Grant-in-Aid for Scientiﬁc Research on Innovative Areas“Research on the Emergence of Hierarchical Structure of Matterby Bridging Particle, Nuclear and Astrophysics in Computational Science”

Quarks to Universein Computational Science(QUCS2012)
Sinya AOKI
University of Tsukuba
Symposium “Quarks to Universe in Computational Science(QUCS2012)”,
December 13-16, 2012, Nara, Japan

Our project
Grant-in-Aid for Scientiﬁc Research on Innovative Areas:
A new Grant from MEXT, which started at 2008.
MEXT=Ministry of Education, Culture, Sports, Science and Technology“Research on the Emergence of Hierarchical Structure of Matterby Bridging Particle, Nuclear and Astrophysics in Computational Science”• Collaboration among particle-, nuclear- and astro- physics• via Computational physics• 5 years Project (2008.12-2013.3).
• O($1.2M)/Year-> O(€1.2M)/Year• 4 planed research groups + 1 central committee• O(20x2) proposed personal researches:• 2 years x twice(2009-2010/2011-2012), O(€15K)/year• workshop, symposium, school, lecturePurpose of the Project and Research Plans
To construct a new research area where researchers in particle, nuclear andastrophysics work coherently to investigate the hierarchical structure of matterfrom quarks and nuclei to supernova explosions and nucleosynthesis via
computational science.
J-PARC (2009-)

Lattice
QCD

BaryonInteraction

Structure and reactionof (Hyper) Nuclei
EoS ofnuclear matter

Neutron Star
SuperNova

Elementary Particle
Computational Science

J-PARC
RIBF

nucleosynthesis

Nuclear Physics
garvitational wave
nuetrino physics

RIBF (2007-)

Astrophysics

Research Organization
Central committee

Leader: Sinya Aoki (University of Tsukuba)

Planed research groups
A01「Vacuum structure and quark dynamics in QCD」
Leader: Tetsuya Onogi (Osaka University)

projects
proposals

A02「Nuclei Structure from quark dynamics」
Leader: Testuo Hatsuda (University of Tokyo->Riken)

projects
proposals

A03「 Supernova explosion and nucleosynthesis
via quark dynamics and nuclei structure」
Leader: Hideyuki Suzuki (Tokyo University of Science)

projects
proposals

A04「Interdisciplinary algorithm and computer simulations」
Leader: Hideo Matsufuru (KEK)

projects

proposals

Thursday, December 13#"$%&'(

Activities(2008.12-2012.12)T. Hatsuda, Y. Ikeda, N. Ishii (Tokyo)

09:00-10:00
Registration
10:00-12:00
Session I
Chair: S. Aoki (Tsukuba)%!"!
Planned
10:00-10:20 Researches
S. Aoki (Tsukuba)
Opening and overview
S. Aoki, T. Doi, T. Inoue,()%*$$)%+*+,-*+.,%-./012(/34/
10:20-10:45
T. Oonogi (Osaka)Particle physics project (A01) report
K. Murano, K. Sasaki (Tsukuba)
10:45-11:10
T. Hatsuda (RIKEN)
Nuclear physics project (A02) report!%'()"5672$34!%$)3"5"6$4"##'78$!"#"$%&'(/
11:10-11:35
H. Suzuki (Tokyo Sci.)
Astrophysics project (A03) report
H. Nemura (Tohoku))%&89'()%'(:;<=)*
11:35-12:00
H. Matsufuru (KEK)
Computational physics project (A04) report&@9:9@A&+B@,&;1<=@CD&@E-&
12:00-13:30
Lunch
A02
NN potential from lattice QCD
13:30-16:00
Session II:?@.%/0FGH16:2(IA01
A04 Chair: T. Hatsuda (RIKEN)
JLDG
13:30-14:20
T. Janka (MPA)
Core-collapse
supernovae
B+3J"56745(K/#LM
He from lattice QCD
14:20-14:50
Y. Sekiguchi (YITP)
Numerical Relativity Simulations of NS-NS binary merger
C6D78N9H8O
14:50-15:40
T. Kennedy (Edinburgh)
Progress of algorithms in lattice gauge simulations($%PQ
15:40-16:00
K. Ishikawa (Hirosima)
Testing SSOR preconditioner for Domainwall/Overlap normal equations
0-0.01
16:00-16:30
Break
RSTR;%+<=-0.02
16:30-18:20
Session III
Chair: H. Suzuki (Tokyo Sci.)
He
X%YH%&'Z%>?
-0.03
16:30-17:00
M. Hayakawa (Nagoya)Numerical approach to QED contribution in the lepton g-2-0.04
17:00-17:20
H. Fukaya (Osaka)
Pion form factors in the epsilon regime-0.05
Mean-field calculation
including proton-neutron mixing in atomic
nuclei --toward
ハイペロン状態方程式(石塚，大西によるSh
17:20-17:40
K. Sato (RIKEN)-0.06
proton-neutron pairing-S1-0.07
17:40-18:00
T. Yoshida(Tokyo)Current Status of Massive Star Evolution
S2
0""exp. (YITP)!"!"
18:00-18:20
K.
KiuchiBlackhole-neutronstarmerger
withneutrinocooling
!
4
4
-0.01
5
A03
18:30-20:30
Poster Session
-0.02
5
!
!"#!
!"#!
!

-0.03
-0.04

3

Friday, December 14-0.05

09:00-10:30-0.07
0.0 2-17 2-16
09:00-09:50
09:50-10:30
10:30-11:00

-0.06

He

Session IV-15-14
Z. Fodor (Wuppertal)
2
2
3
1/L
Y. Akiba (RIKEN)
BreakBaryon EoS

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Chair: S. Hashimoto (KEK) #"!"#%Computational particle physics
Quark-Gluon Plasma
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Proposed Personal Researches (2009-2010)• T. Yamazaki “Lattice QCD and light nuclei”• Y. Kikukawa “Electroweak theory on the lattice”• K. Sasaki “K-π interaction in lattice QCD”
• E. Shintani “Muon anomalous magnetic moment in lattice QCD”
• S. Sasaki “Charmonium Nuclei”• T. Abe “Monte-Carlo no-core shell model for light nuclei”• M. Matsuo “Light and neutrino nuclei reactions in the continuum region”• M. Takano “Variational calculation of EoS for nuclear matter at T=0”
• K. Hashimoto “ Nuclear force and superstring theory”• H. Nemura “Hyperon interactions in lattice QCD and light hyper-nuclei”• S. Nagataki “Gamma ray burst”• Y. Sekiguchi “Numerical relativity for binary neutron star merger”• N. Yasutake “QCD phase transition for the evolution of neutron”• T. Sakurai “Linear algebra for particle, nuclear and astrophysics”• T. Ishikawa “Special purpose machine for higher order corrections”

