cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Perseo fa surf sull’onda calda
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2017

Secondo gli esperti che hanno elaborato i dati, questa onda di gas si è formata alcuni miliardi di anni fa dopo il flyby di un piccolo cluster di galassie che ha attirato parte della vasta riserva di gas di Perseo. La formazione concava è una delle più misteriose e interessanti di questo gigantesco ammasso, relativamente vicino alla Terra
title: ÐÐ»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°: ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ, Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð´Ñ Ð¾Ð´Ñ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ° ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸
Creators: name: ÐÐ¸Ð½Ð¾Ð³ÑÐ°Ð´Ð¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
name: ÐÐ²Ð°Ð½Ð¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
name: Ð¢Ð¾Ð¼ÑÐ¸Ð½ÑÐºÐ°Ñ, ÐÑÐ¸Ð½Ð°
name: Ð¤Ð¸Ð»Ð¸Ð¿Ð¿Ð¾Ð²Ð°, ÐÐ¸Ð»Ð¸Ñ
name: Ð¨Ð°Ð´ÑÐ¸Ð½Ð°, Ð®Ð»Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2017
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
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description: ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð»Ð°Ð½Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐµÐ³Ð¾ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÐºÐ°Ðº Ð¾Ð´Ð¸Ð½ Ð¸Ð· Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ; Ð´Ð°Ð½Ñ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÐµ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð¾ÑÐµÐ½ÐºÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÐ¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð° Ð¸ Ð¸Ð·Ð´Ð°Ð½Ð° Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ Ð·Ð½Ð°ÑÐ¸Ð¼ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð² ÑÑÐµÑÐµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð½Ð°ÑÐºÐ¸ Ð¸ Ð¼Ð¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð¿Ð¾ Ð¿ÑÐ¾ÐµÐºÑÑ Â«ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ°Ñ Ð¸ ÐºÐ¾Ð½ÑÑÐ»ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ° Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ â ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ¾Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÐ¼Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÐ¼Ð¸Â». ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð° Ð´Ð»Ñ ÑÑÐºÐ¾Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÐµÐ¹, ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð¿Ð»Ð°Ð½Ð¾Ð²Ð¾-ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¸ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¸Ñ ÑÐ»ÑÐ¶Ð± Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ, ÑÐ»ÑÑÐ°ÑÐµÐ»ÐµÐ¹ Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ (Ð¿Ð¾ Ð¾ÑÑÐ°ÑÐ»ÑÐ¼)Â», Â«ÐÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÑ, Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð°ÑÐ´Ð¸ÑÂ», Â«ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¸ Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÂ».
M83, dove la supernova è di casa
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2017

La galassia Messier 83 o M83 in breve, a circa 15 milioni di anni luce, è uno degli splendidi oggetti celesti che caratterizzano il cielo meridionale di queste sere. I consigli per individuarla, insieme ai pianeti e ai principali fenomeni celesti visibili a maggio
Piccola nube di Magellano a 1.6 gigapixel
Creators: Redazione Eso
Publisher: name: Media Inaf
Year: 2017

La piccola galassia nella costellazione del Tucano è una caratteristica inconfondibile del cielo australe, anche a occhio nudo. La visione dei telescopi in luce visibile è oscurata dalla polvere interstellare, ma il telescopio infrarosso Vista è riuscito a guardare al di là di questa polvere. Alla guida dello studio, Stefano Rubele dell’Università di Padova
title: ÐÐµÐ¾Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð² Ð¿ÑÐ¸ÑÐ¾Ð´Ð¾Ð¾Ð±ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ðµ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 280400 "ÐÑÐ¸ÑÐ¾Ð´Ð¾Ð¾Ð±ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾"
titleType: Subtitle
Creators: name: ÐÑÐµÑÑÐµÐ², ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹
name: ÐÐ°Ð´ÐµÐ½ÐºÐ¾, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2008
Subjects: ÐÐµÐ¾Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°
ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÐÑÐ¸Ð½ÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ð¹

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ Ð±Ð°Ð·Ð¾Ð²ÑÑ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸ÑÑ Ð³ÐµÐ¾Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼ (ÐÐÐ¡), Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼, Ð±ÑÐ´ÑÑÐ¸Ð¼ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ°Ð¼ Ð¿ÑÐ¸ÑÐ¾Ð´Ð¾Ð¾Ð±ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ, ÐºÐ°Ðº Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ ÐÐÐ¡ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ ÑÑÐµÐ´ÑÑÐ²Ð° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹. ÐÐ¾Ð´ÑÐ¾Ð±Ð½Ð¾ Ð¾Ð±ÑÑÐ¶Ð´Ð°ÑÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² ÐÐÐ¡ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¸ ÑÐ²Ð»ÐµÐ½Ð¸Ð¹ ÑÐµÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ³Ð¾ Ð¼Ð¸ÑÐ°. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÐºÐ°Ðº Ð² ÐÐÐ¡ Ð¼Ð¾Ð¶Ð½Ð¾ ÑÑÑÑÐºÑÑÑÐ¸ÑÐ¾Ð²Ð°ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¾Ð²Ð°ÑÑ Ð½Ð°Ð¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ð±Ð°Ð· Ð´Ð°Ð½Ð½ÑÑ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 280400 "ÐÑÐ¸ÑÐ¾Ð´Ð¾Ð¾Ð±ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾" Ð¸ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð´ÑÑÐ³Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Polvere eri, impulso elettromagnetico diventerai
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2017

