ೔–8 ݄ 9 ೔ɺ‫౎ژ‬େֶ‫ૅج‬෺ཧֶ‫ॴڀݚ‬ɺੈ࿩ਓ (େՏ಺๛)෺ཧֶձ‫۝‬भࢧ෦ձ࠲௕ (Ԟଜ݈Ұ)ૉཻࢠ࿦άϧʔϓૉཻࢠ࿦ҕһձҕһ௕ (‫)࢘߃ాݪ‬11‫֩ࢠݪ‬ཧ࿦‫ߏࣨڀݚ‬੒һീਘ ਖ਼৴ ‫ڭ‬तਗ਼ਫ ྑจ ।‫ڭ‬तদຊ ୖຏ ॿ‫ڭ‬ ത࢜‫ڀݚ‬һ ຸໜ ޻ক େֶӃ ത࢜՝ఔ ࠤʑ໦ ਸ޺ా্ ਅ‫ޔ‬ౢా ॆ޺ߴ‫ ڮ‬७Ұ౉ᬒ ৻ େֶӃ म࢜՝ఔ ੴҪ ༏େߐ಄ ‫ܛ‬

؅໺ ३ฏ

ถଜ ߒ࢘

ࠤʑ෦ ‫ޛ‬๛઒ কҰ ֶ෦ ଔ‫ڀݚۀ‬ੜ 
ळࢁ ཅฏ

Ҫੜ ෢ࢤ

ฏ઒ ༏ਅ

‫ٶ‬ຊ ߉୓

୲౰त‫ۀ‬
෺ཧֶೖ໳ (ീਘਖ਼৴)ɺྔࢠྗֶ Iɾಉԋश (ീਘਖ਼৴ɾদຊୖຏ)ɺಛघ૬ର࿦ͱి
‫( ֶྗؾ‬ീਘਖ਼৴)ɺ෺ཧ਺ֶ I(ਗ਼ਫྑจ)ɺྔࢠྗֶ IIIʢਗ਼ਫྑจʣɺ਺஋‫ࢉܭ‬๏ (ਗ਼ਫྑจ)ɺి࣓‫( ֶؾ‬ਗ਼ਫྑจ)ɺ෺ཧֶಛผ‫ ڀݚ‬I(ീਘਖ਼৴ɾਗ਼ਫྑจɾদຊୖຏ)ɺ෺
ཧֶಛผ‫ ڀݚ‬II(ീਘਖ਼৴ɾਗ਼ਫྑจɾদຊୖຏ)‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ
ߴີ౓ఱମͷߏ଄ʹؔΘΔ QCD ૬ߏ଄ͷ‫( ڀݚ‬ീਘਖ਼৴, Տ໺޺໌ [ࠤլେֶ], Տ໺௨࿠ [‫۝‬भࣃՊେֶ], ҆෢৳ढ़ [ઍ༿޻‫ۀ‬େֶ], ࠤʑ໦ਸ޺ (D3))

QCD ͷ૬ߏ଄ (QCD ૬ਤ) ͱঢ়ଶํఔࣜ͸, Ӊ஦ਐԽͷաఔ΍ߴີ౓ఱମͷੑ࣭Λղ໌͢ΔͨΊʹෆՄܽͳཁૉͰ͋Δɻ͔͠͠, QCD ͷୈҰ‫ݪ‬ཧ‫͋Ͱࢉܭ‬Δ֨ࢠ QCD ‫ܭ‬ࢉ͸༗‫ྖ౓ີݶ‬ҬͰ࣮ߦࠔ೉Ͱ͋ΔͨΊ, ༗‫͚͓ʹ౓ີݶ‬Δ૬ߏ଄ͷ΄ͱΜͲ͸ ෆ֬
ఆͰ͋Δɻຊ‫Ͱڀݚ‬͸, ߴີ౓ྖҬͷ QCD ૬ߏ଄Λ༗ޮ໛‫ܕ‬Λ༻͍ͯղ໌͢Δ͜ͱΛ

12໨ࢦͨ͠ɻ
ߴີ౓ྖҬͰ͸όϦΦϯͷ‫د‬༩͕ຊ࣭తͰ͋Γ, ༗ޮ໛‫͚͓ʹܕ‬ΔόϦΦϯͷऔΓѻ͍ʹ͸ෆఆੑ͕େ͖͍ɻ͜ͷෆఆੑΛͳͨ͘͢Ίʹզʑ͸, ֩෺࣭ͷղੳ͓Αͼதੑࢠ੕ͷ࣭ྔ‫؍‬ଌʹண໨ͨ͠ɻඪ४֩ີ౓෇ۙͷ֩෺࣭ͷੑ࣭͸, ΧΠϥϧ༗ޮ৔ཧ࿦ʹ‫ج‬͍ͮͨ֩ྗΛ༻͍ͯ Brueckner-Hartree-Fock ‫ࢉܭ‬Λߦ͏͜ͱʹΑΓ, ߴ͍৴པੑͰͷղੳ͕ՄೳͰ͋Δɻ͞Βʹߴ͍ີ౓ྖҬͷঢ়ଶํఔࣜ͸ॏΠΦϯিಥ࣮‫ݧ‬ͷղੳ͔Β‫ݟ‬ੵ΋ΒΕ͍ͯΔɻզʑ͸͜ΕΒͷσʔλΛ࠶‫͢ݱ‬ΔΑ͏ʹ֩ࢠؒͷ༗ޮੱྗΛಋೖ͠,ϋυϩϯ૬Λ‫ه‬ड़͢Δ໛‫ͨ͠ͱܕ‬ɻ͞Βʹ, ͜ͷ໛‫ܕ‬Λ༻͍ͯதੑࢠ੕ͷߏ଄Λ‫͠ࢉܭ‬,‫ࡏݱ‬ͷதੑࢠ੕࣭ྔ‫؍‬ଌͷ݁Ռͱແໃ६Ͱ͋Δ͜ͱΛ֬ೝͨ͠ɻ͜ͷΑ͏ʹߏஙͨ͠ϋυϩϯ໛‫ ͱܕ‬EPNJL ໛‫ܕ‬Λ૊Έ߹ΘͤΔ͜ͱʹΑΓ QCD ૬ਤશମͷղੳ͕ՄೳͰ
͋Δɻ͜ͷΑ͏ʹಘΒΕͨ૬ਤ͸, ༗‫ݶ‬Թ౓ͷ֨ࢠ QCD ‫͓ࢉܭ‬Αͼ֩෺࣭ɾதੑࢠ੕
ͷσʔλͱແໃ६ͳ΋ͷͰ͋Δɻຊ‫ڀݚ‬͸ࠤʑ໦ࢯΛத৺ʹਪਐ͞Εͨɻ
֨ࢠ QCD ʹΑΔΧϥʔःณϙςϯγϟϧͷԽֶϙςϯγϟϧґଘੑͷ‫( ڀݚ‬ീਘਖ਼৴,தଜ७ [޿ౡେֶ], ࡈ౻୎໵ [ߴ஌େֶ], Ӭా‫ܡ‬ଠ࿠ [KEK], Տ໺޺໌ [ࠤլେֶ], ࠤʑ໦ਸ޺ (D3), ߴ‫ڮ‬७Ұ (D1))Χϥʔःณϙςϯγϟϧ (ॏΫΥʔΫϙςϯγϟϧ) ͸ॏΠΦϯিಥ࣮‫͚͓ʹݧ‬ΔॏΫΥʔΫଋറঢ়ଶͷ཈੍‫ߏػ‬΍δΣοτͷੑ࣭Λௐ΂ΔࡍʹॏཁͳྔͰ͋Δɻࡢ೥౓ΑΓɺզʑ͸Χϥʔःณϙςϯγϟϧͷ‫਺ڏ‬Խֶϙςϯγϟϧ (μI ) ґଘੑΛௐ΂͖ͯͨɻࠓ೥౓͸‫ٻ‬ΊͨΧϥʔःณϙςϯγϟϧΛ࣮਺Խֶϙςϯγϟϧ (μR ) ྖҬʹ֎ૠͨ͠ɻͦͷ݁ՌɺμR Λେ͖͍ͯ͘͘͠ͱΧϥʔःณϙςϯγϟϧͷߴ͕͞௿͘ͳ͍ͬͯ
͘͜ͱ͕෼͔ͬͨɻ͜Ε͸ɺμ Λେ͖͍ͯ͘͘͠ͱΫΥʔΫؒͷ૬‫͕༻࡞ޓ‬খ͘͞ͳͬ
͍ͯ͘͜ͱΛ͍ࣔͯ͠Δɻ·ͨɺreweighting ๏Λ༻͍ͨઌߦ‫Ͱڀݚ‬͸Χϥʔःณϙςϯγϟϧʹରͯ͠ μR /T ͷ 2 ࣍·Ͱ‫͞ࢉܭ‬Ε͍͕ͯͨɺຊ‫Ͱڀݚ‬͸ μR /T ͷ 4 ࣍΋ແࢹͰ͖ͳ͍ఔͷ‫د‬༩Λ͍࣋ͬͯΔ͜ͱΛࣔͨ͠ɻ͜ΕʹՃ͑ͯɺΧϥʔ Debye ःณ࣭ྔ΋ μR ྖҬʹ֎ૠͨ͠ɻͦͷ݁Ռɺhard thermal loop ۙࣅ΍Φʔμʔͷߴ͍ઁಈ‫ࢉܭ‬ͷ݁ՌͱఆੑతͳҰக͸‫ݟ‬ΒΕ͕ͨɺμR ґଘੑ͸զʑͷ݁Ռͷํ͕େ͖͔ͬͨɻ
ຊ‫ڀݚ‬͸ߴ‫ࢯڮ‬Λத৺ʹਪਐ͞Εɺͦͷ੒Ռ͸ Physical Review ࢽʹ࿦จ͕‫͞ࡌܝ‬Εͨɻ֨ࢠ QCD ʹΑΔΫΥʔΫ਺ີ౓ͷ‫ͱڀݚ‬༗ޮ໛‫ܕ‬ͷߏங (ീਘਖ਼৴, Տ໺޺໌ [ࠤլେֶ], ߴ‫ڮ‬७Ұ (D1), ؅໺३ฏ (M1))༗‫ݶ‬Թ౓ (T )ɺ༗‫ݶ‬Խֶϙςϯγϟϧ (μ) ྖҬʹ͓͚Δ QCD ͷ‫ͯͬͱʹڀݚ‬ɺ༗ޮ໛‫ܕ‬͸‫ͳྗڧ‬πʔϧͰ͋Δɻ͔͠͠ɺ༗ޮ໛‫ܕ‬͸ύϥϝʔλΛ࣋ͪɺෆఆੑΛ‫ؚ‬Ήɻͦ

13ͷෆఆੑΛͳͨ͘͢Ίʹɺզʑ͸ QCD ͷୈҰ‫ݪ‬ཧ‫͋Ͱࢉܭ‬Δ֨ࢠ QCD ‫ࢉܭ‬ͷ݁Ռͱ༗ޮ໛‫ܕ‬ͷ݁ՌΛ߹ΘͤΔ͜ͱͰɺ৴པੑͷߴ͍༗ޮ໛‫ܕ‬ͷߏஙΛ໨ࢦ͍ͯ͠Δɻಛʹɺ༗‫ ݶ‬μ ྖҬͰ͸ΫΥʔΫ਺ີ౓ͱؔ࿈ͨ͠ϕΫλʔ‫ܕ‬૬‫༻࡞ޓ‬ͷޮՌ͕ॏཁͰ͋
Δɻ
ͦ͜Ͱզʑ͸ΫΥʔΫ਺ີ౓ͷ μ ґଘੑΛ֨ࢠ QCD Ͱ‫͠ࢉܭ‬ɺͦͷ݁ՌͱϕΫλʔ‫ܕ‬૬‫༻࡞ޓ‬ͷೖͬͨ EPNJL ໛‫ܕ‬ͷ݁ՌΛ߹Θͤɺ༗‫ ౓ີݶ‬QCD ͷ෺ཧɺಛʹ QCD
૬ਤ΍தੑࢠ੕ͷ෺ཧͷ‫ڀݚ‬ΛਐΊ͍ͯ͘ɻ֨ࢠ QCD Ͱ͸ූ߸໰୊ͷͳ͍‫਺ڏ‬Խֶϙςϯγϟϧ (μI ) ྖҬͰ‫ࢉܭ‬Λ࣮ߦ͠ɺΫΥʔΫ਺ີ౓ͷ μI ґଘੑΛಘͨɻࠓ‫ޙ‬ɺ͜ͷ݁Ռʹ߹͏Α͏ʹ EPNJL ໛‫ܕ‬ͷύϥϝʔλΛ߹ΘͤɺQCD ૬ਤ΍தੑࢠ੕ͷ࣭ྔͱ൒‫ܘ‬ͷؔ܎ɺதؒࢠःณ࣭ྔͷ μ ґଘੑͳͲΛ‫ٻ‬Ί͍ͯ͘ɻຊ‫ڀݚ‬͸ߴ‫ͱࢯڮ‬؅໺ࢯΛத৺ʹਪਐ͞Ε͍ͯΔɻ
༗‫ྖ౓ີݶ‬Ҭʹ͓͚Δ֨ࢠ QCD ‫ࢉܭ‬ख๏ͷ։ൃ (ീਘਖ਼৴, தଜ७ [޿ౡେֶ], Տ໺޺໌ [ࠤլେֶ], ߴ‫ڮ‬७Ұ (D1))Խֶϙςϯγϟϧ (μ) ͕༗‫ݶ‬ͷྖҬͰ͸ɺ֨ࢠ QCD ʹ͓͚ΔΫΥʔΫߦྻ͕ෳૉ਺
ʹͳΓɺΠϯϙʔλϯεαϯϓϦϯάΛ༻͍ͨϞϯςΧϧϩγϛϡϨʔγϣϯ͕ࠔ೉
ͱͳΔɻ͜Ε͕ූ߸໰୊Ͱ͋Δɻ༗‫ ݶ‬μ ྖҬͷ෺ཧΛୈҰ‫ݪ‬ཧ‫͋Ͱࢉܭ‬Δ֨ࢠ QCD Ͱ‫͢ڀݚ‬ΔͨΊʹ͸ɺූ߸໰୊ͷճආ͕ඞཁͰ͋Δɻ͜Ε·Ͱ reweighting ๏ɺ‫਺ڏ‬ԽֶϙςϯγϟϧྖҬ͔Βͷղੳ઀ଓɺώετάϥϜ๏ͳͲ༷ʑͳճආํ๏ʹΑΓ‫͕ڀݚ‬ͳ͞Ε͖ͯͨɻ͔͠͠ɺࠜຊతͳූ߸໰୊ͷղܾ͸೉͍͠ͷ͕‫ݱ‬ঢ়Ͱ͋Δɻ
ͦ͜Ͱզʑ͸ɺैདྷ͔Β͋Δঢ়ଶີ౓Λ༻͍Δํ๏ΛԠ༻ͨ͠ɺ༗‫ྖ౓ີݶ‬Ҭʹ͓͚Δ֨ࢠ QCD ‫ࢉܭ‬ख๏ͷ։ൃʹऔΓ૊ΜͰ͍ΔɻGocksch ʹΑΕ͹ɺ஫໨͢Δ෺ཧྔͷɺ͋ΔΤωϧΪʔͷൣғΛ౳෼ׂ‫ͼٴ‬άϧʔϐϯά͠ɺͦͷΤωϧΪʔάϧʔϓ಺Ͱ֬཰ղऍ͕੒ΓཱͭΑ͏ʹ෼෍Λ‫ٻ‬ΊɺͦΕΛ͍ͭ͘΋ͷΤωϧΪʔάϧʔϓͰߦ͍ɺͦΕͧΕͰ‫ͨͬ·ٻ‬෼෍Λ‫߹͗ܨ‬ΘͤΕ͹ɺ޿͍ൣғͷ֬཰෼෍͕‫·ٻ‬Δɻࠓɺզʑ
͕஫໨͢΂͖෺ཧྔ͸ΫΥʔΫ਺ີ౓Ͱ͋Δɻ͜ͷ֬཰෼෍Λ‫ٻ‬Ίͯήʔδ഑ҐΛूΊΔ͜ͱʹΑΓɺ༗‫ྖ౓ີݶ‬Ҭͷ෺ཧྔΛ௚઀֨ࢠ QCD Ͱ‫͢ࢉܭ‬Δ͜ͱ͕ग़དྷΔɻ޿͍ൣғʹΘͨΔΫΥʔΫ਺ີ౓ͷ֬཰෼෍Λ‫ٻ‬ΊΔඞཁ͕͋Δɻ͔͠͠ɺ༗‫ ݶ‬μ ྖҬͷ‫ࠔ͕ࢉܭ‬೉Ͱ͋Δ͜ͱ͔Βɺ֨ࢠ QCD Λ༻͍ͯ༗‫ݶ‬ͷΫΥʔΫ਺ີ౓Λ࣮‫͢ݱ‬Δ
͜ͱ͸ࠔ೉Ͱ͋Δɻͦ͜ͰΫΥʔΫ਺ີ౓͕༗‫ͳͱݶ‬ΔΑ͏ͳྗΛ࡞ҝతʹ֨ࢠ࡞༻ʹՃ͑ΔɻΫΥʔΫ਺ີ౓͕༗‫ͳʹݶ‬Δ·Ͱήʔδ഑ҐΛΞοϓσʔτͨ͠‫ޙ‬ɺͦͷ࡞ҝతͳྗ͸औΓআ͍ͯɺ্‫ه‬ͷ Gocksch ͷํ๏Λ࢖༻͢Δɻ͜ͷΑ͏ʹͯ͠ΫΥʔΫ਺ີ౓ͷ֬཰෼෍Λ‫ٻ‬ΊΔɻຊ‫ڀݚ‬͸ߴ‫ࢯڮ‬Λத৺ʹਪਐ͞Ε͍ͯΔɻ

14༗ޮ໛‫ܕ‬Λ༻͍ͨϝιϯःณ࣭ྔͷಋग़ͱղੳ (ീਘਖ਼৴, Տ ໺޺໌ [ࠤլେֶ], ࠤʑ໦ਸ޺ (D3), ੴҪ༏େ (M2))֨ࢠ QCD Ͱ‫͞ࢉܭ‬Ε͍ͯΔ෺ཧྔͱͯ͠ɺϝιϯͷःณ࣭ྔ (Mscr ) ͕͋ΔɻҰํɺ༗ޮ໛‫ʹܕ‬ΑΔ Mscr ͷ‫ࢉܭ‬͸ɺܹ͘͠ৼಈ͢Δؔ਺ͷແ‫ੵݶ‬෼Λඞཁͱ͢ΔͨΊࠔ೉Ͱ͋Γɺ͜Ε·Ͱ΄ͱΜͲ‫͞ࢉܭ‬Εͯ͜ͳ͔ͬͨɻͦ͜Ͱɺ༗ޮ໛‫ʹܕ‬ΑΔ Mscr ͷ‫ܭ‬ࢉख๏ͷ։ൃΛ໨ඪͱͨ͠ɻःณ࣭ྔʹؔ͢Δ֨ࢠ QCD ‫ࢉܭ‬ͷ݁ՌΛ࠶‫͢ݱ‬ΔΑ͏ʹ༗ޮ໛‫ܕ‬Λߏங͢Δ͜ͱͰɺ༗ޮ໛‫ܕ‬ͷෆఆੑΛഉআ͢Δͱ͍͏ํ਑Λཱͯͨɻ·ͣɺӡಈྔදࣔʹ͓͚Δϝιϯ૬ؔؔ਺ͷղੳੑΛৄࡉʹ෼ੳ͢Δ͜ͱͰɺMscrͷ‫ࢉܭ‬ख๏ΛߟҊͨ͠ɻෳૉӡಈྔฏ໘্ͷ‫ ͯ͠ͱۃ‬Mscr Λ‫ٻ‬ΊΔࣄ͕Ͱ͖ΔͨΊɺզʑͷख๏͸ैདྷͷख๏ΑΓ΋͸Δ͔ʹ؆ศͰ͋Δɻ͜ͷख๏ʹ‫͖ͮج‬ɺ2 ϑϨʔόʔ
ͷ EPNJL ໛‫ Ͱܕ‬π ϝιϯःณ࣭ྔ (Mπ,scr ) ͷԹ౓ґଘੑΛ‫͠ࢉܭ‬ɺఆੑతͳৼΔ෣͍Λ෼ੳͨ͠ɻMπ,scr ͸ɺ௿ԹͰ͸ҰఆͰ͋Γɺด͡ࠐΊ૬సҠԹ౓ (Tc ) ෇ۙʹͳΔͱ‫্ʹܹٸ‬ঢ͠ɺߴԹʹͳΔʹͭΕͯࣗ༝৔ͷ݁Ռ (2πT ) ʹԼ͔Β͍ۙͮͨɻԹ౓͕

T  2.5Tc (400[MeV]) ఔ౓Ͱ΋ࣗ༝৔͔ΒͷͣΕ͸େ͖͍͜ͱ͔Βɺด͡ࠐΊ૬సҠͷ‫Ͱޙ‬΋ɺΫΥʔΫͷࣗ༝Ψεͱ͍͏ඳ૾͕੒Γཱͨͳ͍͜ͱ͕ࣔࠦ͞Εͨɻ࣍ʹɺ֨ࢠ

QCD ‫ࢉܭ‬ͷ݁Ռͱൺֱ͢Δ͜ͱͰɺ༗ޮ໛‫ݶ੍ʹܕ‬Λ༩͑ΒΕΔ͔‫ݕ‬౼ͨ͠ɻEPNJL໛‫ܕ‬ͷ entanglement ݁߹ͷ‫͞ڧ‬Λௐ੔͢Δ͜ͱͰɺ֨ࢠ QCD ‫ࢉܭ‬Λఆྔతʹ࠶‫͢ݱ‬ΔΑ͏ͳ݁߹ͷ‫͞ڧ‬ΛܾఆͰ͖ͨɻࠓ‫ޙ‬͸ɺଞͷϝιϯःณ࣭ྔʹର͢Δ֨ࢠ QCD ͷ݁Ռͱൺֱ͠ɺ͞Βʹ৴པੑͷߴ͍༗ޮ໛‫ܕ‬Λߏங͢Δɻຊ‫ڀݚ‬͸ੴҪࢯΛத৺ʹਪਐ͞Εɺम࢜࿦จͱͯ͠వΊΒΕͨɻͦͷ੒Ռ͸ PhysicalReview ࢽʹ‫͞ࡌܝ‬ΕͨɻϕΫτϧ‫ܕ‬૬‫ ͕༻࡞ޓ‬QCD ૬ਤͷ༗‫ྖ౓ີݶ‬Ҭʹ‫͢΅ٴ‬Ө‫ڹ‬ͷ‫( ڀݚ‬ീਘਖ਼৴, Տ໺޺໌ [ࠤլେֶ], ߴ‫ڮ‬७Ұ (D1), ੴҪ༏େ (M2), ؅໺३ฏ (M1))

QCD ૬ਤͷ༗‫( ౓ີݶ‬༗‫ݶ‬ΫΥʔΫԽֶϙςϯγϟϧ (μq )) ྖҬͰ͸ූ߸໰୊ͷͨΊɺୈҰ‫ݪ‬ཧ‫͋Ͱࢉܭ‬Δ֨ࢠ QCD ‫ࢉܭ‬Λߦ͏͜ͱ͸ࠔ೉Ͱ͋Δɻͦ͜Ͱɺ༗ޮ໛‫ܕ‬Λ༻͍ͯ༗‫ྖ౓ີݶ‬ҬͰͷ‫ࢉܭ‬Λߦ͏͜ͱ͕ॏཁͱͳΔɻͦͷࡍɺ৴པੑͷߴ͍‫ࢉܭ‬Λߦ͏ͨΊʹ͸ɺෆఆੑ͕Ͱ͖Δ͚ͩഉআ͞Εͨ༗ޮ໛‫ܕ‬Λ࢖༻͢Δ͜ͱ͕๬·ΕΔɻ͜ͷΑ͏ͳ༗ޮ໛‫ܕ‬Λߏங͢Δ͜ͱ͸ɺ֨ࢠ QCD ͕࣮ߦՄೳͳྖҬʹண໨͠ɺ֨ࢠ

QCD ‫ͱࢉܭ‬༗ޮ໛‫ܕ‬ͷ‫ͦࢉܭ‬ΕͧΕΛൺֱ͢Δ͜ͱΛཁ‫͢ٻ‬Δɻූ߸໰୊͕ͳ͍ྖҬͰ͋Δθϩີ౓ɾ༗‫ݶ‬Թ౓ྖҬʹ͓͍ͯɺ֨ࢠ QCD ͷ‫݁ࢉܭ‬ՌΛ͢΂ͯ࠶‫͢ݱ‬Δ༗ޮ໛‫ ͯ͠ͱܕ‬Entanglement Polyakov-loop extended Nambu-Jona-Lasinio(EPNJL) ໛‫ܕ‬
͕͋Δɻզʑ͸ EPNJL ໛‫ܕ‬Λग़ൃ఺ͱ͠ɺ༗‫ྖ౓ີݶ‬Ҭʹ͓͚Δ 2 ϑϨʔόʔ‫ܥ‬Λߟ࡯ͨ͠ɻ༗‫ྖ౓ີݶ‬ҬͰ͸ΫΥʔΫؒʹ৽ͨʹϕΫτϧ‫ܕ‬૬‫͕༻࡞ޓ‬͸ͨΒ͖ɺΫΥʔΫɾϋ

15υϩϯ૬సҠઢͷҐஔ΍ΫΥʔΫ෺࣭ͷঢ়ଶํఔࣜʹେ͖͘Ө‫͢ڹ‬Δ͜ͱ͕஌ΒΕ͍ͯΔɻͦ͜Ͱզʑ͸ɺϕΫτϧ‫ܕ‬૬‫༻࡞ޓ‬Λ‫ؚ‬ΉΑ͏ʹ 2 ϑϨʔόʔ EPNJL ໛‫ܕ‬Λ֦ு͠ɺϕΫτϧ‫ܕ‬૬‫༻࡞ޓ‬ͷ‫ ͞ڧ‬Gv Λܾఆ͢Δ͜ͱΛ໨ඪͱͨ͠ɻGv ͷܾఆΛߦ͏ʹ͋ͨͬͯɺզʑ͸ μq /T (T ͸Թ౓) ʹ͓͍ͯΫΥʔΫ਺ີ౓͕֨ࢠ QCD ʹ‫ܭ͖ͮج‬ࢉ͞Ε͍ͯΔ͜ͱʹண໨ͨ͠ɻ͔͠͠ɺΫΥʔΫ਺ີ౓ࣗ਎͸ූ߸໰୊ͷӨ‫͕ܰڹ‬ඍͳ௿ີ౓ྖҬͰ͸খ͞ͳ஋ΛऔΔͨΊɺGv ͷਫ਼ີͳܾఆʹ͸ෆ޲͖Ͱ͋Δɻͦ͜Ͱɺ
ΫΥʔΫ਺ີ౓Λ Stefan-Boltzmann ‫Ͱݶۃ‬ͷ஋Ͱ‫֨ن‬Խͨ͠෺ཧྔΛఆٛͨ͠ɻզʑ
͸ɺ͜ͷ෺ཧྔ͕ූ߸໰୊͕ͳ͍θϩີ౓ྖҬͰ΋༗‫͋Ͱݶ‬Δ͜ͱΛൃ‫͠ݟ‬ɺ͜Εʹ‫͖ͮج‬ɺैདྷ্‫ݶ‬΋͘͠͸Լ‫ܾ͔͠ݶ‬ΊΒΕ͍ͯͳ͔ͬͨ Gv ΛҰҙతʹܾఆͨ͠ɻ
ࠓ‫ޙ‬͸ɺಘΒΕͨ Gv ͕ΫΥʔΫɾϋυϩϯ૬సҠઢͷҐஔʹ‫͢΅ٴ‬Ө‫ڹ‬ͷఆྔతͳධՁʹՃ͑ɺதੑࢠ੕಺෦ʹ͓͍ͯΫΥʔΫɾϋυϩϯ૬సҠ͕‫͍ͯͬ͜ى‬Δ͔Λߟ࡯͠ɺʮଠཅ࣭ྔͷ 2 ഒͷ࣭ྔΛ΋ͭதੑࢠ੕ʯͷ‫؍‬ଌࣄ࣮ͱໃ६͠ͳ͍ΫΥʔΫ෺࣭ͷঢ়ଶํఔࣜͷߏஙΛ໨ࢦ͢ɻຊ‫ڀݚ‬͸؅໺ࢯΛத৺ʹਪਐ͞Ε͍ͯΔɻNJL ໛‫͚͓ʹܕ‬Δਖ਼ଇԽ๏ґଘੑͷ‫( ڀݚ‬ീਘਖ਼৴, Տ໺޺໌ [ࠤլେֶ], ࠤʑ໦ਸ޺
(D3), ੴҪ༏େ (M2), ถଜߒ࢘ (M1))ɹ ۙ೥ɺQCD ૬ਤͷղ໌Λ໨ࢦͨ͠‫͕ڀݚ‬੝ΜʹߦΘΕ͍ͯΔ͕ɺQCD ͷୈҰ‫ݪ‬ཧ‫͋Ͱࢉܭ‬Δ֨ࢠ QCD ‫ࢉܭ‬͸༗‫ݶ‬ԽֶϙςϯγϟϧྖҬͰ͸ූ߸໰୊Λ࣋ͪɺ‫ࢉܭ‬ࠔ೉Ͱ͋Δɻ͜ͷͨΊɺ༗ޮ໛‫ܕ‬Λ༻͍ͨ QCD ૬ਤͷղੳ͕ߦΘΕ͍ͯΔɻ༗ޮ໛‫ͱܕ‬͸ɺ࠷ॳʹΧοτΦϑεέʔϧΛಋೖ͠ɺͦͷΧοτΦϑεέʔϧΑΓ௿͍ΤωϧΪʔεέʔϧͷ‫ݱ‬৅Λ‫ه‬ड़͢Δ໛‫͋Ͱܕ‬ΔɻQCD ૬ਤͷղ໌ʹ͠͹͠͹༻͍ΒΕΔ

Nambu-Jona-Lasino(NJL) ໛‫Ͱܕ‬͸ɺ3 ࣍‫ݩ‬ӡಈྔΧοτ͕௨ৗ༻͍ΒΕΔɻ͔͠͠ɺ
͜ͷΧοτΦϑ͸ Lorentz ෆมੑΛյ͢ͱ͍͏ܽ఺Λ͍࣋ͬͯΔɻͦ͜Ͱզʑ͸ LorentzෆมੑΛյ͞ͳ͍ਖ਼ଇԽͷํ๏ͱͯ͠ Pauli-Villars ਖ਼ଇԽ΋औΓ্͛ͨɻͦͯ͠ɺΧΠϥϧ૬సҠ΍ด͡ࠐΊ૬సҠͷΦʔμʔύϥϝʔλʢΧΠϥϧ‫ڽ‬ॖɺPolyakov loopʣɺঢ়ଶํఔࣜͷਖ਼ଇԽґଘੑΛௐ΂༗ޮ໛‫ܕ‬ͷଥ౰ੑΛ෼ੳͨ͠ɻ͜ͷղੳʹΑͬͯɺ3࣍‫ݩ‬ӡಈྔΧοτͱ Pauli-Villars ਖ਼ଇԽΛ༻͍ͨ৔߹ͱͰߴԹྖҬʹ͓͍ͯҟͳΔৼ
Δ෣͍Λ͢Δ͜ͱ͕෼͔ͬͨɻ
ຊ‫ڀݚ‬͸ถଜࢯΛத৺ʹਪਐ͞Ε͍ͯΔɻ
ΞΠίφʔϧ൓Ԡཧ࿦ʹΑΔ 6 He ͷ 2 தੑࢠണ཭൓Ԡͷ‫ه‬ड़ (ീਘਖ਼৴ɺদຊୖຏɺॹ
ํҰհ [େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔ।‫ڭ‬त]ɺຸໜ޻ক (PD)ɺߐ಄‫( ܛ‬M2))ɹΞΠίφʔϧ൓Ԡཧ࿦ (ERT) ͸ɺ‫۝‬େάϧʔϓʹΑͬͯఏএ͞Εͨ֩ࢠണ཭൓ԠΛ‫ه‬ड़͢Δཧ࿦Ͱ͋Δɻಉ֩͘͡ࢠണ཭൓ԠΛ‫ه‬ड़͢Δ Glauber ໛‫ͱܕ‬ൺֱͯ͠ɺERT

16

ʹ͸ Coulomb ૬‫༻࡞ޓ‬Λਖ਼֬ʹऔΓѻ͑Δར఺͕͋Δɻࠓ೥౓͸ɺ6 He ͷ 2 தੑࢠണ཭൓Ԡͷղੳʹ͓͍ͯ ERT ͱ Glauber ໛‫ࢉܭܕ‬Λൺֱ͠ɺCoulomb ૬‫༻࡞ޓ‬ͷऔΓѻ͍ͷࠩΛௐ΂ͨɻͦͷ݁ՌɺCoulomb ෼ղաఔ͕ॏཁ
ͱͳΔೖࣹΤωϧΪʔ͕௿͍৔߹΍ඪత͕֩ॏ͍৔߹ͷ൓ԠͰɺGlauber ໛‫ͱܕ‬ͷେ͖ͳҧ͍͕‫ݟ‬ΒΕͨɻERT Λ༻͍Ε͹ɺௐઅύϥϝʔλΛಋೖ͢Δ͜ͱͳ͘ɺ6 He ͷ

2 தੑࢠണ཭൓Ԡͷஅ໘ੵΛඇৗʹྑ͘࠶‫͢ݱ‬Δɻ͜ͷ੒ՌΛ࿦จʹ·ͱΊɺ‫ ࡏݱ‬Physical Review C ࢽʹ౤ߘதͰ͋Δɻຊ‫ڀݚ‬͸ຸໜࢯͱߐ಄ࢯΛத৺ʹਪਐ͞Εͨɻՙిަ‫׵‬൓ԠͷղੳʹΑΔதੑࢠεΩϯްͷܾఆ (ീਘਖ਼৴ɺຸໜ޻ক (PD))ɹதੑࢠεΩϯްͷղੳʹ༗ྗͳํ๏ͷͻͱͭͱͯ͠ɺΞΠιόϦοΫΞφϩάঢ়ଶ(IAS) Λྭ‫͢ى‬Δՙిަ‫׵‬൓Ԡ (p,n)IAS ͕஫໨͞Ε͍ͯΔɻ(p,n)IAS ͸ɺΞΠιεϐ
ϯରশੑͷԼʹཅࢠ஄ੑࢄཚͱ౳Ձͳ൓ԠͰ͋ΓɺޫֶϙςϯγϟϧͷΞΠιϕΫτ
ϧ੒෼ʹ‫͘ڧ‬ґଘ͢Δͱߟ͑ΒΕΔɻຊ‫Ͱڀݚ‬͸ɺ͜ͷ (p,n)IAS Λ৞ΈࠐΈ໛‫ܕ‬Λ༻͍ͨඍࢹత൓Ԡཧ࿦ʹΑͬͯղੳ͠ɺதੑࢠεΩϯްΛਫ਼ີʹܾఆ͢Δ͜ͱΛ໨ࢦ͢ɻࠓ೥౓͸ɺ͞·͟·ͳඪత֩ɾೖࣹΤωϧΪʔʹର͢Δ (p,n)IAS Λ‫ܥ‬౷తʹղੳͨ͠ɻͦͷ݁Ռɺඪత͕͍֩ܰ৔߹ʹ͸࣮‫ݧ‬Λྑ͘࠶‫͢ݱ‬Δ͕ɺඪత͕֩ॏ͍৔߹ʹ͸࣮‫ͱݧ‬ͷͣΕ͕‫ݟ‬ΒΕͨɻ࣮‫ͱݧ‬ͷͣΕ͸ɺඪత͕֩ॏ͘ͳΔ΄Ͳ‫ݦ‬ஶͰ͋Δɻ·ͨɺ͜Ε͸ೖࣹΤωϧΪʔʹΑΒͣ‫ݟ‬ΒΕΔ܏޲Ͱ͋Δ͜ͱ͕෼͔ͬͨɻ͋Δఔ౓ॏ͍֩
Ͱͳ͚Ε͹தੑࢠεΩϯްͱͯ͠ͷҙຯΛ࣋ͨͳ͍ͨΊɺॏ͍ඪత֩Ͱ࣮‫ͱݧ‬ͷͣΕ͕ੜ͡Δ͜ͱ͸ඇৗʹେ͖ͳ໰୊Ͱ͋Δɻࠓ‫ޙ‬͸ɺ(p,n)IAS ͷ൓Ԡ‫ߏػ‬ΛΑΓৄ͘͠ௐ΂ɺ࣮‫ͱݧ‬ͷͣΕͷ‫ݪ‬ҼΛ໌Β͔ʹ͢Δɻຊ‫ڀݚ‬͸ຸໜࢯΛத৺ʹਪਐ͞Ε͍ͯΔɻ

1 தੑࢠണ཭൓ԠΛར༻ͨ͠ E1 ෼ղஅ໘ੵͷಋग़ (ຸໜ޻ক (PD)ɺॹํҰհ [େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔ।‫ڭ‬त]ɺ෱Ҫಙ࿕ [େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔ (D2)]ɺ٢ా਺‫[ و‬େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔ (M1)])
ɹ E1 ෼ղஅ໘ੵͷେ͖͞͸֩ͷ޿͕Γʹ‫͘ڧ‬ґଘ͢ΔͨΊɺ͕֩ϋϩʔ֩Ͱ͋Δ͔Ͳ͏͔ΛܾΊΔͻͱͭͷࢦඪͱߟ͑ΒΕ͍ͯΔɻ͔͠͠ɺ࣮‫ Ͱݧ‬E1 ෼ղஅ໘ੵΛଌఆ͢Δ͜ͱ͸ෆՄೳͰ͋ΔͨΊɺ12 C ͱ 208 Pb ͷҟͳΔඪతʹରͯ͠ 1 தੑࢠണ཭൓Ԡͷஅ໘ੵΛଌఆ͠ɺ12 C ඪతͷஅ໘ੵΛద౰ʹεέʔϦϯάͯ͠ 208 Pb ඪతͷஅ໘ੵ͔Βࠩ͠Ҿ͘͜ͱͰɺE1 ෼ղஅ໘ੵ͕‫ੵݟ‬΋ΒΕ͍ͯΔɻ͜ͷࡍͷεέʔϦϯάҼࢠ͸‫ݧܦ‬తʹܾΊΒΕͨ΋ͷ͕༻͍ΒΕΔ͕ɺͦͷཧ࿦తࠜ‫͕ڌ‬ఆ͔Ͱͳ্͍ɺෆఆੑ͕‫ۃ‬Ίͯେ͖͍ɻͦͷͨΊɺεέʔϦϯά๏ͷଥ౰ੑΛཧ࿦తʹ͔֬ΊΔඞཁ͕͋Δɻຊ‫Ͱڀݚ‬͸ɺεέʔϦϯά๏ʹΑͬͯ‫ٻ‬ΊΒΕΔ E1 ෼ղஅ໘ੵͷଥ౰ੑΛɺΞΠί17φʔϧ൓Ԡཧ࿦ͱ࿈ଓঢ়ଶ཭ࢄԽνϟωϧ݁߹๏Λ༻͍ͯௐ΂ͨɻ͜ΕΒͷख๏Λ༻͍Ε͹ɺཧ࿦‫ࢉܭ‬ͷൣғ಺ͰɺE1 ෼ղஅ໘ੵͱεέʔϦϯά๏ʹΑͬͯ‫ٻ‬Ίͨۙࣅతஅ໘ੵΛ௚઀ൺֱͰ͖ΔɻͦͷΑ͏ͳղੳͷ݁ՌɺεέʔϦϯάҼࢠ͸֩ͷ 1 தੑࢠ෼཭ΤωϧΪʔʹ‫͘ڧ‬ґଘ͢Δ͜ͱ͕෼͔Γɺ·ͨɺεέʔϦϯά๏Λ༻͍࣮ͯ‫ݧ‬తʹܾΊΒΕͨ 31 Ne ͷ E1 ෼ղஅ໘ੵ͕ɺཧ࿦஋ΑΓ 13–20%΋େ͖͍͜ͱΛࣔͨ͠ɻ͜ͷ݁Ռ͸࿦จͱͯ͠·ͱΊΒΕɺProgress of Theoretical and Experimental Physicsࢽ΁ͷ‫ܾ͕ࡌܝ‬ఆͨ͠ɻ

1 ֩ࢠണ཭൓ԠͷղੳʹΑΔ 30 Ne ͷ෼ޫֶతҼࢠͷܾఆ (ຸໜ޻ক (PD)ɺJenny Lee[ཧԽֶ‫ॴڀݚ‬ਔՊՃ଎‫ڀݚث‬ηϯλʔ‫ڀݚ‬һ]ɺ໦ଜਅ໌ [๺ւಓେֶ।‫ڭ‬त]ɺӉ౎໺য়[೔ຊ‫ڀݚߏػྗࢠݪ‬һ]ɺॹํҰհ [େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔ।‫ڭ‬त])
ɹ 30 Ne ͷ‫ج‬ఈঢ়ଶ͸ɺ29 Ne(ਊ֩) ͷ͞·͟·ͳঢ়ଶʹதੑࢠ͕݁߹ͨ͠഑ҐͷॏͶ߹Θͤͱͯ͠‫ه‬ड़Ͱ͖Δɻ෼ޫֶతҼࢠͱ͸ɺ͜ΕΒͷ഑Ґͷׂ߹Λࣔ͢ࢦඪͰ͋Δɻऑ
ଋറ֩ͷ 1 ֩ࢠണ཭൓Ԡͷஅ໘ੵ͸഑Ґͷҧ͍ʹରͯ͠ඇৗʹහ‫͋Ͱײ‬ΔͨΊɺ͜ΕΛར༻ͯ͠ɺ30 Ne ʹ͓͚Δਊ֩ͱதੑࢠͷ഑Ґɺ͓Αͼͦͷ෼ޫֶతҼࢠΛܾఆ͢Δ
͜ͱ͕Ͱ͖Δɻ͜ͷͱ͖ɺ1 ֩ࢠണ཭൓Ԡʹ͓͍ͯ์ग़͞ΕΔΨϯϚઢͷΤωϧΪʔΛಉ࣌ʹଌఆ͢Ε͹ɺਊ֩ͷ֤ঢ়ଶͷྭ‫ى‬ΤωϧΪʔͱରԠ͚ͮͯٞ࿦Ͱ͖Δɻຊ‫Ͱڀݚ‬͸ɺΞΠίφʔϧ൓Ԡཧ࿦Λ༻͍ͯ 30 Ne ͷ 1 ֩ࢠണ཭൓ԠΛղੳ͠ɺ30 Neʹ‫·ؚ‬ΕΔ഑Ґͷ෼ޫֶతҼࢠͱɺਊ֩ 29 Ne ͷεϐϯɾύϦςΟΛௐ΂ͨɻ൓Ԡ‫ࢉܭ‬ʹඞཁͳ 30 Ne ͷ഑ҐΛ‫ه‬ड़͢Δߏ଄໛‫ͯ͠ͱܕ‬ɺ֪໛‫ͱܕ‬൓ରশԽ෼ࢠಈྗֶͷ 2 ͭΛ࠾༻ͨ͠ɻ2 ͭͷ໛‫͕ܕ‬༩͑Δஅ໘ੵͷ‫ࢉܭ‬஋ͱ࣮‫ݧ‬஋Λൺֱ͠ɺ֤഑Ґʹ͓͚Δ෼
ޫֶతҼࢠΛ͓͓Αͦ‫ੵݟ‬΋Δ͜ͱ͕Ͱ͖ͨɻ͞Βʹɺ29 Ne ͷ‫ج‬ఈঢ়ଶͷεϐϯɾύϦςΟ͸ 3/2+ ͱ݁࿦͚ͮΒΕͨɻ‫ࡏݱ‬ɺLee ࢯ͕த৺ͱͳΓɺ͜ͷ݁ՌΛ࿦จʹ·ͱΊ͍ͯΔɻ
൓Ԡஅ໘ੵͷղੳͰ୳Δதੑࢠա৒ Mg ಉҐମͷ‫ج‬ఈঢ়ଶͷੑ࣭ (ീਘਖ਼৴ɺਗ਼ਫྑ
จɺদຊୖຏɺ໦ଜਅ໌ [๺ւಓେֶ।‫ڭ‬त]ɺ෢ஐຑ໹ [ཧ‫ݚ‬ਔՊηϯλʔɺυΠπॏΠΦϯ‫]ॴڀݚ‬ɺ෱ాޫॱ [େࡕେֶ।‫ڭ‬त]ɺ੢ଜଠथ [౦‫ژ‬ཧՊେֶॿ‫]ڭ‬ɺླ໦݈ [࡛‫ۄ‬େֶ‫ڭ‬त]ɺຸໜ޻ক (PD)ɺా্ਅ‫( ޔ‬D2)ɺౢాॆ޺ (D1)ɺ౉ᬒ৻ (D1))ɹཧԽֶ‫ॴڀݚ‬ͷ࣮֩‫ࢪݧ‬ઃ (RIBF) ʹΑͬͯ৽‫ͳح‬σʔλ͕஝ੵ͞Ε͍ͯΔࡢࠓɺ
ʠ island of inversion ʡʹؔ͢Δ‫͕ڀݚ‬վΊͯ஫໨ΛूΊ͍ͯΔɻisland of inversion ͸֩ਤදʹ͓͚Δཅࢠ਺͕ 10∼12 (Ne, Na, Mg)ɺதੑࢠ਺͕ 20∼22 ఔ౓ͷྖҬͰ͋ΓɺྖҬ಺ͷ‫֩ࢠݪ‬͸ʮຐ๏਺ͷഁΕʯ΍ʮҟৗͳม‫ܗ‬ʯͱ͍ͬͨ҆ఆ֩Ͱ͸‫ݟ‬ΒΕͳ͍ੑ࣭Λࣔ͢ɻۙ೥ଌఆ͞Εͨ Mg ಉҐମʹର͢Δ൓Ԡஅ໘ੵʢ‫͕֩ࢠݪͱ֩ࢠݪ‬িಥ͢Δ֬཰ʹରԠͨ͠෺ཧྔʣ΋ྫ֎Ͱ͸ͳ͘ɺ҆ఆ͔֩Βͷ༧૝ΑΓ΋ҟৗʹେ͖͍͜18

ͱ͕ใࠂ͞Ε͍ͯΔɻ
զʑ͸൓ରশԽ෼ࢠಈྗֶ๏ (AMD) ʹΑΓ‫͞ࢉܭ‬Εͨ֩ີ౓ΛΠϯϓοτͱͨ͠ೋॏ৞ΈࠐΈ໛‫ܕ‬Λ༻͍ͯɺଌఆ͞Εͨ Mg ಉҐମʹର͢Δ൓Ԡஅ໘ੵͷཧ࿦తղੳ
Λߦͬͨɻզʑͷ༻͍ͨ͜ͷख๏͸ɺ‫ߏ֩ࢠݪ‬଄ʹԾఆΛஔ͔ͳ͍ඍࢹతཧ࿦Ͱ͋ΔɻAMD ‫ࢉܭ‬ͷ݁Ռɺ31−40 Mg ʹରͯ͠େ͖ͳม‫ݱ͕ܗ‬ΕɺͦΕΛ൓өͯ͠൓Ԡஅ໘ੵͷ࣮‫ݧ‬σʔλΛ֓ͶΑ͘࠶‫ͨ͠ݱ‬ɻ͜ͷ݁Ռ͸ island of inversion Λ௒͑ͨྖҬʹ͓͍ͯ΋େ͖ͳม‫͕ܗ‬ଓ͍͍ͯΔ͜ͱΛҙຯ͓ͯ͠ΓɺN = 20 ͷຐ๏਺ͷΈͳΒͣɺN = 28ͷຐ๏਺΋ഁΕ͍ͯΔ͜ͱΛ‫͍ͯࠦࣔ͘͠ڧ‬ΔɻҰํɺυϦοϓϥΠϯۙ๣֩Ͱ͋Δ37

Mg ʹରͯ͠͸࣮‫ݧ‬σʔλΛաখධՁ͓ͯ͠Γɺ͜ͷ݁Ռ͸ 37 Mg ͕ϋϩʔߏ଄Λ࣋ͭ͜ͱΛ͍ࣔࠦͯ͠Δɻ࣮ࡍɺΫʔϩϯ෼ղ൓Ԡͷஅ໘ੵ͔Β΋ 37 Mg ͸ʮม‫ܗ‬ϋϩʔʯ
Ͱ͋Δ͜ͱ͕ࣔࠦ͞Ε͓ͯΓɺ‫ࡏݱ‬ͷ AMD ͷ໛‫ۭؒܕ‬͸ 37 Mg Λ‫ه‬ड़͢Δͷʹे෼Ͱͳ͍Մೳੑ͕͋Δɻࠓ‫ޙ‬ɺߋʹେ͖ͳ໛‫ۭؒܕ‬Λ༻ҙͨ͠‫ࢉܭ‬Λߦ͏ඞཁ͕͋Δɻ

Mg ಉҐମʹର͢Δ͜ͷղੳ͸ EPJ Web of Conferences ʹ‫͞ࡌܝ‬Εɺߋʹ PhysicalReview ʹ΋౤ߘதͰ͋Δɻདྷ೥౓͸൓Ԡஅ໘ੵͷଌఆ͕‫ʹط‬ऴΘ͍ͬͯΔ Na ΍ Al ಉҐମʹରͯ͠ಉ༷ͷղੳΛߦ͍ɺisland of inversion શମΛ၆ᛌ͢Δɻຊ‫ڀݚ‬͸౉ᬒࢯΛத৺ʹਪਐ͞Εͨɻ
6

He 2+
1 ͔Βͷ 2 தੑࢠ่յͷ‫( ڀݚ‬٠஍ӈഅ [େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔ‫ڀݚ‬һ]ɺদ

ຊୖຏɺຸໜ޻ক (PD)ɺॹํҰհ [େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔ।‫ڭ‬त])
ɹ 6 He ͸ 2 தੑࢠϋϩʔߏ଄Λ΋ͭͱ͞Ε͍ͯΔɻ2 தੑࢠϋϩʔ֩ʹ͓͍ͯ 2 தੑࢠ૬ؔͷ‫ڀݚ‬͸ਫ਼ྗతʹਐΊΒΕ͍ͯΔɻຊ‫Ͱڀݚ‬͸ 6 He ͷྭ‫ڞى‬໐ঢ়ଶ 2+
1 ͔Βͷ 2 தੑࢠ่յϞʔυΛ֩ࢠ͋ͨΓ 240 MeV ͷ 6 He+12 C ࢄཚղੳ͔Βௐ΂ͨɻ͜ͷղੳʹ͓͍ͯ෼ղஅ໘ੵ‫ࢉܭ‬Λ CDCC ๏ʹΑΓদຊࢯ͕ɺͦͷ‫ʹࢉܭ‬ඞཁͳޫֶϙςϯγϟϧ
ͷ‫ࢉܭ‬Λຸໜࢯ͕୲౰ͨ͠ɻྭ‫ڞى‬໐ঢ়ଶ͔Βͷ 2 தੑࢠ่յϞʔυ͸େࡕେֶ֩෺
ཧ‫ڀݚ‬ηϯλʔͷ٠஍ࢯ͕‫ͨ͠ࢉܭ‬ɻຊղੳʹΑΓɺ2+
1 ঢ়ଶʹ͓͚Δ 2 தੑࢠ૬ؔͷଘࡏ͕֬ೝ͞Εͨɻຊ‫ڀݚ‬͸େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔͷ٠஍ࢯʹΑΓਪਐ͞Εɺͦͷ੒Ռ͸ PhysicalReview C ࢽʹ‫͞ࡌܝ‬Εͨɻ
6

Li ೖࣹ൓Ԡʹ͓͚Δ෼ղޮՌͷ‫ܥ‬౷తղੳ (ീਘਖ਼৴ɺদຊୖຏɺॹํҰհ [େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔ।‫ڭ‬त]ɺຸໜ޻ক (PD)ɺ౉ᬒ৻ (D1))ɹຊ‫ڀݚ‬ͷର৅Ͱ͋Δ 6 Li ͸ɺதੑࢠ (n)ɺཅࢠ (p)ɺ4 He ͷ 3 ͭͷཻࢠ͕ͦΕͧΕ؇͘ଋറͨ͠‫ͱ֩ࢠݪ‬Έͳ͢͜ͱ͕Ͱ͖Δɻ͜ͷΑ͏ͳऑଋറͳ‫͕֩ࢠݪ‬ೖࣹ͢Δ൓ԠͰ͸ɺ൓Ԡͷ్தͰೖࣹ͕֩෼ղ͢Δաఔ͕ॏཁͱͳΓɺͦͷޮՌΛਫ਼ີʹऔΓѻ͏͜ͱ͕ඞਢͱͳΔɻຊ‫Ͱڀݚ‬͸ɺ4 ମ࿈ଓঢ়ଶ཭ࢄԽνϟωϧ݁߹๏ (4 ମ CDCC) Λ༻

19

͍ɺ6 Li ͕ 3 ͭͷཻࢠ (n, p, 4 He) ʹ෼ղ͢ΔޮՌΛཅʹऔΓೖΕͨ‫ࢉܭ‬Λߦͬͨɻલ೥౓·Ͱͷ‫Ͱڀݚ‬ɺզʑ͸ʮ௿ΤωϧΪʔೖࣹͷ 6 Li + 209 Bi ஄ੑࢄཚʹ͓͍ͯɺ
6

Li ಺෦ͷ d(ॏཅࢠ) ͕ n ͱ p ʹ෼ղ͢ΔޮՌ͸ແࢹͰ͖Δʯͱ͍͏ఏҊΛͨ͠ɻຊ೥౓

͸ɺ͜ͷఏҊ͕ 6 Li ࢄཚʹ͓͍ͯߋʹීวతͳ΋ͷɺ͢ͳΘͪʮ6 Li ࢄཚʹ͓͍ͯɺ6 Li
಺෦ͷ d ͕ n ͱ p ʹ෼ղ͢ΔޮՌ͸ແࢹͰ͖Δʯ͔Λ‫͢ূݕ‬ΔͨΊɺ4 ମ CDCC Λ༷ʑͳ৚݅ԼͰద༻ͨ͠ɻ۩ମతʹ͸ɺ௿ΤωϧΪʔ (∼20 MeV)ɾதؒΤωϧΪʔ (∼70

MeV)ɾߴΤωϧΪʔ (∼240 MeV) ೖࣹͷɺ͍ܰඪత֩ (12 C)ɾதॏඪత֩ (58 Ni)ɾॏ͍
ඪత֩ (208 Pb) ʹΑΔ 6 Li ஄ੑࢄཚͰ͋Δɻద༻ͨ݁͠Ռɺ208 Pb ඪతʹ͓͍ͯ͸શΤωϧΪʔྖҬͰ࣮‫ݧ‬σʔλΛΑ͘࠶‫͠ݱ‬ɺ͞Βʹɺ58 Ni ඪతʹ͓͍ͯ΋௿ɾதؒΤωϧΪʔྖҬͰ࣮‫ݧ‬σʔλΛΑ͘࠶‫ͨ͠ݱ‬ɻ͔͠͠ҰํɺߴΤωϧΪʔʹ͓͚Δ 58 Ni ඪతࢄཚ΍ɺதɾߴΤωϧΪʔʹ͓͚Δ 12 C ࢄཚʹ͓͍ͯ͸ 4 ମ CDCC ͸࣮‫ݧ‬Λ࠶‫͠ݱ‬͓ͯΒͣɺৄࡉͳղੳʹࢸ͍ͬͯͳ͍ɻશମͷ܏޲ͱͯ͠ɺΫʔϩϯྗ͕ओཁͳ૬‫ޓ‬࡞༻ͱͳΔॏ͍ඪత֩΍௿ΤωϧΪʔࢄཚʹ͓͍࣮ͯ‫ݧ‬σʔλΛ࠶‫͠ݱ‬ɺ֩ྗ͕ओཁ
ͳ૬‫ͳͱ༻࡞ޓ‬Δ͍ܰඪత֩΍ߴΤωϧΪʔࢄཚʹ͓͍࣮ͯ‫ݧ‬σʔλΛ࠶‫ͳ͍ͯ͠ݱ‬͍Α͏Ͱ͋Δɻࠓ‫ޙ‬͸ɺ͜ͷ‫ݪ‬Ҽղ໌Λ໨ඪͱ͢Δɻຊ‫ڀݚ‬͸౉ᬒࢯΛத৺ʹਪਐ͞Εͨɻೋॏ৞ΈࠐΈ໛‫ܕ‬Λ༻͍ͨ 4 He-֩஄ੑࢄཚͷղੳ (ീਘਖ਼৴ɺদຊୖຏɺຸໜ޻ক (PD)ɺ
ߐ಄‫( ܛ‬M2)ɺ๛઒কҰ (M2))ɹ֩ྗʹ‫ͮ͘ج‬ඍࢹత൓Ԡཧ࿦͸ɺ͜Ε·Ͱʹଟ͘ͷ੒ޭΛऩΊ͖ͯͨɻྫ͑͹ɺ֩ࢠ-֩ࢄཚͷஅ໘ੵ΍ภ‫ྔۃ‬ɺ֩-֩ࢄཚͷશ൓Ԡஅ໘ੵͳͲ͸࣮‫ݧ‬ΛΑ͘࠶‫͢ݱ‬Δɻ͠
͔͠ɺ֩-֩ࢄཚͷஅ໘ੵ΍ 4 He-֩ࢄཚ͸ඍࢹత൓Ԡཧ࿦Ͱ‫ܥ‬౷తʹ࣮‫ݧ‬Λ࠶‫ͳ͖Ͱݱ‬͍ͳͲͷ͍͔ͭ͘ͷ໰୊Λ࢒͍ͯ͠Δɻ
ɹೋॏ৞ΈࠐΈ໛‫ܕ‬͸ɺ2 ֩ࢠؒ༗ޮ૬‫( ༻࡞ޓ‬g ߦྻ૬‫ )༻࡞ޓ‬Λೖࣹ֩ີ౓ ρP ͱඪత֩ີ౓ ρT Ͱ৞ΈࠐΉ͜ͱʹΑΓɺ֩-֩ؒͷϙςϯγϟϧΛඍࢹతʹ‫ٻ‬ΊΔख๏Ͱ͋Δɻg ߦྻ૬‫༻࡞ޓ‬͸֩෺࣭தͰͷີ౓ґଘੑΛ࣋ͭ૬‫͋Ͱ༻࡞ޓ‬Γɺg ߦྻ૬‫༻࡞ޓ‬Λ‫಺֩ࢠݪ‬ͷ֩ࢠʹద༻͢Δࡍʹ͸‫ࣅۙ౓ີॴہ‬Λ༻͍Δඞཁ͕͋Δɻ͔͠͠ɺ͜ͷۙࣅ͸ཧ࿦తͳෆఆੑ͕େ͖͘ɺೋॏ৞ΈࠐΈ໛‫౓ີॴہ͍͓ͯʹܕ‬͸௨ৗ ρ = ρP + ρTͱԾఆ͞ΕΔ͕ɺ͜ͷԾఆͷଥ౰ੑ͸ඞͣ͠΋໌֬Ͱ͸ͳ͍ɻɹຊ‫Ͱڀݚ‬͸ 4 He-֩ࢄཚͷ໰୊ͷղܾΛ໨ࢦͨ͠ɻ4 He ͸ඇৗʹྭ‫֩ࢠݪ͍͘ʹ͠ى‬Ͱ͋Γɺ͜ͷੑ࣭ΛऔΓೖΕΔͨΊʹ‫ͯ͠ͱ౓ີॴہ‬ඪత֩ີ౓ͷΈΛ࠾༻͢Δํ๏ΛఏҊͨ͠ɻ͜ͷํ๏Λैདྷͷํ๏ͱൺֱ‫݁ͨ͠ূݕ‬Ռɺಛʹॏ͍ඪత֩ʹରͯ͠ຊ‫Ͱڀݚ‬ఏҊͨ͠ํ๏ʹΑΓɺ࣮‫͕ݧ‬Α͘࠶‫͖Ͱݱ‬Δ͜ͱ͕͔֬ΊΒΕͨɻຊ‫ڀݚ‬͸ߐ಄ࢯΛத৺ʹਪਐ͞Εɺಉࢯͷम࢜࿦จͱͯ͠·ͱΊΒΕͨɻͦͷ੒Ռ͸‫ࡏݱ‬ɺPhysical Review C ࢽʹ౤ߘதͰ͋Δɻ

20

ඍࢹత൓Ԡཧ࿦ʹΑΔ୸ૉಉҐମೖࣹ൓Ԡͷ‫ܥ‬౷తղੳ (ീਘਖ਼৴ɺਗ਼ਫྑจɺদຊୖ
ຏɺ‫ཱݹ‬௚໵ [๺ւಓେֶ]ɺຸໜ޻ক (PD)ɺా্ਅ‫( ޔ‬D2)ɺࠤʑ෦‫( ޛ‬M2))ɹෆ҆ఆ֩ʹ‫ݟ‬ΒΕΔಛ௃ͱͯ͠‫֩ࢠݪ‬ͷີ౓͕ҟৗʹ޿͕ͬͨ Halo ߏ଄͕͋Δɻ

Hartree-Fock-Bogoliubov ๏ʹΑΔղੳʹΑͬͯɺHalo ͷൃୡ͕ର૬ؔྗʹΑͬͯ཈੍͞ΕΔͱ͍͏͜ͱ͕ࣔࠦ͞Ε͍ͯΔɻۙ೥ɺ͜ͷཧ࿦త͕ࣔࠦશ൓Ԡஅ໘ੵͷ‫حۮ‬ੑͱ͍͏‫ݧ࣮Ͱܗ‬తʹ‫͍ͯ͑ݟ‬ΔͷͰ͸ͳ͍͔ͱ͍͏ࢦఠ͕ͳ͞Εͨɻ͔͠͠ɺ൓Ԡஅ
໘ੵͷ‫حۮ‬ੑ͸਺%ͷҧ͍Λࢦ͍ͯ͠ΔͷͰ༷ʑͳӨ‫ڹ‬Λߟྀ͢Δඞཁ͕͋Δɻͦ͜
Ͱɺզʑ͸ඍࢹత൓Ԡཧ࿦Λ༻͍ͯߟ͑ΒΕΔӨ‫ڹ‬ͷதͰ΋ಛʹॏཁͱࢥΘΕΔ֩ഔ
࣭ޮՌͱೖࣹ֩ͷ෼ղޮՌΛ‫ͨ͠ূݕ‬ɻ͜ͷղੳʹΑͬͯɺHalo ֩ʹ͓͚Δഔ࣭ޮՌ͕௨ৗͷ‫֩ࢠݪ‬ͷͦΕͱҟͳΔৼΔ෣͍Λ͢Δ͜ͱ͕෼͔ͬͨɻ·ͨɺઌͷࢦఠΛͨ͠ཧ࿦‫͍͓ͯʹࢉܭ‬͸ແࢹ͞Ε͍ͯͨ෼ղͷޮՌ͕ແࢹͰ͖ͳ͍͜ͱ΋෼͔ͬͨɻ
͜ͷ੒Ռ͸ Physical Review C ࢽʹ‫͞ࡌܝ‬Εͨɻཅࢠ஄ੑࢄཚʹΑΔϋϩʔ֩ͷີ౓෼෍ͷܾఆ (ീਘਖ਼৴ɺদຊୖຏɺ‫ཱݹ‬௚໵ [๺ւಓେֶ]ɺຸໜ޻ক (PD)ɺࠤʑ෦‫( ޛ‬M2))ɹϋϩʔ֩ͷີ౓෼෍Λ୳Δ෺ཧྔͱͯ͠ɺ‫͔͘ݹ‬Β҆ఆ֩ͷີ౓෼෍Λௐ΂Δҝʹ༻͍ΒΕ͖ͯͨೖࣹΤωϧΪʔ਺ඦ MeV/nucleon ͷཅࢠ஄ੑࢄཚͷ֯෼෍͕͋Δɻ͜ͷ֯෼෍ͷ diﬀraction pattern ͸ϋϩʔ֩தͷਊ֩൒‫ͱܘ‬૬͕ؔ͋Δͱ͍͏ࢦఠ͕ͳ
͞Ε͍ͯΔɻۙ೥ɺ࣮‫ٕݧ‬ज़ͷ޲্ʹΑΓ ﬁrst diﬀraction minimum ෇ۙ·Ͱͷେ͖ͳࢄཚ֯ʹ౉ͬͯ֯෼෍ͷଌఆ͕Մೳͱͳͬͨɻ
ͦ͜Ͱɺຊ‫Ͱڀݚ‬͸৽͍࣮͠‫݁ݧ‬Ռ͔Βϋϩʔ֩ 6 He தͷਊ֩ͷঢ়ଶΛௐ΂Δͱͱ΋ʹɺdiﬀraction pattern ͱਊ֩൒‫ܘ‬ͷ૬ؔʹର͢Δ෺ཧతཧղΛ୳‫ͨ͠ٻ‬ɻͦͷ݁Ռɺ
6

He தͷਊ֩͸‫ ཱͨ͠ݽ‬4 He ͱ΄΅ಉ͡ঢ়ଶʹ͋Δ͜ͱ͕֬ೝ͞Εͨɻ·ͨɺ͜ͷೖࣹΤωϧΪʔͷཅࢠ஄ੑ͸ޫֶϙςϯγϟϧͷ‫਺ڏ‬෦෼͕ຊ࣭తͰ͋Δ͜ͱ͕෼͔Γɺ͜Ε͕Ҿ͖‫͢͜ى‬ӨࢄཚΛߟ࡯͢Δ͜ͱʹΑΓ૬ؔʹର͢ΔཧղΛಘͨɻຊ‫ڀݚ‬͸ࠤʑ෦ࢯΛத৺ʹਐΊΒΕɺಉࢯͷम࢜࿦จͱͯ͠·ͱΊΒΕͨɻࠓ‫ޙ‬͸ɺΑΓਊ֩ͷߏ଄͕ඇࣗ໌ͳϋϩʔ֩ʹ͍ͭͯͷղੳΛਐΊΔ༧ఆͰ͋Δɻ
ඍࢹతޫֶϙςϯγϟϧΛ༻͍ͨཅࢠ-֩ࢄཚͷ‫ܥ‬౷తղੳ (ീਘਖ਼৴ɺদຊୖຏɺຸ
ໜ޻ক (PD)ɺ๛઒কҰ (M2))ɹ 2 ֩ࢠؒ༗ޮ૬‫ߏ͍ͯͮجʹ༻࡞ޓ‬ங͞ΕͨޫֶϙςϯγϟϧΛඍࢹతޫֶϙςϯγϟϧͱ‫Ϳݺ‬ɻඍࢹతޫֶϙςϯγϟϧ͸ɺ৞ΈࠐΈ໛‫ܕ‬Λ༻͍ͯ 2 ֩ࢠؒ༗ޮ૬‫ޓ‬࡞༻Λඪత֩ີ౓Ͱ৞ΈࠐΈੵ෼͢Δ͜ͱʹΑΓߏஙͰ͖Δɻ৞ΈࠐΈ໛‫ʹܕ‬ΑΔඍ
ࢹత൓Ԡղੳ͸҆ఆ֩ࢄཚʹ͓͍ͯଟ͘ͷ੒ޭΛऩΊ͖ͯͨɻ͞Βʹɺ࣮‫ࠔ͕ݧ‬೉ͳ21ͨΊʹޫֶϙςϯγϟϧΛ‫ݱ‬৅࿦తʹߏஙͰ͖ͳ͍ෆ҆ఆ֩ࢄཚʹରͯ͠΋ɺ͜ͷ৞ΈࠐΈ໛‫ܕ‬͸༗ޮͳΞϓϩʔνͱͳΔɻ·ͨɺೖཻࣹࢠʹΑͬͯඪత͕֩ྭ‫͞ى‬ΕΔඇ஄ੑࢄཚ͸ɺνϟωϧ݁߹ํఔࣜʹΑΓ‫ه‬ड़͞ΕΔɻ͜ͷͱ͖ʹඞཁͱͳΔ݁߹ϙςϯγϟϧ΋·ͨɺ৞ΈࠐΈ໛‫ܕ‬Λ༻͍ͯߏஙͰ͖Δɻɹຊ‫Ͱڀݚ‬͸ɺMelbourne άϧʔϓͷ g ߦྻ༗ޮ૬‫༻࡞ޓ‬Λ༻͍ͨ৞ΈࠐΈ໛‫ʹܕ‬ΑΓɺཅࢠ-҆ఆ֩ (ෆ҆ఆ֩) ஄ੑࢄཚ͓Αͼཅࢠඇ஄ੑࢄཚΛղੳͨ͠ɻඍࢹతޫֶϙςϯγϟϧ͸ɺཅࢠ-҆ఆ֩஄ੑࢄཚͷ࣮‫ݧ‬Λඍ෼அ໘ੵɺภ‫ۃ‬෼ղೳͱ΋ʹ‫ܥ‬౷తʹ࠶‫͠ݱ‬ɺ͞Βʹඇ஄ੑࢄཚͷඍ෼அ໘ੵΛྑ͘‫ه‬ड़͢Δ͜ͱʹ੒ޭͨ͠ɻ҆ఆ֩ʹର͢Δඍࢹతޫֶϙςϯγϟϧ͸ɺ‫ݱ‬৅࿦తʹߏங͞Εͨޫֶϙςϯγϟϧͱ͍ۙৼΔ
෣͍Λ࣋ͭ͜ͱ͕͔֬ΊΒΕɺෆ҆ఆ֩ʹର͢Δඍࢹతޫֶϙςϯγϟϧ͸ɺ҆ఆ֩ͷ‫ܥ‬౷ੑͱҟͳΔੑ࣭Λ࣋ͭ͜ͱ͕෼͔ͬͨɻ
ɹຊ‫ڀݚ‬͸ຸໜࢯͱ๛઒ࢯΛத৺ʹਪਐ͞Εɺ๛઒ࢯͷम࢜࿦จͱͯ͠·ͱΊΒΕͨɻͦͷ੒Ռ͸ Physical Review C ࢽʹ‫͞ࡌܝ‬Εͨɻ‫֩ࢠݪ‬൓Ԡʹ͓͚ΔΧΠϥϧ༗ޮཧ࿦ 3 ֩ࢠྗͷޮՌ (ീਘਖ਼৴ɺদຊୖຏɺՏ໺௨࿠ [‫۝‬भࣃՊେֶ‫ڭ‬त]ɺຸໜ޻ক (PD)ɺ๛઒কҰ (M2))ɹΧΠϥϧ༗ޮཧ࿦͸ QCD ͱ౳Ձͳ௿ΤωϧΪʔ༗ޮཧ࿦Ͱ͋Γɺ2 ֩ࢠྗ΍ 3 ֩ࢠྗΛ‫ܥ‬౷తʹෆఆੑແܾ͘ఆͰ͖Δཧ࿦ͱͳ͍ͬͯΔɻ3 ֩ࢠྗ͸‫ࡏݱ‬஫໨͞Ε͍ͯΔେ͖ͳ࿩୊ͷͻͱͭͰɺ֩෺࣭ͷ‫ܗ‬੒ʹ͓͍ͯ΋ॏཁͳ໾ׂΛՌͨ͢ͱߟ͑ΒΕ͍ͯΔɻ·ͨɺ֩൓Ԡʹରͯ͠ΧΠϥϧ༗ޮཧ࿦͔Βෆఆੑແܾ͘ఆ͞Εͨ 3 ֩ࢠྗ͕Ͳ
ͷΑ͏ͳޮՌΛ༩͑Δ͔΋େม‫ڵ‬ຯਂ͍ɻɹຊ‫Ͱڀݚ‬͸ɺ֩ࢠ-֩ࢄཚ΍֩-֩ࢄཚʹ͓͚ΔΧΠϥϧ༗ޮཧ࿦ͷ 3 ֩ࢠྗޮՌΛ؆ศͳํ๏ͰධՁͨ͠ɻΧΠϥϧ༗ޮཧ࿦ͷ 2 ֩ࢠྗ͔Β g ߦྻཧ࿦ʹΑΓ֩෺࣭ͷҰཻࢠϙςϯγϟϧΛ‫͜ͱͨ͠ࢉܭ‬Ζɺ‫ݱ‬৅࿦త 2 ֩ࢠྗͰ͋Δ Bonn-B ϙςϯγϟϧ͔Β‫͞ࢉܭ‬Εͨ΋ͷͱඇৗʹࣅ௨ͬͨੑ࣭Λ࣋ͭ͜ͱ͕Θ͔ͬͨɻ͜ͷ͜ͱ͔ΒɺBonn-Bϙςϯγϟϧʹ‫ ͮ͘ج‬Melbourne g ߦྻ૬‫ʹ༻࡞ޓ‬ΧΠϥϧ༗ޮཧ࿦ͷ 3 ֩ࢠྗΛಋ
ೖ͢Δ͜ͱͰɺͦͷޮՌΛ‫͢ূݕ‬Δํ๏ΛఏҊͨ͠ɻͦͷ݁Ռɺ֩-֩ࢄཚͰ͸ඍ෼அ໘ੵͷ֯෼෍‫ Ͱํޙ‬3 ֩ࢠྗޮՌ͕ຊ࣭తͰ͋Γɺ3 ֩ࢠྗΛऔΓೖΕΔ͜ͱͰ࣮‫ݧ‬ΛΑΓ࠶‫͢ݱ‬Δ͜ͱ͕͔֬ΊΒΕͨɻҰํɺ֩ࢠ-֩ࢄཚͰ͸࣮‫ݧ‬σʔλͷར༻Մೳͳલ
ํྖҬʹ͓͍ͯ 3 ֩ࢠྗޮՌ͕খ͘͞ɺΑΓ‫ݧ࣮Ͱํޙ‬σʔλ͕ଌఆ͞ΕΔͱ 3 ֩ࢠྗޮՌͷॏཁੑΛ͔֬ΊΔ͜ͱ͕Ͱ͖Δɻɹຊ‫ڀݚ‬͸๛઒ࢯͱՏ໺ࢯΛத৺ʹਪਐ͞Εɺ๛઒ࢯͷम࢜࿦จͱͯ͠·ͱΊΒΕͨɻͦͷ੒Ռ͸‫ࡏݱ‬ɺPhysical Review C ࢽʹ౤ߘதͰ͋Δɻɹࠓ‫ޙ‬͸ɺΧΠϥϧ༗ޮཧ࿦ͷ 2 ֩ࢠྗͱ 3 ֩ࢠྗ͔Β g ߦྻ૬‫༻࡞ޓ‬Λߏங͠ɺ֩
ࢠ-֩ࢄཚ΍֩-֩ࢄཚͷ‫ܥ‬౷తղੳΛߦ͏ɻ