Proposed Personal Researches (2011-2012)• Y. Taniguchi “QED corrections in lattice QCD”
• S. Ejiri “EoS in lattice QCD at ﬁnite density”• S. Takeda “Phase structure in lattice QCD”
• T. Yamazaki “Light nuclei in lattice QCD”
• H. Fukaya “Qualitative estimate for observables in chiral symmetry breaking”• H. Iida “Interaction between massive quarks in lattice QCD”
• E. Shintani “Neutron electric dipole moment in lattice QCD”
• T. Izubuchi “Lattice QCD simulations in chiral quarks”• S. Sasaki “Hyperon beta decay in lattice QCD”
• K. Hashimoto ”Holography and nuclear force”• A. Umeya “Neutron-rich large hypernuclei in shell model with tensor force”• T. Hanawa “Magnetic hydrodynamics wave in supernova explosion”• K. Nomoto “ R-process nucleosynthesis in supernova explosion ”• H. Sotani “Internal structure of neutron star from gravitational waves”• T. Maruyama “Pasta structure of nuclei”• T. Sakurai “Linear algebra for particle, nuclear and astrophysics”

Collaboration between diﬀerent groups• A01-A02• Nuclear physics in lattice QCD• A02-A03• EoS in neutron star/nuclear matter• A01-A04• Improvement of algorithm & eﬃciency• Data Grid
• Development and maintenance of QCD code
• A03-A04• Code for supernova explosion• parallelization, linear solver• neutrino radiation & transport in 3-dim.

Symposium, Workshop, Lecture, School, etc.
Annual Symposium/Workshop

bottle gifted by
Matsufuru-san

2008.12.1-2 Startup workshop@Tsukuba“Bridging Particle, Nuclear and Astrophysics
in Computational Science”
2010.3.15-16 Joint Symposium@Tokyo“Origin of matter and universe”
2010.11.28-30 International Symposium@Atagawa(hot spring)“From Quarks to Supernovae”

2011.12.3-5 Workshop@Shima“Progress on Bridging Particle, Nuclear and Astrophysics
in Computational Science”

2012.12.13-16 Summary Symposium@Nara“Quarks to Universe in Computational Science (QUCS2012)”

Other Symposia/Workshops

JICFuS=Joint Institute for Computational Fundamental Science

2009.2.23 JICFuS symposium@Tsukuba “Future of fundamental sciencein large scale simulations”
2011.6.23-24 Crossover workshop with ʻNew hadronʼ @Kobe“Challenge in hadron physics”
2012.7.12-13 Crossover workshop with ʻNew hadronʼ @Nagoya“New hadrons in various ﬂavors”
Summer School @Kyoto(organized by Hiyama)“From quarks to supernovae”
2011.8.4-11

1st2012.7.27-31 2nd
about 30 participants(Student, young PD)
Lattice QCD simulations for nuclear force
Few body calculation for He binding energy
EoS calculation and simulation for supernova explosion

Lecture Series for non-experts (organized by Aoki)
1. 2010.6.9-10@Tokyo M. Shibata “Numerical relativity”
2. 2010.12.15-16@Kyoto S. Aoki “Lattice QCD and numerical simulations”
3. 2011.6.8-9@Tokyo K. Kotake “High energy astrophysics”
4. 2012.1.11-12@Kyoto T. Abe “Nuclei shell model”
5. 2012.2.27-28@Riken Y. Funaki “Nuclei cluster model”
6. 2012.6.18-19@Tsukuba M. Hanada “Monte Carlo approach to String/M theory”
7. 2011.11.8-9@Kobe T. Okamoto “Galaxy formation and dark matter”

Awards
2009.2 25th Inoue prize for science, S. Aoki
2010.1 6th JSPS prize, M. Shibata

JSPS= Japan Society for the Promotion of Science

2010.3 4th Young scientist awards of JPS, T. Yamazaki, Y. Ikeda
JPS= The Physical Society of Japan

2011.3 5th Young scientist awards of JPS, T. Abe
2012.3 17th JPS awards for academic paper on physics, S.Aoki-T.Hatsuda-N.Ishii
2012.10 23th Tsukuba prize, S.Aoki-T.Hatsuda-N.Ishii
2012.12 2012 Nishina memorial prize, S.Aoki-T.Hatsuda-N.Ishii

SPIRE(Strategic Program for Innovative Research)
Field 5 “Origin of matter and the universe”
SPIRE: MEXT’s program to promote scientific and engineering applications of K computer.
(FY2011-15)

Field 1

Predictive life sciences, medical care and drug
designField 2 New material and energy creation
Global change prediction for disaster prevention and
Field 3
reduction

RIKEN
Institute of Solid State
Physics, Univ. of Tokyo
JAMSTEC

Field 4 Industrial Innovation

Institute of Industrial Science,
Univ. of Tokyo

Field 5 Origin of matter and the universe

RCCS, Univ. of Tsukuba

Project-1. Lattice QCD
Project-2. Nucleus
Project-3. Supernova Explosion
Project-4. Early Star Formation
Our project is playing a major role in ﬁeld 5.

O(10)Peta Flops supercomputer
available from fall in 2012

1016 = 10 Peta

RIKEN
Fujitsu Limited
November 14, 2011percomputer³.FRPSXWHU´Takes Consecutive No. 1 in World Ranking
Top 500

Rank

Computervendor1

K computer

Fujitsu

2

Tianhe-1A

NUDT

eving world¶s fastest processing speed of 10.51 petaflops and 93.2% operating efficiency

2011.6

country

LINPACK(PFops)

PEAK(PFlops)

Japan

8.162

8.774

China

2.566

4.701

Cray

USA

1.759

2.331

FujitsuJapan

10.51011.280

NUDT

China

2.566

4.701

Cray

USA

1.759

2.331

IBM

USA

16.32520.133

FujitsuJapan

10.51011.280

IBM

USA

8.162

10.066

CRAY

USA

17.59027.113IBMUSA

16.32520.133

FujitsuJapan

10.51011.280tho, November 14, 2011 ± RIKEN and Fujitsu have taken the No. 1 position for the ³K computer´ (*1) on the 38
00 (*2) list announced today in the US (November 14, PST), for a consecutive two terms in a row. The K computer,
ntly under joint development, was designated as being the world¶s fastest supercomputer. The TOP500 was
ously announced in June 2011.