Detriti e polvere cosmica rappresentano un serio problema per le sonde spaziali, questo già lo sapevamo. Ma la minaccia non è solo meccanica: gli impatti possono infatti produrre interferenze radio in grado di disturbare l’elettronica di bordo, come dimostrato già nel 1998 dall’astrofisico dell’Inaf Luigi Foschini. Ora si è chiarito il meccanismo all’origine del fenomeno
The QCD form factor of heavy quarks at NNLO
Creators: name: Gluza, J.
name: Mitov, A.
name: Moch, S.
name: Riemann, T.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present an analytical calculation of the two-loop QCD corrections to the electromagnetic form factor of heavy quarks. The two-loop contributions to the form factor are reduced to linear combinations of master integrals, which are computed through higher orders in the parameter of dimensional regularization epsilon=(4-D)/2. Our result includes all terms of order epsilon at two loops and extends the previous literature. We apply the exponentiation of the heavy-quark form factor to derive new improved three-loop expansions in the high-energy limit. We also discuss the implications for predictions of massive n-parton amplitudes based on massless results in the limit, where the quark mass is small compared to all kinematical invariants.
description: latex, 37 pages, 4 figures
ТЕРГОВ СУДЬЯСИНИНГ ВАКОЛАТЛАРИ  (ЎЗБЕКИСТОН ВА ҚОЗОҒИСТОН РЕСПУБЛИКАЛАРИ ҚОНУНЧИЛИГИ ТАҲЛИЛИДА)
Creators: name: Омонов, Зафаржон
Publisher: name: Zenodo
Year: 2025

description: Мамлакатимизда сўнги йилларда амалга оширилиб келаётган суд-ҳуқуқ тизимидаги ислоҳотлар натижасида жиноят-процессуал қонунчилигига бир қанча янги институтлар кириб келди. Мисол тариқасида, кўрсатувларни олдиндан мустаҳкамлаб қўйиш, айбга иқрорлик бўйича келишув каби институтларни бунга мисол қилиб келтиришимиз мумкин. Қуйида ушбу ислоҳотлар давоми ўлароқ жорий этилган тергов судьяси институти ҳақида тўхталиб ўтишни лозим деб топдик.
Nessun nucleo attivo per la galassia nana
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2017

Grazie alle capacità osservative dello strumento Multi Unit Spectroscopic Explorer del Very Large Telescope, un team di ricercatori è riuscito a scoprire che l’emissione di Heinze 2-10, una galassia nana vicina, è dovuta a bolle di gas in espansione, e non alla presenza di un buco nero attivo al suo centro. L’intervista a Giovanni Cresci, dell’Inaf di Firenze, che ha guidato lo studio
Family life in the apartment environment : a study of the social aspects of apartment housing for families.
Creators: name: Lyman, Eva Georgina Hilda
Publisher: name: University of British Columbia
Year: 2012

description: As our major cities increase in size, more and more families may be expected to prefer central housing in the form of an apartment to the outlying single family house. In the major cities the need to achieve greater densities in order to make more economical use of our land is another factor of growing importance. Although the rate of construction of apartment buildings hag increased in recent years, there has been little recognition of the fact that certain families with children may increasingly wish to live in apartments due to the benefits offered by housing located close to employment, social and cultural facilities. The social values of families differ, depending on the orientation and interests of the members, and may be expected to affect the housing type desired. The group which might be better served by apartment housing may be larger than expected. However, at the present time apartment houses have certain disadvantages for family living. Some complaints which are commonly raised are discussed in this thesis. Clearly any improvements aimed at making the apartment environment suitable for family living must take into account the social needs and roles of the family and its members. A thorough study of sociological literature on the family and its needs was carried out. These needs ape discussed and interpreted in terms of their housing significance and implications for the apartment environment. It is concluded that with some changes in the present way of building apartments, and with the provision of various facilities necessary for family development on a communal or community basis, the apartment environment could be adapted to family living. Additional proof of the feasibility of making the apartment environment acceptable for family life can be seen in the Swedish housing situation. There a large proportion of families with children are housed in three and four story walk-up apartments, without suffering any hardship. The stress in Sweden, moreover, is on community planning with all the requirements of the people in mind, rather than on one isolated aspect of the total picture (i.e. the construction of dwellings). The dwelling unit alone is not considered to be adequate to take care of all the social needs of the family. Facilities for outdoor recreation, hobbies, cultural and other activities, are seen as a necessary extension of the home. They are provided outside the home, but as close as possible to it. Since the Canadian people have lived traditionally in their own houses, some prejudice against other housing types can be expected to linger. However, if the apartment environment provided as many of the amenities popularly associated with the single family home as possible, in addition to being centrally located, public prejudice may be expected to disappear in time.
High frequency susceptibility of a weak ferromagnet with magnetostrictive magnetoelectric coupling: using heterostructures to tailor electromagnon frequencies
Creators: name: Livesey, K. L.
name: Stamps, R. L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: In the first part of this work we calculate the high frequency magnetoelectric susceptibility of a simultaneously ferroelectric and canted antiferromagnetic (also know as weak ferromagnetic) thin film with magnetostrictive magnetoelectric coupling. We show that a dynamic coupling exists between the ferroelectric and optic antiferromagnetic excitations. In the second part of the paper, we calculate using an effective medium method the susceptibility of a heterostructure comprising alternating thin films of such a material together with a ferromagnet. Dipolar magnetic fields serve to couple the ferromagnetic and optic antiferromagnetic modes, which in turn couples the ferromagnetic and ferroelectric excitations. This provides a mechanism for creating "electromagnon" modes in the microwave regime which may be useful for applications.
Quel vuoto incolmabile tra Saturno e gli anelli
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2017