22ඍࢹత൓Ԡ໛‫ʹܕ‬ΑΔ֩ࢠ-Li ΞΠιτʔϓ൓Ԡղੳ (ീਘਖ਼৴ɺদຊୖຏɺ౉ล޾৴

[‫۝‬भେֶ૯߹ཧ޻ֶ෎‫ڭ‬त]ɺॹํҰհ [େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔ।‫ڭ‬त]ɺֲւਸ਼
[‫۝‬भେֶ૯߹ཧ޻ֶ෎ (D1)]ɺ౉ᬒ৻ (M2))ɹ֩༥߹࿍ͷઃ‫ࢠ͍͓֩ͯʹܭ‬-Li ΞΠιτʔϓ (6 Liɺ7 Li) ൓Ԡ͸ॏཁͰ͋Γɺͦͷ‫ܥ‬౷తͳ൓Ԡσʔλ͕ඞཁͱ͞Ε͍ͯΔɻ ͔͠͠ɺதੑࢠͰ͋Δ n ͸ిՙΛ࣋ͨͳ͍ͨΊՃ଎͢Δ͜ͱ΍‫ݕ‬ग़͢Δ͜ͱ͕ඇৗʹࠔ೉Ͱ͋Γɺ࣮‫ݧ‬తʹ͜ͷ൓Ԡͷஅ໘ੵΛ‫ܥ‬౷తʹܾఆ͢Δ͜ͱ͸ɺ‫ݱ‬ஈ֊Ͱ͸ෆՄೳͰ͋ΔɻಛʹɺߴΤωϧΪʔ൓Ԡʹ͓͚Δ
அ໘ੵΛܾఆ͢Δʹ͸ਫ਼ີͳཧ࿦༧ଌ͕ඞཁͱͳΔɻͦ͜Ͱզʑ͸ɺn+6 Liɺ n+7 Liɺ

p+6 Liɺp+7 Li ࢄཚͷਫ਼ີཧ࿦ղੳΛਐΊ͖ͯͨɻ͜Ε·Ͱͷ‫͍͓ͯʹڀݚ‬ɺ6,7 Li Λ d+ αɺt + α ͷ 2 ମ໛‫هͯ͠ͱܕ‬ड़͠ɺ൓ԠաఔͰ෼ղ͢ΔޮՌΛ CDCC ͰऔΓѻͬͨ‫Ͱࢉܭ‬஄ੑࢄཚɺશஅ໘ੵͷ࣮‫ݧ‬Λ‫ܥ‬౷తʹ࠶‫͖Ͱݱ‬Δ͜ͱΛࣔͨ͠ɻຊ೥౓͸ɺ஄ੑࢄཚ͚ͩͰͳ͘ɺ7 Li ࢄཚʹ͓͍ͯ์ग़͞ΕΔ t ͷ֯౓෼෍ͷ‫ʹࢉܭ‬ணख͠ɺ࣮‫ݧ‬σʔλΛ΄΅࠶‫͖Ͱݱ‬Δ͜ͱΛࣔͨ͠ɻ͔͠͠ɺ͋Δ์ग़֯౓ɺ์ग़ΤωϧΪʔͷσʔλʹؔͯ͠͸࣮‫ݧ‬Λ࠶‫͕ͱ͍͜ͳ͖Ͱݱ‬൑໌ͨ͠ɻ͜ͷ໰୊͸ɺ‫ࡏݱ‬‫Ͱࢉܭ‬औΓೖΕ͍ͯΔ໛‫े͕ۭؒܕ‬෼Ͱͳ͍ͱ͍͏͜ͱ͕ߟ͑ΒΕΔҝɺࠓ‫ޙ‬͸໛‫ܕ‬ۭؒΛ޿͛ͨ‫ࢉܭ‬Λߦͳ͏ඞཁ͕͋Δɻ‫ࡏݱ‬ɺ͜ͷ‫ࢉܭ‬͸૯߹ཧ޻ֶ෎ͷֲࢯΛத৺ͱͯ͠ਪਐ͞Ε͍ͯΔɻ
‫ج֩ࢠݪ‬ఈঢ়ଶͷϓϩϨʔτม‫ܗ‬༏੎ͷ‫( ݯى‬ਗ਼ਫྑจɺߴ‫ݪ‬఩࢜ [ҍྛେֶ]ɺాౢ௚
थ [෱Ҫେֶ])ɹଟ͘ͷ‫֩ࢠݪ‬͸ͦͷ‫ج‬ఈঢ়ଶʹ͓͍ͯม‫͍ͯ͠ܗ‬Δ͕ɺͦͷ‫ܗ‬͸࣠ରশͳճసପԁମ‫͋Ͱܕ‬Δɻ͜ͷ৔߹ɺ‫ٿ‬Λ࣠ํ޲ʹԡ͠௵ͨ͠ΦϒϨʔτ‫( ܕ‬ϛΧϯ‫͔ )ܕ‬Ҿ͖৳͹ͨ͠ϓϩϨʔτ‫( ܕ‬ϨϞϯ‫ )ܕ‬ͷ̎छྨ͕ߟ͑ΒΕΔɻฏ‫ۉ‬৔ͱͯ͠ௐ࿨ৼಈࢠϙςϯγϟϧΛߟ͑Δͱ͜ΕΒ̎छྨͷม‫ܗ‬͸ಉ͙͡Β͍ͷස౓Ͱ‫ݱ‬ΕΔ͕ɺ‫࣮ݱ‬ͷ‫Ͱ֩ࢠݪ‬͸ѹ౗తʹϓϩϨʔτ‫ܕ‬ม‫ܗ‬ͷํ͕ଟ͍ɻ͜ͷϓϩϨʔτม‫ܗ‬༏੎ͷ‫ݯى‬͸Կ͔ͱ͍͏͜ͱ͸‫͔͘ݹ‬Βͷ໰୊Ͱ͋Γɺ਺೥લ͔ΒͦΕΛཧղ͢ΔͨΊͷ‫ڀݚ‬Λߦ͍ͬͯΔɻɹ‫֩ࢠݪ‬ͷม‫ܗ‬Λཧղ͢ΔͨΊʹ͸ɺ‫֩ࢠݪ‬ͷଋറΤωϧΪʔʹର͢Δ‫ࢹڊ‬తޮՌ(ӷణ໛‫ܕ‬ΤωϧΪʔ) ͱγΣϧޮՌ (֪ߏ଄ΤωϧΪʔ) Λߟ͑Δඞཁ͕͋Δɻ͜Ε·Ͱͷ‫Ͱڀݚ‬͸ɺओʹγΣϧޮՌͷํΛௐ΂͖͕ͯͨɺࡢ೥౓͔Βɺ‫ࢹڊ‬తޮՌ͕ͲͷΑ͏ʹ‫࣮ݱ‬ͷ‫֩ࢠݪ‬ͷϓϩϨʔτม‫ܗ‬༏੎ঢ়‫ʹگ‬Ө‫ڹ‬Λ༩͑Δ͔Λௐ΂͍ͯΔɻಛʹɺΫʔϩϯੱྗΤωϧΪʔͱද໘ΤωϧΪʔͷޮՌ΍ɺରশΤωϧΪʔͷޮՌɺ·ͨɺମੵอଘ৚݅ͷӨ‫͍ͯͭʹڹ‬ɺ࣭ྔެࣜதͷͦΕͧΕͷ‫د‬༩Λඪ४తͳ஋͔Βมߋ͢Δ͜ͱʹΑͬͯɺϓϩϨʔτม‫ݱ͕ܗ‬ΕΔ֬཰ʹͲͷΑ͏ʹ൓ө͢Δ͔Λௐ΂ͨɻ͜ͷ࣌ɺ‫ࢹڊ‬తΤωϧΪʔͷύϥϝʔλΛม͑Δͱ‫֩ࢠݪ‬ͷଘࡏൣғ (தੑࢠɾཅࢠͷυϦοϓ

23ઢ) ͕େ͖͘มΘͬͯ͠·͏͕ɺγΣϧޮՌʹΑΔϓϩϨʔτม‫ܗ‬༏੎ͷ‫ج‬ຊతͳϝΧχζϜ͸΄ͱΜͲมΘΒͳ͍͜ͱ͕Θ͔ͬͨɻ͔͠͠ͳ͕ΒɺϓϩϨʔτม‫ͱܗ‬ΦϒϨʔτม‫͢߹ڝ͕ܗ‬Δ৔߹ʹ͸ɺ‫ࢹڊ‬తΤωϧΪʔ͕େ͖ͳӨ‫ڹ‬Λ‫͢΅ٴ‬৔߹΋͋Γɺ‫ࢹڊ‬తޮՌ΋ແࢹͰ͖ͳ͍ɻ͜ͷ‫ڀݚ‬͸ҍྛେͷߴ‫ࢯݪ‬Λத৺ʹߦΘΕ͍ͯΔɻ
‫͚͓ʹ֩ࢠݪ‬Δਖ਼࢛໘ମ‫ܕ‬ม‫ܗ‬ͷ‫( ڀݚ‬ਗ਼ਫྑจɺా্ਅ‫( ޔ‬D2)ɺJ. Dudek [ετϥεϒʔϧେֶ])
ɹࠓ೔·Ͱʹ஌ΒΕ͍ͯΔ‫֩ࢠݪ‬ͷଟ͘͸࣠ରশͳճసପԁମม‫͋Ͱܗ‬Δͱߟ͑ΒΕ
͍ͯΔ͕ɺۙ೥ͷฏ‫ۉ‬৔ཧ࿦ʹΑΔ‫Ͱࢉܭ‬ɺ͜Ε·Ͱʹ͋·Γௐ΂ΒΕ͍ͯͳ͍ΤΩκνοΫͳม‫ܗ‬ͷଘࡏ͕༧૝͞Ε͍ͯΔɻͦͷҰͭʹਖ਼࢛໘ମ‫ܕ‬ͷม‫͕͋ܗ‬Γɺಛఆͷཅࢠ਺·ͨ͸தੑࢠ਺ͷ‫֩ࢠݪ‬ͷ҆ఆͳม‫͠ݱ࣮ͯ͠ͱܗ‬ɺ‫ج‬ఈঢ়ଶ·ͨ͸௿ྭ‫ى‬ঢ়ଶͱͳΔͱ‫ظ‬଴͞Ε͍ͯΔɻ͜ΕΒͷಛఆͷཻࢠ਺͸ਖ਼࢛໘ମม‫ܗ‬ͷຐ๏਺ͱ‫ݺ‬͹Εɺཅࢠ਺ͱதੑࢠ਺͕ͱ΋ʹຐ๏਺Ͱ͋Δਖ਼࢛໘ମม‫ܗ‬ͷೋॏด֪ͷ‫Ͱ֩ࢠݪ‬͸ͦͷม‫ܗ‬͸ಛʹ҆ఆͱͳΔɻ
ࡢ೥౓ɺզʑ͸ೋॏด֪ͷ‫ʹ֩ࢠݪ‬Ұཻͭࢠ͕͍࢛ͭͨ໘ମม‫֩حͨ͠ܗ‬ͷճసεϖΫτϧͷ‫ࢉܭ‬Λྔࢠ਺ࣹӨ๏ʹΑΓߦͬͨɻ࢛໘ମม‫ܗ‬ͷม‫͕౓ܗ‬େ͖͍৔߹ɺೋ
ॏด֪ͷ‫Ͱ֩ࢠݪ‬͸ྔࢠεϖΫτϧ͸ҰͭͷճసόϯυͱͳΔɻ͜Εʹର͠ɺ‫֩ح‬ͷ৔߹ʹ͸ม‫͕౓ܗ‬େ͖͘ͱ΋ͦͷεϖΫτϧ͸ෳ਺ͷճసόϯυʹ෼཭͢Δͱ͍͏݁ՌΛಘͨɻ͜ͷΑ͏ͳ෼཭͸௨ৗͷճసପԁମ‫ܕ‬ม‫Ͱܗ‬΋‫ݟ‬ΒΕΔ΋ͷͰ͋Δ͕ɺਖ਼
࢛໘ମճసόϯυͷ৔߹ʹ͸ͦͷ෼཭ͷ࢓ํ͕ͣͬͱෳࡶʹͳ͍ͬͯΔɻ͜ͷճసόϯυͷ෼཭ͷ‫ݪ‬ҼΛ୳ΔͨΊɺຊ೥౓͸ɺਖ਼࢛໘ମม‫ͨ͠ܗ‬ճసମʹҰཻͭࢠ͕͍ͭ
ཻͨࢠɾճసମ໛‫ܕ‬Λ༻͍ͨ෼ੳΛߦͬͨɻ௨ৗͷପԁମม‫ܗ‬ͷ৔߹ͱಉ༷ʹɺཻࢠɾճసମ໛‫Ͱܕ‬͸ਖ਼࢛໘ମม‫ͨ͠ܗ‬ճసମͱ࠷‫ޙ‬ͷཻࢠͷؒʹίϦΦϦ૬‫͕༻࡞ޓ‬ಇ͘ɻͦͷޮՌΛղੳతɾ਺஋తʹ‫͢ࢉܭ‬Δ͜ͱͰɺྔࢠ਺ࣹӨ๏ͷ݁ՌΛ࠶‫͢ݱ‬Δ݁Ռ͕ಘΒΕΔ͜ͱ͕Θ͔Γɺෳ਺ͷճసόϯυ΁ͷ෼཭ͷ‫ݪ‬Ҽ͕ίϦΦϦ૬‫͋Ͱ༻࡞ޓ‬Δ
ͱ݁࿦͚ͮͨɻ͜ͷ‫ڀݚ‬͸ా্ࢯΛத৺ʹߦΘΕ͍ͯΔɻ

Gogny ૬‫ʹ༻࡞ޓ‬ΑΔྔࢠ਺ࣹӨ‫( ࢉܭ‬ਗ਼ਫྑจɺా্ਅ‫( ޔ‬D2))
ɹ‫ߏ֩ࢠݪ‬଄‫͍༻͘޿Ͱࢉܭ‬ΒΕ͍ͯΔ৴པੑͷߴ͍༗ޮ૬‫༻࡞ޓ‬ͷҰͭʹɺ༗‫ݶ‬Ϩϯδͷ Gogny ૬‫͕͋༻࡞ޓ‬Γɺࡢ೥·ͰʹզʑͷάϧʔϓͰ͸͜ͷ૬‫༻࡞ޓ‬Λ༻͍ͨฏ‫ۉ‬৔‫ࢉܭ‬Λߦ͖ͬͯͨɻຊ೥౓͸ɺฏ‫ۉ‬৔ۙࣅͰഁΕͨରশੑΛճ෮ͤ͞Δ͜ͱͰΤωϧΪʔεϖΫτϧͳͲΛ‫ٻ‬ΊΔɺฏ‫ۉ‬৔Λ௒͑ͨཧ࿦ख๏Ͱ͋Δྔࢠ਺ࣹӨ๏ʹ͓͍ͯ΋ Gogny ૬‫༻࡞ޓ‬Λ༻͍Δ͜ͱͷग़དྷΔϓϩάϥϜΛ࡞੒ͨ͠ɻ͜Ε·Ͱͷզʑͷྔࢠ਺ࣹӨ‫Ͱࢉܭ‬͸಺෦ঢ়ଶΛ࡞Δฏ‫ۉ‬৔ͱͯ͠͸ Woods-Saxon ϙςϯγϟϧΛ༻͍Δͷʹର͠ɺྔࢠ਺ࣹӨ๏ͷ‫Ͱࢉܭ‬͸ଟॏ‫ܕۃ‬ͷ‫ݱ‬৅࿦తͳ૬‫༻࡞ޓ‬Λ༻͍͓ͯΓɺ24‫ࢉܭ‬ͷटඌҰ؏ੑΛ͍͍ܽͯͨɻ͔͠͠ɺҰͭͷ Gogny ૬‫͔༻࡞ޓ‬Βग़ൃͯ͠ฏ‫ۉ‬৔Λ‫͠ࢉܭ‬ɺͦͷฏ‫ۉ‬৔ʹΑΔ಺෦ঢ়ଶ͔Βྔࢠ਺ࣹӨ‫ࢉܭ‬Λߦ͏ͱ͍͏ɺ‫׬‬શʹࣗ‫ݾ‬ແ಍ணͳ‫͕ࢉܭ‬Մೳͱͳͬͨ݁ՌɺΑΓఆྔతͳ෼ੳ͕ग़དྷΔΑ͏ʹͳͬͨɻ։ൃͨ͠‫ࢉܭ‬ϓϩάϥϜͰ͸ۭؒ൓సରশੑΛഁͬͨඇৗʹҰൠతͳม‫ܗ‬ঢ়ଶʹྔࢠ਺ࣹӨ๏Λద༻͢Δ͜ͱ͕ग़དྷΔɻ͜ͷϓϩάϥϜΛ༻͍ͯɺզʑ͕͜Ε·Ͱ‫͠ڀݚ‬͖࢛ͯͨ໘ମม‫ܗ‬ͷด֪Ͱ Gogny ૬‫ʹ༻࡞ޓ‬ΑΔྔࢠ਺ࣹӨ๏Λߦͬͨɻਖ਼࢛໘ମม
‫ܗ‬ͷ৔߹ɺճసεϖΫτϧ͸͜Ε·Ͱ༻͍͖ͯͨ Woods-Saxon ϙςϯγϟϧͱଟॏ‫ۃ‬‫ܕ‬ͷ؆୯ͳ૬‫༻࡞ޓ‬Λ༻͍ͨ݁Ռͱඇৗʹ͍ۙ΋ͷͱͳΔ͜ͱ͕Θ͔ͬͨɻ·ͨɺ֯ӡಈྔࣹӨʹΑΔม‫ܗ‬ΤωϧΪʔ໘Λ‫ٻ‬Ίͨ݁Ռɺฏ‫ۉ‬৔ۙࣅͷ࣌ʹൺ΂ͯඇৗʹਂ͍‫ۃ‬খ͕‫ݱ‬ΕΔ͜ͱΛࣔͨ͠ɻ͜ͷϓϩάϥϜͰ͸௨ৗͷପԁମม‫ܗ‬ͷ‫ࢉܭ‬΋΋ͪΖΜՄೳͰ͋Γɺ௨ৗͷม‫֩ܗ‬ͷΤωϧΪʔ໘ͷ‫ࢉܭ‬΋ߦ͍ͬͯΔɻࠓ‫ޙ‬͸ΑΓ‫ܥ‬౷తͳ෼ੳΛߦ͏༧ఆͰ͋Δɻ͜ͷ‫ڀݚ‬͸ా্ࢯΛத৺ʹߦΘΕ͍ͯΔɻ
Ψ΢ε‫ج‬ఈΛ༻͍ͨྔࢠ਺ࣹӨ‫( ࢉܭ‬ਗ਼ਫྑจɺా্ਅ‫( ޔ‬D2)ɺౢాॆ޺ (D1))ɹෆ҆ఆ֩ʹ͓͍ͯ͸ɺϋϩʔߏ଄΍εΩϯߏ଄ͱ͍ͬͨ҆ఆ֩Ͱ͸‫ݟ‬ΒΕͳ͔ͬͨಛ༗ͷߏ଄͕‫͓͔ͯͬͭݟ‬Γɺͦͷճసঢ়ଶʹ͓͍ͯ΋ɺಛ௃తͳੑ࣭͕‫ݱ‬ΕΔ͜ͱ͕‫ظ‬଴͞ΕΔɻ·ͨɺ‫֩ࢠݪ‬ͷճస͸֪ޮՌʹ‫ى‬Ҽ͢Δ‫ݱ‬৅Ͱ͋Δ͕ɺ֪ޮՌ͸ಛఆͷཻࢠ਺ʹ͓͍ͯ‫ͳ͘ڧ‬Δɻͭ·Γɺ҆ఆ֩ͱҟͳΓཻࢠ਺Λࣗ༝ʹબ΂Δͱ͍͑Δෆ҆ఆ֩͸ճసঢ়ଶͷ‫ʹڀݚ‬ରͯ͠༗༻Ͱ͋Δɻ͜Ε·Ͱͷ֯ӡಈྔࣹӨ‫͍͓ʹࢉܭ‬ͯ͸ɺௐ࿨ৼಈࢠ‫ج‬ఈ͕༻͍ΒΕ͍͕ͯͨɺຊ೥౓͸ɺऑଋറΛಛ௃ͱ͢Δෆ҆ఆ֩ͷճసঢ়ଶΛద੾ʹऔΓѻ͑ΔΨ΢ε‫ج‬ఈΛ༻͍ͨྔࢠ਺ࣹӨ‫ࢉܭ‬ΛՄೳʹͨ͠ɻ։ൃͨ͠‫ࢉܭ‬ϓϩάϥϜΛ༻͍ͯɺυϦοϓϥΠϯͷ‫͋Ͱ֩ࢠݪ‬Δ 40 Mg ʹ͍ͭͯ‫ܭ‬ࢉΛߦͬͨɻͦͷ݁Ռɺεϐϯͷ૿Ճͱ‫׳ʹڞ‬ੑϞʔϝϯτ͕େ͖͘‫ݮ‬গ͢Δͱ͍͏
ಛҟͳ;Δ·͍͕‫ݟ‬ΒΕͨɻ·ͨɺௐ࿨ৼಈࢠ‫ج‬ఈΛ༻͍ͨ৔߹ͱΨ΢ε‫ج‬ఈΛ༻͍ͨ৔߹Ͱ͸ɺ‫֩ࢠݪ‬ͷີ౓෼෍ͷԕํͰͷ;Δ·͍͕େ͖͘ҟͳΔʹ΋ؔΘΒͣɺ‫׳‬ੑϞʔϝϯτ͸Α͘Ұக͓ͯ͠ΓɺϋϩʔͷΑ͏ͳ޿͕ͬͨີ౓ߏ଄͕‫׳‬ੑϞʔϝϯτʹӨ‫͍ͳ͠ڹ‬Մೳੑ͕͋Δ͜ͱ͕Θ͔ͬͨɻࠓ‫ޙ‬͸ଞͷෆ҆ఆ֩ʹ͍ͭͯ΋ௐ΂ɺऑଋറ‫Ͱ֩ࢠݪ‬ͷճసӡಈΛΑΓৄࡉʹௐ΂͍ͯ͘༧ఆͰ͋Δɻ͜ͷ‫ڀݚ‬͸ౢాࢯΛத৺ʹߦΘΕ͍ͯΔɻ
ྔࢠ਺ࣹӨ๏ʹΑΔߴ଎ճస͢Δ‫֩ࢠݪ‬ͷඍࢹత‫( ڀݚ‬ਗ਼ਫྑจɺా্ਅ‫( ޔ‬D2)ɺౢ
ాॆ޺ (D1))ɹճసӡಈͱಠཱཻࢠӡಈͱͷ‫߹ڝ‬͸ɺ‫֩ࢠݪ‬ͷ৭ʑͳྖҬʹ͓͍ͯͦͷੑ࣭ʹେ͖ͳӨ‫ڹ‬Λ‫͢΅ٴ‬ɻಛʹɺ֯ӡಈྔͷେ͖ͳ‫͋Ͱݶۃ‬Δߴ଎ճసঢ়ଶ͸ɺ͜ͷ‫ͨ͠߹ڝ‬ঢ়ଶΛௐ΂Δͷʹదͨ͠ঢ়ଶͰ͋Γɺ࣓‫ؾ‬ճస΍ΧΠϥϧೋॏ߲ɺ΢ΥϒϦϯάճసͱ25

͍ͬͨ‫ڵ‬ຯਂ͍ಛҟͳճసόϯυ͕਺ଟ͘ΈΒΕΔɻ·ͨɺෆ҆ఆ֩ʹ͓͍ͯ͸ɺϋϩʔߏ଄΍εΩϯߏ଄ͱ͍ͬͨ҆ఆ֩Ͱ͸‫ݟ‬ΒΕͳ͔ͬͨಛ༗ͷߏ଄͕‫͓͔ͯͬͭݟ‬Γɺͦͷճసঢ়ଶʹ͓͍ͯ΋ɺಛ௃తͰ‫ڵ‬ຯਂ͍ੑ࣭͕‫ݱ‬ΕΔ͜ͱ͕‫ظ‬଴͞ΕΔɻ
΢ΥϒϦϯάճసόϯυ͸ɺ‫ݹ‬యతඇ࣠ରশ߶ମͷࡀࠩӡಈΛྔࢠԽͨ͠ճసόϯυͰ͋ΓɺଞํɺΧΠϥϧೋॏ߲͸̏ͭͷ֯ӡಈྔ͕ӈख‫ࠨͱܥ‬ख‫ڸ͏͍ͱܥ‬өରশͳ̎ͭͷ૊ΈํΛͱΔ͜ͱʹΑΓੜ͡Δೋॏ߲Ͱ͋Δ͕ɺ͜Ε·Ͱͷ‫ʹڀݚ‬ΑΓɺඍࢹతྔࢠ਺ࣹӨ‫͍͓ͯʹࢉܭ‬΋΢ΥϒϦϯάճస΍ΧΠϥϧೋॏ߲͕‫ݱ‬ΕΔ͜ͱ͸֬ೝ͍ͯ͠Δɻ‫ࡏݱ‬ɺ΢ΥϒϦϯάճసʹ͍ͭͯ͸ඇ࣠ରশม‫ܗ‬ͷූ߸΍େ͖͞ʹͲͷΑ͏ʹґଘ͢Δͷ͔ͱ͍͏‫ج‬ຊతͳੑ࣭Λௐ΂͓ͯΓɺΧΠϥϧೋॏ߲ʹ͍ͭͯ͸֯ӡಈྔͷओ͔࣠ΒͷͣΕ΍ి࣓ભҠͷબ୒ଇͳͲΛௐ΂ͯߦ͘༧ఆͰ͋Δɻ·ͨɺ࣓‫ؾ‬తͳରশੑͷഁΕʹΑΔճసӡಈͰ͋Δ࣓‫ؾ‬ճసʹ͍ͭͯ΋ɺͲͷΑ͏ʹ‫ݱ‬ΕΔͷ͔ͷϝΧχζϜΛྔࢠ਺ࣹӨ๏ʹΑΓ‫͢ڀݚ‬Δ༧ఆͰ͋Δɻ͜ͷ‫ڀݚ‬͸ౢాࢯΛத৺ʹߦΘΕ͍ͯΔɻൃද࿦จ ‫ݪ‬ஶ࿦จ 
Diﬀerences and similarities between fundamental and adjoint matters in SU(N) gauge
theories:
H. Kouno, T. Misumi, K. Kashiwa, T. Makiyama, T. Sasaki, and M. Yahiro,
Physical Review D 88 (2013) pp. 016002-1–14
Color screening potential at ﬁnite density in two-ﬂavor lattice QCD with Wilson
fermions:
J. Takahashi, K. Nagata, T. Saito, A. Nakamura, T. Sasaki, H. Kouno, and M. Yahiro,
Physical Review D 88, (2013) pp. 114504-1–15
Conﬁnement and Z3 symmetry in three-ﬂavor QCD:
H. Kouno, T. Makiyama, T. Sasaki, Y. Sakai, and M. Yahiro,
Journal of Physics G: Nuclear and Particle Physics 40 (2013) 095003 (19pp)
Eﬀective model approach to meson screening masses at ﬁnite temperature:
M. Ishii, T. Sasaki, K. Kashiwa, H. Kouno, and M. Yahiro,

26

Physical Review D 89, (2014) pp. 071901(R)-1–6.
Two-color QCD at imaginary chemical potential and its impact on real chemical potential:
K. Kashiwa, T. Sasaki, H. Kouno, and M. Yahiro
Physical Review D 87, (2013) pp. 016015-1–9.
Interplay between the 0+
2 resonance and the nonresonant continuum of the drip-line
two-neutron halo nucleus 22 C:
K. Ogata, T. Myo, T. Furumoto, T. Matsumoto, and M. Yahiro Physical Review C
88, (2013) pp. 0246016-1–4.
6
Two-neutron decay from the 2+
1 state of He:

Y. Kikuchi, T. Matsumoto, K. Minomo, K. Ogata,
Physical Review C 88, (2013) pp. 021602(R)-1–5.
Reaction mechanism in odd-even staggering of reaction cross sections:S. Sasabe, T. Matsumoto, S. Tagami, N. Furutachi, K. Minomo, Y. R. Shimizu, andM. Yahiro,
Physical Review C 88, (2013) pp. 037602-1–4.
Mass-number and isotope dependence of local microscopic optical potentials for polarized proton scattering:
M. Toyokawa, K. Minomo, and M. Yahiro,
Physical Review C 88, (2013) pp. 0546021-1–14.
Microscopic study of tetrahedrally symmetric nuclei by an angular-momentum andparity projection method:
S. Tagami, Y. R. Shimizu, and J. Dudek,
Phys. Rev. C 87, (2013) pp. 054306-1–15.

Proceedings
Meson mass and the sign problem at ﬁnite theta:
T. Sasaki, H. Kouno, and M. Yahiro,
27

Journal of Physics: Conference Series 432 (2013) 012031 (5pp)
Quark-Hadron ࠞ߹૬Λߟྀͨ͠தੑࢠ੕ͷ‫ڀݚ‬:؅໺ ३ฏ, ࠤʑ໦ ਸ޺, ҆෢ ৳ढ़, Տ໺ ௨࿠, Տ໺ ޺໌, ീਘ ਖ਼৴,‫ ڀݚ֩ࢠݪ‬Vol. 58 Supplement 2 (2014) pp. 68-70

New candidate for deformed halo nucleus in Mg isotopes through analysis of reaction
cross sections:
S. Watanabe, K. Minomo, S. Tagami, M. Shimada, M. Kimura, M. Takechi, M. Fukuda,
D. Nishimura, T. Suzuki, T. Matsumoto, Y. R. Shimizu, and M. Yahiro,
EPJ Web of Conferences Vol. 66, 03095 (2014).
൓Ԡஅ໘ੵͷ‫حۮ‬ੑʹ͓͚Δ൓Ԡ‫ߏػ‬:ࠤʑ෦‫ޛ‬, দຊୖຏ, ా্ਅ‫ޔ‬, ‫ཱݹ‬௚໵, ຸໜ޻ক, ਗ਼ਫྑจ, ീਘਖ਼৴‫ڀݚ֩ࢠݪ‬, Volume 58, Supplement 2 (2014) pp. 39–41.
ΧΠϥϧ༗ޮཧ࿦ʹ‫ ͍͠৽ͮ͘ج‬G ߦྻ༗ޮ૬‫༻࡞ޓ‬ͷߏஙʹ޲͚ͯ:๛઒কҰ, ຸໜ޻ক, Տ໺௨࿠, ീਘਖ਼৴‫ڀݚ֩ࢠݪ‬, Volume 58, Supplement 2 (2014) pp. 98–100.
൓Ԡஅ໘ੵͷղੳͰ୳Δதੑࢠա৒ Mg ಉҐମͷੑ࣭:౉ᬒ৻, ຸໜ޻ক, ౢాॆ޺, ా্ਅ‫ޔ‬, ໦ଜਅ໌, ෢ஐຑ໹, ෱ాޫॱ, ੢ଜଠथ, ླ໦݈, দຊୖຏ, ਗ਼ਫྑจ, ീਘਖ਼৴‫ڀݚ֩ࢠݪ‬, Volume 58, Supplement 2 (2014) pp. 103–105.

The suggested presence of the tetrahedral-symmetry in the ground-state conﬁgurationof the 96
40 Zr56 nucleus:
J. Dudek, D. Curien, D. Rouvel, K. Mazurek, Y. R. Shimizu, and S. Tagami,
Physica Scripta 89 (2014), 054007.
Nuclear tetrahedral states and high-spin states studied using quantum number projection method:
S. Tagami, M. Shimada, Y. Fujioka, Y. R. Shimizu, and J. Dudek,
Physica Scripta 89 (2014), 054013.

28

Gogny ૬‫༻࡞ޓ‬Λ༻͍࢛ͨ໘ମม‫֩ܗ‬ͷ‫ڀݚ‬:ా্ਅ‫ޔ‬, ਗ਼ਫྑจ, J. Dudek,‫ڀݚ֩ࢠݪ‬, Volume 58, Supplement 2 (2014) pp.89–91.
ม‫ͨ͠ܗ‬ෆ҆ఆ֩Ͱͷ 2 தੑࢠ૬ؔ:ౢాॆ޺, ా্ਅ‫ޔ‬ɺਗ਼ਫྑจ,‫ڀݚ֩ࢠݪ‬, Volume 58, Supplement 2 (2014) pp.86–88.

 ͦͷଞͷ࿦จ ߨԋ ւ֎Ͱͷߨԋ 
Heavy quark potential at ﬁnite imaginary chemical potential:
J. Takahashi, T. Sasaki, K. Nagata, T. Saito, H. Kouno, M. Yahiro, and A. Nakamura,
Lattice 2013, August 2, Mainz, Germany.
Practical approach to the sign problem at ﬁnite theta-vacuum angle:
T. Sasaki, H. Kouno, and M. Yahiro,
Lattice 2013, July 31, 2013, Mainz, Germany.
The suggested presence of the tetrahedral-symmetry in the ground-state conﬁgurationof the 96
40 Zr56 nucleus:
J. Dudek, D. Curien, D. Rouvel, K. Mazurek, Y. R. Shimizu, and S. Tagami,
20th Nuclear Physics Workshop “Marie & Pierre Curie” on “Structure and Dynamics
of Atomic Nuclei”, September 28, Kazimierz Dolny, Poland.
Nuclear tetrahedral states and high-spin states studied by quantum number projection
method:S. Tagami, M. Shimada, Y. Fujioka, Y. R. Shimizu, and J. Dudek,
20th Nuclear Physics Workshop “Marie & Pierre Curie” on “Structure and Dynamics
of Atomic Nuclei”, September 28, Kazimierz Dolny, Poland.
ҎԼɺϙελʔൃද.

29

Constraints on quark-hadron transition from lattice QCD and neutron-star observation:
T. Sasaki, N, Yasutake, M, Kohno, H. Kouno, and M. Yahiro,
Extreme QCD 2013, August 5, 2013, Bern, Switzerland.
New candidate for deformed halo nucleus in Mg isotopes through analysis of reaction
cross sections:
S. Watanabe, K. Minomo, S. Tagami, M. Shimada, M. Kimura, M. Takechi, M. Fukuda,
D. Nishimura, T. Suzuki, T. Matsumoto, Y. R. Shimizu, and M. Yahiro
International Nuclear Physics Conference (INPC2013), June 4, 2013, Firenze, Italy.

 ࠃ಺Ͱͷߨԋ 
Quark-Hadron ࠞ߹૬Λߟྀͨ͠தੑࢠ੕ͷ‫ڀݚ‬:؅໺ ३ฏ, ࠤʑ໦ ਸ޺, ҆෢ ৳ढ़, Տ໺ ௨࿠, Տ໺ ޺໌, ീਘ ਖ਼৴,ࡾऀएखՆͷֶߍ, 2013 ೥ 8 ݄ 4 ೔, ϗςϧ͖ͨͭ (Ѫ஌‫)ݝ‬
֨ࢠ QCD Λ༻͍ͨ༗‫Ͱܥ౓ີݶ‬ͷΫΥʔΫؒϙςϯγϟϧ:ߴ‫ڮ‬७Ұ, Ӭా‫ܡ‬ଠ࿠, ࡈ౻୎໵, தଜ७, ࠤʑ໦ਸ޺, Տ໺޺໌, ീਘਖ਼৴

RCNP/‫۝‬େ‫ڀݚ‬ձʮϋυϩϯ෺ཧͱ‫֩ࢠݪ‬෺ཧͷΫϩεΦʔόʔʯ 2013 ೥ 9 ݄ 5 ೔,‫۝‬भେֶ
֨ࢠ‫͓ࢉܭ‬Αͼதੑࢠ੕‫؍‬ଌͱແໃ६ͳΫΥʔΫ-ϋυϩϯ૬సҠͷ‫ڀݚ‬:ࠤʑ໦ਸ޺, ҆෢৳ढ़, Տ໺௨࿠, Տ໺޺໌, ീਘਖ਼৴,೔ຊ෺ཧֶձळ‫ق‬େձ, 2013 ೥ 9 ݄ 20 ೔, ߴ஌େֶ֨ࢠ QCD ʹΑΔΫΥʔΫؒϙςϯγϟϧͷԽֶϙςϯγϟϧґଘੑ:ߴ‫ڮ‬७Ұ, ࠤʑ໦ਸ޺, Ӭా‫ܡ‬ଠ࿠, ࡈ౻୎໵, Տ໺޺໌, ീਘਖ਼৴, தଜ७೔ຊ෺ཧֶձळ‫ق‬େձ, 2013 ೥ 9 ݄ 20 ೔, ߴ஌େֶதੑࢠ੕‫؍‬ଌ݁ՌΛߟྀͨ͠ QCD ૬ߏ଄ͷ‫ڀݚ‬:ࠤʑ໦ਸ޺, ҆෢৳ढ़, Տ໺௨࿠, Տ໺޺໌, ീਘਖ਼৴,ୈ 118 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ, 2013 ೥ 11 ݄ 30 ೔, ‫ཹٱ‬ถ޻‫ۀ‬େֶ‫਺ڏ‬ԽֶϙςϯγϟϧྖҬͷ֨ࢠ QCD ‫ʹࢉܭ‬ΑΔΫΥʔΫ਺ີ౓ͷ‫ڀݚ‬:30ߴ‫ڮ‬७Ұ, ࠤʑ໦ਸ޺, Ӭా‫ܡ‬ଠ࿠, Տ໺޺໌, ീਘਖ਼৴, தଜ७ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ, 2013 ೥ 11 ݄ 30 ೔, ‫ཹٱ‬ถ޻‫ۀ‬େֶ

Meson screening mass ͷಋग़๏ͱͦͷԠ༻:ੴҪ༏େ, ࠤʑ໦ਸ޺, Տ໺޺໌, ീਘਖ਼৴ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ, 2013 ೥ 11 ݄ 30 ೔, ‫ཹٱ‬ถ޻‫ۀ‬େֶࠞ߹૬Λߟྀͨ͠தੑࢠ੕಺෦ͷ QCD ૬సҠ:؅໺ ३ฏ, ࠤʑ໦ ਸ޺, ҆෢ ৳ढ़, Տ໺ ௨࿠, Տ໺ ޺໌, ീਘ ਖ਼৴,ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ, 2013 ೥ 11 ݄ 30 ೔, ‫ཹٱ‬ถ޻‫ۀ‬େֶ

NJL ໛‫͚͓ʹܕ‬Δਖ਼ଇԽ๏ґଘੑʹ͍ͭͯ:ถଜߒ࢘, ੴҪ༏େ, ࠤʑ໦ਸ޺, Տ໺޺໌, ീਘਖ਼৴ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ,2013 ೥ 11 ݄ 30 ೔, ‫ཹٱ‬ถ޻‫ۀ‬େֶ

QCD ૬ਤͱ֩෺࣭ঢ়ଶํఔࣜ:ࠤʑ໦ਸ޺, ‫ڥ‬༞ೋ, ҆෢৳ढ़, Տ໺௨࿠, Տ໺޺໌, ീਘਖ਼৴,‫۝‬େ෼໺ԣஅ‫ڀݚܕ‬ձ -ΫΥʔΫɾ‫֩ࢠݪ‬ɾதੑࢠ੕Λ၆ᛌ͢Δ- , 2014 ೥ 3 ݄ 5 ೔, ‫۝‬भେֶ༗‫ྖ౓ີݶ‬Ҭͷ֨ࢠ QCD ‫ࢉܭ‬ख๏ͷ։ൃ:ߴ‫ڮ‬७Ұ, ࠤʑ໦ਸ޺, Տ໺޺໌, ീਘਖ਼৴, தଜ७೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձ, 2014 ೥ 3 ݄ 28 ೔, ౦ւେֶMeson screening mass ͷԹ౓ɾີ౓ґଘੑʹର͢Δ༗ޮ໛‫ܕ‬Λ༻͍ͨղੳ:ੴҪ༏େ, ࠤʑ໦ਸ޺, ദߒ࢘, Տ໺޺໌, ീਘਖ਼৴೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձ, 2014 ೥ 3 ݄ 28 ೔, ౦ւେֶ֩ࢠണ཭൓ԠͷղੳʹΑΔ෼ޫֶతҼࢠͷܾఆͱͦͷෆఆੑ:ຸໜ޻ক, দຊୖຏ, ॹํҰհ, ീਘਖ਼৴RCNP ‫ڀݚ‬ձ ֩ࢠɾϋΠϖϩϯଟମ‫͚͓ʹܥ‬ΔΫϥελʔ‫ݱ‬৅, 2013 ೥ 7 ݄ 26 ೔, KGUؔ಺ϝσΟΞηϯλʔ൓Ԡஅ໘ੵͷ‫حۮ‬ੑʹ͓͚Δ൓Ԡ‫ߏػ‬:ࠤʑ෦‫ޛ‬, দຊୖຏ, ా্ਅ‫ޔ‬, ‫ཱݹ‬௚໵, ຸໜ޻ক, ਗ਼ਫྑจ, ീਘਖ਼৴31

2013 ೥౓‫ऀࡾ֩ࢠݪ‬एखՆͷֶߍ, 2013 ೥ 8 ݄ 5 ೔, ϗςϧ͖ͨͭ (Ѫ஌‫)ݝ‬ΧΠϥϧ༗ޮཧ࿦ʹ‫ ͍͠৽ͮ͘ج‬G ߦྻ༗ޮ૬‫༻࡞ޓ‬ͷߏஙʹ޲͚ͯ:๛઒কҰ, ຸໜ޻ক, Տ໺௨࿠, ീਘਖ਼৴2013 ೥౓‫ऀࡾ֩ࢠݪ‬एखՆͷֶߍ, 2013 ೥ 8 ݄ 8 ೔, ϗςϧ͖ͨͭ (Ѫ஌‫)ݝ‬4 ମ CDCC ๏ʹ͓͚Δ཭ࢄత෼ղஅ໘ੵͷ࿈ଓԽͱͦͷԠ༻:দຊୖຏ

RCNP/‫۝‬େ‫ڀݚ‬ձ ‫֩ࢠݪ‬෺ཧͱϋυϩϯ෺ཧͷΫϩεΦʔόʔ, 2013 ೥ 9 ݄ 4 ೔, ‫۝‬भେֶΧΠϥϧ༗ޮཧ࿦ͱ G ߦྻཧ࿦ʹΑΔɺQCD ʹ‫͍֩ͨͮج‬൓Ԡͷཧղʹ޲͚ͯ:๛઒কҰ, ຸໜ޻ক, Տ໺௨࿠, ീਘਖ਼৴

RCNP/‫۝‬େ‫ڀݚ‬ձ ‫֩ࢠݪ‬෺ཧͱϋυϩϯ෺ཧͷΫϩεΦʔόʔ, 2013 ೥ 9 ݄ 5 ೔, ‫۝‬भେֶg ߦྻ৞ΈࠐΈ໛‫ܕ‬ΞϓϩʔνʹΑΔඍࢹత֩൓Ԡ࿦:ຸໜ޻ক

RCNP/‫۝‬େ‫ڀݚ‬ձ ‫֩ࢠݪ‬෺ཧͱϋυϩϯ෺ཧͷΫϩεΦʔόʔ, 2013 ೥ 9 ݄ 6 ೔, ‫۝‬भେֶ

CDCC analysis of breakup eﬀects on 6 Li elastic scattering:
S. Watanabe, T. Matsumoto, K. Minomo, K. Ogata, and M. Yahiro
The 12th CNS International Summer School (CNSSS13), August 28, 2013, Saitama,
Japan, Center for Nuclear Study (CNS), the University of TokyoΞΠίφʔϧ൓Ԡཧ࿦ʹΑΔதੑࢠണ཭൓Ԡஅ໘ੵͷ‫ࢉܭ‬:দຊୖຏ, ຸໜ޻কɼॹํҰհɼീਘਖ਼৴
೔ຊ෺ཧֶձळ‫ق‬େձ, 2013 ೥ 9 ݄ 21 ೔, ߴ஌େֶΧΠϥϧ༗ޮཧ࿦ʹ‫ ͍͠৽ͮ͘ج‬G ߦྻ૬‫༻࡞ޓ‬ͷߏஙͱඍࢹత൓Ԡղੳ:๛઒কҰ, ຸໜ޻ক, Տ໺௨࿠, ീਘਖ਼৴೔ຊ෺ཧֶձळ‫ق‬େձ, 2013 ೥ 9 ݄ 21 ೔, ߴ஌େֶඍࢹతཧ࿦ʹΑΔՙిަ‫׵‬൓Ԡͷղੳ:32ຸໜ޻ক, ീਘਖ਼৴೔ຊ෺ཧֶձळ‫ق‬େձ, 2013 ೥ 9 ݄ 21 ೔, ߴ஌େֶ6

Li ஄ੑࢄཚʹ͓͚Δ෼ղޮՌͷ‫ܥ‬౷ੑ:౉ᬒ৻, দຊୖຏ, ຸໜ޻ক, ॹํҰհ, ീਘਖ਼৴೔ຊ෺ཧֶձळ‫ق‬େձ, 2013 ೥ 9 ݄ 21 ೔, ߴ஌େֶ‫֩ࢠݪ‬൓Ԡʹ͓͚Δ 3 ֩ࢠྗͷޮՌ:๛઒কҰ, ຸໜ޻ক, Տ໺௨࿠, ീਘਖ਼৴ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ, 2013 ೥ 11 ݄ 30 ೔, ‫ཹٱ‬ถ޻‫ۀ‬େֶ

Melbourne ༗ޮ૬‫ͱ༻࡞ޓ‬ΧΠϥϧ༗ޮཧ࿦ͷ 3 ֩ࢠྗޮՌ:๛઒কҰ, ຸໜ޻ক, Տ໺௨࿠, ീਘਖ਼৴ab initio ֩ଟମ໰୊ϫʔΫγϣοϓ, 2014 ೥ 2 ݄ 11 ೔, ‫౎ژ‬େֶΧΠϥϧ༗ޮཧ࿦ 3 ֩ࢠྗΛ‫ؚ‬Μͩ༗ޮ૬‫֩ͱ༻࡞ޓ‬-֩ࢄཚ:ຸໜ޻ক, ๛઒কҰ, Տ໺௨࿠, ീਘਖ਼৴ab initio ֩ଟମ໰୊ϫʔΫγϣοϓ, 2014 ೥ 2 ݄ 11 ೔, ‫౎ژ‬େֶඍࢹతཧ࿦ʹΑΔ island of inversion ͷ୳ࡧ:౉ᬒ৻, ຸໜ޻ক, ౢాॆ޺, ా্ਅ‫ޔ‬, ໦ଜਅ໌, ෢ஐຑ໹, ෱ాޫॱ, ੢ଜଠथ, ླ໦݈, দຊୖຏ, ਗ਼ਫྑจ, ീਘਖ਼৴ab initio ֩ଟମ໰୊ϫʔΫγϣοϓ, 2014 ೥ 2 ݄ 11 ೔, ‫౎ژ‬େֶঢ়ଶํఔࣜࡦఆͷ൓Ԡ࿦తΞϓϩʔν:ຸໜ޻ক, ๛઒কҰ, ౉ᬒ৻, ౢాॆ޺, ా্ਅ‫ޔ‬, ໦ଜਅ໌, Տ໺௨࿠, ෢ஐຑ໹, ੢ଜଠथ, ླ໦݈, ෱ాޫॱ, দຊୖຏ, ਗ਼ਫྑจ, ീਘਖ਼৴‫۝‬େ෼໺ԣஅ‫ڀݚܕ‬ձ -ΫΥʔΫɾ‫֩ࢠݪ‬ɾதੑࢠ੕Λ၆ᛌ͢Δ- , 2014 ೥ 3 ݄ 5 ೔, ‫۝‬भେֶ൓Ԡஅ໘ੵͰ୳Δ Mg ಉҐମͷ‫ج‬ఈঢ়ଶͷੑ࣭ സΩཧ࿦ͷ‫͔఺؍‬ΒസΩ:౉ᬒ৻, ຸໜ޻ক, ౢాॆ޺, ా্ਅ‫ޔ‬, ໦ଜਅ໌, ෢ஐຑ໹, ෱ాޫॱ, ੢ଜଠथ, ླ໦݈, দຊୖຏ, ਗ਼ਫྑจ, ീਘਖ਼৴[RIBF-ULIC-029] Progress and Future Plans of the Research Group for Reaction Cross
Sections, 2014 ೥ 3 ݄ 11 ೔, ཧ‫ݚ‬33

Island of Inversion ‫ͦͼٴ‬ͷपลʹ͓͚Δ Mg ಉҐମͷੑ࣭:౉ᬒ৻, ຸໜ޻ক, ౢాॆ޺, ా্ਅ‫ޔ‬, ໦ଜਅ໌, ෢ஐຑ໹, ෱ాޫॱ, ੢ଜଠथ, ླ໦݈, দຊୖຏ, ਗ਼ਫྑจ, ീਘਖ਼৴೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձ, 2014 ೥ 3 ݄ 28 ೔, ౦ւେֶΧΠϥϧ༗ޮཧ࿦ͷ 3 ֩ࢠྗޮՌΛ‫ؚ‬Ή G ߦྻ૬‫༻࡞ޓ‬:๛઒কҰ, ຸໜ޻ক, Տ໺௨࿠, ീਘਖ਼৴೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձ, 2014 ೥ 3 ݄ 30 ೔, ౦ւେֶ֩-֩ࢄཚ͓Αͼ෼ղ൓Ԡʹର͢ΔΧΠϥϧ༗ޮཧ࿦ 3 ֩ࢠྗͷޮՌ:ຸໜ޻ক, ๛઒কҰ, Տ໺௨࿠, ീਘਖ਼৴೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձ, 2014 ೥ 3 ݄ 30 ೔, ౦ւେֶཅࢠ஄ੑࢄཚʹΑΔϋϩʔ֩ͷີ౓෼෍ͷܾఆ:ࠤʑ෦‫ޛ‬, দຊୖຏ, ຸໜ޻ক, ‫ཱݹ‬௚໵, ീਘਖ਼৴೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձ, 2014 ೥ 3 ݄ 30 ೔, ౦ւେֶGogny ૬‫༻࡞ޓ‬Λ༻͍࢛ͨ໘ମม‫֩ܗ‬ͷ‫ڀݚ‬:ా্ਅ‫ޔ‬, ਗ਼ਫྑจ, J. Dudek,

2013 ೥౓‫ऀࡾ֩ࢠݪ‬एखՆͷֶߍ, 2013 ೥ 8 ݄ 8 ೔, ϗςϧ͖ͨͭ (Ѫ஌‫)ݝ‬ม‫ͨ͠ܗ‬ෆ҆ఆ֩Ͱͷ 2 தੑࢠ૬ؔ:ౢాॆ޺, ా্ਅ‫ޔ‬ɺਗ਼ਫྑจ,2013 ೥౓‫ऀࡾ֩ࢠݪ‬एखՆͷֶߍ, 2013 ೥ 8 ݄ 8 ೔, ϗςϧ͖ͨͭ (Ѫ஌‫)ݝ‬఺‫܈‬ͷࣹӨԋࢉࢠΛ༻͍࢛ͨ໘ମม‫ܗ‬εϖΫτϧͷ෼ੳ:ా্ਅ‫ޔ‬, ਗ਼ਫྑจ, J. Dudek,೔ຊ෺ཧֶձळ‫ق‬େձ, 2013 ೥ 9 ݄ 21 ೔, ߴ஌େֶே૔Ωϟϯύε
Ψ΢ε‫ج‬ఈΛ༻͍ͨม‫ͨ͠ܗ‬ෆ҆ఆ֩ͷճసঢ়ଶͷ‫ڀݚ‬:ౢాॆ޺, ా্ਅ‫ޔ‬ɺਗ਼ਫྑจ,೔ຊ෺ཧֶձळ‫ق‬େձ, 2013 ೥ 9 ݄ 21 ೔, ߴ஌େֶே૔Ωϟϯύε
‫͚͓ʹ֩ࢠݪ‬Δ࢛໘ମม‫ܗ‬ʕGogny ૬‫༻࡞ޓ‬Λ༻͍ͨྔࢠ਺ࣹӨ‫ࢉܭ‬:34

ా্ਅ‫ޔ‬, ਗ਼ਫྑจ, J. Dudek,ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ, 2013 ೥ 11 ݄ 30 ೔, ‫ཹٱ‬ถ޻‫ۀ‬େֶΨ΢ε‫ج‬ఈʹΑΔऑଋറม‫֩ࢠݪܗ‬ͷճసঢ়ଶͷ‫ڀݚ‬:ౢాॆ޺, ా্ਅ‫ޔ‬ɺਗ਼ਫྑจ,ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ, 2013 ೥ 11 ݄ 30 ೔, ‫ཹٱ‬ถ޻‫ۀ‬େֶ

Gogny ૬‫༻࡞ޓ‬Λ༻͍ͨྔࢠ਺ࣹӨʹΑΔ࢛໘ମม‫ܗ‬ͷ‫ڀݚ‬:ా্ਅ‫ޔ‬, ਗ਼ਫྑจ, J. Dudek,೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձ, 2013 ೥ 3 ݄ 27 ೔, ౦ւେֶভೆΩϟϯύε
Ψ΢ε‫ج‬ఈΛ༻͍ͨม‫ͨ͠ܗ‬ෆ҆ఆ֩ͷճసঢ়ଶͷ‫ ڀݚ‬II:
ౢాॆ޺, ా্ਅ‫ޔ‬ɺਗ਼ਫྑจ,೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձ, 2013 ೥ 3 ݄ 27 ೔, ౦ւେֶভೆΩϟϯύε
‫֩ࢠݪ‬ͷภॏม‫ܗ‬༏੎ʹ͓͚Δ Strutinsky ๏ͷ‫ࢹڊ‬త෦෼ͷ‫د‬༩̞̞:ߴ‫ݪ‬఩࢜, ాౢ௚थ, ਗ਼ਫྑจ,೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձ, 2013 ೥ 3 ݄ 27 ೔, ౦ւେֶভೆΩϟϯύε
ҎԼ, ϙελʔൃද.
༗‫ྖ౓ີݶ‬Ҭʹ͓͚ΔΧϥʔःณϙςϯγϟϧ:ߴ‫ڮ‬७Ұ, Ӭా‫ܡ‬ଠ࿠, ࡈ౻୎໵, தଜ७, ࠤʑ໦ਸ޺, Տ໺޺໌, ീਘਖ਼৴‫ڀݚݚج‬ձʮ೤৔ͷྔࢠ࿦ͱͦͷԠ༻ʯ2013 ೥ 8 ݄ 26 ೔, ‫౎ژ‬େֶ‫ૅج‬෺ཧֶ‫ॴڀݚ‬൓Ԡஅ໘ੵͷղੳͰ୳Δதੑࢠա৒ Mg ಉҐମͷੑ࣭:౉ᬒ৻, ຸໜ޻ক, ౢాॆ޺, ా্ਅ‫ޔ‬, ໦ଜਅ໌, ෢ஐຑ໹, ෱ాޫॱ, ੢ଜଠथ, ླ໦݈, দຊୖຏ, ਗ਼ਫྑจ, ീਘਖ਼৴2013 ೥౓‫ऀࡾ֩ࢠݪ‬एखՆͷֶߍ, 2013 ೥ 8 ݄ 5 ೔, ϗςϧ͖ͨͭ (Ѫ஌‫)ݝ‬ΧΠϥϧ༗ޮཧ࿦ʹ‫ ͍͠৽ͮ͘ج‬G ߦྻ༗ޮ૬‫༻࡞ޓ‬ͷߏஙʹ޲͚ͯ:๛઒কҰ, ຸໜ޻ক, Տ໺௨࿠, ീਘਖ਼৴2013 ೥౓‫ऀࡾ֩ࢠݪ‬एखՆͷֶߍ, 2013 ೥ 8 ݄ 5 ೔, ϗςϧ͖ͨͭ (Ѫ஌‫)ݝ‬൓Ԡஅ໘ੵͷ‫حۮ‬ੑʹ͓͚Δ൓Ԡ‫ߏػ‬:35

ࠤʑ෦‫ޛ‬, দຊୖຏ, ా্ਅ‫ޔ‬, ‫ཱݹ‬௚໵, ຸໜ޻ক, ਗ਼ਫྑจ, ീਘਖ਼৴2013 ೥౓‫ऀࡾ֩ࢠݪ‬एखՆͷֶߍ, 2013 ೥ 8 ݄ 5 ೔, ϗςϧ͖ͨͭ (Ѫ஌‫)ݝ‬֎෦ࢿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ, ಛผ‫ڀݚ‬һ঑ྭඅୈҰ‫ݪ‬ཧ‫͍ͨͮجʹࢉܭ‬༗ޮ໛‫ʹܕ‬ΑΔ QCD ૬ਤɾQCD ঢ়ଶํఔࣜͷఆྔతܾఆ
‫ڀݚ‬୅දऀ: ࠤʑ໦ਸ޺
จ෦লՊֶ‫ڀݚ‬අิॿۚ, ಛผ‫ڀݚ‬һ঑ྭඅθ ਅۭΛߟྀͨ֨͠ࢠ QCD ʹΑΔ QCD ૬ߏ଄ͷղ໌‫ڀݚ‬୅දऀ: ߴ‫ڮ‬७ҰจՊলՊֶ‫ڀݚ‬අิॿۚɺಛผ‫ڀݚ‬һ঑ྭඅඍࢹతཧ࿦ʹΑΔෆ҆ఆ֩ͷߏ଄ͱ൓Ԡͷ‫ܥ‬౷తղ໌‫ڀݚ‬୅දऀ: ຸໜ޻কจՊলՊֶ‫ڀݚ‬අิॿۚɺಛผ‫ڀݚ‬һ঑ྭඅඍࢹత൓Ԡɾߏ଄ཧ࿦ʹΑΔෆ҆ఆ֩ߏ଄ͷ‫ܥ‬౷తղ໌‫ڀݚ‬୅දऀ: ౉ᬒ৻จՊলՊֶ‫ڀݚ‬අิॿۚɺಛผ‫ڀݚ‬һ঑ྭඅྔࢠ਺ࣹӨ๏Λ༻͍ͨ‫͚͓ʹ֩ࢠݪ‬ΔΤΩκνοΫͳม‫ܗ‬ɾճసঢ়ଶͷ‫ڀݚ‬‫ڀݚ‬୅දऀ: ా্ਅ‫ޔ‬จՊলՊֶ‫ڀݚ‬අิॿۚɺ‫ج‬൫‫( ڀݚ‬C)
ߴεϐϯɾΤΩκνοΫม‫֩ࢠݪܗ‬ͷ‫ڀݚ‬‫ڀݚ‬୅දऀ: ਗ਼ਫྑจ จ෦লՊֶ‫ڀݚ‬අิॿۚҎ֎ͷ֎෦ࢿۚ ೔ຊֶज़ৼ‫ڵ‬ձಛผ‫ڀݚ‬һ౳‫ڞͼٴ‬ಉ‫ڀݚ‬ͷ࠾୒ (ֶ֎͔Βͷड͚ೖΕΛ‫ؚ‬Ή)36ຸໜ޻কɺ೔ຊֶज़ৼ‫ڵ‬ձಛผ‫ڀݚ‬һ (PD)ࠤʑ໦ਸ޺ɺ೔ຊֶज़ৼ‫ڵ‬ձಛผ‫ڀݚ‬һ (DC1)ా্ਅ‫ޔ‬ɺ೔ຊֶज़ৼ‫ڵ‬ձಛผ‫ڀݚ‬һ (DC2)ߴ‫ڮ‬७Ұɺ ೔ຊֶज़ৼ‫ڵ‬ձಛผ‫ڀݚ‬һ (DC1)౉ᬒ৻ɺ೔ຊֶज़ৼ‫ڵ‬ձಛผ‫ڀݚ‬һ (DC1)ଞେֶͰͷ‫ڭͱڀݚ‬ҭਗ਼ਫྑจɿେࡕେֶཧֶ෦Ͱʮ‫֩ࢠݪ‬ͷߴ଎ճసঢ়ଶʯͱ͍͏λΠτϧͰ̏೔ؒͷूதߨٛΛߦͬͨɻ
ֶ෦̐೥ੜଔ‫ڀݚۀ‬ʲલ‫ظ‬ʳळࢁཅฏɺҪੜ෢ࢤɺฏ઒༏ਅɺ‫ٶ‬ຊ߉୓ (୲౰: দຊ)ίϯϐϡʔλΛ༻͍ͨ‫ڀݚ֩ࢠݪ‬௒ೖ໳ʲ‫ظޙ‬ʳฏ઒༏ਅɺ‫ٶ‬ຊ߉୓ (୲౰: ീਘɺਗ਼ਫɺদຊ)৔ͷྔࢠ࿦ɺ֩൓Ԡ࿦ɺ֩ߏ଄࿦ͷྠߨɾ‫ڀݚ‬म࢜࿦จੴҪ༏େ: (ࢦಋ‫ڭ‬һ, ീਘਖ਼৴): ༗‫ݶ‬Թ౓ʹ͓͚Δதؒࢠःณ࣭ྔͷ༗ޮ໛‫ʹܕ‬ΑΔಋग़ߐ಄‫ܛ‬:(ࢦಋ‫ڭ‬һɺീਘਖ਼৴ɺদຊୖຏ): ೋॏ৞ΈࠐΈ໛‫͚͓ʹܕ‬Δ༗ޮ૬‫༻࡞ޓ‬ͷີ౓ґଘੑͷऔΓѻ͍ࠤʑ෦‫ޛ‬:(ࢦಋ‫ڭ‬һɺീਘਖ਼৴ɺদຊୖຏ): ཅࢠ஄ੑࢄཚʹΑΔϋϩʔ֩ͷີ౓෼෍ͷܾఆ๛઒কҰ:(ࢦಋ‫ڭ‬һɺീਘਖ਼৴): ‫֩ࢠݪ‬஄ੑࢄཚʹ͓͚Δ̏֩ࢠྗޮՌ

ത࢜࿦จࠤʑ໦ਸ޺: (ࢦಋ‫ڭ‬һɺീਘਖ਼৴): QCD thermodynamics under extreme conditions

37(‫ݶۃ‬ঢ়ଶʹ͓͚Δ QCD ೤ྗֶ)[2014 ೥ 3 ݄त༩]ͦͷଞͷ‫׆‬ಈͱ੒Ռࠤʑ໦ਸ޺: ηϛφʔ (University of Wroclaw, Division of Elementary Particle The-ory)ࠤʑ໦ਸ޺: αΠΤϯεΧϑΣʹͯߨԋຸໜ޻ক: RCNP/‫۝‬େ‫ڀݚ‬ձʮ‫֩ࢠݪ‬෺ཧͱϋυϩϯ෺ཧͷΫϩεΦʔόʔʯ, ੈ࿩ਓຸໜ޻ক: ‫۝‬େ෼໺ԣஅ‫ڀݚܕ‬ձ —ΫΥʔΫɾ‫֩ࢠݪ‬ɾதੑࢠ੕Λ၆ᛌ͢Δ—, ੈ࿩ਓ୅ද¡ຸໜ޻ক: େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔཧ࿦෦ηϛφʔ, ߨࢣ౉ᬒ৻: ‫ऀࡾ֩ࢠݪ‬एखՆͷֶߍ, ‫֩ࢠݪ‬ύʔτੈ࿩ਓ38Ӊ஦෺ཧཧ࿦
‫ߏࣨڀݚ‬੒һ‫ڮ‬ຊ ਖ਼ষ ‫ڭ‬तࢁԬ ‫ڭॿ ۉ‬ொా ਅඒ ॿ‫ڭ‬খ໺ উਉ (H25 ೥ 10 ݄ΑΓ) ॿ‫ڭ‬

E. P. B. A. Thushari ςΫχΧϧελοϑ໺ా ৗ༤ (2013 ೥ 9 ݄·Ͱ) ςΫχΧϧελοϑ େֶӃ ത࢜՝ఔ 
দඌ ߁ल

٠஑ ೭޺

 େֶӃ म࢜՝ఔ Ұ੓ ྒྷଠ࿠ख௩ ‫ܒ‬

ྛాߊଠ࿕

෱ా ྒྷฏ

ߴ໦ ߁ฏ

कా ՂӬ

ࡾદ ‫ܛ‬ਓ ֶ෦ ଔ‫ڀݚۀ‬ੜ 
২໦ ༤࠸

Ӊࠜ ྒྷฏ

‫ेޒ‬ཛྷ ॣଠӬ໺ ཾଠ࿠ ๚໰‫ ऀڀݚ‬தଜ ཧԝ୲౰त‫ۀ‬• ‫ڮ‬ຊਖ਼ষ
ശ࡚஍۠: ࠷ઌ୺෺ཧֶɺࣗવՊֶ֓࿦ (લ‫ظ‬ʣ, Ӊ஦෺ཧֶ (‫)ظޙ‬ҏ౎஍۠: ྗֶ‫ૅج‬ɾಉԋश (લ‫)ظ‬• ࢁԬ‫ۉ‬ശ࡚஍۠ɿཧ‫ܥ‬ओ୊Պ໨ III(લ‫ظ‬, ‫)ظޙ‬, ෺ཧֶθϛφʔϧ (‫)ظޙ‬ҏ౎஍۠ɿࣗવՊֶ૯߹࣮‫( ݧ‬લ‫ظ‬, ‫)ظޙ‬, গਓ਺ηϛφʔ (‫)ظޙ‬• খ໺উਉ
ശ࡚஍۠ɿి࣓‫ ֶؾ‬Iɾಉԋशʢ‫ظޙ‬ʣҏ౎஍۠ɿͳ͠

39‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ
Χϥʔ௒఻ಋঢ়ଶͷΫΥʔΫ෺࣭Λߟྀͨ͠ߴີ౓੕ͷྫྷ٫‫ڮ( ࢉܭ‬ຊਖ਼ষɼ໺ాৗ༤)Χϥʔ௒఻ಋΛ‫ؚ‬ΉΫΥʔΫɾϋυϩϯࠞ߹૬ͱ֩ࢠͷ௒ྲྀಈΛߟྀͨ͠ߴີ౓ੑ (ϋΠϒϦου੕) ͷྫྷ٫‫ࢉܭ‬Λৄࡉʹߦͬͨɻ‫ڈ‬೥౓·ͰɺCassiopeia A(Ҏ߱: Cas A) ͷԹ౓มԽΛઆ໌ՄೳͳϞσϧͷߏஙɺ͓ΑͼͦΕΛ༻͍ͨྫྷ٫‫ࢉܭ‬Λߦ͍ͬͯͨɻ͔͠͠ͳ͕Βɺঢ়ଶํఔ͕ࣜଞͷ‫؍‬ଌ݁Ռ (ಛʹ M  2.0M ͷ‫؍‬ଌ݁Ռ) ͱໃ६͍ͯͨͨ͠Ίɺ࠷େ࣭ྔ͕ M > 2.0M ΛຬͨͤΔΫΥʔΫ෺࣭·Ͱߟྀͨ͠ঢ়ଶํఔࣜΛಋೖ͠ϞσϧΛߏங͢Δඞཁ͕ੜͨ͡ɻM > 2.0M
Λຬͨ͢ΫΥʔΫ෺࣭ೖΓͷঢ়ଶํఔࣜΛ༻͍ɺྫྷ٫Ϟσϧ (Χϥʔ௒఻ಋɾ֩ࢠͷ௒ྲྀಈΛߟྀ) Λߏஙͨ͠ɻςετ‫ࢉܭ‬ͷஈ֊Ͱ͋Δ͕ɺҎલͷঢ়ଶํఔࣜͰ֬ೝ͞Ε͍ͯͨɺ“ॏ͍੕͕ྫྷ͑ʹ͍ܰ͘͘੕͕ྫྷ͑΍͍͢” ͱ͍͏ঢ়‫گ‬ͷ࠶‫ݱ‬Λ֬ೝͨ͠ɻࠓ‫ޙ‬͸ɺ͜ͷ 2.0M ʹ౸ୡՄೳͳঢ়ଶํఔࣜΛ༻͍ɺৄࡉͳྫྷ٫‫͓ࢉܭ‬Αͼ࿈੕‫͚͓ʹܥ‬Δ೤తਐԽʹ΋֦ு͍ͯ͘͠༧
ఆͰ͋Δɻ·ͨɺ৽ͨʹग़͖ͯͨ Cas A ͷ‫؍‬ଌ݁Ռ (‫ྫྷͳٸ‬٫͕‫ )͍ͳ͍͖ͯى‬Λઆ໌Մೳͳ
‫ࢉܭ‬Λߦ͍ɺ‫֩ࢠݪ‬෺ཧͱໃ६ͷͳ͍தੑࢠͷ௒ྲྀಈϞσϧͷ੕΁ͷԠ༻Λ୳͍͖͍ͬͯͨɻ
Observational constraints of cosmological models with variable equation of state(‫ڮ‬ຊਖ਼ষ, E. P. B. A. Thushari)
Analyzing the dark energy equation of state is one of the useful way to avoid the barriers whichappear through the modiﬁcation of the theoretical models. We focus our attention on how the
evolving Equation of state (EoS) for matter and dark energy can modify the standard model.
Rather than investigating a speciﬁc dark energy model, the number of dark energy models
including the cosmological constant through the variable EoS has been proposed (Hannestad& E. Motsel 2004). Later on J. Ponce de Leon (2012) has investigated how the evolving
equation of matter and dark energy might modify the ΛCDM paradigm. These authors
have done analytical simulation to investigate the signiﬁcant role of dark energy and how theprimordial equation of state of matter contribute to the present acceleration and so on. We
focus on constructing a cosmological model with the observations to have the appropriate
EoS. Since these models are having the cosmological parameters like Hubble parameter(H),energy density parameter (Omega), decelerating parameter (q) and stateﬁnder parameter (r),it allows to express them as functions of redshift. Modiﬁcation has done through the variable
EoS for the matter mixture. Then the parametrization of dark energy is also considered. It is
ﬁne tuning to constrain the parameters through the observations and we use SNIa observation
to investigate the validity of this model at the present stage of acceleration.
਌੕ͷ֎૚ͷҧ͍ʹΑΔ௒৽੕࢒֚‫ܗ‬੒࣌ͷ෺࣭ࠞ߹ͷγϛϡϨʔγϣϯ (‫ڮ‬ຊਖ਼ষ, দඌ߁ल)௒৽੕࢒֚ Cassiopeia A(CasA) Ͱ‫ݟ‬ΒΕΔΑ͏ͳ Fe ͱ Si ͷ෺࣭ࠞ߹ͷϝΧχζϜΛௐ΂ΔͨΊʹɺ௒৽੕രൃ௚‫͔ޙ‬Β௒৽੕࢒֚‫ܗ‬੒·Ͱͷ‫ٿ‬ରশ‫ࢉܭ‬Λߦ͍ɺͲͷΑ͏ͳϞσϧͰྲྀମෆ҆ఆੑʹΑΔ Fe ͱ Si ͷ෺࣭ࠞ߹͕‫͜ى‬Δͷ͔ௐ΂ͨɻࡢ೥౓͸ɺ਌੕ͷ߃੕෩ͷ଎౓ͱ
Wolf-Rayet wind ͷ‫ܧ‬ଓ࣌ؒΛύϥϝʔλͱͯ͠‫ڀݚ‬ΛߦͬͨͷͰɺࠓ೥౓͸͞Βʹ਌੕ͷ֎૚ΛύϥϝʔλʹՃ͑ͯγϛϡϨʔγϣϯͨ͠ɻͦͷ݁Ռɺ߃੕෩ͷ଎౓΍ wind ͷ‫ܧ‬ଓ࣌ؒ͸ Fe ΍ Si ෼෍ͷ࣌ؒਐԽʹ΄ͱΜͲӨ‫ڹ‬Λ༩͑ͳ͍͕ɺ਌੕ͷ֎૚͸ඇৗʹେ͖ͳӨ‫ڹ‬Λ༩͑Δ͜ͱ͕෼͔ͬͨɻ͞Βʹྲྀମෆ҆ఆੑʹΑΓ Fe ͱ Si ͷ෺࣭ࠞ߹Λ‫ͨ͢͜ى‬Ίʹ͸਌੕ͷ
He ૚͕߃੕෩ʹΑΓଟࣦ͘ΘΕ͍ͯΔඞཁ͕͋Δ͜ͱ͕෼͔ͬͨɻҰํɺ‫؍‬ଌ͔Β͸ Cas A͸ II̱‫ܕ‬௒৽੕രൃΛ‫͕ͱͨ͜͜͠ى‬෼͔͓ͬͯΓɺͦΕ΄Ͳ He ֎૚Λࣦ͍ͬͯͳ͍ͱߟ͑ΒΕ͍ͯΔɻࠓ‫ޙ‬͸ɺզʑͷγϛϡϨʔγϣϯͷ݁Ռͱ‫؍‬ଌͷᴥᴪΛղܾ͢΂ٞ͘࿦Λߦ͏ඞཁ͕͋Δɻେ࣭ྔ੕ͷ߃੕ਐԽ͓Αͼ௒৽੕രൃʹ͓͚Δ triple-α ൓Ԡ཰ͷෆఆੑʹΑΔӨ‫ڮ( ڹ‬ຊਖ਼ষ,٠஑೭޺, খ໺উਉ)2009 ೥ʹ Ogata et al. ʹΑͬͯ৽͘͠ triple-Ћ൓Ԡ཰ (OKK rate) ͕ൃද͞Εͨɻtriple -α ൓Ԡ40͸̏ͭͷϔϦ΢Ϝ͔Β̍ͭͷ୸ૉΛ߹੒͢Δ൓ԠͰ͋Δɻ͜ͷ൓Ԡ཰͸߃੕಺ͰϔϦ΢Ϝ೩ম͕‫͖ى‬ΔԹ౓Ͱैདྷͷ΋ͷ (Fynbo et al. 2005)(Fynbo rate) ΑΓ 105 ఔ౓େ͖͍ɻ·ͨɺtripleЋ൓Ԡ͸߃੕಺ͷ‫ݩ‬ૉ૊੒Ϟσϧ͕มΘΔՄೳੑ͕͋Δɻtriple-Ћ൓Ԡ͸ɺਐԽʹ͓͚Δओཁͳ‫ݩ‬ૉͰ͋Δ 1 2C ͱ 1 6O ʹؔΘΔॏཁͳ൓ԠͰ͋ΓɺOKK rate Λ༻͍ͨ߃੕ਐԽ‫ࢉܭ‬ฒͼʹ‫ݩ‬ૉ߹੒‫ࢉܭ‬͸ैདྷͷ݁ՌΛม͑ΔՄೳੑ͕͋Δɻͦ͜ͰɺOKK rate ͱ Fynbo rate ʹ͍ͭͯେ࣭ྔ੕ʹ͓͚Δ‫ݩ‬ૉ߹੒ʹ͍ͭͯ߃੕ਐԽͱ௒৽੕രൃͷ‫ࢉܭ‬Λߦͳ͍݁ՌΛൺֱͨ͠ɻ
8M He core ϞσϧΛ༻͍ͯ‫ࢉܭ‬ΛߦͬͨɻHe ೩ম࣌ʹ OKK rate Ͱ͸ 12 C ͕ա৒ʹ࡞ΒΕɺͦͷ෼ 16 O ͕‫ݮ‬গ͢Δͱ͍͏݁Ռ͕ಘΒΕͨɻͦͷ‫ޙ‬ͷ೩মஈ֊Ͱ΋͜ΕΒͷӨ‫͕ڹ‬දΕɺࢎૉ૚͕ωΦϯ૚ʹ͔ΘΔͳͲਐԽͷ࠷ऴஈ֊Ͱͷߏ଄ʹӨ‫ڹ‬Λ༩͑Δ͜ͱ͕෼͔ͬͨɻ߃੕಺
෦Ͱੜ੒͞Εͨ‫ݩ‬ૉͷྔΛ‫؍‬ଌͱൺֱ͢ΔͨΊʹ௒৽੕രൃʹΑͬͯ‫ݩ‬ૉͷ์ग़ྔΛ‫͠ࢉܭ‬ɺۜՏͷϋϩʔʹଘࡏ͢Δ߃੕ͷද໘ͷ૊੒ͱൺֱͨ͠ɻ12 C ͱ 16 O ͷൺʹ͍ͭͯ OKK rate Ͱ͸‫؍‬ଌͱେ͖͘ҟͳΔ݁Ռͱͳͬͨɻ·ͨɺ4M -16M He core ʹ͍ͭͯ 4 Ϟσϧͷ‫ࢉܭ‬Λߦ͍ɺ߃੕ͷ࣭ྔͷҧ͍ʹ΋ͨΒ͢Ө‫ڹ‬Λௐ΂ͨɻ4M ϞσϧͰ͸ Ne ೩ম࣌ʹத৺Ͱ͸ͳ͘֎ଆͰ೩ম͕࢝·ΓɺΑΓ௿࣭ྔͷ߃੕ͷৼΔ෣͍Λࣔͨ͠ɻ͞ΒͳΔղੳΛਐΊɺ‫؍‬ଌͱͷൺֱΛߦ͏༧ఆͰ͋Δɻ
৽͍͠ఱମ֩൓Ԡ཰ͱӉ஦ॳ‫ݩظ‬ૉ߹੒ (‫ڮ‬ຊਖ਼ষ, தଜཧԝɼҰ੓ྒྷଠ࿠)Ӊ஦ॳ‫͖ىʹظ‬Δ‫ݩ‬ૉ߹੒͸Ϗοάόϯ‫ݩ‬ૉ߹੒ (BBN) ͱΑ͹Εɺܰ‫ݩ‬ૉ (4 HeɼD ౳) ͷ‫ى‬‫ݯ‬Λઆ໌Ͱ͖Δཧ࿦ͱͯ͠੒ޭΛऩΊ͖ͯͨɻ͔͠͠ͳ͕ΒɺBBN ͔Β༧ଌ͞ΕΔ֤ܰ‫ݩ‬ૉͷྔͱ‫؍‬ଌ஋͸ඞͣ͠΋Ұக͍ͯ͠ͳ͍ɻࠓճɺ֩൓Ԡ཰ґଘੑΛௐ΂Δҝʹ Descouvemont etal.(2004) ʹΑͬͯ‫ٻ‬ΊΒΕͨ֩൓Ԡ཰ͱɺNACRE-II ͷ൓Ԡ཰ (2013) Λ༻͍ൺֱΛߦͬͨɻซ
ͤͯ Monte Carlo ๏Λ༻͍Δ͜ͱͰ൓Ԡ཰ͷෆఆੑ΋ߟྀͨ͠ɻͦͷ݁Ռɺதੑࢠण໋ͷ࠷৽஋
880.1±1.1 ඵΛ༻͍Δ‫ݶ‬ΓɺBBN ͷओཁ‫ݩ‬ૉͰ͋Δ 4 He ͱ D ͷཧ࿦஋͔Β baryon-to-photon
ratio η ͷ஋͕ܾ·Βͳ͍ࣄΛࣔͨ͠ɻͦ͜Ͱɺ͜ΕΛղܾ͢Δҝʹඇඪ४Ϟσϧͱͯ͠ϨϓτϯඇରশੑΛߟྀͨ͠ BBN ϞσϧΛ࠾༻͠‫ࢉܭ‬Λߦͬͨɻ͜ͷඇରশੑ͸ՙిதੑͳχϡʔτϦϊηΫλʔͷଘࡏͷͨΊʹ‫ڐ‬༰͞ΕΔɻ͜ΕΛߟྀͨ݁͠Ռɺ4 He ͱ D ͔Β η ͷൣғΛܾΊΔࣄ͕Ͱ͖ΔΑ͏ʹͳΓɺ·ͨඇରশੑʹର͢Δ੍‫ݶ‬Λಘͨɻதੑࢠ੕ͷྫྷ٫ͱঢ়ଶํఔࣜʹ͍ͭͯ (‫ڮ‬ຊਖ਼ষɼ໺ాৗ༤ɼྛాߊଠ࿕)Cassiopeia A ͷத৺ఱମ͸தੑࢠ੕Ͱ͋Δͱߟ͑ΒΕ͍ͯΔɻ࠷৽ͷ‫؍‬ଌʹΑΕ͹ɺ͜ͷఱମͷද໘Թ౓ͷ‫؍‬ଌ݁Ռ͸ैདྷͷ‫؍‬ଌͱҟͳΔ݁ՌΛࣔͨͨ͠Ίɺఱମͷ࣭ྔɺද໘૊੒ɺঢ়ଶ
ํఔࣜɺྫྷ٫ϓϩηεʹॏ఺Λஔ͖ɺ࠷৽ͷ‫؍‬ଌ݁Ռ͕࠶‫͔͏Ͳ͔͍ͳ͖Ͱݱ‬ௐ΂ͨɻ݁Ռɺ
ैདྷͷ‫؍‬ଌ݁ՌͰ͸ඞཁͱ͞Εͨ Non-Standard ͳྫྷ٫ϓϩηε͕ͳ͘ͱ΋ɺ৚݅࣍ୈͰ͸‫؍‬ଌ݁ՌΛઆ໌Ͱ͖ΔͷͰ͸ͳ͍͔ͱߟ͍͑ͯΔɻ਌੕ͷඇ‫ٿ‬ରশੑ͕௒৽੕രൃ಺෦ͷྲྀମෆ҆ఆੑʹ‫͢΅ٴ‬Ө‫ڮ( ڹ‬ຊਖ਼ষ, খ໺խਉ, ख௩‫)ܒ‬਌੕ͷඇ‫ٿ‬ରশੑ͕௒৽੕രൃ಺෦ͷྲྀମෆ҆ఆੑʹ༩͑ΔӨ‫ڹ‬Λௐࠪ͢ΔͨΊɺ؆୯ͳϞσϧΛͨͯͯ਺஋‫ࢉܭ‬Λߦͬͨɻઌߦ‫ʹڀݚ‬ΑΓɺॏྗ่յ௚લͷେ࣭ྔ੕಺෦Ͱ͸‫͍ڧ‬ཚྲྀ͕
ੜ͡ΔՄೳੑ͕༗Δ͜ͱ͕ࣔࠦ͞Ε͍ͯΔʢArnett+2011ʣɻ͜Ε·Ͱ͸‫ٿ‬ରশͳ਌੕ΛԾఆͯ͠‫ࢉܭ‬Λߦ͓ͬͯΓɺඇ‫ٿ‬ରশͳ਌੕ʹ͍ͭͯ͸ߟྀ͍ͯ͠ͳ͔ͬͨɻͦ͜Ͱɺඇ‫ٿ‬ରশੑͷ൓өͱͯ͠௒৽੕಺෦ʹ༷ʑͳઁಈΛ༩͑ɺ‫ࢉܭ‬Λߦͬͨɻͦͷ݁Ռɺ‫ٿ‬ରশͳ਌੕͔Βͷ‫ͱࢉܭ‬ൺֱͯ͠େ͖ͳҧ͍͸‫ݟ‬ΒΕͳ͔ͬͨɻࠓ೥౓͸‫ࢉܭ‬ղ૾౓ͷ޲্΍࣍‫ݩ‬ൺֱղੳΛߦ͏༧ఆͰ͋Δɻಥൃఱମ‫ݱ‬৅ͷϑΥϩʔΞοϓ‫؍‬ଌ (ࢁԬ‫)ۉ‬୹͍λΠϜεέʔϧͰޫ౓มಈ͢Δʮಥൃఱମʯͷ‫ڀݚ‬ΛਐΊ͍ͯΔɻࡢ೥౓·ͰʹҾ͖ଓ͖,ຊ೥౓΋, ᛙ৽੕ɾ৽੕ɾ௒৽੕ʹ͍ͭͯ, ൃ‫ݟ‬௚‫ޙ‬ͷ෼ޫ΍ଌޫͳͲΛ௨ͯͦ͡ͷੑ࣭ͷղ໌Λ໨ࢦ͢ɻߨԋͳͲΛ௨ͯ͡, ಥൃఱମͷൃ‫ݟ‬΍ϑΥϩʔΞοϓ‫؍‬ଌͷॏཁੑΛૌ͑, ෼໺Λ‫׆‬ੑԽ͍ͯ͘͠ɻຊ೥౓͸, ࠃࡍఱจֶ࿈߹ IAU ʹ͓͚Δ৽ఱମ৘ใͷऔΓѻ͍Λ‫׆‬ੑԽ͢Δ͜ͱΛ໨ඪͱͨ͠ɻಥൃఱମͷϑΥϩʔΞοϓɾൃ‫֬ݟ‬ೝΛ਺݅ߦͳͬͨɻ৽ఱମʹಛԽͨ͠ߨ