TOP500-ranked K computer system has 864 computer racks equipped with a total of 88,128 CPUs. The system
ved the world¶s best LINPACK (*3) benchmark performance of 10.51 petaflops (quadrillion floating-point operations
econd) with a computer efficiency ratio of 93.2%.

3

2011.11

Jaguar10 Supercomputers on the TOP500 List

Rank

1

Computer

K computer

2
Tianhe-1A
2012.63

Jaguar4

Nebulae

5

TSUBAME 2.0

6

Cielo

7

Pleiades2012.118
Hopper9

Tera-100

10Roadrunner

1
2

K computer
Site

VendorCountry
Tianhe-1A

RIKEN Advanced
Institute for
Computational Science(AICS)
National
Supercomputing Centerin Tianjin
DOE/SC/Oak Ridge
National Laboratory
National
Supercomputing Centrein Shenzhen (NSCS)
GSIC Center, Tokyo
Institute of Technology
DOE/NNSA/LANL/SNL
NASA/Ames ResearchCenter/NAS
DOE/SC/LBNL/NERSC
Commissariat al¶Energie Atomique(CEA)
DOE/NNSA/LANL

MaximalLINPACK
performanceachieved

3

JaguarJapan

10,510

1

NUDT
China
Sequoia

2,566

2

Cray Inc.
US
K computer

1,759

3

Dawning

Mira

China

1,271

NEC/HP

Japan

1,192

Cray Inc.

US

1,110

SGI

US

1,088

US

1,054

1
2
3

Fujitsu

Titan
Cray
Inc.

Bull SAFranceSequoiaIBMUS

K computer

1,050
1,042

certification ceremony will be held at SC11, the International Conference for High Performance Computing,orking, Storage and Analysis, being held in Seattle, Washington in the United States. The ceremony is schedulede place on November 15, 2011 PST (November 16, 2011 in Japan).

Future• summarize activities of the project in this symposium.
• no succeeding proposal to this project in Grant-in-Aid for ScientiﬁcResearch on Innovative Areas, but• a large part of activities will run under the Field-5 of SPIRE from 2013.
• 3 research projects +1 new project• Summer School, Lecture Series• Support, QCD common code(Bridge++)• Our sprits for interdisciplinary collaborations will remain important for the
success of Field-5.

December 13 (Thur.) -16 (Sun.), 2012
Nara Prefectural New Public Hall
Nara Prefectural New Public Hall
Thursday, December 13
09:00-10:00
Registration
Thursday, December
13
10:00-12:00
09:00-10:00
10:00-10:20
10:00-12:00
10:20-10:45
10:00-10:20
10:45-11:10
10:20-10:45
11:10-11:35
10:45-11:10
11:35-12:00
11:10-11:35
12:00-13:30
11:35-12:00
13:30-16:00
12:00-13:30
13:30-14:20
13:30-16:00
14:20-14:50
13:30-14:20
14:50-15:40
14:20-14:50
15:40-16:00
14:50-15:40
16:00-16:30
15:40-16:00
16:30-18:20
16:00-16:30
16:30-17:00
16:30-18:20
17:00-17:20
16:30-17:00
17:00-17:20
17:20-17:40

SessionI
Registration
S.Session
Aoki (Tsukuba)
I
T.
Oonogi(Osaka)S. Aoki (Tsukuba)
T.
(RIKEN)
T.Hatsuda
Oonogi (Osaka)H.
Sci.)
T. Suzuki
Hatsuda(Tokyo(RIKEN)H.
Matsufuru(KEK)
H. Suzuki (Tokyo Sci.)
Lunch
H. Matsufuru (KEK)
SessionLunch II
T.
Janka (MPA)
SessionIIY.
(YITP)
T. Sekiguchi
Janka (MPA)
T.
(Edinburgh)
Y.Kennedy
Sekiguchi(YITP)
K.
Ishikawa(Hirosima)
T. Kennedy (Edinburgh)
Break
K. Ishikawa (Hirosima)
SessionBreak IIIM.
Hayakawa
Session
III (Nagoya)
H.
(Osaka)M.Fukaya
Hayakawa(Nagoya)
H.SatoFukaya(Osaka)K.
(RIKEN)

17:20-17:40
17:40-18:00
18:00-18:20
17:40-18:00
18:00-18:20
18:30-20:30
18:30-20:30

K.Yoshida
Sato (RIKEN)
T.
(Tokyo)K.
(YITP)
T.Kiuchi
Yoshida(Tokyo)K. Kiuchi(YITP)
PosterSessionPoster Session

Symposium program

Chair: S. Aoki (Tsukuba)
Openingandoverview
Chair: S.
Aoki(Tsukuba)
Particle
physics
project
Opening and overview (A01) report
NuclearParticle physics project (A02)(A01) report
Astrophysics
project(A03)
reportNuclear physics
project(A02)
reportComputational
physics
project(A04)
Astrophysics project (A03) report report
Computational physics project (A04) report
Chair: T. Hatsuda (RIKEN)
Core-collapse
supernovae
Chair: T. Hatsuda(RIKEN)
Numerical
Relativity
Simulations of NS-NS binary merger
Core-collapse
supernovae

Progressof Relativity
algorithmsSimulations
in lattice gauge
simulations
Numericalof NS-NSbinary merger
Testing
SSOR
preconditioner
for
Domainwall/Overlap
normal equations
Progress of algorithms in lattice gauge simulations
Testing SSOR preconditioner for Domainwall/Overlap normal equations
Chair: H. Suzuki (Tokyo Sci.)
Numerical
to QED Sci.)
contribution in the lepton g-2
Chair: H. approach
Suzuki (Tokyo
Pion
form factors
in theepsilonregime in the lepton g-2
Numerical
approach
to QED
contribution
Mean-fieldcalculation
proton-neutron mixing in atomic nuclei --toward
Pion form factors
in theincluding
epsilon regime
proton-neutron
pairing--including proton-neutron mixing in atomic nuclei --toward
Mean-field calculation
Current
Status ofpairing-Massive Star Evolution
proton-neutronBlackhole-neutronstar merger
with neutrino cooling
Current
Status of Massive
Star Evolution
Black hole-neutron star merger with neutrino cooling

A03(Invited)
A04(Invited)