La divisione che separa l'atmosfera del sesto pianeta e l'anello più interno presenta dei livelli di polvere davvero bassi, in contrasto con il piano degli anelli. I dati del secondo dei 22 tuffi del gran finale arriveranno domani
Variants of bosonisation in Parabosonic algebra. The Hopf and super-Hopf structures
Creators: name: Kanakoglou, K.
name: Daskaloyannis, C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Rings and Algebras (math.RA)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 16S40, 16W30, 57T05

description: Parabosonic algebra in finite or infinite degrees of freedom is considered as a $\mathbb{Z}_{2}$-graded associative algebra, and is shown to be a $\mathbb{Z}_{2}$-graded (or: super) Hopf algebra. The super-Hopf algebraic structure of the parabosonic algebra is established directly without appealing to its relation to the $osp(1/2n)$ Lie superalgebraic structure. The notion of super-Hopf algebra is equivalently described as a Hopf algebra in the braided monoidal category ${}_{\mathbb{CZ}_{2}}\mathcal{M}$. The bosonisation technique for switching a Hopf algebra in the braided monoidal category ${}_{H}\mathcal{M}$ (where $H$ is a quasitriangular Hopf algebra) into an ordinary Hopf algebra is reviewed. In this paper we prove that for the parabosonic algebra $P_{B}$, beyond the application of the bosonisation technique to the original super-Hopf algebra, a bosonisation-like construction is also achieved using two operators, related to the parabosonic total number operator. Both techniques switch the same super-Hopf algebra $P_{B}$ to an ordinary Hopf algebra, producing thus two different variants of $P_{B}$, with ordinary Hopf structure.
description: 27 pages, some typos of the journal version are corrected and a couple of references added
Materia oscura, misteriosa e inafferrabile
Creators: Carlo Burigana
Publisher: name: Media Inaf
Year: 2017

Sarà fredda, tiepida o calda? E soprattutto: di cos’è fatta? Ipotizzata e resa pressoché indispensabile da osservazioni astrofisiche e cosmologiche, ma a oggi mai rilevata direttamente, della materia oscura sappiamo pochissimo. Più domande che risposte, dunque, per la sostanza di cui sembra essere costituito, in gran parte, il cosmo
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² ÑÑÐ½Ð½ÐµÐ»ÑÐ½Ð¾-ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ ÐºÐ²Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐ¼ GaAs/AlGaAs Ð² Ð¿ÑÐ¾Ð´Ð¾Ð»ÑÐ½ÑÑ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð»ÑÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¨ÑÐ¼Ð¸Ð»Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð»Ñ
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Ð¸Ð½ÑÑÐ°ÐºÑÐ°ÑÐ½ÑÐ¹ Ð´Ð¸Ð°Ð¿Ð°Ð·Ð¾Ð½ ÑÐ¿ÐµÐºÑÑÐ°

description: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð´Ð¾Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð½Ð° ÑÐ¿ÐµÐºÑÑÑ Ð¿Ð¾Ð³Ð»Ð¾ÑÐµÐ½Ð¸Ñ ÑÐ²ÐµÑÐ° ÑÑÐµÐ´Ð½ÐµÐ³Ð¾ Ð¸Ð½ÑÑÐ°ÐºÑÐ°ÑÐ½Ð¾Ð³Ð¾ Ð´Ð¸Ð°Ð¿Ð°Ð·Ð¾Ð½Ð° Ð¸ Ð½Ð° ÑÐ¿ÐµÐºÑÑÑ Ð¼ÐµÐ¶Ð·Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¾ÑÐ¾Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ð¸ Ð² Ð´Ð²Ð¾Ð¹Ð½ÑÑ ÑÑÐ½Ð½ÐµÐ»ÑÐ½Ð¾-ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ ÐºÐ²Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐ¼Ð°Ñ GaAs/AlGaAs. ÐÐ¾Ð´ÑÐ»ÑÑÐ¸Ñ Ð¼ÐµÐ¶Ð¿Ð¾Ð´Ð·Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð³Ð»Ð¾ÑÐµÐ½Ð¸Ñ Ð¸ Ð¼ÐµÐ¶Ð·Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¾ÑÐ¾Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ð¸ Ð¿Ð¾Ð»ÐµÐ¼ ÑÐ²ÑÐ·Ð°Ð½Ñ Ñ Ð¿ÐµÑÐµÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸ÐµÐ¼ Ð³Ð¾ÑÑÑÐ¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¾Ð² Ð¼ÐµÐ¶Ð´Ñ Ð¿Ð¾Ð´Ð·Ð¾Ð½Ð°Ð¼Ð¸ ÑÐ·ÐºÐ¾Ð¹ Ð¸ ÑÐ¸ÑÐ¾ÐºÐ¾Ð¹ ÑÐ¼, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð¾Ð±ÑÐµÐ¼Ð½Ð¾Ð³Ð¾ Ð·Ð°ÑÑÐ´Ð° Ð² ÑÑÑÑÐºÑÑÑÐµ. ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¿ÐµÐºÑÑÐ¾Ð² Ð¼Ð¾Ð´ÑÐ»ÑÑÐ¸Ð¸ Ð¿Ð¾Ð³Ð»Ð¾ÑÐµÐ½Ð¸Ñ Ð¸ ÑÐ¾ÑÐ¾Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ð¸ Ð² ÑÐ¸Ð»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð´Ð¾Ð»ÑÐ½ÑÑ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð»ÑÑ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð» Ð¾ÑÐµÐ½Ð¸ÑÑ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÑ Ð³Ð¾ÑÑÑÐ¸Ñ Ð½Ð¾ÑÐ¸ÑÐµÐ»ÐµÐ¹ Ð·Ð°ÑÑÐ´Ð°.
description: The influence of the lateral electric field on the mid-infrared intersubband light absorption and interband photoluminescence in double tunnel-coupled GaAs/AlGaAs quantum wells was investigated. Intersubband absorption modulation and interband photoluminescence modulation are associated with electron redistribution between subbands of narrow and wide quantum wells and space charge variation in the structure. Analysis of the absorption and photoluminescence modulation spectra under high lateral electric field was allowed to estimate hot carrier temperature.
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ° ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÑÐ±ÐµÐ²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð°Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ
ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð°Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ
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ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ°