41ԋ΍‫ࣥࣄه‬චͳͲ, ಥൃఱମʹ͍ͭͯप஌‫ൃܒ‬Λߦͳͬͨɻࠃࡍతʹ৽ఱମ৘ใΛऔΓѻ͏ఱจిใதԝ‫ ہ‬CBAT (http://www.cbat.eps.harvard.edu/) ͸‫ࡏݱ‬, ਓखͱࢿۚ྆໘͕ෆ଍
Ͱ͋Γɺͦͷରࡦ͸‫ٸ‬຿Ͱ͋ΔɻࢁԬ͸ࠃࡍఱจֶ࿈߹ IAU ʹ͓͍ͯ CBAT Λ౷‫ׅ͢‬Δୈ 6
ҕһձͷҕһ௕ͱͯ͠, ͜ͷରԠࡦΛࡦఆதͰ͋Δɻ࣍೥౓Ҏ߱΋, ಥൃఱମ΁ͷ࣮஍ଈԠΛଓ
͚Δͱͱ΋ʹ, CBAT ͷ‫׆‬ੑԽΛ໛ࡧ͢ΔɻΞʔΧΠϒఱจֶͷߏங (ࢁԬ‫ۉ‬, ߴ໦߁ฏ, ࡾદ‫ܛ‬ਓ)σδλϧԽٕज़΍ίϯϐϡʔλωοτϫʔΫͷൃలʹΑΓ, αʔϕΠ‫؍‬ଌͳͲͰ࡞੒͞Εͨఱମσʔλϕʔε΍ը૾Λ༻͍ͨఱମ‫ʹڀݚ‬σʔλϕʔεఱจֶ͕, ۙ೥ՄೳʹͳΓ‫ޫ٭‬Λཋͼ͍ͯΔɻΘΕΘΕ͸͜ΕʹՃ͑, அยతͳࢿྉ΋༻͍ͨʮΞʔΧΠϒఱจֶʯΛఏҊ࣮͠ફ
͢Δɻࠓ೥౓ͷ໨ඪ͸, ଞͷ໨తͰಘΒΕͨαʔϕΠը૾ʹ͓͚Δ௒৽੕γϣοΫϒϨʔΫΞ΢τͷ૞ࡧ, ͓Αͼ๲େͳଌޫσʔλͷ‫͋Ͱ༻׆‬Δɻ೔ຊεϖʔεΨʔυ‫ڠ‬ձ͕ӡ༻͢Δඒ੕εϖʔεΨʔυηϯλʔͰ͸, ਓ޻Ӵ੕ͷτϥοΩϯά΍஍‫ۙ઀ٿ‬খ࿭੕ͷ‫ݕ‬ग़Λ໨తͱͨ͠
αʔϕΠ‫؍‬ଌΛ࣮ࢪ͍ͯ͠Δɻ͜ͷαʔϕΠը૾Ͱ௒৽੕Λ‫ݕ‬ग़Ͱ͖ͳ͍͔Λ‫ݕ‬౼͍ͯ͠Δɻ
ࠓ೥౓͸, ௒৽੕രൃͷিܸ೾͕߃੕ද໘ʹୡͨ͠ॠؒͷγϣοΫϒϨʔΫΞ΢τ͕ඒ੕ը૾Ͱ
ͱΒ͑ΒΕ͍ͯΔ͔Ͳ͏͔૞ࡧ͠, ࣮ྫ͸‫ݟ‬౰Βͳ͔͕ͬͨํ๏Λཱ֬ͨ͠ɻ࣍೥౓͸, ඒ੕ηϯλʔը૾ͷΈ͔Βͷ৽͍͠௒৽੕ͷ‫ݕ‬ग़Λ໨ࢦ͢ɻέϓϥʔ‫؍‬ଌ‫ػ‬͸, ‫֎ܥ‬࿭੕ͷτϥϯδο
τ‫ݕ‬ग़Λ໨ࢦͯ͠, ߴਫ਼౓͔ͭߴ࣌ؒ෼ղͷ߃੕ଌޫσʔλΛ஝ੵ͍ͯ͠Δɻ͜ΕΛ༻͍ͨ߃੕ຊମͷมಈʹ͍ͭͯͷ‫͕ڀݚ‬੝ΜʹߦͳΘΕ͍ͯΔ͕ɺଟ͘ͷ‫Ͱڀݚ‬͸ର৅ͱͳΔ߃੕ΛߜΔͳͲͯ͠, σʔλશମΛѻ͍ͬͯͳ͍ɻࠓ೥౓͸, େྔσʔλΛ͢΂ͯѻ͏ख๏Λ໛ࡧ͠, प‫ظ‬ղੳʹ͍ͭͯ͸શྔͷ࢖༻ΛՄೳʹͨ͠ɻ࣍೥౓͸ଞͷํ๏ʹΑΔղੳΛ࣮ࢪ͢ΔɻεϖʔεσϒϦͷՄࢹޫ‫؍‬ଌ (ࢁԬ‫)ۉ‬஍‫ٿ‬पճ‫ي‬ಓʹ͓͚ΔεϖʔεσϒϦ͸૿ՃͷҰ్ΛͨͲ͓ͬͯΓ, Ӊ஦ར༻ͷେ͖ͳ‫ڴ‬ҖͱͳΓͭͭ͋Δɻಛʹ, ഁࡅΠϕϯτͰൃੜ͢ΔσϒϦͷัଊͱ௥੻͸, ࠓ‫ޙ‬ͷӉ஦‫ڥ؀‬Λେ͍ʹࠨӈ͢Δɻࠓ೥౓͸, σϒϦ‫؍‬ଌʹ͓͚Δ࠲ඪ‫ܥ‬ม‫׵‬Λߟ࡯ͨ͠ɻIHIɾJAXA ͱਐΊΔडୗ‫ڀݚ‬, ࡾඛॏ޻ͱͷ‫ڞ‬ಉ‫ڀݚ‬ͷͦΕͧΕͰ, ৽ͨͳ‫؍‬ଌ‫ܭ‬ըΛࡦఆͨ͠ɻ࣍೥౓Ҏ߱, ࣮ࡍʹ‫؍‬ଌΛߦͳ͍, औಘσʔλΛ༻͍ͯ‫ݕ‬ग़΍ղੳํ๏ͷ͞ΒͳΔվྑΛߦͳ͏ɻ޻ֶ‫ڀݚ‬ӃߤۭӉ஦޻ֶ෦໳ͷՖా‫ڭ‬त౳ͱͷ‫ڞ‬ಉ‫͋Ͱڀݚ‬Δɻ
ఱจֶͷࣾձɾֶߍ‫ڭ‬ҭ΁ͷ‫ࢁ( ༻׆‬Ԭ‫)ۉ‬ఱจֶΛৼ‫͠ڵ‬ɺՊֶ‫ڭ‬ҭΛ޿ΊΔͨΊʹ, ֤छ‫׆‬ಈΛ޿͘ߦͳ͍ͬͯ͘ɻࠓ೥౓͸, શࠃಉࣣ࣌༦ߨԋձ, ֤छߨԋձͳͲ਺ଟ͘ͷ࣮ફΛߦͳͬͨɻ2007 ೥౓͔Β։࠵͍ͯ͠ΔαΠΤϯ
εύϒΛ 4 ճ࣮ࢪͨ͠ɻ໊‫ݹ‬԰ࢢͰͷαΠΤϯεύϒʹίʔσΟωʔλͱͯ͠ࢀՃͨ͠ɻ͞ΒʹࡾୋࢢͰ͸, ೔ຊఱจֶձఱମൃ‫ݟ‬৆౳ͷड৆ऀΛғΉαΠΤϯεύϒΛ։࠵ͨ͠ɻʮϖΨεεఱମ‫؍‬ଌࣨʯΛ༻͍ͨߴ೥࣍‫ڭ‬ཆՊ໨ʮ๬ԕ‫ݟͰڸ‬ΔӉ஦‫ڥ؀‬ʯΛલ೥౓ʹҾ͖ଓ͍ͯ։ߨ
ͨ͠ɻࢁԬ͸ɺ೔ຊఱจֶձ‫ڭ‬ҭ୲౰ཧࣄʹՃ͑, શࠃಉࣣ࣌༦ߨԋձ࣮ߦҕһ, ೔ຊֶज़ձٞ
ʹ͓͚Δେֶ‫ڭ‬ҭͷ࣭อূʹ͔͔Δఱจֶ෼໺ͷ‫ج‬४ࡦఆҕһձ (ҕһ௕) ͳͲଟ༷ͳ໾ׂΛ୲͓ͬͯΓ, ࠓ‫ޙ‬΋ΑΓ‫׆ʹൃ׆‬ಈ͍ͯ͘͠ɻ
ϒϥοΫϗʔϧ߱ணԁ൫ͷ 3 ࣍‫ ݩ‬MHD ਺஋‫( ࢉܭ‬ொాਅඒ)࣭ྔ߱ணͷ‫ͳͱݯى‬Δ࣓‫ؾ‬ཚྲྀͷॳ‫࣓ظ‬৔ߏ଄ґଘੑʹؔͯ͠ௐ΂ΔͨΊʹ߱ணԁ൫શମΛ‫ܭ‬ࢉྖҬʹ‫ؚ‬Ή̏࣍‫ྲྀؾ࣓ݩ‬ମ਺஋࣮‫ݧ‬Λߦͬͨɻॳ‫࣓ظ‬৔ߏ଄ͱͯ͠ɺճసํ޲੒෼ͷΈΛ࣋ͭऑ͍ํҐ֯ํ޲࣓৔ΛԾఆͨ͠ωοτ࣓৔ͷ༗ΔϞσϧͱɺ੺ಓ໘ʹ൓ରশͳํҐ֯ํ޲࣓৔Λ༩͑ΔࣄͰ‫ܥ‬શମͷωοτ࣓৔͕ແ͍ϞσϧͱͰ‫ࢉܭ‬Λߦͬͨɻͦͷ݁Ռɺωοτ࣓৔ͷແ͍ϞσϧͰ͸ɺ༗ΔϞσϧΑΓ΋ɺ‫ॴہ‬తͳ֯ӡಈྔ༌ૹ཰ʹҧ͍͸ແ͍ࣄɺ͔࣭͠͠ྔ߱
ண཰͸൒෼ఔ౓ʹͳΔࣄ͕Θ͔ͬͨɻ͜ͷҧ͍͸ɺ‫ܥ‬ͷӔߏ଄ͷҧ͍ʹ‫ى‬Ҽ͓ͯ͠Γɺωοτ࣓৔ͷແ͍ϞσϧͰ͸খ͞ͳεέʔϧͷཚྲྀ͕୎ӽ͢Δࣄ͕Θ͔ͬͨɻ௒৽੕രൃʹ͓͚Δ෺࣭ࠞ߹ (খ໺উਉ)௒৽੕രൃͷিܸ೾͕੕ͷதΛ఻ൖ͢ΔաఔͰ, ௒৽੕രൃͷඇ‫ٿ‬ରশੑ, ͋Δ͍͸਌੕ͷඇ‫ٿ‬42ରশͳߏ଄ʹ‫ى‬Ҽ͢Δ෺࣭ࠞ߹ʹΑΓ, രൃͷ‫ݩ‬ૉ߹੒Ͱ࡞ΒΕΔ 56 Ni ͕‫ٿ‬ରশͰ༧૝͞ΕΔ
ΑΓང͔ʹ֎ଆ΁ӡ͹ΕͯΔ͜ͱ͕௒৽੕ 1987A ͷ‫؍‬ଌ͔Β஌ΒΕ͍ͯΔ. രൃͷඇ‫ٿ‬ରশੑͱ਌੕ͷখ͞ͳ༳Β͗Λߟྀͨ͠෺࣭ࠞ߹ͷ 2 ࣍‫਺ݩ‬஋࣮‫ݧ‬Λલ೥౓·Ͱʹߦ͍, Ϋϥϯϓঢ়ͷരൃ͕ॏཁͰ͋Δ͜ͱΛࣔͨ͠. ਌੕ͷരൃલͷߏ଄͸ཧ࿦తʹ͸ྑ͘෼͔͍ͬͯͳ͍͕, ରྲྀʹΑΓൺֱతେ͖ͳ༳Β͕͗ੜ͡ΔՄೳੑ͕ࢦఠ͞Ε͍ͯΔ. ຊ೥౓͸, ΑΓେ͖ͳ਌੕ͷඇ‫ٿ‬ରশੑʹண໨͠, ෺࣭ࠞ߹ͷ 2 ࣍‫ߴݩ‬ղ૾౓ྲྀମ‫ࢉܭ‬Λߦͬͨ. ͦͷ݁Ռ, ίώʔϨϯτ͔ͭ‫ʹ୺ۃ‬େ͖ͳৼ෯ͷઁಈΛՃ͑ͨϞσϧͰ‫؍‬ଌΛ࠶‫͢ݱ‬ΔՄೳੑ͕͋Δ͜ͱ͕෼͔ͬͨ. དྷ೥౓͸ߋʹৄࡉʹௐ΂, 2 ࣍‫ݟͰࢉܭݩ‬ΒΕΔ਺஋త໰୊Λղܾ͢ΔͨΊ, 3 ࣍‫ࢉܭݩ‬΋ߦ͏༧
ఆͰ͋Δ. ঘ, ຊ‫ڀݚ‬͸ JSPS ֎ࠃਓಛผ‫ڀݚ‬һ (ཧ‫ॴݚ‬ଐ) ͷ Mao ࢯͱͷ‫ڞ‬ಉ‫͋Ͱڀݚ‬Δ.
௒৽੕࢒֚ͷଟ࣍‫਺ݩ‬஋࣮‫( ݧ‬খ໺উਉ)௒৽੕࢒֚͸௒৽੕രൃͷিܸ೾͕੕ؒ෺࣭‫ͼٴ‬௒৽੕രൃ์ग़‫ݩ‬ૉΛஆΊΔ͜ͱͰి೾, X
ઢ, ΨϯϚઢͰً͘ఱମͰ͋Δ. ి࣓೾‫؍‬ଌͱཧ࿦Λಥ͖߹ΘͤΔ͜ͱʹΑΓ, ௒৽੕࢒֚ʹ͓
͚Δ์ࣹաఔ, Ӊ஦ઢͷཻࢠՃ଎, ௒৽੕രൃʹ͓͚Δ෺࣭ࠞ߹, ௒৽੕രൃϝΧχζϜ΁ࣔࠦΛ༩͑Δ͜ͱ͕‫ظ‬଴͞ΕΔ. ۙ೥ͷ௒৽੕࢒֚ Cas A ͷ‫؍‬ଌ͔Β, ֤‫ݩ‬ૉͷ෼෍͕‫ٿ‬ରশ͔Βஶͣ͘͠Ε͍ͯΔ͜ͱ͕෼͔ͬͨ. ଟ࣍‫ݩ‬ͷ௒৽੕࢒֚Ϟσϧʹ‫࣓ిͮ͘ج‬೾์ࣹͷཧ࿦తධՁ͕ඞཁͰ͋Δ. ͦ͜Ͱ, ۭؒ 3 ࣍‫ݩ‬ͷ௒৽੕࢒֚ϞσϧΛߏங͢ΔͨΊ, ଟ࣍‫ݩ‬ͷྲྀମ਺஋‫ܭ‬ࢉίʔυͷ։ൃʹऔΓ૊Μͩ. ֤์ग़‫ݩ‬ૉ͔ΒͷًઢΛධՁ͢ΔͨΊ, ॏཁͳҎԼͷ෺ཧաఔΛߴղ૾౓ྲྀମ‫ࢉܭ‬ίʔυ FLASH ʹ૊ΈࠐΜͩ. 1. ΤωϧΪʔํఔࣜʹ͓͚ΔిࢠͱΠΦϯͷ 2 ྲྀମͷऔΓѻ͍. 2. ֤‫ݩ‬ૉͷඇฏߧి཭౓‫ࢉܭ‬. 3. ిࢠͱΠΦϯͷΫʔϩϯিಥʹΑΔΤ
ωϧΪʔͷ؇࿨աఔ. ࠓ೥౓͸ۭؒ 1 ࣍‫ݩ‬, 2 ࣍‫Ͱݩ‬ίʔυͷଥ౰ੑΛઌߦ‫ͱڀݚ‬ൺֱ͠‫͠ূݕ‬ͨ. དྷ೥౓͸ 3 ࣍‫΁ݩ‬ͷ֦ு, ‫ݸ‬ʑͷ௒৽੕࢒֚΁ͷద༻Λ͠, ֤෺ཧաఔͷٞ࿦Λߦ͏.
௒৽੕രൃʹ͓͚Δ r-process ‫ݩ‬ૉ߹੒ (খ໺উਉɺ‫ڮ‬ຊਖ਼ষɺ෱ాྒྷฏ)தੑࢠั֫աఔ r-process ͷఱମαΠτ͸௕೥ͷಾͰ͕͋ͬͨɺ৽ͨͳ r-process αΠτͱͯ͠ɺcollapsar ͱ‫ݺ‬͹ΕΔ௒৽੕രൃϝΧχζϜΛఏҊ͢Δɻcollapsar ͷ߱ணԁ൫಺Ͱதੑࢠั͕֫
ਐΉͱ r-process ʹ༗རʹಇ͕͘ɺ࣮ࡍʹγϛϡϨʔγϣϯʹΑΓதੑࢠա৒ʹͳΔ͜ͱ͕֬ೝ͞Εͨɻࠓ‫ޙ‬ɺχϡʔτϦϊ༌ૹ΍࣓৔ͷޮՌɺ֩൓ԠΤωϧΪʔੜ੒ΛऔΓѻ͑ΔΑ͏ʹྲྀମίʔυΛվྑ͠ɺr-process ωοτϫʔΫ‫ࢉܭ‬Λߦ͍ͬͯ͘ɻൃද࿦จ ‫ݪ‬ஶ࿦จ • Cooling of Compact Stars with Color Superconducting Phase in Quark Hadron
Mixed Phase
T. Noda, M. Hashimoto, N. Yasutake, T. Maruyama, T. Tatsumi, M. Fujimoto
The Astrophysical Journal, 2013, Vol. 765, 1–5• R-Process Nucleosynthesis in MHD Jet Explosions of Core-Collapse Supernovae
Motoaki Saruwatari, Masa-aki Hashimoto, Ryohei Fukuda, and Shin-ichiro
Fujimoto
43

Journal of Astrophysics, Volume 2013(2013),Article ID 506146, 1–13,
http://dx.doi.org/10.1155/2013/506146• Constraint on Heavy Element Production in Inhomogeneous Big-Bang Nucleosynthesis from the Light Element Observations
Riou Nakamura, Masa-aki Hashimoto, Shin-ichiro Fujimoto, and KatsuhikoSato Journal of Astrophysics, Volume 2013 (2013), Article ID 587294, 1–9,
http://dx.doi.org/10.1155/2013/587294• Matter Mixing in Aspherical Core-collapse Supernovae: A Search for Possible Conditions for Conveying 5 6Ni into High Velocity Regions
M. Ono, S. Nagataki, H. Ito, S.-H. Lee, J. Mao, M. Hashimoto, A. Tolstov
The Astrophysical Journal, 2013, 773, 161–189, doi:10.1088/0004-637X/773/161• Numerical Experiments For Nuclear Flashes Toward Superbursts In An Accreting Neutron Star
M. Hashimoto, R.Kuromizu, M. Ono, T. Noda, M. Fujimoto
Journal of Astrophysics, in press• Orbit determination by genetic algorithm and application to GEO observation :Hideaki Hinagawa, Toshiya Hanada, Hitoshi Yamaoka,
ADVANCES IN SPACE RESEARCH, 53 (2014) pp. 532-542

Proceedings• ͦͷଞͷ࿦จ • : Dwarf Nova in Aquila = PNV J19150199+0719471 :K. Itagaki, T. Kojima, S. Nakano, Y. Sakurai, Y. Nakamura, H. Yamaoka, T.
Yusa, S. Dallaporta, U. Murani, P. Brlas, E. Waagen, F. Guenther, A. Oksanen,
J. Hambsch, P. Hallsten, L. Izzo, Toshihide Noguchi, R. Pickard, D. Blane, and
G. Poyner :Central Bureau Electronic Telegrams, No. 3554, 2013
• : Supernova 2013gn IN NGC 5557 = PSN J14182850+3630244 :K. Ayani, and H. Yamaoka :Central Bureau Electronic Telegrams, No. 3727, 201344• : Supernova 2013hg = PSN J12095569+2953513 :K. Ayani, and H. Yamaoka :Central Bureau Electronic Telegrams, No. 3753, 2013
• : Supernova 2013hu in NGC 3693 = PSN J11280786-1311336 :K. Ayani, and H. Yamaoka :Central Bureau Electronic Telegrams, No. 3776, 2014
• : Supernova 2014J in M82 = PSN J09554214+6940260 :S. J. Fossey, B. Cooke, G. Pollack, M. Wilde, T. Wright, M. Verstraaten, K.
Itagaki, H. Kaneda, H. Yamaoka, S. Kiyota, E. Guido, N. Howes, M. Nicolini,
L. Elenin, I. Molotov, J. Brimacombe, T. Noguchi, S. Nakano, G. Masi, and P.
Schmeer :Central Bureau Electronic Telegrams, No. 3792, 2014
• : Supernova 2014L in M99 = PSN J12184868+1424435 :T. Zhang, X. Wang, J. Mo, J. Chen, H. Yamaoka, K. Itagaki, S. Kiyota, E. Guido,
N. Howes, M. Nicolini, P. Bacci, R. Bacci, G. Masi, F. Nocentini, P. Schmeer, M.
Mancini, and M. Burali :Central Bureau Electronic Telegrams, No. 3795, 2014• ͳͥ௒৽੕ූ߸͕ͳ͍ͷʁ :ࢁԬ ‫ ۉ‬:ʮ੕φϏʯ2013 ೥ 6 ݄߸ (Vol. 14, No. 6), 51 – 51
• ʮ؆୯ͳ‫ͿֶͰࢉܭ‬ఱจֶʯͷεεϝ :ࢁԬ ‫ ۉ‬:NYAISAS ϝʔϧϚΨδϯ, No. 118 (2013)• ଜࢁઌੜͷࢥ͍ग़ :ࢁԬ ‫ ۉ‬:ʮఱจ݄ใʯ2013 ೥ 11 ݄߸ (Vol. 106, No. 11), 757 – 758• ϕςϧΪ΢ε͸͍ͭരൃ͢Δͷʁ :ࢁԬ ‫ ۉ‬:ʮ݄‫ͪ͏ץ‬Ύ͏ʯ2014 ೥ 1 ݄߸ (Vol. 30, No. 10), 4 – 9• ϓϥωλϦ΢Ϝ൪૊ۜՏమಓ 999 ੺͍੕ϕςϧΪ΢ε͍ͷͪͷً͖ʹ‫ݟ‬Δʮ੕ͷੜͱࢮʯ :ࢁԬ ‫ ۉ‬:ʮ੕φϏʯ2014 ೥ 3 ݄߸ (Vol. 15, No. 3), 26 – 31
• CCD ࣌୅Ͱ࠷΋͍ۙ Ia ‫ܕ‬௒৽੕ɹ M82 ͷ௒৽੕ 2014J :ࢁԬ ‫ ۉ‬:ʮ੕φϏʯ2014 ೥ 4 ݄߸ (Vol. 15, No. 4), 48 – 49
• ରஊʮੈքΛ஌Γ͍ͨɺӉ஦Λ఻͍͑ͨʯ— ఱจֶΛ௨ͯ͡‫఺ݪ‬Λߟ͑Δ — :ࢁԬ ‫ۉ‬, ߴ࠺ਅ࣍࿠ :ʮീࣄʯୈ 30 ߸, 36 – 5845ஶॻ• χϡʔτϯผ࡭ Ӊ஦ਤ ৽վగ ୈ̎൛ :খࡕɹ३, ੨໦ɹ࿨ޫ, ០ɹल඙, Ոɹਖ਼ଇ, ૔ຊɹ‫ܓ‬, খ‫ٱ‬อɹӳҰ࿠, খྛɹ‫ݑ‬ਖ਼,ۨ‫ٶ‬ɹ޾உ, ࠤʑ໦ɹথ, ਿࢁɹ௚, ాଜɹ‫ݩ‬ल, ‫ࢁ؍‬ɹਖ਼‫ݟ‬, ࢁԬɹ‫ۉ‬, ٢઒ɹਅ, ٢ాɹ௚‫ل‬, ౉෦ɹ५Ұ, ࢢိɹᕃᢛ, ઒ӽɹࢸࡩ, ย‫ۅ‬ɹ‫ڿ‬, ُ୩ɹ࿨‫ٱ‬,χϡʔτϯϓϨεɺ144 ทɺ2013 ೥ 9 ݄ 10 ೔.
• Newton Highlight 79ւ෦ɹએஉ, த઒ɹ‫و‬༤, ૆෕ߐɹٛ໌, ࢁԬɹ‫ۉ‬, ඌ࡚ɹ༸ೋ, Ԭଜɹఆۣ, ౉෦ɹ५Ұ, ੴࠇɹਖ਼ਓ
Newton Korea, 144 ท, 2014 ೥ 2 ݄ 10 ೔• ఱจֶ༂ਐͷ 400 ೥‫ྗڠ‬ɿࢁԬ ‫͔΄ۉ‬χϡʔτϯผ࡭, χϡʔτϯϓϨε, 160 ท, 2009 ೥ 5 ݄ 15 ೔ߨԋ ւ֎Ͱͷߨԋ • Thermal Evolution of Compact Stars with Color Superconducting Quark
Matter :T. Noda, N. Yasutake, M. Hashimoto, T. Maruyama, T. Tatsumi, M. Y.
Fujimoto
International Conference “The Structure and Signals of Neutron Stars, from
Birth to Death”, Florence, Italy, 2014 ೥ 3 ݄ 24 ೔-28 ೔ ࠃ಺Ͱͷߨԋ • Նͷ੕ۭͱӉ஦ਤ̎̌̍̏ : ࢁԬ‫ۉ‬શࠃಉࣣ࣌༦ߨԋձ 2013, ෱Ԭࢢผ෎ެຽ‫ؗ‬, 2013 ೥ 7 ݄ 7 ೔• Ӊ஦ͷҰੜΛҰຕͷϙελʔʹʂɹӉ஦ਤ̎̌̍̏ : ࢁԬ‫ۉ‬શࠃಉࣣ࣌༦ߨԋձ 2013, य़೔ࢢ੕ͷ‫ؗ‬, 2013 ೥ 7 ݄ 7 ೔• ੕ۭΛோΊΔͷ͕΋ͬͱָ͘͠ͳΔʂɹՆͷ໷ͷఱจֶߨ࠲ : ࢁԬ‫ۉ‬શࠃಉࣣ࣌༦ߨԋձ 2013, ΞϰΝϯςΟฤू෦ओ࠵, ఱਆύʔΫϏϧ (෱Ԭࢢதԝ۠), 2013 ೥ 7 ݄ 18 ೔46• ʮӉ஦Λ‫ޠ‬Δʯʂ ٞ࿦ͱ౼࿦ :઒ӽਗ਼Ҏ, ౦৓ॱ࣏, ࢁԬ‫ۉ‬, ฏࢁ‫׮‬, ٢Ԭਸ਼थ, ถᖒӳ඙, ‫ݹ‬Ӝ৽࢘
ୈ 12 ճαΠΤϯεΧϑΣˏ;͓͔͘, ෱ԬΞδΞϏδωεηϯλʔ (෱Ԭࢢதԝ۠), 2013 ೥ 7 ݄ 19 ೔

• Ұຕͷϙελʔʹ٧·ͬͨ࠷৽ͷӉ஦૾ : ࢁԬ‫ۉ‬શࠃಉࣣ࣌༦ߨԋձ 2013, େ໺৓ࢢ๺ίϛϡχςΟηϯλʔ, 2013 ೥ 7 ݄

20 ೔• ࣣ༦ͱՆͷ੕ۭͱଠཅͷ‫׆‬ಈͱӉ஦ਤ 2013 : ࢁԬ‫ۉ‬ఱจߨԋձ, ෱Ԭࢢதଜࡾཅߴߍ, 2013 ೥ 7 ݄ 27 ೔

• ϕςϧΪ΢ε͸ɺ·ͩ͋Δͷ͔ʁʢ੕ͷ࠷‫ظ‬Λߟ͑Δʣ :౔ࠤ੣, ࢁԬ‫ۉ‬, େ੢ߒ࣍੕ΧϑΣΈ΍͗࠲, ౦๺େֶ, 2013 ೥ 9 ݄ 9 ೔• খ࿭੕૞ࡧը૾ʹΑΔγϣοΫϒϨʔΫΞ΢τͷ୳ࡧ :ߴ໦߁ฏ, ࢁԬ‫ۉ‬, ࡔຊ‫ڧ‬೔ຊఱจֶձ 2013 ೥ळ‫ق‬೥ձ, ౦๺େֶ, 2013 ೥ 9 ݄ 10 ೔

• Kepler มޫ੕ͷ HR ਤʹ͓͚Δ෼෍ :ࡾદ‫ܛ‬ਓ, ࢁԬ‫ۉ‬2013 ೥౓ɹ࿈੕‫ܥ‬ɾมޫ੕ɾ௿Թ౓੕‫ڀݚ‬ձ, ‫۝‬भେֶ, 2013 ೥ 11 ݄ 25 ೔
• খ࿭੕૞ࡧը૾ʹΑΔγϣοΫϒϨʔΫΞ΢τͷ୳ࡧ :ߴ໦߁ฏ, ࢁԬ‫ۉ‬, ࡔຊ‫ڧ‬2013 ೥౓ɹ࿈੕‫ܥ‬ɾมޫ੕ɾ௿Թ౓੕‫ڀݚ‬ձ, ‫۝‬भେֶ, 2013 ೥ 11 ݄ 25 ೔• ౙͷ੕ۭΛཱྀ͠Α͏ʂ :ࢁԬ‫ۉ‬ίυϞ to αΠΤϯεΧϑΣ, ശ࡚ਫ଒‫( ؗ‬෱Ԭࢢ౦۠), 2014 ೥ 2 ݄ 11 ೔

• ᯁੴͷ࿩ :ࢁԬ‫ۉ‬ఱจߨԋձ, େ໺৓ࢢ๺ίϛϡχςΟηϯλʔ, 2014 ೥ 2 ݄ 15 ೔

• Discovery of an X-ray ﬂash from a nova explosion on MAXI J0158-744 andsearch for X-ray ﬂashes for other novae :Mikio Morii, Takehiro Mihara, Hitoshi Yamaoka, Jun Shimanoe, Hiroshi
47Tomida, Nobuyuki Kawai, Masaru Matsuoka, MAXI Team
Suzaku-MAXI 2014: Expanding the Frontiers of the X-ray Universe, Ehime
University (Matsuyama, Ehime, Japan), 2014 Feb. 20.
• ଠཅ‫ܥ‬Λͭ͘Ζ͏ʂ :ࢁԬ‫ۉ‬͜Ͳ΋ͬͱ͍͕ͩ͘, ΞΠϥϯυγςΟ(෱Ԭࢢ౦۠), 2014 ೥ 3 ݄ 1 ೔• ֤छࢿ੍֨౓ͱͷൺֱ :ࢁԬ‫ۉ‬ୈ̔ճɹ੕ۭҊ಺ਓʢ੕ͷιϜϦΤʣࢿ֨ೝఆ੍౓γϯϙδ΢Ϝ, ‫۝‬भେֶ,2014 ೥ 3 ݄ 9 ೔• ੕໺ଜ੕ͷιϜϦΤཆ੒ߨ࠲-ओ೚ߨࢣͱͯ͠ :ࢁԬ‫ۉ‬ୈ̔ճɹ੕ۭҊ಺ਓʢ੕ͷιϜϦΤʣࢿ֨ೝఆ੍౓γϯϙδ΢Ϝ, ‫۝‬भେֶ,2014 ೥ 3 ݄ 10 ೔• େֶ‫ڭ‬ҭʹ͓͚Δ൚ֶՊͷʮखΛಈ͔͢ఱจֶʯͷ࣮ફ :ࢁԬ‫ۉ‬೔ຊఱจֶձ 2014 ೥य़‫ق‬೥ձ, ࠃࡍ‫ج‬ಜ‫ڭ‬େֶ, 2014 ೥ 3 ݄ 19 ೔

• ‫۝‬भେֶϖΨεεϓϩδΣΫτʹΑΔӉ஦‫ڭ‬ҭͱͦͷ੒Ռ :౻‫ ݪ‬ஐࢠ, ླ໦ ӈจ, Ֆా ढ़໵, ࢁԬ ‫ۉ‬೔ຊఱจֶձ 2014 ೥य़‫ق‬೥ձ, ࠃࡍ‫ج‬ಜ‫ڭ‬େֶ, 2014 ೥ 3 ݄ 19 ೔

• Kepler Λ༻͍ͨ߃੕ͷޫ౓มಈͷ౷‫ܭ‬తௐࠪʹ޲͚ͯ :ࡾદ‫ܛ‬ਓ
ୈ 43 ճఱจఱମ෺ཧएखՆͷֶߍ, ‫ٶ‬৓ଂԦϩΠϠϧϗςϧ (‫ٶ‬৓‫܊ాמݝ‬ଂԦொ), 2013 ೥ 7 ݄ 29 ೔-8 ݄ 1 ೔• ߱ணԁ൫ͷάϩʔόϧ MHD γϛϡϨʔγϣϯ :ொాਅඒɺதଜ‫ݡ‬ਔɺদ‫྄࣏ݩ‬
ֶձ໊ɿSTE γϛϡϨʔγϣϯ‫ڀݚ‬ձɹˍɹଠཅ஍‫ٿ‬࿭੕‫ܥ‬ՊֶʢSTPʣγ
ϛϡϨʔγϣϯɾϞσϦϯάٕ๏ษ‫ڧ‬ձɹ߹ಉ‫ूڀݚ‬ձ - Ӊ஦ϓϥζϚɾେ‫ؾ‬ɾఱମ - 2013 ೥ 12 ݄ 24 ೔ʔ 2013 ೥ 12 ݄ 27 ೔

• ඇରশͳ௒৽੕രൃʹ͓͚Δ෺࣭ࠞ߹- 56 Ni ͕ߴ଎౓ྖҬ΁ӡ͹ΕΔ৚݅ͷ୳ࠪɿ

48খ໺উਉ, ௕୍ॏത, ҏ౻༟‫و‬, LEE, Shiu-Hang, MAO, Jirong, ‫ڮ‬ຊਖ਼ষ,

TOLSTOV, Alexeyୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ, ‫ཹٱ‬ถ޻‫ۀ‬େֶ, 2013 ೥ 11 ݄ 30 ೔• ଟ࣍‫ݩ‬ͷ௒৽੕രൃ͓Αͼ௒৽੕࢒֚Ϟσϧ, ॏ‫ݩ‬ૉͷ‫ݯى‬ɿখ໺উਉୈ̓ճϒϥοΫϗʔϧ࣓‫ݍؾ‬ษ‫ڧ‬ձ, ‫۽‬ຊେֶ, 2014 ೥ 3 ݄ 3 ೔-5 ೔• Eﬀct of triple-alpha reaction rates on the stellar evolution of massive stars :Yukihiro Kikuchi, M. Ono, Y. Matsuo, M. Hashimoto, S. Fujimoto
Supernovae and Gamma-Ray Bursts 2013, Conference on Supernovae, Yukawa
Institute for Theoretical Physics, Kyoto 2013 University, October 28 - November 1, 2013
• Triple-alpha ൓Ԡ཰ͷෆఆੑ͕େ࣭ྔ੕ͷਐԽͳΒͼʹ s-process ‫ݩ‬ૉ߹੒ʹ
༩͑ΔӨ‫ ڹ‬:٠஑೭޺, ‫ڮ‬ຊਖ਼ষ, খ໺উਉ, ౻ຊ৴Ұ࿠ୈ̍̍̕ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ, ‫ཹٱ‬ถ޻‫ۀ‬େֶ,2013 ೥ 11 ݄ 30 ೔ (౔)• ௒৽੕രൃʹ͓͚Δ෺࣭ࠞ߹ͷ੕प෺࣭ґଘੑ :দඌ߁लɺ‫ڮ‬ຊਖ਼ষɺখ໺উਉɺ௕ୌॏതɺ‫ݻ‬෢‫ܚ‬ɺࢁాষҰɺࢁԼ࿨೭
೔ຊఱจֶձ 2013 ೥ळ‫ق‬େձ, ౦๺େֶ, 2013 ೥ 9 ݄ 10 ೔–12 ೔• Dependence of the Mixing Between the Elements on Circumstellar Mediums
During Supernova Expansions :দඌ߁ल, ‫ڮ‬ຊਖ਼ষ, খ໺উਉ, ௕ୌॏത, ‫ݻ‬஛‫ܚ‬, ࢁాষҰ, ࢁԼ࿨೭Supernovae and Gamma-Ray Bursts 2013, ‫౎ژ‬େֶ, 2013 ೥ 10 ݄ 28 ೔–11
݄1೔• ੕प෺࣭෼෍͕௒৽੕࢒֚‫ܗ‬੒աఔͰͷ෺࣭ࠞ߹ʹ༩͑ΔӨ‫ ڹ‬:দඌ߁ल, ‫ڮ‬ຊਖ਼ষ, খ໺উਉ, ௕ୌॏത, ‫ݻ‬஛‫ܚ‬, ࢁాষҰ, ࢁԼ࿨೭ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ, ‫ཹٱ‬ถ޻‫ۀ‬େֶ, 2013 ೥ 11 ݄ 30 ೔

• Long Time Evolutionary Simulations in Supernova Included the Uncertainties of Circumstellar Medium and Stellar Envelop :দඌ߁ल, ‫ڮ‬ຊਖ਼ষ, খ໺উਉ, ௕ୌॏത, ‫ݻ‬஛‫ܚ‬, ࢁాষҰ, ࢁԼ࿨೭Multi-messengers from Core-Collapse Supernovae, ෱Ԭେֶ, 2013 ೥ 12 ݄ 2
೔-6 ೔

49

• Cooling of compact stars with color superconductivity :໺ాৗ༤, ‫ڮ‬ຊਖ਼ষ, ҆෢৳ढ़, ‫ࢁؙ‬හ‫ؽ‬, ୥හོ, ౻ຊਖ਼ߦ‫౎ژ‬େֶ‫֩ࢠݪ‬άϧʔϓओ࠵‫ڀݚ‬ձʮKyoto Meeting 2013Sʯ, ‫౎ژ‬େֶ, 2013
೥ 6 ݄ 8 ೔-9 ೔• ϋΠϒϦου੕ʹ͓͚ΔΧϥʔ௒఻ಋͱ֩ࢠͷ௒ྲྀಈͷྫྷ٫ʹର͢ΔӨ‫ڹ‬:໺ాৗ༤, ‫ڮ‬ຊਖ਼ষ, ҆෢৳ढ़, ‫ࢁؙ‬හ‫ؽ‬, ୥හོ, ౻ຊਖ਼ߦ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ୈ 119 ճࢧ෦ྫձ, ‫ཹٱ‬ถ޻‫ۀ‬େֶ, 2013 ೥ 11 ݄ 30 ೔

• Cooling of the compact star in Cassiopeia A:
໺ాৗ༤, ‫ڮ‬ຊਖ਼ষ, ҆෢৳ढ़, ‫ࢁؙ‬හ‫ؽ‬, ୥හོ, ౻ຊਖ਼ߦ‫౎ژ‬େֶ‫֩ࢠݪ‬άϧʔϓओ࠵‫ڀݚ‬ձʮKyoto Meeting 2013Wʯ, ‫౎ژ‬େֶ,2013 ೥ 12 ݄ 21 ೔-22 ೔• Χϥʔ௒఻ಋঢ়ଶͷΫΥʔΫ෺࣭͕தੑࢠ੕ͷྫྷ٫ʹ‫͢΅ٴ‬Ө‫ڹ‬:໺ాৗ༤, ‫ڮ‬ຊਖ਼ষ, ҆෢৳ढ़, ‫ࢁؙ‬හ‫ؽ‬, ୥හོ, ౻ຊਖ਼ߦՊ‫ݚ‬අ৽ֶज़ྖҬʮ࣮‫؍ͱݧ‬ଌͰղ͖໌͔͢தੑࢠ੕ͷ֩෺࣭ʯ தੑࢠ੕֩෺࣭‫ڀݚ‬ձ, ཧԽֶ‫( ॴڀݚ‬࿨ޫࢢ), 2013 ೥ 12 ݄ 27 ೔-28 ೔• Thorne-Zytkow ఱମ‫ܗ‬੒࣌ͷதੑࢠ੕ʹ‫ڊ‬੕૬‫༻࡞ޓ‬:᳃໺ॏ೭, ໺ా ৗ༤, େ௬͔͓Γ, খ໺উਉ೔ຊఱจֶձ 2014 ೥य़‫ق‬೥ձಛผηογϣϯ, ࠃࡍ‫ج‬ಜ‫ڭ‬େֶ, 2014 ೥ 3 ݄

19 ೔-22 ೔• Ϗοάόϯ‫ݩ‬ૉ߹੒ʹ͓͚Δ 4He ͷ૊੒ൺɿҰ੓ྒྷଠ࿠ɼதଜཧԝɼ‫ڮ‬ຊਖ਼ষɼߥҪ‫ࡾݡ‬ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձɼ‫ཹٱ‬ถ޻‫ۀ‬େֶɼ2013 ೥ 11 ݄

• ֩൓Ԡ཰ͷϏοάόϯ‫ݩ‬ૉ߹੒΁‫͢΅ٴ‬Ө‫ڹ‬:Ұ੓ྒྷଠ࿠ɼதଜཧԝɼ‫ڮ‬ຊਖ਼ষɼߥҪ‫ࡾݡ‬
ୈ 26 ճཧ࿦࠙γϯϙδ΢Ϝɼ౦‫ژ‬େֶ, 2013 ೥ 12 ݄

• Ϗοάόϯ‫ݩ‬ૉ߹੒͔ΒͷχϡʔτϦϊͷॖୀύϥϝʔλʹର͢Δ੍‫ݶ‬ɿҰ੓ྒྷଠ࿠ɼதଜཧԝɼ‫ڮ‬ຊਖ਼ষɼߥҪ‫ࡾݡ‬೔ຊఱจֶձ 2014 ೥य़‫ق‬೥ձɼࠃࡍ‫ج‬ಜ‫ڭ‬େֶɼ2014 ೥ 3 ݄• Cassiopeia A தੑࢠ੕ͷ೤ਐԽͷϞσϧԽ :ྛాߊଠ࿕, ໺ాৗ༤, ‫ڮ‬ຊਖ਼ষ, ౻ຊਖ਼ߦ೔ຊఱจֶձ 2013 ळ‫ق‬೥ձ, ౦๺େֶ, 2013 ೥ 9 ݄ 10 ೔-12 ೔

50• R-processs Nucleosynthesis In Supernova Explosions :R. Fukuda, M. Saruwatari, M, Hashimoto, S. Fujimoto
Muti-Messengers from Core-Collapse Supernovae, ෱Ԭେֶ, 2013 ೥ 12 ݄
2-6 ೔
• ௒৽੕ r-process ͱ ﬁssion :෱ాྒྷฏ, ‫ڮ‬ຊਖ਼ষ, খ໺উਉ෺ཧֶձ‫۝‬भࢧ෦ྫձ, ‫ཹٱ‬ถ޻‫ۀ‬େֶ, 2013 ೥ 11 ݄ 30 ೔֎෦ࢿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ 
1. ‫ج‬൫‫( ڀݚ‬C) ɹʮτϦϓϧЋఱମ֩൓Ԡ཰΁ͷӉ஦෺ཧֶ͔Βͷ੍‫ݶ‬ʯɹʢH24–H26ʣ
‫ڀݚ‬୅දऀ:ɹ‫ڮ‬ຊਖ਼ষ
2. एख‫( ڀݚ‬B)
ʮۜՏΨεԁ൫ͷ࣓‫ྲྀؾ‬ମ਺஋࣮‫ݧ‬ɿ࣓‫্ුؾ‬ϧʔϓɾӔঢ়࿹িܸ೾ʹΑΔཻࢠՃ଎ͷ‫د‬༩ʯ (H23–H26)‫ڀݚ‬୅දऀɿொాɹਅඒ
3. ‫ج‬൫‫( ڀݚ‬B)
ʮ࣓‫ྲྀؾ‬ମ਺஋࣮‫ ͱݧ‬X ઍ‫؍‬ଌͷ࿈‫ʹܞ‬ΑΔϒϥοΫϗʔϧީิఱମͷঢ়ଶભҠͷղ໌ʯɹ (H23 –H 25)‫ڀݚ‬෼୲ऀɿொాɹਅඒ จ෦লՊֶ‫ڀݚ‬අิॿۚҎ֎ͷ֎෦ࢿۚ ଞେֶͰͷ‫ڭͱڀݚ‬ҭ٠஑೭޺: ‫۝‬भ࢈‫ۀ‬େֶ‫ڭૅج‬ҭαϙʔτηϯλʔʹඇৗ‫ۈͯ͠ͱࢣڭۈ‬຿͠, ෺ཧɾ਺ֶͷ‫ݸ‬ผࢦಋΛߦͬͨɻ
໺ాৗ༤: ‫ཹٱ‬ถ޻‫ߴۀ‬౳ઐ໳ֶߍͰʮԠ༻෺ཧ IIʯʮ෺ཧʯͷߨٛΛߦͬͨɻ໺ాৗ༤: ‫ཹٱ‬ถ޻‫ۀ‬େֶ޻ֶ෦ʹ͓͍ͯʮ෺ཧֶ I ʯʮ෺ཧֶ࣮‫ݧ‬ʯͷߨٛΛߦͬͨɻࢁԬ‫ۉ‬ɿதଜֶԂେֶʹͯʮ஍ֶʯͷߨٛΛߦͬͨɻߴ໦߁ฏɿ‫۝‬भ࢈‫ۀ‬େֶ‫ڭૅج‬ҭαϙʔτηϯλʔʹඇৗ‫ۈͯ͠ͱࢣڭۈ‬຿͠, ෺ཧɾ਺ֶͷ‫ݸ‬ผࢦಋΛߦͬͨɻֶ෦̐೥ੜଔ‫ڀݚۀ‬51‫ेޒ‬ཛྷ ॣଠ (ࢦಋ‫ڭ‬һɼ‫ڮ‬ຊਖ਼ষ)ɿॏྗ่յ‫ܕ‬௒৽੕രൃʹ͓͚Δ Ni ͷੜ੒ྔͱ๲
ு଎౓২໦༤࠸ (ࢦಋ‫ڭ‬һɼ‫ڮ‬ຊਖ਼ষ)ɿr-process ʹ͓͚Δॏ‫ݩ‬ૉ߹੒ͱ ﬁssion ͷӨ‫ڹ‬Ӊࠜྒྷฏ (ࢦಋ‫ڭ‬һɼ‫ڮ‬ຊਖ਼ষɼࢁԬ‫)ۉ‬ɿඒ੕εϖʔεΨʔυηϯλʔը૾Λ༻͍ͨ௒৽੕ͷଌޫ
Ӭ໺ཾଠ࿠ (ࢦಋ‫ڭ‬һɼ‫ڮ‬ຊਖ਼ষɼࢁԬ‫)ۉ‬ɿඒ੕ηϯλʔ‫؍‬ଌը૾ʹΑΔ௒৽੕ͷޫ౓‫ۂ‬ઢͷ࡞੒म࢜࿦จҰ੓ྒྷଠ࿠ (ࢦಋ‫ڭ‬һɼ‫ڮ‬ຊਖ਼ষ)ɿ৽͍͠ఱମ֩൓Ԡ཰ͱӉ஦ॳ‫ݩظ‬ૉ߹੒ߴ໦߁ฏ (ࢦಋ‫ڭ‬һɼ‫ڮ‬ຊਖ਼ষɼࢁԬ‫)ۉ‬ɿখ࿭੕୳ࠪը૾Λ༻͍ͨ௒৽੕ Shock Breakout
୳ࡧ

ത࢜࿦จ

ֶ֎Ͱͷֶձ‫׆‬ಈࢁԬ‫ۉ‬ɿ೔ຊఱจֶձཧࣄ, ‫ڭ‬ҭҕһձҕһ௕, δϡχΞηογϣϯ࣮ߦҕһձҕһ,

IAU Commission 6 President, ಉ Division B DSC,
2013 ೥࿈੕‫ܥ‬ɾมޫ੕ɾ௿Թ౓੕‫ڀݚ‬ձੈ࿩ਓ୅ද
೔ຊֶज़ձٞ෺ཧֶҕһձ IAU ෼ՊձʹΦϒβʔόʔࢀՃडୗ‫ڀݚ‬ɾຽؒͱͷ‫ڞ‬ಉ‫ڀݚ‬ࢁԬ‫ۉ‬ɿ‫ࣜג‬ձࣾ IHI ͔Βͷडୗ‫ڀݚ‬ʮະ஌εϖʔεσϒϦͷޮ཰తͳ୳ࡧํ๏ͷ‫ݚ‬‫ڀ‬ʯ(୅දऀɿՖాढ़໵ (޻ֶ‫ڀݚ‬Ӄ)) ʹ෼୲ऀͱͯ͠ࢀՃࢁԬ‫ۉ‬ɿ‫ࣜג‬ձࣾࡾඛॏ޻ͱ
ͷ‫ڞ‬ಉ‫ڀݚ‬ʮεϖʔεσϒϦʹؔ͢Δ‫ڞ‬ಉ‫ڀݚ‬ʯ(୅දऀɿՖాढ़໵ (޻ֶ‫ڀݚ‬Ӄ)) ʹ෼୲ऀͱͯ͠ࢀՃ
ͦͷଞͷ‫׆‬ಈͱ੒Ռ• ‫۝‬େɾ‫۽‬େ߹ಉηϛφʔɿ‫۝‬भ஍۠‫۝‬ॏ‫ڞ‬ಉ‫ݚ‬मॴʹ͓͍ͯɺେֶӃੜओ࠵ͷ‫ڀݚ‬ൃදձΛߦͬͨɻ2013 ೥ 9 ݄ 4 ೔-9 ݄ 7 ೔• ࢁԬ‫ۉ‬ɿ‫۝‬भେֶࠃࡍӉ஦ఱ‫ؾ‬Պֶɾ‫ڭ‬ҭηϯλʔ஦ۭࡂ֐༧ଌ‫ڀݚ‬෦໳ʹซ೚

52

• 2013 ೥ 6 ݄ʹେࡕࢢཱՊֶ‫Ͱؗ‬։࠵͞Εͨʮఱจֶֶ͕΂Δେֶ߹ಉઆ໌ձʯʹࢀՃɺ‫۝‬भେֶʹ͓͚Δఱจֶ‫ڭ‬ҭʹ͍ͭͯઆ໌ͨ͠ (ࢁԬ)ɻ
• 2013 ೥݄ʹࠤլ‫ཱݝ‬Ӊ஦Պֶ‫Ͱؗ‬ʮӉ஦Λֶ΂Δେֶ߹ಉઆ໌ձ in ‫۝‬भʯΛ࣮ߦҕһ௕ͱͯ͠ӡӦͨ͠ (ࢁԬ)ɻ
• ෱Ԭࢢ಺ʹͯαΠΤϯεύϒΛ 4 ճʢ2013 ೥ 6 ݄, 10 ݄, 12 ݄, 14 ೥ 3 ݄ʣ։࠵͠
ͨʢ࣮ࢪҕһɿࢁԬʣɻ໊‫ݹ‬԰ࢢͰαΠΤϯεύϒΛ։࠵ͨ͠ (ࢁԬ)ɻ• ͦͷଞςϨϏɾϥδΦɾWebɾ஍Ҭͷఱจ୆౳ͰఱจֶղઆΛߦͳͬͨ (ࢁԬ)ɻ• ‫ཱݝ࡚ٶ‬ԆԬߴߍͰग़લत‫ۀ‬Λߦͳͬͨ (2013 ೥ 10 ݄)ɻ

53ૉཻࢠ࣮‫ࣨڀݚݧ‬‫ߏࣨڀݚ‬੒һ઒ӽ ਗ਼Ҏ ‫ڭ‬त٢Ԭ ਸ਼थʢRCAPPʣ ।‫ڭ‬त౦৓ ॱ࣏ ।‫ڭ‬त৫ా ‫ڭॿ ק‬Ի໺ ӯढ़ʢRCAPPʣ ॿ‫ڭ‬຤‫ ݪ‬େ‫ڭॿ װ‬ ത࢜‫ڀݚ‬һ ਢ౻ ༟࢘ʢֶज़‫ڀݚ‬һʣҪ্ ‫ࡾݚ‬ʢಛ೚‫ڭ‬तʣߐ࡚ ఩࿠ʢಛ೚‫ڭ‬तʣɹɹࢁ‫ ޱ‬ത࢙ʢֶज़‫ڀݚ‬һʣ େֶӃ म࢜՝ఔ ্໺ ᠳ‫ݹ‬Ӝ ৽࢘େੴ ߤௐ ᠳฏদຊ ‫ޛ‬‫ ࡚ٶ‬ཅฏాத ‫ؾݩ‬

෋ా ཾ඙

ాத ૱Ұ

த‫ ډ‬༐थ ֶ෦ ଔ‫ڀݚۀ‬ੜ ֯ ௚޾ॅా ‫׮‬थ

ߴా लࠤ

௕ᖒ ཌྷ

௕ౡ ‫׮‬੐ฏҪ ‫׮‬ਓ୲౰त‫ۀ‬• ઒ӽശ࡚஍۠ɿίΞηϛφʔʢલ‫ظ‬ʣɺ෺ཧֶθϛφʔϧʢ‫ظޙ‬ʣҏ౎஍۠ɿ෺ཧֶ IIIʢલ‫ظ‬ɾ‫ظޙ‬ʣɺྗֶ‫ૅج‬ɾԋशʢલ‫ظ‬ʣ• ౦৓ശ࡚஍۠ɿૉཻࢠ෺ཧֶʢ‫ظޙ‬ʣҏ౎஍۠ɿྗֶ‫ૅج‬ɾԋशʢલ‫ظ‬ʣ• ٢Ԭശ࡚஍۠ɿ‫֩ࢠݪ‬ɾߴΤωϧΪʔ࣮‫ֶݧ‬ʢ‫ظޙ‬ʣҏ౎஍۠ɿࣗવՊֶ૯߹࣮‫ݧ‬ʢલ‫ظ‬ʣ• ৫ాശ࡚஍۠ɿ‫ૅج‬෺ཧ࣮‫ֶݧ‬ɾಉ࣮‫ݧ‬ʢ‫ظޙ‬ʣ54• ຤‫ݪ‬ҏ౎஍۠ɿࣗવՊֶ૯߹࣮‫ݧ‬ʢ‫ظޙ‬ʣ‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ

CERN-LHC ʹ͓͚Δ ATLAS ࣮‫( ݧ‬઒ӽ ਗ਼Ҏɺ౦৓ ॱ࣏ɺ৫ా ‫ק‬ɺԻ໺ ӯढ़)εΠεɾδϡωʔϒ߫֎ʹ͋ΔԤभ߹ಉ‫( ߏػڀݚ֩ࢠݪ‬CERN) ͷେ‫ܕ‬ϋυϩϯিಥ‫ܕ‬Ճ଎‫( ث‬LHC) ʹ͓͍ͯɺࠃࡍ‫ڞ‬ಉ‫ ڀݚ‬ATLAS ࣮‫ݧ‬Λਪਐ͍ͯ͠ΔɻLHC Ճ଎‫ث‬͸

2013 ೥ 1 ݄ʹӡసΛҰ୴ఀࢭ͠ɺॏ৺‫ܥ‬ΤωϧΪʔΛઃ‫ܭ‬஋Ͱ͋Δ 13 – 14 TeV ΁૿‫͢ڧ‬ΔͨΊɺՃ଎‫ث‬վमͷ௕‫ظ‬γϟοτμ΢ϯʹೖͬͨɻࠓ೥౓͸ɺγϦίϯ൒ಋମඈ੻‫ݕ‬ग़‫ث‬ͷӡసɾҡ࣋ɾվྑɺϘτϜδΣοτಉఆΞϧΰϦζϜͷ։ൃɺώοάεཻࢠͷੑ࣭ͷ‫ڀݚ‬ɺ‫ݕ‬ग़‫ث‬ΞοϓάϨʔυ‫ܭ‬ըͷࡦఆΛਐΊͨɻ• γϦίϯ൒ಋମඈ੻‫ݕ‬ग़‫ث‬ͷӡసɾҡ࣋ɾվྑ (઒ӽ ਗ਼Ҏɺ౦৓ ॱ࣏ɺ৫ా
‫ק‬ɺԻ໺ ӯढ़)ϏʔϜিಥ఺͔Βൃੜ͢Δଟ਺ͷՙిཻࢠͷ‫ݕ‬ग़Ͱ͸ɺATLAS ‫ݕ‬ग़‫಺࠷ث‬૚ʹ഑ஔͨ͠಺෦ඈ੻‫ݕ‬ग़‫͕ث‬ॏཁͳ໾ׂΛՌͨ͢ɻ಺෦ඈ੻‫ݕ‬ग़‫ث‬ͷ͏ͪɺզʑͷάϧʔϓ͸γϦίϯ൒ಋମඈ੻‫ݕ‬ग़‫( ث‬SemiConductor Tracker :SCT) ͷӡసʹਫ਼ྗతʹऔΓ૊Έɺ‫׆‬ಈΛ౷‫ׅ͢‬Δ Calibration Coordinator(౦৓)ɺData Quality Coordinator (Ի໺) Λ୲͖ͬͯͨɻSCT ‫ݕ‬ग़‫ث‬ͷӡసʹࢀՃ͢Δࠃ಺‫ؔػڀݚ‬ͷ͏ͪɺ‫۝‬भେֶ͸ CERN ʹελοϑ͕ৗற͍ͯ͠
ΔͨΊɺେֶؒͰ࿈‫ڀݚͯ͠ܞ‬ΛਐΊΔ͏͑Ͱத৺త໾ׂΛ୲͍ͬͯΔɻ‫ݕ‬ग़‫ث‬ͷӡసͰ͸ɺ‫ڍ‬ಈͷมԽΛஞ࣍తʹσʔλϕʔεʹ൓өͤ͞ɺԁ‫ͳ׈‬িಥࣄ৅ͷ࠶ߏ੒Λ࣮‫ͨ͠ݱ‬ɻ‫ݕ‬ग़‫ث‬શମͷ 99 %Ҏ্Λਖ਼ৗʹಈ࡞ͤ͞ɺऔಘ
σʔλͷ 99 %Ҏ্Λ෺ཧղੳʹ༻͍Δ͜ͱΛՄೳʹ͍ͯ͠Δɻ·ͨɺLHCՃ଎‫࠶͕ث‬Քಇ͢Δ 2015 ೥Ҏ߱͸ɺॏ৺‫ܥ‬ΤωϧΪʔΛ૿‫͠ڧ‬ɺॠؒϧϛϊγςΟ΋޲্ͤ͞ΔͨΊɺσʔλऩूγεςϜʹ͔͔ΔෛՙΛ෼ࢄ͢Δඞཁ
͕͋Δɻ͜Ε·Ͱͱಉఔ౓ͷߴ͍ޮ཰ͰσʔλΛऩू͢ΔͨΊͷಡΈग़͠ճ࿏਺ΛධՁ͠ɺ௕‫ظ‬γϟοτμ΢ϯதͷγεςϜվྑํ਑Λܾఆͨ͠ɻ͞Βʹɺ2015 ೥Ҏ߱ʹऔಘ͢ΔσʔλΛ෺ཧղੳʹ༻͍ΔͨΊͷ൑ఆ‫ج‬४ʹ͍ͭͯɺӡ༻४උΛਐΊ͍ͯΔɻಛʹɺ಺෦ඈ੻‫ݕ‬ग़‫ث‬ͷ Pixel ‫ݕ‬ग़‫ ͱث‬TRT‫ݕ‬ग़‫ث‬ͷ৘ใΛ૊Έ߹ΘͤΔ͜ͱʹΑΓૣ‫ʹظ‬ҟৗΛ‫ݕ‬஌͠ɺӡసʹϑΟʔυόοΫΛ͔͚Δ͜ͱΛ໨ࢦ͍ͯ͠Δɻ• ϘτϜδΣοτಉఆΞϧΰϦζϜͷ։ൃ (઒ӽ ਗ਼Ҏɺ౦৓ ॱ࣏ɺԻ໺ ӯढ़)ώοάεཻࢠͷϘτϜΫΥʔΫର΁่յΛ͸͡ΊɺϘτϜΫΥʔ ΫΛ‫ݯى‬55

ͱ͢ΔδΣοτ (b-jet) Λऴঢ়ଶʹ࣋ͭॏཁͳ෺ཧաఔ͕ଟ͘ଘࡏ͢ΔͨΊɺ

b-jet ͷಉఆ͸ ATLAS ࣮‫Ͱݧ‬ॏཁͳ໾ׂΛՌͨ͢ɻb-jet Λଞͷ͍ܰΫΥʔΫΛ‫͢ͱݯى‬ΔδΣοτͱ۠ผ͢Δख๏͕ɺb-tagging Ͱ͋ΔɻATLAS ࣮‫Ͱݧ‬ඪ४ͱ͢Δ b-tagging ͸ MV1 ͱ‫ݺ‬͹Εɺb-jet ʹର͢Δ‫ݕ‬ग़ޮ཰͕ 70 %ͷ৔߹ɺ͍ܰΫΥʔΫΛ‫͢ͱݯى‬Δ jet Λ 1/100 ʹআ‫͢ڈ‬Δ͜ͱ͕Ͱ͖ΔɻMV1͸ɺෳ਺ͷ b-tagging ΞϧΰϦζϜΛ neural network Λ༻͍ͯ߹੒ͨ͠΋ͷͰ͋Γɺͦͷ͏ͪ࠷΋‫د‬༩͕େ͖͍ JetFitter ʹ͍ͭͯৄࡉͳ‫ڀݚ‬Λߦͬͨɻ

JetFitter ͸ɺδΣοτͷํ޲ΛԾ૝తʹཻࢠͷ‫͑ߟͱ੻ي‬Δ͜ͱʹΑͬͯɺෳ਺ͷೋ่࣍յ఺Λޮ཰తʹ࠶ߏ੒͢ΔΞϧΰϦζϜͰ͋ΔɻJetFitter Λγ
ϛϡϨʔγϣϯαϯϓϧʹద༻ͯ͠ਅͷ่յաఔͱൺֱ͠ɺۙ઀͢ΔҟͳΔ
ཻࢠ͕ಉҰͷཻࢠͱͯ͠‫ߏ࠶ͯͬޡ‬੒͞Εͯ͠·͏ࣄ৅ (fake) ͕ߴ͍ӡಈྔྖҬͰ༏੎ʹͳΔ͜ͱΛఆྔతʹࣔͨ͠ɻLHC Ճ଎‫࠶͕ث‬Քಇ͢Δ 2015 ೥Ҏ߱ͷ࣮‫Ͱݧ‬͸ɺ͜ͷ fake ࣄ৅Λ཈੍ͭͭ͠ߴ͍ b-tagging ޮ཰Λҡ࣋͢Δ͜ͱ͕՝୊Ͱ͋Δɻ• ώοάεཻࢠͷੑ࣭ͷ‫ڀݚ‬ʢ৫ా ‫ק‬ʣ
2012 ೥ 7 ݄ʹ ATLAS ࣮‫ ͱݧ‬CMS ࣮‫͕ݧ‬ඪ४໛‫ܕ‬ώοάεཻࢠͷ୳ࡧʹ͓͍ͯ৽ཻࢠΛൃ‫ͨ͠ݟ‬ɻզʑͷάϧʔϓ͸ɺഎ‫ࣄܠ‬৅͕গͳ͘ɺ৴߸༗ҙ౓ͷߴ่͍յϞʔυͱͯ͠ɺώοάεཻࢠ͕ Z ཻࢠରʹ่յ͠ɺ֤ Z ཻࢠ͕Ϩϓτϯ (ిࢠ·ͨ͸ϛϡʔΦϯ) ରʹ่յ͢Δɺ4 Ϩϓτϯνϟϯωϧͷ‫ڀݚ‬ʹ஫ྗ͖ͯͨ͠ɻಛʹɺղੳ༻σʔλͷੜ੒ͱ‫ܥ‬౷‫ࠩޡ‬ͷධՁΛ୲౰ͨ͠ɻ
৽ཻࢠ͕ώοάεཻࢠͱҰக͢Δ͔൱͔Λܾఆ͢ΔͨΊɺ৽ཻࢠͷଞཻࢠͱͷ݁߹ͱεϐϯɾύϦςΟΛ‫ͨ͠ڀݚ‬ɻ݁߹ͷେ͖͞ʹΑΓɺੜ੒அ໘ੵ΍่յ෼‫ذ‬ൺ͕มԽ͢Δɻऴঢ়ଶͷ෇ՃతͳδΣοτ΍Ϩϓτϯͷ༗ແΛௐ΂
Δ͜ͱͰɺੜ੒աఔͷ৘ใΛऔΓग़ͤΔɻ͜Ε·Ͱʹऔಘͨ͠σʔλΛ༻͍ͯಘͨήʔδϘιϯͱϑΣϧϛΦϯʹର͢Δ݁߹ͷ஋͸ɺඪ४໛‫ܕ‬ώοάεཻࢠͷ৔߹ʹ‫ظ‬଴͞ΕΔ஋ͱ౷‫͓ࠩޡܭ‬Αͼ‫ܥ‬౷‫ࠩޡ‬ͷൣғ಺ͰҰகͨ͠ɻεϐϯ (J) ͱύϦςΟ(P ) Λ 4 ͭͷϨϓτϯͷ֯౓෼෍΍Ϩϓτϯରͷෆม࣭ྔ෼෍͔Βܾఆͯ͠ɺඪ४໛‫ܕ‬ώοάεཻࢠͱಉ͡ J P = 0+ Ͱ͋Δͱ͍͏݁ՌΛ 10 ݄ʹֶज़࿦จͱͯ͠ग़൛ͨ͠ɻಉ݄ɺBrout-Englert-Higgs (BEH)‫ߏػ‬Λఏএͨ͠ F. Englert ͱ P.W. Higgs ʹϊʔϕϧ෺ཧֶ৆͕त༩͞Εɺ

BEH ‫͕ߏػ‬༧ଌ͢ΔώοάεཻࢠΛ ATLAS ࣮‫ ͱݧ‬CMS ࣮‫ͨ͜͠ݟൃ͕ݧ‬ͱ͕ड৆ཧ༝ʹ໌‫͞ه‬Εͨɻࠓ೥౓ͷ‫ޙ‬൒Ͱ͸ɺ‫ݕ‬ग़‫ث‬ͷֱਖ਼ͷվળɾγϛϡϨʔγϣϯαϯϓϧͷ࠶ੜ੒ɾղੳख๏ͷվྑʹΑΓɺ‫ܥ‬౷‫ࠩޡ‬Λେ෯ʹ௿‫ͨͤ͞ݮ‬ɻ2014 ೥౓લ൒ʹ͸࠷ऴ݁ՌΛ࿦จͱͯ͠ެද͢Δ༧ఆͰ͋Δɻ56

• ‫ݕ‬ग़‫ث‬ΞοϓάϨʔυ‫ܭ‬ը (઒ӽ ਗ਼Ҏɺ౦৓ ॱ࣏ɺ৫ా ‫ק‬ɺԻ໺ ӯढ़)‫ߦݱ‬ͷ LHC Ճ଎‫ث‬͸ 2022 ೥·Ͱӡసͨ͠‫ޙ‬ɺՃ଎‫ث‬վྑʹΑΓॠؒϧϛϊγςΟΛ 5 × 1034 cm−2 s−1 ʹ૿‫͠ڧ‬ɺ2025 ೥͔ΒߴϧϛϊγςΟLHC (HL-

LHC) ͱͯ͠࠶Քಇͤ͞ɺΤωϧΪʔϑϩϯςΟΞ෺ཧΛ͞Βʹਪਐ͢Δ‫ܭ‬ըͰ͋Δɻͦͷ‫ܭ‬ըʹରԠ͠ɺATLAS ࣮‫Ͱݧ‬͸‫ݕ‬ग़‫ث‬ΛΞοϓάϨʔυ͢
Δ‫ܭ‬ըΛਐΊ͍ͯΔɻಛʹେ‫ن‬໛ͳ‫ܭ‬ըͱͯ͠ɺ಺෦ඈ੻‫ݕ‬ग़‫ث‬શମΛ৽‫ܕ‬ͷ଱์ࣹઢγϦίϯ‫ݕ‬ग़‫ߏͰث‬੒͢Δɻզʑͷάϧʔϓ͸ɺγϦίϯ‫ݕ‬ग़‫ث‬ΞοϓάϨʔυ‫ܭ‬ըʹࢀը͢ΔͨΊɺϐΫηϧɾετϦοϓ‫ݕܕ‬ग़‫ث‬ͷ։ൃʹඞਢͰ͋Δ൒ಋମ࣮૷ͱੑೳධՁΛՄೳͱ͢Δʮ࣍ੈ୅γϦίϯ൒ಋମ‫ݕ‬ग़‫ث‬։ൃγεςϜʯͷಋೖΛ‫ݕ‬౼͖ͯͨ͠ɻγεςϜ͸ɺࠃࡍϦχΞίϥΠ
μʔ‫ܭ‬ըͰਪਐ͢ΔγϦίϯɾλϯάεςϯి࣓ΧϩϦϝʔλͷ։ൃʹ΋‫ڞ‬༻Ͱ͖ΔɻγεςϜͷಋೖʹΑΓɺΞϧϛઢϫΠϠʔϘϯσΟϯάɾηϯαʔͱಡΈग़͠νοϓͷϓϩʔϏϯάɾଟνϟϯωϧి‫ؾ‬ಛੑධՁͱσʔλऩूɾిࢠճ࿏γϛϡϨʔγϣϯͱઃ‫ܭ‬ɾ༗‫ݶ‬ཁૉ๏ʹΑΔྗֶత͓Αͼ೤తઃ‫ܭ‬ɾࣄ৅γϛϡϨʔγϣϯ͕ՄೳͱͳΓɺҰ‫ͨ͠؀‬։ൃ‫ڥ؀‬Λߏங͢Δ͜ͱ͕Ͱ͖Δɻདྷ೥౓ͷಋೖɾՔಇΛ໨ࢦ͠ɺࠓ೥౓͸γεςϜͷ࢓༷Λࡦఆͨ͠ɻ
ࠃࡍϦχΞίϥΠμʔ‫ܭ‬ը (઒ӽ ਗ਼Ҏɺ٢Ԭ ਸ਼थɺ຤‫ ݪ‬େ‫װ‬ɺਢ౻ ༟࢘ɺҪ্ ‫ࡾݚ‬ɺߐ࡚ ఩࿠ɺ্໺ ᠳɺ‫ ࡚ٶ‬ཅฏɺ෋ా ཾ඙)࣍ੈ୅Ճ଎‫ܭݧ࣮ث‬ըʮࠃࡍϦχΞίϥΠμʔʯ(ILC) ͷͨΊͷ෺ཧͱଌఆ‫ث‬ͷ‫ڀݚ‬Λߦ͍ͬͯΔɻຊ೥౓͔Β຤‫ݪ‬େ‫͕ڭॿװ‬ຊ‫ڀݚ‬ͷਪਐͷͨΊՃΘΓɺ͜Ε·ͰͷΧϩϦϝʔλ‫ʹڀݚ‬Ճ͑ɺγϛϡϨʔγϣϯΛ༻͍ͨ෺ཧղੳɾΞϧΰϦζϜ։ൃΛ৽ͨʹ࢝Ίͨɻ• ి࣓ΧϩϦϝʔλ༻γϦίϯύου‫ݕ‬ग़‫ث‬ͷ։ൃ‫ڀݚ‬ʢ઒ӽ ਗ਼Ҏɺ٢Ԭ ਸ਼थɺ຤‫ ݪ‬େ‫װ‬ɺਢ౻ ༟࢘ɺ‫ ࡚ٶ‬ཅฏɺ෋ా ཾ඙ʣ

ILC ࣮‫Ͱݧ‬͸ɺδΣοτʹର͢Δ༏ΕͨΤωϧΪʔ෼ղೳ͕ඞཁͰ͋ΓɺͦͷͨΊʹ Particle Flow Algorithm (PFA) ͱ‫ݺ‬͹ΕΔղੳํ๏͕ߟҊ͞Εͨɻ

PFA Ͱ͸ɺδΣοτதͷ‫ݸ‬ʑͷཻࢠΛΧϩϦϝʔλͰ෼཭͢Δࣄ͕ཁͱͳͬ
͓ͯΓɺͦͷͨΊʹ͸ 3 ࣍‫ݩ‬తʹࡉ෼Խ͞Εͨి࣓ΧϩϦϝʔλ͕ඞཁͱͳ
ΔɻILD ‫ݕ‬ग़‫Ͱث‬͸λϯάεςϯΛ‫ٵ‬ऩମͱ͢ΔαϯϓϦϯά‫ܕ‬ΧϩϦϝʔλΛߟ͓͑ͯΓɺηϯαʔ෦෼ʹ͸γϦίϯύουͱγϯνϨʔλετϦο
ϓ͕ఏҊ͞Ε͍ͯΔɻγϦίϯύουʹ͍ͭͯ͸ϑϥϯεͷ‫ؔػڀݚ‬ʢLLR

Ecole Polytechnique, LAL Orsayʣͱ೔෹‫ڞ‬ಉͰਐΊ͓ͯΓɺ೔ຊͰ͸‫۝‬भେֶ͕ͦͷ‫͍ͯͬͳͱ఺ڌ‬Δɻຊ೥౓͸੺֎ઢϨʔβʔΛ༻͍ͨγϦίϯύο
υͷԠ౴ಛੑଌఆ૷ஔΛ։ൃͨ͠ɻ͜Ε͸γϦίϯύουͷಛఆ෦Ґʹٙࣅ

57৴߸ͱͯ͠ϨʔβʔΛೖࣹ͠ଞηϧ΁ͷΫϩετʔΫ౳Λଌఆ͢Δ૷ஔͰɺ‫ࡏݱ‬͸ύου୺෦ʹ഑ஔ͢ΔΨʔυϦϯάͷ෇ۙʹϨʔβΛೖࣹ͠ɺΨʔυϦϯάͷߏ଄ͷҧ͍ʹΑΔӨ‫ڹ‬ධՁΛߦ͍ͬͯΔɻ·ͨɺલ೥౓ʹ։ൃͨ͠ϦʔΫిྲྀɺ੩ి༰ྔಛੑͷࣗಈ‫ܭ‬ଌ૷ஔΛ༻͍ͯɺ৽ͨͳ࢓༷ͷγϦίϯ
ύουͷධՁ΋ߦͬͨɻདྷ೥౓͸ɺηϧͷి‫ۃ‬෦Λϝογϡঢ়ʹՃ޻ͨ͠γϦίϯύουΛ༻͍ͯɺϨʔβʔΛϐΫηϧ಺ʹೖࣹͨ͠৔߹ͷԠ౴΋ௐ΂
Δ༧ఆͰ͋Δɻ• ϋΠϒϦουࣜి࣓ΧϩϦϝʔλͷ‫ڀݚ‬ʢ઒ӽ ਗ਼Ҏɺ٢Ԭ ਸ਼थɺ຤‫ ݪ‬େ‫װ‬ɺਢ౻ ༟࢘ɺ্໺ ᠳʣ