A04
A01 A01
A02
A03

Friday, December 14
Friday, December
14 IV
09:00-10:30
Session09:00-10:30
IV
09:00-09:50
Z.Session
Fodor (Wuppertal)
09:00-09:50
Z. Akiba
Fodor (RIKEN)(Wuppertal)
09:50-10:30
Y.
09:50-10:30
Y. Akiba (RIKEN)
10:30-11:00
Break
10:30-11:00
Break V
11:00-12:30
Session11:00-12:30
V
11:00-11:50
J.SessionCarlson (LANL)
11:00-11:50
J. Sakurai
Carlson (RIKEN/Tokyo)(LANL)
11:50-12:30
H.
11:50-12:30
H. Sakurai (RIKEN/Tokyo)
12:30-14:00
Lunch
12:30-14:00
Lunch VI
14:00-16:00
Session14:00-16:00
Session14:00-14:40
H.
Tamura VI(Tohoku)
14:00-14:40
H.Abe
Tamura(Tohoku)
14:40-15:10
T.
(Tokyo)14:40-15:10
T.
Abe(Tokyo)15:10-15:40
T. Doi (RIKEN)
15:10-15:40
T. TogashiDoi (RIKEN)
15:40-16:00
H.
(Waseda)15:40-16:00
H. Togashi (Waseda)
16:00-16:30
Break
16:00-16:30
Break VII
16:30-18:10
Session
16:30-18:10
SessionVII
16:30-16:50
G.
Cossu (KEK)
16:30-16:50
G.Inoue
Cossu(Nihon)(KEK)
16:50-17:10
T.
16:50-17:10
T.
Inoue(Nihon)17:10-17:30
S. Ejiri (Niigata)
17:10-17:30
S. Tsunoda
Ejiri (Niigata)17:30-17:50
Y.
(Tokyo)17:30-17:50
Y.
Tsunoda(Tokyo)
17:50-18:10
S. Wanajo (NAOJ)
17:50-18:10
S. Wanajo (NAOJ)
19:30Banquet
19:30Banquet

Chair: S. Hashimoto (KEK)
Chair: S. Hashimoto(KEK)
Computational
particle physics
Computational
particle physics
Quark-Gluon
PlasmaQuark-Gluon PlasmaA01(Invited)Exp

Chair: T. Nakatsukasa (RIKEN)
Chair: T. Nakatsukasa(RIKEN)
Computational
nuclear physics
Computational
Nuclearphysicsnuclear
at RIBFphysics
Nuclear physics at RIBF

A02(Invited)Exp

Chair: E. Hiyama (RIKEN)
Chair: E. Hiyama(RIKEN)
Strangenessnuclear physics
StrangenessnuclearNo-coreMonte
Carlophysics
shell model towards ab initio nuclear structure
No-coreMonte
Carlomodel towards ab initio nuclear structure
Hadron interactions onshell
the lattice
Hadron interactions
the lattice
Variational
Study of ona Nuclear
Equation of State for Core-Collapse Supernovae
Variational Study of a Nuclear Equation of State for Core-Collapse Supernovae

Exp

Chair: H. Matsufuru (KEK)
Chair:
H. Matsufuru
Finitetemperature
study(KEK)of axial symmetry on the lattice
Finite temperature
axial symmetry on the lattice
Neutronstars from study
LatticeofQCD
Neutronstars
fromLattice
QCD
Study of finite density lattice QCD by the histogram method
Study ofof medium-massfinite density latticeby the histogram
methodStudynucleiQCD
by large-scale
shell model
calculations
Studyofmedium-massnucleibylarge-scale
shell
model
calculations
r-process: supernovae vs. neutron star mergers
r-process: supernovae vs. neutron star mergers

A03

A02
A02
A03
A01
A01
A03

A02
A02

Symposium programSymposium program
Poster Program
A01-P1
A01-P2
A01-P3
A01-P4
A01-P5
A01-P6
A01-P7
A01-P8
A02-P9
A02-P10
A02-P11
A02-P12
A02-P13
A02-P14
A02-P15
A02-P16
A02-P17
A02-P18
A02-P19
A02-P20
A02-P21
A02-P22
A02-P23
A03-P24
A03-P25
A03-P26
A03-P27
A03-P28
A03-P29

X. Feng (KEK)
Y. Aoki (KMI, Nagoya Univ.)
K. Kanaya (Univ. of Tsukuba)
T. Kaneko (KEK)
Y.-G. Cho (Univ. of Tsukuba)
Y. Nakagawa (Niigata Univ.)
M. Hanada (KEK)
S. Furui (Teikyo Univ.)
B. Charron (Univ. of Tokyo)
Y. Ikeda (RIKEN)
N. Ishii (CCS, Univ. of Tsukuba)
F. Uchiyama (KEK)
S. Ohnishi (Tokyo Tech. /RIKEN)
S. Ozaki (Yonsei Univ.)
K. Sasaki (CCS, Univ. of Tsukuba)
H. Suno (RIKEN)
H. Toki (RCNP, Osaka Univ.)
H. Nemura (Univ. of Tsukuba)
K. Fukukawa (RIKEN)
K. Horii (RCNP, Osaka Univ.)
T. Myo (Osaka Inst. of Technology)
K. Murano (RIKEN)
M. Yamada (Univ. of Tsukuba)
M. Okamoto (Univ. of Tsukuba)
H. Sotani (NAOJ)
M. Takano (Waseda Univ.)
K. Takahashi (Univ. of Tokyo)
S. Nagataki (YITP, Kyoto Univ.)
K. Nakamura (NAOJ)