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ°Ð¿Ð¸ÑÐºÐ¸Â». Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐ°Ð¿Ð¸ÑÐºÐ¸Â» Ð¿Ð¾ÑÑÐµÐ´ÑÑÐ²Ð¾Ð¼ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¾Ð½Ð»Ð°Ð¹Ð½ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½ÐµÐ³Ð°ÑÐ¸Ð²Ð½ÑÐµ Ð¼Ð¾Ð¼ÐµÐ½ÑÑ Ð² Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐ°Ð¿Ð¸ÑÐºÐ¸Â». Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÑ Ð´Ð»Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¾Ð²Ð°ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ° Ð¸ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº Ð¾Ð±ÑÐ°ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð¾ÑÐºÑÑÑÐ¸Ñ Ð¾Ð½Ð»Ð°Ð¹Ð½ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð½Ð° Ð±Ð°Ð·Ðµ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ³Ð¾ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· Ð´Ð¾ÑÐ¾Ð´Ð¾Ð² Ð¸ ÑÐ°ÑÑÐ¾Ð´Ð¾Ð² Ð¾Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¾Ð½Ð»Ð°Ð¹Ð½ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹. ÐÐ½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð¾Ð½Ð»Ð°Ð¹Ð½ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ ÑÐ²ÐµÐ»Ð¸ÑÐ¸ÑÑ ÑÐ¾Ð²Ð°ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾Ñ Ð¸ Ð¿ÑÐ¸Ð±ÑÐ»Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸.
Additional file 1 of Sarcopenia negatively affects postoperative short-term outcomes of patients with non-cirrhosis liver cancer
Creators: name: Yang, Jinhuan
name: Wang, Daojie
name: Ma, Lei
name: An, Xuewen
name: Hu, Zijing
name: Zhu, Huili
name: Zhang, Wanqian
name: Chen, Kaiwen
name: Ma, Jun
name: Yang, Yan
name: Wu, Lijun
name: Chen, Gang
name: Wang, Yi
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Cardiology

description: Additional file 1: Table_S1. Hematological indicators of the first admission among the groups. Table_S2. Postoperative hematological indicators among the groups. Table_S3. Logistic Regression for Predictive Factors of Postoperative Complications.
Dark matter, più “fuzzy” che “cold”
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2017

Uno studio su 13 ammassi di galassie osservate con Chandra tenta di ricavare nuovi indizi assumendo un’ipotesi alternativa al modello di materia oscura fredda. I risultati, pubblicati su Mnras, suggeriscono che la materia oscura potrebbe avere anche una natura ondulatoria dovuta a effetti quantistici
title: ÐÐ¾Ð²ÑÑÐµÐ½Ð¸Ðµ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÐ¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð¸Ð½ÑÑÐ°ÑÑÑÑÐºÑÑÑÑ Ð¿ÑÐ¸ Ð¿Ð¸ÑÐ°Ð½Ð¸Ð¸ Ð¾Ñ ÑÐµÑÐµÐ¹ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÑÑÐµÐ²Ð°, Ð¡Ð¾ÑÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐ¸ Ð¿ÑÐ¾Ð¼Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹
Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐ¸
Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐ¸ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ
Ð¢ÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ½ÑÐµ Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ð¸

description: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÐ¸ Ð³Ð¾ÑÐ¾Ð´ÑÐºÐ¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐµÑÐ¸ Ð³. Ð¡Ð²ÐµÑÐ¾Ð³Ð¾ÑÑÐº, Ð¾ÑÐµÐ½ÐµÐ½Ñ ÑÐ¾ÐºÐ¸ Ð¾Ð´Ð½Ð¾ÑÐ°Ð·Ð½Ð¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ñ Ð·Ð°ÑÐ¸ÑÑ Ð¾Ñ Ð½Ð¸Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð²ÑÐ±Ð¾Ñ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ.
Il senso di Euclid per l’infrarosso
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2017

Consegnati i primi rivelatori per lo spettrofotometro Nisp, la “retina” perfetta per osservare il vicino infrarosso. Nuovo traguardo per Euclid, la missione Esa dedicata allo studio dell’universo oscuro. Il punto con Luca Valenziano, responsabile scientifico per Inaf del progetto e operation manager dello strumento
Gravitational-wave astronomy: Observational results and their impact
Creators: name: Shawhan, Peter S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The successful construction and operation of highly sensitive gravitational-wave detectors is an achievement to be proud of, but the detection of actual signals is still around the corner. Even so, null results from recent searches have told us some interesting things about the objects that live in our universe, so it can be argued that the era of gravitational-wave astronomy has already begun. In this article I review several of these results and discuss what we have learned from them. I then look into the not-so-distant future and predict some ways in which the detection of gravitational-wave signals will shape our knowledge of astrophysics and transform the field.
description: Based on invited talk at the 8th Amaldi Conference on Gravitational Waves (Columbia U, New York, June 2009); accepted by Classical and Quantum Gravity
Simultaneous Qualitative And Quantitative Identification Of Multiple Targets By Polymerase Chain Reaction On Microarray
Creators: name: Zakharova, Natalia V
name: Drobyshev, Alexei L
name: Khodakov, Dmitry A
name: Myznikova, Anna I
name: Gorban, Irina A
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantitative Methods (q-bio.QM)
subject: FOS: Biological sciences