ILC ଌఆ‫ث‬ͷి࣓ΧϩϦϝʔλʹ༻͍Δηϯαʔͱͯ͠ɺੑೳతʹ͸γϦίϯύου͕࠷దͱߟ͑ΒΕΔ͕ɺίετ͕ߴ͗͢Δͱ‫ݒ‬೦͞Ε͍ͯΔɻҰํɺγϯνϨʔλετϦοϓ͸ൺֱత҆ՁͰ͋Δ͕ɺετϦοϓߏ଄ʹΑΔΰʔετΠϝʔδͷͨΊɺੑೳ͕ए‫ྼׯ‬Δͱߟ͑ΒΕ͍ͯΔɻͦ͜ͰɺαϯϓϦϯάΧϩϦϝʔλதʹγϦίϯύου૚ͱγϯνϨʔλετϦοϓ૚Λ૊Έ߹ΘͤΔࣄͰʢϋΠϒϦουࣜి࣓ΧϩϦϝʔλʣɺ༏ΕͨδΣοτΤω
ϧΪʔ෼ղೳΛҡ࣋͠ͳ͕ΒίετΛେ෯ʹ࡟‫͢ݮ‬ΔࣄΛߟ͑ɺγϛϡϨʔγϣϯʹΑΔ‫ڀݚ‬ΛਐΊ͍ͯΔɻຊ೥౓͸γϦίϯύουͱγϯνϨʔλετϦοϓͷ૊Έ߹Θͤํ΍‫ٵ‬ऩମͷްΈɺϨΠϠ਺౳Λ‫ܥ‬౷తʹมԽͤͯ͞
γϛϡϨʔγϣϯΛߦ͍ੑೳͷҧ͍Λॏ఺తʹௐ΂ͨɻདྷ೥౓͸ͦΕΛ‫ʹݩ‬࠷దͳϋΠϒϦουΧϩϦϝʔλͷߏ଄Λܾఆ͢Δͱͱ΋ʹɺ࣮ࡍʹ 2 छྨͷηϯαʔΛ૊Έ߹Θ࣮ͤͨ‫ػ‬Λ੡࡞͠ϏʔϜςετΛ໨ࢦ͢ɻ• γϦίϯి࣓ΧϩϦϝʔλࢼ࡞‫ػ‬ͷੑೳධՁʢ઒ӽ ਗ਼Ҏɺ٢Ԭ ਸ਼थɺ຤‫ݪ‬େ‫װ‬ɺਢ౻ ༟࢘ɺ্໺ ᠳɺ‫ ࡚ٶ‬ཅฏʣγϦίϯి࣓ΧϩϦϝʔλͷٕज़ϓϩτλΠϓͷ։ൃʹࢀՃ͠ɺϏʔϜςετ͓ΑͼσʔλղੳΛߦͬͨɻϏʔϜςετ͸ࡢ೥౓ʹҾ͖ଓ͖ 2013 ೥ 7݄ʹυΠπͷ DESY ‫͍ߦͯʹॴڀݚ‬ɺզʑ͸‫ݱ‬஍ʹ͓͚Δσʔλऩूʹߩ‫ݙ‬͢Δͱͱ΋ʹσʔλղੳΛओಋతʹߦͬͨɻࠓճͷϏʔϜςετͰ͸ಛʹύϫʔύϧεӡస (ൃ೤અ‫ݮ‬ͷͨΊ ILC Ճ଎‫ث‬ͷαΠΫϧ (5Hz) ʹ߹Θͤͯඞཁͳ࣌ؒͷΈిྗΛ‫͢څڙ‬Δ) ࣌ͷੑೳ҆ఆੑʹ͍ͭͯௐ΂ɺిྗΛ౤ೖ͔ͯ͠Β 600 Жඵఔ౓ͷ‫ؒظ‬͸ήΠϯͷมಈ͕‫ݟ‬ΒΕΔ͜ͱΛൃ‫ͨ͠ݟ‬ɻདྷ೥౓Ҏ߱͸ɺࡢ೥·Ͱ͸ओʹϑϥϯεͰߦΘΕ͍ͯͨσʔλऩू‫ܥ‬ͷ։ൃΛ‫۝‬भେֶଆͰ΋ຊ֨తʹਐΊΔ༧ఆͰ͋ΓɺͦͷͨΊϑϥϯεͷσʔλऩू‫ܥ‬ͷ‫۝‬भେֶ΁ͷҠసΛਐΊ͍ͯΔɻ͜ΕΛ༻͍ͯདྷ೥౓͸σʔλऩू‫ܥ‬ͷվྑΛߦ͍ɺ࣍ճͷΑΓେ‫ن‬໛ͳϏʔϜςετʹඋ͑Δɻ·ͨγϦίϯి58

࣓ΧϩϦϝʔλҎ֎ͷ ILC ଌఆ‫ͱث‬ͷ‫ڠ‬ௐಈ࡞΋ॏཁͳ՝୊Ͱ͋Γɺ͜Ε͸‫۝‬भେֶͷάϧʔϓ͕த৺ͱͳͬͯऔΓ૊Ή͜ͱʹͳ͍ͬͯΔɻ

• ILC ෺ཧղੳ͓ΑͼͦΕΛ༻͍ͨଌఆ‫࠷ث‬దԽʢ઒ӽ ਗ਼Ҏɺ٢Ԭ ਸ਼थɺ຤‫ ݪ‬େ‫װ‬ɺਢ౻ ༟࢘ɺ෋ా ཾ඙ʣ

LHC ࣮‫͍͓ͯʹݧ‬ώοάεཻࢠ͕ൃ‫͞ݟ‬Εɺ·ͨ৽෺ཧʹ܎ΘΔཻࢠ͸ࠓͷ
ͱ͜Ζൃ‫͞ݟ‬Ε͍ͯͳ͍ɻ͜ͷ‫ݱ‬ঢ়Λ౿·͑ͯɺILC ‫ݐ‬ઃ΁ͷॏཁͳεςοϓͱͯ͠ɺILC ͷ෺ཧతҙٛΛΑΓ໌֬ʹ͢Δ͜ͱ͓Αͼ ILC ͷଌఆ‫ث‬Λ෺ཧʹ߹ΘͤͯվΊͯ࠷దԽ͢Δ͜ͱ͕‫ٻ‬ΊΒΕ͍ͯΔɻILC ࣮‫͍͓ͯʹݧ‬͸·ͣώοάεཻࢠͷਫ਼ີଌఆ͕‫ۃ‬Ίͯॏཁͳ෺ཧͰ͋ΔɻILC ͷώοάεଌఆ͸ LHC ͱൺ΂ͯΑΓϞσϧඇґଘ͔ͭ֨ஈͷਫ਼౓Ͱώοάεͱཻ֤ࢠͷ݁߹ఆ਺Λ‫ٻ‬ΊΒΕΔ͜ͱ͕ಛ௕Ͱ͋Δɻ͜ͷϞσϧඇґଘͷώοάεଌఆͷཁͱͳΔͷ͕ώοάε൓௓࣭ྔ෼෍Λ༻͍ͨ ZH શஅ໘ੵଌఆͰ͋Δɻ͜ͷଌఆ͸ Z ͕Ϩϓτϯରʹ่յ͢Δ৔߹͕΋ͬͱ΋ղੳ͠΍͍͕͢ɺZ ͕ϋυϩϯରʹ่յ͢Δ৔߹΋ར༻͢Δ͜ͱͰ͞Βʹ֨ஈͷਫ਼౓্ঢ͕‫ظ‬଴Ͱ͖Δɻຊ‫Ͱࣨڀݚ‬͸͜ͷ Z ͕ϋυϩϯରʹ่յ͢Δ৔߹ͷ ZH શஅ໘ੵଌఆΛਪਐ͍ͯ͠Δɻ͜ͷϞʔυ͸ϨϓτϯରͷϞʔυʹൺ΂౷‫਺ܭ‬͸֨ஈʹଟ͍͕ɺόοΫάϥ΢ϯυͷ෼཭͓Αͼώοάεͷ่յʹର͢ΔґଘੑΛ཈͑Δ͜ͱ͕೉͍ͨ͠Ί֨ஈʹࠔ೉ͳղੳςʔϚͰ͋Δɻ‫ʹͰ·ࡏݱ‬ɺຊϞʔυΛ༻͍ͯͷશஅ໘ੵଌఆ͸Ϩϓτϯରͱಉఔ౓ͷਫ਼౓͕ಘΒΕ͕ͨɺࠓ‫͞ޙ‬Βʹߴ౓͔ͭ࠷దͳղੳख๏Λಋೖ͠ɺਫ਼౓ΛϨϓτϯରͷ൒෼ఔ౓·ͰߴΊΔ͜ͱΛ໨ࢦͯ͠‫ڀݚ‬Λ͢͢ΊΔɻ·ͨɺτοϓཻࢠͱώοάεཻࢠͷ݁߹Λ௚઀ଌఆ͢Δ ttH ϓϩηε΋ ILC Ͱಛʹॏཁͳ෺ཧͷҰͭͰ͋Δɻ͜Εʹؔͯ͠΋ຊ‫୲͕ࣨڀݚ‬౰͠ɺҎલͷ΋ͷΛ্ճΔਫ਼౓ͷղੳ݁Ռ͕ಘΒΕ͍ͯΔɻ͜Ε΋‫ܥ‬౷‫ࠩޡ‬ͷධՁ΍ղੳͷ͞ΒͳΔվળΛߦ͏ɻ·ͨɺ͜ΕΒͷղੳ݁Ռ͓Αͼଞͷղੳ݁Ռ΋༻͍ͯ ILD ଌఆ‫͚͓ʹث‬Δ࠷దͳߏ଄Λ‫ূݕ‬͠ɺܾఆʹࢀը͍ͯ͘͠༧ఆͰ͋Δɻ

• ILC ࠃ಺ީิ஍ͷௐࠪ‫ݕ‬౼ͱҰຊԽͷͨΊͷཱ஍ධՁʢ઒ӽਗ਼Ҏɺ٢Ԭਸ਼थɺߐ࡚఩࿠ɺҪ্‫ࡾݚ‬ʣ

ILC ͷࠃ಺‫ݐ‬ઃީิ஍͸෱Ԭ‫ݝ‬ɾࠤլ‫͕ͨ·ʹݝ‬Δഎৼࢁ஍ͱ‫ؠ‬ख‫ݝ‬ͷ๺্ࢁ஍ʹߜΒΕ͍ͯΔɻΘΕΘΕ͸ɺߴΤωϧΪʔՃ଎‫ߏػڀݚث‬ʢKEKʣͷٕज़‫ྗڠ‬Λಘͯɺ෱Ԭ‫ݝ‬ɺࠤլ‫ͱͱݝ‬΋ʹഎৼࢁ஍ͷ஍࣭ௐࠪͱ࠷దϧʔτͷ‫ݕ‬౼Λߦ͖ͬͯͨɻຊ೥౓͸ฏ੒̎̏೥౓ୈ̏࣍ิਖ਼༧ࢉʹΑΔ KEK ͔Βͷडୗ‫ڀݚ‬ʮࠃࡍϦχΞίϥΠμʔ‫ܭ‬ը (ILC) ࢪઃ‫ݐ‬ઃʹ܎Δ‫ݱ‬஍ௐࠪʯͷ݁ՌΛ·ͱΊɺ݄̓ʹ KEK ΁ͷใࠂΛߦͬͨɻ59ฏ੒̎̑೥݄̍ʹɺILC ઓུձٞͷ΋ͱʹૉཻࢠ࣮‫ ͱ໊̓ऀڀݚݧ‬ILC ࢪઃͷઐ໳Ո໊̍Ͱߏ੒͞ΕΔ ILC ཱ஍ධՁձٞʢ‫ڞ‬ಉٞ௕ɿ઒ӽʢ‫۝‬भେֶʣɺ
ࢁຊʢ౦๺େֶʣ͕ઃཱ͞Εɺࠃ಺ީิ஋ҰຊԽʹ޲͚ͯɺٕज़తͳ‫ͱ఺؍‬ࣾձ‫ڥ؀‬ͷ‫͔఺؍‬Β̎ͭͷީิ஍ͷֶज़తɾՊֶతධՁΛ։࢝ͨ͠ɻ‫۝‬भେֶ͸ɺࠤլେֶɺ෱Ԭ‫ݝ‬ɺࠤլ‫ݝ‬ɺ‫۝‬भ‫ࡁܦ‬࿈߹ͱ‫ͯ͠ྗڠ‬ɺٕज़ධՁͱࣾ
ձ‫جڥ؀‬൫ධՁͷͨΊͷࢿྉΛ࡞੒͠ɺILC ཱ஍ධՁձٞʹఏग़ͨ͠ɻILC
ཱ஍ධՁձٞ͸ٕज़ઐ໳ҕһձɺࣾձ‫جڥ؀‬൫ධՁઐ໳ҕһձͰͷٞ࿦Λ;·͑ͯධՁΛߦͳ͍ɺ͞ΒʹࠃࡍϨϏϡʔΛ‫Ͱ͑͏ͨܦ‬ɺ8 ݄ 23 ೔ʹʮ๺্ࢁ஍Λ࠷దͱ͢ΔʯධՁ݁ՌΛެදͨ͠ɻͳ͓ɺ‫۝‬भେֶɾࠤլେֶ͸ฏ੒̎̒೥݄̍ʹ‫ڀݚ‬ձΛઃཱͯ͠ɺILC ཱ஍ධՁձٞͷධՁ಺༰ͷ‫ূݕ‬Λ࢝Ί͍ͯΔɻຊ‫ࣨڀݚ‬͸ɺILC ‫ݐ‬ઃ஍͕Ͳ͜Ͱ͋ͬͯ΋ɺͦͷ࣮‫ڀݚ͚ͨ޲ʹݱ‬‫׆‬ಈɾਪਐ‫׆‬ಈΛࠓ‫ޙ‬΋ߦͳ͍ͬͯ͘ɻ
ϛϡʔΦϯɾిࢠస‫׵‬աఔͷ୳ࡧ (઒ӽ ਗ਼Ҏɺ౦৓ ॱ࣏ɺ٢Ԭ ਸ਼थɺࢁ‫ ޱ‬ത࢙ɺେੴ ߤɺத‫ ډ‬༐थ)ҵ৓‫ݝ‬౦ւଜʹ͋Δେ‫౓ڧ‬ཅࢠՃ଎‫ࢪث‬ઃ J-PARC ͷϋυϩϯ࣮‫ࢪݧ‬ઃʹ͓͍ͯɺϛϡʔΦϯ͕ిࢠʹస‫͢׵‬ΔաఔΛ୳ࡧ͢ΔͨΊɺCOMET ࣮‫( ݧ‬J-PARC E21 ࣮‫ )ݧ‬Λࠃࡍ‫ڞ‬ಉ‫Ͱڀݚ‬ਐΊ͍ͯΔɻੈք࠷ߴ‫౓ڧ‬ͷύϧεϛϡʔΦϯϏʔϜΛੜ੒͢Δ࣮‫ࢪݧ‬ઃ͕ຊ೥౓͔Β‫ݐ‬ઃΛ։࢝͠ɺ‫ݕ‬ग़‫ث‬ͷ։ൃΛߦ͍ͬͯΔɻ• ి࣓ΧϩϦϝʔλͷ։ൃʢ઒ӽ ਗ਼Ҏɺ౦৓ ॱ࣏ɺ٢Ԭ ਸ਼थɺࢁ‫ ޱ‬ത࢙ɺେੴ ߤɺத‫ ډ‬༐थʣߴ‫ڥ؀཰਺ܭ‬ԼͰిࢠͷΤωϧΪʔΛଌఆ͠ɺࣄ৅τϦΨʔʹ࢖༻͢ΔͨΊͷి࣓ΧϩϦϝʔλͷ։ൃΛਐΊ͍ͯΔɻ࣓৔͕͋ΔਅۭதͰಈ࡞ͤ͞ɺߴ
ΤωϧΪʔ෼ղೳͱ଎͍࣌ؒԠ౴Λඞཁͱ͢ΔͨΊɺGSO ·ͨ͸ LYSO ݁থΛΞόϥϯγΣɾϑΥτμΠΦʔυͰಡΈग़͢͜ͱΛ‫ݕ‬౼͍ͯ͠Δɻ࠾༻
ީิͰ͋Δ݁থΛ༻͍ͯɺϓϩτλΠϓ‫ݕ‬ग़‫ͱث‬ಡΈग़͠ճ࿏Λ੡࡞ɺσʔλऩूγεςϜͷߏஙΛߦ͍ɺJ-PARC ϋυϩϯ࣮‫ࢪݧ‬ઃͷ K1.1BR ϏʔϜϥΠϯͰςετ࣮‫( ݧ‬J-PARC T51 ࣮‫ )ݧ‬ΛߦͬͨɻϏʔϜੑೳͷෆఆੑͷൣғͰྑ޷ͳ݁ՌΛಘ͕ͨɺϏʔϜλΠϜͷॖখʹΑΓଌఆ‫ܭ‬ը͕ະফԽͰ
͋ͬͨɻ࠷ऴ݁ՌΛಘΔ΂͘ɺಡΈग़͠ճ࿏ͱిࢠͷೖࣹҐஔΛଌఆ͢Δγ
ϯνϨʔγϣϯϑΝΠόʔ‫ݕ‬ग़‫ث‬Λվྑ͠ɺߴ඼࣭ͷిࢠϏʔϜ͕ར༻Ͱ͖
Δ౦๺େֶిࢠޫཧֶ‫ڀݚ‬ηϯλʔͰ࠶౓ςετ࣮‫( ݧ‬՝୊൪߸ 2768) Λߦͬͨɻ྆݁থʹ͍ͭͯɺΤωϧΪʔ 105 MeV ෇ۙͰ 5 %ఔ౓ҎԼͷΤωϧΪʔ෼ղೳΛಘΔ͜ͱʹ੒ޭͨ͠ɻ࠷ऴ݁ՌΛདྷ೥౓தʹ·ͱΊɺ࣮‫͢༻࠾ʹػ‬Δ݁থΛܾఆ͢Δ༧ఆͰ͋Δɻ

60

• Phase-I τϦΨʔ‫ݕ‬ग़‫ث‬ͷ։ൃʢ઒ӽ ਗ਼Ҏɺ౦৓ ॱ࣏ɺ٢Ԭ ਸ਼थɺத‫ډ‬༐थʣ

COMET ࣮‫ݧ‬ͷୈҰஈ֊ (Phase-I) Ͱ͸ɺO(10−15 ) ͷൃ‫ͨ·( ౓ײݟ‬͸্‫ݶ‬஋ઃఆ) Ͱͷ࣮‫ݧ‬Λ‫ܭ‬ը͓ͯ͠Γɺԁ౵‫ܕ‬υϦϑτνΣϯόʔͱτϦΨʔ‫ݕ‬ग़‫ث‬Λ૊Έ߹Θͤͨ‫ݕ‬ग़‫ث‬γεςϜ͕ओཁͳ໾ׂΛՌͨ͢ɻզʑͷάϧʔϓ͸ɺτϦΨʔ‫ݕ‬ग़‫ث‬ͷ։ൃΛਐΊ͍ͯΔɻిࢠΛτϦΨʔ͢ΔͨΊɺUV ΞΫϦϧΛνΣϨίϑ᫔ࣹମͱ͠ɺޫ‫ݕ‬ग़‫͋Ͱث‬Δ Multi-Pixel Photon Counter(MPPC) ʹΑΔಡΈग़͠Λ‫ݕ‬౼͍ͯ͠Δɻ͞Βʹɺ৴߸-എ‫ܠ‬ൺͷ޲্ͱλΠϛϯά৘ใΛఏ‫͢ڙ‬ΔͨΊɺMPPC ಡΈग़͠ʹΑΔϓϥενοΫγϯν
ϨʔλΛ૊Έ߹ΘͤΔɻࠓ೥౓͸ɺUV ΞΫϦϧͷްΈͷ࠷దԽɺUV ΞΫϦϧͱϓϥενοΫγϯνϨʔλΛ෴͏൓ࣹࡐɾःޫࡐͷ࠷దԽɺMPPC Λ༻͍ͨಡΈग़͠ʹ͍ͭͯɺӉ஦ઢࢼ‫ݧ‬Λߦͬͨɻ࠷ऴઃ‫͚ͨ޲ʹܭ‬։ൃΛਐΊΔͨΊɺདྷ೥౓ʹ౦๺େֶిࢠޫཧֶ‫ڀݚ‬ηϯλʔͰͷిࢠϏʔϜʹΑΔςετ࣮‫ݧ‬Λ‫ܭ‬ը͠ɺͦͷ४උΛਐΊ͍ͯΔɻCOMET ࣮‫ࢪݧ‬ઃͰ͸ɺ๲େͳதੑࢠྔ͕༧૝͞ΕΔͨΊɺதੑࢠྔͷධՁͱ MPPC ͷ์ࣹઢ଱ੑΛ‫ݚ‬‫͢ڀ‬Δ͜ͱ͕ࠓ‫ޙ‬ͷ՝୊Ͱ͋Δɻ• ϏʔϜཻࢠࣝผੑೳͷ‫ڀݚ‬ʢ઒ӽ ਗ਼Ҏɺ౦৓ ॱ࣏ɺ٢Ԭ ਸ਼थɺࢁ‫ ޱ‬ത࢙ʣ
COMET ࣮‫ݧ‬ͷ Phase-I Ͱ͸ɺԁ౵‫ܕ‬υϦϑτνΣϯόʔͱτϦΨʔ‫ݕ‬ग़‫ث‬ʹΑΔ෺ཧϥϯʹՃ͑ɺॳΊͯੜ੒͢ΔϛϡʔΦϯϏʔϜͷੑ࣭Λৄࡉʹௐ΂Δ͜ͱ͕ෆՄܽͰ͋ΔɻPhase-I ʹ͓͚ΔϛϡʔΦϯϏʔϜͷ‫ڀݚ‬͸ɺO(10−17 ) ͷൃ‫ͨ·( ౓ײݟ‬͸্‫ݶ‬஋ઃఆ) Λ໨ࢦͨ͠ COMET ࣮‫ݧ‬ͷୈೋஈ֊ (Phase-II) ΁ਐΉͨΊʹ΋ॏཁͰ͋ΔɻಛʹɺϛϡʔΦϯϏʔϜதͷిࢠɾύΠதؒࢠɾ൓ཅࢠͳͲͷഎ‫ࢠཻܠ‬Λࣝผ͢Δ͜ͱ͕‫ݤ‬ΛѲΔɻ‫ݕ‬ग़‫ʹث‬͸ɺPhase-II ʹ͓͚Δ෺ཧϥϯͷͨΊʹ։ൃΛਐΊ͍ͯΔετϩʔνϡʔϒඈ੻‫ݕ‬ग़‫࣓ిͱث‬ΧϩϦϝʔλΛ༻͍Δ‫ܭ‬ըͰ͋ΓɺγϛϡϨʔγϣϯΛ༻͍ͨ‫ݕ‬ग़‫ث‬ͷϏʔϜཻࢠࣝผੑೳͷ‫ڀݚ‬Λ։࢝ͨ͠ɻ‫ݕ‬ग़‫ث‬ͷ഑ஔͳͲͷ࠷దԽΛਐΊΔ༧ఆͰ͋ΔɻϛϡʔΦϯҟৗ࣓‫ؾ‬Ϟʔϝϯτɾి‫ؾ‬૒‫ࢠۃ‬Ϟʔϝϯτͷଌఆ (઒ӽ ਗ਼Ҏɺ౦৓ ॱ࣏ɺ٢Ԭ ਸ਼थɺ‫ݹ‬Ӝ ৽࢘ɺௐ ᠳฏ)ҵ৓‫ݝ‬౦ւଜʹ͋Δେ‫౓ڧ‬ཅࢠՃ଎‫ࢪث‬ઃ J-PARC ͷ෺࣭ɾੜ໋Պֶ࣮‫ࢪݧ‬ઃ (MLF)ʹ͓͍ͯɺϛϡʔΦϯͷҟৗ࣓‫ؾ‬Ϟʔϝϯτͱి‫ؾ‬૒‫ࢠۃ‬ϞʔϝϯτΛଌఆ͢Δ࣮‫ݧ‬(J-PARC E34 ࣮‫ )ݧ‬Λࠃࡍ‫ڞ‬ಉ‫Ͱڀݚ‬ਐΊ͍ͯΔɻ‫ྫྷۃ‬ϛϡʔΦϯϏʔϜΛ༻͍ͨશ͘৽͍͠ଌఆ‫ݪ‬ཧʹ‫͋Ͱݧ࣮ͮ͘ج‬Γɺຊ೥౓͔Β‫ݕ‬ग़‫ث‬։ൃΛ։࢝ͨ͠ɻ

• γϦίϯετϦοϓ‫ݕ‬ग़‫༻ث‬ಡΈग़͠νοϓͷ։ൃʢ઒ӽ ਗ਼Ҏɺ౦৓ ॱ࣏ɺ61٢Ԭ ਸ਼थɺ‫ݹ‬Ӝ ৽࢘ɺௐ ᠳฏʣϛϡʔΦϯͷҟৗ࣓‫ؾ‬Ϟʔϝϯτ (g − 2) ͷଌఆ͸ɺถࠃϒϧοΫϔϒϯࠃཱ‫( ॴڀݚ‬BNL) ͷ E821 ࣮‫ ͕ݧ‬0.54 ppm ͷਫ਼౓Ͱૉཻࢠඪ४໛‫( ܕ‬SM) ͔Β

3 σ ͷͣΕΛൃද͠ɺSM Λ௒͑Δ෺ཧ (BSM) ͷ୳ࡧʹ͓͍ͯॏཁͳҐஔΛ઎Ί͍ͯΔɻ·ͨɺి‫ؾ‬૒‫ࢠۃ‬Ϟʔϝϯτ (EDM) ͷଌఆ͸ɺBNL E821 ࣮‫ݧ‬
͕ 1.9 × 10−19 e · cm ͷ্‫ݶ‬஋Λ༩͕͑ͨɺ༗‫ݶ‬ͷ஋͕ BSM ͷଘࡏΛࣔࠦ͢ΔͨΊɺҟৗ࣓‫ؾ‬Ϟʔϝϯτͷଌఆͱฒͼॏཁੑ͕ߴ͍ɻզʑ͕ J-PARC Ճ଎‫ ث‬MLF ࢪઃͰ४උΛਐΊ͍ͯΔ৽͍࣮͠‫ݧ‬͸ɺ‫ྫྷۃ‬ϛϡʔΦϯϏʔϜΛੜ੒ɾՃ଎͠ɺऩଋి৔Λ༻͍ͣʹ௒ߴਫ਼౓࣓৔தʹϛϡʔΦϯΛ஝ੵ͢Δ
͜ͱʹΑΓɺg − 2 Λ 0.1 ppm ͷਫ਼౓ͰɺEDM Λ 10−21 e · cm ͷ্‫ݶ‬஋·ͰɺͦΕͧΕΛ෼཭ͯ͠ଌఆ͠ɺBMS Λ୳ࡧ͢Δ໺৺తͳ‫ܭ‬ըͰ͋Δɻ͜ͷ࣮‫ݧ‬ΛՄೳͱ͢Δ‫ݕ‬ग़‫ث‬͸ɺϛϡʔΦϯΛ஝ੵ͢Δ࣓৔಺ʹઃஔ͢Δߴ‫཰਺ܭ‬γϦίϯετϦοϓ‫ݕ‬ग़‫͋Ͱث‬ΔɻϛϡʔΦϯͷ่յͰੜ੒͞ΕΔཅిࢠͷඈ੻ΛγϦίϯετϦοϓ‫ݕ‬ग़‫ث‬ͷώοτ৘ใ͔Β࠶ߏ੒͢Δɻ࣮‫ٕݧ‬ज़తʹ௅ઓతͳ఺͸ɺฏ‫ۉ‬ώοτ‫ Ͱ཰਺ܭ‬1 ετϦοϓ͋ͨΓ 1.6 MHz ͔Βೋܻ௿͍ྖҬ·Ͱɺߴ‫ݕ‬ग़ޮ཰Ͱಈ࡞͢Δ͜ͱ͕ཁ‫͞ٻ‬ΕΔ͜ͱͰ͋Δɻͦͷ‫ݕ‬ग़‫ث‬Λ࣮‫͢ݱ‬ΔͨΊʹɺγϦίϯετϦοϓ‫ݕ‬ग़‫͍༻ʹث‬ΔಡΈग़͠νοϓͷ։ൃΛਐΊ͍ͯΔɻࠓ೥౓͸ɺిࢠճ࿏γϛϡϨʔγϣϯʹΑΔνοϓͷධՁɺධՁ‫ج‬൘্ʹ࣮૷ͨ͠νοϓͷੑೳධՁΛߦͬͨɻͦͷධՁʹ‫͖ͮج‬ɺདྷ೥౓ʹ‫ܭ‬ը͍ͯ͠Δ J-PARC Ճ଎‫ ث‬MLF ࢪઃͱ౦๺େֶిࢠޫཧֶ‫ڀݚ‬ηϯλʔʹ͓͚ΔϏʔϜςετͷ४උΛਐΊͨɻདྷ೥౓͸ɺϏʔϜςετʹ
ΑΔධՁΛߦ͍ɺ࣮‫ػ‬Λ໨ࢦͨ࣍͠‫ظ‬ϓϩτλΠϓͷ։ൃɾ੡࡞Λ໨ࢦ͢ɻதੑࢠΛ༻͍ͨ‫ૅج‬෺ཧ (٢Ԭ ਸ਼थɺদຊ ‫ޛ‬ɺాத‫)ؾݩ‬• ߴਫ਼౓தੑࢠ่յण໋ଌఆ࣮‫ݧ‬ʢ٢Ԭਸ਼थɺాத‫ؾݩ‬ʣզʑ͸ҵ৓‫ݝ‬౦ւଜͷ J-PARC Ճ଎‫ث‬Λ༻͍ͯதੑࢠ่յण໋Λߴਫ਼౓Ͱଌ
ఆ͢Δ࣮‫ݧ‬Λਪਐ͍ͯ͠Δɻதੑࢠण໋Λಋग़͢ΔͨΊʹ͸தੑࢠͷϑϥοΫεͱЌ่յͷྔΛ஌Δඞཁ͕͋Δ͕ɺ͜Ε·ͰߦΘΕ͖࣮ͯͨ‫Ͱݧ‬͸தੑࢠͱนͱͷ૬‫༻࡞ޓ‬΍ϑϥοΫεͷ‫ܥ‬౷‫͕ࠩޡ‬໰୊ͱͳ͍ͬͯͨɻ͜Εʹର͠ɺզʑͷ࣮‫Ͱݧ‬͸ϑϥοΫεͱЌ่յిࢠΛ TPC ‫ݕ‬ग़‫Ͱث‬ಉ࣌ଌఆ͢Δ͜ͱʹΑΓɺ͜Ε·Ͱͷ࣮‫ʹݧ‬൐͍ͬͯͨ‫ܥ‬౷‫ࠩޡ‬Λճආ͢Δ͜ͱ͕Մೳͱ
ͳΔɻզʑ͸ɺ͜ͷ৽ͨͳख๏Λ༻͍ͯ 0.1a ͷਫ਼౓Ͱதੑࢠͷण໋Λଌఆ͢Δ͜ͱΛ໨ࢦ͍ͯ͠Δɻຊ೥౓͸ 2012 ೥ 6 ݄ʹऔಘͨ͠ίϛογϣχϯάϥ
ϯͷσʔλղੳΛߦͬͨɻৄࡉͳղੳʹઌཱͪɺͻͱͭͻͱͭͷΠϕϯτΛ
໨Ͱ‫֬ͯݟ‬ೝ͢ΔɺΞΠεΩϟϯΛߦͬͨɻͦͷ݁Ռɺน͔Βൃੜ͢Δ α ઢ62΍์ిͳͲ͕എ‫ࣄܠ‬৅ʹͳΔͱ͍͏͜ͱΛಥ͖ࢭΊͨɻͦͷ‫ޙ‬ɺઌߦ࣮‫ͱݧ‬ಉ༷ͷղੳख๏Λ༻͍ͯղੳΛߦͬͨɻͦͷաఔͰɺGeant4 Λ༻͍ͨγϛϡϨʔγϣϯߏஙΛߦͬͨɻ࣮‫ݧ‬σʔλͱγϛϡϨʔγϣϯͰΤωϧΪʔ΍ཻࢠͷඈͿ‫Ͳͳ཭ڑ‬ͷ༷ʑͳ෼෍ͷൺֱΛߦ͕ͬͨɺ·ͩվળͷ༨஍͕͋ͬͨɻ
࣍೥౓͸ͦͷվળʹऔΓ૊Ή༧ఆͰ͋Δɻ• ௿ΤωϧΪʔதੑࢠͷখ֯ࢄཚΛ༻͍ͨະ஌૬‫༻࡞ޓ‬ͷ୳ࡧ࣮‫ݧ‬ʢ٢Ԭਸ਼थɺ
দຊ‫ޛ‬ʣ
զʑ͸௿ΤωϧΪʔͷதੑࢠͱ‫ر‬Ψε‫ࢠݪ‬ͷࢄཚʹΑΓφϊϝʔτϧεέʔϧͰະ஌ͷ૬‫༻࡞ޓ‬Λ୳ࡧ͢Δ࣮‫ܭݧ‬ըΛཱҊ͍ͯ͠Δɻ౰֘೥౓Ͱ͸ɺࢄཚΨεࢼྉ༰‫ث‬ͷ૭ࡐબఆ࣮‫ݧ‬Λߦ͍ɺࢄཚΨεࢼྉ༰‫ث‬Λ‫׬‬੒ͤ͞Δ༧ఆ
Ͱ͕͋ͬͨɻ૭ࡐબఆ࣮‫ݧ‬͸ɺ࣮‫ࢪ࣮ݧ‬༧ఆͰ͋ͬͨ J-PARC Ճ଎‫ࢪث‬ઃ͕౰֘೥౓தӡసΛఀࢭ͍ͯͨͨ͠Ί࣮ࢪ͕ෆՄೳͰ͋ͬͨɻͦͷͨΊɺ͢Ͱʹऔಘͯ͋ͬͨ͠༧උσʔλͷৄࡉͳղੳ‫͜ͼٴ‬ͷͨΊʹ৽‫ن‬։ൃͨ͠ϞϯςΧϧϩγϛϡϨʔγϣϯΛ૊Έ߹Θͤͯɺ‫ݒ‬೦͞Ε͍ͯͨ૭ࡐʹΑΔഎ‫ܠ‬ࣄ৅͕ຊ࣮‫ݧ‬ͷো֐ͱͳΒͳ͍͜ͱΛࣔͨ͠ɻ·ͨɺඪతཻࢠͷ೤ӡಈΛߟྀ࣮ͨ͠‫ܥݧ‬ͷγϛϡϨʔγϣϯΛ৽ͨʹ։ൃ͠ɺଌఆ‫ܥ‬ͷ࠷దԽΛߦͬͨɻͦͷ݁ՌɺதੑࢠϏʔϜμΫτ͔Β 1m Լྲྀʹඪత༰‫ث‬ɺ͞Βʹ 3m Լྲྀʹதੑࢠ‫ݕ‬ग़‫ث‬Λઃஔ͢ΔࣄͰଌఆ͕࣌ؒ࠷খʹͳΔ͜ͱ͕෼͔ͬͨɻൃද࿦จ ‫ݪ‬ஶ࿦จ 
G. Aad et al. [ATLAS Collaboration], “Search for a Multi-Higgs Boson Cascade in√
W + W − bb events with the ATLAS detector in pp collisions at s = 8 TeV”, Phys.
Rev. D 89, 032002 (2014).
G. Aad et al. [ATLAS Collaboration], “Standalone vertex ﬁnding in the ATLAS muon
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boson using ATLAS data”, Phys. Lett. B 726, 120-144 (2013).
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G. Aad et al. [ATLAS Collaboration], “Measurement of the Azimuthal Angle De65

pendence of Inclusive Jet Yields in Pb+Pb Collisions at√

sN N = 2.76 TeV with the

ATLAS detector”, Phys. Rev. Lett. 111, 152301 (2013).
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Neutral Particles in the ATLAS Detector”, JINST 8, P07015 (2013).
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W W/W Z → lνjj decay channels with the ATLAS detector at s = 7 TeV”, Phys.
Rev. D 87, 112006 (2013).
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ton and ETmiss ﬁnal state in√s = 7 TeV proton-proton collisions using the ATLAS

detector”, Phys. Rev. D 88, 012001 (2013).
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s = 7 TeV using the ATLAS detector”, Eur. Phys. J. C 73, 2509 (2013).
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in pp collisions at s = 7 TeV with the ATLAS detector”, JHEP 1306, 033 (2013).
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pp collisions at√

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C.Adloﬀ et al.
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Validation of GEANT4 Monte Carlo models with a highly granular scintillator-steel
hadron calorimeter:
C.Adloﬀ et al.
JINST 8, P07005 (2013), doi:10.1088/1748-0221/8/07/P07005
Track segments in hadronic showers in a highly granular scintillator-steel hadron calorimeter:
C.Adloﬀ et al.
JINST 8, P09001 (2013), doi:10.1088/1748-0221/8/09/P09001

Proceedings
The Performance of the Physics Prototype of the CALICE ScWECAL for ILD:
Yuji Sudo
Proceedings of the CHEF2013 Conference - Eds. J.-C. Brient, R. Salerno, and Y.
Sirois, pp.145-151, ISBN 978-2-7302-1624-1, 2013
Simulation Study for the Hybrid ECAL for ILD:
Hiraku Ueno
Proceedings of the CHEF2013 Conference - Eds. J.-C. Brient, R. Salerno, and Y.
Sirois, pp.279-285, ISBN 978-2-7302-1624-1, 2013ߨԋ69

 ւ֎Ͱͷߨԋ 
Status of Higgs Searches
Junji Tojo on behalf of the ATLAS and CMS Collaborations
Flavor Physics and CP Violation (FPCP2013), 19-24 May 2013, Rio de Janeiro
A consideration of combined DAQ for hybrid ECAL:
Suehara Taikan
CALICE Collaboration meeting, 19-21 March 2014, Argonne
Study of the response of the CALICE Si-W ECAL physics-prototype to positrons:
Miyazaki Youhei
CALICE Collaboration meeting, 19-21 March 2014, Argonne
Silicon sensor study for ILD ECAL:
Tomita Tatsuhiko
CALICE Collaboration meeting, 19-21 March 2014, Argonne
Si ECAL TB analysis: ramp up time of the electronics:
Sudo Yuji
CALICE Collaboration meeting, 19-21 March 2014, Argonne
Simulation Study for the Hybrid ECAL:
Ueno Hiraku
CALICE Collaboration meeting, 19-21 March 2014, Argonne
Beam test performance of the SiECAL technological prototype:
Sudo Yuji
LCWS13, 11-15 Nov 2013, Tokyo
Simulation study of the Hybrid ECAL for ILC:
Ueno Hiraku
LCWS13, 11-15 Nov 2013, Tokyo
Study of the response of the CALICE SiW ECAL physics-prototype to positorons:
Miyazaki Youhei
70

LCWS13, 11-15 Nov 2013, Tokyo
A study of silicon sensors for ILD ECAL:
Tomita Tatsuhiko
LCWS13, 11-15 Nov 2013, Tokyo
Linear Collider Detectors:
Kawagoe Kiyotomo
27 Oct - 2 Nov 2013, Seoul
R&D for the ECAL:
Sudo Yuji
2013 ILD meeting, 24-26 Sep 2013, Cracow
Silicon sensor study for ILD ECAL:
Yoshioka Tamaki
CALICE Collaboration meeting, 9-11 Sep 2013, Annecy
Study of the response of the CALICE SI-W ECAL physics prototype to positorons:
Miyazaki Youhei
CALICE Collaboration meeting, 9-11 Sep 2013, Annecy
Si Sensor Study for ILD Calorimeter:
Yuji Sudo
ECFA LC2013, 27-31 May 2013, Humburg
The performance of the Physics Prototype of the CALICE ScWECAL for ILD
Yuji Sudo
ECFA LC2013, 27-31 May 2013, Humburg
Simulation study of the hybrid Ecal:
Hiraku Ueno
ECFA LC2013, 27-31 May 2013, Humburg
The Performance of the Physics Prototype of the CALICE ScWECAL for ILD:
71

Yuji Sudo
CHEF2013, 22-25 April 2013, Paris
Simulation Study for the Hybrid ECAL for ILD:
Hiraku Ueno
CHEF2013, 22-25 April 2013, Paris ࠃ಺Ͱͷߨԋ 
125 GeV Higgs at the LHC : h ˠ ZZ,WW :Susumu Oda on behalf of the ATLAS and CMS Collaborations
Higgs and Beyondɺ2013 ೥ 6 ݄ɺ౦๺େֶ
LHC-ATLAS ࣮‫͚͓ʹݧ‬Δ H → Z (∗) Z (∗) → 4l νϟϯωϧΛ༻͍ͨώοάεཻࢠͷ‫ݚ‬‫ڀ‬:৫ా‫ק‬ɺଞ ATLAS Collaboration
ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձɺ2013 ೥ 11 ݄ɺ‫ཹٱ‬ถ޻‫ۀ‬େֶ

Present and future of physics at the LHC experiments :Susumu Oda
Workshop on High-energy QCD and nucleon structureɺ2014 ೥ 3 ݄ɺKEK ౦ւΩϟϯύεH ˠ ZZ(combined) spin/CP ଌఆ :৫ా‫ק‬৽ֶज़ྖҬ ʮઌ୺Ճ଎‫ ث‬LHC ͕੾Γ୓͘ςϥεέʔϧͷૉཻࢠ෺ཧֶʯ‫ڀݚ‬ձɺ2014೥ 3 ݄ɺ౦‫ژ‬େֶ

LHC-ATLAS ࣮‫͚͓ʹݧ‬Δ H → Z (∗) Z (∗) → 4l νϟϯωϧΛ༻͍ͨώοάεཻࢠͷ‫ݚ‬‫ڀ‬:৫ా‫ק‬ɺଞ ATLAS Collaboration೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ2014 ೥ 3 ݄ɺ౦ւେֶ
γϯϙδ΢ϜߨԋʮILC ͷ෺ཧʢ࣮‫ݧ‬ʣʯ:຤‫ݪ‬େ‫װ‬72೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ2014 ೥ 3 ݄ 27 ೔ʙ30 ೔ɺ౦ւେֶভೆΩϟϯύε
ϦχΞίϥΠμʔ࣮‫͚͓ʹݧ‬Δ࣭ྔ 125GeV ͷώοάεʹର͢Δτοϓ౬઒݁߹ͷଌఆਫ਼౓ͷධՁ: ਢ౻༟࢘೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ2014 ೥ 3 ݄ 27 ೔ʙ30 ೔ɺ౦ւେֶভೆΩϟϯύε

ILD ʹ͓͚Δ ECAL ͷͨΊͷγϦίϯ‫ݕ‬ग़‫ث‬ͷಛੑ‫ͱڀݚ‬Ϩʔβʔ΁ͷԠ౴ଌఆ:෋ాཾ඙೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ2014 ೥ 3 ݄ 27 ೔ʙ30 ೔ɺ౦ւେֶভೆΩϟϯύε

ILC ʹ͓͚Δ Si-W ి࣓ΧϩϦϝʔλࢼ࡞‫ػ‬ͷੑೳ‫ڀݚ‬:‫࡚ٶ‬ཅฏ
೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ2014 ೥ 3 ݄ 27 ೔ʙ30 ೔ɺ౦ւେֶভೆΩϟϯύε

ILC ʹ͓͚Δి࣓ΧϩϦϝʔλͷͨΊͷγϦίϯ‫ݕ‬ग़‫ث‬ͷϨʔβʔΛ༻͍ͨಛੑ‫ڀݚ‬:෋ాཾ඙ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձɺ2013 ೥ 11 ݄ 30 ೔ɺ‫ཹٱ‬ถ޻‫ۀ‬େֶ

ILC ʹ͓͚Δ Si-W ࡉ෼ׂి࣓ΧϩϦϝʔλࢼ࡞‫ػ‬ͷੑೳ‫ڀݚ‬:‫࡚ٶ‬ཅฏ
ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձɺ2013 ೥ 11 ݄ 30 ೔ɺ‫ཹٱ‬ถ޻‫ۀ‬େֶγϯϙδ΢ϜߨԋʮILC ͷ෺ཧʯ:٢Ԭਸ਼थ೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɺ2013 ೥ 9 ݄ɺߴ஌େֶ

ILC ʹ͓͚Δ ILD ECAL ͷϋΠϒϦουߏ଄ͷ࠷దԽ:্໺ᠳ೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɺ2013 ೥ 9 ݄ɺߴ஌େֶ

ILC ࣮‫༻ݧ‬γϦίϯి࣓ΧϩϦϝʔλ technological prototype ͷੑೳධՁ;ਢ౻༟࢘೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɺ2013 ೥ 9 ݄ɺߴ஌େֶ

ILC ʹ͓͚Δి࣓ΧϩϦϝʔλͷͨΊͷγϦίϯ‫ݕ‬ग़‫ث‬ͷϨʔβʔΛ༻͍ͨಛੑ‫ڀݚ‬:
73

෋ాཾ඙
೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɺ2013 ೥ 9 ݄ɺߴ஌େֶ

ILC ʹ͓͚Δ Si-W ࡉ෼ׂి࣓ΧϩϦϝʔλࢼ࡞‫ػ‬ͷੑೳධՁ:‫࡚ٶ‬ཅฏ
೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɺ2013 ೥ 9 ݄ɺߴ஌େֶ
ૉཻࢠ͔ΒӉ஦Λ୳Δɹ–ώοάεཻࢠͱίϥΠμʔ࣮‫–ݧ‬઒ӽਗ਼ҎΫϥϒؔ੢ɹߨԋձɺ2014 ೥ 03 ݄ 13 ೔ૉཻࢠͱӉ஦ɿώοάεཻࢠͱ͸Կ͔઒ӽਗ਼Ҏֶߍ๏ਓদඌֶԂɹग़લत‫ۀ‬ɺ2013 ೥ 11 ݄ 08 ೔ɹɹૉཻࢠͰӉ஦ͷಾʹഭΔɹ– LHC ͱ ILC –઒ӽਗ਼Ҏ‫۝‬भେֶɹϗʔϜΧϛϯάσʔߨԋɺ2013 ೥ 10 ݄ 09 ೔ɹɹࠃࡍϦχΞίϥΠμʔʢILCʣ‫ܭ‬ըʹ͍ͭͯ઒ӽਗ਼Ҏ೔ຊٕज़࢜ձ‫۝‬भຊ෦ɹ‫ݚ‬मձߨԋɺ2013 ೥ 07 ݄ 27 ೔ɹӉ஦ͱ෺࣭ͷ‫ʹݯى‬ഭΔɿώοάεཻࢠͱࠃࡍϦχΞίϥΠμʔ઒ӽਗ਼ҎՊֶΛ‫ޠ‬Δձɹߨԋձɺ2013 ೥ 07 ݄ 13 ೔ɹࠃࡍϦχΞίϥΠμʔ‫ܭ‬ըͱ͸Կ͔઒ӽਗ਼Ҏ‫۝‬भ‫ࡁܦ‬࿈߹ձɹߨԋձɺ2013 ೥ 06 ݄ 11 ೔ɹɹɹώοάεཻࢠͱίϥΠμʔ઒ӽਗ਼Ҏ‫۝‬भେֶ෺ཧֶՊಉ૭ձɹߨԋɺ2013 ೥ 06 ݄ 06 ೔ɹ74ɹ෺࣭ɾӉ஦ͷ‫ʹݯى‬ഭΔ ILC ‫ܭ‬ը઒ӽਗ਼Ҏ෱Ԭࢢɾ‫۝‬भେֶɹ෱Ԭࢢࢢຽߨԋձɺ2013 ೥ 05 ݄ 22 ೔ɹࠃࡍϦχΞίϥΠμʔʹ͍ͭͯʢ‫͔ऀڀݚ‬Β઒ӽਗ਼Ҏ౔໦ֶձ੢෦ࢧ෦ɹ૯ձߨԋɺ2013 ೥ 04 ݄ 24 ೔ɹɹࠃࡍϦχΞίϥΠμʔͱ౎ࢢ‫ܭ‬ը઒ӽਗ਼Ҏ౎ࢢ‫ܭ‬ըֶձ‫۝‬भࢧ෦ɹߨԋձɺ2013 ೥ 04 ݄ 07 ೔
ɹɹJ-PARC ͰͷϛϡʔΦϯిࢠస‫ݧ࣮ࡧ୳׵‬ʢCOMET ࣮‫ݧ‬ʣʹ͓͚Δి࣓ΧϩϦϝʔλͷ։ൃ‫ ڀݚ‬:େੴߤ೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɺ2013 ೥ 9 ݄ɺߴ஌େֶ

J-PARC ͰͷϛϡʔΦϯిࢠస‫( ݧ࣮ࡧ୳׵‬COMET ࣮‫͚͓ ʹ )ݧ‬Δి࣓ΧϩϦϝʔλͷ։ൃ‫ ڀݚ‬:େੴߤୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձɺ2013 ೥ 11 ݄ɺ‫ཹٱ‬ถ޻‫ۀ‬େֶ

J-PARC ͰͷϛϡʔΦϯ-ిࢠస‫׵‬աఔ୳ࡧ࣮‫( ݧ‬COMET ࣮‫͚͓ʹ )ݧ‬Δ MPPC Λ༻͍ͨνΣϨϯίϑτϦΨʔ‫ݕ‬ग़‫ث‬ͷ։ൃ :த‫ډ‬༐थ
ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձɺ2013 ೥ 11 ݄ɺ‫ཹٱ‬ถ޻‫ۀ‬େֶ

J-PARC ͰͷϛϡʔΦϯ-ిࢠస‫׵‬աఔ୳ࡧ࣮‫ݧ‬ʢCOMET ࣮‫ݧ‬ʣʹ͓͚Δ MPPC Λ༻͍ͨνΣϨϯίϑτϦΨʔ‫ݕ‬ग़‫ث‬ͷ։ൃ :த‫ډ‬༐थ
೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ2014 ೥ 3 ݄ɺ౦ւେֶভೆΩϟϯύε

J-PARC ϛϡʔΦϯ g-2/EDM ࣮‫ݧ‬ɿγϦίϯετϦοϓ‫ݕ‬ग़‫༻ث‬ಡΈग़͠ճ࿏ͷཁ‫ٻ‬ੑೳ :‫ݹ‬Ӝ৽࢘

75

೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ2014 ೥ 3 ݄ɺ౦ւେֶভೆΩϟϯύε

J-PARC ϛϡʔΦϯ g-2/EDM ࣮‫ݧ‬ɿγϦίϯετϦοϓ‫ݕ‬ग़‫ ༻ث‬ASIC ͷੑೳධՁ :ௐᠳฏ೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ2014 ೥ 3 ݄ɺ౦ւେֶভೆΩϟϯύε

֎෦ࢿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚɺಛผਪਐ‫ڀݚ‬

ILC ͷͨΊͷ࠷ઌ୺ଌఆ‫ث‬ͷࠃࡍత৽ల։
‫ڀݚ‬෼୲ऀ ઒ӽਗ਼Ҏ (‫ڀݚ‬୅දऀ ౦๺େֶ ࢁຊ‫)ۉ‬จ෦লՊֶ‫ڀݚ‬අิॿۚɺ৽ֶज़ྖҬ‫ڀݚ‬ઌ୺Ճ଎‫ ث‬LHC ͕੾Γ୓͘ςϥεέʔϧͷૉཻࢠ෺ཧֶʙਅۭͱۭ࣌΁ͷ৽ͨͳ௅
ઓɿLHC Ͱͷൃ‫͕ݟ‬ಋ࣍͘ੈ୅ΤωϧΪʔϑϩϯςΟΞͷൃల‫ڀݚ‬෼୲ऀ ઒ӽਗ਼Ҏ (‫ڀݚ‬୅දऀ ౦‫ژ‬େֶ ۨ‫޾ٶ‬உ)จ෦লՊֶ‫ڀݚ‬අิॿۚɺಛผਪਐ‫ڀݚ‬࠷ߴ‫౓ڧ‬ϛϡʔΦϯϏʔϜʹΑΔϛϡʔΦϯɾϨϓτϯϑϨʔόʔඇอଘ୳ࡧͷ৽ల։‫ڀݚ‬෼୲ऀ ౦৓ॱ࣏ (‫ڀݚ‬୅දऀ େࡕେֶ ‫ٱ‬໺ྑ޹)จ෦Պֶল‫ڀݚ‬අิॿۚɺएख‫ ڀݚ‬B
௿ΤωϧΪʔதੑࢠࢄཚΛ༻͍ͨφϊϝʔτϧεέʔϧͰͷॏྗ‫ ٯ‬2 ৐ଇ‫ݧ࣮ূݕ‬‫ڀݚ‬୅දऀ ٢Ԭਸ਼थ จ෦লՊֶ‫ڀݚ‬අิॿۚҎ֎ͷ֎෦ࢿۚ ߴΤωϧΪʔՃ଎‫ߏػڀݚث‬ɿେֶ౳࿈‫ࢧܞ‬ԉࣄ‫ۀ‬‫۝‬भେֶ-KEK ͷ࿈‫ʹܞ‬ΑΔՃ଎‫ث‬Պֶͷਪਐɾ‫ܗ఺ڌڀݚ‬੒ͱएख‫ऀڀݚ‬ҭ੒ࣄ‫ۀ‬୅දऀ ઒ӽਗ਼Ҏֶ෦̐೥ੜଔ‫ڀݚۀ‬֯ ௚޾ɺॅా ‫׮‬थɺߴా लࠤɺాத ૱Ұɺ௕ᖒ ཌྷɺ௕ౡ ‫׮‬੐ɺฏҪ ‫׮‬ਓɿ(ࢦಋ76‫ڭ‬һɺ઒ӽਗ਼Ҏ)ɿϛϡʔΦϯͷण໋ଌఆम࢜࿦จ• ্໺ᠳɿ(ࢦಋ‫ڭ‬һɺ઒ӽਗ਼Ҏ)ɿࠃࡍϦχΞίϥΠμʔ‫ܭ‬ըʹ͓͚ΔϋΠϒϦουి࣓ΧϩϦϝʔλͷߏ଄࠷దԽʹ޲͚ͨ‫ڀݚ‬• େੴߤɿ(ࢦಋ‫ڭ‬һɺ౦৓ॱ࣏)ɿJ-PARC ʹ͓͚ΔϛϡʔΦϯిࢠస‫׵‬աఔ୳ࡧ࣮‫࣓ి༻ݧ‬ΧϩϦϝʔλͷ‫ڀݚ‬։ൃ• দຊ‫ޛ‬ɿ(ࢦಋ‫ڭ‬һɺ٢Ԭਸ਼थ)ɿ௿ΤωϧΪʔதੑࢠࢄཚΛ༻͍ͨφϊϝτεέʔϧͰͷॏྗ‫ ٯ‬2 ৐ଇͷ‫ূݕ‬• ‫࡚ٶ‬ཅฏɿ(ࢦಋ‫ڭ‬һɺ઒ӽਗ਼Ҏ)ɿILC ʹ͓͚Δ Si-W ࡉ෼ׂి࣓ΧϩϦϝʔλࢼ࡞‫ػ‬ͷੑೳ‫ڀݚ‬ֶ֎Ͱͷֶձ‫׆‬ಈ• ઒ӽ೔ຊ෺ཧֶձɿ୅ٞһߴΤωϧΪʔ෺ཧֶ‫ऀڀݚ‬ձٞɿߴΤωϧΪʔҕһձҕһߴΤωϧΪʔ෺ཧֶ‫ऀڀݚ‬ձٞɿILC ઓུձٞҕһߴΤωϧΪʔ෺ཧֶ‫ऀڀݚ‬ձٞɿILC ཱ஍ධՁձٞ‫ڞ‬ಉٞ௕ߴΤωϧΪʔՃ଎‫ߏػڀݚث‬ɿϦχΞίϥΠμʔ‫ܭ‬ըਪਐҕһձҕһߴΤωϧΪʔՃ଎‫ߏػڀݚث‬ɿେ‫ܕ‬γϛϡϨʔγϣϯ‫ܭ‬ըਪਐҕһձҕһߴΤωϧΪʔՃ଎‫ߏػڀݚث‬ɿ೔ถՊֶٕज़‫ߴۀࣄྗڠ‬ΤωϧΪʔ෺ཧ‫ڀݚ‬‫ܭ‬ըҕһձҕһ౦‫ژ‬େֶૉཻࢠ෺ཧࠃࡍ‫ڀݚ‬ηϯλʔɹ‫ڠڀݚ‬ٞձҕһ• ౦৓೔ຊ෺ཧֶձ‫۝‬भࢧ෦ҕһ• ٢Ԭ೔ຊ෺ཧֶձૉཻࢠ࣮‫ྖݧ‬ҬӡӦҕһ
೔ຊ෺ཧֶձ‫۝‬भࢧ෦ҕһ77ߴΤωϧΪʔχϡʔεฤूҕһडୗ‫ڀݚ‬ɾຽؒͱͷ‫ڞ‬ಉ‫ڀݚ‬• ߴΤωϧΪʔՃ଎‫͔ߏػڀݚث‬Βͷडୗ‫ڀݚ‬ʮࠃࡍϦχΞίϥΠμʔ‫ܭ‬ը(ILC) ࢪઃ‫ݐ‬ઃʹ܎Δ‫ݱ‬஍ௐࠪʯʢ୅දɿ઒ӽਗ਼Ҏʣ• ‫۝‬भେֶͱϑϥϯε CNRS/IN2P3 ͱͷ‫ڞ‬ಉ‫ڀݚ‬ʮి࣓ΧϩϦϝʔλͷͨΊͷγϦίϯηϯαʔͷ։ൃʯ(೔ຊଆ‫ڀݚ‬୅දऀ : ઒ӽਗ਼Ҏ)ͦͷଞͷ‫׆‬ಈͱ੒ՌҰൠ޲͚ߨԋ
ʮՃ଎‫ث‬ͷ͋Δ·ͪ - CERN ‫ࠃؼ‬ใࠂʯ :౦৓ ॱ࣏ࠃࡍϦχΞίϥΠμʔ (ILC) Ԡԉ‫ا‬ըɺ෱Ԭ‫ݝ‬෱Ԭࢢɺ2013 ೥ 4 ݄ʮࢲ͕ώοάεཻࢠΛ‫ͨ͠·͚ͭݟ‬ʯ:౦৓ ॱ࣏ࠤլେֶެ։ߨ࠲ʮώοάεཻࢠ͕‫͔ͨͬͭݟ‬ʂʯɺࠤլ‫ࠤݝ‬լࢢɺ2013 ೥ 7 ݄ʮૉཻࢠ෺ཧֶͷ࠷ઌ୺ʯ :౦৓ ॱ࣏দࢁதԝߴߍʮֶ෦ɾֶՊ‫ڀݚ‬ձ (େֶ໛ٖत‫)ۀ‬ʯɺѪඤ‫ݝ‬দࢁࢢɺ2013 ೥ 7 ݄
ʮCERN ͷ໨తͱ੒Ռ - ILC ༠கͷҙٛʹ͍ͭͯʯ౦৓ ॱ࣏෱Ԭࢢٞ CERN ࢹ࡯ஂɾࢹ࡯ใࠂձɺ෱Ԭ‫ݝ‬෱Ԭࢢɺ2013 ೥ 7 ݄ʮ࠷ઌ୺ͷૉཻࢠ෺ཧֶʯ :౦৓ ॱ࣏‫۝‬भେֶΦʔϓϯΩϟϯύεɺ෱Ԭ‫ݝ‬෱Ԭࢢɺ2013 ೥ 8 ݄78ཻࢠ෺ཧֶߨ࠲ (‫ݧ࣮֩ࢠݪ‬άϧʔϓ)‫ߏࣨڀݚ‬੒һ໺࿊఩෉ ‫ڭ‬तɹ৿ాߒհ ‫ڭ‬तए‫ڱ‬ஐ࢚ ।‫ڭ‬तࣉ੢ߴ ।‫ڭ‬त౻ా‫܇‬༟ ॿ‫ڭ‬ɹࡔ‫ޱ‬૱ࢤ ॿ‫ڭ‬લా๛࿨ ٕज़৬һ େֶӃ ത࢜՝ఔ ࢁ‫ޱ‬༞޾ େֶӃ म࢜՝ఔ େத‫ܙو‬

ၲ‫ۄ‬େี

੢ࢁ‫ݑ‬Ұ

෱Ӭ୓

લా༟࢙

҆ా३ฏ

‫ڇ‬ඌࠃ‫ٱ‬

Ӵ౻ཽҰ

ాඌ੒ষ

ߴඌल໌

੒ਗ਼ٛത

੢ඌ߁‫و‬

ᖛ‫݈ݩ‬Ұ

ྛ‫ܚ‬ଠɹ൐஧඙ɹ ֶ෦ ଔ‫ڀݚۀ‬ੜ ֲၭዉɹ‫ؒٱ‬େฏ

খౡ୓࿠ਐ౻༎ีాதହ‫و‬

ా୺৺ւ৽໊޹ࡈଇদ‫ګ‬জ

ࢁຊᠳ໵୲౰त‫ۀ‬
ྗֶ‫ૅج‬ɾಉԋश (໺࿊఩෉ɺࣉ੢ߴ)ɺίΞηϛφʔ (ए‫ڱ‬ஐ࢚)ɺ
গਓ਺ηϛφʔ (ࣉ੢ߴ)ɺి࣓‫( ֶؾ‬໺࿊఩෉)ɺࣗવՊֶ૯߹࣮‫ࣉ( ݧ‬੢ߴ)ɺ
෺ཧֶ࠷લઢ (ࣉ੢ߴ)ɺྗֶ (ए‫ڱ‬ஐ࢚)ɺి࣓‫ ֶؾ‬Iɾಉԋश (৿ాߒհ)ɺ
࠷ઌ୺෺ཧֶ (ࡔ‫ޱ‬૱ࢤ)ɺ‫֩ࢠݪ‬෺ཧֶ (໺࿊఩෉)ɺ
෺ཧֶ࣮‫ߒా৿( ݧ‬հɺ౻ా‫܇‬༟ɺࡔ‫ޱ‬૱ࢤɺए‫ڱ‬ஐ࢚ɺࣉ੢ߴ)ɺ
෺ཧֶθϛφʔϧ (৿ాߒհɺए‫ڱ‬ஐ࢚)ɺ‫֩ࢠݪ‬ɾߴΤωϧΪʔ࣮‫ߒా৿( ֶݧ‬հ)ɺ
‫( ݧ࣮֩ࢠݪ‬ए‫ڱ‬ஐ࢚)‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ
֩಺֩ࢠؒ૬‫༻࡞ޓ‬ͷ‫ڀݚ‬ͷͨΊͷதੑࢠεϐϯଌఆ‫ܥ‬ͷ։ൃ (҆ా३ฏɺए‫ڱ‬ஐ࢚)‫֩ࢠݪ‬ഔ࣭಺ʹ͓͍ͯɺ֩ࢠɾதؒࢠͷੑ࣭͕มԽ͢Δʮഔ࣭ޮՌʯ͕͋Δͷ͔൱͔͸‫֩ࢠݪ‬෺ཧʹ͓͍ͯ‫ڵ‬ຯਂ͍ςʔϚͰ͋Δɻഔ࣭ޮՌΛௐ΂Δ্Ͱɺ֩಺Ͱͷ֩ࢠ

79֩ࢠࢄཚʹରԠ͢Δ֩ࢠϊοΫΞ΢τ൓Ԡ͸༗ޮͰ͋Δɻզʑ͸ɺExclusive ͳ (p, n p)൓ԠͷੈքॳͷଌఆΛߦ͏͜ͱΛ໨ࢦ͍ͯ͠ΔɻͦͷͨΊʹɺ(1) தੑࢠภ‫౓ۃ‬ଌఆɺ(2)Exclusive ଌఆɺͷ 2 ͭͷཁૉΛ༗͢Δ (p, n p) ൓Ԡʹ͓͚Δภ‫ۃ‬Ҡߦྔଌఆ‫ܥ‬ͷ։ൃΛߦͬͨɻͦͷ݁Ռɺ6 Li ‫ ͼٴ‬12 C ྆ඪతʹରͯ͠ 1s ‫ي‬ಓͱ 1p ‫ي‬ಓͷ෼཭ʹ੒ޭ͠ɺඍ෼அ໘ੵ‫ͼٴ‬ภ‫ۃ‬෼ղೳͷऔಘʹ੒ޭͨ͠ɻ͞Βʹɺภ‫ۃ‬Ҡߦྔʹؔͯ͠΋ɺॴఆͷ࣌ؒͷଌఆΛߦ͏͜ͱͰഔ࣭ޮՌͷ‫ʹڀݚ‬ඞཁͳਫ਼౓͕ಘΒΕΔͱͷ݁࿦Λಘͨɻεϐϯภ‫ۃ‬ཅࢠʹΑΔෆ҆ఆ֩ͷ൓Ԡɾߏ଄‫ڀݚ‬ʢࡔ‫ޱ‬૱ࢤʣۙ೥ɺෆ҆ఆ֩ʹ͓͚Δςϯιϧྗɾεϐϯ‫ي‬ಓྗɾࡾମྗͳͲͷεϐϯґଘ૬‫࡞ޓ‬༻ͷಇ͖͕஫໨ΛूΊ͍ͯΔɻ͜ΕΒͷ૬‫༻࡞ޓ‬ͷ‫ݱ‬ΕΛௐ΂ΔͨΊɺෆ҆ఆ֩ϏʔϜ࣮‫༻ݧ‬ͷੈք།Ұͷภ‫ۃ‬ཅࢠඪతΛ༻͍ͯɺεϐϯࣗ༝౓Λ‫͔ͨ͠׆‬ෆ҆ఆ֩‫ڀݚ‬ΛਐΊ͍ͯΔɻຊ೥౓͸ಛʹɺཧ‫ ݚ‬RI ϏʔϜϑΝΫτϦʔʹ͓͍ͯʮ1. ཅࢠ஄ੑࢄཚ
࣮‫ݧ‬ʯ‫ͼٴ‬ʮ2. ཅࢠ‫ڞ‬໐ࢄཚ࣮‫ݧ‬ʯΛ਱ߦ͢ΔͨΊͷ४උΛूதతʹਐΊͨɻ·ͨɺ૷ஔ։ൃͷաఔʹ͓͚Δ෺ੑతͳ‫ڀݚ‬ʮ3. ๕߳଒ࡾॏ߲ภ‫ۃ‬աఔͷղ໌ʯ΋ਪਐͨ͠ɻ
ɹ̍ɽʮཅࢠ஄ੑࢄཚʯɹ஄ੑࢄཚʹ͓͚Δεϐϯ‫ي‬ಓ݁߹ͷऑԽʹܾؔͯ͠ఆతͳ݁
࿦ΛಘΔͨΊɺ൓Ԡཧ࿦ͷཱ֬͞ΕͨதߴΤωϧΪʔ 200MeV/A ʹ͓͚Δ p-6He ภ‫ۃ‬෼ղೳଌఆΛཧ‫ ݚ‬RIBF ʹͯ਱ߦ͢Δɻ͜ͷ໨తͷͨΊɺେ‫ܘޱ‬ͷภ‫ۃ‬ཅࢠඪతγεςϜΛߏங͠ɺैདྷͷ̒ഒ‫ڧ‬ɺੈք࠷େͷମੵΛ࣋ͭࢼྉΛภ‫ͤ͞ۃ‬Δ͜ͱʹ੒ޭ͠
ͨɻ·ͨɺภ‫౓ۃ‬ͷ޲্ͷͨΊͷϚΠΫϩ೾ճ࿏‫৽ͼٴ‬೾௕Ϩʔβʔͷ։ൃɺ͞Βʹɺߴ෼ղೳͷ൓௓ཅࢠ‫ݕ‬ग़‫ث‬΍ଟਊઢ‫ܕ‬υϦϑτνΣϯόʔ౳ɺ‫ݕ‬ग़‫ث‬ηοτΞοϓͷ
ߏஙΛਐΊ͍ͯΔɻɹ̎ɽʮཅࢠ‫ڞ‬໐ࢄཚʯɹཅࢠ‫ڞ‬໐ࢄཚ͸ɺཅࢠա৒֩ͷඇଋറঢ়ଶΛ‫͢ڀݚ‬ΔͨΊͷ‫ͳྗڧ‬ख๏Ͱ͋Δɻෆ҆ఆ֩ʕཅࢠ‫ڞ‬໐ࢄཚʹ͓͚Δॳͷภ‫ۃ‬෺ཧྔଌఆͱͯ͠୸ૉ
̕–ཅࢠࢄཚ࣮‫ݧ‬ͷϚγϯλΠϜ͕ೝΊΒΕͨ͜ͱΛड͚ɺ௿ΤωϧΪʔ୸ૉ̕ϏʔϜ։ൃ࣮‫ݧ‬ɺ‫ͼٴ‬ബບภ‫ۃ‬ཅࢠඪతͷ։ൃΛਐΊͨɻɹ̏ɽʮࡾॏ߲ภ‫ۃ‬աఔͷղ໌ʯɹඪతʹ༻͍͍ͯΔภ‫ݪۃ‬ཧ͸·ͩղ໌͞Ε͍ͯͳ͍෦෼΋ଟ͘ɺ෺ੑతʹ΋‫ڵ‬ຯ͕࣋ͨΕ͍ͯΔɻຊ೥౓͸ɺͦͷ಺ͷ๕߳଒෼ࢠྭ‫ى‬ঢ়ଶͷण໋‫ͼٴ‬εϐϯ֨ࢠ؇࿨ܾ࣌ؒఆͷͨΊͷղੳख๏ΛߟҊ͠ɺ݁ՌΛ౤ߘ࿦จͱ
ͯ͠·ͱΊ࢝Ί͍ͯΔɻ

(p, 2p) ൓ԠΛ༻͍ͨ Ca ͷཻ̍ࢠ‫౓ڧ‬෼෍ଌఆ (෱Ӭ୓ɺࡔ‫ޱ‬૱ࢤɺ໺࿊఩෉)ۙ೥ͷෆ҆ఆ֩෺ཧͷൃలʹΑͬͯɺதੑࢠա৒֩ͳͲ҆ఆྖҬ͔Β཭Εͨ‫֩ࢠݪ‬ͷ֪ߏ଄͕҆ఆྖҬͱ͸ҟͳ͍ͬͯΔ͜ͱ͕෼͔ͬͯདྷͨɻͦͷ֪ߏ଄มԽΛੜΈग़͢‫ݪ‬ҼͷҰͭͱͯ͠ɺେ௩ࢯఏএͷςϯιϧྗʹΑΔɺϞϊϙʔϧޮՌ͕͋Δɻ͜ͷޮՌ͕͋Δͱɺཅࢠͷ j> ‫ي‬ಓͱ j< ‫ي‬ಓͱͷΤωϧΪʔ͕ࠩɺಛఆͷ‫ي‬ಓͷதੑࢠ਺80ʹԠͯ͡มԽ͢Δɻ͜ͷޮՌͷ‫ʹূݕ‬͸ɺf7/2 ‫ي‬ಓͷதੑࢠ਺͕େ͖͘ҟͳΔ Ca ಉҐମͰཅࢠͷ d3/2 ‫ي‬ಓͱ d5/2 ‫ي‬ಓͷ (ฏ‫ )ۉ‬ΤωϧΪʔࠩͷมԽΛௐ΂Δ͜ͱ͕༗ޮͰ͋Δɻͦ͜Ͱɺ(p, 2p)
൓ԠΛ༻͍ͯ྆‫ي‬ಓͷ‫౓ڧ‬෼෍Λௐ΂ΔϓϩάϥϜΛ࢝Ί͍ͯΔɻ͜ͷଌఆͰ͸ɺ‫ݸ‬ʑͷ४ҐΛ෼཭ଌఆ͢ΔͨΊʹߴ෼ղೳ͕ཁ‫͞ٻ‬ΕΔͨΊɺ਺೥લ͔Β RCNP ͷ 2 ΞʔϜεϖΫτϩϝʔλ‫ܥ‬ͷߴ෼ղೳԽʹऔΓ૊Έɺࡢ೥౓·Ͱͷ։ൃͰ ΔE=160keV Λୡ੒ɺຊଌఆ࣮ࢪʹ໨ॲΛ͚ͭͨɻ͜ͷ݁Ռʹ‫ ͍ͯͮج‬2013 ೥ 5 ݄ʹ RCNP ʹ͓͍࣮ͯ‫ݧ‬Λߦͬͨɻ

RCNP ͷภ‫ۃ‬ΠΦϯ‫ݯ‬ͷෆௐͰϏʔϜͷ࣭ɾྔͱ΋ॆ෼Ͱ͸ͳ͔͕ͬͨɺ‫ݶ‬ΒΕͨσʔλ͔ΒɺEp = 200 MeV Ͱͷ (p, 2p) ൓Ԡ͕‫ي‬ಓͷಉఆͱཻ̍ࢠ‫౓ڧ‬ͷநग़ͷ‫ͳྗڠ‬खஈʹͳΔ͜ͱΛ֬ೝ͠ɺ͜Ε·Ͱ 1d3/2 Ͱ͋Δͱߟ͑ΒΕ͍ͯͨྖҬʹ 1d5/2 ‫͕౓ڧ‬ࠞࡏ͍ͯ͠Δ͜ͱΛ‫͍ͨͩ͠ݟ‬ɻ

pd ෼ղ൓Ԡʹ͓͚Δ Space Star ҟৗ (૬ྑ‫ࢸݐ‬ɺେத‫ܙو‬ɺલా༟࢙)p+d ˠ p+p+n ෼ղ൓Ԡ͔Βͷ 3 ֩ࢠ͕ɺ(a) ਖ਼ 3 ֯‫ܗ‬Λͳͯ͠ԕ͔͟Γɺ(b) ͦͷਖ਼ 3֯‫͕ܗ‬ϏʔϜ࣠ͱਨ௚ͱͳΔӡಈֶ৚݅Λ Space StarʢSSʣͱ‫Ϳݺ‬ɻ1989 ೥ʹ En = 13

MeV Ͱͷ̽+d ˠ̽+̽+p ൓Ԡͷ SS அ໘ੵ͕‫ ͳີݫ‬Faddeev ‫ࢉܭ‬஋ͱ໿ 30%߹Θͳ͍‫ݱ‬৅͕ใࠂ͞Ε SS anomaly ͱ‫ݺ‬͹Ε͍ͯΔɻ͔͠͠ɺ4 ൒ੈ‫ࠓͨͬܦل‬΋ SS anomalyͷ‫ݪ‬Ҽ͕ղ໌͞Ε͍ͯͳ͍ɻզʑ͸ɺߴ৴པ౓ͰଌఆͰ͖Δ p+d ˠ p+p+n ൓ԠͰ SS

anomaly Λ 1998 ೥͔Β‫ܥ‬౷తʹௐ΂ɺ15 ೥‫ޙ‬ͷࠓ೥౓Ͱ࣮‫ݧ‬Λ‫ͨྃ͠׬‬ɻࡢ೥౓·Ͱͷ࣮‫Ͱݧ‬ɺp+d ˠ p+p+n ͷҟৗ͸(a) ਖ਼ࡾ֯‫ܗ‬৚݅Ͱ࠷େʹͳΔɺ(b) ਨ௚৚݅Ͱ࠷େʹͳΔɺͱͷ݁ՌΛಘͨɻͭ·Γɺҟৗ͸ SS ৚݅Ͱ࠷େʹͳΔɺͱ൑໌ͨ͠ɻࠓ೥౓Ͱɺ(c)ΤωϧΪʔґଘੑͷௐࠪΛऴ͑ͨɻ݁Ռ͸ҎԼͷͱ͓Γɻ(c) p+d ˠ p+p+n ͷ SS ҟৗ͸ E(p-beam) = 7.5, 9.5, 13 MeV Ͱ໿ −8%ͰҰఆͰ͋Δɻ͜ΕΒ (a),(b),(c) ͷ SS anomaly ͷಛ࣭͔Βɺཧ࿦Ո͕ૣ‫ݪʹٸ‬ҼΛղ໌͢΂͖Ͱ͋Δɻ௒ॏ‫ݩ‬ૉͷ୳ࡧʢ੒ਗ਼ٛതɺ౻ా‫܇‬༟ɺ৿ాߒհʣ
ཧԽֶ‫ॴڀݚ‬ͷઢ‫ܗ‬Ճ଎‫( ث‬RILAC) ͔Βͷେ‫౓ڧ‬ॏΠΦϯϏʔϜΛ༻͍ɺ৽͍͠௒
ॏ‫ݩ‬ૉͷ୳ࡧ࣮‫ݧ‬Λߦ͍ͬͯΔɻࠓ೥౓͸ 12 ݄ʹ 248 Cmʢ‫ࢠݪ‬൪߸ 96ʣඪతʹ 48 Caʢ‫ࢠݪ‬൪߸ 20ʣϏʔϜΛরࣹ͠ɺ‫׬‬શ༥߹൓ԠʹΑͬͯ߹੒͞ΕΔ‫ࢠݪ‬൪߸ 116 ͷ Lv
ʢϦόϞϦ΢Ϝʣͷ߹੒࣮‫ݧ‬Λߦͬͨɻ͜ͷ൓Ԡ͸ϩγΞɺυ΢ϒφʹ͋ΔϑϨϩϑ֩81൓Ԡ‫ॴڀݚ‬ʢFLNRʣ΍ɺυΠπͷॏΠΦϯՊֶ‫ॴڀݚ‬ʢGSIʣͰ͢Ͱʹ‫ߦ͕ڀݚ‬ΘΕ͍ͯΔ͕ɺͦΕΒͷ࣮‫݁ݧ‬ՌΛ௥ೝ͢Δ݁ՌΛಘͨɻ߹੒͞Εͨ֩छ͸ 292 Lv ͓Αͼ
293