A03-P30

S. Furusawa (Waseda Univ.)

A03-P31
A03-P32
A03-P33

K. Hotokezaka (Kyoto Univ.)
K. Masuda (Univ. of Tokyo)
N. Yasutake (Chiba Tech.)

Time-like pion form factor in lattice QCD
Exploring for Walking Technicolor from QCD -Towards the Composite Higgs ModelQuark matter at high temperatures and low densities on the lattice
Precision determination of the CKM matrix element |Vus|
O(a^2)-improved lattice fermions with exact chiral symmetry
Lattice study of the phase structure in finite density QCD with a histogram method
Numerical Approach to Supersymmetric Gauge Theories and String/M-theory
Dark matter and the triality symmetry of leptons and quarks
Pion-pion interaction from lattice QCD
LQCD study of pi-Sigma and KN interactions
2+1 flavor QCD result of nuclear forces
Extreme neutron rich nuclei in the beginning of formation of matter in universe
Production Reaction of KbarNN-piYN Resonance and KbarN interaction
Lattice study of low energy charmoninum-hadron scattering
Coupled channel approach to S=-2 baryon-baryon system in Lattice QCD
Application of the Gaussian expansion method to cold atomic few-body systems
Tensor optimized shell model and the role of delta for finite nuclei
Study of LambdaNucleon-SigmaNucleon interaction from lattice QCD
Three-Nucleon Scattering by the Quark-Model Baryon-Baryon Interaction fss2
Tensor optimized few-body for light nuclei
Tensor optimized shell model using bare interaction for light nuclei
Spin-Orbit force in the NN system from Lattice QCD
Omega-Omega interaction on the LatticeNon-uniform nuclear matter in neutron star crust
Possibility to restrict on neutron star matter by using asteroseismology
Variational Study of Nuclear Matter with an Explicit Energy FunctionalCore collapse of an O+Ne core
Central Engine of Long Gamma-Ray Bursts and Resulting Explosive Nucleosynthesis
Multi-dimensional Simulations of Core-collapse Supernovae
The influence of nuclear statistical equilibrium equation of state on core-collapse
supernova simulations of massive stars
0HDVXUHPHQWRIWKHHTXDWLRQRIVWDWHZLWKJUDYLWDWLRQDOZDYHGHWHFWRUVHadron-Quark Crossover and Massive Hybrid Stars with StrangenessNon-uniform structures in hadron-quark phase transition with Dyson-Schwinger method

3 best posters will be selectedby the committee.

Symposium programDecember 13 (Thur.) -16 (Sun.), 2012
Nara Prefectural New Public Hall
Nara Prefectural New Public Hall
Thursday, December 13
09:00-10:00
Registration
Thursday, December
13
10:00-12:00
09:00-10:00
10:00-10:20
10:00-12:00
10:20-10:45
10:00-10:20
10:45-11:10
10:20-10:45
11:10-11:35
10:45-11:10
11:35-12:00
11:10-11:35
12:00-13:30
11:35-12:00
13:30-16:00
12:00-13:30
13:30-14:20
13:30-16:00
14:20-14:50
13:30-14:20
14:50-15:40
14:20-14:50
15:40-16:00
14:50-15:40
16:00-16:30
15:40-16:00
16:30-18:20
16:00-16:30
16:30-17:00
16:30-18:20
17:00-17:20
16:30-17:00
17:00-17:20
17:20-17:40

SessionI
Registration
S.Session
Aoki (Tsukuba)
I
T.
Oonogi(Osaka)S. Aoki (Tsukuba)
T.
(RIKEN)
T.Hatsuda
Oonogi (Osaka)H.
Sci.)
T. Suzuki
Hatsuda(Tokyo(RIKEN)H.
Matsufuru(KEK)
H. Suzuki (Tokyo Sci.)
Lunch
H. Matsufuru (KEK)
SessionLunch II
T.
Janka (MPA)
SessionIIY.
(YITP)
T. Sekiguchi
Janka (MPA)
T.
(Edinburgh)
Y.Kennedy
Sekiguchi(YITP)
K.
Ishikawa(Hirosima)
T. Kennedy (Edinburgh)
Break
K. Ishikawa (Hirosima)
SessionBreak IIIM.
Hayakawa
Session
III (Nagoya)
H.
(Osaka)M.Fukaya
Hayakawa(Nagoya)
H.SatoFukaya(Osaka)K.
(RIKEN)

17:20-17:40
17:40-18:00
18:00-18:20
17:40-18:00
18:00-18:20
18:30-20:30
18:30-20:30

K.Yoshida
Sato (RIKEN)
T.
(Tokyo)K.
(YITP)
T.Kiuchi
Yoshida(Tokyo)K. Kiuchi(YITP)
PosterSessionPoster Session

Symposium program

Chair: S. Aoki (Tsukuba)
Openingandoverview
Chair: S.
Aoki(Tsukuba)
Particle
physics
project
Opening and overview (A01) report
NuclearParticle physics project (A02)(A01) report
Astrophysics
project(A03)
reportNuclear physics
project(A02)
reportComputational
physics
project(A04)
Astrophysics project (A03) report report
Computational physics project (A04) report
Chair: T. Hatsuda (RIKEN)
Core-collapse
supernovae
Chair: T. Hatsuda(RIKEN)
Numerical
Relativity
Simulations of NS-NS binary merger
Core-collapse
supernovae

Progressof Relativity
algorithmsSimulations
in lattice gauge
simulations
Numericalof NS-NSbinary merger
Testing
SSOR
preconditioner
for
Domainwall/Overlap
normal equations
Progress of algorithms in lattice gauge simulations
Testing SSOR preconditioner for Domainwall/Overlap normal equations
Chair: H. Suzuki (Tokyo Sci.)
Numerical
to QED Sci.)
contribution in the lepton g-2
Chair: H. approach
Suzuki (Tokyo
Pion
form factors
in theepsilonregime in the lepton g-2
Numerical
approach
to QED
contribution
Mean-fieldcalculation
proton-neutron mixing in atomic nuclei --toward
Pion form factors
in theincluding
epsilon regime
proton-neutron
pairing--including proton-neutron mixing in atomic nuclei --toward
Mean-field calculation
Current
Status ofpairing-Massive Star Evolution
proton-neutronBlackhole-neutronstar merger
with neutrino cooling
Current
Status of Massive
Star Evolution
Black hole-neutron star merger with neutrino cooling

A03(Invited)
A04(Invited)

A04
A01 A01
A02
A03

Friday, December 14
Friday, December
14 IV
09:00-10:30
Session09:00-10:30
IV
09:00-09:50
Z.Session
Fodor (Wuppertal)
09:00-09:50
Z. Akiba
Fodor (RIKEN)(Wuppertal)
09:50-10:30
Y.
09:50-10:30
Y. Akiba (RIKEN)
10:30-11:00
Break
10:30-11:00
Break V
11:00-12:30
Session11:00-12:30
V
11:00-11:50
J.SessionCarlson (LANL)
11:00-11:50
J. Sakurai
Carlson (RIKEN/Tokyo)(LANL)
11:50-12:30
H.
11:50-12:30
H. Sakurai (RIKEN/Tokyo)
12:30-14:00
Lunch
12:30-14:00
Lunch VI
14:00-16:00
Session14:00-16:00
Session14:00-14:40
H.
Tamura VI(Tohoku)
14:00-14:40
H.Abe
Tamura(Tohoku)
14:40-15:10
T.
(Tokyo)14:40-15:10
T.
Abe(Tokyo)15:10-15:40
T. Doi (RIKEN)
15:10-15:40
T. TogashiDoi (RIKEN)
15:40-16:00
H.
(Waseda)15:40-16:00
H. Togashi (Waseda)
16:00-16:30
Break
16:00-16:30
Break VII
16:30-18:10
Session
16:30-18:10
SessionVII
16:30-16:50
G.
Cossu (KEK)
16:30-16:50
G.Inoue
Cossu(Nihon)(KEK)
16:50-17:10
T.
16:50-17:10
T.
Inoue(Nihon)17:10-17:30
S. Ejiri (Niigata)
17:10-17:30
S. Tsunoda
Ejiri (Niigata)17:30-17:50
Y.
(Tokyo)17:30-17:50
Y.
Tsunoda(Tokyo)
17:50-18:10
S. Wanajo (NAOJ)
17:50-18:10
S. Wanajo (NAOJ)
19:30Banquet
19:30Banquet