description: An approach for multiplex qualitative and quantitative microarray-based PCR analysis has been proposed. The characteristics of PCR executed on a gel-based oligonucleotide microarray with immobilized forward primers and a single common reverse primer in solution were investigated for several DNA targets. One-stage multiplex on-chip PCR was studied for simultaneous amplification of herpes simplex viruses types 1 and 2, cytomegalovirus DNA, and bacteriophage lambda DNA as an internal control. Additionally the joint analysis of increased number of targets (with addition of Chlamydia trachomatis, Mycoplasma hominis, and Ureaplasma urealyticum DNA) was done in two-stage version of assay: first stage was in-tube PCR with target-specific primers, while the reverse ones contained 5'-adapter region; the second stage was on-chip amplification with immobilized target-specific forward primers and adapter as common reverse primer in solution. The possible application of one-stage reaction for human cDNA analysis was additionally demonstrated with utilization of a common poly-T-containing primer in solution. SYBR green I; and Cy-5 labeled dUTP were used for real-time and end-point detection of specific PCR products. The efficiencies of both one-stage and two-stage reactions was shown to be strongly dependent on magnesium and primers concentrations. Quantitative PCR in the both versions was studied with 10-fold serial dilutions of phage lambda DNA. The method enabled detection of 6 DNA copies per reaction for both versions of assay. The quantitative interval for one-stage reaction covered eight orders of concentration. The revealed significant effect of gel pad size on microarray PCR effectiveness has been discussed.
Agn, i nuclei galattici attivi
Creators: Marcello Giroletti
Publisher: name: Media Inaf
Year: 2017

Nelle regioni centrali di ogni galassia si trova un buco nero supermassiccio. Nella maggior parte dei casi sono in fase dormiente. Ma all’incirca in una galassia su dieci il buco nero è vispissimo, e nelle sue vicinanze viene emessa una quantità di radiazione persino superiore a quella della galassia che lo ospita
Cassini spericolata, mai così vicina a Saturno
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2017

Si è tuffata a volo radente attorno al pianeta, passando nello stretto varco tra l’atmosfera e il bordo più interno degli anelli. Le immagini che ha inviato a Terra sono le più ravvicinate mai ottenute. Prossima immersione il 2 maggio
title: ÐÑÐ¾ÐµÐºÑ ÑÐµÑÑÑÐµÑ ÑÑÐ°Ð¶Ð½Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð° (ÑÐ°ÑÑÐµÑ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐµÐ¹Ð½Ð¾Ð², ÐÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð°ÑÑ Ð¸ÑÐµÐºÑÑÑÐ½Ð¾-ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ°ÑÑÑ
Ð¾Ð±ÑÐµÐ¼Ð½Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐ¾ÐµÐ½Ð¸Ñ
Ð²Ð½ÐµÑÐ½ÑÑ Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½ÑÑ Ð¾ÑÐ´ÐµÐ»ÐºÐ°
ÑÐ°ÑÑÐµÑ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ¾Ð»Ð¾Ð½Ð½Ñ

description: Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð² Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐ½Ð¾-ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ Ð¸ÑÑÐ¾Ð´Ð½ÑÐµ Ð´Ð°Ð½Ð½ÑÐµ Ðº Ð¿ÑÐ¾ÐµÐºÑÑ, Ð¼ÐµÑÑÐ¾ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¾Ð±ÑÐµÐºÑÐ° Ñ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸ÐµÐ¼ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸.Ð Ð³ÐµÐ½ÐµÑÐ°Ð»ÑÐ½Ð¾Ð¼ Ð¿Ð»Ð°Ð½Ðµ Ð¾ÑÐ¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¾ Ð·Ð´Ð°Ð½Ð¸Ðµ Ñ ÑÐ°Ð·Ð¼ÐµÑÐ°Ð¼Ð¸, ÑÐ»Ð¸ÑÑ, Ð¿Ð°ÑÐºÐ¸. ÐÐ°Ð½Ð° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾ Ð¿Ð°ÑÐºÐ¾Ð²ÐºÐµ, Ð¿Ð°ÑÐºÐµ Ð¸ Ñ.Ð´. Ð Ð¾Ð±ÑÐµÐ¼Ð½Ð¾-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ð¼ Ð¿ÑÐ½ÐºÑÐµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿Ð»Ð¾ÑÐ°Ð´Ð¸ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ð¹, Ð²ÑÑÐ¾ÑÐ½Ð¾ÑÑÑ Ð·Ð´Ð°Ð½Ð¸Ñ, Ð³Ð¾Ð²Ð¾ÑÐ¸ÑÑÑ Ð¾ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¸ Ð¸ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ð¸ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ð¹. Ð¢Ð°Ðº Ð¶Ðµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ°Ð±Ð»Ð¸ÑÐ° Ñ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¼Ð¸ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÑÐ¼Ð¸. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð¾Ð±ÑÐµÐ³Ð¾ ÑÐ¾Ð¿ÑÐ¾ÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ¿Ð»Ð¾Ð¿ÐµÑÐµÐ´Ð°ÑÐµ Ð¾Ð³ÑÐ°Ð¶Ð´ÐµÐ½Ð¸Ñ. ÐÐ° ÐºÐ°Ð¶Ð´ÑÐ¹ ÑÐ·ÐµÐ» Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½ÑÑ Ð¸ Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð½Ð°Ð³ÑÑÐ·Ð¾Ðº. Ð Ð¿ÑÐ¾ÐµÐºÑÐµ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÐºÐ¾Ð»Ð¾Ð½Ñ Ð¸ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½Ñ
Quantum filter reduction for measurement-feedback control via unsupervised manifold learning
Creators: name: Nielsen, Anne E. B.
name: Hopkins, Asa S.
name: Mabuchi, Hideo
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We derive simple models for the dynamics of a single atom coupled to a cavity field mode in the absorptive bistable parameter regime by projecting the time evolution of the state of the system onto a suitably chosen nonlinear low-dimensional manifold, which is found by use of local tangent space alignment. The output field from the cavity is detected with a homodyne detector allowing observation of quantum jumps of the system between states with different average numbers of photons in the cavity. We find that the models, which are significantly faster to integrate numerically than the full stochastic master equation, largely reproduce the dynamics of the system, and we demonstrate that they are sufficiently accurate to facilitate feedback control of the state of the system based on the predictions of the models alone.
description: 15 pages, 6 figures
Let’s go to Mars. The game
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2017