Lv Ͱ͋Δɻ‫ݕ‬ग़ޮ཰ʹ͓͍ͯ͸ੈք࠷ߴͷ஋Λಘͨɻ·ͨ‫ࡏݱ‬ղੳதͰ͋Δ͕ 292 Lv

ͷ α ่յνΣʔϯͷதʹࠓ·Ͱ͸֬ೝ͞Ε͍ͯͳ͔ͬͨɺ284 Cnʢί΃ϧχγ΢Ϝɺ‫ݪ‬
ࢠ൪߸ 112ʣͷ α ่յ͕‫؍‬ଌ͞Ε͍ͯΔՄೳੑ͕ߴ͍ɻ͞Βʹ͸ 284 Cn ͷ α ่յͷ່֩
Ͱ͋Δ 280 DsʢμʔϜελν΢Ϝɺ‫ࢠݪ‬൪߸ 110ʣ͸ະ஌ͷಉҐମͰ͋Γɺ৽֩छ͕ൃ
‫͞ݟ‬Ε͍ͯΔՄೳੑ͕ߴ͍ɻࠓ‫ޙ‬͸͜ͷ࣮‫ݧ‬ͷ͞ΒͳΔ௥ࢼΛߦ͏ͱͱ΋ʹ 50 Ti ϏʔϜʹΑΔ৽‫ݩ‬ૉ୳ࡧ࣮‫ݧ‬Λ‫ܭ‬ը͍ͯ͠Δɻ
̎தੑࢠ‫ڞ‬໐୳ࡧख๏ͷ։ൃ (૬ྑ‫ࢸݐ‬ɺେத‫ܙو‬ɺલా༟࢙)nn ؒ૬‫༻࡞ޓ‬͸௚઀࣮‫͍ͳ͖Ͱ͕ݧ‬ͷͰະ֬ఆͰ͋Δɻ2010 ʹ Witala ͱ Gloeckel
͕ɺnn ૬‫ ͕༻࡞ޓ‬8%ఔ౓‫ͳ͍ڧ‬Β nn-QFS ҟৗ͕આ໌Ͱ͖ɺnn ‫ڞ‬໐͕ଘࡏ͢ΔՄೳ
ੑ͕͋Δɺͱࢦఠͨ͠ɻͦ͜Ͱզʑ͸ nn ‫ڞ‬໐ͷଘ൱Λௐ΂ΔͨΊʹɺD(d,n)3 He Ͱੜ
੒͢Δ n-beam Λ༻͍ͯஅ໘ੵΛଌఆ͢ΔͨΊͷ४උ‫ڀݚ‬ΛਐΊͨɻ࣮‫্ݧ‬ͷ໰୊఺͸ɺD(n,p)nn ͔Βͷ p ͕ඍྔͳ͜ͱͱɺD(d,n)3 He ͔Βͷେྔͷ͕̽Si ‫ݕ‬ग़‫ʹث‬όοΫάϥϯυ (BG) Λੜͤ͡͞Δ͜ͱͰ͋Δɻલ೥౓ʹ͸ D ‫ؾ‬ମඪతΛվྑ͠ɺԖʴύϥϑΟϯःณͷޮՌͱ?E-E ‫ݕܕ‬ग़‫ث‬ͷੑೳΛௐ΂ͨɻࠓ೥౓͸ɺ(n,p)൓ԠΛ‫୸͍ͳ͜͞ى‬ૉͰ‫ݕ‬ग़‫ث‬ͷεϦοτͱγʔϧυΛ࡞Γɺ͔ͭ̽ःณޮՌେͷమΛ
࠷େ 40cm ް͞ (૯ॏྔ 200kg) ʹ഑ஔͯ͠‫ݕ‬ग़‫ث‬Λ෴ͬͨɻͦͷ݁Ռɺ̽‫ى‬Ҽͷ̿-BG
͸ D(n,p)nn ͔Βͷ p ༧૝ྔͱಉఔ౓ʹͳͬͨɻຊ‫Ͱڀݚ‬ɺD(n,p)nn ͷ nn ‫ڞ‬໐୳ࡧํ๏ͷΊͲ͕͍ͭͨɻ‫ݕ‬ग़‫ث‬ΛΨεʴ Si ʹ͢Ε͹ɺຊଌఆ͕ߦ͑ΔͩΖ͏ɻɹϏʔϜΛύϧεԽͯ͠ඈߦ࣌ؒࠩ΋ଌఆ͢Ε͹͞Βʹ BG ͕‫ݮ‬ΒͤΔɻ
ఱମϔϦ΢Ϝ-୸ૉ֩༥߹൓Ԡ଎౓ͷଌఆ (౻ా‫܇‬༟ɺ ࢁ‫ޱ‬༞޾ɺ ాඌ੒ষɺ ੒ਗ਼ٛതɺ ᖛ‫݈ݩ‬Ұɺ ൐஧඙ɺ ૬ྑ‫)ࢸݐ‬ϔϦ΢Ϝ೩ম‫ظ‬ͷ߃੕Ͱ‫͜ى‬Δఱମ֩൓Ԡ 12 C+4 He→16 O+γ ͷશஅ໘ੵଌఆʹ͓͍ͯɺ൓ԠΤωϧΪʔ Ecm = 1.2 MeV Ͱͷσʔλऔಘʹ੒ޭͨ͠ɻ͜Ε͸ 16 O Λ௚઀ଌ
ఆ͢Δํ๏Ͱ͸ੈքॳͷσʔλͰ͋Δɻࡢ೥·Ͱʹ 16 O ͷόοΫάϥ΢ϯυ͕ඪతʹ෇ணͨ͠ࢎԽൽບ͔Βൃੜ͍ͯ͠ΔࣄΛಥ͖ࢭΊΒΕ͍ͯͨͷͰɺͦͷରࡦΛߦͬͨɻඪత༰‫ث‬ͷ಺‫ܘ‬Λ޿͛ɺඪత্ྲྀͷ 2ΧॴʹεϦοτΛઃஔ͢ΔࣄͰϏʔϜ͕༰‫ث‬ͷࢎԽൽບʹ৮Εͳ͍༷ͳϏʔϜ௨͠ΛՄೳͱͨ͠ɻͦͷଞͷ൓Ԡੜ੒ 16 O ͱಉ͡ΤωϧΪʔΛ࣋ͭ 12 C όοΫάϥ΢ϯυ͸
։ൃͨ͠ΠΦϯνΣϯόʔ (E–ΔE Χ΢ϯλ) Λ༻ཻ͍ͯࢠࣝผΛߦ͍ɺআ‫͢ڈ‬Δࣄ͕ग़དྷͨɻ

Ecm = 1.0 MeV ҎԼͰͷଌఆͷͨΊʹ Recoil Mass Separator ͷཱମ֯ΞΫηϓλϯ
82εͷ֦େΛߦͬͨɻQ2, Q4 ࣓ੴΛେ‫ܘޱ‬ͷ෺ʹަ‫͠׵‬ɺElectric Deﬂector ͷ‫ۃ‬൘‫཭ڑ‬Λ޿͛Δվ଄Λߦͬͨɻproton ͷϖϯγϧϏʔϜΛ༻͍ͯଌఆ͠ɺϏʔϜ࣠ʹର্ͯ͠Լɺࠨӈ‫ ʹڞ‬±2 ౓Ҏ্ͷΞΫηϓλϯε͕͋ΔࣄΛ֬ೝͨ͠ɻ
௕‫ظ‬ଌఆͷͨΊͷ He Ψε॥‫ܥ؀‬΋։ൃ͕‫ྃ͠׬‬ɺਖ਼ৗʹಈ࡞͍ͯ͠ΔࣄΛ֬ೝͨ͠ɻ
Ψεඪతʹ࢖༻ͨ͠ He ͷ 95%͸ϙϯϓͰճऩ͞Εͨ‫ޙ‬ɺΫϥΠΦྫྷౚ‫ྫྷͰػ‬٫͞Εͨ೤ަ‫ث׵‬΍ϑΟϧλʔΛ௨ͬͯෆ७෺͕औΓআ͔ΕɺϦβʔόλϯΫʹஷଂ͞Εඪతʹ࠶ར༻͞ΕΔɻ12 C ϏʔϜͱඪతͱͷ஄ੑࢄཚΛଌఆ͠ɺෆ७෺ͷࠞ߹ׂ߹͕ 0.1%Ҏ
ԼͰ༗Δࣄ͕֬ೝ͞Εͨɻ࣍೥౓ͷλϯσϜγϟοτμ΢ϯ·Ͱʹ TOF ‫ݕ‬ग़‫ث‬ͷ։ൃΛߦ͍ɺEcm = 1.0 MeVͰͷஅ໘ੵଌఆΛ‫ͤྃ͞׬‬Δ༧ఆͰ͋Δɻ
௿ΤωϧΪʔෆ҆ఆ֩ϏʔϜʹΑΔෆ҆ఆ֩ͷ‫ࣉ( ڀݚ‬੢ߴ)

RI ϏʔϜΛ༻͍ͯෆ҆ఆ֩ͷ‫ڞ‬໐४ҐΛ୳ࡧ͠ɺෆ҆ఆ֩ͷߏ଄΍ෆ҆ఆ͕֩ؔ༩͢
Δఱମ֩൓Ԡʹ͍ͭͯͷ஌‫ݟ‬ΛಘΔ͜ͱΛ໨ඪʹ͍ͯ͠Δɻຊ೥౓͸࣮‫ݧ‬σʔλ͕΄ͱΜͲͳ͍ཅࢠඇଋറ֩ 10 N ͷϨϕϧΛௐ΂ΔͨΊɺ௿ΤωϧΪʔ 9 C ϏʔϜͱภ‫ۃ‬ཅࢠඪతΛ༻͍ͨ 9 C+p ‫ڞ‬໐஄ੑࢄཚͷଌఆ‫ܭ‬ըΛ RIBF PAC ʹఏҊ͠ɺςετϚγ
ϯλΠϜΛऔಘͨ͠ɻདྷ೥౓Ҏ߱ʹςετ࣮‫ݧ‬Λ࣮ࢪ͢Δ༧ఆͰ͋Δɻ

RFɾՙిަ‫׵‬ΠΦϯ‫ݯ‬ͷ։ൃ (ྛ‫ܚ‬େɺ‫ڇ‬ඌࠃ‫ٱ‬ɺࣉ੢ߴ)খ‫ن‬໛ɾ௿ίετͷ RI ϏʔϜੜ੒๏ͱͯ͠ɺण໋͕਺෼Ҏ্ͷதɾ௕ण໋ෆ҆ఆ֩ͷ̎࣍ΠΦϯΛΨε෼ࢠͷ‫Ͱܗ‬ΠΦϯ‫ʹݯ‬஫ೖ͠ɺෛΠΦϯͱͯ͠Ҿ͖ग़͠ɺλϯσϜՃ଎‫ʹث‬ΑΓՃ଎͢Δͱ͍͏ख๏ͷ։ൃΛ໨ࢦ͍ͯ͠Δɻຊ೥౓͸ɺকདྷͷ 11 C ΍ 14 CϏʔϜੜ੒Λ೦಄ʹஔ͖ɺ୸ૉΛ‫ؚ‬ΜͩΨε෼ࢠͰ͋Δඇ์ࣹੑ CO2 Λ RFɾՙిަ‫׵‬ΠΦϯ‫΁ݯ‬஫ೖ͠ɺ୸ૉϏʔϜΛҾ͖ग़͢ςετΛߦͬͨɻࠓ‫ޙ‬ɺӡస৚݅ͷ࠷దԽΛߦ͍ɺଞͷΨεΛ༻͍ͨςετ΋ߦ͏༧ఆͰ͋ΔɻՃ଎‫ྔ࣭ث‬෼ੳͷ։ൃͱར༻ (੢ࢁ‫ݑ‬ҰɺӴ౻ཽҰɺߴඌल໌ɺ໺࿊఩෉ɺࡔ‫ޱ‬૱ࢤ)‫۝‬େͷλϯσϜՃ଎‫ث‬Λ༻͍ͨՃ଎‫ྔ࣭ث‬෼ੳγεςϜͷ࣮༻ԽͷͨΊɺΠΦϯ‫ݯ‬ɺϏʔϜ༌ૹ‫ܥ‬ɺ‫ݕ‬ग़‫ܥث‬ͷվྑΛߦ͍ͬͯΔɻཧ‫ܥ‬ͷΩϟϯύεҠస͕ 2015 ೥౓ʹܾఆ͠ɺͦΕʹ൐ͬͯശ࡚λϯσϜՃ଎‫ ͕ث‬2014 ೥຤ʹγϟοτμ΢ϯ͞ΕΔ͜ͱʹͳͬͨͨΊɺҏ౎ΩϟϯύεͰͷ࣮‫ݱ‬Λ‫ݟ‬ਾ͑ͨ։ൃ‫׆‬ಈΛߦͬͨɻϏʔϜ༌ૹ‫ܥ‬ͷ։ൃͱͯ͠͸ɺՃ଎‫ͱྲ্ྀث‬ԼྲྀͷϏʔϜΤϛολϯεΛଌఆɺͦͷൺֱ͔ΒɺՃ଎‫ث‬ετϦούʔບͰΤϛολϯε૿େ͕͋Δ͜ͱΛ֬ೝͨ͠ɻ
·ͨɺϚϧνΞϊʔυΠΦϯνΣϯόʔʹ͍ͭͯ͸ɺ࣮ࡍʹ 13 C ཻࢠͱ 14 C ཻࢠͷ‫ݕ‬ग़৴߸Λൺֱ͠ɺσʔλॲཧʹΑͬͯ෼཭౓ 85 ՄೳͰ͋Δͱͷ݁ՌΛಘͨɻͦΕͱಉ83࣌ʹɺి‫ؾ‬తόοΫάϥ΢ϯυʹΑͬͯ෼ղೳ͕ѱԽ͍ͯ͠Δ͜ͱ͕֬ೝ͞ΕͨͨΊɺGEM(Ψεిࢠ૿෯ບ) Λૠೖͯ͠ए‫ׯ‬ͷΨε૿෯Λߦ͏͜ͱΛ‫ݕ‬౼͍ͯ͠ΔɻՃ଎‫ث‬ɾϏʔϜԠ༻ՊֶηϯλʔͰͷλϯσϜՃ଎‫ࢪث‬ઃͷ‫ݐ‬ઃ (ࣉ੢ߴɺ໺࿊఩෉)‫ࡏݱ‬ɺҏ౎ΩϟϯύεͷՃ଎‫ث‬ɾϏʔϜԠ༻Պֶηϯλʔ (ҎԼɺՃ଎‫ث‬ηϯλʔʣʹ
͓͍ͯɺ8 MV λϯσϜՃ଎‫ث‬ͷઃஔΛਐΊ͍ͯΔɻຊՃ଎‫ث‬ͷओཁ‫ثػ‬͸ɺ‫౎ژ‬େֶཧֶ෦͔Β‫۝‬भେֶ΁ 2012 ೥౓ʹҠઃ͞Εͨ΋ͷͰ͋ΓɺՃ଎‫ث‬λϯΫɺSF6 ΨεɾϦβʔόʔλϯΫɺ੍‫ܥޚ‬ɺΠΦϯ‫ݯ‬ɺϏʔϜϥΠϯͷҰ෦ͳͲҠઃ͕ࠔ೉ͳ΋ͷ΍࿝‫ٺ‬Խͨ͠΋ͷ͸‫۝‬भେֶͰߋ৽ͭͭ͋͠Δɻ2013 ೥౓͸ 6 ݄͔Β೥౓຤·ͰɺλϯσϜՃ଎‫ث‬ɾ࣮‫ݧ‬౩ (ҎԼɺ৽౩) ͷ‫ݐ‬ઃ͕Ճ଎‫ث‬ηϯλʔͷ FFAG Ճ଎‫ث‬౩ͷྡʹ૿ઃ͢Δ‫ߦͰܗ‬ΘΕͨɻ͜ͷ৽౩͸ɺ2012 ೥౓ʹλϯσϜՃ଎‫ث‬ઃஔ࡞‫ۀ‬ͷͨΊʹԾઃ͞ΕͨϓϨϋϒ౩ΛऔΓғΈͳ͕Β‫ݐ‬ઃ͞Εɺ৽౩‫׬‬੒‫ʹޙ‬ϓϨϋϒ౩ͷนͱ԰͕ࠜऔ
Γআ͔ΕͨɻҰํɺՃ଎‫ث‬ௐ੔࡞‫ۀ‬͸৽౩‫ݐ‬ઃલͷ 4 ݄ͱ 5 ݄ͷΈʹߦΘΕɺ͜Ε·ͰʹɺՃ଎‫ث‬λϯΫͷਅۭςετ͓Αͼ‫ס‬૩ѹॖۭ‫ʹؾ‬ΑΔՃѹςετ͕‫ྃ͠׬‬ɺ·੍ͨ‫ܥޚ‬ςετͷҰ෦͕ߦΘΕͨɻ2014 ೥ 4 ݄͔ΒՃ଎‫ث‬ௐ੔࡞‫࠶͕ۀ‬։͞Εɺ2014೥౓಺ʹ࠷ॳͷϏʔϜՃ଎͕ߦΘΕΔ༧ఆͰ͋Δɻൃද࿦จ ‫ݪ‬ஶ࿦จ 
Extraction of anti-analog giant dipole resonance and neutron skin thickness for 208 Pb
J. Yasuda, T. Wakasa, M. Okamoto, M. Dozono, K. Hatanaka, M. Ichimura, S. Kuroita,
Y. Maeda, T. Noro, Y. Sakemi, M. Sasano, and K. Yako
Prog. Theor. Exp. Phys. 063D02 (2013).
Observation of Low- and High-Energy Gamow-Teller Phonon Excitations in Nuclei
Y. Fujita, H. Fujita, T. Adachi, C.L. Bai, A. Algora, G.P.A. Berg, P.von Brentano,
G. Colo, M. Csatlos, J.M. Deaven, E.Estevez Aguado, C. Fransen, D.De Frenne,
K. Fujita, E. Ganioglu, C.J. Guess, J. Gulyas, K. Hatanaka, K. Hirota, M. Honma,
D. Ishikawa, E. Jacobs, A. Krasznahorkay, H. Matsubara, K. Matsuyanagi, R. Meharchand, F. Molina, K. Muto, K. Nakanishi, A. Negret, H. Okamura, H.J. Ong, T. Otsuka,
N. Pietralla, G. Perdikakis, L. Popescu, B. Rubio, H. Sagawa, P. Sarriguren, C. Scholl,Y. Shimbara, Y. Shimizu, G. Susoy, T. Suzuki, Y. Tameshige, A. Tamii, J.H. Thies,84M. Uchida, T. Wakasa, M. Yosoi, R.G.T. Zegers, K.O. Zell, and J. Zenihiro
Phys. Rev. Lett. 112, 112502 (2014).
Proton polarization in photo-excited aromatic molecule at room temperature enhanced
by intense optical source and temperature control:
S. Sakaguchi, T. Uesaka, T. Kawahara, T. Ogawa, L. Tang, T. Teranishi, Y. Urata, S.
Wada, and T. Wakui
Nuclear Instruments and Methods in Physics Research B 317 (2013) 679?684.
Investigation of the thermonuclear 18 Ne(α,p)21 Na reaction rate via resonant elastic
scattering of 21 Na + p:
L.Y. Zhang, J.J. He, A. Parikh, S.W. Xu, H. Yamaguchi, D. Kahl, S. Kubono, P. Mohr,J. Hu, P. Ma, S. Z. Chen, Y. Wakabayashi, H.W. Wang, W.D. Tian, R.F. Chen,
B. Guo, T. Hashimoto, Y. Togano, S. Hayakawa, T. Teranishi, N. Iwasa, T. Yamada,T. Komatsubara, Y. H. Zhang, and X. H. Zhou,
Physical Review C 89 (2014) 015804.
Low-energy radioactive ion beam production of 22 Mg:
N.N. Duy, S. Kubono, H. Yamaguchi, D. Kahl, Y. Wakabayashi, T. Teranishi, N. Iwasa,
Y.K. Kwon, L.H. Khiem, Y.H. Kim, J.S. Song, J. Hu, Y. Ayyad,
Nucl. Instrum. Methods Phys. Res. A723 (2013) 99.
The 18 Ne(α,p)21 Na breakout reaction in x-ray bursts: Experimental determination of
spin-parities for α resonances in 22 Mg via resonant elastic scattering of 21 Na+p:
J.J. He, L.Y. Zhang, A. Parikh, S.W. Xu, H. Yamaguchi, D. Kahl, S. Kubono, J. Hu,
P. Ma, S.Z. Chen, Y. Wakabayashi, B.H. Sun, H.W. Wang, W.D. Tian, R.F. Chen,
B. Guo, T. Hashimoto, Y. Togano, S. Hayakawa, T. Teranishi, N. Iwasa, T. Yamada,T. Komatsubara,
Physical Review C 88 (2013) 012801.
Resonant scattering of 22 Na+p studied by the thick-target inverse-kinematic method:
S.J. Jin, Y.B. Wang, J. Su, S.Q. Yan, Y.J. Li, B. Guo, Z.H. Li, S. Zeng, G. Lian,
X.X. Bai, W.P. Liu, H. Yamaguchi, S. Kubono, J. Hu, D. Kahl, H.S. Jung, J.Y. Moon,
C.S. Lee, T. Teranishi, H.W. Wang, H. Ishiyama, N. Iwasa, T. Komatsubara,
B.A. Brown,
85Physical Review C 88 (2013) 035801.

Proceedings
Decomposing spin-dipole resonances by complete polarization transfer measurements:
T. Wakasa, M. Okamoto, M. Dozono, K. Hatanaka, M. Ichimura, S. Kuroita, Y. Maeda,
H. Miyasako, T. Noro, T. Saito, Y. Sakemi, T. Yabe, and K. Yako
AIP Conf. Proc. 1524, 46 (2013).
Resonance scattering experiments with radioactive nuclear beams - Recent results andfuture plans:
T. Teranishi, S. Sakaguchi, T. Uesaka et al.,AIP Conf. Proc. 1525 (2013) 552–557.
Search for Perpendicular Plane Anomaly in pd breakup at Ep = 13 MeV:
S. Kimura, K. Sagara, K. Ishibashi, S. Tanaka, Y. Maeda, and K. Ohnaka
Few-Body Systems Vol. 54 #7-10 (2013) 1293-1296.
Measurement of 4 He(12 C,16 O) Ѝ in inverse kinematics:
K. Fujita, K. Sagara, T. Teranishi, M. Iwasaki, D. Kodama, S. Liu, S. Matsuda, T.
Mitsuzumi, J. Y. Moon, M. T. Rosary, and H. Yamaguchi
Few-Body Systems Vol. 54 #7-10 (2013) 1603-1606.

ߨԋ ւ֎Ͱͷߨԋ 
Study of anti-analog giant dipole resonance in 208 Pb(p, n) and neutron skin thicknessfor 208 Pb:
J. Yasuda, T. Wakasa, M. Okamoto, M. Dozono, K. Hatanaka, M. Ichimura, S. Kuroita,
Y. Maeda, T. Noro, Y. Sakemi, M. Sasano, and K. Yako
International Nuclear Physics Conference (INPC2013), June 2013, Florence, Italy(p, pN ) studies with spin measurements at intermediate energies:
T. Noro86

2nd International Workshop on Quasi-Free Scattering with Radioactive-Ion Beams(QFS-RB13), Sep. 2013, Terceira, Portugal)
Study of Unstable Nuclei with Spin-polarized Protons:
S. Sakaguchi
Nuclear Physics Seminar, Institute for Basic Science, Daejeon, Korea, 19 Feb., 2014.
Study of Unstable Nuclei with Spin-polarized Protons:
S. Sakaguchi
Nuclear Physics Seminar, Kyungpook National University, Daegue, Korea, 17 Feb.,
2014.
Recent Results on Superheavy Element Research at RIKEN:
K. Morita
International conference FUSION14, February 2014, New Delhi, India
Recent Few-Nucleon Experiments and Discrepancies to be solved:
K. Sagara (invited)
The 22nd European Conference on Few Body Problems in Physics, Krakow Poland,
2013.9.9-13.
Feasibility study of nn-resonance state search using 2H(n,p)nn reaction at En=12 MeV:
Y. Maeda, K. Sagara, K. Ohnaka, K. Ishibashi, S. Tanaka, S. Kimura, S. Kuroita
The 22nd European Conference on Few Body Problems in Physics, Krakow Poland,
2013.9.9-13.
Systematic measurement of pd breakup cross section around Space Star:
K. Ohnaka, K. Sagara, Y. Maeda, K. Ishibashi, S. Kimura, S. Tanaka, T. Fukunaga,
J. Yasuda, T. Yabe, K. Yashima, Y. Eguchi, H. Shimoda, T.Sueta, S. Kuroita
The 22nd European Conference on Few Body Problems in Physics, Krakow Poland,
2013.9.9-13.
Direct Measurement of 4He (12C, 16O) Ѝ cross section with RMS at TUTL:
K. Sagara
Workshop in Caserta Direct measurements in Nuclear Astrophysics with Recoil Mass87

separators, 2014.10.04-05, Caserta, Italy.

 ࠃ಺Ͱͷߨԋ 
Anti-analog giant dipole resonance and neutron skin thickness in 208 Pb:
J. Yasuda, T. Wakasa, M. Okamoto, M. Dozono, K. Hatanaka, M. Ichimura, S. Kuroita,
Y. Maeda, T. Noro, Y. Sakemi, M. Sasano, and K. YakoTHe 12th Asia Paciﬁc Physics Conference (APPC12), July 2013, Tokyo, Japan
Superheavy Element Research at RIKEN:
K. Morita
The 12th Asia Paciﬁc Physics Conference (APPC12), July 2013, Chiba, Japan
Ecm=1.2MeV ҎԼͰͷ 4 He(12 C,16 O) Ѝ൓Ԡͷ௚઀ଌఆ:౻ా‫܇‬༟ɼ૬ྑ‫ࢸݐ‬ɼࣉ੢ߴɼࢁ‫ޱ‬༞޾ɼၲ‫ۄ‬େีɼ੒ਗ਼ٛതɼాඌ੒ষɼᖛ‫݈ݩ‬Ұɼ൐஧඙೔ຊ෺ཧֶձ
৽ൃ‫ݟ‬ͷ 113 ൪‫ݩ‬ૉʖ‫ݱ‬୅ͷ࿉ۚज़ʖɿ৿ాߒհཧԽֶ‫ॴڀݚ‬Ұൠެ։ಛผߨԋɺཧԽֶ‫ॴڀݚ‬ɺ4 ݄ (2013).

113 ൪৽‫ݩ‬ૉͷ୳ࡧɿ৿ాߒհۙະདྷ΁ͷট଴ঢ়ʢՊֶٕज़ɾֶज़੓ࡦ‫ॴڀݚ‬ओ࠵ߨԋձʣɺจ෦Պֶলɺ5 ݄ (2013).
৽‫ݩ‬ૉͷ୳ࡧʖ‫ݱ‬୅ͷ࿉ۚज़ʖɿ৿ాߒհཧԽֶ‫ॴڀݚ‬Պֶߨԋձɺ౦‫ژ‬ɺ10 ݄ (2013)ɽ
৽‫ݩ‬ૉͷ୳ࡧʖ‫ݱ‬୅ͷ࿉ۚज़ʖɿ৿ాߒհཧԽֶ‫ॴڀݚ‬Պֶߨԋձɺௗ੘ɺௗ੘தֶߍɺ߳ೇதֶߍɺௗ੘ߴ౳ֶߍɺ11 ݄ (2013)ɽ
৽‫ݩ‬ૉͷ୳ࡧʖ‫ݱ‬୅ͷ࿉ۚज़ʖ
ɿ

88

৿ాߒհ
౦‫ژ‬େֶ෺ཧ‫ࣨڭ‬ίϩΩ΢Ϝɺ౦‫ژ‬ɺ12 ݄ (2013)ɽ
৽‫ݩ‬ૉͷ୳ࡧʖ‫ݱ‬୅ͷ࿉ۚज़ʖɿ৿ాߒհߨԋձɺࡔ‫ߍߴށ‬ɺ࡛‫ۄ‬ɺ12 ݄ (2013)ɽ
৽‫ݩ‬ૉͷ୳ࡧʖ‫ݱ‬୅ͷ࿉ۚज़ʖɿ৿ాߒհ෱Ԭ޻‫ۀ‬େֶ౔༵ஊ࿩ձɺ෱Ԭɺ12 ݄ (2013)ɽ
৽‫ݩ‬ૉͷ୳ࡧʖ‫ݱ‬୅ͷ࿉ۚज़ʖɿ৿ాߒհ೔ຊԽֶձࢢຽߨ࠲ɺ໊‫ݹ‬԰େֶɺ3 ݄ (2014)ɽ
ཅࢠ஄ੑࢄཚͷΞΠιεϐϯۭؒ΁ͷ֦ுͰ୳ΔதੑࢠεΩϯްͱঢ়ଶํఔࣜ:ࡔ‫ޱ‬૱ࢤ
‫۝‬େ෼໺ԣஅ‫ڀݚܕ‬ձ –ΫΥʔΫɾ‫֩ࢠݪ‬ɾதੑࢠ੕Λ၆ᛌ͢Δ–ɺ‫۝‬भେֶɺ3 ݄ (2014).

Preparation status of SAMURAI13 experiment:
S. Sakaguchi
SAMURAI International Workshop, Tokyo Institute of Technology, Tokyo, Japan, 9Sept., 2013.
λϯσϜՃ଎‫͚͓ʹث‬Δ RF ՙిަ‫ܕ׵‬ΠΦϯ‫ݯ‬ͷ։ൃɿྛ‫ܚ‬େɺࣉ੢ߴɺ‫ڇ‬ඌࠃ‫ٱ‬ɺଇদ‫ګ‬জୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ,2013 ೥ 11 ݄ 30 ೔, ‫ཹٱ‬ถ޻‫ۀ‬େֶ‫۝‬भେֶλϯσϜΛ༻͍ͨ AMS ଌఆͷ։ൃɿӴ౻ཽҰୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ,2013 ೥ 11 ݄ 30 ೔, ‫ཹٱ‬ถ޻‫ۀ‬େֶՃ଎‫ث‬஌Δ௒෼ੳͷͨΊͷϚϧνΞϊʔυΠΦϯνΣϯόͷ։ൃɿ੢ࢁ‫ݑ‬ҰɺӴ౻ཽҰɺখౡ୓࿠ɺ৽໊޹ࡈ
ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ,2013 ೥ 11 ݄ 30 ೔, ‫ཹٱ‬ถ޻‫ۀ‬େֶ

89ఱମ֩൓Ԡ 12C ʴЋˠ 16O ʴЍͷ Ecm=1.2MeV ʹ͓͚Δશ൓Ԡஅ໘ੵଌఆ:൐஧඙, ૬ྑ‫ࢸݐ‬, ౻ా‫܇‬༟, ࢁ‫ޱ‬༞޾, ၲ‫ۄ‬େี, ੒ਗ਼ٛത, ᖛ‫݈ݩ‬Ұ, ాඌ੒ষ, ‫ؒٱ‬ଠฏ, ɹֲၭዉ
ୈ 119 ճ೔ຊ෺ཧֶք‫۝‬भࢧ෦ྫձɺ‫ཹٱ‬ถ޻‫ۀ‬େֶɹ 2013 ೥ 11 ݄ 30 ೔

Ecm=1MeV ҎԼͰͷ 4He(12C,16O) ЍଌఆͷͨΊͷ൓௓࣭ྔ෼ੳ‫ث‬վ଄:ాඌ੒ষ, ࢁ‫ޱ‬༞޾, ౻ా‫܇‬༟, ૬ྑ‫ࢸݐ‬, ၲ‫ۄ‬େี, ੒ਗ਼ٛത, ᖛ‫݈ݩ‬Ұୈ 119 ճ೔ຊ෺ཧֶք‫۝‬भࢧ෦ྫձɺ‫ཹٱ‬ถ޻‫ۀ‬େֶɹ 2013 ೥ 11 ݄ 30 ೔̳̿෼ղ൓Ԡʹ͓͚Δ Star Anomaly ͷ‫ܥ‬౷తଌఆ:େத‫و‬ዳɺ૬ྑ‫ࢸݐ‬, લా༟࢙, ੴ‫ڮ‬࿨‫ٱ‬, ໦ଜॣଠ࿠, ాதᠳ‫ج‬, ෱Ӭ୓ɺ҆ా३ฏɺ໼
෦ୡ໵ɺീౢ‫ܙ‬հɺࠇ൘ᠳ
ୈ 119 ճ೔ຊ෺ཧֶք‫۝‬भࢧ෦ྫձɺ‫ཹٱ‬ถ޻‫ۀ‬େֶɹ 2013 ೥ 11 ݄ 30 ೔

nn ෼ղ൓ԠΛ༻͍ͨ nn ‫ڞ‬໐ঢ়ଶ୳ࡧͷͨΊͷ࣮‫ݧ‬ख๏ʹؔ͢Δ‫ڀݚ‬:લా༟࢙, ૬ྑ‫ࢸݐ‬, େத‫و‬ዳɺੴ‫ڮ‬࿨‫ٱ‬, ໦ଜॣଠ࿠, ాதᠳ‫ج‬, ࠇ൘ᠳୈ 119 ճ೔ຊ෺ཧֶք‫۝‬भࢧ෦ྫձɺ‫ཹٱ‬ถ޻‫ۀ‬େֶɹ 2013 ೥ 11 ݄ 30 ೔֎෦ࢿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ ‫ج‬൫‫( ڀݚ‬B) ʮఱମΤωϧΪʔʹ͓͚Δ୸ૉʖϔϦ΢Ϝ༥߹൓Ԡશஅ໘ੵͷ௚઀ଌఆʯ
ʢ૬ྑ‫ࢸݐ‬ɹ 2012ʙ2014 ೥౓)‫ج‬൫‫( ڀݚ‬C) ʮ࣍ੈ୅‫ܕ‬ෆ҆ఆ֩൓Ԡ࣮‫ ͚ͨ޲ʹݧ‬RI ੜ੒ɾՃ଎ͷ৽ख๏։ൃʯ

(ࣉ੢ߴ 2012ʙ2014 ೥౓)एख‫( ڀݚ‬B) ʮ௿ΤωϧΪʔෆ҆ఆ֩ϏʔϜ࣮‫༻ݧ‬ͷബບภ‫ۃ‬ཅࢠඪతͷ։ൃʯ(ࡔ‫ޱ‬૱ࢤ 2013ʙ2015 ೥౓)৽ֶज़ྖҬ‫ྖڀݚ( ڀݚ‬ҬఏҊ‫ )ܕ‬ʮྫྷ٫ෆ҆ఆ‫ࢠݪ‬Λ༻͍ͨిࢠి‫ؾ‬૒‫ࢠۃ‬ೳ཰୳ࡧʯ

(‫ڀݚ‬୅දऀ:ञ‫ݟ‬ହ‫׮‬ɺ෼୲ऀ:ए‫ڱ‬ஐ࢚)90ֶ෦̐೥ੜଔ‫ڀݚۀ‬(1) ֲၭዉ : ʢࢦಋ‫ڭ‬һɺ৿ాߒհʣ
4

He(12 C,16 O) Ѝ࣮‫͚͓ʹݧ‬Δඪత෇͔ۙΒͷ 16 O όοΫάϥϯυ I(2) ‫ؒٱ‬େฏ : ʢࢦಋ‫ڭ‬һɺ৿ాߒհʣ
4

He(12 C,16 O) Ѝ࣮‫͚͓ʹݧ‬Δඪత෇͔ۙΒͷ 16 O όοΫάϥϯυ II(3) খౡ୓࿠ : ʢࢦಋ‫ڭ‬һɺ໺࿊఩෉ʣ
ΠΦϯνΣϯόΛ༻͍ͨಉҐମ෼཭ೳͷධՁ(4) ਐ౻༎ี : ʢࢦಋ‫ڭ‬һɺए‫ڱ‬ஐ࢚ʣΞΠιόϦοΫɾΞφϩάঢ়ଶ΁ͷભҠΛ༻͍࣭ͨྔެࣜͷΫʔϩϯ߲ͷ܎਺ͷଌఆ(5) ాதହ‫ و‬: ʢࢦಋ‫ڭ‬һɺ৿ాߒհʣ
‫ؾ‬ମॆర‫ܕ‬൓௓෼཭‫( ث‬GARIS) ͷಈ࡞‫ݪ‬ཧ?

(6) ా୺৺ւ : ʢࢦಋ‫ڭ‬һɺए‫ڱ‬ஐ࢚ʣΞΠιόϦοΫΞφϩάঢ়ଶΛར༻ͨ͠‫֩ࢠݪ‬ͷిՙ൒‫ܘ‬ͷଌఆ(7) ৽໊޹ࡈ : ʢࢦಋ‫ڭ‬һɺ໺࿊఩෉ʣ
ҏ౎Ωϟϯύε৽ϏʔϜϥΠϯͷͨΊͷి࣓ੴͷੑೳධՁ(8) ଇদ‫ګ‬জ : ʢࢦಋ‫ڭ‬һɺࣉ੢ߴʣ
RF ՙిަ‫׵‬ΠΦϯ‫ݯ‬ͷ։ൃ(9) ࢁຊᠳ໵ : ʢࢦಋ‫ڭ‬һɺ৿ాߒհʣ
‫ؾ‬ମॆర‫ܕ‬൓௓෼཭‫( ث‬GARIS) ͷಈ࡞‫ݪ‬ཧ?
म࢜࿦จେத‫ܙو‬ɿ(ࢦಋ‫ڭ‬һɺए‫ڱ‬ஐ࢚)

pd ෼ղ൓Ԡʹ͓͚Δ Space Star Anomaly ͷ֬ఆͱΤωϧΪʔґଘੑͷ‫ڀݚ‬ၲ‫ۄ‬େีɿ(ࢦಋ‫ڭ‬һɺ৿ాߒհ)Ecm = 1.2 MeV Ͱͷ 4 He(12 C,16 O)γ ൓Ԡ༧උଌఆͱ He ॥‫ܥ؀‬։ൃ੢ࢁ‫ݑ‬Ұɿʢࢦಋ‫ڭ‬һɺ໺࿊఩෉ʣ
‫۝‬େλϯσϜՃ଎‫ث‬Λ༻͍ͨ AMS γεςϜͷ։ൃ— ϏʔϜΤϛολϯεଌఆͱ‫ݕ‬ग़‫Ͱث‬ͷϏʔϜࣝผ —෱Ӭ୓ɿʢࢦಋ‫ڭ‬һɺ໺࿊఩෉ʣ

(p, 2p) ൓ԠʹΑΔ Ca ͷཻ̍ࢠ‫౓ڧ‬෼෍ଌఆલా༟࢙ɿ(ࢦಋ‫ڭ‬һɺए‫ڱ‬ஐ࢚)nn ঢ়ଶ୳ࡧͷͨΊͷ 2 H(n,p)nn ൓Ԡͷ௿όοΫάϥϯυଌఆ҆ా३ฏɿ(ࢦಋ‫ڭ‬һɺए‫ڱ‬ஐ࢚)91֩಺֩ࢠؒ૬‫༻࡞ޓ‬ͷ‫ڀݚ‬ͷͨΊͷதੑࢠεϐϯଌఆ‫ܥ‬ͷ։ൃֶ֎Ͱͷֶձ‫׆‬ಈ໺࿊఩෉ɿ೔ຊ෺ཧֶձ ୅ٞһɺJ-PARC ์ࣹઢ҆શҕһձҕһ֩෺ཧҕһձҕһɺେࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔӡӦҕһձҕһࠃࡍॿ‫ݴ‬ҕһ (2004 ೥ 4 ݄ʙʣए‫ڱ‬ஐ࢚ : େࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔ‫ܭڀݚ‬ը‫ݕ‬౼ઐ໳ҕһձҕһେࡕେֶ֩෺ཧ‫ڀݚ‬ηϯλʔ࣮‫ݧ‬՝୊৹ࠪઐ໳ҕһձҕһࣉ੢ߴ :೔ຊ෺ཧֶձ‫۝‬भࢧ෦ҕһ૬ྑ‫ ࢸݐ‬: Asia-Paciﬁc Conference on Few-Body Problems in Physics (APFB)ͦͷଞͷ‫׆‬ಈͱ੒Ռମ‫ݧ‬ೖֶɾ࣮‫ݧ‬ʮ෺࣭Λಁա͢Δཻࢠઢʯ2014 ೥ 3 ݄ 24 ೔ (ࣉ੢ߴ)

92෺ੑཧ࿦‫ࣨڀݚ‬‫ߏࣨڀݚ‬੒һ٢৿໌ ।‫ڭ‬तদҪ३ ॿ‫ڭ‬ େֶӃ ത࢜՝ఔ ຤দ҆༝ඒ (‫)ֶٳظޙ‬দຊ޾հ (‫)ֶٳظޙ‬தଜ༗Ֆ໺‫৻ޱ‬ฏ

‫ྒݪ‬ฏ

ࢁాҰ༤

 େֶӃ म࢜՝ఔ 
Ҫ্խ࿠

ࢁ๺஌࢙

‫ڕ‬Ԭ༐༎

Ԭ࣍૱ ֶ෦ ଔ‫ڀݚۀ‬ੜ Ѩ෦ ݈ଠ࣌দ ‫װ‬෋ా ੟໵୲౰त‫ۀ‬౷‫ ֶྗܭ‬II(٢৿໌)ɺ౷‫ิֶྗܭ‬श (٢৿໌)ɺඇฏߧ෺ཧֶ (٢৿໌)ɺྗֶ‫ૅج‬ಉԋश (٢৿໌)ɺྗֶ‫ૅج‬ಉԋश (দҪ३)ɺ෺ཧ਺ֶԋश (দҪ३)‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ

[I] ඇฏߧ‫ܥ‬ɾෳࡶ‫ܥ‬Λத৺ͱͨ͠෺ੑཧ࿦
1. աྫྷ٫ӷମɺΨϥεసҠͷ਺஋తɺཧ࿦త‫ڀݚ‬(a) ̏࣍‫ݩ‬୯੒෼ӷମͷΨϥεసҠ (দຊ޾հɺদҪ३)
LJG ϙςϯγϟϧϞσϧཻࢠͷ୯੒෼‫Ͱܥ‬෼ࢠಈྗֶγϛϡϨʔγϣϯΛߦͬͨɻߴ͍ѹྗԼͰ͸݁থ΁ɺ௿͍ѹྗԼͰ͸Ψϥε΁
సҠ͢Δ͜ͱ͕Θ͔͍ͬͯΔɻதఔ౓ͷѹྗԼͰ͸ɺҰ࣍సҠͯ͠ɺप‫ߏظ‬଄ͷͳ͍ߴີ౓૬ʹͳΔɻ֦ࢄ܎਺ͷԹ౓ґଘ͕ΞϨχ΢ε
‫͋Ͱܕ‬Δ͜ͱ͔Βɺߴີ౓૬͕ӷମͰ͋ΔՄೳੑΛ‫ݕ‬౼ͨ͠ɻ(b) GPGPU Λ༻͍ͨߴ଎γϛϡϨʔγϣϯͷ։ൃ (দຊ޾հɺদҪ३)ɿGPGPU Λར༻ͯ͠ɺ෼ࢠಈྗֶγϛϡϨʔγϣϯͷ௒ฒྻԽΛࢼΈͨɻ

93

(c) δϟϯϓ଴ͪ࣌ؒ෼෍ͷର਺ൃࢄ (দҪ३)Ψϥεதͷ෼ࢠͷδϟϯϓ֦ࢄʹ͍ͭͯ଴ͪ࣌ؒͷۭؒ૬ؔʹ͍ͭͯղੳͨ͠ɻ

2. ༳ಈࢄҳؔ܎ࣜͷഁΕͷද‫ࠤాݪͱݱ‬ʑެࣜ (ࢁాҰ༤ɺ٢৿໌)ଟ਺ͷϥϯδϡόϯཻࢠͷີ౓৔Ͱ‫ه‬ड़͞ΕΔ‫ܥ‬Λ৔ͷΦʔόʔμϯϓϥϯδϡόϯϞσϧͱ‫Ϳݺ‬ɻ͜ͷϞσϧͷա౉తӡಈྔ৔ʹؔ͢Δ༳ಈࢄҳؔ܎ࣜͷഁΕ͕ఆৗൃ೤཰ͱ݁ͼͭ͘͜ͱΛࣔͨ͠ɻ[II] Խֶ෺ཧͷཧ࿦త‫ڀݚ‬
1. ଟ੒෼༹ഔதͰͷେ͖ͳ༹࣭ͷ֦ࢄͷ‫( ڀݚ‬தଜ༗Ֆɺ٢৿໌)2 ੒෼߶ମ‫༹ٿ‬ഔதͰͷ༹࣭ͷ֦ࢄ܎਺Λɺ༹࣭पΓͷ༹ഔͷີ౓෼෍ΛߟྀͰ͖Δཧ࿦Λ༻͍ͯ‫ͨ͠ࢉܭ‬ɻ2 ੒෼༹ഔͷࠞ߹ൺ΍൒‫ܘ‬ൺʹΑ֦ͬͯࢄ܎਺͸มԽ͠ɺྲྀମྗֶͷετʔΫε-ΞΠϯγϡλΠϯଇ͕େ͖͘ഁΕΔ৔߹͕͋Δ͜ͱ͕෼͔ͬͨɻ·ͨɺ͜ͷഁΕ༹͕࣭ද໘
Ͱͷ༹ഔཻࢠͷີ౓ͱ‫͍ڧ‬૬͕ؔ͋Δ͜ͱΛ໌Β͔ʹͨ͠ɻ

2. ݀தͷཻࢠͷฏߧঢ়ଶͱμΠφϛοΫεͷ‫ྒݪ( ڀݚ‬ฏɺ٢৿໌)‫ۭ͍ؒڱ‬ͷதʹ༹࣭͕ೖΔ‫ݱ‬৅͸ɺγϟϖϩϯͷ‫ػ‬ೳɺABC τϥϯεϙʔλʔͳͲ͋Γɺ‫ج‬ຊతͳ‫ݱ‬৅Ͱ͋Δɻ͜ͷΑ͏ͳ‫ݱ‬৅ʹ༹͓͍ͯഔ
༹͕࣭ʹ༩͑ΔӨ‫ڹ‬Λ TDDFT(ಈతີ౓൚ؔ਺ཧ࿦) Λ༻͍ͯཧ࿦ͷఆࣜԽΛߦͬͨɻ·ͨɺ༹࣭͕౳଎౓Ͱಈ͍͍ͯΔͱ͖ͷ༹ഔͷ֬཰ີ౓෼෍ͷ࣌ؒมԽΛ਺஋తʹ໌Β͔ʹ͠ɺଟ͘ͷ༹ഔ͕‫ʹۭ͍ؒڱ‬ด͡ࠐΊΒΔ͜ͱ͕෼͔ͬͨɻ

3. ‫ޮׇރ‬ՌʹΑΔ୿ന࣭ͷ݁থԽ (຤দ҆༝ඒɺ٢৿໌)‫ޮׇރ‬ՌʹΑΔ୿ന࣭ͷ݁থԽϝΧχζϜΛ໌Β͔ʹ͢Δҝʹɺ୿ന࣭͓Αͼ݁থԽࡎͱͯ͠ͷߴ෼ࢠΛେখ̎੒෼ͷ߶ମ‫ʹܥ‬ϞσϧԽͨ͠‫ܥ‬Λѻͬͨɻখཻࢠ͕༩͑Δେཻࢠؒͷ࣮ޮతͳҾྗʹ͍ͭͯɺ͜Ε·Ͱͷ‫Ͱڀݚ‬͸؆୯ͳ୯‫ۃ‬খͷϞσϧ͕࢖ΘΕ͖ͯͨɻຊ‫Ͱڀݚ‬͸ੵ෼ํఔࣜཧ࿦Λ༻͍ͨΑΓෳࡶͳ݁ՌΛ࠾༻͠ɺͦΕΛѻ͏ͨΊͷཧ࿦Λཱ֬ͨ͠ɻ

4. ࢀর߶ମ‫ܥٿ‬ͷ‫ ʹࢉܭ‬RY ۙࣅΛ࢖ͬͨ೤ྗֶઁಈ࿦ (‫ڕ‬Ԭ༐༎ɺ٢৿
໌)݁থԽͷ‫ڀݚ‬Λ؆ศʹߦ͏ͨΊɺRamakrishnan-Yussouﬀ(RY) ۙࣅΛ࢖ͬͨ೤ྗֶઁಈ࿦ΛఆࣜԽ͠ɺ୿ന࣭ͷ݁থԽʹԠ༻͢Δ͜ͱΛ໨ඪʹ͍ͯ͠Δɻࢀর‫߶ͯ͠ͱܥ‬ମ‫ٿ‬ΛऔΓɺ݁থͱӷମͷࣗ༝ΤωϧΪʔ94

ࠩΛ RY ۙࣅͰ‫͢ࢉܭ‬Δɻ͞Βʹɺ߶ମ‫ٿ‬Ҏ֎ͷ૬‫༻࡞ޓ‬Λઁಈͱͯ͠
औΓೖΕΔͨΊɺͦͷࣜͷ‫ܗ‬Λಋग़ͨ͠ɻདྷ೥౓͸ɺ۩ମతͳ‫ʹܥ‬Ԡ༻͠ɺଞͷํ๏ͱൺֱͯ͠ਫ਼౓Λ໌Β͔ʹ͢Δɻ

5. ಈతີ౓൚ؔ਺ཧ࿦Λ༻͍ͨϚΠΫϩϨΦϩδʔͷ‫( ڀݚ‬Ҫ্խ࿠ɺ٢
৿໌)ϚΠΫϩϨΦϩδʔͰ͸ɺෳࡶྲྀମͷ಺෦ʹૠೖ͞Εͨϓϩʔϒཻࢠͷӡಈͷ༷ࢠ͔Βɺͦͷෳࡶྲྀମͷྗֶతੑ࣭͕ܾఆ͞ΕΔɻ͜ͷ࣌ɺෳࡶྲྀମͷߏ੒ཻࢠʢίϩΠυཻࢠͳͲʣಉ࢜ͷ૬‫͕༻࡞ޓ‬ϓϩʔϒཻࢠͷӡಈʹӨ‫ڹ‬Λ‫͢΅ٴ‬ɻຊ‫Ͱڀݚ‬͸ɺίϩΠυ༹ӷͷϚΠΫϩϨΦϩ
δʔʹ૬౰͢Δ؆୯ͳ໰୊ઃఆͷԼͰɺίϩΠυཻࢠؒͷ૬‫͕༻࡞ޓ‬ϓϩʔϒཻࢠͷӡಈʹ‫͢΅ٴ‬Ө‫͍ͯͭʹڹ‬ɺಈతີ౓൚ؔ਺ཧ࿦Λ༻͍ͯ਺஋తʹௐ΂ͨɻ

6. ΞΠϯγϡλΠϯͷ೪౓ࣜͷ֦ு (ࢁ๺஌࢙ɺ٢৿໌)༹࣭पΓͷ༹ഔ࿨ͷޮՌΛߟྀͯ͠ɺ༹ഔཻࢠͷີ౓෼෍͔Β༹ӷͷ೪౓Λ‫͢ࢉܭ‬Δཧ࿦ΛఆࣜԽͨ͠ɻ͜ΕʹΑΓɺ༹ӷͷ೪౓͸༹ഔཻࢠͷ෼෍ͷӨ‫ڹ‬Λେ͖͘ड͚Δ͜ͱΛ໌͔ʹͨ͠ɻಛʹɺ༹࣭ʖ༹ഔؒʹҾྗ͕ಇ͘৔߹ʹ༹ӷͷ೪౓Λ‫͠ࢉܭ‬ɺҾྗ͕େ͖͍΄Ͳ೪౓΋େ͖͘ͳΔ͜ͱ͕໌Β͔ͱͳͬͨɻ

7. ૬‫఺༻࡞ޓ‬ϞσϧʹΑΔಈతີ౓൚ؔ਺ཧ࿦ͷ෼ࢠӷମ΁ͷ֦ு (Ԭ࣍૱ɺ٢৿໌)
ಈతີ౓൚ؔ਺ཧ࿦͸୯७ӷମͷμΠφϛΫεΛ‫ه‬ड़͢Δཧ࿦Ͱ͋Δ
͕ɺຊ‫Ͱڀݚ‬͸͜ͷཧ࿦Λ૬‫఺༻࡞ޓ‬ϞσϧʹΑͬͯ෼ࢠӷମʹద༻Ͱ
͖Δཧ࿦΁ͱ֦ுͨ͠ɻ·ͨͦΕΛ༻͍ͯೋ‫ࢠݪ‬෼ࢠʹ֤ؔͯ͠αΠτ͝ͱʹີ౓৔ͷ࣌ؒมԽΛ਺஋తʹ‫͠ࢉܭ‬ɺಘΒΕͨ݁ՌΛ୯७ӷମͷ΋ͷͱൺֱ͢Δ͜ͱͰ෼ࢠӷମಛ༗ͷಈతੑ࣭Λ໌Β͔ʹͨ͠ɻൃද࿦จ ‫ݪ‬ஶ࿦จ 
Perturbation Theory of Large-Particle Diﬀusion in a Binary Solvent Mixture:
Yuka Nakamura, Akira Yoshimori, and Ryo Akiyama,
Journal of the Physical Society of Japan, Vol. 83 064601 (2014).

95

A Uniﬁed Proof of the Harada-Sasa equality for Underdamped and Overdamped Systems:
Kazuo Yamada and Akira Yoshimori,
Journal of the Physical Society of Japan, Vol. 83 053001 (2014).
Coarse-grained forms for equations describing the microscopic motion of particles in a
ﬂuid:
Shankar P. Das and Akira Yoshimori,Phys. Rev. E, Vol. 88 043008 (2013) [8 pages].
A theoretical framework for calculations of the structural relaxation time on the basisof the free energy landscape theory:
Toru Ekimoto, Akira Yoshimori, Takashi Odagaki and Takashi Yoshidome
Chemical Physics letters, Vol. 577 , Pages 58-61 (2013).
A non-perturbative approach to freezing of superfuid 4He in density functional theory,
T. Minoguchi1, D.E. Galli, M. Rossi and A. Yoshimori
Journal of Physics: Conference Series. 400, 012050, (2013)
Proceedings
Eﬀects of Solvation Structure on Diﬀusion of Large Particle in Binary Mixture Studied
by Perturbation Theory:
Yuka Nakamura, Akira Yoshimori, and Ryo Akiyama,
Journal of Molecular Liquids, ҹ࡮தControl of solid-phase stability by interaction potential with two minima:
A. Suematsu, A. Yoshimori, M. Saiki, J. Matsui, T. Odagaki,
Journal of Molecular Liquids, ҹ࡮தߨԋ ւ֎Ͱͷߨԋ 
Entropic eﬀects of solvent on big sphere dynamics into a cylindrical vessel,
Ryohei Hara, Ken-ichi Amano, Masahiro Kinoshita and Akira Yoshimori,“Statphys25”, July 21 - 26, 2013 Seoul National University, Seoul, Korea
96 ࠃ಺Ͱͷߨԋ 
ʮControl of solid-phase stability by interaction potential with two minimaʯ(ট଴ߨԋ)
A. Suematsu, A. Yoshimori, M. Saiki, J. Matsui, T. Odagaki,”7th Mini-Symposium on Liquids” ‫۝‬भେֶ,7 ݄ 5 ೔-7 ݄ 6 ೔, 2013
ʮPhase stability of a double-minimum potential system ʯ຤দ҆༝ඒ, ٢৿໌, ࠽໦ক࢙, দҪ३, খా֞޹”7th Mini-Symposium on Liquids” ‫۝‬भେֶ,7 ݄ 5 ೔-7 ݄ 6 ೔, 2013
ʮPerturbation theory of large particle diﬀusion in a binary solventʯதଜ༗Ֆɺ٢৿໌ɺळࢁྑɺࢁ‫ؽޱ‬”7th Mini-Symposium on Liquids” ‫۝‬भେֶ,7 ݄ 5 ೔-7 ݄ 6 ೔, 2013
ʮEﬀects of particle correlation on microrheologyʯҪ্խ࿠ɺ٢৿໌

”7th Mini-Symposium on Liquids” ‫۝‬भେֶ,7 ݄ 5 ೔-7 ݄ 6 ೔, 2013
ʮA study of phase transition using interaction potential with two minimaʯ຤দ҆༝ඒ, ٢৿໌, ࠽໦ক࢙, দҪ३, খా֞޹”33rd International Conference on Solution Chemistry”‫౎ژ‬,7 ݄ 7 ೔-7 ݄ 12 ೔,2013
ʮPerturbation theory of large particle diﬀusion in a binary solventʯதଜ༗Ֆɺ٢৿໌ɺळࢁྑɺࢁ‫ؽޱ‬”33rd International Conference on Solution Chemistry” ‫౎ژ‬,7 ݄ 7 ೔-7 ݄ 12 ೔,2013ʮ‫ޮׇރ‬ՌʹΑΔ૬సҠʯ຤দ҆༝ඒ, ٢৿໌, ळࢁྑ, தଜ༗Ֆ”೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձ” ಙౡ,9 ݄ 25 ೔-9 ݄ 28 ೔,2013ʮେ͖ͳཻࢠͷ֦ࢄʹ͓͚Δ༹ഔͷॆర཰ͷޮՌʯதଜ༗Ֆɺ٢৿໌ɺळࢁྑ

”೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձ” ಙౡ,9 ݄ 25 ೔-9 ݄ 28 ೔,2013ʮϚΠΫϩϨΦϩδʔʹ͓͚Δཻࢠؒ૬‫༻࡞ޓ‬ͷޮՌʯ

97Ҫ্խ࿠ɺ٢৿໌

”೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձ” ಙౡ,9 ݄ 25 ೔-9 ݄ 28 ೔,2013ʮϞσϧΨϥεʹ͓͚Δॎ೾‫؍‬ଌͷ࠶ߟʯଜதਖ਼ɺদҪ३ɺඉ౉อळ

”೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձ” ಙౡ,9 ݄ 25 ೔-9 ݄ 28 ೔,2013ʮཻࢠؒ૬‫ۃʹ༻࡞ޓ‬খ͕̎ͭ͋Δ‫ܥ‬ͷଟ༷ੑʯদຊ޾հɺদҪ३”ୈ 4 ճ‫ࢉܭ‬౷‫ܭ‬෺ཧֶ‫ڀݚ‬ձ” Ӊ෦,10 ݄ 5 ೔-10 ݄ 6 ೔,2013
ʮApplication of a Liquid Theory to Colloidal Dispersion SystemsʯҪ্խ࿠ɺ٢৿໌

”3rd International Conference on Molecular Simulation” ฌ‫ݿ‬,11 ݄ 18 ೔-11 ݄ 20 ೔,2013“A Theory of Phase Transition for Two-Minimum Potential Systems”
Ayumi Suematsu, Akira Yoshimori, Masafumi Saiki, Jun Matsui and Takashi Odagaki”3rd International Conference on Molecular Simulation” ฌ‫ݿ‬,11 ݄ 18 ೔-11 ݄ 20 ೔,2013
ʮ The observation of the longitudinal wave velocity in a model supercooled liquidʯଜதਖ਼ɺদҪ३ɺඉ౉อळ

”3rd International Conference on Molecular Simulation” ฌ‫ݿ‬,11 ݄ 18 ೔-11 ݄ 20 ೔,2013ʮ֦ࢄ܎਺ʹ͓͚Δ༹ഔ࿨ͷޮՌʯதଜ༗Ֆɺ٢৿໌ɺळࢁྑ

”ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ” ෱Ԭ,11 ݄ 30 ೔,2013ʮίϩΠυ෼ࢄ‫ܥ‬ͷ‫ࠤాݪ‬ʑެࣜʯࢁాҰ༤ɺ٢৿໌

”ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ” ෱Ԭ,11 ݄ 30 ೔,2013ʮίϩΠυ෼ࢄ‫ܥ‬ͷμΠφϛΫεʹ͓͚Δཻࢠؒ૬‫༻࡞ޓ‬ͷޮՌʯҪ্խ࿠ɺ٢৿໌

”ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ” ෱Ԭ,11 ݄ 30 ೔,201398ʮཻࢠؒ૬‫ۃʹ༻࡞ޓ‬খ͕̎ͭ͋Δ‫ܥ‬ͷ‫ݻ‬ӷసҠ ʯদຊ޾հɺদҪ३”ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ” ෱Ԭ,11 ݄ 30 ೔,2013
ʮA Study of Microrheology by the Time Dependent Density Functional TheoryʯҪ্խ࿠ɺ٢৿໌

”5th JCS International Symposium on Theoretical Chemistry” ಸྑ,12 ݄ 2 ೔-12 ݄ 6
೔,2013
ʮDepletion eﬀects on diﬀusion in a binary hard sphere mixtureʯதଜ༗Ֆɺ٢৿໌ɺळࢁྑ

”Nagoya Symposium on Depletion Forces: Celebrating the 60th Anniversary of the
Asakura-Oosawa Theory” Ѫ஌,3 ݄ 14 ೔-3 ݄ 15 ೔,2014
ʮDepletion eﬀects on dynamics in microrheologyʯҪ্խ࿠ɺ٢৿໌

”Nagoya Symposium on Depletion Forces: Celebrating the 60th Anniversary of the
Asakura-Oosawa Theory” Ѫ஌,3 ݄ 14 ೔-3 ݄ 15 ೔,2014
ʮDepletion eﬀects on viscosity of solutionʯࢁ๺஌࢙ɺ٢৿໌

”Nagoya Symposium on Depletion Forces: Celebrating the 60th Anniversary of the
Asakura-Oosawa Theory” Ѫ஌,3 ݄ 14 ೔-3 ݄ 15 ೔,2014ʮ‫ޮׇރ‬ՌʹΑΔ݁থԽͷ༗ޮϙςϯγϟϧΛ࢖ͬͨ‫ڀݚ‬ʯ຤দ҆༝ඒ, ٢৿໌, ळࢁྑ, தଜ༗Ֆ”೔ຊ෺ཧֶձ 2014 य़‫ق‬େձ” ਆಸ઒,3 ݄ 27 ೔-3 ݄ 30 ೔,2014ʮ༹ഔͷཻࢠੑΛߟྀͨ͠ͱ͖ͷ༹࣭ͷ֦ࢄͷཧ࿦ʯதଜ༗Ֆɺ٢৿໌ɺळࢁྑ

”೔ຊ෺ཧֶձ 2014 य़‫ق‬େձ” ਆಸ઒,3 ݄ 27 ೔-3 ݄ 30 ೔,2014ʮίϩΠυ෼ࢄ‫ܥ‬ͷϚΠΫϩϨΦϩδʔʯҪ্խ࿠ɺ٢৿໌

”೔ຊ෺ཧֶձ 2014 य़‫ق‬େձ” ਆಸ઒,3 ݄ 27 ೔-3 ݄ 30 ೔,201499ʮ༹ഔͷཻࢠੑΛߟྀͨ͠ͱ͖ͷ༹ӷͷ೪ੑͷཧ࿦ʯࢁ๺஌࢙ɺ٢৿໌

”೔ຊ෺ཧֶձ 2014 य़‫ق‬େձ” ਆಸ઒,3 ݄ 27 ೔-3 ݄ 30 ೔,2014ʮ૬‫఺༻࡞ޓ‬Ϟσϧʹ͓͚Δಈతີ౓൚ؔ਺ཧ࿦ʯ
Ԭ࣍૱ɺ٢৿໌ɺ٢ా‫ل‬ੜ”೔ຊ෺ཧֶձ 2014 य़‫ق‬େձ” ਆಸ઒,3 ݄ 27 ೔-3 ݄ 30 ೔,2014֎෦ࢿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ ‫ج‬൫‫( ڀݚ‬C) “ੜ໋‫ݱ‬৅ʹର͢Δਫ෼ࢠͷಈతޮՌ” ʢ‫ڀݚ‬୅දऀɿ٢৿໌ʣ(৽‫)ن‬೔ຊֶज़ৼ‫ڵ‬ձಛผ‫ڀݚ‬һ౳‫ڞͼٴ‬ಉ‫ڀݚ‬ͷ࠾୒ (ֶ֎͔Βͷड͚ೖΕΛ‫ؚ‬Ή)தଜ༗Ֆɺ೔ຊֶज़ৼ‫ڵ‬ձಛผ‫ڀݚ‬һ (DC2)ֶ෦̐೥ੜଔ‫ڀݚۀ‬Ѩ෦ ݈ଠɿ(ࢦಋ‫ڭ‬һɺ٢৿໌)ɿ୿ന࣭ͷѹྗมੑͱ‫ܗ‬ଶ೤ྗֶ෋ా ੟໵ɿ(ࢦಋ‫ڭ‬һɺদҪ३)ɿପԁཻࢠ‫ܥ‬ͷ‫ݻ‬ӷసҠम࢜࿦จҪ্ խ࿠ɿ(ࢦಋ‫ڭ‬һɺ٢৿໌)ɿಈతີ౓൚ؔ਺ཧ࿦Λ༻͍ͨϚΠΫϩϨΦϩδʔͷ‫ڀݚ‬ࢁ๺ ஌࢙ɿ(ࢦಋ‫ڭ‬һɺ٢৿໌)ɿ༹ӷͷ೪౓ʹ͓͚Δ༹ഔͷ෼෍ͷޮՌͦͷଞͷ‫׆‬ಈͱ੒Ռ

1. ΦʔϓϯΩϟϯύε

100

2. ߴߍੜମ‫ݧ‬ೖֶʮΰϜ஄ੑʯ࣮शʢ४උͷΈʣ101౷‫ܭ‬෺ཧֶ ‫ࣨڀݚ‬‫ߏࣨڀݚ‬੒һத੢ ल ‫ڭ‬त໺ଜ ਗ਼ӳ ।‫ڭ‬तࡔ্ ‫و‬༸ ॿ‫ڭ‬ ത࢜‫ڀݚ‬һ ઃָ ‫ګ‬ฏ େֶӃ ത࢜՝ఔ ۙ౻ ༸Ұ࿠ େֶӃ म࢜՝ఔ ૔ຊ ཾਫམ ‫ݑ‬ҰύΫ υϯώϣϯ

෢‫ޛ ٱ‬೭

தඌɹ޾

৿ॏ ॱฏ

 ֶ෦ ଔ‫ڀݚۀ‬ੜ 
҆౻ େߊ

޻౻ ୡ໼

ळࢁ ཅฏ

 ‫ڀݚ‬ੜ 
Daniel Krüger ๚໰‫ ऀڀݚ‬ૣ੉ ༑ඒ೫
୲౰त‫ۀ‬
த੢ɿ ίΞηϛφʔʢશֶʣɺ෺ཧֶ࠷લઢɺྔࢠྗֶ I ิम૬సҠͷ౷‫ֶྗܭ‬ɺ౷‫ܭ‬෺ཧֶ I໺ଜɿ ίΞηϛφʔɺྗֶ‫ૅج‬ɾಉԋश (શֶʣɺҰൠ૬ର࿦ɺྔࢠ౷‫ܭ‬෺ཧֶ (େֶӃʣࡔ্ɿ ෺ཧֶ‫ૅج‬ԋशɺ౷‫ ֶྗܭ‬I ԋश‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ

1. ೤ਫ্ͷඍখਫణ (த੢)ɿ೤͍ίʔώʔ΍ߚ஡ͳͲͷ೤ਫද໘ʹ‫ݟ‬ΒΕΔന͍౬‫ؾ‬ͷബບ͓ΑͼͦΕʹُ྾͕ೖΔΑ͏ʹ‫͑ݟ‬Δ‫ݱ‬৅ͷ࣮‫ݧ‬త‫࡯؍‬Λߦͬͨɻߴ଎ϏσΦΛ༻͍ͨ‫ݦ‬ඍ‫࡯؍ڸ‬ͷ݁Ռɺബບ͸௚‫ ܘ‬10μm ఔ౓ͷඍখਫ

102ణ͔ΒͳΓɺͦΕΒ͸ਫ໘͔Β 10μm ఔ౓ͷۭதʹු༡͍ͯ͠Δ͜ͱɺُ྾
͕ೖͬͨΑ͏ʹ‫͑ݟ‬Δͷ͸ͦͷਫణ͕ूஂམண͍ͯ͠Δ͜ͱɺͦΕ͸Ұͭͷਫణͷফ໓͕Ҿ͖ۚʹͳ͓ͬͯΓɺ̍ m/s ఔ౓ͷ೾໘ͱͯ͠఻Θ͍ͬͯΔ͜
ͱ͕෼͔ͬͨɻʢࢢ઒ʢ‫ژ‬େʣͱͷ‫ڞ‬ಉ‫ڀݚ‬ʣ

2. μΠϥλϯτྲྀମͷͣΓ೪Խৼಈ (த੢)ɿย‫܀‬คਫͷΑ͏ͳคମɾྲྀମͷࠞ߹෺͸ඇৗʹ‫ͣͳܹٸ‬Γ೪ԽΛࣔ͢͜ͱ͕஌ΒΕ͓ͯΓɺզʑ͸ͦͷ‫ݱ‬৅࿦తϞσϧΛߏ੒͢Δ͜ͱʹΑΓͦΕ͕γΞͷԼͰ೪Խঢ়ଶͱ؇࿨ঢ়ଶΛߦ͖
དྷ͢Δࣗൃৼಈɺ͢ͳΘͪͣΓ೪ԽৼಈΛ͢Δ͜ͱΛࣔ͠ɺ͞Βʹ࣮‫ݧ‬త‫؍‬࡯ʹ੒ޭ͍ͯͨ͠ɻࠓ೥౓͸ɺͣΓ೪Խৼಈʹ͓͚ΔγϦϯμʔ಺ͷ೪Խߏ଄Λௐ΂ΔͨΊʹɺγϦϯμʔ‫ʹ࣠ͼٴ‬ѹྗηϯαʔΛऔΓ෇͚ɺৼಈ࣌ͷγϦϯμʔ֎นͷѹྗ‫͔͔ʹ࣠ͼٴ‬Δྗͷෆ‫ۉ‬ҰੑΛௐ΂ͨɻʢӬ߂ʢઋ୆ߴઐʣɺ‫ޚ‬खચʢNBIʣͱͷ‫ڞ‬ಉ‫ڀݚ‬ʣ

3. ࢴͷΫϥϯϓϦϯά (ૣ੉ɺத੢ɺࡔ্)ɿࢴ͸ൺֱత༰қʹં‫͛ۂ‬ΒΕΔ͕ɺͦͷ໘ੵΛ͔͑ΔΑ͏ͳม‫ʹܗ‬ରͯ͠͸ඇৗʹେ͖ͳ఍߅Λࣔ͢ɻͦͷΑ͏ͳੑ࣭ͷͨΊʹɺࢴΛແ࡞ҝʹ‫ؙ‬Ίͨͱ͖ͷࠩ͠౉͠ͷ௕͞ R ͸ɺࢴͷେ͖͞ L ʹରͯ͠ίϯύΫτͳߏ଄͔Β༧૝͞ΕΔৼΔ෣͍ R ∼ L2/3 ΑΓ΋େ͖͘ͳΔɻ͜ͷ༷ͳࢴͷੑ࣭Λɺ̎࣍‫ݩ‬෺ମͷંΓͨͨΈߏ଄ͱ͍͏ΑΓҰൠతͳ࿮૊ΈͰཧղ͢ΔͨΊʹɺ୯७ͳϞσϧԽʹΑΔ‫ػࢉܭ‬γϛϡϨʔγϣϯΛ४උ͍ͯ͠Δɻʢૣ੉ͱͷ‫ڞ‬ಉ‫ڀݚ‬ʣ

4. คମଯੵதͷৼಈϞʔυղੳ (૔ຊɺத੢ɺࡔ্)ɿคମଯੵதͷԻ೾ͷ఻೻Λղੳ͢ΔͨΊʹɺ‫ػࢉܭ‬γϛϡϨʔγϣϯΛߦͬͨɻ཭ࢄཁૉ๏ (DEM) ʹΑΓ࡞੒ͨ̎࣍͠‫ݩ‬ͷคମଯߏ଄Λ༻͍ͯɺઢ‫ܗ‬͹Ͷͱ࣭఺ͷ‫ܥ‬ͷৼಈϞʔυͷղੳΛߦͬͨɻͦͷ݁Ռɺߴ͍ৼಈ਺Λ΋ͭϞʔυͰৼ෯ͷ‫ࡏہ‬Խ͕‫ݟ‬ΒΕͨɻคମଯੵߏ଄͕ૄͰ͋Δ΄Ͳɺ‫ࡏہ‬Խ͕‫ݟ‬ΒΕΔप೾਺ྖҬ͕޿͘
ͳΔ͜ͱ͕෼͔ͬͨɻ࣍ʹɺઢ‫ܗ‬͹Ͷʹ‫ݮ‬ਰΛೖΕͨ‫Ͱܥ‬ɺ1 ͭͷཻࢠʹਖ਼‫ݭ‬తͳྗΛՃ͑ͨ৔߹ͷಁա཰Λ‫ٻ‬Ίͨɻಁա཰ͷৼಈ਺ґଘੑ͸ඇৗʹෳࡶʹͳΓɺLiu ͱ Nagel Βͷ࣮‫( ݧ‬PRL,1992) ͱྨࣅͷߏ଄Λࣔͨ͠ɻ

5. ໢ঢ়ߴ෼ࢠ಺ͷμΠφϛΫε (ਫམɺࡔ্ɺத੢)ɿ1 ࣍‫ݩ‬ϙϦϚʔͷϞσϧΛ 2 ࣍‫֦ʹݩ‬ுͨ͠ɺ໢ঢ়ߴ෼ࢠͷμΠφϛΫεΛௐ΂ͨɻಛʹɺ‫಺ܥ‬ͷϞϊϚʔͷฏ‫̎ۉ‬৐มҐΛ਺஋γϛϡϨʔγϣϯʹΑͬͯௐ΂ɺதؒ࣌ؒྖҬͰ࣌ؒͷࢦ਺͕̍ΑΓ΋খ͍͞ѥ֦ࢄ͢Δ͜ͱΛࣔͨ͠ɻ໢ঢ়ߴ෼ࢠͷฏߧߏ଄͸ɺ೤༳Β͗ͷԼͰ΋ฏୱͳฏ໘ߏ଄ΛͱΔ͜ͱ͕஌ΒΕ͍ͯΔ͕ɺͦ

103

ΕʹରԠͯ͠ɺฏ໘ʹର͢Δ֦ࢄํ޲ʹΑ֦ͬͯࢄͷࢦ਺͕ҟͳΔ͜ͱΛ໌͔ʹͨ͠ɻ

6. ٰ࠭ͷμΠφϛΫε (தඌɺத੢ɺࡔ্)ɿ ٰ࠭͸࠭ͷྔ΍෩޲͖ͷมԽʹΑ༷ͬͯʑͳ‫ܗ‬ଶΛͱΔ͜ͱ͕஌ΒΕ͍ͯΔɻಛʹɺҰํํ޲͔Β෩͕ਧ͘৔߹ʹ͸෩޲͖ʹਨ௚ͳԣํ޲ʹٰ͕࠭࿈ͳΔԣྻٰ͕࠭҆ఆԽ͠ɺ‫ق‬અʹΑΓҟͳΔ̎ํ޲͔Β෩͕ਧ͘৔߹ʹ͸ฏ‫ۉ‬ͷ෩޲ʹରͯ͠ฏߦʹٰ͕࠭ฒͿॎྻٰ͕࠭҆ఆԽ͢Δ͜ͱ͕‫ʹ࡯؍‬ΑΓ஌ΒΕ͍ͯΔ͕ɺ྆ऀͷؔ܎͸ඞͣ͠΋໌Β͔Ͱ͸ͳ͍ɻͦ͜Ͱɺԣྻٰ࠭ͷμΠφϛΫεΛ‫ه‬ड़͢Δॖ໿໛‫ܕ‬ͷͻͱͭͰ͋Δͻ΋໛‫ܕ‬Λ༻͍ͯɺࣼΊ͔Β෩͕ਧ͘৔߹ͷԣྻٰ࠭ʹର
Ԡ͢Δఆৗղͷઢ‫҆ܗ‬ఆੑΛௐ΂ͨɻ

7. ͣΓྲྀͷԼͰͷ૬෼཭μΠφϛΫε (ύΫɺࡔ্ɺத੢)ɿԹ౓ͳͲͷύϥϝλΛม͑Δ͜ͱʹΑΓɺ୯Ұ૬͔Β̎૬‫ڞ‬ଘঢ়ଶ΁సҠͤͨ࣌͞ʹ‫ݱ‬ΕΔߏ଄͸ɺ‫ܥ‬ͷྲྀମྗֶతੑ࣭ʹେ͖͘ґଘ͢Δɻैདྷɺ෼཭ͨ̎͠૚ͷ೪ੑ܎਺͕౳͍͠৔߹ʹ͍ͭͯ‫͕͞ڀݚ‬Ε͖͕ͯͨɺ೪ੑ͕ҟͳΔ৔߹ʹ૬ͷߏ଄͕ͲͷΑ͏ʹͳΔ͔ɺ਺஋γϛϡϨʔγϣϯʹΑͬͯௐ΂Δɻࠓ೥౓͸ɺͦͷҝͷ‫ػࢉܭ‬ίʔυͷ։ൃΛߦ͍ɺ༧උతͳ݁ՌΛಘͭͭ͋Δɻ

8. ࡉ޸Λ༻͍ͨෆ‫ن‬ଇ෼‫࠯ذ‬ͷΩϟϥΫλϦθʔγϣϯ (ࡔ্):ɹߴ෼ࢠ࠯Λߏ੒͢ΔϞϊϚʔͷதʹɺ݁߹ख͕̏Ҏ্͋ΔՕॴ͕͋Δͱɺͦ͜Ͱ͸ࢬ෼͔Ε͕ൃੜ͢Δɻ͜ͷΑ͏ͳ෼‫͕ذ‬ෆ‫ن‬ଇʹଟ਺ଘࡏ͢Δ࠯Λෆ‫ن‬ଇ෼‫( ࠯ذ‬randomly branched polymer) ͱ͍͏ɻࡉ؅ (nano-channel) ಺ʹ߆ଋ͞Εͨෆ‫ن‬ଇ෼‫࠯ذ‬ͷඇࣗ໌ͳ੩తɺಈతੑ࣭͍ͭͯͷεέʔϦϯάଇΛߏங͠ɺͦͷ෺ཧత‫ݯى‬Λٞ࿦ͨ͠ɻ·ͨɺͦΕΛ‫ʹج‬ɺࡉ޸ (nano-pore) Λ༻͍ͨෆ‫ن‬ଇ෼‫࠯ذ‬ͷ৽ͨͳΩϟϥΫςϦθʔγϣϯ๏ΛఏҊͨ͠ɻɹʢF.