Chair: S. Hashimoto (KEK)
Chair: S. Hashimoto(KEK)
Computational
particle physics
Computational
particle physics
Quark-Gluon
PlasmaQuark-Gluon PlasmaA01(Invited)Exp

Chair: T. Nakatsukasa (RIKEN)
Chair: T. Nakatsukasa(RIKEN)
Computational
nuclear physics
Computational
Nuclearphysicsnuclear
at RIBFphysics
Nuclear physics at RIBF

A02(Invited)Exp

Chair: E. Hiyama (RIKEN)
Chair: E. Hiyama(RIKEN)
Strangenessnuclear physics
StrangenessnuclearNo-coreMonte
Carlophysics
shell model towards ab initio nuclear structure
No-coreMonte
Carlomodel towards ab initio nuclear structure
Hadron interactions onshell
the lattice
Hadron interactions
the lattice
Variational
Study of ona Nuclear
Equation of State for Core-Collapse Supernovae
Variational Study of a Nuclear Equation of State for Core-Collapse Supernovae

Exp

Chair: H. Matsufuru (KEK)
Chair:
H. Matsufuru
Finitetemperature
study(KEK)of axial symmetry on the lattice
Finite temperature
axial symmetry on the lattice
Neutronstars from study
LatticeofQCD
Neutronstars
fromLattice
QCD
Study of finite density lattice QCD by the histogram method
Study ofof medium-massfinite density latticeby the histogram
methodStudynucleiQCD
by large-scale
shell model
calculations
Studyofmedium-massnucleibylarge-scale
shell
model
calculations
r-process: supernovae vs. neutron star mergers
r-process: supernovae vs. neutron star mergers

A03

A02
A02
A03
A01
A01
A03

A02
A02

09:00-10:20
SessionSaturday,December
15 VIII

09:00-09:40
09:00-10:20
09:40-10:20
09:00-09:40
10:20-10:50
09:40-10:20
10:50-12:20
10:20-10:50
10:50-11:20
10:50-12:20
11:20-11:50
10:50-11:20
11:50-12:20
11:20-11:50
12:20-13:50
11:50-12:20
13:50-15:20
12:20-13:50
13:50-14:20
13:50-15:20
14:20-14:50
13:50-14:20
14:20-14:50
14:50-15:20

K. Makishima
Session
VIII (Tokyo/RIKEN)
T.Makishima
Iijima (Nagoya)
K.
(Tokyo/RIKEN)
BreakT. Iijima (Nagoya)
Session IX
BreakT. Yamazaki
Session
IX (Nagoya)
K.Yamazaki
Nagata (Hirosima)
T.
(Nagoya)
Y.Nagata
Suwa (YITP)K.
(Hirosima)
Lunch
Y.
Suwa (YITP)
Session X
Lunch
S.W. KimX(Osaka)
Session
S. Motoki
(KEK)
S.W.
Kim (Osaka)
S.A.Motoki(KEK)
Imakura(Tsukuba)

Chair: T. Oonogi (Osaka)
PhysicsT.and
Astrophysics
of Compact Stars
Chair:
Oonogi(Osaka)Hadronandspectroscopy
withofa Compact
variety ofStars
flavors
Physics
Astrophysics

Hadron spectroscopy with a variety of flavors
Chair: T. Doi (RIKEN)
Calculationof light
nuclei from lattice QCD
Chair:
T. Doi(RIKEN)
Finite density
latticenuclei
QCDfrom
at lowtemperature
Calculationof light
lattice
QCD
PhysicalIngredientsin Core-Collapse
Supernova Explosion Mechanism
Finitedensitylattice QCD
at low temperature

14:50-15:20
16:00-18:00
16:00-16:50
16:00-18:00
17:00-17:50
16:00-16:50
18:00-19:30
17:00-17:50

Physical Ingredients in Core-Collapse Supernova Explosion Mechanism
Chair: K. Sumiyoshi (Numazu)
Cosmologicalsolutions (Numazu)in the Lorentzian matrix model
Chair:
K. Sumiyoshi
Common codesolutions
system for
the Lorentzian
lattice QCDmatrix
simulations
Cosmologicalin themodel
Aparametertuningtechniqueofaweighted
Jacobi-type
Common code system for the lattice QCD simulations preconditioner and its
application to supernova simulations
A parameter tuning technique of a weighted Jacobi-type preconditioner and its
A.
ImakuraSession(Tsukuba)
SpecialChair: S. Aoki (Tsukuba)
application to supernova simulations
T. Maskawa(KMI, Nagoya Univ.) Chair:⌧௦♫఍࡜⛉ᏛSpecialSessionS. Aoki (Tsukuba)
T.Maskawa
Kobayashi(KMI,(Tokyo)͆ࣄࢵࢢࢫ⢏Ꮚ͇ࡢⓎぢ࡜௒ᚋࡢᒎᮃ
T.
Nagoya Univ.) ⌧௦♫఍࡜⛉Ꮫ࢖ࣥࣇ࢛࣮࣐࣑࣮ࣝࢸ࢕ࣥࢢ ఍㆟ᐊ ḟୡ௦䝅䝇䝔䝮ㄪᰝ᳨ウWG䛸䛾ពぢ஺᥮఍ (ཧຍ⮬⏤)T.
Kobayashi (Tokyo)͆ࣄࢵࢢࢫ⢏Ꮚ͇ࡢⓎぢ࡜௒ᚋࡢᒎᮃ

18:00-19:30

࢖ࣥࣇ࢛࣮࣐࣑࣮ࣝࢸ࢕ࣥࢢ ఍㆟ᐊ

Exp
Exp
A01
A01
A03
A01
A04
A04

ḟୡ௦䝅䝇䝔䝮ㄪᰝ᳨ウWG䛸䛾ពぢ஺᥮఍ (ཧຍ⮬⏤)Sunday, December 16
09:00-10:40
SessionSunday,December
16 XI