Disponibile per Android, iOs e Pc. Già scaricata da oltre 50mila appassionati. Ricca di personaggi e densa di citazioni cinematografiche. È la app più marziana del momento. Ce la siamo fatta descrivere da uno degli scienziati del progetto Upwards, Marco Giuranna, dell’Inaf Iaps di Roma
Getti relativistici dalla galassia sbagliata
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2017

Utilizzando i dati provenienti dallo strumento Circe al Gran Telescopio Canarias e dal satellite Fermi della Nasa, un gruppo di ricercatori guidati da Filippo D'Ammando, dell’Istituto di radioastronomia dell’Inaf di Bologna, ha scoperto emissione variabile nei raggi gamma da galassie di tipo narrow-line Seyfert 1 rivelando la presenza di una possibile nuova classe di nuclei galattici attivi con getti relativistici
Spontaneously broken parity and consistent cosmology with transitory domain walls
Creators: name: Mishra, Sasmita
name: Yajnik, Urjit A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Domain wall structure which may form in theories with spontaneously broken parity is generically in conflict with standard cosmology. It has been argued that Planck scale suppressed effects can be sufficient for removing such domain walls. We study this possibility for three specific evolution scenarios for the domain walls, with evolution during radiation dominated era, during matter dominated era, and that accompanied by weak inflation. We determine the operators permitted by the supergravity formalism and find that the field content introduced to achieve desired spontaneous parity breaking makes possible Planck scale suppressed terms which can potentially remove the domain walls safely. However, the parity breaking scale, equivalently the majorana mass scale $M_R$ of the right handed neutrino, does get constrained in some of the cases, notably for the matter dominated evolution case which would be generic to string theory inspired models giving rise to moduli fields. One left-right symmetric model with only triplets and bidoublets is found to be more constrainted than another admitting a gauge singlet.
Svelare la grana del cosmo? È un gioco di coppia
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2017

Ci sono volute settimane di supercalcolo, un algoritmo d’intelligenza artificiale, venticinque rarissime coppie di quasar e un giovane cosmologo originario di San Daniele del Friuli, ora ricercatore postdoc a Cambridge, per osservare in dettaglio le increspature del mezzo intergalattico
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð±Ð°Ð½ÐºÐ¸Ð½Ð³Ð° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ Â«ÐÐ»ÑÑÐ°-ÐÐ°Ð½ÐºÂ»)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¥Ð°ÑÑÐ¼Ð°Ð½Ð½, ÐÐ³Ð¾Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð±Ð°Ð½Ðº
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐ Â«ÐÐ»ÑÑÐ°-ÐÐ°Ð½ÐºÂ».
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ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÑÐ¾Ð¹ ÑÐµÐ»Ð¸ Ð² ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð±Ð°Ð½ÐºÐ¸Ð½Ð³Ð°, ÐµÐ³Ð¾ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° Ð¸ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð±Ð°Ð½ÐºÐ¸Ð½Ð³Ð° Ð² Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ Ð·Ð° ÑÑÐ±ÐµÐ¶Ð¾Ð¼, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐ Â«ÐÐ»ÑÑÐ°-ÐÐ°Ð½ÐºÂ».
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title: Ð Ð°Ð·Ð²Ð¸ÑÐ¸Ðµ ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼ÑÑÐ»ÐµÐ½Ð¸Ñ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ñ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ðº Ð½Ð°ÑÑÐ½ÑÐ¼ Ð´ÐµÐ±Ð°ÑÐ°Ð¼ Ð½Ð° Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¼ ÑÐ·ÑÐºÐµ
title: Development of critical thinking of postgraduate students in the field of experimental medicine in the process of preparation for scientific debates in english
Creators: name: ÐÐ°Ð³ÑÐ°Ð¼Ð¾Ð²Ð°, ÐÐ¸Ð½Ð°
name: ÐÐµÐ´ÐµÑÐ½Ð¸ÐºÐ¾Ð²Ð°, ÐÐ°ÑÐ¸Ñ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð°Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ð°

description: ÐÐ¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° ÐºÐ°Ð´ÑÐ¾Ð² Ð²ÑÑÑÐµÐ¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð² Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÑÑÐµ Ð² Ð²ÑÐ·Ð°Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ñ, Ð½Ð°Ð¿ÑÐ¸Ð¼ÐµÑ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ Ð¿Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¼ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð°Ð¼ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÑ Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð½Ð¾ Ð¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ Ð¿Ð¾ ÑÐ°ÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ, ÐºÐ°Ðº Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾ Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¹ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº. Ð¢Ð°Ðº, Ð½Ð° ÑÐµÐ³Ð¾Ð´Ð½ÑÑÐ½Ð¸Ð¹ Ð´ÐµÐ½Ñ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð°Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ð°Â» Ð¸ Â«ÐÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð½Ð°ÑÐºÐ¸Â» Ð·Ð° Ð¿ÐµÑÐ¸Ð¾Ð´ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ 3 Ð³Ð¾Ð´Ð° Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ ÑÐ³Ð»ÑÐ±Ð¸ÑÑ ÑÐ²Ð¾Ð¸ Ð·Ð½Ð°Ð½Ð¸Ñ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð¸ÑÑ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð° Ð±Ð°Ð·Ðµ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ¸Ð¹ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ¾Ð², Ð½Ð¾ Ð¸ Ð¿ÑÐ¾Ð¹ÑÐ¸ ÑÐ·ÑÐºÐ¾Ð²ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾ Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÑ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¾ÑÐ²Ð¾ÐµÐ½Ð¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÐ½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐºÂ» Ð² ÑÐµÑÐµÐ½Ð¸Ðµ Ð´Ð²ÑÑ Ð»ÐµÑ.
Growth studies in the reindeer (Rangifer tarandus) : with an analysis of population changes in the Mackenzie Delta herd over the period 1938-1958
Creators: name: Krebs, Charles J.
Publisher: name: University of British Columbia
Year: 2012