Brochard-Wyart (Institute Curie) ͱͷ‫ڞ‬ಉ‫ڀݚ‬ʣ
9. ߴ෼ࢠ࠯ͷࡉ޸௨ա‫ݱ‬৅ (ࡔ্):ɹߴ෼ࢠ࠯ͷࡉ޸௨ա‫ݱ‬৅ʹ͍ͭͯɺࡢ೥
౓·Ͱɺࡉ޸௨աલͷ෦෼ (cis-side) ͷΈʹண໨͢Δ͜ͱʹΑΓɺ͜ͷաఔΛ‫ه‬ड़͢ΔಈతεέʔϦϯάଇΛཱ͖֬ͯͨ͠ɻࠓ೥౓͸ɺ͜Ε·Ͱͷ‫Ͱڀݚ‬ߟྀ͞Εͯ͜ͳ͔ͬͨࡉ޸Λ௨աͨ͠෦෼࠯ͷޮՌ (trans-side eﬀect) ʹ͍ͭͯɺߴ෼ࢠ࠯ͷඇฏߧμΠφϛΫεͷҰൠ࿦ͷཱ৔͔Βٞ࿦Λߦͬͨɻͦͷ݁Ռɺࡢ೥౓·Ͱͷ݁Ռʹ༗‫ݶ‬αΠζิਖ਼ޮՌΛ༩͑Δ͜ͱ͕໌Β͔ʹͳͬͨɻʢᜊ౻ʢ‫ژ‬େ෱Ҫηϯλʔʣͱͷ‫ڞ‬ಉ‫ڀݚ‬ʣ

10. ήϧͷೞΕ (ࡔ্):ɹϚΠΫϩϝʔλεέʔϧͷඍখӷణ಺ʹೋछྨͷਫ༹ੑߴ෼ࢠʢPEG ͱθϥνϯʣΛ಺แͯ͠Թ౓ΛԼ͛Δͱೋ૬ʹ૬෼཭Λ‫ى‬104͜͢ɻߋʹԹ౓Λ௿Լ͢ΔͱɺθϥνϯͷήϧԽʹ൐͍ɺӷణશମ͕େ͖͘
ม‫ܗ‬Λ‫͢͜ى‬৔߹͕͋Δɻ͜͜Ͱ͸ɺήϧ૬ͱ PEG Ϧον૬ͱͷք໘ΤωϧΪʔͱήϧͷ஄ੑΤωϧΪʔͷ‫͕߹ڝ‬ॏཁͱͳΔɻ͜ͷ‫ݱ‬৅ΛɺήϧͷೞΕ (wetting) ͱ͍͏ࢹ఺͔Βߟ࡯͠ɺ࣮‫݁ݧ‬ՌͱͷൺֱΛߦͬͨɻʢ༄ᖒɺ୙઒ɺಖాʢ‫۝‬େʣͱͷ‫ڞ‬ಉ‫ڀݚ‬ʣ

11. ඇ૬༹ੑϒϨϯυͷަྲྀి৔ʹର͢ΔႩஅԠྗԠ౴ (ઃָɺࡔ্)ɿߴ෼ࢠ༹
ӷͷࠞ߹ӷମͳͲͷɺ૬෼཭ͨ͠ϒϨϯυʹγΞΛ͔͚ɺ଎౓ޯ഑ͷํ޲ʹަྲྀి৔Λ͔͚ͨͱ͖ͷႩஅԠྗͷԠ౴ͷ༷ࢠΛɺཧ࿦ͱ਺஋‫ࢉܭ‬Λ༻͍ͯղੳͨ͠ɻཧ࿦Ͱ͸̎૬ྲྀମͷߏ੒ํఔࣜΛ༩͑Δ౔ҪɺଠాΒͷཧ࿦Λ‫ʹݩ‬ɺి৔ͷޮՌΛऔΓೖΕͨߏ੒ํఔࣜΛಋग़ͨ͠ɻͦͷߏ੒ํఔࣜΛ‫ݩ‬ʹి৔ʹର͢ΔႩஅԠྗͷԠ౴ͷ༷ࢠΛ਺஋‫ʹࢉܭ‬Αͬͯௐ΂ͨͱ͜Ζɺ࣮‫֬Ͱݧ‬ೝ͞Ε͍ͯΔԠ౴ͷ༷ࢠͱఆੑతʹҰகͨ͠ɻ(ଠా (౦େ) ͱͷ‫ڞ‬ಉ‫)ڀݚ‬12. ஗ԆϑΟʔυόοΫΛ༻͍ͨ Turing ύλʔϯͷ੍‫( ޚ‬ઃָ)ɿޫ‫ײ‬डੑͷࢼༀΛ༻͍ͨ൓ԠͰ͋Δ CDIMA ൓Ԡͷ਺஋Ϟσϧʹ஗ԆϑΟʔυόοΫΛՃ͑Δ͜ͱͰɺTuring ύλʔϯͷ੍‫ޚ‬ΛࢼΈͨɻޫ‫ײ‬डੑͷޮՌ͸ઢ‫͠ͱܗ‬ɺͦͷ߲ʹ஗ԆϑΟʔυόοΫΛಋೖ͢Δɻ਺஋࣮‫ݧ‬ͷ݁Ռɺ࣌ؒ஗ΕͱϑΟʔυόοΫͷ‫͕͋౓ڧ‬Δ஋Λ௒͑Δͱ੩ࢭߏ଄͕ෆ҆ఆʹͳΓɺ఻ൖ΍ৼಈͳͲଟ࠼ͳৼΔ෣͍Λࣔ͢͜ͱ͕෼͔ͬͨɻ·ͨɺ੩ࢭঢ়ଶ͔Β఻ൖঢ়ଶ΁ͷ෼‫఺ذ‬Λৼ෯ํఔࣜͷཧ࿦ղੳΑΓ‫ٻ‬ΊɺͦΕ͕਺஋࣮‫ݧ‬ͷ݁Ռͱ΋Α͘Ұக͢Δ͜ͱΛࣔͨ͠ɻ(ೖ (౦େ)ɺ֎࡚ (ՖԦ)ɺଠా (౦େ) ͱͷ‫ڞ‬ಉ‫)ڀݚ‬13. αΠτ൓సͷ‫Ͱܥ‬ͷͻͶΓ‫ڥ‬ք৚݅ (෢‫ٱ‬ɺ໺ଜ)ɿS=1/2 εϐϯఐࢠ‫ͭʹܥ‬͍ͯɼܻ૬‫࣓ڧ͕༻࡞ޓ‬ੑʔ൓‫࣓ڧ‬ੑͷΑ͏ʹަସ͢Δ৔߹͸ɼϦϯΫʹର
͢Δۭؒ൓సରশੑ͕ͳΓͨͨͳ͍ɽ͕ͨͬͯ͠ Gaussian సҠͳͲΛܾΊΔͷʹ༗ޮͰ͋ͬͨͻͶΓ‫ڥ‬ք৚݅๏͕ͦͷ··Ͱ͸࢖͑ͳ͍ɽ͜ͷ໰୊ʹ͍ͭͯɼαΠτʹର͢ΔΔۭؒ൓సͱͻͶΓ‫ڥ‬ք৚݅Λཱ྆ͤ͞Δํ๏Λ‫ݟ‬ग़ͨ͠ɽ͜Ε͸ɼަସ࣓৔ͷ͋Δ໰୊΍ɼϑΣϦ࣓ੑͷ‫ʹܥ‬΋Ԡ༻͕Ͱ͖Δɽ

14. ϑϥετϨʔτͨ͠εϐϯ‫ܥ‬ͷ੔߹ʔඇ੔߹ભҠ (৿ॏɺ໺ଜ)ɿ࣍ۙ઀૬‫ޓ‬࡞༻ͷ͋Δ S=1/2 εϐϯ࠯ͰϘϯυަ୅ͷ͋Δ‫Ͱܥ‬ͷ੔߹ʔඇ੔߹ભҠʹ͍ͭͯɼ‫ڀݚ‬Λߦ͍ͬͯΔɽ

105

ൃද࿦จ

 ‫ݪ‬ஶ࿦จ 
1. Ryota Nishino, Takahiro Sakaue, and Hiizu Nakanishi, PLOS ONE 8(4)(2013) e60938; “Transcription ﬂuctuation eﬀects on biochemical oscillations”
2. Jun’ichi Wakou, Hiroyuki Kitagishi, Takahiro Sakaue, and Hiizu Nakanishi, Phys. Rev. E87 (2013) 042201 [11 pages]. “Inelastic collapse in onedimensional driven systems under gravity”
3. Sahin-Ichiro Nagahiro, Hiizu Nakanishi and Namiko Mitarai, EPL 104 (2013)
28002 [6 pages]. “Experimental observation of shear thickening oscillation”
4. Hiizu Nakanishi, Takahiro Sakaue, and Jun’ichi Wakou, J. Chem. Phys. 139,
214105 (2013)[11 pages]. “Hamilton-Jacobi method for molecular distribution function in a chemical oscillator”
5. T. Saito and T. Sakaue, Phys. Rev. E, 88, 042606:1-5 (2013). “Cis-transdynamical asymmetry in driven polymer translocation”
6. T. Sakaue and F. Brochard-Wyart, Macro Letters, 3, 194-197 (2014). “NanoporeBased Characterization of Branched Polymers”
7. R. Iri, Y. Tonosaki, K. Shitara, and T. Ohta, J. Phys. Soc. Jpn, 83 (2014)
024001:1-5. “Dynamics of Turing Pattern under Time-Delayed Feedback”

Proceedingsஶॻ

M. Yanagisawa, T. Sakaue and K. Yoshikawa, “Characteristic Behavior of Crowding
Macromolecules Conﬁned in Cell-Sized Droplets” (Chapter 7 in “New Models of the
Cell Nucleus: Crowding, Entropic Forces, Phase Separation and Fractals”, edited by R.
Hancock and K.W. Jeon, Academic Press), International Review of Cell and Molecular
Biology,307, 175-204 (2014).
ߨԋ ւ֎Ͱͷߨԋ 
1. Hiizu NAKANISHI, STATPHYS25, July 22-26, 2013, Seoul, Kore, “HamiltonJacobi analysis of molecular distribution function in a chemical oscillator”(oral)

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2. T. Sakaue, STATPHYS25, 2013/7/25 (Seoul, Korea) , “Statistics and Geometrical Picture of Ring Polymer Melts”ʢposterʣ3. Hiizu Nakanishi, Biocomplex seminar at NBI, University of Copenhagen,2013/9/11n “Storm in a Teacup: dynamics of micro-droplets on hot water
surface”
4. Mahito Ohata, Masatoshi Ichikawa and Hiizu Nakanishi, International Soft
Matter Conference 2013 September 15-19, 2013 at Rome, Italy, “Storm in a
Teacup: dynamics of micro-droplets on hot water surface”

 ࠃ಺Ͱͷߨԋ 
1. ࡔ্‫و‬༸ɺจ෦Պֶলɹੜ໋ಈଶγεςϜՊֶਪਐ‫఺ڌ‬ʮ֩಺ΫϩϚνϯɾϥΠϒμΠφϛΫεͷ਺ཧ‫఺ڌڀݚ‬ʯɺ޿ౡେֶɺ2013/7/12ɺʮછ৭ମͷߴ࣍ߏ଄ʙඥͷབྷΈ߹͍ͱ͍͏ࢹ఺͔Βʯ
2. ೔ຊ෺ཧֶձɹ 2013 ೥ळ‫ق‬େձɺ2013 ೥ 9 ݄ 25 ೔ʙ28 ೔ɺԙɿಙౡେֶ
(a) த੢लɼएੜ५Ұɼࡔ্‫و‬༸ɺʮϋϛϧτϯϠίϏ๏ʹΑΔԽֶ Fokker-Planckํఔࣜͷඇఆৗղʯ(b) ࡔ্‫و‬༸ɼத੢लɺʮք໘༳Β͗ʹ͓͚Δ‫ه‬ԱޮՌͱҟৗ֦ࢄʯ(c) ༄ᖒ࣮ึɼ୙઒৻ฏɼࡔ্‫و‬༸ɼಖాণ೭ɺʮϛΫϩӷణ಺Ͱͷߴ෼ࢠ༹ӷͷ૬෼཭ͱήϧԽʹΑΔύλʔϯ‫ܗ‬੒ʯ(d) ᜊ౻୓໵ɼࡔ্‫و‬༸ɺʮCrumpled Globule ʹ͓͚Δඪࣝ͞ΕͨϞϊϚʔͷҟৗ֦ࢄʯ
3. ୈ̍̍̕ճɹ೔ຊ෺ཧֶձɹ‫۝‬भࢧ෦ྫձɺԙ ‫ཹٱ‬ถ޻‫ۀ‬େֶ, 2013 ೥ 11 ݄ 30 ೔(a) ૔ຊཾ, த੢ल, ࡔ্‫و‬༸ɺʮคମଯੵ෺ͷৼಈϞʔυղੳʯ(b) தඌ޾, த੢लɺࡔ্‫و‬༸ɺʮԣྻٰ࠭ͷઢ‫҆ܕ‬ఆੑ ࣼΊ͔Β෩͕ਧ͍ͨ৔߹ʯ(c) ਫམ‫ݑ‬Ұ, ࡔ্‫و‬༸, த੢लʮtethered membrane ͷμΠφϛΫεʯ(d) ୙઒৻ฏ, ࡔ্‫و‬༸ɺಖాণ೭, ༄ᖒ࣮ึʮϚΠΫϩεέʔϧۭؒ಺Ͱͷߴ෼ࢠਫ༹ӷͷ૬෼཭ͱήϧԽʹΑΔύλʔϯ‫ܗ‬੒ʯ
4. ໺ଜ ਗ਼ӳɼԬຊ ਗ਼ඒ, རࠜ઒ ޹, ࡔҪ పɺྔࢠεϐϯ‫ڀݚܥ‬ձ (෱Ҫେֶ,2013 ೥
12 ݄ 14 ೔)ɺʮF-AF ladder(αΠτ൓సෆม) ‫Ͱܥ‬ͷͻͶΓ‫ڥ‬ք৚݅ͱύϦςΟʯ
5. ࡔ্‫و‬༸ɺ͓஡ͷਫঁࢠେֶ෺ཧֶՊɺ2014/2/4ɺ“Ring Polymer Melt” ɹɹɹ
6. ೔ຊ෺ཧֶձɹୈ 69 ճ೥࣍େձɺԙɿ౦ւେֶ, 2014 ೥ 3 ݄ 27 ೔ʙ30 ೔(a) ਫམ‫ݑ‬Ұɼத੢लɼࡔ্‫و‬༸ʮ໢ঢ়෼ࢠͷμΠφϛΫεʯ(b) Ӭ߂ਐҰ࿠ɼத੢लɼ‫ޚ‬खચࡊඒࢠʮͣΓ೪Խৼಈʹ͓͚Δෆ‫ۉ‬Ұ೪Խߏ଄ͷ࣮‫ݧ‬త‫؍‬ଌʯ(c) ࢢ઒ਖ਼හɼക໦ਸߒɼେാਅ඙ɼத੢लʮίʔώʔͷ౬‫ ؾ‬ʙු༡͢Δඍখਫణͱͦͷूஂফ໓ʙʯ(d) རࠜ઒޹ɼԬຊਗ਼ඒɼҾ‫ݪ‬ढ़࠸ɼࡔҪపɼ৿ॏॱฏɼ໺ଜਗ਼ӳɺʮܻ૬‫༻࡞ޓ‬͕ަ୅ͨ͠ҟํత S=1/2 ϥμʔͷ‫ج‬ఈঢ়ଶ IIʯ

107

(e) ໺ଜਗ਼ӳɼ৿ॏॱฏɼརࠜ઒޹ɼԬຊਗ਼ඒɼҾ‫ݪ‬ढ़࠸ɼࡔҪపɺʮܻ૬‫༻࡞ޓ‬͕ަ୅ͨ͠ҟํత S=1/2 ϥμʔͷ‫ج‬ఈঢ়ଶ IIIʯ(f) ᜊ౻୓໵ɼࡔ্‫و‬༸ɺʮ৳ு͞ΕΔߴ෼ࢠ࠯ͷա౉తաఔʹ͓͚Δ༳Β͗ʯ(g) ઃָ‫ګ‬ฏɼࡔ্‫و‬༸ɼଠాོ෉ɺʮඇ૬༹ੑϒϨϯυͷৼಈి৔ʹର͢ΔႩஅ
ԠྗԠ౴ʯ

֎෦ࢿۚ

 จ෦লՊֶ‫ڀݚ‬අิॿۚ 
1. த੢लɺ๖ժɺʮਫ໘্ͷඍখਫణͷੜ੒ɾු༡‫ͦͱߏػ‬ͷूஂӡಈɿίʔώʔͷ౬‫ؾ‬ͷ෺ཧֶʯʢ‫ڀݚ‬୅දʣ
2. ໺ଜɹਗ਼ӳɺ‫ج‬൫ (C) ʮྔࢠεϐϯ࠯ʹ͓͚Δ৽‫ح‬૬ͷਫ਼ີ୳ࡧͱϨϕϧεϖΫτϩείϐʔʯ(‫ڀݚ‬෼୲ऀ)
3. ࡔ্‫و‬༸ɺ‫ج‬൫ (B) ʮඇ૬༹ੑϒϨϯυͷి‫ؾ‬೪ੑޮՌʯ(‫ڀݚ‬୅ද)ֶ෦̐೥ੜଔ‫ڀݚۀ‬

1. ҆౻ɹେߊɺʮೋॏৼΓࢠͷॳ‫ظ‬஋Ӷහੑʯ
2. ޻౻ɹୡ໼ɺʮsite percolation ͱ invasion percolation ͷൺֱʯ
3. ळࢁɹཅฏɺʮΧΦε‫ي‬ಓͷγϛϡϨʔγϣϯʯम࢜࿦จ

1. ૔ຊ ཾɺʮคମଯੵதͷৼಈϞʔυղੳʯ
2. ਫམ ‫ݑ‬Ұɺʮ໢ঢ়ߴ෼ࢠͷμΠφϛΫεʯֶ֎Ͱͷֶձ‫׆‬ಈ

1. த੢लɺ೔ຊ෺ཧֶձ ୅ٞһɺ෺ੑҕһձ‫ࣄװ‬
2. ໺ଜਗ਼ӳɺ೔ຊ෺ཧֶձ ձࢽฤूҕһ108‫ڽ‬ॖ‫ܥ‬ཧ࿦‫ߏࣨڀݚ‬੒һՏ߹৳ ।‫ڭ‬त੒ਗ਼म ।‫ڭ‬त େֶӃ म࢜՝ఔ 
தଜॣ໵

෱೭্ະདྷ

 ֶ෦ ଔ‫ڀݚۀ‬ੜ 
݀Ҫ༤ଠ

ཷ৻Ұ࿕

୲౰त‫ۀ‬
෺ཧֶ I(Տ߹৳)ɺྗֶ‫ૅج‬ɾಉԋश (Տ߹৳)ɺ೤ͱ೾ಈ࿦‫( ૅج‬Տ߹৳)ɺ
෺ཧ਺ֶ II(Տ߹৳)ɺྗֶ‫ૅج‬ɾಉԋश (੒ਗ਼म)ɺ෺ཧֶ૯߹ԋश (੒ਗ਼म)ɺ
ඇઢ‫ܗ‬෺ཧֶ (੒ਗ਼म)‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ

Ge(111)c(2×8) ද໘ͷ҆ఆߏ଄ͱ४҆ఆߏ଄ (Տ߹৳ɺ݀Ҫ༤ଠ)Ge(111) ਗ਼ড়ද໘ͷ҆ఆߏ଄͸ɺc(2×8) ߏ଄Ͱ͋Δ͜ͱ͕ैདྷΑΓ஌ΒΕ͍ͯΔɻ
Ge(111)c(2×8) ද໘ʹ͸ɺϢχοτηϧ͋ͨΓɺ̐ͭͷΞυΞτϜͱ̐ͭͷϨετΞτ
Ϝ͕͋Δɻ͔͠͠ɺͦͷߏ଄ͷ೤త༳Β͗ʹ͍ͭͯ͸ɺ஌ΒΕ͍ͯͳ͍ɻզʑ͸ɺୈҰ‫ݪ‬ཧ‫͖ͮجʹࢉܭ‬ɺGe(111)c(2×8) ද໘ͷ҆ఆߏ଄Λ‫ٻ‬Ίͨɻ݁Ռ͸ɺ࣮‫ͱݧ‬Α͍ҰகΛࣔͨ͠ɻ͞ΒʹɺΞυΞτϜɺϨετΞτϜͷ‫ॴہ‬഑ஔΛม͑ͯɺୈҰ‫ݪ‬ཧ‫ࢉܭ‬ʹ‫ͮ͘ج‬४҆ఆߏ଄୳ࠪΛߦ͍ɺ̏ͭͷ४҆ఆߏ଄Λൃ‫ͨ͠ݟ‬ɻ̍ͭͷ҆ఆߏ଄ɺ̏
ͭͷ४҆ఆߏ଄ͷؒͰɺ̐ͭͷϨετΞτϜͷ഑ஔ͸ɺͦΕͧΕɺ̎஋తͳ഑ஔΛऔΔɻΞυΞτϜͷ഑ஔ͸ɺϨετΞτϜͷ഑ஔʹैଐ͢Δ͜ͱΛ໌Β͔ʹͨ͠ɻSn ‫ٵ‬ண Si(111) ද໘ͷஔ‫( ؕܽ׵‬Տ߹৳)√√Sn ‫ٵ‬ண Si(111) ද໘ͷ҆ఆߏ଄͸ɺ( 3 × 3) ߏ଄Ͱ͋Δͱ‫ݴ‬ΘΕ͍ͯΔɻ͜Ε͸ɺୈҰ‫ݪ‬ཧ‫ࢉܭ‬ͷ݁Ռͱ΋Ұக͢Δɻ͔͠͠ɺ௿Թ࣮‫Ͱݧ‬ͷ STM Λ࢖ͬͨɺిྲྀεϖΫτϧ࣮‫Ͱݧ‬͸ɺSn ͷߴ͕̎͞஋తʹΏͬ͘Γ༳Β͙͜ͱ͕ใࠂ͞Ε͍ͯΔɻ͜Ε͸ɺ√√( 3 × 3) ߏ଄ͱໃ६͢ΔɻैདྷΑΓɺSTM Ͱ Sn ‫ٵ‬ண Si(111) ද໘ʹ͸ɺSi ͷஔ‫ܽ׵‬109͕ؕଘࡏ͢Δ͜ͱ͕஌ΒΕ͍ͯΔɻզʑ͸ɺୈҰ‫ݪ‬ཧ‫ ͖ͮجʹࢉܭ‬Si ஔ‫͕͋ؕܽ׵‬Δ‫Ͱܥ‬ͷߏ଄‫ࢉܭ‬ΛߦͬͨɻSi ஔ‫ؕܽ׵‬ͷଘࡏ͕ Sn ഑ஔͷ̎஋ੑΛҾ͖‫໌͕ͱ͜͢͜ى‬Β͔ʹͳͬͨɻ͜Ε͸ɺఆੑతʹ͸࣮‫݁ݧ‬ՌΛ࠶‫͢ݱ‬Δɻ
‫ࡉ࢝ݪ‬๔ͷ৘ใॲཧγεςϜͷ‫ڀݚ‬/‫ڭ‬ҭ (੒ਗ਼मɺ௡ా൏)ຊςʔϚʹؔͯ͠ࠓ೥౓͸ɺ‫ڀݚ‬੒Ռͷग़൛Λ໨ඪͱ͓ͯ͠ΓɺϓϨϓϦϯταʔόʔͰͷެ։͸ୡ੒ͨ͠ɻֶज़ࡶࢽ΁ͷग़൛͸དྷ೥౓ͷ໨ඪͱ͢Δɻۙ೥໌Β͔ʹͳͬͨϛχ̧̣̖ͷ‫ػ‬ೳʹཱ‫͠٭‬ɺࡉ๔಺ͷ࠷΋‫࢝ݪ‬తͳ৘ใॲཧγεςϜΛ‫ߏʹ্ػࢉܭ‬ஙͨ͠ɻैདྷߟ͑ΒΕΔ͜ͱͷͳ͔ͬͨϔϦΧʔθ༷λϯύΫ࣭ͷಋೖʹΑΓɺटඌҰ؏ͨ͠ಈ࡞ͷϧʔϓΛดͤ͡͞Δ͜ͱ͕Ͱ͖ͨɻ
ΦʔτϙΠΤγεूஂͷਐԽೳͷ‫ڀݚ‬/‫ڭ‬ҭ (੒ਗ਼मɺদ౻߂‫)ڭ‬ຊςʔϚʹؔͯ͠ࠓ೥౓͸ɺ‫ڀݚ‬੒Ռͷग़൛Λ໨ඪͱ͍͕ͯͨ͠ɺ߲࣍ͷग़൛࡞‫ۀ‬Λ༏ઌͤͨͨ͞Ίະ࣮ͩߦͰ͖͍ͯͳ͍ɻग़൛࡞‫ۀ‬Λདྷ೥౓ͷ໨ඪͱ͢ΔɻΦʔτϙΠΤγεͱੜ໋ΛಉҰࢹ͢Δߟ͕͑͋Δ͕ɺΦʔτϙΠΤγε‫ܥ‬͸ਐԽೳΛ࣋ͨͳ͍ͷͰੜ໋ͱ͸‫͍ͳ͑ݴ‬ɻզʑ͸ΦʔτϙΠΤγεʹೝ஌‫ػ‬ೳΛ࣮૷ͯ͠ࡉ
๔ʹਐԽೳΛ࣋ͨͤͨɻ۩ମతʹ͸ࢷ࣭ೋॏບʹ‫ػ‬ೳੑλϯύΫ࣭ΛຒΊࠐΈɺ‫ڥ؀‬ͱͷ‫ڞ‬ਐԽΛՄೳʹͨ͠ɻ͜ΕΒͷࡉ๔ूஂͷਐԽγϛϡϨʔγϣϯΛߦͬͨɻΦϦΰϚʔϫʔϧυʹ͓͚ΔҨ఻ࢠෳ੡ͷ‫ݯى‬ͷ‫ڀݚ‬/‫ڭ‬ҭ (੒ਗ਼मɺࠤ౻େհ)ຊςʔϚʹؔͯ͠ࠓ೥౓͸ɺֶձൃද͓Αͼ‫ڀݚ‬੒Ռͷग़൛Λ໨ඪͱ͍ͯͨ͠ɻલ
ऀ͸ୡ੒͠ɺ‫ऀޙ‬͸ϓϨϓϦϯταʔόʔͰͷެ։͸ୡ੒ͨ͠ɻֶज़ࡶࢽ΁ͷग़൛͸དྷ೥౓ͷ໨ඪͱ͢Δɻੜ໋‫ݯى‬ͷԾઆͱͯ͠զʑ͕ఏএ͍ͯ͠ΔΦϦΰϚʔϫʔϧυͷ࿮૊Έʹ͓͍ͯɺҨ఻ࢠΛෳ੡͢ΔϝΧχζϜʹ͍ͭͯৄ͘͠ߟ࡯͠ɺ‫ݧ࣮ػࢉܭ‬ΛߦͬͨɻΦϦΰϚʔϫʔϧυʹ͓͚ΔΞφϩά৘ใͷ‫ڀݚ‬/‫ڭ‬ҭ (੒ਗ਼मɺதଜॣ໵)ຊςʔϚʹؔͯ͠ࠓ೥౓͸ɺम࢜࿦จͷ‫׬‬੒Λ໨ඪͱ͓ͯ͠Γୡ੒ͨ͠ɻདྷ೥౓͸ɺֶձൃද͓Αͼ‫ڀݚ‬੒Ռͷग़൛Λ໨ඪͱ͢Δɻ
߹੒ੜ෺ֶ΍ΞετϩόΠΦϩδʔʹ͓͍ͯ‫ࡉ࢝ݪ‬๔Λߏங͢Δࡍͷࢦ਑ͱͳΔΑ
͏ͳࡉ๔ϞσϧΛߟҊͨ͠ɻ‫ܗ‬ঢ়ۭؒΛ༻͍ͯσδλϧͳҨ఻ίʔυ͕੒ཱ͢ΔҎલͷΞφϩάͳ‫ࡉ࢝ݪ‬๔γεςϜΛΦϦΰϚʔϫʔϧυͷ࿮૊ΈͰ‫ͨ͠૷࣮ʹ্ػࢉܭ‬ɻ͜ͷࡉ๔γεςϜ͸৘ใͷղऍ߲ͱͳΓจ຺ґଘੑΛࣔ͢ɻ௒఻ಋΏΒ͗ཧ࿦ͷ‫( ڀݚ‬੒ਗ਼म)110ຊςʔϚʹؔͯ͠͸ɺ‫ܧ‬ଓతʹ‫͕ڀݚ‬ਐߦதͰ͋Δɻࠓ೥౓͸ɺ೤ྲྀʹର͢Δ Ward ߃౳ࣜͷ Feynman ਤʹΑΔਖ਼͍͠ཧղΛࣔ͠ɺϓϨϓϦϯταʔόʔʹެ։ͨ͠ɻ͜Ε·Ͱʹଘࡏͨ͠จ‫ݙ‬͸ɺ͜ΕΛཧղ͍ͯ͠ͳ͍ͷͰɺ΄ͱΜͲ͕‫ޡ‬ΓΛ‫ؚ‬Μͩ΋ͷͱͳ͍ͬͯΔɻ
ߴԹ௒఻ಋମͷϗʔϧޮՌͷཧ࿦ͷ‫( ڀݚ‬੒ਗ਼म)ຊςʔϚʹؔͯ͠͸ɺ‫ܧ‬ଓతʹ‫͕ڀݚ‬ਐߦதͰ͋Δɻ
ߴԹ௒఻ಋମͷਖ਼ৗۚଐ૬ʹ͓͚ΔϗʔϧޮՌͷཧ࿦͸ɺ௕೥ʹ౉ͬͯ࿦૪͕ଓ͍
͖ͯͨ໰୊Ͱ͕͋ͬͨɺ࠷΋఻౷తͳΞϓϩʔνΛ࠷΋஧࣮ʹ਱ߦ͢Δ͜ͱʹΑͬͯɺ࣮‫ݧ‬Λઆ໌͠ɺ͔ͭɺ࿦ཧతʹ΋टඌҰ؏ͨ͠ཧ࿦Λ‫׬‬੒ͤͨ͞ɻ‫ࡏݱ‬ɺ༌ૹ‫ݱ‬৅ͷ༷ʑͳఆࣜԽͷൺֱ‫ݕ‬౼Λߦ͍ɺզʑͷ݁Ռͷྺ࢙తҐஔ͚ͮΛఆΊͭͭ͋Δɻൃද࿦จ ͦͷଞͷ࿦จ 
Replication of proto-RNAs sustained by ligase-helicase cycle in oligomer world:
Daisuke Sato, Osamu Narikiyo
arXiv:1306.0199.
Translation by adaptor-helicase cycle in oligomer world:
Hayato Tsuda, Osamu Narikiyo
arXiv:1307.3857.
A Diagrammer’s Note on Superconducting Fluctuation Transport for Beginners: Supplement. Jonson-Mahan Transmutation:
Osamu Narikiyo
arXiv:1309.4257.

ߨԋ ࠃ಺Ͱͷߨԋ 
Replication of proto-RNAs sustained by ligase-helicase cycle in oligomer world:111ࠤ౻େհɺ੒ਗ਼म
ୈ 36 ճ೔ຊ෼ࢠੜ෺ֶձ೥ձ (2013 ೥ 12 ݄ 4 ೔)ֶ෦̐೥ੜଔ‫ڀݚۀ‬݀Ҫ༤ଠɿ(ࢦಋ‫ڭ‬һɺՏ߹৳)ɿGe(111)c(2x8) ߏ଄ʹ͓͚Δ࠷҆ఆߏ଄ͱ४҆ఆߏ଄ཷ৻Ұ࿕ɿ(ࢦಋ‫ڭ‬һɺ੒ਗ਼म)ɿԽֶ൓Ԡ‫ܥ‬ͷߦ͏‫ࢉܭ‬म࢜࿦จதଜॣ໵ɿ(ࢦಋ‫ڭ‬һɺ੒ਗ਼म): ΦϦΰϚʔϫʔϧυʹ͓͚Δ‫ࡉ࢝ݪ‬๔γεςϜֶ֎Ͱͷֶձ‫׆‬ಈՏ߹৳ɿ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ͷࢧ෦௕ͦͷଞͷ‫׆‬ಈͱ੒Ռ෺ཧֶ‫ࣨڭ‬໦༵ஊ࿩ձʮ͔͕ͨ Hubbard Ϟσϧ͞ΕͲ Hubbard Ϟσϧʯ(੒ਗ਼म)‫۝‬भେֶେֶӃཧֶ‫ڀݚ‬Ӄ෺ཧֶ෦໳ (2013 ೥ 10 ݄ 31 ೔)෺ੑίϩΩ΢ϜʮΠϯϑϨʔγϣϯӉ஦ͷΤϯτϩϐʔʯ(੒ਗ਼म)‫۝‬भେֶେֶӃཧֶ‫ڀݚ‬Ӄ෺ཧֶ෦໳෺ੑ‫ૅج‬࿦ (2013 ೥ 6 ݄ 11 ೔)ૉཻࢠཧ࿦ηϛφʔʮ͍·͞Β Ward ߃౳ࣜʯ(੒ਗ਼म)‫۝‬भେֶେֶӃཧֶ‫ڀݚ‬Ӄ෺ཧֶ෦໳ૉཻࢠཧ࿦ (2013 ೥ 12 ݄ 13 ೔)

112࣓ੑ෺ཧֶ
‫ߏࣨڀݚ‬੒һ࿨ా༟จ ‫ڭ‬तޫా‫ ߂ڿ‬।‫ڭ‬तઙ໺‫ڭॿ ߦو‬ େֶӃ म࢜՝ఔ കా ਅ࢙‫ࣷت‬৔ӳ‫ޗ‬߹໦ ༔༞ߴ‫߶ ݪ‬෱Ҫ തষ઒‫ ݟ‬༸Ұ࿠෍઒ ‫ࢤܟ‬

౻ຊ ޼

લ઒ Ղ࿕

҆Ӭ ྑࢠ

 ֶ෦ ଔ‫ڀݚۀ‬ੜ 
ߕ໦ ٛਓ

ాᬒ ޼༞

ࢁຊ ҏਧ

 ๚໰‫ ऀڀݚ‬ࡾଜ ޭ࣍࿠ʢେࡕ෎ཱେֶ޻ֶ‫ڀݚ‬Պ ।‫ڭ‬त)Alexander V. AndreevʢInstitute of Physics, Academy of Sciences, Prague, Czech
Republicʣྛ ޷Ұʢ౦๺େֶۚଐࡐྉ‫ ॴڀݚ‬।‫ڭ‬तʣ౵Ҫ ஐ࢚ (ߴً౓ޫՊֶ‫ڀݚ‬ηϯλʔ ෭ओ‫ڀݚװ‬һ)௕୩઒ ޼ (޿ౡେֶେֶӃ૯߹Պֶ‫ڀݚ‬Պ ॿ‫)ڭ‬େࢁ ‫( ࢘ݚ‬౦๺େֶۚଐࡐྉ‫ ॴڀݚ‬।‫ڭ‬त)୲౰त‫ۀ‬
ྗֶ‫ૅج‬ɾಉԋश (࿨ా༟จʣɺ෺ཧֶθϛφʔϧ (࿨ా༟จʣɺ෺ੑ෺ཧֶ II (࿨ా༟จʣɺ෺ཧֶ૯࿦ (࿨ా༟จʣɺ࣓ੑମ෺ཧֶ (࿨ా༟จʣɺྗֶ‫ૅج‬ɾಉԋश (ޫా‫߂ڿ‬ʣɺ෺ཧֶ૯߹࣮‫ݧ‬ʢޫా‫߂ڿ‬ʣɺࣗવՊֶ૯߹࣮‫ݧ‬ʢޫా‫߂ڿ‬ʣɺ෺ཧֶ૯߹࣮‫ݧ‬ʢઙ໺‫ߦو‬ʣ‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ
‫ڊ‬େ࣓‫ؾ‬೤ྔޮՌΛࣔ͢ Mn Խ߹෺Λ༻͍࣓ͨ‫ྫྷؾ‬ౚ࡞‫ۀ‬෺࣭ͷ։ൃʢ࿨ా༟จɺߴ‫߶ ݪ‬ɺ෍઒‫ࢤܟ‬ʣ

113

Fe2 P ‫ܕ‬Λ࣋ͭ (Mn,Fe)2 (P,Si) Խ߹෺͸‫ڊ‬େ࣓‫ؾ‬೤ྔޮՌΛࣔ͢ɽ͜ͷ෺࣭Λϕʔεͱ࣓ͨ͠‫ྫྷؾ‬ౚࡐྉͷ։ൃͱͦͷ෺ཧΛௐ΂͍ͯΔɽࡢ೥౓ͷ Ru ஔ‫ʹ׵‬Ҿ͖ଓ͖ɼࠓ
೥౓͸ Fe Λ Ni ΍ Cu Ͱஔ‫͍ͯͭʹܥͨ͠׵‬ௐ΂ɼͱ͘ʹ Ni ஔ‫ʹ׵‬ΑͬͯԹ౓ώεςϦγε͕େ෯ʹ‫ݮ‬গ͢Δ͜ͱΛ‫ݟ‬ग़ͨ͠ɽ·ͨԹ౓ώεςϦγεͷ෯ͱͻͣΈͷ૬ؔʹ͍ͭͯ΋ௐ΂ͨɽ͞Βʹ (Mn,Fe):(P,Si) ͷ࢓ࠐΈ૊੒ൺΛ 2:1 ͔Β (P,Si)-rich ʹͣΒ͢͜ͱʹΑͬͯɼෆ७෺૬ (MnFe)3 Si ͷੳग़͕཈͑ΒΕɼΩϡϦʔԹ౓ͷίϯτϩʔϧ͕༰қʹͳΔ͜ͱΛ໌Β͔ʹͨ͠ɽ‫ࡏݱ‬Պֶ‫ڀݚ‬අิॿۚͷަ෇Λड͚ͯɼߴਫ਼౓
࣓৔தࣔࠩ૸ࠪ೤ྔ‫ܭ‬Λ։ൃதͰ͋Δɽ
࣓৔த఻ಋ‫ݱ‬৅ͷ‫ڀݚ‬ʢ࿨ా༟จɺ߹໦༔༞ɺલ઒Ղ࿕ɺࢁຊҏਧʣ࠷ۙɺ࣓‫ؾ‬఍߅΍ϗʔϧޮՌͱ͍࣓ͬͨ৔தͰͷ఻ಋ‫ݱ‬৅ʹ‫ڵ‬ຯΛ࣋ͪɺ‫ڀݚ‬ΛਐΊ͍ͯΔɻର৅͸ 3d ిࢠ‫ܥ‬ͷวྺిࢠϝλ࣓ੑମ΍ 4f ిࢠ‫ܥ‬ͷՁ਺సҠ෺࣭Ͱ͋Δɽલऀʹ͍ͭͯ͸ࡢ೥ Co(S1−x Sex )2 ͷ࣓‫ؾ‬఍߅͕วྺిࢠϝλ࣓ੑసҠʹΑͬͯେ෯ʹ
૿Ճ͢Δ͜ͱΛ‫ݟ‬ग़ͨ͠ɽ͜Ε͸όϯυ෼‫ʹۃ‬Αͬͯ௨ৗͷৗ࣓ੑମ͔ΒϋʔϑϝλϦοΫͳ‫࣓ڧ‬ੑ΁ͷసҠʹΑΔ΋ͷͱߟ͍͑ͯΔ͕ɼҟৗϗʔϧޮՌ΋࣓৔தͰେ͖
ͳδϟϯϓΛࣔ͠ɼ͜ͷߟ͑Λࢧ͍࣋ͯ͠Δɽ·ͨ EuNi2 Si2 ͸ѹྗԼͰՁ਺సҠ͢Δ
͕ɼϗʔϧޮՌͷԹ౓ґଘੑʹ͓͍ͯϗʔϧ܎਺͕ෛ͔Βਖ਼΁ͱେ͖͘δϟϯϓ͢Δ
͜ͱΛॳΊͯ‫؍‬ଌͨ͠ɽ͜Ε͸Ձ਺సҠʹ൐͍఻ಋిࢠ਺͕มԽͨ͜͠ͱʹΑΔਖ਼ৗϗʔϧޮՌͷมԽͰ͋Δͱߟ͑ɼ‫ࡏݱ‬ղੳΛਐΊ͍ͯΔɽͦͷଞʹ EuNi2 P2 ͷ࣓‫ؾ‬఍߅ͷූ߸͕Թ౓ʹΑͬͯ൓స͢Δ͜ͱ΋‫ݟ‬ग़ͨ͠ɽՁ਺டংసҠ෺࣭ YbPd ͷ‫ڀݚ‬ʢޫా‫߂ڿ‬ɺ࿨ా༟จɺాᬑ޼༞ʣ

YbPd ͸ཱํথ CsCl ‫ߏܕ‬଄ͱ͍͏୯७ͳ݁থߏ଄Ͱ͋Γͳ͕Βɺ4 ͭͷ૬సҠΛࣔ͢෺࣭ͱͯ͠஌ΒΕɺͦͷ͏ͪͷ 3 ͭͷ૬సҠͷ‫͕ߏػ‬ෆ໌Ͱ͋ͬͨɻզʑ͸ SPring-8ͷ౵Ҫࢯɺ޿ౡେͷ௕୩઒ࢯΒͱͷ‫ڞ‬ಉ‫ Ͱڀݚ‬X ઢඇ஄ੑࢄཚ࣮‫ݧ‬Λߦ͕ͬͨɺͦ͜
͔Β‫ٻ‬ΊΒΕͨϑΥϊϯ෼ࢄؔ܎ʹ Yb ͷՁ਺༳ಈ͕ؔ༩͍ͯ͠Δ͜ͱ͕໌Β͔ʹͳͬͨɻ·ͨɺ͜ͷ෺࣭ͷ७ྑͳค຤ࢼྉΛಘΔ͜ͱ͕ࠔ೉Ͱ͕͋ͬͨɺ৽͍͠೤ॲཧํ๏
ʹΑΓค຤ X ઢճંϐʔΫ͕Ӷ͍ࢼྉΛಘΔ͜ͱʹ੒ޭͨ͠ɻ௿ԹͰଌఆͨ͠ͱ͜Ζɺ্ͷ૬సҠʹ൐ͬͯճંϐʔΫ͕෼྾͢Δ༷ࢠ͕‫؍‬ଌ͞Εͯ௿Թͷߏ଄Λ໌Β͔ʹ͢Δ͜ͱ͕Ͱ͖ͨɻདྷ೥౓͸͜ͷค຤ͷ७ྑԽΛਐΊͯɺΑΓৄࡉʹߏ଄Λௐ΂Δͱͱ΋ʹɺதੑࢠճંɺX ઢ‫ٵ‬ऩ΍ NMR ͳͲͷ‫ڞ‬ಉ‫ൃʹڀݚ‬ల͍ͤͯ͘͞༧ఆͰ͋Δɻ

EuTP(T=Pt,Pd) ͷՁ਺సҠ͓ΑͼՁ਺டংసҠͷ‫ڀݚ‬ʢޫా‫߂ڿ‬ɺ࿨ా༟จɺകా
ਅ࢙ɺ҆Ӭྑࢠʣ

EuPtP ͸ Eu ͷฏ‫ۉ‬Ձ਺͕Թ౓มԽ͠ɺಉ࣌ʹՁ਺டংߏ଄ͷप‫͕ظ‬มԽ͢Δಛҟͳ
114

෺࣭Ͱ͋Δɻࡢ೥౓ͷߴѹԼి‫ؾ‬఍߅ଌఆʹΑͬͯɺߴѹԼͰߋʹՁ਺͕มԽͯ͠৽
ͨͳՁ਺டংߏ଄͕ग़‫͍ͯ͠ݱ‬Δ͜ͱΛࣔࠦ͢Δ݁ՌΛಘͨͷͰɺຊ೥౓͸ SPring-8
ͷਫ຀ࢯɺՏଜࢯΒͱߴѹԼͰ X ઢ‫ٵ‬ऩ࣮‫ݧ‬Λߦ͍ɺߴѹɺ௿ԹԼͰՁ਺Λଌఆͨ͠ɻ
ѹྗҹՃͱ‫ʹڞ‬Ձ਺͸ 3 Ձํ޲΁γϑτ͍ͯ͠Δ͜ͱ͕໌Β͔ʹͳ͕ͬͨɺѹྗԼͰԹ౓ΛมԽͤͯ͞΋Ձ਺͸΄ͱΜͲมԽ͠ͳ͍͜ͱ͕෼͔ͬͨɻ·ͨɺEuPtP ͷ Pt αΠτΛ Pd Ͱஔ͖‫ ͨ͑׵‬EuPdP ࢼྉͷ࡞੡ʹ੒ޭͨ͠ɻ͜ͷࢼྉ͸ѹྗԼͷ EuPtP ͷৼ෣ΛৗѹԼͰ࣮‫͍ͯ͠ݱ‬Δ‫͋Ͱܥ‬Δͱ༧૝͞ΕΔɻৗѹͰ͸Ձ਺సҠͳͲͷҟৗ͸‫ݟ‬ΒΕͳ͔͕ͬͨɺߴѹԼͰ৽ͨͳ૬సҠ͕ग़‫͢ݱ‬Δ͜ͱ͕໌Β͔ʹͳͬͨɻདྷ೥౓
͸͜ͷৼ෣ΛΑΓৄࡉʹௐ΂Δͱͱ΋ʹɺؔ࿈෺࣭Ͱ͋Δ EuNiP ΍ EuPdAs ͷࢼྉ࡞੡Λ໨ࢦ͢ɻ

EuRh2 Si2 ‫͚͓ʹܥ‬Δ࣓৔༠‫ى‬Ձ਺సҠͷ఻ಋ‫ݱ‬৅ʢޫా‫߂ڿ‬ɺ࿨ా༟จɺ‫ࣷت‬৔ӳ‫ޗ‬ɺ౻ຊ޼ʣ

EuRh2 Si2 ͸ 1GPa ఔ౓ͷѹྗͰՁ਺సҠ͕༠‫͞ى‬ΕΔ͜ͱΛ౰άϧʔϓͰൃ‫ͨ͠ݟ‬ɻ͜ͷѹྗԼʹ͓͍ͯ͸ൺֱతऑ͍࣓৔ (∼ 7T) Ͱ΋Ձ਺సҠ͕༠‫͢ى‬Δ͜ͱ͕Θ͔Γɺ࣓৔༠‫ى‬Ձ਺సҠʹ͍༷ͭͯʑͳ෺ੑଌఆ͔Βௐ΂Δ͜ͱ͕Մೳʹͳͬͨɻզʑ͸ి‫఻ؾ‬ಋͷ‫͔఺؍‬ΒՁ਺సҠΛௐ΂Δ͜ͱΛ໨తͱͯ͠ɺѹྗԼͷ EuRh2 Si2 ͱৗѹԼͷ

Eu(Rh0.7 Ir0.3 )2 Si2 ͷ࣓‫ؾ‬఍߅ଌఆΛߦͬͨɻͦͷ݁Ռɺલऀ͸‫ࢠݪ‬ஔ‫׵‬Λߦ͍ͬͯͳ
͍ΫϦʔϯͳ‫͋Ͱܥ‬ΓɺՁ਺సҠʹΑΔ࣓‫ࢄؾ‬ཚͷ૿େ͓ΑͼɺߋͳΔ࣓৔ʹΑΔ࣓
‫ࢄؾ‬ཚͷ‫ݮ‬গʹΑ࣓ͬͯ‫ؾ‬఍߅ͷৼ෣Λઆ໌Ͱ͖ͨɻҰํɺ‫ऀޙ‬͸ Ir ஔ‫ʹ׵‬ΑΔϥϯμϜωεͷಋೖ͕࣓‫ؾ‬఍߅ͷৼ෣ʹӨ‫ڹ‬Λ‫͓ͯ͠΅ٴ‬ΓɺಛʹՁ਺సҠ͕‫͜ى‬Δલͷෛͷ࣓‫ؾ‬఍߅ͷ‫ݪ‬Ҽ͕Α͘Θ͔Βͳ͍ɻ͜ͷ෺࣭ʹ͍ͭͯ͸ɺύϧε‫࣓ڧ‬৔Λར༻ͨ͠Ձ਺ଌఆ͓Αͼ࣓‫ؾ‬ԁೋ৭ੑଌఆΛ౦๺େۚ‫ݚ‬ͷ໐ւࢯΒͱߦ͓ͬͯΓɺ࣍೥౓͸ͦΕΒͷ݁ՌΛ‫ؚ‬Ί࣓ͯ‫ؾ‬఍߅ͷৼ෣ʹ͍ͭͯղ໌Λ໨ࢦ͢ɻΫϩϛζϜԽ߹෺ͷ࣓ੑʢઙ໺‫ߦو‬ɺ෱Ҫതষʣ֎෦͔Βͷ༷ʑͳܹࢗʹΑΓ෺࣭ͷ৭͕Մ‫ٯ‬తʹมԽ͢ΔΫϩϛζϜ‫ݱ‬৅Λ༗͢ΔϞϦϒσϯࢎίόϧτʢCoMoO4 ʣʹ஫໨ͨ͠ɻ͜ͷ෺࣭͸ɺ͜Ε·Ͱதੑࢠճં΍ൺ೤ଌఆʹΑͬͯ௿ԹͰͷ࣓‫ߏؾ‬଄͕ใࠂ͞Ε͍ͯΔ͕ɺৄࡉͳ࣓ੑʹ͍ͭͯ͸΄ͱΜͲ໌Β͔ʹ͞Ε͍ͯͳ͍ɻͦ͜Ͱɺ৭ͷมԽʹ൐͏࣓‫ؾ‬ҟৗͷ༗ແΛ‫؍‬ଌ͢ΔͨΊ࣓Խ཰ͷԹ౓ґଘੑɺ௿ԹͰͷ࣓ੑΛղ໌͢ΔͨΊ࣓Խաఔ΍ൺ೤ଌఆͳͲͷ෺ੑଌఆΛߦͬͨɻͦͷ݁Ռɺ‫ظ‬଴͍ͯͨ͠৭ͷมԽʹ൐͏࣓‫ؾ‬తੑ࣭ͷҟৗ͸࢒೦ͳ͕Β‫؍‬ଌ͢Δ͜ͱ͸Ͱ͖ͳ͔ͬͨɻ͔͠͠ɺൺ೤ଌఆ΍࣓Խաఔʹ͓͍ͯɺա‫ʹڈ‬ใࠂ͞Ε࣓ͨ‫ߏؾ‬଄Λࢧ࣋͢Δ݁Ռ͕ಘΒΕͨɻಛʹɺ࣓৔தൺ೤ͷԹ౓ґଘੑͷ࣮‫͍͓ʹݧ‬ͯɺಛҟͳ 3 ͭͷஞ࣓࣍‫ؾ‬సҠΛ‫؍‬ଌͨ͠ɻ·ͨɺ࣓Խաఔʹଟஈ࣓Խεςοϓ͕‫؍‬115

ଌ͞Ε͍ͯΔ͜ͱͳͲ͔Βɺ࣓৔༠‫ى‬ͷ৽͍͠ྔࢠ‫ڽ‬ॖ૬͕ଘࡏ͍ͯ͠Δ͜ͱ͕‫ظ‬଴͞ΕΔɻࠓ‫ޙ‬ɺ࣓‫ڞؾ‬໐΍தੑࢠࢄཚ࣮‫ݧ‬౳ʹΑΔඍࢹతଌఆʹ͓͍࣓ͯ‫ؾ‬తੑ࣭ͷղ໌ΛࢼΈ͍ͨɻ
ࡾ࣍‫ݩ‬൓‫࣓ڧ‬ੑମͷ࣓‫رؾ‬ऍޮՌʢઙ໺‫ߦو‬ɺߕ໦ٛਓʣ

RbMnF3 ͸ɺ࣓ੑΠΦϯͰ͋Δ Mn2+ (S=5/2) ͕୯७ཱํ֨ࢠΛ‫ܗ‬੒ͨ͠ࡾ࣍‫ݩ‬ϋΠθϯϕϧά൓‫࣓ڧ‬ੑଳͷ୅දతͳϞσϧ෺࣭ͷҰͭͰ͋ΔɻύʔίϨʔγϣϯೱ౓ (cp )ΑΓ͞Βʹ‫ر‬ऍͨ͠ RbMnc Mg1−c F3 Ͱ͸ɺগ਺ (༗‫ݸ )ݶ‬ͷ Mn2+ ΠΦϯ͕൓‫࣓ڧ‬ੑతʹ݁߹ͨ͠εϐϯΫϥελʔΛ‫ܗ‬੒͠ϥϯμϜʹ෼෍͍ͯ͠Δɻ͜Ε·Ͱɺ‫رʹ୺ۃ‬ऍͨ͠ RbMn0.03 Mg0.97 F3 ͷ࣓ԽଌఆΛύϧε࣓৔Λ༻͍ͯߦͬͨͱ͜Ζɺ࣓Խ M (H)‫࣓ͼٴ‬Խͷ࣓৔ඍ෼ dM /dH ‫ۂ‬ઢ͔Β໌Β͔ʹ 10 ‫ݸ‬ͷεςοϓঢ়ͷҟৗ͕‫؍‬ଌ͞Εɺಛʹ dM /dH ‫ۂ‬ઢʹ͸ΑΓଟ͘ͷඍࡉߏ଄ϐʔΫ͕‫؍‬ଌ͞Εͨɻͦͷ‫ݯى‬Λ໌Β͔ʹ͢ΔͨΊɺҟͳΔ‫ر‬ऍೱ౓ͷࢼྉΛ߹੒ͱύϧε࣓৔ͱಉ͡‫ݱ‬৅ͷ‫؍‬ଌ͕‫ظ‬଴͞ΕΔަྲྀ࣓Խ཰ͷଌఆΛ։࢝ͨ͠ɻͦͷ݁Ռɺύεϧ࣓৔ԼͰͷ࣓Խաఔͷඍࡉߏ଄Λަྲྀ࣓Խ཰ଌఆͰ΋‫؍‬ଌ͠ɺ‫ر‬ऍೱ౓ͷ૿Ճʹ൐͍ඍࡉߏ଄ϐʔΫ͕઱໌ʹ‫ݱ‬ΕΔ͜ͱ
֬ೝͨ͠ɻࠓ‫ޙ‬ɺ޿ൣͳԹ౓‫࣓ͼٴ‬৔ྖҬʹ͓͍ͯଌఆΛ࣮ࢪ͢Δ༧ఆͰ͋Δɻൃද࿦จ ‫ݪ‬ஶ࿦จ 
Charge Density Wave and Superconductivity of RPt2 Si2 (R = Y, La, Nd, and Lu):
Yutaro Nagano, Nobutaka Araoka, Akihiro Mitsuda, Hideki Yayama, Hirofumi Wada,
Masaki Ichihara, Masahiko Isobe and Yutaka Ueda
J. Phys. Soc. Japan vol. 82 (2013) 064715.
Origins of Phase Transitions in Valence Fluctuating YbPd:
Akihiro Mitsuda, Masaki Sugishima, Takumi Hasegawa, Satoshi Tsutsui, Masahiko
Isobe, Yutaka Ueda, Masayuki Udagawa, Hirofumi Wada
J. Phys. Soc. Japan 82 (2013) 084712.
Valence transition induced by pressure and magnetic ﬁeld in antiferromagnet EuRh2 Si2 2:
Akihiro Mitsuda, Suguru Hamano and Hirofumi Wada
J. Korean Phys. Soc. 62 (2013) 1787-1791.

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Phase diagram and Eu valence state in EuPtP1−x Asx :Masaki Sugishima, Akihiro Mitsuda and Hirofumi Wada J. Korean Phys. Soc. 62(2013) 2019-2023 ͦͷଞͷ࿦จ ࣨԹ࣓‫ྫྷؾ‬ౚࡐྉͱͯ͠ͷ Mn Խ߹෺:࿨ా༟จɼย‫ߴۅ‬େ
೔ຊ AEM ֶձࢽ ୈ 21 ‫ר‬, ୈ 1 ߸,ʢ2013ʣ46-51.

ߨԋ ւ֎Ͱͷߨԋ 
Magnetocaloric Eﬀect and Magnetoresistance due to Itinerant Electron Metamagnetictransition in Co(S1−x Sex )2 :Hirofumi Wada, Daichi Kawasaki and Yoshiro Maekawa
International Symposium on Frontiers in Materials Science (FMS2013), Hanoi ࠃ಺Ͱͷߨԋ ‫ྨ౔ر‬Խ߹෺ɾ࣓‫ྫྷؾ‬ౚࡐྉͷ෺ཧͱ์ࣹޫϝεό΢Ξʔ෼ޫ๏΁ͷ‫ظ‬଴:࿨ా༟จ
ୈ 1 ճઌਐత์ࣹޫϝεό΢Ξʔ෼ޫ‫ڀݚ‬ձిࢠͷடংԽ‫ݱ‬৅ ʕՁ਺டংͱిՙີ౓೾ʕ:࿨ా༟จ೔ຊۚଐֶձ‫۝‬भࢧ෦ɾ೔ຊమ߯‫ڠ‬ձ‫۝‬भࢧ෦ ୈ 293 ճࡐྉՊֶஊ࿩ձ

(Mn,Fe,X)2−δ (P,Si)(M=Ni,Cu) ͷ࣓‫ؾ‬೤ྔޮՌͱ࣓‫ؾ‬తੑ࣭:ߴ‫߶ݪ‬ɼ࿨ా༟จɼย‫ߴۅ‬େ೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձߗ X ઢޫిࢠ෼ޫʹΑΔ EuNi2 (Si1−x Gex )2 (x =0.70, 0.79, 0.82) ͷԹ౓༠‫ى‬Ձ਺సҠͷ‫ڀݚ‬:

117ࢢ໦উ໵ɼࡾଜޭ࣍࿠ɼ҆ᜊଠཅɼ‫޾޹ॅڕ‬ɼຊฒ఩ɼখྛେ༞ɼࠤ౻ਔɼ಺ւ༗‫ر‬ɼ্ాໜయɼޫా‫߂ڿ‬ɼ࿨ా༟จɼా‫޿޾ޱ‬ɼౡా‫ݡ‬໵ɼੜఱ໨തจɼ୩‫ޱ‬խथ೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձ

Eu(Rh1−x Mx )2 Si2 (M=Ir,Co) ʹ͓͚ΔԽֶతѹྗ‫࣓ͼٴ‬৔ޮՌ:‫ࣷت‬৔ӳ‫ޗ‬ɼ඿໺୎ɼޫా‫߂ڿ‬ɼۙ౻ߊ߂ɼۚಓߒҰɼਫ຀ਔҰ࿕ɼ৽ాਗ਼จɼ࿨ా
༟จ೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձ୯݁থ EuNi2 Ge2 ͷѹྗԼͰͷϗʔϧޮՌଌఆ:߹໦༔༎ɼޫా‫߂ڿ‬ɼ࿨ా༟จ
೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձ

EuPtP ͷѹྗԼ X ઢ‫ٵ‬ऩ෼ޫ:കాਅ࢙ɼᚸುӫथɼޫా‫߂ڿ‬ɼਫ຀ਔҰ࿕ɼՏଜ௚‫ݾ‬ɼੴদ௚थɼ౉ลਅਔɼ࿨ా
༟จ೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձՁ਺సҠΛࣔ͢ Eu ‫ܥ‬Խ߹෺ͷ NMR ʹΑΔ‫ڀݚ‬:੢୩޹ೋɼਫ‫ؽށ‬ɼໂా‫׮‬໻ɼখࢁַलɼ্ాޫҰɼখ‫෉޹ݪ‬ɼޫా‫߂ڿ‬ɼਿౡਖ਼थɼ
࿨ా༟จ೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձ

CoMoO4 ͷ࣓‫ؾ‬తੑ࣭ͱΫϩϛζϜ੍‫ޚ‬:෱Ҫതষɼ‫ٱ‬อࠀོɼઙ໺‫ߦو‬ɼ࿨ా༟จɼॾ෋େथɼҴ֞༞࣍ɼՏߐୡ໵ɼࡾాູɼ
দඌথɼۚಓߒҰɼࠤ౻୎೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձೋஈՁ਺டংసҠΛࣔ͢ EuPtP ͷߴѹޮՌ:ޫా‫߂ڿ‬ɼകాਅ࢙ɼᚸುӫथɼদྛ࿨޾ɼਫ຀ਔҰ࿕ɼՏଜ௚‫ݾ‬ɼੴদ௚थɼ্চ
ඒ໵ɼ౉ลਅਔɼ࿨ా༟จ
೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձ

(La, Pt)-NMR ʹΑΔ LaPt2 Si2 ͷిՙີ౓೾ͱ௒఻ಋͷ‫ڀݚ‬:‫ٱ‬อప࿠ɼ໦࡚ହӳɼখख઒߃ɼ౻लथɼӬ໺༤ଠ࿠ɼߥԬ৴ོɼޫా‫߂ڿ‬ɼ࿨ా༟จ

118

೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձΫϩϛοΫԽ߹෺ CuMoO4 ͷ࣓ੑͱ݁থཻ‫ܘ‬ͷ૬ؔ:ઙ໺ ‫ߦو‬, ෱Ҫതষ, ‫ٱ‬อࠀོ, ࡾాູ, দඌথ, ۚಓߒҰ, ຀੉‫ܓ‬ਖ਼, ҏ౻རॆ೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձ

Cu2 O(SO4 ) ͷߏ଄ͱ࣓‫ؾ‬తੑ࣭:઒‫ݟ‬༸Ұ࿠, ෱Ҫതষ, ઙ໺‫ߦو‬, ࿨ా༟จ, Ҵ֞༞࣍, Տߐୡ໵, দඌথ, ۚಓߒҰ೔ຊ෺ཧֶձ ୈ 119 ճ‫۝‬भࢧ෦ྫձ

֎෦ࢿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚɺ௅ઓత๖ժ
࣓‫ؾ‬೤ྔޮՌଌఆͷͨΊͷߴਫ਼౓࣓৔தࣔࠩ૸ࠪ೤ྔ‫ܭ‬ͷ։ൃ‫ڀݚ‬୅දऀɿ࿨ా༟จ
೔ຊֶज़ৼ‫ڵ‬ձՊֶ‫ڀݚ‬අิॿۚɺ‫ج‬൫ C(Ұൠ)Ձ਺సҠɾՁ਺டংʹ஫໨ͨ͠Ϣʔϩϐ΢ϜԽ߹෺ͷ৽‫ح‬෺ੑ୳ࡧͱ‫ߏػ‬ղ໌‫ڀݚ‬୅දऀɿޫా‫߂ڿ‬೔ຊֶज़ৼ‫ڵ‬ձՊֶ‫ڀݚ‬අิॿۚɺ‫ج‬൫ C(Ұൠ)ෳ߹‫ڥ؀‬Լʹ͓͚ΔϞϦϒσϯࢎಔͷϚϧνΫϩϛζϜͷߏஙͱΫϩϛζϜཻ‫ܘ‬ґଘੑ‫ڀݚ‬୅දऀɿઙ໺‫ߦو‬ จ෦লՊֶ‫ڀݚ‬අิॿۚҎ֎ͷ֎෦ࢿۚ 
JST A-STEP FS εςʔδ γʔζ‫ࡏݦ‬ԽλΠϓ࣓‫ۭؾ‬ௐγεςϜ։ൃͷͨΊͷ೤ަ‫ߏػ׵‬ͷ‫ڀݚ‬‫ڀݚ‬୅දऀ:ࢁԼ‫ܟ‬Ұ࿕

NEDO ҕୗࣄ‫ۀ‬ʮলΤωϧΪʔֵ৽ٕज़։ൃࣄ‫ۀ‬ʯઌಋ‫ڀݚ‬࣓‫ؾ‬ώʔτϙϯϓٕज़ͷ‫ڀݚ‬։ൃ119‫ڀݚ‬୅දऀ:ฏ໺௚थଞେֶͰͷ‫ڭͱڀݚ‬ҭ࿨ా༟จɿ෱Ԭେֶཧֶ෦Ͱ‫ݶۃ‬෺࣭ՊֶͷߨٛΛ൒‫୲ظ‬౰ͨ͠ɽֶ෦̐೥ੜଔ‫ڀݚۀ‬ߕ໦ ٛਓɿ
ʢࢦಋ‫ڭ‬һɺઙ໺‫ߦو‬ʣ
ɿRbMnF3 ͷ࣓‫رؾ‬ऍޮՌాᬒ ޼༞ɿ
ʢࢦಋ‫ڭ‬һɺޫా‫߂ڿ‬ʣɿՁ਺டংసҠΛࣔ͢ YbPd ͷ७ྑค຤ࢼྉ࡞੡ࢁຊ ҏਧɿ
ʢࢦಋ‫ڭ‬һɺ࿨ా༟จʣ
ɿՁ਺༳ಈ෺࣭ EuNi2 P2 ͷ఻ಋ෺ੑम࢜࿦จ
ɿEuTP(T=Pt,Pd) ʹ͓͚ΔՁ਺సҠɾՁ਺டংసകా ਅ࢙:ʢࢦಋ‫ڭ‬һɺޫా‫߂ڿ‬ʣҠͷѹྗޮՌ
‫ࣷت‬৔ ӳ‫ޗ‬: (ࢦಋ‫ڭ‬һɺޫా‫߂ڿ‬ʣɿ੩ਫѹ‫ͼٴ‬Խֶతѹྗ༠‫ى‬Ձ਺సҠΛࣔ͢

EuRh2 Si2 ʹ͓͚Δ ࣓৔ޮՌ߹໦ ༔༎ɿ
ʢࢦಋ‫ڭ‬һɺ࿨ా༟จʣ
ɿEuNi2 Ge2 ͷѹྗԼϗʔϧޮՌߴ‫߶ ݪ‬ɿʢࢦಋ‫ڭ‬һɺ࿨ా༟จʣ
ɿҰ࣓࣍‫ؾ‬૬సҠԽ߹෺ (Mn,Fe,X)2−δʢP,Si) (X=Ni,Cu)ͷ࣓ੑͱ࣓‫ؾ‬೤ྔޮՌ෱Ҫ തষɿ
ʢࢦಋ‫ڭ‬һɺઙ໺‫ߦو‬ʣɿ ΫϩϛοΫԽ߹෺ CoMoO4 ͷ࣓‫ؾ‬తੑ࣭֎ࠃਓཹֶੜͷड͚ೖΕֶ֎Ͱͷֶձ‫׆‬ಈ࿨ా༟จɿ೔ຊ෺ཧֶձ ୈ 69 ‫ظ‬ɹ୅ٞһ࿨ా༟จɿ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ҕһͦͷଞͷ‫׆‬ಈͱ੒Ռ࿨ా༟จɿElsevier ࣾ Physica B ΤσΟλʔ࿨ా༟จɿ‫࣓ڧ‬৔ϑΥʔϥϜ ‫ࣄװ‬࿨ా༟จɿ‫۝‬भେֶ௿Թηϯλʔ௕࿨ా༟จɿ‫۝‬भେֶ৽Ωϟϯύε‫ܭ‬ըઐ໳ҕһ࿨ా༟จɿ‫۝‬भେֶཧֶ෦෇ଐ‫ۃ‬௿Թ࣮‫ࣨݧ‬௕ޫా‫߂ڿ‬ɿ‫۝‬भେֶ௿ԹηϯλʔӡӦҕһ120

ޫా‫߂ڿ‬ɿ‫۝‬भେֶཧֶ෦ෟଐ‫ۃ‬௿Թ࣮‫ࣨݧ‬ӡӦҕһޫా‫߂ڿ‬ɿ‫۝‬भେֶཧֶ෦লΤωϧΪʔରࡦҕһձҕһޫా‫߂ڿ‬ɿ‫۝‬भେֶཧֶ෦େֶઆ໌ձҕһઙ໺‫ߦو‬ɿ‫۝‬भେֶཧֶ෦෦໳ࢧԉࣨ૬ஊһઙ໺‫ߦو‬ɿ‫۝‬भେֶཧֶ෦ෟଐ‫ۃ‬௿Թ࣮‫ࣨݧ‬ӡӦҕһઙ໺‫ߦو‬ɿ‫۝‬भେֶཧֶ෦ֶੜੜ‫׆‬૬ஊҕһ121ྔࢠඍখ෺ੑʢ൒ಋମ෺ཧʣI‫ߏࣨڀݚ‬੒һ౉෦ߦஉ ‫ڭ‬तߥҪɹ‫ ؽ‬।ॿ‫ڭ‬୲౰त‫ۀ‬
෺ੑ෺ཧֶ IIIʢ౉෦ʣ‫ࢠݪ‬෼ࢠͷ෺ཧֶʢ౉෦ʣి࣓‫ ֶؾ‬IIʢ౉෦ʣ൒ಋମ෺ཧֶʢେֶӃʣʢ౉෦ʣ
શֶ‫ڞ‬௨‫ڭ‬ҭ ྗֶ‫ૅج‬ಉԋश (ि 2 ճ:ҏ౎)ʢ౉෦ʣ
શֶ‫ڞ‬௨‫ڭ‬ҭ ‫ݱ‬୅෺ཧ (޻ֶ෦:ҏ౎)ʢ౉෦ʣ
શֶ‫ڞ‬௨‫ڭ‬ҭ ‫ݱ‬୅෺ཧ (ཧֶ෦:ҏ౎)ʢ౉෦ʣ
શֶ‫ڞ‬௨‫ڭ‬ҭ ෺ཧֶ 3 ‫ ظޙ‬1/4ʢ౉෦ʣߴ೥࣍‫ڭ‬ཆɹ ࣗવՊֶ֓࿦ લ‫ ظ‬1/4ʢ౉෦ʣ࠷ઌ୺෺ཧֶʢֶ෦ 3 ೥ΦϜχόε 1 ճ෼ʣʢ౉෦ʣ
෺ཧֶ࣮‫ݧ‬ʢલ‫ظ‬ʣʢߥҪʣ෺ཧֶ࣮‫ݧ‬ʢ‫ظޙ‬ʣʢߥҪʣ‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ

(1) ‫ڧ‬༠ిମࢎԽ෺ͷ૬సҠͰͷ఻ಋҟৗͷղ໌ʢ౉෦ʣɿ
BaTiO3 ͷ૬సҠͰͷ఻ಋҟৗଌఆ‫ܥ‬ͷԹ౓੍‫Ͳͳޚ‬ͷਫ਼ີԽͱภޫಉ࣌‫࡯؍‬Λߦͬͨɻ(2) ‫ڧ‬༠ిମࢎԽ෺ͷද໘ిࢠ૚ͷ֬ఆʢ౉෦ʣ:BaTiO3 ୯݁থͷද໘఻ಋɿࢎԽ෺‫ڧ‬༠ిମ͸ɺ൓ి৔ͷӨ‫ڹ‬͸ɺ‫ۃ‬ബԽ͢ΔͱਙେͰɺ
Ԡ༻্΋ॏཁͳ໰୊Ͱ͋Δɻզʑ͸ɺ͜ͷΑ͏ͳ‫ڊ‬େͳిք͕͋Δͱɺ‫ڧ‬༠ిମͷ࠷ද໘͸୯७ͳઈԑମͱ‫ͱ͍ͳͤͳݟ‬ఏҊ͠ɺॳ‫ߴͯ͠ͱূݕظ‬ਅۭதͰ BaTiO3 ͷද໘఻ಋΛଌఆ͠ɺࢧ࣋͢Δ݁ՌΛಘ͍ͯΔɻ͜ͷཱ৔͔Βɺ൓ిքཧ࿦Λ‫ݟ‬௚͠ɺैདྷཱ֬ͨ͠ͱߟ͑ΒΕ͍ͯΔ‫ڧ‬༠ిମͷ̍̔̌ ˃෼Ҭͷཧ࿦Λ‫ݟ‬௚ͨ͠࡞ͬͨཧ࿦Λ122ࡢ೥ʹҾ͖ଓ͖վྑͨ͠ɻ
དྷ೥౓ɺ(3) ͷ݁Ռͱ૯߹ͯ͠ɺ‫ࢠݪ‬ϨϕϧͰ੍‫ڧͨ͠ޚ‬༠ిମࢎԽ෺ͷද໘ిࢠ૚ͷ෺ੑղ໌͢Δɻ(3) ௒ߴਅۭ AFM ʹΑΔද໘‫ڀݚ‬ʢ౉෦ʣɿ௒ߴਅۭ AFM ʹΑΓ௒ਗ਼ড়ͳද໘ͷ෼ҬΛଌఆ͠ɺैདྷͷ෼Ҭཧ࿦Ͱ͸આ໌Ͱ্͖ͣ
‫ه‬ͷࣗ෼ͨͪͷཧ࿦ʹ߹͏͜ͱΛൃ‫ͨ͠ݟ‬ɻདྷ೥౓ɺ༠ిମͷ̍̔̌ ˃෼Ҭͷཧ࿦ͷվగཧ࿦ͷఏग़Λߦ͏ɻ(4) ද໘ʹΑΒͳ͍όϧΫ఻ಋͷΈʹΑΔ੔ྲྀ‫ݱ‬৅ͷൃ‫ͱݟ‬ཧ࿦ʢ౉෦)ɿ
͜ͷ੔ྲྀ‫ݱ‬৅ͷཧ࿦Λͭ͘Γ࣮‫݁ݧ‬ՌΛৄࡉʹ࠶‫͖ͨͰݱ‬ɻདྷ೥౓ɺࢎԽ෺‫ڧ‬༠ిମ୯݁থͷ૬సҠͰͷ఻ಋҟৗͱ‫ڧ‬༠ిମΤϐλΩγϟϧബບͷ఻ಋҟৗͷͷղ໌ʹ༻͍Δ༧ఆͰ͋Δɻ(5) ४प‫ߏظ‬଄ଟ૚ບͷ೤఻ಋʢߥҪʣɿ४प‫ߏظ‬଄ଟ૚ບͷ೤఻ಋ‫ڀݚ‬Λਪਐ͍ͯ͠Δɻ௒఻ಋ઀߹̼̠ྫྷౚ‫ػ‬ͷஅ೤ͷͨΊͷ‫ͱڀݚૅج‬४प‫ߏظ‬଄Ͱͷ೤఻ಋ‫ڀݚ‬Λ௨ͯ͡४प‫ߏظ‬଄Ͱͷ෺ੑ‫ڀݚ‬Λͳ͢͜ͱΛҙਤ͍ͯ͠Δɻ࣮‫ݧ‬తʹ‫͢ڀݚ‬ΔͨΊʹࠓ೥౓࠾୒͞Εͨ௅ઓత๖ժ‫ڀݚ‬Պ‫ݚ‬අͰ੡࡞͢Δ४प‫ߏظ‬଄ଟ૚ບ࡞੡૷ஔ΍೤఻ಋ཰ଌఆ૷ஔͷઃ‫ܭ‬Λͨ͠ɻ·ͨɺ‫ػࢉܭ‬γϛϡϨʔγϣϯΛ४උ͍ͯ͠Δɻ(6) ϏεϚε‫ߴܥ‬Թ௒఻ಋମͷ୯݁থதͷ௒Ի೾ͷԻ଎ଌఆʹؔ͢Δ࿦จࣥච (ߥҪ)ɿൃද࿦จ

 ‫ݪ‬ஶ࿦จ 
Y. Watanabe,Proper Permittivity for Depolarization Field in Perfectly Insulating Ferroelectric and Examination of Background Permittivityies ,Ferroelectrics,in press
Proceedings
Y. Watanabe, Y. Urakami, D. Matsumoto, S. Kaku, S.-W. Cheong, G. A. Thomas, and
S. Miyauchi Novel Electrical Conduction of Insulators under Examination of Defects
and Injection and Relationship to Theories of Ferroelectric Domains. Proceedings of
MRS spring meeting 2014 (submitted)
123

ߨԋ

 ւ֎Ͱͷߨԋ ࠃࡍձٞ ট଴ߨԋ

Y. Watanabe, S. Kaku, S. Miyauchi, S.-W Cheong, D. Matsumoto and Y. Urakami,
Statics and Dynamics of cc and ac Domains of Virtually Intrinsic Ferroelectric in Clean
Limit,International Meeting on Ferroelectricity (IMF13) ,2013.09.02.
ࠃࡍձٞ

Y. Watanabe,Proper permittivity for depolarization ﬁeld in perfect insulator and examination of background permittivity,International Meeting on Ferroelectricity (IMF13)International Meeting on Ferroelectricity (IMF13), ࠲௕.
 ࠃ಺Ͱͷߨԋ ౉෦ɺ޻‫ۀ‬Խ͕୓͘‫ڧ‬༠ిମͷల๬ɿɹ΄ͱΜͲࣗ༝ͳిࢠ͕։͘৽͍͠‫ڧ‬༠ిମͷੈք, ଜాֶज़৽‫ஂࡒڵ‬ɹॿ੒ۚଃఄࣜ
֎෦ࢿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ ߥҪ‫ ؽ‬୅ද, ϑΥϊϯ༌ૹ੍‫ྫྷ̠̼ͱޚ‬ౚ‫ػ‬ͷͨΊͷ४प‫ߏظ‬଄ଟ૚ບʹΑΔϑΥϊ
ϯ೤఻ಋͷஅ೤, ௅ઓత๖ժ‫ ڀݚ‬ɹ՝୊൪߸ 23654104,
ฏ੒ 23 ೥౓ʙฏ੒ 25 ೥౓ଞେֶͰͷ‫ڭͱڀݚ‬ҭ

Wien ޻Պେֶ,Austria ɹ๚໰ֶ֎Ͱͷֶձ‫׆‬ಈ

Integrated Ferroelectrics ࢽ ฤूҕһ (౉෦)ͦͷଞͷ‫׆‬ಈͱ੒Ռ124

ଜాֶज़ৼ‫ஂࡒڵ‬ɹબߟҕһ (౉෦)ࠃཱϚϨʔγΞେֶ֎෦ධՁҕһ (౉෦)ϦΧϨϯτ‫ڭ‬ҭઃఆͱิॿ (౉෦)ମ‫ݧ‬ೖֶʢ‫঺ڀݚ‬հઆ໌ʣ(౉෦)༠ిମͷॳาߨٛ, ؔ੢஍۠‫౉( ۀا‬෦)ެ։ಛ‫ ڐ‬2013-075356 ߸ɹۚଐࢎԽ෺Λ‫ؚ‬Ήϔςϩ઀߹Λ༗͢Δߏ଄ମ (౉෦)ւ֎๚໰‫ ऀڀݚ‬2013.11,Prof. Janssen, University of Nijimegen, Neatherlandsʢ౉෦ʣ125‫ݻ‬ମిࢠ෺ੑߨ࠲
‫ߏࣨڀݚ‬੒һ໦ଜ ਸ ‫ڭ‬तࢁా ࿨ਖ਼ ॿ‫ڭ‬େ੢ ߛฏ ॿ‫ڭ‬ ത࢜‫ڀݚ‬һ ࢁా ৾໵ େֶӃ म࢜՝ఔ ౘ έΠγϯ ֶ෦ ଔ‫ڀݚۀ‬ੜ 
খ໺ ༤അ

઒๺ ௚࢙

୲౰त‫ۀ‬
ྗֶ‫ૅج‬ɾԋश (໦ଜਸ)ɺ ෺ཧֶ૯߹࣮‫ాࢁ( ݧ‬࿨ਖ਼)ɺ෺ཧֶ‫( ݧ࣮ૅج‬େ੢ߛฏ)‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ

Nb/Cu/NiFe ࡾ૚ߏ଄ʹ͓͚ΔεϐϯμΠφϛΫεʢখ໺༤അɺେ੢ߛฏɺ໦ଜਸʣ
ৗ఻ಋମ͔Β௒఻ಋମʹ஫ೖ͞Εͨిࢠ͸ɺ௒఻ಋମ಺ͰΫʔύʔରͱͳΓɺ௒఻ಋిྲྀΛ‫ܗ‬੒͢Δɻ௨ৗɺΫʔύʔର͸εϐϯҰॏ߲ͱͳΔͨΊɺ௒఻ಋిྲྀͱεϐϯྲྀ͸ॏ৞ͤͣɺ௒఻ಋମ͸७εϐϯྲྀʹͱͬͯઈԑମతଘࡏʹͳΔͱ‫ظ‬଴͞ΕΔɻ७
εϐϯྲྀ͸ඇ‫ॴہ‬εϐϯ஫ೖ๏ʹΑΓ‫ܗ‬੒Ͱ͖Δ͕ɺԣ‫ܕ‬εϐϯόϧϒૉࢠͰ͸ɺ஫ೖిྲྀʹΑΔൃ೤͔Β௒఻ಋΪϟοϓ͕‫ݮ‬গ͠ɺ໌ྎͳ‫؍‬ଌ͕ࠔ೉Ͱ͋Δɻͦ͜Ͱຊ‫ݚ‬‫Ͱڀ‬͸ɺిྲྀΛ༻͍ͳ͍εϐϯϙϯϐϯά๏ʹΑΓɺৗ఻ಋମʗ௒఻ಋମ઀߹ʹ͓͚
Δ७εϐϯྲྀʹ͍࣮ͭͯ‫ݧ‬తʹௐ΂͍ͯΔɻ
ࢼྉ͸ɺߴਅۭ੒ບ૷ஔΛ༻͍ͯ࡞੡ͨ͠ Nb/Cu/NiFe ࡾ૚ߏ଄Ͱ͋ΔɻNiFe ૚Λ‫࣓ڧ‬ੑ‫ڞ‬໐ͤ͞Δ͜ͱͰ Cu ૚ʹ‫ܗ‬੒͞ΕΔ७εϐϯྲྀ͸ɺNb/Cu ք໘ʹ౸ୡ͢Δɻຊ
‫Ͱڀݚ‬͸ɺNb ૚ͷ௒఻ಋసҠલ‫ޙ‬ͷ Py ͷ‫࣓ڧ‬ੑ‫ڞ‬໐εϖΫτϧΛଌఆ͢Δ͜ͱͰɺ

Nb/Cu ք໘ʹ͓͚Δ७εϐϯྲྀͷ༌ૹಛੑʹ͍ͭͯௐ΂ͨɻಘΒΕͨ৴߸͸ैདྷͷ
NiFe ୯૚ບʹൺ΂ɺઢ෯͕޿͘ͳ͓ͬͯΓɺNb ૚΁ͷεϐϯྲྀͷ‫ٵ‬ऩ͕ੜ͍ͯ͡Δͷ͕֬ೝͰ͖ͨɻNb Λ௒఻ಋঢ়ଶʹ͢ΔͱɺNiFe ͷ‫࣓ڧ‬ੑ‫ڞ‬໐εϖΫτϧͷઢ෯ʹ໌ྎ

126ͳมԽ͕‫ݱ‬Εɺ७εϐϯྲྀͷ൓ࣹޮՌΛࣔࠦ͢Δ݁ՌΛಘͨɻεϐϯภ‫ۃ‬φϊΪϟοϓి‫ʹۃ‬ΑΔ GdOx ͷ఻ಋಛੑ੍‫ޚ‬ʢ઒๺௚࢙ɺେ੢ߛฏɺࢁ
ా࿨ਖ਼ɺ໦ଜਸʣ
ిք༠‫ۚى‬ଐ-ઈԑମసҠ‫ݱ‬৅͸ɺ࣍ੈ୅ͷφϊిࢠσόΠεͱͯ͠ͷՄೳੑ΋ൿΊ͓ͯΓɺࠃࡍతʹਫ਼ྗతͳ‫ߦ͕ڀݚ‬ΘΕ͍ͯΔɻ͔͠͠ͳ͕Βɺ૬సҠϝΧχζϜͷ
ඍࢹత‫ݯى‬౳ɺະղ໌ͳ఺΋ଟ͘࢒͞Ε͍ͯΔɻҰํͰɺ૬సҠΛ‫͢͜ى‬෺࣭͸ɺMn
ࢎԽ෺ɺGd ࢎԽ෺ɺCo υʔϓ Ti ࢎԽ෺ͳͲɺ࣓ੑΛ࣋ͭ‫ࢠݪ‬Λ‫ؚ‬Μͩ෺࣭Ͱߏ੒͞
Ε͍ͯΔ৔߹͕ଟ͘ɺ૬సҠʹ൐͍εϐϯঢ়ଶʹ΋ԿΒ͔ͷભҠ͕‫ݱ‬ΕΔՄೳੑ΋‫ظ‬଴Ͱ͖Δɻͦ͜Ͱຊ‫Ͱڀݚ‬͸ɺGdOx Λϕʔεʹͨ͠૬సҠσόΠεʹ͓͍ͯɺ‫࣓ڧ‬ੑి‫ۃ‬φϊΪϟοϓΛ༻͍ͨ৽‫ͳح‬ԣ‫ܕ‬૬సҠσόΠεߏ଄Λ࡞੡͠ɺGdOx ͷ૬సҠ੍‫ޚ‬ɺ‫ࡐۃిͼٴ‬ྉʹ͓͚Δεϐϯͷ໾ׂ౳ʹ͍࣮ͭͯ‫ݧ‬తʹௐ΂͍ͯΔɻ࣮‫ࢼݧ‬ྉ
͸ GdOx ബບ্ͷ Metal ి‫ۃ‬Λ௨ిஅઢ๏ʹΑΓஅઢ͠ɺి‫ʹۃ‬φϊΪϟοϓΛ‫ܗ‬੒͢Δ͜ͱͰɺMetal/GdOx/Metal ઀߹Λ࡞੡ͨ͠ɻࠓճ͸ɺి‫ࡐۃ‬ྉͱͯ͠ CoFeB Λ
༻͍ͨࢼྉͷ I-V ಛੑʹ͓͍ͯɺ2V ෇ۙͰ‫ͳܹٸ‬఍߅มԽ͕‫؍‬ଌ͞Ε͓ͯΓɺ‫࣓ڧ‬ੑి‫ۃ‬Λ༻͍ͨۚଐ-ઈԑମసҠʹ੒ޭͨ͠΋ͷͱߟ͑ΒΕΔɻൃද࿦จ ‫ݪ‬ஶ࿦จ 
Wide range tuning of resonant frequency for a vortex core in a regular triangle magnet:
S. Yakata, T. Tanaka, K. Kiseki, K. Matsuyama and T. Kimura,
Scientiﬁc Reports 3 (2013) pp. 3567
Thermal gradient driven enhancement of pure spin current at room temperature in
nonlocal spin transport devices:
S. R. Bakaul, S. Hu and T. Kimura,Phys. Rev. B 88 (2013) pp. 184407
Thermo-electric eﬀect in a nano-sized crossed Permalloy/Cu junction under high bias
current:
C. Mu, S. Hu, J. Wang and T. Kimura,Appl. Phys. Lett. 103 (2013) pp. 132408

127

Measurement of the ferromagnetic resonance of a single micron dot by using a vector
network analyzer:
K. Yamanoi, T. Manago, S. Yakata and T. Kimura,
J. Korean Phys. Soc. 63 (2013) pp. 800
Spin Wave Excitation and Propagation Properties in a Permalloy Film:
K. Yamanoi, S. Yakata, T. Kimura and T. Manago,
Jpn. J. Appl. Phys. 52 (2013) pp. 083001
Detection of edge magnetic state by a ballistic bend resistance measurement:
T. Matsunaga, K. Furukawa, Y. Kanda, M. Hara, T. Nomura and T. Kimura,Appl. Phys. Lett. 102 (2013) pp. 252405
Size Dependence of Ferromagnetic Resonance Frequency in Submicron Patterned Magnet:
T. Manago, K. Yamanoi, S. Yakata and T. Kimura,
Jpn. J. Appl. Phys. 52 (2013) pp. 053001

ߨԋ ւ֎Ͱͷߨԋ 
Wide-range tuning of vortex-core resonance using asymmetric conﬁned potential in atriangular permalloy dot:
S. Yakata and T. Kimura,
MML2013, Kyoto, Japan (May, 2013)
T. Kimura, Generation of large spin current in metallic nanostructures and its application ɹ Energy Materials Nanotechnology (EMN) east meeting, Beijing, China, (Sept.
2013)
Giant thermal spin accumulation in NLSV structure by using CoFeAl/Cu interface atroom temperature:
S. Hu and T. Kimura,
128

MMM 2013, Denver, U.S.A. (Nov., 2013)
Detection of nonlinear vortex oscillation under strong RF magnetic ﬁeld using anisotropic
magnetoresistance eﬀect:
X. Cui, S. Yakata and T. Kimura,
MMM 2013, Denver, U.S.A. (Nov., 2013)
T. Kimura, Highly eﬃcient thermal spin injection using CoFeAl injector, EMN fallmeeting, Orland U.S.A., (Dec. 2013) ࠃ಺Ͱͷߨԋ φϊϐϥʔ‫ܕ‬ඇ‫ॴہ‬εϐϯόϧϒʹ͓͚Δߴޮ཰७εϐϯྲྀͷੜ੒:໺ଜཽ໵ɼ‫މ‬গᐢɼ໦ଜਸ
೔ຊ෺ཧֶձळ‫ق‬େձɺಙౡେֶɺ2013 ೥ 9 ݄εϐϯภ‫ۃ‬φϊΪϟοϓి‫ʹۃ‬ΑΔ GdOx ͷ఻ಋಛੑ੍‫ޚ‬:઒๺௚࢙ɼେ੢ߛฏɼ໦ଜਸ
೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ౦ւେֶɺ2014 ೥ 3 ݄

Nb/Cu/NiFe ࡾ૚ߏ଄ʹ͓͚ΔεϐϯμΠφϛΫε:খ໺༤അɼେ੢ߛฏɼ໦ଜਸ
೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ౦ւେֶɺ2014 ೥ 3 ݄

Nb/Cu/NiFe ࡾ૚ߏ଄Λ༻͍ͨ௒఻ಋঢ়ଶʹΑΔεϐϯྲྀ൓ࣹ‫ݱ‬৅ͷଌఆ:େ੢ߛฏɼখ໺༤അɼ໺ଜཽ໵ɼ໦ଜਸ
೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɺ౦ւେֶɺ2014 ೥ 3 ݄

Nb/Cu/Py ࡾ૚ߏ଄ʹ͓͚Δ७εϐϯྲྀ༌ૹಛੑ:খ໺༤അɼେ੢ߛฏɼ઒๺௚࢙ɼ໺ଜཽ໵ɼ໦ଜਸ
ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձɺ‫ཹٱ‬ถ޻‫ۀ‬େֶɺ2013 ೥ 11 ݄

Pd φϊίϯλΫτʹ͓͚Δۙ౻ޮՌ:ՈӬߛҰ࿠ɼߴా߂थɼେ੢༤‫و‬ɼҴ֞༞࣍ɼ௰Ҫ޺೭ɼ໦ଜਸɼՏߐୡ໵
ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձɺ‫ཹٱ‬ถ޻‫ۀ‬େֶɺ2013 ೥ 11 ݄

129εϐϯ஫ೖʹΑΔ GdOx ബບͷిࢠ૬సҠ੍‫ޚ‬ͷࢼΈ:઒๺௚࢙ɼେ੢ߛฏɼՈ‫ܗ‬་ɼ໦ଜਸ
ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձɺ‫ཹٱ‬ถ޻‫ۀ‬େֶɺ2013 ೥ 11 ݄

Py தͷεϐϯ೾఻ൖʹ͓͚Δ‫ݮ‬ਰ௕ͷ࣓৔ґଘੑ:ࢁ໺ҪҰਓɼՈ‫ܗ‬་ɼ໦ଜਸɼᚸ࠭୎࢙
‫۝‬भද໘ɾਅۭ‫ڀݚ‬ձɺ෱Ԭେֶɺ2013 ೥ 6 ݄Ґ૬ॖ໿ʹ‫࣓ͮ͘ج‬ੑମൃৼૉࢠͷ஫ೖಉ‫ߏػظ‬ͷ࠷దԽઃ‫ܭ‬:தాҰ‫ل‬ɼాத‫ٱ‬ཅɼՈ‫ܗ‬་ɼ໦ଜਸ
೔ຊԠ༻਺ཧֶձ ਺ཧઃ‫ڀݚܭ‬෦ձɺΞΫϩε෱Ԭɺ2013 ೥ 9 ݄֎෦ࢿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚɺ‫ج‬൫‫( ڀݚ‬S)
७εϐϯྲྀ஫ೖʹΑΔ࣓‫ؾ‬૬సҠͷબ୒త੍‫৽ֵͱޚ‬తφϊεϐϯσόΠε΁ͷԠ༻‫ڀݚ‬୅දऀɿ໦ଜ ਸจ෦লՊֶ‫ڀݚ‬අิॿۚɺ௅ઓత๖ժ‫ڀݚ‬७εϐϯྲྀͷ‫ॴہ‬஫ೖʹΑΔଟϏοτ৘ใॻࠐΈٕज़ͷ૑ग़‫ڀݚ‬୅දऀɿ໦ଜ ਸ จ෦লՊֶ‫ڀݚ‬අิॿۚҎ֎ͷ֎෦ࢿۚ Ωϟϊϯࡒஂ ‫ॿڀݚ‬੒ϓϩάϥϜʮ࢈‫جۀ‬൫ͷ૑ੜʯεϐϯ‫ٵ‬ऩޮՌΛ༻͍ͨ‫ۃ‬ඍࡉεϐϯΫʔϦϯάσόΠεͷ։ൃ‫ڀݚ‬୅දऀɿ໦ଜ ਸ೔ຊֶज़ৼ‫ڵ‬ձಛผ‫ڀݚ‬һ౳‫ڞͼٴ‬ಉ‫ڀݚ‬ͷ࠾୒ (ֶ֎͔Βͷड͚ೖΕΛ‫ؚ‬Ή)
ࢁా ৾໵

130

ֶ෦̐೥ੜଔ‫ڀݚۀ‬খ໺༤അ:(ࢦಋ‫ڭ‬һɺ໦ଜਸ):Nb/Cu/Py ࡾ૚ߏ଄ʹ͓͚Δ७εϐϯྲྀ༌ૹಛੑɻ
઒๺௚࢙:(ࢦಋ‫ڭ‬һɺ໦ଜਸ):εϐϯ஫ೖʹΑΔ GdOx ബບͷిࢠ૬సҠ੍‫ޚ‬ͷࢼΈɻम࢜࿦จౘ έΠγϯ:(ࢦಋ‫ڭ‬һɺ໦ଜਸ):࣓۠ߏ଄੍‫͞ޚ‬Εͨφϊ࣓ੑମʹ͓͚Δεϐϯ஫ೖࣗྭൃৼ‫ݱ‬৅ɻ֎ࠃਓཹֶੜͷड͚ೖΕౘ έΠγϯ

ͦͷଞͷ‫׆‬ಈͱ੒ՌߴߍੜͷͨΊͷମ‫ݧ‬ೖֶ 2014 ೥ 3 ݄‫۝‬भେֶ঺հ (Մ໵༮ஓԂ) 2013 ೥ 11 ݄‫۝‬भେֶ঺հ (ஜࢵதԝߴߍ) 2013 ೥ 10 ݄ग़લߨٛʢ౦ஜߴߍʣ2013 ೥ 12 ݄131௿࣍‫ࢠిݩ‬෺ੑ‫ߏࣨڀݚ‬੒һ໼ࢁӳथ ‫ڭ‬त େֶӃ म࢜՝ఔ ಺ࢁ‫ܒ‬հ

Լా༔ଠ

٢࡚૱Ұ࿠

ඉ‫ޱ‬ਖ਼࿨ཱ઒ ༤େ ֶ෦ ଔ‫ڀݚۀ‬ੜ 
ࡔຊਝ

ࣲా௚࠸

 ๚໰‫ ऀڀݚ‬Ali Gamal Hafez Ernassel Rabie୲౰त‫ۀ‬
෺ཧֶಛผ‫ ڀݚ‬Iɺ෺ཧֶಛผ‫ ڀݚ‬IIɺ෺ཧֶ૯߹࣮‫ݧ‬ɺ෺ཧ࣮‫ֶݧ‬ɺ࠷ઌ୺෺ཧֶ
‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ
ʢ̍ʣϔϦ΢Ϝ໘্ͷ 2 ࣍‫ܥࢠిݩ‬ͷҳग़཰ͷଌఆʢԼాɺ໼ࢁʣ
͜Ε·Ͱͷ‫Ͱڀݚ‬͸ɺӷମϔϦ΢Ϝ໘্ͷ 2 ࣍‫ܥࢠిݩ‬ͷӡಈ͸໘಺ʹ‫ݶ‬ΒΕΔ৔߹͕΄ͱΜͲͰ͋ͬͨɻࠓճ͸ɺ໘ʹਨ௚্ํʹిࢠ͕ҳग़͢Δࡍͷ଎౓ʹ͍ͭͯ‫ڀݚ‬Λߦͬͨɻ͢Ͱʹɺ2 ࣍‫ܥࢠిݩ‬͸௿Թɾߴີ౓ͷిࢠঢ়ଶͰ΢Οάφʔ݁থ΁సҠ͢Δ͜ͱ͕஌ΒΕ͍ͯΔ͕ɺసҠ఺ۙ๣ͷ‫͍ڱ‬Թ౓ൣғͰϔΩα૬͕ଘࡏ͢Δ͜ͱ͕ཧ࿦తʹ༧ଌ͞Ε͍ͯΔ͕ɺ͜Ε͸ະ࣮ͩ‫ݧ‬ΑΓ֬ೝ͞Ε͍ͯͳ͍ɻ͜ͷ‫ڀݚ‬ͷ࠷ऴత໨త͸ɺ΢Οάφʔ݁থసҠ఺ʹ͓͚ΔϔΩα૬ͷଘࡏΛҳग़཰ʹ‫ݱ‬ΕΔҟৗʹΑΓ֬ೝ͢Δ͜ͱͰ͋ΔɻࠓճɺϔϦ΢ϜԹ౓ͷ௿ԹͰಈ࡞͢Δ૿෯‫ث‬Λ༻͍ͯɺ‫౓ײ‬Λ޲্ͤͨ͞ɻ࣮‫݁ݧ‬Ռ͸ɺҳग़཰Λిࢠີ౓ͷؔ਺ͱͯ͠ଌఆ͢Δ͜ͱ͕ՄೳͰ͋Δ
͜ͱΛࣔͨ͠ɻࠓ‫ޙ‬ɺԹ౓Λ 100mK ఔ౓·ͰԼ͛ɺ΢Οάφʔ݁থసҠ఺ۙ๣Ͱͷҳग़཰ͷଌఆΛ໨ࢦ͢ɻʢ̎ʣӷମਫૉ্ͷ 2 ࣍‫ܥࢠిݩ‬ͷి‫఻ؾ‬ಋʢඉ‫ޱ‬ɺ໼ࢁʣ௿Թӷମ্ͷ 2 ࣍‫ܥࢠిݩ‬ͷ࣮‫ݧ‬͸ɺଟ͕͘ϔϦ΢Ϝ্ͰߦΘΕ͍ͯΔɻ͜Ε·Ͱʹɺӷମਫૉ্ͷ 2 ࣍‫ܥࢠిݩ‬ͷ࣮‫ݧ‬͸਺ྫʹ‫ݶ‬ΒΕ͓ͯΓɺߴԹͰͷి‫఻ؾ‬ಋ౓ͷ௿Լ

132͕ɺਫૉதʹൃੜ͢Δ๐ʹΑΔిࢠͷফ໓Ͱઆ໌͞Ε͍ͯͨɻࠓճɺൺֱతߴԹͷ 20K
ҎԼͰਫ਼ີʹి‫఻ؾ‬ಋΛଌఆ͠ɺ͜ͷߟ࡯͕ਖ਼͍͔͠Λ‫ͨ͠ূݕ‬ɻͦͷ݁Ռɺա‫ڈ‬ͷσʔλ͸Թ౓ґଘੑ͕େ͖͗͢Δ͜ͱ͕Θ͔Γɺ๐ʹΑΔిࢠͷফ໓͚ͩͰ͸આ໌Ͱ͖ͳ͍͜ͱ͕໌Β͔ʹͳͬͨɻʢ̏ʣ2 ஈஅ೤ফ࣓ྫྷౚ‫ػ‬ͷ։ൃʢ٢࡚ɺ໼ࢁʣ

100mK ҎԼͷԹ౓Λੜ੒͢ΔҰൠతͳํ๏ͱͯ͠‫ر‬ऍྫྷౚ‫͕͋ػ‬Δɻ͔͠͠ɺෳࡶͳ
He Ψεͷ॥‫؀‬γεςϜ͕ඞཁͰ͋Δ͜ͱɺ௒ྲྀಈ He ͷ࿙ΕͳͲͷ໰୊͕ଟ͍ɻHe ΨεΛ༻͍ͳ͍࣓‫ྫྷؾ‬ౚ‫ػ‬͸ͦΕΒͷ໰୊͕ͳ͍ͨΊকདྷ༗๬Ͱ͋Δɻ͔͠͠ɺϫϯγϣο
τͷྫྷ٫ํࣜͰ͋ΔͨΊ࿈ଓతͳ௿Թҡ͕࣋Ͱ͖ͳ͍ɻࠓճɺ೤εΠονΛ༻͍ͨ 2 ஈྫྷ٫γεςϜΛ։ൃ͢Δ͜ͱͰɺকདྷͷ࿈ଓӡసํࣜ΁ͷՄೳੑΛ୳Δ͜ͱΛߦͬͨɻ

2 ͭͷΫϩϜΧϦϛϣ΢όϯʢCPAʣιϧτϐϧΛ੡࡞͠ɺ྆ऀΛΠϯδ΢Ϝ೤εΠονΛ༻͍ͯ઀ଓ͠ɺ೤εΠονͷ ON/OFF ͸௒఻ಋϚάωοτ͔Βͷ࿙Ε࣓৔Λར༻
͢Δ͜ͱͰɺ2 ஈஅ೤ফ࣓Λߦͬͨɻͦͷ݁Ռɺ໿ 80mK ͷ௿Թ͕ಘΒΕɺ࿙Ε࣓৔ʹΑΔ೤εΠονͷ੾ସ͕ՄೳͰ͋Δ͜ͱΛࣔͨ͠ɻൃද࿦จ ‫ݪ‬ஶ࿦จ 
1. Oscillation mode transformation of edge magnetoplasmons in two-dimensional electron system on liquid-helium surface,
Shuji Yamanaka, Toshikazu Arai, Anju Sawada, Akira Fukuda, Hideki Yayama,
Low Temp. Phys., Vol.39, No.10, pp.842-850, 2013.
2. Eﬀect of SC on frequency content of geomagnetic data using DWT Application: SC
automatic detection,
Essam Ghamry, Ali G. Hafez, Kiyohumi Yumoto, Hideki Yayama,
Earth Planets Space, Vol.65, pp.1007-1015, 2013.
3. Oscillation mode transformation of edge magnetoplasmons in two-dimensional electron system on liquid-helium surface,
Shuji Yamanaka, Toshikazu Arai, Anju Sawada, Akira Fukuda, Hideki Yayama,Fiz. Nizk. Temp., Vol.39, No.10, pp.1086-1095, 2013.

133

4. Charge Density Wave and Superconductivity of RPt2Si2 (R = Y, La, Nd, and Lu),
Yutaro Nagano, Nobutaka Araoka, Akihiro Mitsuda, Hideki Yayama, Hirofumi Wada,
Masaki Ichihara, Masahiko Isobe, Yutaka Ueda,
J. Phys. Soc. Jpn., Vol.82, 2013, pp.064715 1-5.
5. Systematic examination of the Geomagnetic Storm Sudden Commencement using
multi resolution analysis,
Ali G. Hafez, Essam Ghamry, Hideki Yayama and Kiyohumi Yumoto,Adv. Space Res., Vol.51, pp.39-49, 2013.
6. Un-decimated discrete wavelet transform based algorithm for extraction of geomagnetic storm sudden commencement onset of high resolution records,
Ali G. Hafez, Essam Ghamry, Hideki Yayama and Kiyohumi Yumoto,Comp. Geosci., Vol.51, pp.143-152, 2013.

 ͦͷଞͷ࿦จ 
1. ໼ࢁӳथ, ֩அ೤ফ࣓ྫྷ٫ III, ‫۝‬भେֶ௿ԹηϯλʔͩΑΓ No.8, 2014. p.18.

ߨԋ ւ֎Ͱͷߨԋ ֶ෦̐೥ੜଔ‫ڀݚۀ‬ࡔຊਝɺࣲా௚࠸ʢࢦಋ‫ڭ‬һɿ໼ࢁʣɿӷମਫૉ্ͷ 2 ࣍‫ܥࢠిݩ‬ͷి‫఻ؾ‬ಋम࢜࿦จԼా༔ଠɿӷମϔϦ΢Ϝ໘্ͷ 2 ࣍‫ܥࢠిݩ‬ͷҳग़཰ଌఆ٢࡚૯Ұ࿠ɿ2 ஈஅ೤ফ࣓ྫྷౚ‫ػ‬ͷ։ൃ

134ඉ‫ޱ‬ਖ਼࿨ɿӷମਫૉ্ͷ 2 ࣍‫ܥࢠిݩ‬ֶ֎Ͱͷֶձ‫׆‬ಈԠ༻෺ཧֶձ‫۝‬भࢧ෦ཧࣄ

डୗ‫ڀݚ‬ɾຽؒͱͷ‫ڞ‬ಉ‫ڀݚ‬໼ࢁɿʮ‫ۃ‬௿ԹΫϥΠΦελοτͷ։ൃʯɺʢ‫ג‬ʣ௿Թٕज़‫ͱॴڀݚ‬ͷ‫ڞ‬ಉ‫ڀݚ‬

135

ෳࡶ෺ੑ‫ૅج‬‫ߏࣨڀݚ‬੒һ໦ଜ߁೭ ‫ڭ‬तਫ໺େհ ।‫ڭ‬त‫ؠ‬Լ༃޹ ॿ‫ڭ‬ େֶӃ ത࢜՝ఔ ࠇࢁɹߊ࢘໺‫׮๎ޱ‬

Heev Ayade େֶӃ म࢜՝ఔ 
Ҫ࡚๜ٛ

ాதখඦ߹

ੴ֞෢࢜

த໺༟ੜ

େ‫ٱ‬อɹল‫ޗ‬‫ۄ‬Ҫୡ࠸
༗দɹ‫׮‬

༞Լɹַࢤ

উా߁ฏ
ࢁຊɹঊ

ߴ‫ڮ‬ɹ݈ଠ࿠

দԬɹྑ੖দ‫ݩ‬ɹେ‫ޗ‬ ֶ෦ ଔ‫ڀݚۀ‬ੜ 
Տଜོ߂

‫ڤݪ܀‬

༗ཹਅਓ

૿ా૖େ

 ‫ڀݚ‬ੜ ுɹ௨Lara Gay Villaruz Moccoro୲౰त‫ۀ‬
ి࣓‫( ֶؾ‬໦ଜ߁೭)ɺྗֶ‫ૅج‬ɾಉԋश (໦ଜ߁೭)ɺ෺ੑ෺ཧֶ I(໦ଜ߁೭)ɺ෺ཧֶ

III(໦ଜ߁೭)ɺෳࡶ‫ܥ‬෺ཧֶ (໦ଜ߁೭)ɺ೤ͱ೾ಈ࿦‫( ૅج‬ਫ໺େհ)ɺ෺ཧֶθϛφʔϧ (ਫ໺େհ)ɺ෺ཧίΞ?(ਫ໺େհ)ɺ࠷ઌ୺෺ཧֶ (‫ؠ‬Լ༃޹)ɺ෺ཧֶ૯߹࣮‫ؠ( ݧ‬Լ༃޹)‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ ࠓ೥౓ͷ໨ඪ ˓৽‫ͳن‬Ϩʔβʔτϥοϓख๏ͷ։ൃ΍ɺͦΕʹΑΔྗଌఆɾཻࢠૢ࡞ΛίϩΠυ‫ܥ‬ʹద༻͠ɺͦͷ෺ੑଌఆ‫ͼٴ‬ඇઢ‫ڍܗ‬ಈͷղ໌Λߦͳ͏͜ͱΛ໨ࢦͨ͠ɻʢ̍, ̏ʣ˓ෳࡶͳιϑτϚλʔෳ߹‫͚͓ʹܥ‬Δ‫ॴہ‬ϨΦϩδʔ‫ڍ‬ಈ΍૬෼཭աఔͳͲΛৄࡉʹղ໌͢Δ͜ͱΛ໨ࢦͨ͠ɻʢ̎ɼ̒ʣ

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˓༷ʑͳίϩΠυཻࢠͷ࡞੒΍ɺͦͷ෼ࢄ‫͚͓ʹܥ‬Δू߹త‫ڍ‬ಈͳͲΛղ໌͢Δ͜ͱ
Λ໨ࢦͨ͠ɻʢ̐ɼ̑ɼ̓ɼ̔ʣ
˓‫ڵ‬ຯਂ͍ӷথͷ૬‫ڍ‬ಈΛ NMR Ͱௐ΂Δ͜ͱΛ໨తͱͨ͠ɻʢ̕ʣ
˓ΠΦϯӷମͷΨϥεసҠΛ NMR ͱγϛϡϨʔγϣϯͰղ໌͢Δ͜ͱΛ໨తͱͨ͠ɻ
ʢ̍̌ʣ˓ϚΠΫϩϨΦϩδʔ‫ܭ‬ଌ๏ʹϑΟʔυόοΫ‫ߏػ‬Λಋೖ͠ɺࡉ๔΍όΫςϦΞͷूஂӡಈ౳ͷ‫͍ڧ‬ඇฏߧ‫ܥ‬ͷ༳Β͗Ԡ౴ͷಉ࣌‫؍‬ଌΛ࣮‫͢ݱ‬Δɻʢ̍̍ʣ
˓ࡉ๔ࠎ֨΍ίϩΠυ‫ܥ‬ͷྗֶԠ౴ʹඇΞϑΝΠϯͳԠ౴͕Ռͨ͢໾ׂΛϚΠΫϩϨ
ΦϩδʔʹΑΔ޿ଳҬ‫ܭ‬ଌʹΑΓ࣮ূ͢Δɻʢ̍̎ʣ
˓ actin-myosin gel ΍༡૸όΫςϦΞ༹ӷ౳ͷ active system தʹ͓͚Δඇฏߧ༳Β͕͗৽͍͠ Levy ෼෍ͷΫϥεʹଐ͍ͯ͠Δ͜ͱɺ͓Αͼͦͷ෼෍‫ܗ‬ঢ়ͷղੳղΛ໌Β͔ʹ͢Δɻʢ̍̏ʣ
˓֤छࡉ๔நग़ӷͷྗֶಛੑΛ‫ܭ‬ଌ͢Δ͜ͱͰɺࡉ๔಺෦‫ڥ؀‬ͷΨϥεతৼΔ෣͍Λ໌Β͔ʹ͢Δ͜ͱΛ໨ࢦͨ͠ɻ ࠓ೥౓ͷ੒Ռ ʢ̍ʣ ωϚνοΫӷথதͷίϩΠυཻࢠؒ૬‫༻࡞ޓ‬ͷ‫ڀݚ‬ʢҪ࡚ɺՏଜɺ‫ؠ‬Լɺ໦ଜʣ
ωϚνοΫӷথதʹϛΫϩϯαΠζͷίϩΠυཻࢠΛ෼ࢄͤ͞Δͱͦͷք໘Ͱͷӷথ഑޲ঢ়ଶʹґଘͯ͠ɺίϩΠυؒʹӷথͷ஄ੑΛഔհͱͨ͠૬‫͕༻࡞ޓ‬ಇ͘͜ͱ͕
஌ΒΕ͍ͯΔɻΘΕΘΕ͸̎ຊͷޫϐϯηοτΛ༻͍ͯ̎ͭͷίϩΠυཻࢠΛัଊ͠ɺͦΕΒͷҐஔΛมԽͤͭͭ͞ɺτϥοϓҐஔͷඍখͳมԽΛͦͷ‫ݦ‬ඍ‫͔૾ڸ‬Β‫؍‬ଌ͢
Δ͜ͱͰཻࢠؒ૬‫༻࡞ޓ‬ͷ௚઀ଌఆΛߦͬͨɻຊ೥౓͸͜ͱʹɺͦͷཻࢠؒ૬‫༻࡞ޓ‬ཻ͕ࢠɾܽؕରͷλΠϓʹΑͬͯมԽ͢Δ͜ͱɺి৔ͷҹՃʹΑΓมԽ͢Δ͜ͱͳͲΛ‫ͨ͠ڀݚ‬ɻ·ͨɺཻࢠؒྗͷଌఆ๏ͱͯ͠৽ͨͳྲྀମྗֶతͳิਖ਼ΛߦͬͨϑϦʔϦϦʔε๏ͷ։ൃ΋ߦͬͨɻʢ̎ʣࠞ߹ࢷ࣭ϦϙιʔϜͷޫϐϯηοτʹΑΔม‫ྗͱܗ‬ଌఆʢ༞Լɺ༄ᖒɺ‫ؠ‬Լɺ໦ଜʣଟ੒෼ࢷ࣭͔ΒͳΓບ಺Ͱ૬෼཭͢ΔϕγΫϧߏ଄ʢϦϙιʔϜʣ಺ʹෳ਺ͷίϩΠυཻࢠΛૠೖ͠ɺͦͷ͏ͪ̎ͭΛϨʔβʔʹΑΓ൓ରํ޲ʹҾͬுͬͨɻ͢ΔͱϕγΫϧ͕‫ٿ‬ঢ়ˠϨϞϯঢ়ˠ‫ٿ‬ʴ๮ঢ়ͱมԽͨ͠Γɺଠ͍෦෼ͱࡉ͍෦෼͕਺चͭͳ͗
ͱͳͬͨ‫ܗ‬ଶΛऔΔͳͲɺ༷ʑͳ‫ڵ‬ຯਂ͍‫ڍ‬ಈ͕‫ݱ‬Εͨɻʢ̏ʣϗϩάϥϑΟοΫޫϐϯηοτͷ։ൃʢେ‫ٱ‬อɺ‫ؠ‬Լɺ໦ଜʣ

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ޫۭؒมௐ‫ث‬Λ༻͍ͯҐ૬ϗϩάϥϜΛ࡞੒͠ɺଟ఺ͷޫτϥοϓΛՄೳʹͨ͠ɻߋʹཻࢠʹ֯ӡಈྔΛ༩͑ΔޫӔΛෳ਺࡞੒͢Δ͜ͱʹ੒ޭͨ͠ɻ։ൃͨ͠γεςϜΛ
༻͍ͯɺྲྀମతʹ݁߹ͨ͠ଟཻࢠ‫ܥ‬ͷࣔ͢ूஂӡಈͷղ໌ΛࢼΈͨɻͦͷ݁ՌɺϦϛοταΠΫϧӡಈɾΫϥελʔ‫ܗ‬੒ͳͲɺ૬‫༻࡞ޓ‬ͷඇઢ‫ܗ‬ੑʹ‫ى‬Ҽ͢Δಛ௃తͳ‫ڍ‬ಈΛ‫͢࡯؍‬Δ͜ͱʹ੒ޭ͠ɺ਺஋γϛϡϨʔγϣϯͳͲʹΑΓͦͷ෺ཧత‫ߏػ‬ͷҰ୺Λղ໌͢Δ͜ͱ͕Ͱ͖ͨɻ
ʢ̐ʣίϩΠυ݁থͷੜ੒ɾ༥ղաఔͷ‫ڀݚ‬ʢాதɺ‫ؠ‬Լɺ໦ଜʣ
ޫϐϯηοτͷϨʔβʔΛಋిੑബບʹরࣹ͢Δ͜ͱͰ࡞੒ͨ͠ɺ‫ॴہ‬೤ޯ഑Λ༻ཻ͍ͯࢠΛूੵ͠ɺίϩΠυ݁থΛ࡞੒Ͱ͖Δɻ͞ΒʹɺϨʔβʔরࣹΛࢭΊΔ͜ͱͰɺ͜ͷ̎࣍‫ݩ‬ίϩΠυ݁থͷ༥ղաఔΛ‫ݟ‬Δ͜ͱ΋Ͱ͖Δɻ͜ͷੜ੒ɾ༥ղաఔʹؔ͠ɺ‫ݦ‬ඍ‫ʹڸ‬ΑΔ࣮࣌ؒ‫࡯؍‬Λߦͳͬͨɻͦͷ݁Ռɺ݁থԽͷ‫ۦ‬ಈྗ͸೤ӭಈޮՌͰఆੑతʹઆ໌Ͱ͖Δ͜ͱ͕෼͔ͬͨɻ·ͨ༥ղ͸݁থ‫ڥ‬ք͔Β͚ͩͰͳ͘಺෦͔Β΋ਐߦ͢Δ͜ͱɺ‫ͦͼٴ‬ͷࡍͷཻࢠடংͷมԽ͕̎࣍‫ܥࢠཻݩ‬ͷ૬సҠͱؔ࿈͕͋Δ
͜ͱ͕໌Β͔ͱͳͬͨɻ͜ΕΒͷ࣮‫݁ݧ‬ՌΛઆ໌͢ΔͨΊʹϒϥ΢ϯμΠφϛΫεɾγ
ϛϡϨʔγϣϯΛߦ͍ɺ࣮‫ͱݧ‬Α͍ҰகΛΈͨɻʢ̑ʣϠψεཻࢠͷ࡞੒ͱͦͷ‫ߏूڽ‬଄ͷ‫ڀݚ‬ʢ໺‫ޱ‬ɺ‫ؠ‬Լɺ໦ଜʣ
γϦΧཻࢠ΁ۚৠண͠ɺͦΕΛνΦʔϧԽ͢Δ͜ͱʹΑΓɺ਌ਫ໘ɾૄਫ໘Λ࣋ͬͨ྆਌ഔੑίϩΠυཻࢠ (Ϡψεཻࢠ) Λ࡞੒ͨ͠ɻ͜ͷϠψεཻࢠ-ਫ-༉̏੒෼‫͍͓ʹܥ‬ͯɺͦͷք໘‫׆‬ੑ‫ڍूڽͼٴ‬ಈͷηοέϯ෼ࢠ‫ͱܥ‬ͷ૬ҧΛ࣮‫ʹݧ‬ΑΓղ໌ͨ͠ɻ·༹ͨഔͷྟքޮՌΛར༻ͯ͠Ϡψεཻࢠؒͷҟํతͳ૬‫༻࡞ޓ‬Λਫ਼ີʹ੍‫͢ޚ‬Δ͜ͱ
ʹ΋੒ޭ͠ɺͦΕΛར༻ͯ͠‫ߏूڽ‬଄‫ܗ‬੒ʹ͓͚Δ֊૚ੑΛղ໌ͨ͠ɻʢ̒ʣ ӷথి‫ؾ‬ରྲྀ‫ܥ‬ͷ̏࣍‫࡯؍ݩ‬ʢউాɺߴ‫ڮ‬ɺ‫ؠ‬Լɺ໦ଜʣ
ෛͷ༠ి཰ҟํੑΛ࣋ͭӷথʹి৔ΛҹՃ͢ΔࣄʹΑΓੜ͡Δి‫ؾ‬ରྲྀʹର͠ɺӷথ഑޲ํ޲Λ൓өͨ͠‫ޫܬ‬Λൃ͢Δ৭ૉΛ༻͍ɺ̏࣍‫ݩ‬తʹରྲྀߏ଄Λ‫ͨ͠࡯؍‬ɻͦͷ݁ՌɺίϨεςϦοΫӷথ‫͍͓ͯʹܥ‬ɺա‫ڈ‬ͷ‫͔ڀݚ‬Β༧૝͞Ε͍ͯͨ΋ͷͷ࣮ࡍʹ͸֬ೝ͞Ε͍ͯͳ͔ͬͨύλʔϯભҠաఔΛɺॳΊͯ໌֬ʹ‫͢࡯؍‬Δ͜ͱ͕Ͱ͖ͨɻʢ̓ʣ ҟํతίϩΠυཻࢠͷӡಈʢদ‫ݩ‬ɺ‫ؠ‬Լɺ໦ଜʣ
थࢷ੡ͷίϩΠυཻࢠΛߴ෼ࢠϑΟϧϜ಺ʹ෼ࢄͤ͞ɺཻࢠ͕ΨϥεసҠ఺Ҏ্ʹͳΔԹ౓ͰϑΟϧϜΛҾ͖৳͹͢͜ͱͰɺҰ࣠Ԇ৳͞Εͨପԁঢ়ཻࢠΛ࡞੒ͨ͠ɻͦ
ͷཻࢠΛ௜఼ͤ͞ɺ̎࣍‫ݩ‬తͳϒϥ΢ϯӡಈΛ‫͠࡯؍‬ɺը૾ղੳʹΑΓ֦ࢄ‫ڍ‬ಈΛௐ΂ͨɻ͢Δͱɺ࣌ؒεέʔϧʹΑΓॏ৺ͷ֦ࢄ͕ճస֦ࢄͷӨ‫ڹ‬Λड͚Δ͜ͱ͕෼͔ͬ

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ʢ̔ʣ ྟքޮՌΛར༻ͨ͠ίϩΠυཻࢠͷ‫ूڽ‬ΩωςΟΫεͷղ໌ʢ‫ۄ‬Ҫɺ‫ؠ‬Լɺ໦ଜʣ౳ํతͳίϩΠυཻࢠΛਫ-ϧνδϯྟք૊੒༹ӷʹ෼ࢄͤ͞ɺҰ૬ঢ়ଶ͔ΒঢԹ͠ྟք఺ʹ͚͍ۙͮͯ͘ͱɺཻࢠؒͷҾྗ͕࿈ଓతʹ૿େ͢Δɻ͜ͷ‫ݱ‬৅Λར༻͠ɺҾྗͷେ͖͞ʹΑΓίϩΠυཻࢠͷ̎࣍‫ݩ‬తͳ‫ूڽ‬ΩωςΟΫε͕ͲͷΑ͏ʹมԽ͢Δ͔Λௐ΂ͨɻͦͷ݁ՌɺҾྗͷ૿ՃʹΑͬͯΑΓύʔίϨʔτ͠΍͘͢ͳΔՄೳੑ͕ࣔࠦ͞Εͨɻ
ʢ̕ʣϦΤϯτϥϯτӷথͷ૬‫ڍ‬ಈͷղ໌ (த໺ɺ໦ଜ)Թ౓߱Լ࣌ʹ౳ํ૬ˠωϚνοΫ૬ˠεϝΫνοΫ૬ˠωϚνοΫ૬ͱมԽ͢ΔϦΤϯτϥϯτӷথͷ૬‫ڍ‬ಈΛ NMR ʹΑΓௐ΂ͨɻͦͷ݁Ռɺdimer ‫ܗ‬੒͕ͦͷಛҟͳ૬‫ڍ‬ಈʹେ͖͘Ө‫͢ڹ‬Δ͜ͱΛ֬ೝ͠ɺ·ͨ෼ࢠͷ֤෦෼ͷӡಈੑ͕֤૬ʹΑΓେ͖͘ҟͳΔ͜ͱΛ‫ݟ‬ग़ͨ͠ɻʢ̍̌ʣΠΦϯӷମͷ‫( ڀݚ‬ੴ֞ɺদԬɺ໦ଜ)Πϛμκʔϧ‫ܥ‬ΠΦϯӷମͷΨϥεసҠΛ NMR ‫ͼٴ‬γϛϡϨʔγϣϯʹΑΓௐ΂ͨɻͦͷ݁Ռɺ݁থͱΨϥεঢ়ଶͷӡಈͷ૬ҟ΍ɺ༷ʑͳ‫ߏॴہ‬଄ͷ‫ܗ‬੒͕໌Β͔ͱͳͬͨɻʢ̍̍ʣϑΟʔυόοΫ૿‫ڧ‬ϚΠΫϩϨΦϩδʔͷ։ൃʢM. Bremerich, H.Ayadeɺ༗দɺ੢ᖒɺਫ໺ʣ
ޫτϥοϓͨ͠ϓϩʔϒཻࢠͷมҐΛ̐෼ׂϑΥτμΠΦʔυͰਫ਼ີ‫ܭ‬ଌ͠ɺ͞Βʹ‫ܭ‬ଌ৴߸Λ΋ͱʹϐΤκ‫ۦ‬ಈεςʔδɺ͓Αͼ̖̤̙Λߴ଎ϑΟʔυόοΫ੍‫ͳ͠ޚ‬͕Β active-passive ϚΠΫϩϨΦϩδʔ‫ܭ‬ଌΛߦͬͨɻैདྷ‫͗͢ڧ‬Δඇฏߧ༳Β͗ͷͨΊʹϓϩʔϒཻࢠΛ҆ఆัଊͰ͖ͳ͍ࢼྉʢࡉ๔಺෦΍༡૸όΫςϦΞ༹ӷʣͰϚΠΫϩϨΦϩδʔ‫ܭ‬ଌΛߦ͍ɺ༳ಈࢄҳఆཧͷഁΕ΍ඇฏߧ༳Β͗ͷ෼෍‫ܗ‬ঢ়ͷղੳΛߦͬͨɻʢ̍̎ʣࡉ๔ࠎ֨ͷඇઢ‫͔ͭܗ‬ඇ౳ํ͔ͭඇΞϑΝΠϯͳྗֶԠ౴ʢD. Head, ஑ลӵඒɺதӹ࿕ࢠɺP.Zhang, ໦ԼӳɺL.G. Villaruz, ҆౻঵࢘ɺਫ໺ʣ
ࡉ๔ࠎ֨ʹ࣠ରশͳԠྗΛՃ͑ͭͭ޿ଳҬϚΠΫϩϨΦϩδʔΛߦͬͨɻͦͷͷඇઢ‫͔ͭܗ‬ඇ౳ํͳԠ౴Λఆྔతʹղੳ͢Δ͜ͱͰɺ10-10kHz ͷϚΫϩͳϨΦϝʔλͰ͸‫ܭ‬ଌͰ͖ͳ͍தؒप೾਺ҬʹΞϑΝΠϯ͔ͭ஄ੑతͳྗֶԠ౴͕ଘࡏ͢Δ͜ͱΛ໌

139Β͔ʹ͠ɺͦΕҎԼͷप೾਺Ҭʹ͓͚Δ؇࿨͕ωοτϫʔΫͷඇΞϑΝΠϯม‫ʹܗ‬ΑΔ΋ͷͰ͋Δ͜ͱΛ࣮ূͨ͠ɻ
ʢ̍̏ʣࡉ๔ࠎ֨ͷඇฏߧ༳Β͗͸৽͍͠Ϋϥεͷ Levy ෼෍ʹଐ͢ΔʢHeev Ayadeɺ

Irwin Zaid, ਫ໺ʣඇฏߧͳࡉ๔ࠎ֨ʢΞΫνϯ/ϛΦγϯήϧʣதʹ͓͚ΔϚΠΫϩϨΦϩδʔ‫ܭ‬ଌʹΑΓ‫؍‬ଌ͞ΕΔඇฏߧ༳Β͕͗ɺ৽͍͠Ϋϥεͷ Levy ෼෍ʹଐ͍ͯ͠Δ͜ͱΛ໌Β͔ʹͨ͠ɻ·ͨɺͦͷ෼෍‫ܗ‬ঢ়Λɺྗੜ੒ͷಈྗֶ΋ߟྀʹ͍Εͨ࣌ؒൃల͢Δղੳղͱͯ͠‫ٻ‬Ίͨɻ͜ΕʹΑΓࡉ๔ࠎ֨಺෦ʹ͓͚Δྗੜ੒Λ༳Β͔͗Βਪఆ͢Δ͜ͱ͕Մೳʹͳͬͨɻ
ʢ̍ 4ʣΦϐΦΠυ৴߸఻ୡෳ߹ମͷߏ଄‫ܗ‬੒ͱμΠφϛΫεʹϑΟϥϛϯ A ͕Ռͨ͢໾ׂʢLara Gay Villaruz, ਫ໺ʣΦϐΦΠυ৘ใ఻ୡෳ߹ମͷ૊৫Խʹରͯ͠ FLNA ͕Ռͨ͢໾ׂΛੜԽֶత͓Αͼ෺ཧత (φϊϝΧχΫε,1 ෼ࢠ‫ܭ‬ଌ) ख๏Λ༻͍ͯ௚઀‫ܭ‬ଌ͢Δ͜ͱΛ໨ඪͱͨ͠ɻFLNA͕ 2 ࣍‫ݩ‬ບ಺ͷ৴߸఻ୡෳ߹ମͷ૊৫Խͱࡉ๔ (ࠎ֨) ͷ 3 ࣍‫ߏݩ‬଄ͱΛ݁ͼ͚ͭΔޮ
ՌΛղ໌͢ΔͨΊʹɺࡉ๔ບͱ௚Լͷࡉ๔ࠎ֨ͷྗֶಛੑΛ྆ํௐ΂ɺ MOP-R ͷ‫ػ‬ೳͱͷ૬ؔΛ‫ٻ‬ΊΔ͜ͱʹΑΓɺΦϐΦΠυ‫ܥ‬௟௧ࡎʹର͢Δ଱ੑͦͷଞͷ෭࡞༻ͷൃ‫ʹݱ‬ରͯ͠ FLNA ͕Ռ͍ͨͯ͠Δ໾ׂͱͦͷ‫໌͕ߏػ‬Β͔ʹͳΔɻ
ʢ̍̑ʣ༡૸όΫςϦΞ‫ݒ‬୙ӷதʹ͓͚Δඇฏߧ༳Β͗ͷ౷‫ܭ‬෼෍ʢ‫ڤݪ܀‬ɺ༗ཹਅਓɺ

Heev Ayade, Irwin Zaid, ਫ໺େհʣ
ഓཆӷதͰ༡૸͢ΔόΫςϦΞʢେ௎‫ە‬ʣ΍୯ࡉ๔ඍੜ෺ʢΫϥϛυϞφεʣ͕ੜΈग़͢ඇฏߧ༳Β͕͗ Levy ͷ҆ఆ෼෍ʹଐ͢Δ͜ͱΛ໌Β͔ʹͨ͠ɻͦͷ࣌ؒൃలΛղ
ੳ͢Δ͜ͱͰɺඇฏߧ༳Β͗ʹ LEVY ෼෍͕ීวతʹ‫ݱ‬ΕΔ‫ͱߏػ‬৚݅Λ໌Β͔ʹ͢Δ͜ͱ͕ࠓ‫ޙ‬ͷ՝୊Ͱ͋Δɻ དྷ೥౓ͷ໨ඪ ‫ڀݚ‬ʢ̍ʖ̍̑ʣͷ͞ΒͳΔൃలɺ‫ڭͼٴ‬ҭͷॆ࣮ɻൃද࿦จ ‫ݪ‬ஶ࿦จ 
Interparticle force between diﬀerent types of nematic colloids:

140

Kuniyoshi Izaki and Yasuyuki Kimura,Physical Review E, 87, 062507 (2013) ɹStable cluster phase of Janus particles in two dimensions:
Yasutaka Iwashita, Yasuyuki Kimura,Soft Matter 9, 10694 (2013)
Hydrodynamic eﬀects in the measurement of interparticle forces in nematic colloids:
Kuniyoshi Izaki and Yasuyuki Kimura,Physical Review E, 88, 054501 (2013) ɹ
local mechanical response in semiﬂexible polymer networks subjected to an axisymmetric prestress:
David Head and Daisuke Mizuno,
Physical Review E 22717 88 (2013)
High-frequency aﬃne mechanics and nonaﬃne relaxation in a model cytoskeleton:
David Head, Emi Ikebe, Akiko Nakamasu, Peijuan Zhang, Lara Gay Villaruz, Suguru
Kinoshita, Shoji Ando and Daisuke Mizuno,
Physical Review E 42711 89 (2014)ߨԋ ւ֎Ͱͷߨԋ 
Hydrodynamically induced collective motion of optically driven colloidal particles ona ring:Yasuyuki Kimura, Shuhei Shibata and Yuriko Sassa,
International Soft Matter Conference 2013, Rome, Italy, September 15-19, 2013
Patterns in hexagonally close-packed Janus colloidal monolayer:
Y. Iwashita, and Y. Kimura,International Soft Matter Conference 2013, Rome, Italy, September 15-19, 2013
Cluster structures of Janus colloidal particles controlled by tunable attractive interac141

tion:
Y. Iwashita, and Y. Kimura,International Soft Matter Conference 2013, Rome, Italy, September 15-19, 2013
Melting of an Isolated Two-dimensional Colloidal Crystal:
Sayuri Tanaka, Yasutaka Iwashita and Yasuyuki Kimura,International Soft Matter Conference 2013, Rome, Italy, September 15-19, 2013
Aggregates of Amphiphilic Janus Particles in a Binary Liquid Mixture:
Tomohiro Noguchi, Yasutaka Iwashita and Yasuyuki Kimura,International Soft Matter Conference 2013, Rome, Italy, September 15-19, 2013
Microrheology study of crowding eﬀects on cell mechanics:
Kenji Nishizawa, Kei Fujiwara, Miho Yanagisawa and Daisuke Mizuno,
International Soft Matter Conference 2013, Rome, Italy, September 15-19, 2013
Levy statistics and dynamics in active cytoskeletons:
Irwin Zaid, Heev Ayade and Daisuke Mizuno,
International Soft Matter Conference 2013, Rome, Italy, September 15-19, 2013
Interparticle force between nematic colloids:
Yasuyuki kimura and Kuniyoshi Izaki,
12th European Conference on Liquid Crystals, Rhodes, Greece, September 22-27, 2013
Interaction between nematic colloids with diﬀerent types of defects:
Kuniyoshi Izaki, Yasutaka Iwashita and Yasuyuki kimura,
12th European Conference on Liquid Crystals, Rhodes, Greece, September 22-27, 2013
Levy statistics and dynamics in active cytoskeletons:
Daisuke Mizuno,
2013 SPP Physics Congress, University of San Carlos, Cebu city, PhilippinesɼOctober24, 2013
Levy statistics and dynamics in active cytoskeletons:
Daisuke Mizuno,
142

Taiwan International Workshop on Biological Physics and Complex Systems (BioComplexTaiwan-2013)ɼNational Taiwan University, July 19, 2013
Levy statistics and dynamics in active cytoskeletons:
Daisuke Mizunoɼ
15th SPVM National Physics Conference in Davao, Davao City, PhilippinesɼOctober
26, 2013
Athermal Fluctuations of Probe Particles in Active Cytoskeletal Network:
Heev Ayade, Irwin Zaid, Daisuke Mizuno,
KITP conference ”Active Processes in Living and Nonliving Matter” University ofCalifornia, Santa Barbara, USAɼFebruary 10, 2014
Athermal Fluctuations of Probe Particles in Active Cytoskeletal Network:
Heev Ayade, Irwin Zaid, Daisuke Mizuno,
58th annual meeting of Biophysical Society, Moscone Convention Center, San Francisco, USAɼFebruary 16, 2014
Non-Gauss athermal ﬂuctuations in Bacterial bath :Masato Aridome, takasi kurihara, Heev Ayade, Irwin Zaid, Daisuke Mizuno,
KITP conference ”Active Processes in Living and Nonliving Matter”, Kavli Institutefor Theoretical Physics, University of California, Santa Barbara, USA ɼFebruary 12,
2014
Non-Gauss athermal ﬂuctuations in Bacterial bath:
Masato Aridome, takasi kurihara, Heev Ayade, Irwin Zaid, Daisuke Mizuno,
58th annual meeting of Biophysical Society, Moscone Convention Center, San Francisco, USAɼFebruary 18, 2014 ࠃ಺Ͱͷߨԋ Ϡψεཻࢠͷࣗ‫ݾ‬૊৫Խ:‫ؠ‬Լɹ༃޹
ୈ 3 ճιϑτϚλʔ‫ڀݚ‬ձ

143ωϚνοΫίϩΠυؒ૬‫༻࡞ޓ‬ͷଌఆ๏ͷൺֱͱͦͷԠ༻:Ҫ࡚ ๜ٛɺ‫ؠ‬Լ ༃޹ɺ໦ଜ ߁೭ୈ 3 ճιϑτϚλʔ‫ڀݚ‬ձӷথి‫ؾ‬ରྲྀʹ‫ۦ‬ಈ͞ΕͨίϩΠυཻࢠ‫ܥ‬ͷ‫ڍ‬ಈ:ߴ‫݈ ڮ‬ଠ࿠ɺ‫ؠ‬Լ ༃޹ɺ໦ଜ ߁೭ୈ 3 ճιϑτϚλʔ‫ڀݚ‬ձ‫ͱٿ‬ପԁ͔ΒͳΔίϩΠυ‫ܥ‬ͷߏ଄:দ‫ ݩ‬େ‫ޗ‬ɺ‫ؠ‬Լ ༃޹ɺ໦ଜ ߁೭ୈ 3 ճιϑτϚλʔ‫ڀݚ‬ձਫʔ༉ࠞ߹‫͚͓ʹܥ‬Δ྆਌ഔੑϠψεཻࢠ͕‫ܗ‬੒͢Δ‫ߏूڽ‬଄:໺‫׮๎ ޱ‬ɺ‫ؠ‬Լ ༃޹ɺ໦ଜ ߁೭ୈ 3 ճιϑτϚλʔ‫ڀݚ‬ձԁ‫্؀‬Λޫ‫ۦ‬ಈ͞ΕͨίϩΠυ‫ܥ‬ͷࣔ͢ϦζϜӡಈ:େ‫ٱ‬อ ল‫ޗ‬ɺ‫ؠ‬Լ ༃޹ɺ໦ଜ ߁೭ୈ 3 ճιϑτϚλʔ‫ڀݚ‬ձ༗‫ݶ‬αΠζͷೋ࣍‫ݩ‬ίϩΠυ‫ूڽ‬ମͷ༥ղͷ‫ڀݚ‬:ాத খඦ߹ɺ‫ؠ‬Լ ༃޹ɺ໦ଜ ߁೭ୈ 3 ճιϑτϚλʔ‫ڀݚ‬ձҰ࣠৳௕͞Εͨ૬෼཭ϦϙιʔϜͷม‫ܗ‬:༞Լ ַࢤɺ༄ᖒ ࣮ึɺ‫ؠ‬Լ ༃޹ɺ໦ଜ ߁೭ୈ 3 ճιϑτϚλʔ‫ڀݚ‬ձଟ༷ͳߴ෼ࢠͷࠞΈ߹͍ޮՌ͕ࡉ๔಺೪ੑ΁‫͢΅ٴ‬Ө‫ڹ‬:੢ᖒ ‫࣏ݡ‬ʢ‫۝‬େӃཧʣɺ౻‫ܚ ݪ‬ʢ౦๺େӃ޻ʣɺ༄ᖒ ࣮ึɺਫ໺ େհୈ 3 ճιϑτϚλʔ‫ڀݚ‬ձίϩΠυ෼ࢠͷࣗ‫ݾ‬૊৫Խ:‫ؠ‬Լɹ༃޹
ୈ 3 ճιϑτͳ෺޻ͷະདྷΛߟ͑Δձ

144

Ϡψεཻࢠ 2 ࣍‫͚͓ʹࢠ֨ݩ‬Δํ޲டং:‫ؠ‬Լɹ༃޹ɺ໦ଜɹ߁೭
೔ຊ෺ཧֶձɹୈ 69 ճ೥࣍େձ
ӷথి‫ؾ‬ରྲྀதʹ෼ࢄͨ͠ίϩΠυཻࢠ‫ܥ‬ͷ༌ૹͱ֦ࢄ:ߴ‫݈ڮ‬ଠ࿠ɼ‫ؠ‬Լ༃޹ɼ໦ଜ߁೭
೔ຊ෺ཧֶձɹୈ 69 ճ೥࣍େձ
ϠψεཻࢠΛར༻ͨۚ͠ଐ໘ͷ‫ݻ‬ମ༠ిମඃ෴:໺‫׮๎ޱ‬ɼ‫ؠ‬Լ༃޹ɼ໦ଜ߁೭
೔ຊ෺ཧֶձɹୈ 69 ճ೥࣍େձ
ྲྀମ૬‫͢༻࡞ޓ‬Δޫ‫ۦ‬ಈཻࢠ‫ܥ‬ͷࣔ͢ϦζϜӡಈ:େ‫ٱ‬อল‫ޗ‬ɼ‫ؠ‬Լ༃޹ɼ໦ଜ߁೭
೔ຊ෺ཧֶձɹୈ 69 ճ೥࣍େձ
ޫϐϯηοτʹΑΓҰ࣠ม‫͞ܗ‬Εͨ૬෼཭ϦϙιʔϜ:༞Լַࢤɼ༄ᖒ࣮ึɼ‫ؠ‬Լ༃޹ɼ໦ଜ߁೭
೔ຊ෺ཧֶձɹୈ 69 ճ೥࣍େձ
ࡉ๔಺ϚΠΫϩϨΦϩδʔʹର͢Δ෼ࢠࠞΈ߹͍ޮՌ:੢ᖒ‫࣏ݡ‬ɼ౻‫ܚݪ‬ɼ༄ᖒ࣮ึɼਫ໺େհ
೔ຊ෺ཧֶձɹୈ 69 ճ೥࣍େձ
༳ಈࢄҳఆཧΛഁΔੜ͖෺ͷඇฏߧ༳Β͗ͷ౷‫ܭ‬෼෍ :ਫ໺େհ
ୈ 69 ճ೔ຊ෺ཧֶձ೥࣍େձγϯϙδ΢ϜʮಈతΏΒ͗ͷීว๏ଇʯ౦ւେֶ, 2014
೥ 03 ݄ 28 ೔ޫϐϯηοτΛ༻͍ͨ૬෼཭ϦϙιʔϜͷҰ࣠ม‫ܗ‬:༞Լַࢤ, ༄ᖒ࣮ึ, ‫ؠ‬Լ༃޹, ໦ଜ߁೭ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
ߴ෼ࢠήϧͷ޿ଳҬϚΠΫϩϨΦϩδʔ:‫ڤݪ܀‬, ༗ཹਅਓ, ਫ໺େհ145

ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
༡૸όΫςϦΞ‫ݒ‬୙ӷதʹ͓͚Δඇฏߧ༳Β͗ͷ౷‫ܭ‬෼෍:༗ཹਅਓ, ‫ڤݪ܀‬,Heev AyadeA, Irwin Zaid, ਫ໺େհୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
ӷথి‫ؾ‬ରྲྀʹΑΔίϩΠυͷ༌ૹͱ֦ࢄ:ߴ‫݈ڮ‬ଠ࿠, ‫ؠ‬Լ༃޹, ໦ଜ߁೭ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
‫ͱٿ‬ପԁཻࢠ͔ΒͳΔίϩΠυ‫ܥ‬ͷߏ଄:দ‫ݩ‬େ‫ޗ‬, ాதখඦ߹, ‫ؠ‬Լ༃޹, ໦ଜ߁೭ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
ϠψεཻࢠʹΑΔۚଐཻࢠͷඃ෴ߏ଄‫ܗ‬੒:໺‫׮๎ޱ‬, ‫ؠ‬Լ༃޹, ໦ଜ߁೭ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
ྟք༝དྷ૬‫ʹ༻࡞ޓ‬ΑΔҟछཻࢠࠞ߹‫ܥ‬ͷ‫ूڽ‬:‫ؠ‬Լ༃޹, ໦ଜ߁೭, ‫ۄ‬Ҫୡ࠸ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
༗‫ݶ‬αΠζͷೋ࣍‫ݩ‬ίϩΠυ݁থͷ‫ڀݚ‬:ాதখඦ߹, ‫ؠ‬Լ༃޹, ໦ଜ߁೭ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
ޫ‫ۦ‬ಈཻࢠ‫ܥ‬ͷμΠφϛΫε:େ‫ٱ‬อল‫ޗ‬, ૿ా૖େ, ‫ؠ‬Լ༃޹, ໦ଜ߁೭ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
ϗϩάϥϑΟοΫޫϐϯηοτΛ༻ཻ͍ͨࢠૢ࡞:૿ా૖େ, େ‫ٱ‬อল‫ޗ‬, ‫ؠ‬Լ༃޹, ໦ଜ߁೭ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
ωϚνοΫίϩΠυ૬‫༻࡞ޓ‬ͷ৽ͨͳଌఆ๏:146

Ҫ࡚๜ٛ, Տଜོ߂, ‫ؠ‬Լ༃޹, ໦ଜ߁೭ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
ి৔ԼͰͷωϚνοΫίϩΠυؒ૬‫༻࡞ޓ‬:Տଜོ߂, Ҫ࡚๜ٛ, ‫ؠ‬Լ༃޹, ໦ଜ߁೭ୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
ϦΤϯτϥϯτӷথ 6OCBɾ8OCB ͷ NMR:
த໺༟ੜ, ໦ଜ߁೭, ொాޫஉୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
ΠΦϯӷମ [DEME][BF4] ͱਫͷࠞ߹෺ͷ NMR:
দԬྑय़, ໦ଜ߁೭, ொాޫஉୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
ΠΦϯӷମ bmimPF6 ͷ૬సҠͱμΠφϛΫεɹɹʖ NMR ʹΑΔଌఆʕ:ੴ֞෢࢜, ໦ଜ߁೭, ொాޫஉୈ 119 ճ೔ຊ෺ཧֶձ‫۝‬भࢧ෦ྫձ
Ϡψεཻࢠͱۚଐཻࢠͷෳ߹ߏ଄:໺‫׮๎ޱ‬ɼ‫ؠ‬Լ༃޹ɼ໦ଜ߁೭
೔ຊ෺ཧֶձɹ 2013 ೥ळ‫ق‬େձ༗‫ݶ‬αΠζͷೋ࣍‫ݩ‬ίϩΠυ݁থͷফ໓աఔ:ాதখඦ߹ɼ‫ؠ‬Լ༃޹ɼ໦ଜ߁೭
೔ຊ෺ཧֶձɹ 2013 ೥ळ‫ق‬େձ֎ྗԼͰͷϦϙιʔϜͷ૬෼཭ͱม‫ܗ‬:༞Լַࢤɼ༄ᖒ࣮ึɼ‫ؠ‬Լ༃޹ɼ໦ଜ߁೭
೔ຊ෺ཧֶձɹ 2013 ೥ळ‫ق‬େձପԁཻࢠΛ༻͍ͨߏ଄‫ܗ‬੒:দ‫ݩ‬େ‫ޗ‬ɼాதখඦ߹ɼ‫ؠ‬Լ༃޹ɼ໦ଜ߁೭
೔ຊ෺ཧֶձɹ 2013 ೥ळ‫ق‬େձ

147ӷথి‫ؾ‬ରྲྀதͷίϩΠυཻࢠ‫ܥ‬ͷμΠφϛΫε:ߴ‫݈ڮ‬ଠ࿠ɼ‫ؠ‬Լ༃޹ɼ໦ଜ߁೭
೔ຊ෺ཧֶձɹ 2013 ೥ळ‫ق‬େձޫ‫ۦ‬ಈίϩΠυ‫ܥ‬ͷμΠφϛΫε:େ‫ٱ‬อল‫ޗ‬ɼࣲాबฏɼ‫ؠ‬Լ༃޹ɼ໦ଜ߁೭
೔ຊ෺ཧֶձɹ 2013 ೥ळ‫ق‬େձࡉ๔಺ϚΠΫϩϨΦϩδʔʹର͢Δ෼ࢠࠞΈ߹͍ޮՌ:੢ᖒ‫࣏ݡ‬ɼ౻‫ܚݪ‬ɼ༄ᖒ࣮ึɼਫ໺େհ
೔ຊ෺ཧֶձɹ 2013 ೥ळ‫ق‬େձి‫ؾ‬ӭಈޫࢄཚͷ‫( ૅج‬ট଴ߨԋ):໦ଜ ߁೭
ୈ 25 ճࢄཚ‫ڀݚ‬ձ 2013 ೥ 11 ݄ 15 ೔ HULIC HALL

Microrheology of equilibrium and non-equilibrium complex ﬂuids (Invited):
Yasuyuki Kimura
Workshop on Non-Equilibrium Complex Fluids, March 6 , 2014 Tokyo Metropolitan
University (Hachioji, Tokyo)
Athermal Fluctuations of Probe Particles in Active Cytoskeletal Networks:
Zaid Irwin, Ayade Heev, Yeomans Julia, Mizuno Daisukeୈ 51 ճ೔ຊੜ෺෺ཧֶձ೥ձ The 51st Annual Meeting of the BSJɼposter, ‫౎ژ‬ɺΞωοΫεϗʔϧɼ2013/10/28

Nonlinear stress propagation, anisotropic stiﬀening, and nonaﬃne relaxations in cytoskeletal networks:ਫ໺ େհ, Villaruz Lara, தӹ ࿕ࢠ, ஑ล ӵඒ, Head David,
ୈ 51 ճ೔ຊੜ෺෺ཧֶձ೥ձ The 51st Annual Meeting of the BSJɼposter, ‫౎ژ‬ɺΞωοΫεϗʔϧɼ2013/10/28

Molecular crowding eﬀects on intracellular mechanical environments:੢ᖒ‫࣏ݡ‬, ౻‫ܚݪ‬, ༄ᖒ࣮ึ, ਫ໺େհ,೔ຊੜ෺෺ཧֶձ 2013 ೥ձʢ‫ࡍࠃ౎ژ‬ձٞ৔ɼ2013 ೥ 10 ݄148ੜ͖෺ͷඇฏߧ༳Β͗ͷ౷‫ܭ‬෼෍ͱྗֶಛੑ:ਫ໺େհ
ୈ 7 ճ෺ੑՊֶྖҬԣஅ‫ڀݚ‬ձ (ྖҬ߹ಉ‫ڀݚ‬ձ) ౦‫ژ‬େֶɾ෢ాϗʔϧɹ 2013 ೥ 12݄1೔ϚΠΫϩϨΦϩδʔΛ༻͍ͨࡉ๔಺෦ͷྗֶಛੑͷ‫ڀݚ‬ʙ෼ࢠͷࠞΈ߹͍ޮՌʙ:੢ᖒ‫࣏ݡ‬, ౻‫ܚݪ‬, ༄ᖒ࣮ึ, ਫ໺େհ,ୈҰճ੢೔ຊඇฏߧϛχγϯϙδ΢Ϝɼ‫۝‬भେֶ 2013 ೥ 5 ݄

Glass-like behavior in cells:੢ᖒ‫࣏ݡ‬, ౻‫ܚݪ‬, Marcel Bremerich, ༄ᖒ࣮ึ, ਫ໺େհ,7th Mini-Symposium on Liquidsɼ‫۝‬भେֶɼ2013 ೥ 7 ݄ੜ͖෺ͷඇฏߧ༳Β͗ɾࠞΈ͍͋ޮՌͱྗֶಛੑ:ਫ໺େհ༳Β͗ͱߏ଄ͷ‫ڠ‬૗ɿඇฏߧ‫͚͓ʹܥ‬Δීว๏ଇͷ֬཰ୈҰճྖҬ‫ڀݚ‬ձ, KKR ϗςϧ೤ւɺ2013 ೥ 12 ݄ 25 ೔ʕ12 ݄ 27 ೔ੜମιϑτϚλʔͷඇฏߧྗֶ‫ܭ‬ଌγεςϜͷ։ൃ:ਫ໺େհɺ

2013 Ѵ঳ࢠࡒஂॿ੒‫ൃڀݚ‬දձ, ϗςϧάϥϯυώϧࢢϲ୩ɺ2013 ೥ 7 ݄ 29 ೔ࡉ๔ूஂ͕‫ܗ‬੒͢Δ૊৫ͷඇઢ‫ܗ‬ɾඇฏߧϝΧχΫεͱࣗൃੜ੒ྗͷ‫؍‬ଌ:ਫ໺େհϛΫϩ͔ΒϚΫϩ΁֊૚Λ௒͑Δடং‫ܗ‬੒ͷϩδοΫ 2013 ೥౓൝ձٞ, ୶࿏ເ෣୆ࠃ
ࡍձٞ৔ɺ2013 ೥ 6 ݄ 12 ೔ʕ14 ೔ϚΠΫϩϨΦϩδʔΛ༻͍ͨඇฏߧ‫ܥ‬ʢੜ͖෺ʣͷྗֶ‫ܭ‬ଌ:ਫ໺େհ,ϛΫϩ͔ΒϚΫϩ΁֊૚Λ௒͑Δடং‫ܗ‬੒ͷϩδοΫՆ߹॓‫ڀݚ‬ձ୶࿏ເ෣୆ࠃࡍձ
ٞ৔ɺ2013 ೥ 8 ݄ 26 ೔ʕ28 ೔

֎෦ࢿۚ

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 จ෦লՊֶ‫ڀݚ‬අิॿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ (৽ֶज़ྖҬ)ɺ‫ܭ‬ը‫ڀݚ‬ඇ೤తʹ‫ۦ‬ಈ͞ΕͨόΠΦϚλʔͷඇฏߧಈྗֶ
‫ڀݚ‬୅දऀɿ໦ଜ߁೭
จ෦লՊֶ‫ڀݚ‬අิॿۚɺ‫ج‬൫‫( ڀݚ‬B)
ϚϧνϏʔϜ̏࣍‫ݩ‬ϚΠΫϩϨΦϩδʔ‫ݦ‬ඍ‫ڸ‬ͷ։ൃͱͦͷιϑτϚλʔ΁ͷԠ༻‫ڀݚ‬୅දऀɿ໦ଜ߁೭
จ෦লՊֶ‫ڀݚ‬අิॿۚɺ௅ઓత๖ժ‫ڀݚ‬ΤΩκνοΫίϩΠυ‫ܥ‬ͷ৽‫ߏۭؒ࣌ن‬଄ͷ‫ڀݚ‬‫ڀݚ‬୅දऀɿ໦ଜ߁೭
จ෦লՊֶ‫ڀݚ‬අิॿۚɺएख‫( ڀݚ‬A)
ࡉ๔಺෦ͷඇฏߧྗֶʹ‫ͮ͘ج‬ඇ೤త༳ಈྗͷ‫ܭ‬ଌ‫ڀݚ‬୅දऀ :ɹਫ໺େհ
จ෦লՊֶ‫ڀݚ‬අิॿۚɺ௅ઓత๖ժ‫ڀݚ‬ଟཻࢠޫτϥοϓʹΑΔਆ‫ࡉܦ‬๔ͷ࣠ࡧ৳௕ͷ੍‫ͦͱޚ‬ͷಛҟੑͷ‫ݯى‬ͷղ໌‫ڀݚ‬୅දऀ :ɹਫ໺େհ
จ෦লՊֶ‫ڀݚ‬අิॿۚɺएख‫( ڀݚ‬B)
ίϩΠυ෼ࢠͷࣗ‫ݾ‬૊৫Խ‫ڀݚ‬୅දऀɿ‫ؠ‬Լ༃޹ จ෦লՊֶ‫ڀݚ‬අิॿۚҎ֎ͷ֎෦ࢿۚ ෢ాՊֶ‫ॿڀݚ‬੒ਓ޻ࠎࡉ๔ωοτϫʔΫʹ͓͚Δྗֶܹࢗ৘ใ఻ୡաఔͷղੳ‫ڀݚ‬୅දऀ :ɹਫ໺େհ
಺౻‫ه‬೦Պֶৼ‫ஂࡒڵ‬ྗֶܹࢗΛ‫ݕ‬ग़͢Δ͜ͱͰࣗΒΛ࡞Γม͑Δਓ޻ࠎγεςϜͷ։ൃ‫ڀݚ‬୅දऀ :ɹਫ໺େհ

150

೔ຊֶज़ৼ‫ڵ‬ձಛผ‫ڀݚ‬һ౳‫ڞͼٴ‬ಉ‫ڀݚ‬ͷ࠾୒ (ֶ֎͔Βͷड͚ೖΕΛ‫ؚ‬Ή)ଞେֶͰͷ‫ڭͱڀݚ‬ҭֶ෦̐೥ੜଔ‫ڀݚۀ‬Տଜོ߂ɿ(ࢦಋ‫ڭ‬һɺ໦ଜ߁೭)ɿి৔ԼͰͷωϚνοΫίϩΠυͷཻࢠؒྗଌఆ
૿ా૖େɿ(ࢦಋ‫ڭ‬һɺ໦ଜ߁೭)ɿϗϩάϥϑΟοΫޫϐϯηοτʹΑΔཻࢠૢ࡞ͷ‫ݚ‬‫ڀ‬༗ཹਅਓɿ(ࢦಋ‫ڭ‬һɺਫ໺େհ) ༡૸όΫςϦΞ‫ݒ‬୙ӷதʹ͓͚Δඇฏߧ༳Β͗ͷ౷‫ܭ‬෼෍ɿ
‫ڤݪ܀‬ɿ(ࢦಋ‫ڭ‬һɺਫ໺େհ) ߴ෼ࢠήϧͷ޿ଳҬϚΠΫϩϨΦϩδʔɿम࢜࿦จҪ࡚๜ٛɿ(ࢦಋ‫ڭ‬һɺ໦ଜ߁೭)ɿωϚνοΫӷথதͷҟํతཻࢠؒ૬‫ͦͱ༻࡞ޓ‬ͷԠ༻‫ۄ‬Ҫୡ࠸ɿ(ࢦಋ‫ڭ‬һɺ໦ଜ߁೭ɾ‫ؠ‬Լ༃޹)ɿ༹ഔͷྟքੑΛར༻ͨ͠ίϩΠυ‫ूڽ‬ͷ੍‫ޚ‬উా߁ฏɿ(ࢦಋ‫ڭ‬һɺ໦ଜ߁೭)ɿίϨεςϦοΫӷথి‫ؾ‬ରྲྀͷύλʔϯͷ‫ڀݚ‬ాதখඦ߹ɿ(ࢦಋ‫ڭ‬һɺ໦ଜ߁೭)ɿ༗‫ݶ‬αΠζͷೋ࣍‫ݩ‬ίϩυ݁থͷ‫ڀݚ‬ੴ֞෢࢜ɿ(ࢦಋ‫ڭ‬һɺ໦ଜ߁೭)ɿΠΦϯӷମʦbmimʧʦPF6 ʧͷ NMR ଌఆͱ෼ࢠಈ
ྗֶγϛϡϨʔϣϯத໺༟ੜɿ(ࢦಋ‫ڭ‬һɺ໦ଜ߁೭)ɿ1H-,13C-NMR ʹΑΔϦΤϯτϥӷথ 6OCB-8OCB
ͷμΠφϛΫεͷ‫ڀݚ‬༗দ‫׮‬ɿ(ࢦಋ‫ڭ‬һɺ໦ଜ߁೭)ɿ֎ྗҹՃԼʹ͓͚ΔϑΟʔυόοΫΛ༻͍ͨࡉ๔಺ϚΠϩϨΦδʔ
ࢁຊঊɿ(ࢦಋ‫ڭ‬һɺ໦ଜ߁೭)ɿ‫ݦ‬ඍ‫༻࡯؍ڸ‬ಁੳηϧΛ͍ͨΞΫνϯ-ϛΦγϯήϧ
ͷϚΠΫϩϨδʔ֎ࠃਓཹֶੜͷड͚ೖΕHeev Ayade (ਫ໺େհ)Lara Gay Villaruz (ਫ໺େհ)151