09:00-09:30
09:00-10:40
09:30-09:50
09:00-09:30
09:50-10:20
09:30-09:50
10:20-10:40
09:50-10:20
10:40-11:10
10:20-10:40
11:10-12:30
10:40-11:10
11:10-11:40
11:10-12:30
11:10-11:40
11:40-12:10

J. W. LeeXI(KEK)
SessionYamada(KEK)
J.N.W.
Lee (KEK)
M.Yamada
Kimura (KEK)(Hokkaido)N.
A. Kimura
Umeya (Hokkaido)
(NIT)
M.
Break
A.
Umeya (NIT)
Session XIIBreakK. Nakazato
SessionXII (Tokyo Sci.)
K.
(TokyoSci.)
K.Nakazato
Sumiyoshi(Numazu)

11:40-12:10
12:10-12:30
12:30-14:00
12:10-12:30
14:00-14:45
12:30-14:00
14:45-14:55
14:00-14:45
15:00
14:45-14:55

K.
(Numazu)
A.Sumiyoshi
Mizuta (KEK)
Lunch
A.
Mizuta (KEK)
Poster Award (3 talks)
Lunch
Closing
Address
PosterAward(3 talks)
AdjournAddress
Closing

15:00

Adjourn

Chair: S. Ejiri (Niigata)
Large Nc
theory and chiral random matrix theory
Chair:
S. gauge
Ejiri (Niigata)
Exploring
manytheory
flavorand
QCD
on thelatticematrix theory
Large
Nc gaugechiralrandom0RGLI\LQJDQG3URELQJ1XFOHDU6WUXFWXUHE\ȁ3DUWLFOH
Exploring
many flavor QCD on the lattice
Lambda Hypernuclei of He isotope with TOSM + UCOM0RGLI\LQJDQG3URELQJ1XFOHDU6WUXFWXUHE\ȁ3DUWLFOH

Lambda Hypernuclei of He isotope with TOSM + UCOM
Chair: K. Hashimoto (Osaka)
Stellar Core
Collapse andExotic Matter
Chair:
K. Hashimoto(Osaka)Numerical modeling of core-collapse supernovae with progress in nuclear physics andStellar Core Collapse and Exotic Mattersupercomputing
Numerical modeling of core-collapse supernovae with progress in nuclear physics and
Jet Opening angle of gamma-ray burst outflows
supercomputing
Jet Opening angle of gamma-ray burst outflows
Chair: S. Aoki (Tsukuba)
Chair: S. Aoki (Tsukuba)

A01
A01
A02
A02
A03
A03
A03

09:00-10:20
SessionSaturday,December
15 VIII

09:00-09:40
09:00-10:20
09:40-10:20
09:00-09:40
10:20-10:50
09:40-10:20
10:50-12:20
10:20-10:50
10:50-11:20
10:50-12:20
11:20-11:50
10:50-11:20
11:50-12:20
11:20-11:50
12:20-13:50
11:50-12:20
13:50-15:20
12:20-13:50
13:50-14:20
13:50-15:20
14:20-14:50
13:50-14:20
14:20-14:50
14:50-15:20

K. Makishima
Session
VIII (Tokyo/RIKEN)
T.Makishima
Iijima (Nagoya)
K.
(Tokyo/RIKEN)
BreakT. Iijima (Nagoya)
Session IX
BreakT. Yamazaki
Session
IX (Nagoya)
K.Yamazaki
Nagata (Hirosima)
T.
(Nagoya)
Y.Nagata
Suwa (YITP)K.
(Hirosima)
Lunch
Y.
Suwa (YITP)
Session X
Lunch
S.W. KimX(Osaka)
Session
S. Motoki
(KEK)
S.W.
Kim (Osaka)
S.A.Motoki(KEK)
Imakura(Tsukuba)

Chair: T. Oonogi (Osaka)
PhysicsT.and
Astrophysics
of Compact Stars
Chair:
Oonogi(Osaka)Hadronandspectroscopy
withofa Compact
variety ofStars
flavors
Physics
Astrophysics

Exp
Exp

Hadron spectroscopy with a variety of flavors
Chair: T. Doi (RIKEN)
Calculationof light
nuclei from lattice QCD
Chair:
T. Doi(RIKEN)
Finite density
latticenuclei
QCDfrom
at lowtemperature
Calculationof light
lattice
QCD
PhysicalIngredientsin Core-Collapse
Supernova Explosion Mechanism
Finitedensitylattice QCD
at low temperature

14:50-15:20
16:00-18:00
16:00-16:50
16:00-18:00
17:00-17:50
16:00-16:50
18:00-19:30
17:00-17:50

Physical Ingredients in Core-Collapse Supernova Explosion Mechanism
Chair: K. Sumiyoshi (Numazu)
Cosmologicalsolutions (Numazu)in the Lorentzian matrix model
Chair:
K. Sumiyoshi
Common codesolutions
system for
the Lorentzian
lattice QCDmatrix
simulations
Cosmologicalin themodel
Aparametertuningtechniqueofaweighted
Jacobi-type
Common code system for the lattice QCD simulations preconditioner and its
application to supernova simulations
A parameter tuning technique of a weighted Jacobi-type preconditioner and its
A.
ImakuraSession(Tsukuba)
SpecialChair: S. Aoki (Tsukuba)
application to supernova simulations
T. Maskawa(KMI, Nagoya Univ.) Chair:⌧௦♫఍࡜⛉ᏛSpecialSessionS. Aoki (Tsukuba)
T.Maskawa
Kobayashi(KMI,(Tokyo)͆ࣄࢵࢢࢫ⢏Ꮚ͇ࡢⓎぢ࡜௒ᚋࡢᒎᮃ
T.
Nagoya Univ.) ⌧௦♫఍࡜⛉Ꮫ࢖ࣥࣇ࢛࣮࣐࣑࣮ࣝࢸ࢕ࣥࢢ ఍㆟ᐊ ḟୡ௦䝅䝇䝔䝮ㄪᰝ᳨ウWG䛸䛾ពぢ஺᥮఍ (ཧຍ⮬⏤)T.
Kobayashi (Tokyo)͆ࣄࢵࢢࢫ⢏Ꮚ͇ࡢⓎぢ࡜௒ᚋࡢᒎᮃ