description: A study of the growth of reindeer (Rangifer tarandus) was carried out during the spring and summer of 1958 in the Mackenzie Delta, N.W.T. Growth rates were obtained for four fawns over this period. Their growth is described by Brody's equation and the von Bertalanffy equation. The rate of growth of reindeer fawns is slightly less than that of the Columbian Black-tailed Deer, whereas the birth weight of the reindeer is double that of the Black-tailed Deer. A description of the relative growth of several body measurements is given. Hind foot length, heart girth, height-at-withers, muzzle circumference, and antler length were measured. The measurement error of height-at-withers and muzzle circumference limits the usefulness of this data. The changes in herd numbers and composition of the Mackenzie Delta Reindeer Herd over the period 1938-1958 are analyzed. Of the three population determining factors (natality, mortality, and dispersal), dispersal (losses by straying) was by far most important and natality (number of fawns) was least important in determining the total annual increment to the herd over the period 1938-1958. The age distribution of the herd over the period 1938-1958 has been relatively stable.
title: Learning through comparison when studying evidence and policy
Creators: name: Smith, Katherine E.
name: Andersen, Niklas A.
name: Pattyn, Valérie
Publisher: name: Strathprints - University of Strathclyde
Year: 2025

description: The aim of this special themed section is to demonstrate the conceptual and empirical contribution that comparative perspectives offer in advancing scholarship on the evidence-policy interplay. It is motivated by our sense that a lack of comparative analysis within this area of research risks conceptual confusion and contributes to limited engagement with the more political dimensions of evidence use. It brings together four papers which, between them: examine evidence use across different government ministries within the same country; provide a cross-national comparison of parliamentary institutions to support evidence use; explore variations in evaluation approaches within different national settings; and reflect on how perspectives on evidence shift when researchers become politicians, trying to navigate complex policy environments. We use this editorial to reflect on three cross-cutting themes that emerge from these four contributions. First, a tendency for dominant disciplines to shape evidence cultures in policy settings. Second, the complexity of policy making, which, in democracies, necessarily includes political dimensions. These two themes inform a third, the need for realism when working to support the use of evidence in policy. We conclude by arguing that this themed section highlights the contextual, divergent and contingent nature of evidence use in policy. By showcasing four contrasting approaches to comparative analysis of evidence use, we hope to encourage a desire to learn from, and reflect on, the insights provided by less familiar contexts and disciplines, while also underlining the necessity of considering the political and democratic dimensions of evidence use in policy.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð°Ð»ÑÑÐµÑÐ½Ð°ÑÐ¸Ð²Ð½ÑÑ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐºÐ»Ð°Ð´ÑÐºÐ¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ°
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐºÐ¾Ð², ÐÐµÐ½Ð½Ð°Ð´Ð¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¡ÐºÐ»Ð°Ð´Ñ
Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ðµ Ñ ÑÐ°Ð½ÐµÐ½Ð¸Ðµ Ð²ÐµÑÐµÐ¹
Ð±Ð¾ÐºÑÑ Ð´Ð»Ñ Ñ ÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð²ÐµÑÐµÐ¹

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ²Ð»ÑÐµÑÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð±Ð¾ÐºÑÐ¾Ð² Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ. Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð¾ÑÐµÐ½ÐºÐ° Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐºÐ»Ð°Ð´Ð° Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð²ÐµÑÐµÐ¹ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð°Ð»ÑÑÐµÑÐ½Ð°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð±Ð¾ÐºÑÐ¾Ð² Ð´Ð»Ñ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ¾ÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð¿ÑÐ¾ÐºÐ°ÑÐ°. Ð ÑÐ°Ð¼ÐºÐ°Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐºÑÑÐµÐ³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÑÐ½ÐºÐ° Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð¸ ÑÐºÐ»Ð°Ð´ÑÐºÐ¸Ñ ÑÑÐ»ÑÐ³ Ð² ÑÐµÐ»Ð¾Ð¼. ÐÐ·ÑÑÐµÐ½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐºÐ»Ð°Ð´Ð° Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð²ÐµÑÐµÐ¹. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«Ð ÐÐ¡ÐÐÐÐÂ». Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¿ÑÐ¾ÐµÐºÑ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° ÐºÐ¾ÑÐ¸Ð´Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±Ð¾ÐºÑÐ¾Ð² Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð¸ Ð´Ð¾ÐºÐ°Ð·Ð°Ð½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐºÐ»Ð°Ð´Ð° Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ.
An investigation of the mycorrhiza of Douglas-fir seedlings.
Creators: name: Pentland, Gertrude Draper
Publisher: name: University of British Columbia
Year: 2012