ு௨ʢਫ໺େհʣ

Benjamin Brunel (୹‫ظ‬ɹ 5 έ݄ɹਫ໺େհ)ֶ֎Ͱͷֶձ‫׆‬ಈࢄཚ‫ڀݚ‬ձӡӦҕһ ɹʢ໦ଜʣ
ιϑτϚλʔ‫ڀݚ‬ձӡӦҕһ ɹʢ໦ଜʣ
೔ຊੜ෺෺ཧֶձɹ஍۠ҕһ (ਫ໺)ͦͷଞͷ‫׆‬ಈͱ੒Ռฏ੒̎̒೥෺ཧֶՊମ‫ݧ‬ೖֶߨԋձɹʮޫͰϛΫϩͳ෺ମΛૢΔʯɹʢ݄̏ɺ໦ଜʣ

152

ෳࡶྲྀମ
‫ߏࣨڀݚ‬੒һಖాণ೭ ‫ڭ‬त༄ᖒ࣮ึ ॿ‫ڭ‬ େֶӃ ത࢜՝ఔ ࢁԼ༟ଠ࿕ େֶӃ म࢜՝ఔ 
୙઒৻ฏ

ࢁԼହ߂

٢ా‫྄و‬

ࠤ౻‫و׮‬

੢ᖒ‫࣏ݡ‬

 ֶ෦ ଔ‫ڀݚۀ‬ੜ 
ਗ਼ాᠳ

౻Ҫརً

୲౰त‫ۀ‬
ࣗવՊֶ૯߹࣮‫ݧ‬ʢ༄ᖒ࣮ึʣ
෺ཧֶಛผߨٛ A(෺ཧֶ࠷લઢ)ʢ༄ᖒ࣮ึʣ
‫ૅج‬෺ཧ࣮‫ֶݧ‬ɾಉ࣮‫ݧ‬ʢಖాণ೭ɾ༄ᖒ࣮ึʣ
ྗֶ‫ૅج‬ɾಉԋशʢಖాণ೭ʣ
೤ͱ೾ಈ࿦‫ૅج‬ʢಖాণ೭ʣ
೤ྗֶʢಖాণ೭ʣ
‫ڀݚ‬ɾ‫ڭ‬ҭ໨ඪͱ੒Ռ
ߴ෼ࢠࠞ߹༹ӷʹ͓͚Δ૬෼཭ͱήϧԽʹؔ͢Δ‫( ڀݚ‬ಖాণ೭ɺ༄ᖒ࣮ึɺࢁԼ༞
ଠ࿕)θϥνϯͳΒͼʹϙϦΤνϨϯάϦίʔϧʢ̥̜̚ʣ͸Α͘஌ΒΕͨਫ༹ੑߴ෼ࢠͰ
͋Δɽ͜ΕΒͷߴ෼ࢠΛࠞ߹ͨ͠ਫ༹ӷʹ͓͍ͯ‫ڵ‬ຯਂ͍૬෼཭‫ݱ‬৅͕‫͍ͩ͞ݟ‬Εͨɽզʑ͸ɺ͜ͷ૬෼཭‫ݱ‬৅ͷϝΧχζϜΛ໌Β͔ʹ͢Δ͜ͱΛ໨తͱͯ͠‫ڀݚ‬Λߦͬͨɽ̥̜̚ͷ෼ࢠྔΛมԽͤͯ͞ଌఆΛߦͬͨͱ͜Ζɺ૬෼཭఺ͷԹ౓͸̥̜̚ͷ෼ࢠྔʹ‫͘ڧ‬ґଘ͢Δͱ͍͏͜ͱ͕໌Β͔ͱͳͬͨɽϞσϧࡉ๔಺Ͱͷਫੑೋ૬෼཭ͱήϧԽʹΑΔύλʔϯ‫ܗ‬੒ (༄ᖒ࣮ึɺಖాণ೭ɺ୙઒৻ฏ) ࡉ๔಺͸ଟ༷͔ͭଟྔͷੜମߴ෼ࢠ͔Β੒Δߴ೪஄ੑྲྀମͰຬͨ͞Ε͍ͯΔɽ͜ͷࡉ๔಺‫ڥ؀‬ͷϞσϧ‫ͯ͠ͱܥ‬ɼϛ

153

Ϋϩͳ༉தਫణͷ಺෦ʹθϥνϯɾ̥̜̚ਫ༹ӷΛ಺แ͢Δ࣮‫ݧ‬Λߦͬͨɽ͜ͷߴ෼ࢠࠞ߹ਫ༹ӷ͸ɼԹ౓௿Լʹ൐ͬͯਫੑೋ૬෼཭ͱθϥνϯͷήϧԽΛࣔ͢ɽθϥνϯͱӷణք໘ͱͷ૬‫ͱ༻࡞ޓ‬ɺ૬෼཭ΛήϧԽʹΑͬͯఀࢭ͢Δ͜ͱʹΑͬͯɺଟ༷
ͳϛΫϩήϧɾύλʔϯΛੜΈग़͢͜ͱʹ੒ޭͨ͠ɽ
૬෼཭ͨ͠ήϧͷ༌ૹಛੑ (ಖాণ೭ɺ༄ᖒ࣮ึɺࢁԼହ߂)தੑͷߴ෼ࢠଟ౶ͱͯ͠ར༻͞Ε͍ͯΔΞΨϩʔε͸ɺਫ༹ӷதʹ͓͍ͯήϧΛ‫ܗ‬੒ͨ͠ͷͪʹ૬෼཭Λੜ͡Δ͜ͱ͕஌ΒΕ͍ͯΔɽ૬෼཭ʹΑΔ಺෦ߏ଄มԽ͕ήϧͷ෺ੑʹ༩͑ΔӨ‫ڹ‬Λ໌Β͔ʹ͢ΔͨΊɼΞΨϩʔεήϧͷߴ෼ࢠ໢໨ͱਫؒͷຎࡲ܎਺Λଌఆͨ͠ɽ͞Βʹήϧͷߏ଄αΠζΛఆྔԽ͠ɼ͜Εͱήϧͷຎࡲ܎਺ͱͷ૬ؔؔ܎Λ‫ݟ‬ग़͢͜ͱ͕Ͱ͖ͨɽ
઀ணͨ͠ӷణؒʹൃੜ͢Δ઀ணྗධՁʢ༄ᖒ࣮ึɺಖాণ೭ɺ٢ా‫྄و‬ʣࢷ࣭ບͰ෴ΘΕͨϛΫϩαΠζͷ༉தਫణΛ̎ͭ઀ணͤͨ͞ࡍʹൃੜ͢Δ઀ணྗ͕ɼӷణք໘Λ෴͏ࢷ࣭ͷछྨʹΑͬͯͲ͏มԽ͢Δͷ͔ΛఆྔతʹධՁͨ͠ɽࢷ࣭ͷ୸Խਫૉ࠯ʹ‫·ؚ‬ΕΔ୸ૉ਺͕͋Δఆ਺ ΑΓ΋খ͘͞ͳΔͱɼ઀ணྗ͕‫ݮʹܹٸ‬গ͢Δ͜ͱΛ‫ݟ‬ग़͠ɺ‫ݪ‬ஶ࿦จͱͯ͠·ͱΊΔ͜ͱ͕Ͱ͖ͨɽ
ి‫ؾ‬తʹதੑͳήϧͷ๲५‫ڍ‬ಈʢಖాণ೭ɺࠤ౻‫و׮‬ʣి‫ؾ‬తʹதੑͳδϝνϧΞΫϦϧΞϛυήϧʹɺղ཭‫ج‬Λ࣋ͭϞϊϚʔΛ‫ڞ‬ॏ߹ͤ͞Δ͜ͱͰɺήϧͷମੵ૬సҠʹ͓͚ΔΠΦϯԽͷӨ‫ڹ‬Λղੳͨ͠ɽ͜ͷήϧ͸Ξητ
ϯਫ༹ӷԼͰऩॖ͢Δ͕ɺͦͷऩॖ཰͸ήϧͷղ཭౓ʹ‫͘ڧ‬ґଘͨ͠ɽղ཭౓͕খ͞
͍࣌͸ɺΞητϯೱ౓ͷ૿Ճʹ൐ͬͯήϧ͸࿈ଓతʹऩॖɾ࠶๲५͢ΔϦΤϯτϥϯ
τͷ‫ڍ‬ಈΛࣔͨ͠ɽҰํͷղ཭౓͕େ͖͍࣌͸ɺ͋ΔΞητϯೱ౓Ͱෆ࿈ଓతʹॖΉ͜ͱ͕෼͔ͬͨɽདྷ೥౓͸‫ܥ‬ͷԹ౓੍‫ޚ‬ɺి৔੍‫ޚ‬౳ΛࢼΈΔ͜ͱͰɺΠΦϯԽͨ͠ήϧͷ๲५ɾऩॖ‫ݱ‬৅Λղ໌͍ͨ͠ɽ
ࡉ๔಺෦ͷ೪ੑʹର͢Δଟ੒෼ߴ෼ࢠࠞΈ߹͍ޮՌͷӨ‫ڹ‬ʢ༄ᖒ࣮ึɺ੢ᖒ‫࣏ݡ‬ʣࡉ๔಺‫ڥ؀‬Λ෺ཧతʹཧղ͢Δ্Ͱ͸ɼࡉ๔಺ͷྗֶతಛ௃Λղ໌͢Δ͜ͱ͕ඞཁͰ
͋Δɽຊ‫Ͱڀݚ‬͸̍छྨͷ୿ന࣭͔ΒͳΔ BSA ༹ӷͱɺ਺ඦछྨͷ୿ന࣭͔ΒͳΔࡉ
๔நग़ӷʹ͍ͭͯ೪ੑ཰Λଌఆ͠ɺͦͷೱ౓ґଘੑ͔Βࡉ๔಺ͷ෼ࢠࠞΈ߹͍ޮՌʹ
ഭͬͨɽBSA ༹ӷͰ͸ίϩΠυ‫ݒ‬୙ӷͷΨϥεసҠલ‫ݱۦ‬৅ͱಉ͡Α͏ͳৼΔ෣͍͕‫ݟ‬ΒΕΔ͕ɼࡉ๔நग़ӷͰ͸ΑΓ௿͍ߴ෼ࢠೱ౓Ͱ೪ੑ཰ͷൃࢄࢄҳ͕‫͜ى‬Δ͜ͱ͕
෼͔ͬͨɽࠓ‫ޙ‬͸ଟ੒෼‫Ͱܥ‬͸ΑΓ௿ೱ౓Ͱ೪ੑࢄҳ͕‫͜ى‬Δཧ༝Λ෺ཧతʹ໌Β͔
ʹ͍ͨ͠ɽ

154

Triton ਫ༹ӷͷಶ఺‫ۂ‬ઢͱ૬෼཭ʢಖాণ೭ɺਗ਼ాᠳʣ
ҰൠʹඇΠΦϯੑք໘‫׆‬ੑࡎͷਫ༹ӷ͸Թ౓Λ্͍͛ͯ͘ͱന୙͠, ͜ͷͱ͖ͷԹ౓Λಶ఺ͱ͍͏. ຊ‫Ͱڀݚ‬͸, ୅දతͳඇΠΦϯੑք໘‫׆‬ੑࡎͰ͋Δ Triton X-100 ͱ Triton

X-114 ͷಶ఺ͷೱ౓ґଘੑΛ໌Β͔ʹͨ͠. ࠓ‫ޙ‬ͷ‫Ͱڀݚ‬͸, ͜ΕΒͷ֤‫ܥ‬ͷεϐϊμ
ϧ‫ۂ‬ઢΛܾఆ͠, ·ͨ, ༗‫ػ‬ԘΛఴՃͨ͠ͱ͖ͷ૬‫ڍ‬ಈͷมԽΛ໌Β͔ʹ͢Δ͜ͱΛ໨ࢦ͢.
઀ணͨ͠ϛΫϩӷణ಺ʹ͓͚Δ૬෼཭υϝΠϯͷ഑޲ʢ༄ᖒ࣮ึɺಖాণ೭ɺ౻Ҫརًʣ઀ணͨ̎ͭ͠ͷӷణ಺ʹߴ෼ࢠࠞ߹༹ӷΛ෧ೖͯ͠૬෼཭ͤͨ͞ࡍʹɺ૬෼཭ͷ഑ஔ΁઀ணͨ͠ບք໘͕‫͢΅ٴ‬Ө‫ڹ‬Λղੳͨ͠ɽͦͷ݁Ռɼ૬෼཭ք໘͸ϛΫϩӷణͷ઀ண໘ʹରͯ͠ɼਨ௚͔ਫฏͷͲͪΒ͔ʹଗ͏͜ͱ͕෼͔ͬͨɽ͜ͷ͜ͱ͸ɼϛΫϩۭؒ಺Ͱͷ૬෼཭഑ஔ͸όϧΫ‫࠷Ͱܥ‬΋ࢧ഑తͱͳΔ૬෼཭ք໘ுྗ͚ͩͷ‫د‬༩Ͱ͸ܾ
·ΒͣɺपғͷϛΫϩӷӷք໘ͷӨ‫ڹ‬Λ‫͘ڧ‬ड͚Δ͜ͱΛҙຯ͢Δɽࠓ‫ޙ‬͸͜ͷ‫ߏػ‬Λ໌Β͔ʹ͢Δɽൃද࿦จ ‫ݪ‬ஶ࿦จ 
Generation of giant unilamellar liposomes containing biomacromolecules at physiological intracellular concentrations using hypertonic conditions Kei Fujiwara and Miho
Yanagisawa, ACS Synthetic Biology, in press.
Sol-gel transition and phase separation in ternary system of gelatin-water-poly(ethylene
glycol) oligomer Yutaro Yamashita, Miho Yanagisawa, and Masayuki Tokita, Journalof Molecular Liquids, in press.
Phase separation in binary polymer solution: gelatin/Poly(ethylene glycol) system
Miho Yanagisawa, Yutaro Yamashita, Sada-atsu Mukai, Annaka Masahiko, and Masayuki
Tokita Journal of Molecular Liquids, in press.
Characteristic behavior of crowding macromolecules conﬁned in cell-sized droplets Miho
Yanagisawa, Takahiro Sakaue, and Kenichi Yoshikawa. International Review of Cell

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and Molecular Biology, 307 (2014) pp. 175-204.
Adhesive force between paired microdroplets coated with lipid monolayers Miho Yanagisawa, Taka-aki Yoshida, Miyuki ɹ Furuta, Satoshi ɹ Nakata, and Masayuki Tokita,
Soft Matter, 9 (2013) pp. 5891-5897.
Phase behaviors of agarose gel Takaharu ɹ Morita, Takayuki ɹ Narita, Sada-atsu
Mukai, Miho Yanagisawa, and Masayuki Tokita. AIP Advances, 3 (2013) p. 042128.
Structure and frictional properties of colloid gel. Masayuki Tokita Polymers, 6 (2014)
651-666ஶॻʮήϧͷ࣮ۭؒߏ଄ղੳʯಖాণ೭
ʮήϧͷ҆ఆԽͱ‫ػ‬ೳੑ෇༩ɾ࣍ੈ୅΁ͷԠ༻։ൃʯʢٕज़৘ใ‫ڠ‬ձฤʣ෼୲ࣥච
ʮҰ࣍‫ࢄ֦ݩ‬൓Ԡ‫͚͓ʹܥ‬ΔήϧԽͱύλʔϯ‫ܗ‬੒ʯ੒ా‫ߦو‬ɼԬଜ߳ಸɼಖాণ೭
ʮήϧςΫϊϩδʔϋϯυϒοΫʯʢ‫ࣜג‬ձࣾΤψɾςΟʔɾΤεฤʣ෼୲ࣥච
ʮ‫װج‬෺ཧֶʯ‫ాݪ‬ɾ෭ౡɾ‫܀‬মɾ໼ࢁɾಖాɾຊঙഓ෩‫ؗ‬ɼ෼୲ࣥචߨԋ ւ֎Ͱͷߨԋ 
Spontaneous patterning of gels by conﬁning to microspheres ɹʢϙελʔʣ༄ᖒ ࣮ึ, ୙઒ɹ৻ฏ, ࡔ্ ‫و‬༸, ಖా ণ೭

International Soft Matter Conference 2013ɼΠλϦΞɾϩʔϚʢ2013 ೥ 9 ݄ 17 ೔ʣ
Microrheology study of crowding eﬀects on cell mechanics ɹʢϙελʔʣ੢ᖒ‫࣏ݡ‬, ౻‫ܚݪ‬, Marcel Bremerich, ༄ᖒ࣮ึ, ਫ໺େհInternational Soft Matter Conference 2013ɼΠλϦΞɾϩʔϚʢ2013 ೥ 9 ݄ 18 ೔ʣ ࠃ಺Ͱͷߨԋ 
156

Glass-like behavior in cells੢ᖒ‫࣏ݡ‬, ౻‫ܚݪ‬, ༄ᖒ࣮ึ, ਫ໺େհ7th Mini-Symposium on Liquidsɼ‫۝‬भେֶ੢৽ϓϥβʢ2013 ೥ 7 ݄ 5 ೔ʣɹHydrodynamic friction of phase-separated agarose gelࢁԼ ߁߂, ༄ᖒ ࣮ึ, ಖా ণ೭

7th Mini-Symposium on Liquidsɼ‫۝‬भେֶ੢৽ϓϥβʢ2013 ೥ 7 ݄ 5 ೔ʣ
Phase behavior of binary polymer solution: Gelatin-PEG-water systemࢁԼ༞ଠ࿕ɼ༄ᖒ࣮ึɼಖాণ೭

7th Mini-Symposium on Liquidsɼ‫۝‬भେֶ੢৽ϓϥβʢ2013 ೥ 7 ݄ 5 ೔ʣ
Spontaneous patterning of gels by conﬁning polymer mixture to microspheres༄ᖒ࣮ึʢট଴ߨԋʣ

7th Mini-Symposium on Liquidsɼ෱Ԭ੢ਞϓϥβʢ2013 ೥ 7 ݄ 6 ೔ʣࡉ๔಺ϚΠΫϩϨΦϩδʔʹର͢Δ෼ࢠࠞΈ߹͍ޮՌ੢ᖒ‫࣏ݡ‬, ౻‫ܚݪ‬, ༄ᖒ࣮ึ, ਫ໺େհ೔ຊ෺ཧֶձ 2013 ೥ळେձ, ಙౡେֶʢ2013 ೥ 9 ݄ 25 ೔ʣθϥνϯɾPEGɾਫ 3 ੒෼‫ܥ‬ͷ૬‫ڍ‬ಈͷ PEG ෼ࢠྔґଘੑࢁԼ༞ଠ࿕ɼ༄ᖒ࣮ึɼಖాণ೭
೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɼಙౡେֶʢ2013 ೥ 9 ݄ 27 ೔ʣ૬෼཭ͨ͠ήϧͷྲྀମྗֶతຎࡲ
ࢁԼହ߂ɼ༄ᖒ࣮ึɼಖాণ೭
೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɼಙౡେֶʢ2013 ೥ 9 ݄ 27 ೔ʣΤνϨϯάϦίʔϧɾΦϦΰϚʔਫ༹ӷதʹ͓͚ΔϙϦΞΫϦϧΞϛυήϧͷ๲५‫ڍ‬ಈࠤ౻‫و׮‬ɼ༄ᖒ࣮ึɼಖాণ೭
೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɼಙౡେֶʢ2013 ೥ 9 ݄ 27 ೔ʣϛΫϩӷణ಺Ͱͷߴ෼ࢠ༹ӷͷ૬෼཭ͱήϧԽʹΑΔύλʔϯ‫ܗ‬੒༄ᖒ࣮ึɼ୙઒৻ฏɼࡔ্‫و‬༸ɼಖాণ೭

157

೔ຊ෺ཧֶձ 2013 ೥ळ‫ق‬େձɼಙౡେֶʢ2013 ೥ 9 ݄ 27 ೔ʣ

Aqueous phase separation and sol-gel phase transition of biopolymer blend in cell-sized
droplets༄ᖒ࣮ึʢট଴ߨԋʣ
ୈ 51 ճ೔ຊੜ෺෺ཧֶձ೥ձ, ‫ࡍࠃ౎ژ‬ձٞ৔ʢ2013 ೥ 10 ݄ 28 ೔ʣ

Molecular crowding eﬀects on intracellular mechanical environments੢ᖒ‫࣏ݡ‬, ౻‫ܚݪ‬, ༄ᖒ࣮ึ, ਫ໺େհ೔ຊੜ෺෺ཧֶձ 2013 ೥ձ,ʢ2013 ೥ 10 ݄ 29 ೔ʣࡉ๔αΠζখ๔΁ͷߴ෼ࢠ෧ೖʹΑΔ৽‫ػن‬ೳ૑੒༄ᖒ ࣮ึʢট଴ߨԋʣ

2013 ೥೔ຊԽֶձதࠃ࢛ࠃࢧ෦େձ, ޿ౡେֶʢ2013 ೥ 11 ݄ 16 ೔ʣଟ༷ͳߴ෼ࢠͷࠞΈ߹͍ޮՌ͕ࡉ๔಺೪ੑ΁‫͢΅ٴ‬Ө‫ڹ‬੢ᖒ‫࣏ݡ‬, ౻‫ܚݪ‬, ༄ᖒ࣮ึ, ਫ໺େհୈ̏ճιϑτϚλʔ‫ڀݚ‬ձɼट౎େֶ౦‫ژ‬ʢ2013 ೥ 12 ݄ 13 ೔ʣήϧͷྲྀମྗֶతຎࡲ
ࢁԼହ߂ɼ༄ᖒ࣮ึɼಖాণ೭
೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɼ౦ւେֶʢ2014 ೥ 3 ݄ 27 ೔ʣߴ෼ࢠࠞ߹༹ӷʹ͓͚Δ૬෼཭ͱήϧԽͷΧοϓϦϯά
ࢁԼ༞ଠ࿕ɼ༄ᖒ࣮ึɼಖాণ೭
೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɼ౦ւେֶʢ2014 ೥ 3 ݄ 27 ೔ʣి‫ؾ‬తʹதੑͳήϧͷ๲५‫ڍ‬ಈࠤ౻‫و׮‬ɼ༄ᖒ࣮ึɼಖాণ೭
೔ຊ෺ཧֶձୈ 69 ճ೥࣍େձɼ౦ւେֶʢ2014 ೥ 3 ݄ 27 ೔ʣɽࡉ๔಺෦ͷ೪ੑʹର͢Δଟ੒෼ߴ෼ࢠࠞΈ߹͍ޮՌͷӨ‫ڹ‬੢ᖒ‫࣏ݡ‬, ౻‫ܚݪ‬, ༄ᖒ࣮ึ, ਫ໺େհ೔ຊ෺ཧֶձ 69 ճ೥࣍େձɼ౦ւେֶʢ2014 ೥ 3 ݄ 27 ೔ʣ

158ੜମߴ෼ࢠ༹ӷͷ೪஄ੑͱ૬෼཭‫ڍ‬ಈ༄ᖒ࣮ึʢট଴ߨԋʣ೔ຊ෺ཧֶձ 69 ճ೥࣍େձɼ౦ւେֶʢ2014 ೥ 3 ݄ 27 ೔ʣϛΫϩӷణ಺Ͱͷߴ෼ࢠ༹ӷͷ૬෼཭ͱήϧԽʹΑΔ࠲۶‫ݱ‬৅༄ᖒ࣮ึɼ୙઒৻ฏɼࡔ্‫و‬༸ɼࢁԼ༞ଠ࿠ɼಖాণ೭
೔ຊ෺ཧֶձ 69 ճ೥࣍େձɼ౦ւେֶʢ2014 ೥ 3 ݄ 28 ೔ʣ֎෦ࢿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚ จ෦লՊֶ‫ڀݚ‬අิॿۚɺएख‫( ڀݚ‬B)
ଟࡉ๔Ϟσϧͷߏஙͱࡉ๔ؒ૬‫༻࡞ޓ‬ͷ੍‫ޚ‬‫ڀݚ‬୅දऀɿ༄ᖒ࣮ึ
จ෦লՊֶ‫ڀݚ‬අิॿۚɺ৽ֶज़ྖҬ‫ڀݚ‬ʢ‫ྖڀݚ‬ҬఏҊ‫ܕ‬ʣιϑτϚλʔ෺ཧʹΑΔඇରশϛΫϩήϧͷ૑੒ͱ੍‫ޚ‬‫ڀݚ‬୅දऀɿ༄ᖒ࣮ึ จ෦লՊֶ‫ڀݚ‬අิॿۚҎ֎ͷ֎෦ࢿۚ ҕ೚‫ܦ‬ཧۚɹχϓϩύον‫ࣜג‬ձࣾಖాণ೭ֶ෦̐೥ੜଔ‫ڀݚۀ‬ਗ਼ాᠳɿʢࢦಋ‫ڭ‬һɼಖాণ೭ʣTriton ਫ༹ӷͷಶ఺‫ۂ‬ઢͱ૬෼཭
౻Ҫརًɿʢࢦಋ‫ڭ‬һɼ༄ᖒ࣮ึʣ઀ணͨ͠ϛΫϩӷణ಺ʹ͓͚Δ૬෼཭υϝΠϯͷ഑
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159

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֎ࠃਓཹֶੜͷड͚ೖΕࢁԼ༟ଠ࿕ɿ
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160

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162ᖹᡂ㸰㸳ᖺᗘྛ✀ጤဨ㸦‫ࡣۑ‬ጤဨ㛗㸧㒊㛛㛗࣭Ꮫ⛉㛗࣭ᑓᨷ㛗㸸ᕝ㉺๪㒊㛛㛗㸸୰すᑗ᮶ィ⏬ጤဨ㸸‫ۑ‬ᕝ㉺㸪ᮌᮧ(ᗣ)㸪ᮌᮧ(ᓫ)㸪㔝࿅㸪ඵᑜ㸪୰すᩍ⫱ㄢ⛬ጤဨ㸸‫ۑ‬㬍⏣㸪ඵᑜ㸪ᕝ㉺㸪ⱝ⊃㸪ΎỈ㸪ᡂΎ㸪Ỉ㔝㸪ᆏୖ㸪ᒾୗධヨጤဨ఍ጤဨ㛗㸦඲࡚ࡢධヨ㛵㐃ጤဨ఍ࡢ⤫ᣓ㸧㸸ᮌᮧ(ᗣ)
ຓࡢ఍ᖿ஦㸸ᆏཱྀⓒᖺྐ㸸ඵᑜ㸪‫ۑ‬୰す㸪ඵᑜ㸪ᯇ஭♫఍㐃ᦠጤဨ㸸‫ۑ‬Ώ㒊࢟ࣕࣥࣃࢫ⛣㌿㸸ᮌᮧ(ᗣ)ዡᏛ㔠㈨᱁᳨ウጤဨ㸸‫ۑ‬ᶫᮏ㸪ᮌᮧ(ᓫ)㸪ྜྷ᳃⤒⌮ጤဨ㸸‫ۑ‬㔝࿅㸪ᮌᮧ(ᗣ)ᴗ⦼ホ౯㒊఍㸸‫ۑ‬ᶫᮏ㸪Ώ㒊ᑵ⫋࣭ᡂ⦼⟶⌮ᢸᙜ㸸‫ۑ‬࿴⏣㸪ᑎすᅗ᭩㸸‫ۑ‬ᡂΎ㸪ᑎす᝟ሗጤဨ఍㸸‫ۑ‬ᑎす㸪㔝ᮧ㸪ᮾᇛ㸪ᒣᒸᨭ⥺ LAN ⟶⌮⪅㸸ᑎすᗈሗጤဨ㸸‫⊃ⱝۑ‬㸪ྜྷᒸࠊᯇ஭
኱Ꮫ㝔ㄝ᫂఍㸸‫ۑ‬ග⏣㸪ዟᮧᖺḟሗ࿌ᢸᙜ㸸‫ۑ‬Ώ㒊㸪Ἑྜㄯヰ఍㸸Ώ㒊
ᩍဨ✚ࡳ❧࡚➼఍ィ㸸ྜྷ᳃ᩍဨචチ᭦᪂ㅮ⩦㸸‫ۑ‬Ώ㒊㸪ⱝ⊃య㦂ධᏛ࣭ධᏛ࢚࢜ࣜࣥࢸ࣮ࢩࣙࣥᐇ᪋ጤဨ㸸‫ྜྷۑ‬ᒸ㸪Ỉ㔝㸪⸨⏣㸪ᒣ⏣㸪Ⲩ஭

163

H25 ᖺᗘ ≀⌮Ꮫᩍᐊㄯヰ఍➨㸯ᅇᩍᐊㄯヰ఍㢟┠㸸ࠕᡃࠎࡣᏱᐂࢆ࡝ࡇࡲ࡛⌮ゎࡋࡓࡢ࠿ࠖ
ㅮᖌ㸸ᮡᒣ ┤ Ặ (ྡྂᒇ኱Ꮫ኱Ꮫ㝔⌮Ꮫ◊✲⛉ ᩍᤵ)᪥᫬㸸9 ᭶ 26 ᪥(ᮌ) 16:30㹼
ሙᡤ㸸≀⌮➨୍఍㆟ᐊ㸦⌮Ꮫ㒊㸰ྕ㤋㸯㝵㸰㸯㸳㸲㸧➨ 2 ᅇᩍᐊㄯヰ఍㢟┠㸸ࠕ࢞ࣛࢫ㌿⛣ືຊᏛ࡟ࡘ࠸࡚ࠖ
ㅮᖌ㸸ᑠ㈏ ᫂Ặ㸦ி㒔኱Ꮫྡ㄃ᩍᤵ㸪஑ᕞ኱Ꮫᐈဨᩍᤵ㸧᪥᫬㸸 10 ᭶ 2 ᪥㸦Ỉ㸧
㸪14 ᫬-15 ᫬ 30 ศሙᡤ㸸≀⌮➨୍఍㆟ᐊ㸦⌮Ꮫ㒊㸰ྕ㤋㸯㝵㸰㸯㸳㸲㸧➨㸱ᅇᩍᐊㄯヰ఍㢟┠㸸
ࠕ◁₍࡜⮬↛ᛶ̺ሙࡢ⌮ㄽࢆࡇ࠼࡚̺ࠖ
ㅮᖌ㸸ᕝྜ ග Ặ (ி㒔኱Ꮫ኱Ꮫ㝔⌮Ꮫ◊✲⛉࣭ᩍᤵ)᪥᫬㸸10 ᭶ 31 ᪥(ᮌ) 15:50㹼
ሙᡤ㸸≀⌮➨୍఍㆟ᐊ㸦⌮Ꮫ㒊㸰ྕ㤋㸯㝵㸰㸯㸳㸲ྕᐊ㸧➨ 4 ᅇ≀⌮Ꮫᩍᐊㄯヰ఍ㅮ⩏㢟┠㸸ࡺࡽࡂࡢᐃ⌮࠿ࡽᑟ࠿ࢀࡿ㠀ᖹ⾮ᐃᖖ⣔ࡢ⇕ຊᏛᵓ㐀ㅮᖌ㸸୰ᕝᑦᏊẶ㸦Ⲉᇛ኱Ꮫ⌮Ꮫ㒊≀⌮Ꮫ⛉㸧᪥᫬㸸11 ᭶ 6 ᪥㸦Ỉ㸧 16㸸00㹼17㸸00ሙᡤ㸸➨୍఍㆟ᐊ㸦2154 ᐊ㸧
➨ 5 ᅇᩍᐊㄯヰ఍ㅮ₇㢟┠㸸ᗘㄏ㉳౯ᩘ㌿⛣ࢆ♧ࡍ Eu ໬ྜ≀ࡢ㟁Ꮚ≧ែ㸸◳ X ⥺ග㟁Ꮚศග࡟ࡼࡿ◊✲ㅮ  ᖌ㸸 ୕ᮧ ຌḟ㑻 Ặ㸦኱㜰ᗓ❧኱ᏛᕤᏛ◊✲⛉࣭෸ᩍᤵ㸧᪥  ᫬㸸 㸯㸯 ᭶ 㸯㸱 ᪥ (Ỉ)  16㸸00㸫17㸸30ሙᡤ㸸 ➨ 1 ఍㆟ᐊ㸦2154 ᐊ㸧

➨ 6 ᅇ ≀⌮ᩍᐊㄯヰ఍
ㅮ₇㢟┠㸸 ࣑࣮࡛ࣗ࢜ࣥ᥈ࡿ⣲⢏Ꮚࡢ኱⤫୍⌮ㄽ

164ㅮ ᖌ 㸸 ᳃ ಇ๎(ᮾி኱Ꮫ⣲⢏Ꮚᅜ㝿◊✲ࢭࣥࢱ࣮࣭ᩍᤵ)᪥ ᫬ 㸸 2013 ᖺ 11 ᭶ 18 ᪥㸦᭶㸧16:30 ࡼࡾሙ ᡤ 㸸 ≀⌮➨㸯఍㆟ᐊ (⌮ 2 ྕ㤋 2154 ྕᐊ㸧➨ 7 ᅇ ≀⌮ᩍᐊㄯヰ఍
ㅮ₇㢟┠㸸 ๰Ⓨࡍࡿ࢚࢟ࢰࢳࢵࢡཎᏊ᰾ㅮ  ᖌ㸸 Ḉ஭ ༤൤Ặ㸦ᮾி኱Ꮫ኱Ꮫ㝔⌮Ꮫ◊✲⛉࣭ᩍᤵ㸭 ⌮໬Ꮫ◊✲ᡤ࣭୺௵◊✲ဨ㸧᪥  ᫬㸸 㸯㸰᭶㸱᪥㸦ⅆ㸧㸯㸴㸸㸱㸮ࡼࡾሙ  ᡤ㸸 ஑ᕞ኱Ꮫ⌮Ꮫ㒊≀⌮Ꮫ⛉ ➨㸯఍㆟ᐊ㸦㸰㸯㸳㸲ྕᐊ㸧➨㸶ᅇᩍᐊㄯヰ఍
ㅮ₇㢟┠㸸 ࣮ࣞࢨ࣮෭༷ཎᏊ࡛᥈ࡿ཯≀㉁ᾘኻࡢㅦ
ㅮ  ᖌ㸸 㓇ぢ Ὀᐶ Ặ㸦ᮾ໭኱Ꮫࢧ࢖ࢡࣟࢺ࣭ࣟࣥࣛࢪ࢜࢔࢖ࢯࢺ࣮ࣉࢭࣥࢱ࣮࣭ᩍᤵ㸧᪥  ᫬㸸 㸯㸰᭶㸯㸶᪥ (Ỉ)  16㸸30㸫18㸸00ሙᡤ㸸 ➨㸯఍㆟ᐊ㸦2154 ᐊ㸧

➨ 9 ᅇᩍᐊㄯヰ఍㸦᪥ᮏ≀⌮Ꮫ఍஑ᕞᨭ㒊≉ูㅮ₇఍㸧ㅮ₇㢟┠㸸 High-field magnetization of Tm2Fe17 single crystal
ㅮᖌ㸸 Dr. Alexander V. Andreev(Institute of Physics, Academy of Sciences, Prague, Czech Republic)᪥ ᫬㸸12 ᭶ 19 ᪥(ᮌ) 15㸸00㸫16㸸30ሙ ᡤ㸸஑ᕞ኱Ꮫ⌮Ꮫ㒊 2 ྕ㤋≀⌮Ꮫᩍᐊ➨୍఍㆟ᐊ㸦⚟ᒸᕷᮾ༊⟽ᓮ 6-10-1㸧஑ᕞ኱Ꮫ≀⌮ᩍᐊ➨ 10 ᅇ≀⌮ㄯヰ఍ࠕIsing ᆺ┦஫స⏝ࢆࡍࡿ⣔ࡢ㔞Ꮚࡺࡽࡂࠖㅮᖌ㸸 ༡ ࿴ᙪ෸ᩍᤵ(ྡྂᒇ኱Ꮫ኱Ꮫ㝔ከඖᩘ⌮⛉Ꮫ◊✲⛉)᪥᫬㸸12 ᭶ 26 ᪥(ᮌ) 16:00㹼17:00
ሙᡤ㸸≀⌮Ꮫ⛉➨㸯఍㆟ᐊ(2154 ᐊ)

165

H25 ᖺᗘ ≀⌮ᏛᩍᐊỈ᭙ᮌ᭙ㄯヰ఍

㹆25 ᖺᗘ➨ 1 ᅇ≀⌮Ꮫᩍᐊ Ỉ᭙ㄯヰ఍ㅮ₇㢟┠ᕼᅵ㢮㔠ᒓ໬ྜ≀࡟࠾ࡅࡿ౯ᩘ୙Ᏻᐃୗࡢ☢ᛶ◊✲ㅮ ᖌ 㸸ග⏣ ᬡᘯ᪥᫬㸸2013 ᖺ 5 ᭶ 1 ᪥㸦Ỉ㸧16㸸30 - 17㸸50ሙᡤ㸸≀⌮➨ 2 ㅮ⩏ᐊ㹆25 ᖺᗘ➨ 2 ᅇ≀⌮Ꮫᩍᐊ Ỉ᭙ㄯヰ఍ㅮ₇㢟┠ࣖࢾࢫ⢏Ꮚࡢ⮬ᕫ⤌⧊໬ㅮ ᖌ 㸸 ᒾୗ 㟹Ꮥ᪥᫬㸸2014 ᖺ᭶ 9 ᪥㸦Ỉ㸧ሙᡤ㸸≀⌮➨ 2 ㅮ⩏ᐊ㹆25 ᖺᗘ➨㸱ᅇ≀⌮Ꮫᩍᐊ Ỉ᭙ㄯヰ఍ㅮ₇㢟┠㉸ᑐ⛠⌮ㄽࡢᑠࡉ࡞㝵ᒙᛶၥ㢟࡜      ㉸ᑐ⛠ᛶࡢ◚ࢀࡢ࣑࣮ࣛࢪࣗ፹௓ᶵᵓ
ㅮ ᖌ 㸸 ዟᮧ ೺୍᪥᫬㸸2013 ᖺ㸴᭶ 26 ᪥㸦Ỉ㸧17㸸00 - 18㸸20ሙᡤ㸸≀⌮➨ 2 ㅮ⩏ᐊ㹆25 ᖺᗘ➨㸲ᅇ≀⌮Ꮫᩍᐊ Ỉ᭙ㄯヰ఍ㅮ₇㢟┠㹐㹇ࣅ࣮࣒࡟ࡼࡿ୙Ᏻᐃ᰾ࡢඹ㬆≧ែࡢ◊✲ㅮ ᖌ 㸸 ᑎす 㧗᪥᫬㸸2013 ᖺ 7 ᭶ 24 ᪥㸦Ỉ㸧17㸸00 - 18㸸20ሙᡤ㸸≀⌮➨ 2 ㅮ⩏ᐊᖹᡂ 25 ᖺᗘ➨ 1 ᅇ≀⌮Ꮫᩍᐊ ᮌ᭙ㄯヰ఍
ㅮ₇㢟┠

ࡓ࠿ࡀ Hubbard ࣔࢹࣝ ࡉࢀ࡝ Hubbard ࣔࢹࣝㅮ ᖌ 㸸 ᡂΎ ಟ᪥᫬㸸2013 ᖺ 10 ᭶ 31 ᪥㸦ᮌ㸧17㸸00 - 18㸸20ሙᡤ㸸≀⌮➨୍ㅮ⩏ᐊ

166

ᖹᡂ 25 ᖺᗘ➨ 2 ᅇ≀⌮Ꮫᩍᐊ ᮌ᭙ㄯヰ఍
ㅮ₇㢟┠ࡂࡾࡂࡾᅛయㅮ ᖌ 㸸ᯇ஭῟᪥᫬㸸2013 ᖺ 11 ᭶ 28 ᪥㸦ᮌ㸧16㸸30 - 17㸸50ሙᡤ㸸≀⌮➨୍ㅮ⩏ᐊ
ᖹᡂ 25 ᖺᗘ➨ 3 ᅇ≀⌮Ꮫᩍᐊ ᮌ᭙ㄯヰ఍
ㅮ₇㢟┠ࢫࣆࣥ⣔ࡢ magnetism ࡜ chromism ࡢ┦㛵ㅮ ᖌ 㸸 ὸ㔝 ㈗⾜᪥᫬㸸2013 ᖺ 12 ᭶ 19 ᪥㸦ᮌ㸧17㸸00 - 18㸸20
ሙᡤ㸸≀⌮➨୍ㅮ⩏ᐊ

167

2013 ᖺᗘ ≀ᛶᇶ♏ㄽࢥ࣒ࣟ࢟࢘㛤ദ୍ぴ➨୍ᅇ (2013 ᖺ 4 ᭶ 23 ᪥)㔝ᮧ Ύⱥ (⤫ィ≀⌮)ࠕ࣮ࣞࢨ࣮෭༷ࡢ≀⌮ 2ࠖ➨஧ᅇ (2013 ᖺ 5 ᭶ 9 ᪥)ᒣཱྀ ဴ⏕ (஑ᕞ኱Ꮫ኱Ꮫ㝔ᕤᏛ◊✲㝔ᶵᲔᕤᏛ㒊㛛)  ࠕ㧗ศᏊࢤࣝࡢࡍ࡭ࡾᦶ᧿ࠖ
➨୕ᅇ (2013 ᖺ 5 ᭶ 21 ᪥)タᴦ ᜤᖹ (⤫ィ≀⌮)  ࠕ཯ᛂᣑᩓ⣔࡟࠾ࡅࡿᒁᅾࣃࢱ࣮ࣥࡢࢲ࢖ࢼ࣑ࢡࢫࠖ
➨ᅄᅇ (2013 ᖺ 5 ᭶ 28 ᪥)す᳃ ᣅ (ᗈᓥ኱Ꮫ࣭⌮࣭ᩘ⌮ศᏊ⏕࿨⌮Ꮫᑓᨷ)
ࠕ࢔ࣜࡢ᥇㣵⾜ື࡟࠾ࡅࡿỴ᩿࡜ࡺࡽࡂࠖ
➨஬ᅇ (2013 ᖺ 6 ᭶ 11 ᪥)ᡂΎ ಟ (จ⦰⣔⌮ㄽ)
ࠕ࢖ࣥࣇ࣮ࣞࢩࣙࣥᏱᐂࡢ࢚ࣥࢺࣟࣆ࣮ࠖ
➨භᅇ (2013 ᖺ 6 ᭶ 25 ᪥)ྜྷ᳃ ᫂ (≀ᛶ⌮ㄽ)ࠕࢥࣟ࢖ࢻศᩓ⣔ࡢ⢒ど໬ࠖ➨୐ᅇ (2013 ᖺ 7 ᭶ 16 ᪥)ᯇ஭ ῟ (≀ᛶ⌮ㄽ)
ࠕࢥ࣮ࢩ࣮ศᕸࠖ

➨ඵᅇ (2013 ᖺ 10 ᭶ 10 ᪥)ᆏୖ ㈗ὒ (⤫ィ≀⌮)ࠕ␗ᖖ࡞ᣑᩓ࡟ࡘ࠸࡚ࡢヰ㢟ࠖ➨஑ᅇ (2013 ᖺ 11 ᭶ 6 ᪥)  (ව㸸➨ 4 ᅇᩍᐊㄯヰ఍㸧

168



୰ᕝ ᑦᏊ㸦Ⲉᇛ኱Ꮫ⌮Ꮫ㒊≀⌮㸧ࠕࡺࡽࡂࡢᐃ⌮࠿ࡽᑟ࠿ࢀࡿ㠀ᖹ⾮ᐃᖖ⣔ࡢ⇕ຊᏛᵓ㐀ࠖ➨༑ᅇ (2013 ᖺ 11 ᭶ 21 ᪥)
୰ᮧ ᭷ⰼ 㸦≀ᛶ⌮ㄽ㸧  ࠕ኱ࡁ࡞⢏Ꮚࡢᣑᩓ࡜ Stokes-Einstein ๎ࠖ➨༑୍ᅇ (2013 ᖺ 12 ᭶ 12 ᪥)  㸦ව㸸EEP ࢭ࣑ࢼ࣮㸧
Walter Reisner 㸦Department of Physics, McGill University㸧 "Conformational Sculpting of DNA in Nanoconfinement"➨༑஧ᅇ (2014 ᖺ 1 ᭶ 9 ᪥) 
Cecilia Lovkvist 㸦Niels Bohr Institute㸧"Improved contact prediction in proteins:
Using pseudolikelihoods to infer Potts models "➨༑୕ᅇ (2014 ᖺ 1 ᭶ 23 ᪥) ཎㄹᖹ 㸦≀ᛶ⌮ㄽ㸧ࠕKomatsu-Nakagawa representation ࡢ⤂௓ࠖ➨༑ᅄᅇ (2014 ᖺ 2 ᭶ 6 ᪥) 㔝ཱྀៅᖹ 㸦≀ᛶ⌮ㄽ㸧ࠕProductivity dispersion: Facts, Theory, and Implications 㸦ㄽᩥ⤂௓㸧ࠖ➨༑஬ᅇ (2014 ᖺ 2 ᭶ 20 ᪥) 㸦」㞧≀ᛶ࡜ྜྠ㛤ദ㸧
Gijs Wuite 㸦VU University Amsterdam 㸧"Measuring the physics that drives DNA-protein interactions "➨༑භᅇ (2014 ᖺ 2 ᭶ 27 ᪥) ㏆⸨ ὒ୍㑻 㸦⤫ィ≀⌮㸧
ࠕSustainable Energyࠖ

169ฏ੒ 25 ೥౓‫۝‬େ‫֩ࢠݪ‬ηϛφʔ։࠵Ұཡ
ୈ 908 ճ 2013 ೥ 4 ݄ 12 ೔ʢۚʣߨࢣɿീਘ ਖ਼৴ ࢯ (‫۝‬भେֶ)ԋ୊ɿ֩෺ཧֶΛల๬͢Δ
ୈ 909 ճ 2013 ೥ 5 ݄ 24 ೔ʢۚʣߨࢣɿॹํ Ұհ ࢯ (େࡕେֶ RCNP)ԋ୊ɿ୸ૉ 22 ͷඇଋറྭ‫ى‬ঢ়ଶͷଘࡏ‫ܗ‬ଶ
ୈ 910 ճ 2013 ೥ 5 ݄ 31 ೔ʢۚʣߨࢣɿ૬ྑ ‫۝( ࢯ ࢸݐ‬भେֶɾ‫ڞ‬ಉ‫ڀݚ‬һ)ԋ୊ɿ3 ֩ࢠ‫ͱݧ࣮ܥ‬ະղ໌ͷ‫ݱ‬৅ୈ 911 ճ 2013 ೥ 7 ݄ 12 ೔ʢۚʣߨࢣɿদ࡚ ߒ೭ ࢯ (౦‫ژ‬େֶେֶӃ ޻ֶ‫ڀݚܥ‬Պ ‫ࡍࠃྗࢠݪ‬ઐ߈)ԋ୊ɿ129I-AMS Λར༻ͨ͠஍‫ڥ؀ٿ‬Պֶͷ‫ڀݚ‬ʢࣗવγεςϜͱਓҝ‫ݯى‬γεςϜʣୈ 912 ճ 2013 ೥ 7 ݄ 12 ೔ʢۚʣߨࢣɿࡾ୐ ହే ࢯ (౦‫ژ‬େֶେֶӃ ޻ֶ‫ڀݚܥ‬Պ ‫ࡍࠃྗࢠݪ‬ઐ߈)ԋ୊ɿ෱ౡୈҰ‫ݯىނࣄॴిൃྗࢠݪ‬ͷ์ࣹੑϤ΢ૉಉҐମൺͷਪఆ
ୈ 913 ճ 2013 ೥ 7 ݄ 17 ೔ʢਫʣߨࢣɿླ໦ ‫ݡ‬ೋ ࢯ (‫۝‬भ޻‫ۀ‬େֶ γχΞɾΞΧσϛʔ)ԋ୊ɿ༗ޮ૬‫༻࡞ޓ‬ཧ࿦ͷྺ࢙ͱల๬
ୈ 914 ճ 2013 ೥ 10 ݄ 23 ೔ʢਫʣߨࢣɿਫࢁ Ұਔࢯ (େࡕେֶ RCNP)ԋ୊ɿ࿈ଓঢ়ଶཻࢠৼಈ݁߹๏ʹ‫ߏ֩ͮ͘ج‬଄ɾ֩൓Ԡͷ౷Ұత‫ه‬ड़
ୈ 915 ճ 2014 ೥ 1 ݄ 29 ೔ʢਫʣߨࢣɿI-O. Stamatescu ࢯ (Heidelberg)ԋ୊ɿApproaching ﬁnite density QCD using Complex Langevin Simulation
ୈ 916 ճ 2014 ೥ 3 ݄ 3 ೔ʢਫʣߨࢣɿؔᖒ Ұ೭ ࢯ (ஜ೾େֶ)ԋ୊ɿTDHF ‫ʹࢉܭ‬ΑΔଟ֩ࢠҠߦ൓Ԡͷ‫ڀݚ‬170

ୈ 917 ճ 2014 ೥ 3 ݄ 14 ೔ʢۚʣߨࢣɿദ ߒ࢘ ࢯ (ཧ‫ ݚ‬BNL)ԋ୊ɿEﬀective model approach to phase structures of QCD and QCD-like theory171         ᖹᡂ  ᖺᗘ㠀ᖖ໅ㅮᖌ୍ぴ
Ꮫ㒊ᢸᙜ
ㅮᖌ

ᡤᒓ

㢟┠

ධబṇᖾ ஑ᕞᕤᴗ኱Ꮫ᝟ሗᕤᏛ㒊⏕≀≀⌮Ꮫ

኱Ꮫ㝔ᢸᙜ
ㅮᖌ

ᡤᒓ

㢟┠

༡࿴ᙪ

ྡྂᒇ኱Ꮫ኱Ꮫ㝔ከඖᩘ⌮⛉Ꮫ◊✲⛉㻌ྍゎ᱁Ꮚᶍᆺ࡜㸯ḟඖ☜⋡㐣⛬㓇ぢὈᐶᮾ໭኱Ꮫࢧ࢖ࢡࣟࢺ࣭ࣟࣥࣛࢪ࢜࢔࢖ࢯ ࣮ࣞࢨ࣮෭༷ཎᏊ࡟ࡼࡿᇶᮏᑐ

᳃ಇ๎ࢺ࣮ࣉࢭࣥࢱ࣮

⛠ᛶࡢ≀⌮

ᮾி኱Ꮫ⣲⢏Ꮚ≀⌮ᅜ㝿◊✲䝉䞁䝍䞊㻌ᶆ‽⌮ㄽࢆ㉸࠼ࡿ᪂ࡋ࠸⣲⢏Ꮚ≀⌮⌧㇟ࡢ᥈ồᮡᒣ┤ྡྂᒇ኱Ꮫ኱Ꮫ㝔⌮Ꮫ◊✲⛉

ほ

୕ᮧຌḟ

኱㜰ᗓ❧኱Ꮫ኱Ꮫ㝔ᕤᏛ◊✲⛉㻌ග㟁Ꮚศගἲ࡟ࡼࡾほ

㑻
ᕝྜග

ⓗᏱᐂㄽ
ࡉࢀࡿ

ᙉ┦㛵≀㉁ࡢ㟁Ꮚ≧ែி㒔኱Ꮫ኱Ꮫ㝔⌮Ꮫ◊✲⛉ᘻ⌮ㄽࡢᒎᮃ࣮㠀ᦤືⓗᐃᘧ໬ࢆ୰ᚰ࡜ࡋ

Ḉ஭༤൤ᮾி኱Ꮫ኱Ꮫ㝔⌮Ꮫ⣔◊✲⛉⌮໬Ꮫ◊5, ࣅ࣮࣒࡛ᣅࡃ୙Ᏻᐃ᰾≀⌮✲ᡤோ⛉ຍ㏿ჾ◊✲ࢭࣥࢱ࣮
୰ᕝᑦᏊ㠀ᖹ⾮⣔ࡢ⤫ィຊᏛⲈᇛ኱Ꮫ⌮Ꮫ㒊㻌

172

  ᖹᡂ㸰㸳ᖺᗘእᅜே◊✲⪅➼ཷධグ㘓ᡤᒓ࣭⫋࣭Ặྡᅜ⡠ ⌮Ꮫ◊✲㝔䞉እᅜே≉ ࣂࣥࢢࣛࢹ
ู◊✲ဨ㻌

࢕ࢩࣗ

ཷධࡢ┠ⓗ

ཷධᮇ㛫

ཷධ⪅

᪥ ᮏᏛ⾡ ᣺⯆఍ 䞉እ ᅜ 㸰㸲ᖺ㸯㸮ᮌᮧ㻔ᓫ㻕

ே≉ู◊✲ဨ㻌

᭶㸯᪥ࠥ
㸰㸴ᖺ㸷᭶

㻮㻭㻷㻭㼁㻸㻘㻌㻿㻚㻾㻚㻌㸱㸮᪥ ᭶  ᪥ࠥ ┦Ⰻ䝘䝫䝸➨ 㻞 ኱Ꮫ䞉‽ᩍᤵ㻌 ࢖ࢱࣜ࢔

ኳయ᰾཯ᛂᐇ㦂⿦㻸㼡㼏㼕㼛㻌㻳㼕㼍㼘㼍㼚㼑㼘㼘㼍㻌⨨࣭ᡭἲ࡟㛵ࡍࡿ㆟ㄽ  ᭶  ᪥࠾ࡼࡧࢭ࣑ࢼ࣮ࢻ ࢖ ࢶࢩ ࣥࢡ ࣟࢺ ࣟ ࢻ࢖ࢶ◊✲ᡴࡕྜࢃࡏ࣭ࢭ࣑ 㸯㸯᭶㸳᪥ࣥ◊✲ᡤ '(6< ࣭୺௵

ࢼ࣮ㅮ₇

ᕝ㉺

ࠥ
㸯㸯᭶㸴᪥

◊✲ဨ)HOL[6HINRZ㻵㼚㼟㼠㼕㼠㼡㼠㼑㻌 㼛㼒㻌 㻼㼔㼥㼟㼕㼏㼟 䠈ࢳ࢙ࢥ㻭㼏㼍㼐㼑㼙㼥㻌 㼛㼒㻌 㻿㼏㼕㼑㼚㼏㼑㼟 䞉☢ᛶ࡟㛵ࡍࡿඹྠ◊

㸯㸰᭶㸯㸰

✲

᪥ࠥ

㻼㼞㼛㼒㼑㼟㼟㼛㼞㻌㸯㸰᭶㸰㸮㻭㼘㼑㼤㼍㼚㼐㼑㼞㻌㼂㻚㻌㻭㼚㼐㼞㼑㼑㼢㻌᪥㼂㼞㼕㼖㼑 ኱Ꮫᩍᤵ㻌

࢜ࣛࣥࢲ

ඹྠ◊✲

㸰᭶㸯㸳᪥

࿴⏣

Ỉ㔝

ࠥ

㻳㼕㼖㼟㻌㼃㼡㼕㼠㼑㻌㸱᭶㸯㸳᪥
㻵㻼㻮㻿㻛㻯㻺㻾㻌 ༤ኈ㻌

ࣇࣛࣥࢫ

ඹྠ◊✲

㸱᭶㸵᪥ࠥ Ỉ㔝㸱᭶㸰㸷᪥

㻯㼍㼠㼔㼑㼞㼕㼚㼑㻌㼀㼍㼞㼐㼕㼚㻌䝃䞁䜹䝹䝻䝇኱Ꮫ㻌 ᩍᤵ㻌 ࣇ࢕ࣜࣆࣥ

ඹྠ◊✲

㸱᭶㸯㸴᪥

Ỉ㔝㻌

㹼

㻾㼛㼙㼙㼑㼘㻌㻮㼍㼏㼍㼎㼍㼏㻌㸱᭶㸰㸳᪥
㻴㼑㼕㼐㼑㼘㼎㼑㼞㼓 ኱Ꮫᩍᤵ㻌

ࢻ࢖ࢶ

ࢭ࣑ࢼ࣮

㸯᭶㸰㸷᪥
㹼

㻵㻙㻻㻚㻌㻿㼠㼍㼙㼍㼠㼑㼟㼏㼡㻌㸯᭶㸱㸯᪥




173

ඵᑜ㻌

㸰㸳ᖺᗘ ᩍ⫱ㄢ⛬ጤဨ఍άືሗ࿌
ጤဨ㛗㸸㬍⏣ᩍᤵጤဨඵᑜᩍᤵ㸪ΎỈ෸ᩍᤵ㸪ᡂΎ෸ᩍᤵ㸪ⱝ⊃෸ᩍᤵ㸪Ỉ㔝෸ᩍᤵ㸪ᒾୗຓᩍ㸪ᆏୖຓᩍ
ᚑ᮶ࡢࠕඹ㏻ᩍ⫱ࠖࡀ㸪ᖹᡂ  ᖺᗘ࡟ࠕᇶᖿᩍ⫱ࠖ࡟⛣⾜࣭ᐇ᪋ࡉࢀࡿࡇ࡜࡟
క࠸ᐇົࡀከ࠿ࡗࡓ㸬㸯ࠊ኱Ꮫ㝔ᩍ⫱ㅮ⩏ᐇ᪋⛉┠ࡢぢ࡞࠾ࡋࢆ⾜࠸㸪ᐇ᪋⛉┠ࢆᩚ⌮ࡋࡓࠋᇶ♏⛉┠ࡢぢ࡞࠾ࡋࢆ⾜࠸㸪⌧⾜  ⛉┠ࢆ  ⛉┠࡟ࡋࡓࠋ
࣒࣐࢝ࣜ࢟ࣗࣛࢵࣉࢆసᡂࡋࡓࠋ
㸰ࠊᏛ㒊ᩍ⫱ᇶᖿᩍ⫱ࡢᐇ᪋࡟క࠸㸪Ꮫ㒊  ᖺḟ௨㝆ࡢᑓᨷᩍ⫱ࢆᨵṇࡋࡓࠋᚲಟ⛉┠ࡢぢ࡞࠾ࡋࠋ᪂つ⛉┠ࡢ㛤ㅮࠋ᫬㛫๭ࡢኚ᭦ࠋ
ᇶᖿᩍ⫱ࢆྵࡴ࣒࣐࢝ࣜ࢟ࣗࣛࢵࣉࡢసᡂ㸦 ᖺᗘࡲ࡛⥅⥆㸧ࠋ㸱ࠊ⌮Ꮫ㒊࣒࢝ࣜ࢟ࣗࣛ :*ᇶᖿᩍ⫱࡜⌮Ꮫ㒊ᑓᨷᩍ⫱⛉┠࡜ࡢㄪᩚࠋ㸲ࠊ ᖺḟᐇ᪋ࡢᐇ㦂⛉┠ࡢ෌⦅ఀ㒔࡛ࡢᐇ᪋ࢆ┠ᣦࡋࡓᐇ㦂ෆᐜࡢ᳨ウࢆ⾜ࡗࡓࠋ㸳ࠊ㒊㛛 )' ࡢᐇ᪋኱Ꮫ㝔ᩍ⫱࡟ࡘ࠸࡚ࠋ
㸴ࠊ≉◊㓄ᒓࡢ᪉ἲ
≉◊㓄ᒓࡢ᪉ἲࢆぢ࡞࠾ࡋࡓࠋ
㸵ࠊᇶᖿᩍ⫱࡟ࡘ࠸࡚
ᇶᖿᩍ⫱ᒚಟせ㡯ࡢసᡂࠋ
㐍⣭᮲௳ࡢ⟇ᐃࠋ㸶ࠊ᝟ሗ⌮Ꮫศᒓ࡟ࡘ࠸࡚
᝟ሗ⌮Ꮫ⛉࡜ࡢ༠㆟ࢆ⾜࠸㸪ศᒓ᫬ᮇࡢぢ࡞࠾ࡋ㸪ኚ᭦ࡋࡓࠋ

174ᖹᡂ㸰㸳ᖺᗘ ≀⌮Ꮫ㒊㛛ࣇ࢓࢝ࣝࢸ࢕࣭ࢹ࢕࣋ࣟࢵࣉ࣓ࣥࢺሗ࿌

ࠕ኱Ꮫ㝔ᩍ⫱ࡢ࠶ࡾ᪉࡟ࡘ࠸࡚ࠖ
㛤ദ᪥᫬㸸  ᖺ  ᭶  ᪥ 㔠    㹼  ᫬㛫⛬ᗘ㛤ദሙᡤ㸸 ≀⌮Ꮫ⛉➨୍ㅮ⩏ᐊ  㸦 ྕᐊ㸧 ≀⌮Ꮫ㒊㛛࡛ࡣࠊ኱Ꮫ㝔⌮Ꮫ◊✲㝔࣭኱Ꮫ㝔⌮Ꮫᗓ࣭⌮Ꮫ㒊ࡢ୰ᮇ┠ᶆ࣭୰ᮇィ⏬ࢆ㍈࡟ࣇ࢓࢝ࣝࢸ࢕࣭ࢹ࢕࣋ࣟࢵࣉ࣓ࣥࢺࢆ⾜ࡗ࡚࠸ࡿࠋ ᮏᖺᗘࡣࠊ
ࠕ኱Ꮫ㝔ᩍ⫱ࡢ࠶ࡾ᪉࡟ࡘ࠸࡚ࠖࢆࢸ࣮࣐࡟ࣇ࢓࢝ࣝࢸ࢕ࢹ࢕࣋ࣟ
ࣉ࣓ࣥࢺࢆ⾜ࡗࡓࠋ඲ᩍဨࢆᑐ㇟࡜ࡋࡓ㛤ദ᪥࡟࠾ࡅࡿ㆟ㄽ࡟ඛ❧ࡕࠊᮏ㒊㛛ฟ㌟࡛⌧ᅾࡣࢥ࣌ࣥࣁ࣮ࢤࣥ኱Ꮫࢽ࣮ࣝࢫ࣮࣎࢔◊✲ᡤࡢᚚᡭὙ⳯⨾Ꮚ෸ᩍᤵࡀ᮶᪥ࡉࢀࠊࠕ*UDGXDWHVFKRROHGXFDWLRQLQ'HQPDUN LQFRPSDULVRQZLWKWKH
-DSDQHVHV\VWHPࠖࡢ㢟┠࡛ㅮ₇ࢆ⾜ࡗ࡚࠸ࡓࡔ࠸ࡓࠋࢹ࣐࣮ࣥࢡ࡟࠾ࡅࡿ≀⌮ศ㔝ࡢ኱Ꮫ㝔ᩍ⫱ࡢヲ⣽࡟ࡘ࠸࡚⤂௓ࡋ࡚࠸ࡓࡔࡃࡇ࡜࡛ࠊᮏᏛ࡟࠾ࡅࡿᩍ⫱ࡢ࠶ࡾ᪉࡟ࡘ࠸࡚㆟ㄽࡍࡿࡓࡵࡢཧ⪃࡟࡞ࡗࡓࠋ  ᖺ  ᭶  ᪥ 㔠    㹼 㛤ദࡉࢀࡓࣇ࢓࢝ࣝࢸ࢕ࢹ࢕࣋ࣟࢵࣉ
࣓ࣥࢺ࡟࠾࠸࡚ࡣࠊࡲࡎࠊඵᑜᩍᤵࡀ᪂ࡓ࡟సᡂࡉࢀࡓࠕ኱Ꮫ㝔ᩍ⫱ࡢ┠ⓗ࡜฿㐩┠ᶆ࡟ࡘ࠸࡚ࠖ
㸦ཎ᱌㸧࡟ࡘ࠸࡚ㄝ࣭᫂⤂௓ࡉࢀࠊᩍဨࡢព㆑ࡢ⤫୍ࡀᅗࡽࢀࡿ࡜࡜ࡶ࡟ࠊཎ᱌࠿ࡽࡢⱝᖸࡢಟṇࡀ㆟ㄽࡉࢀࡓࠋࡑࡢᚋࠊΎỈ෸ᩍᤵࡀࠊ
᮶ᖺᗘ࠿ࡽᐇ᪋ࡉࢀࡿ኱Ꮫ㝔࣒࢝ࣜ࢟ࣗࣛࡢኚ᭦࡟㛵ࡋࠊࡑࡢ┠ⓗࡸ⤒⦋ࢆຓᩍࢆྵࡵࡓ඲యࡢሙ࡛ㄝ᫂ࡉࢀࡓࠋࡲࡓࠊ⌧ᅾసᡂ୰ࡢ኱Ꮫ㝔ࡢᒚಟ࣐ࢵࣉ࡟
ࡘ࠸࡚ࡶ⤂௓ࡉࢀࠊ㆟ㄽࡀ⾜ࢃࢀࡓࠋࡑࡢᚋࠊ୰すᩍᤵ࣭㬍⏣ᩍᤵࡀࠊ኱Ꮫ㝔ᩍ⫱ࢆᨵၿࡍࡿࡓࡵࡢࣔࢹࣝࢣ࣮ࢫࡸලయⓗ࡞ฎ᪉⟢࡟ࡘ࠸࡚ㅮ₇ࢆ⾜ࡗ࡚࠸ࡓࡔࡁࠊ᭱ᚋ࡟ࣇ࣮ࣜࢹ࢕ࢫ࢝ࢵࢩࣙࣥࢆ⾜ࡗࡓࠋ኱Ꮫ㝔ᩍ⫱ࡢᅾࡾ᪉࡟㛵ࡋ࡚ࡣࠊࡑࡢ௚࡟ࡶ㸯㸧኱Ꮫ㝔ㅮ⩏࡜኱Ꮫ㝔⏕ࡢ㛗ᮇ࡟ࢃࡓࡿฟᙇᐇ㦂ࠊ㸰㸧ᑵ⫋άື࡜኱Ꮫ㝔ᩍ⫱ 㸱㸧ಟኈ࣭༤ኈㄢ⛬Ꮫ⏕ࡢᐃဨ඘㊊⋡ࡢၥ㢟࡜ᨵၿ᪉ἲ
࡟ࡘ࠸࡚ 㸲㸧እᅜேᩍဨࡢᚲせᛶ ➼ࠎࠊᵝࠎ࡞ၥ㢟ࡀᥦ㉳ࡉࢀ࡚࠾ࡾࠊⰋ
࠸ࣈࣞ࢖ࣥࢫࢺ࣮࣑ࣥࢢࡢᶵ఍࡜ࡶ࡞ࡗࡓࠋୖグ࡟㛵ࡍࡿሗ࿌᭩㸦ㅮ₇ࡢࢫࣛ࢖ࢻヨᩱࠊ㆟஦ࡢ඲グ㘓ࡀ㞟㘓ࡉࢀ࡚࠸ࡿ㸧ࢆసᡂࡋࠊ㆟ㄽࡢヲ⣽ࢆࡑࡇ࡟グࡋࡓࠋ

175ᖹᡂ 25 ᖺᗘ ධᏛ⪅ᩘ࡜༞ᴗ⪅ᩘ≀⌮Ꮫ⛉≀⌮Ꮫ⛉㸱ᖺḟ⦅ධಟኈㄢ⛬㸦≀⌮Ꮫᑓᨷ㸧༤ኈㄢ⛬㸦≀⌮Ꮫᑓᨷ㸧

176

ධᏛ⪅ᩘ

༞ᴗ⪅ᩘ

㸴㸴

㸳㸴

㸱

㸫

㸲㸯

㸲㸱

㸶

༤ኈᏛ఩ྲྀᚓ⪅㸲

2013 ᖺᗘࡢᑵ⫋࣭㐍Ꮫ≧ἣ௒ᖺᗘࡣಟኈ࡜Ꮫ㒊Ꮫ⏕࡛ᑐ↷ⓗ࡞≧ἣ࡟࡞ࡗࡓ㸬௒ᖺࡢಟኈࡣ౛ᖺࡼࡾᩘࡀከࡃ㸪௻ᴗᑵ⫋⪅ᩘࡶ༤ኈᚋᮇㄢ⛬㐍Ꮫ⪅ᩘࡶ᫖ᖺࡼࡾቑຍࡋࡓ㸬ᬒẼࡀᑡࡋୖྥ࠸࡚ࡁࡓࡓࡵ࠿㸪ᑵ⫋࡛ࡁ࡞࠸࡜࠸࠺⌮⏤࡛␃ᖺࡋࡓಟኈࡣ࡯࡜ࢇ࡝࠸࡞࠿ࡗࡓ㸬≀⌮ᏛᑓᨷࡢᏛ⏕ࡢᑵ⫋ࡣ⮬⏤ᛂເ࡜ࣜࢡ࣮ࣝࢱ࣮ࢆ㏻ࡋ࡚ࡢᑵ⫋άືࡀ኱༙࡛࠶ࡿ㸬௒ᖺᗘࡶ 2 ᭶㹼3 ᭶࡟࠿ࡅ࡚
OB ࡢࣜࢡ࣮ࣝࢱ࣮࡟ࡼࡿ≀⌮Ꮫ⛉⏕ྥࡅࡢ఍♫ㄝ᫂఍ࢆ 10 ᅇ࡯࡝㛤ദࡋ࡚࠾ࡾ㸪ࡑࡢຠᯝࡣ኱ࡁ࠸ࡼ࠺࡛࠶ࡿ㸬୍᪉㸪Ꮫ㒊࡛ࡣ␃ᖺࡋࡓᏛ⏕ࡀ㏆ᖺ࡟࡞ࡃከ࠿ࡗࡓ㸬ࡇࡢࡓࡵಟ
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ཎᏊຊ㛤Ⓨᶵᵓ࡟ࡶ 1 ྡ᥇⏝ࡉࢀ࡚࠸ࡿ㸬༤ኈㄢ⛬㐍Ꮫ㸦ྵ ௚኱Ꮫ㸧

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༤ኈࡢ㐍㊰࣭ᑵ⫋༤ኈㄢ⛬ࢆಟ஢ࡋࡓே࡛ࡣ 1 ྡࡀᏛ᣺ࡢ࣏ࢫࢻࢡ㸪2 ྡࡀ኱Ꮫࡢ༤ኈ◊✲ဨ࡟᥇⏝ࡉࢀ࡚࠸ࡿ㸬Ꮫ㒊⏕ࡢ㐍㊰࣭ᑵ⫋ಟኈ㐍Ꮫࡣ 36 ྡ㸦஑኱≀⌮ 30 ྡ ௚኱Ꮫ࣭௚Ꮫᗓ 6 ྡ㸧㸪Ẹ㛫௻ᴗ࡟ᑵ⫋ 2 ྡ㸪ᩍဨ 1ྡ㸪␃ᖺ࡜ᮍᐃࡀ 12 ྡ㸪㏥Ꮫ࣭ࡑࡢ௚ࡀ 1 ྡ࡛࠶ࡗࡓ㸬177ମ‫ݧ‬ೖֶɾެ։ߨ࠲ใࠂ
୲౰ɿ٢Ԭਸ਼थ

ฏ੒ 26 ೥ 3 ݄ 23 ೔ (೔)ʙ24(݄) ͷ 2 ೔ؒʹΘͨͬͯɺʮୈ 17 ճମ‫ݧ‬෺ཧֶʯΛ࣮ࢪͨ͠ɻྫ೥ɺय़‫ٳ‬Έͷ‫ ߍߴʹؒظ‬1ɾ2 ೥ੜΛର৅ͱͯ͠ 3 ೔࣮ؒࢪ͖͕ͯͨ͠ɺΞϯέʔτͰ
3 ೔௨͏ͷ͸େมͰ͋Δͱͷҙ‫͕ݟ‬ଟ͘‫ͤد‬ΒΕͨ͜ͱ͔Βɺ5 ೥લ͔Β‫ظ‬೔Λ 2 ೔ؒʹ୹ॖ࣮ͯ͠ࢪ͍ͯ͠Δɻ·ͨɺηϛφʔ෦෼Λެ։ߨ࠲ͱͯ͠Ұൠ޲͚ʹ޿͘ղ์͠ɺେֶ΁ͷ
3 ೥࣍ฤೖΛߟ͍͑ͯΔߴ౳ઐ໳ֶߍੜ΁ͷઆ໌ձΛ݉Ͷ͍ͯΔɻྫ೥ͱಉ༷ʹɺ෱Ԭ‫಺ݝ‬ͷશͯͷߴߍͱपล‫ݝ‬ͷ༗ྗߴߍʹҊ಺ঢ়ΛૹΓɺࢀՃऀΛืूͨ͠ͱ͜Ζɺ37 ໊ͷࢀՃ͕͋ͬͨɻ·ͨɺҰൠ޲͚ͷެ։ߨ࠲΁ͷਃࠐऀ 24 ໊ɺߴઐੜ 9 ໊Ͱɺશମडߨऀ਺͕ 70 ໊ʹୡͨ͠ɻࠓ೥͸ 25 ೔ʹେֶͷଔ‫ࣜۀ‬ɺ27 ೔͔Β෺ཧֶձ͕͋ͬͨͨΊɺ೔༵೔Λ‫ؚ‬Ή೔ఔͱͳͬͨɻॳ೔ͷηϛφʔ͸೔༵೔Ͱ͋ͬͨͨΊެ։ߨ࠲ͷԠืऀ͕ྫ೥ΑΓଟ͘ɺ·ͨɺೋ೔໨ͷ 24 ೔͕ଔ‫ࣜۀ‬ͷߴߍ͕ଟ਺͋ͬͨͨΊମ‫ݧ‬ೖֶͷԠืऀ͸ྫ೥ΑΓগͳ͔ͬͨɻ࣮
ࡍͷηϛφʔɾ࣮‫ݧ‬ͷ಺༰ɺεέδϡʔϧɺ୲౰ऀ͸Լ‫ه‬ͷϓϩάϥϜʹࣔ͢ɻମ‫ݧ‬ೖֶࢀՃऀͷॅॴ͸෱ԬΛத৺ʹɺେ෼ɺ‫۽‬ຊɺ௕࡚ɺࠤլɺ‫࡚ٶ‬ɺ޿ౡͳͲ޿ൣғʹΘ͍ͨͬͯΔɻ࠷ऴ೔ʹดߍࣜΛߦ͍ɺࠓ‫ޙ‬ͷվળͷͨΊʹΞϯέʔτΛ͓‫͍ͨ͠ئ‬ɻମ‫ݧ‬ೖֶʹ 2 ೔ؒࢀՃͨ͠ߴߍੜʹରͯ͠શൠͷ‫ײ‬૝ʹ͍ͭͯฉ͍ͨ݁ՌΛ࠷‫ޙ‬ͷάϥϑʹࣔ͢ɻ‫ڵ‬ຯʢ໘ന͍ʔී௨ʔ໘ന͘ͳ͍ʣͱ೉қ౓ʢ೉͍͠ʔී௨ʔқ͍͠ʣʹ͍ͭͯ౴͑ͯ΋Β͍ɺ֤ੜె͕Ͳͷ૊Έ߹ΘͤͰճ౴͔ͨ͠Λू‫ͨ͠ܭ‬΋ͷͰ͋ΔɻશମͷΞϯέʔτͰ࠷΋ଟ͍ճ౴͸ʮ໘നͯ͘೉қ౓΋ͪΐ͏Ͳྑ͍ʯɺ2 ൪໨͸ʮ໘ന͍͕೉͍͠ʯͰ͋Γɺ֓Ͷ޷ධͰ͋ͬ
ͨͱߟ͍͑ͯΔɻ࣮‫Ͱݧ‬͸ʮ໘നͯ͘೉қ౓΋ͪΐ͏Ͳྑ͍ʯ͕ѹ౗తʹଟ͘ɺʮ࣮‫ָ͕͠ݧ‬͔ͬͨʯͱ͍͏੠΋ฉ͔Εͨɻ͔͠͠ɺࡢ೥౓͔ΒҾ͖ଓ͖ಛʹηϛφʔʹ͓͍ͯʮ໘ന͍
Ұํɺ಺༰͕೉͍͠ʯͱ͍͏੠͕΍΍ଟ͋͘ΔͷͰɺࠓ‫ޙ‬ɺվળͷ༨஍͕͋ΔͱࢥΘΕΔɻ

10:00ʙ11:00
11:10ʙ12:00
12:00ʙ13:30
13:30ʙ14:20
14:30ʙ15:20
ɹ 15:30ʙ

2014 ೥ 3 ݄ 23 ೔ (೔)։ߍࣜʮޫͰϛΫϩͷੈքΛૢΔʯ
(໦ଜ‫ڭ‬त)ன‫ٳ‬Έ‫ۃڀ‬ͷ෺ཧ๏ଇΛ͙͞Δʙૉཻࢠཧ࿦ͷੈքʙʢླ໦‫ڭ‬तʣʮϏοάόϯӉ஦ͱ෺࣭ਐԽʯ
(‫ڮ‬ຊ‫ڭ‬त)ղࢄ

2014 ೥ 3 ݄ 24 ೔ (݄)
10:00ʙ10:05 ࣮‫ݧ‬ͷ஫ҙ
10:10ʙ12:10 ࣮‫( ݧ‬AʙD ͔Β 1 ςʔϚ)
12:10ʙ13:10 ன‫ٳ‬Έ
13:10ʙ13:15 ू߹
13:20ʙ15:20 ࣮‫( ݧ‬AʙD ͔Β 1 ςʔϚ)
15:30ʙ15:45 ดߍࣜʲ࣮‫ݧ‬ςʔϚʢ୲౰ऀʣʳ
A. ෺࣭Λಁա͢Δཻࢠઢʢࣉ੢ɹߴʣ
B. ‫ۃ‬௿Թͷੈքʢઙ໺ɹ‫ߦو‬ʣC. ௒఻ಋΛମ‫͢ݧ‬Δʢࢁాɹ࿨ਖ਼ʣ
D. ޫͷճંͱ೾ͷෆࢥٞʙ೾ಈͷॏͶ߹Θͤͱߴߍɾେֶͷ਺ֶʙʢߥҪ ‫ؽ‬ʣ

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