description: A study was made to determine if there is a growth response in Douglas-fir seedlings to the presence of mycorrhizal associations. Nursery, potted and pure culture experiments were carried out to induce the formation of mycorrhiza on Douglas-fir seedlings. Seedlings from natural areas were examined to give an indication of the types of mycorrhiza which occur and the age at which they are formed. Variation in the number and type of mycorrhiza as determined by site factors was studied. Well-developed mycorrhiza were found in natural seedlings as young as three months old. Most of the seedlings examined showed well-developed mycorrhiza by the end of the first growing season. Only typical ectotrophic mycorrhiza were found in Douglas-fir seedlings. They occurred in a range of sites, but the occurrence could not be correlated with variation in site factors. In the nursery and potted experiments there were no significant differences between the treatments as indicated by the height, root volume or number of mycorrhiza of the seedlings. All attempts to induce the formation of mycorrhiza on Douglas-fir seedlings in pure culture were unsuccessful.
Isoscalar giant resonances in the Sn nuclei and implications for the asymmetry term in the nuclear-matter incompressibility
Creators: name: Li, T.
name: Garg, U.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We have investigated the isoscalar giant resonances in the Sn isotopes using inelastic scattering of 386-MeV alpha-particles at extremely forward angles, including 0deg. We have obtained completely "background-free inelastic-scattering spectra for the Sn isotopes over the angular range 0deg--9deg and up to an excitation energy of 31.5 MeV. The strength distributions for various multipoles were extracted by a multipole decomposition analysis based on the expected angular distributions of the respective multipoles. We find that the centroid energies of the isoscalar giant monopole resonance (ISGMR) in the Sn isotopes are significantly lower than the theoretical predictions. In addition, based on the ISGMR results, a value of K_{tau} = -550 \pm 100 MeV is obtained for the asymmetry term in the nuclear incompressibility. Constraints on interactions employed in nuclear structure calculations are discussed on the basis of the experimentally-obtained values for K_(infty) and K_(tau).
description: Accepted for publication in Physical Review C. Minor revisions in text and labeling of figures
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð¹ Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÐºÐ¸ Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð¸Ð¼ÐµÑÑÐµÐ¹ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð² Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ Ð·Ð° ÑÑÐ±ÐµÐ¶Ð¾Ð¼ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐºÐµÐ° Ð´Ð¾Ð¼Â»)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð ÑÐ·Ð°Ð½Ð¾Ð²Ð°, ÐÐµÑÐ¾Ð½Ð¸ÐºÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð°Ñ Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÐºÐ°
ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð°Ñ Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÐºÐ°
ÐÐºÐµÐ° Ð´Ð¾Ð¼
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐÐÐ ÐÐÐÂ». Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð¹ Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÐºÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¸Ð¼ÐµÑÑÐµÐ³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð·Ð° ÑÑÐ±ÐµÐ¶Ð¾Ð¼ Ð¸ Ð² Ð Ð¾ÑÑÐ¸Ð¸.Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð¼Ð°ÑÑÑÑÑÐ¾Ð² Ð´Ð»Ñ Ð¿ÐµÑÐµÐ²Ð¾Ð·ÐºÐ¸ ÐºÐ¾Ð½ÑÐµÐ¹Ð½ÐµÑÐ° Ñ Ð¼ÐµÐ±ÐµÐ»ÑÑ Ð² ÑÐ¼ÐµÑÐ°Ð½Ð½Ð¾Ð¼ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¼ ÑÐ¾Ð¾Ð±ÑÐµÐ½Ð¸Ð¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÑÐµÐ²Ð¾Ð³Ð¾ Ð³ÑÐ°ÑÐ¸ÐºÐ° Ð¸Ð· ÐÐ°Ð»ÑÐ½Ñ (ÐÐ¸ÑÐ°Ð¹) Ð² ÐÐ¾ÑÐºÐ²Ñ. ÐÐ¾ÑÑÐ¸ÑÐ°Ð½Ñ ÐºÑÐ¸ÑÐµÑÐ¸Ð¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐ½Ð½Ð¾ÑÑÐ¸ ÐÐ°Ð¿Ð»Ð°ÑÐ°, ÐÑÑÐ²Ð¸ÑÐ°, ÐÐ°Ð»ÑÐ´Ð°, Ð¡ÑÐ²Ð¸Ð´Ð¶Ð°.
Phase diagram and large deviations in the free-energy of mean-field spin-glasses
Creators: name: Parisi, Giorgio
name: Rizzo, Tommaso
Publisher: name: arXiv
Year: 2008
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We consider the probability distribution of large deviations in the spin-glass free energy for the Sherrington-Kirkpatrick mean field model, i.e. the exponentially small probability of finding a system with intensive free energy smaller than the most likely one. This result is obtained by computing $Φ(n,T)=T \bar{Z^n}/ n$, i.e. the average value of the partition function to the power $n$ as a function of $n$. We study in full details the phase diagram of $Φ(n,T)$ in the $(n,T)$ plane computing in particular the stability of the replica-symmetric solution. At low temperatures we compute $Φ(n,T)$ in series of $n$ and $τ=T_c-T$ at high orders using the standard hierarchical ansatz and confirm earlier findings on the $O(n^5)$ scaling. We prove that the $O(n^5)$ scaling is valid at all orders and obtain an exact expression for the coefficient in term of the function $q(x)$. Resumming the series we obtain the large deviations probability at all temperatures. At zero temperature the analytical prediction displays a remarkable quantitative agreement with the numerical data. A similar computation for the simpler spherical model is also performed and the connection between large and small deviations is discussed.
description: Detailed study of the phase diagram and proof of the fifth order scaling at all temperatures, final version accepted on PRB
เทคนิคการปลูกแก่นตะวันในประเทศไทยและแนวทางการใช้ประโยชน์จากหัวแก่นตะวันในอุตสาหกรรมอาหาร
Creators: name: นรินทร์ เจริญพันธ์
Publisher: name: กองบริหารการวิจัย
Year: 2564
Subjects: แก่นตะวัน
เทคนิคการปลูก
อินูลิน
อุตสาหกรรมอาหาร

description: วารสารวิทยาศาสตร์และเทคโนโลยี, 29, 6, 919-940