18:00-19:30

࢖ࣥࣇ࢛࣮࣐࣑࣮ࣝࢸ࢕ࣥࢢ ఍㆟ᐊ

A01
A01
A03
A01
A04
A04

ḟୡ௦䝅䝇䝔䝮ㄪᰝ᳨ウWG䛸䛾ពぢ஺᥮఍ (ཧຍ⮬⏤)Sunday, December 16
09:00-10:40
SessionSunday,December
16 XI

09:00-09:30
09:00-10:40
09:30-09:50
09:00-09:30
09:50-10:20
09:30-09:50
10:20-10:40
09:50-10:20
10:40-11:10
10:20-10:40
11:10-12:30
10:40-11:10
11:10-11:40
11:10-12:30
11:10-11:40
11:40-12:10

J. W. LeeXI(KEK)
SessionYamada(KEK)
J.N.W.
Lee (KEK)
M.Yamada
Kimura (KEK)(Hokkaido)N.
A. Kimura
Umeya (Hokkaido)
(NIT)
M.
Break
A.
Umeya (NIT)
Session XIIBreakK. Nakazato
SessionXII (Tokyo Sci.)
K.
(TokyoSci.)
K.Nakazato
Sumiyoshi(Numazu)

11:40-12:10
12:10-12:30
12:30-14:00
12:10-12:30
14:00-14:45
12:30-14:00
14:45-14:55
14:00-14:45
15:00
14:45-14:55

K.
(Numazu)
A.Sumiyoshi
Mizuta (KEK)
Lunch
A.
Mizuta (KEK)
Poster Award (3 talks)
Lunch
Closing
Address
PosterAward(3 talks)
AdjournAddress
Closing

15:00

Adjourn

Chair: S. Ejiri (Niigata)
Large Nc
theory and chiral random matrix theory
Chair:
S. gauge
Ejiri (Niigata)
Exploring
manytheory
flavorand
QCD
on thelatticematrix theory
Large
Nc gaugechiralrandom0RGLI\LQJDQG3URELQJ1XFOHDU6WUXFWXUHE\ȁ3DUWLFOH
Exploring
many flavor QCD on the lattice
Lambda Hypernuclei of He isotope with TOSM + UCOM0RGLI\LQJDQG3URELQJ1XFOHDU6WUXFWXUHE\ȁ3DUWLFOH

A01
A01
A02
A02

■会場■ 奈良県新公会堂（近鉄奈良駅から徒歩20分、JR奈良駅からバス停「大仏殿春日大社前」下車徒歩3分）
Lambda Hypernuclei of He isotope with TOSM + UCOM
Chair: K. Hashimoto (Osaka)
A03
Stellar Core
Collapse andExotic Matter
Chair:
K. Hashimoto(Osaka)Numerical modeling of core-collapse supernovae with progress in nuclear physics and
A03
Stellar Core Collapse and Exotic Mattersupercomputing
Numerical modeling of core-collapse supernovae with progress in nuclear physics and
Jet Opening angle of gamma-ray burst outflows
A03
supercomputing
Jet Opening angle of gamma-ray burst outflows
Chair: S. Aoki (Tsukuba)
至京都

至京都

奈良県文化会館

至
阪
奈
道
路

東大寺

国立美術館

南大門

奈良県庁

近鉄奈良駅

興福寺

国立博物館

至天理

Chair: S. Aoki (Tsukuba)

奈良公園

奈良県新公会堂
至
春
日
大
社
・
若
草
山

09:00-10:20
SessionSaturday,December
15 VIII

09:00-09:40
09:00-10:20
09:40-10:20
09:00-09:40
10:20-10:50
09:40-10:20
10:50-12:20
10:20-10:50
10:50-11:20
10:50-12:20
11:20-11:50
10:50-11:20
11:50-12:20
11:20-11:50
12:20-13:50
11:50-12:20
13:50-15:20
12:20-13:50
13:50-14:20
13:50-15:20
14:20-14:50
13:50-14:20
14:20-14:50
14:50-15:20

K. Makishima
Session
VIII (Tokyo/RIKEN)
T.Makishima
Iijima (Nagoya)
K.
(Tokyo/RIKEN)
BreakT. Iijima (Nagoya)
Session IX
BreakT. Yamazaki
Session
IX (Nagoya)
K.Yamazaki
Nagata (Hirosima)
T.
(Nagoya)
Y.Nagata
Suwa (YITP)K.
(Hirosima)
Lunch
Y.
Suwa (YITP)
Session X
Lunch
S.W. KimX(Osaka)
Session
S. Motoki
(KEK)
S.W.
Kim (Osaka)
S.A.Motoki(KEK)
Imakura(Tsukuba)

Chair: T. Oonogi (Osaka)
PhysicsT.and
Astrophysics
of Compact Stars
Chair:
Oonogi(Osaka)Hadronandspectroscopy
withofa Compact
variety ofStars
flavors
Physics
Astrophysics

Hadron spectroscopy with a variety of flavors
Chair: T. Doi (RIKEN)
Calculationof light
nuclei from lattice QCD
Chair:
T. Doi(RIKEN)
Finite density
latticenuclei
QCDfrom
at lowtemperature
Calculationof light
lattice
QCD
PhysicalIngredientsin Core-Collapse
Supernova Explosion Mechanism
Finitedensitylattice QCD
at low temperature

14:50-15:20
16:00-18:00
16:00-16:50
16:00-18:00
17:00-17:50
16:00-16:50
18:00-19:30
17:00-17:50

Physical Ingredients in Core-Collapse Supernova Explosion Mechanism
Chair: K. Sumiyoshi (Numazu)
Cosmologicalsolutions (Numazu)in the Lorentzian matrix model
Chair:
K. Sumiyoshi
Common codesolutions
system for
the Lorentzian
lattice QCDmatrix
simulations
Cosmologicalin themodel
Aparametertuningtechniqueofaweighted
Jacobi-type
Common code system for the lattice QCD simulations preconditioner and its
application to supernova simulations
A parameter tuning technique of a weighted Jacobi-type preconditioner and its
A.
ImakuraSession(Tsukuba)
SpecialChair: S. Aoki (Tsukuba)
application to supernova simulations
T. Maskawa(KMI, Nagoya Univ.) Chair:⌧௦♫఍࡜⛉ᏛSpecialSessionS. Aoki (Tsukuba)
T.Maskawa
Kobayashi(KMI,(Tokyo)͆ࣄࢵࢢࢫ⢏Ꮚ͇ࡢⓎぢ࡜௒ᚋࡢᒎᮃ
T.
Nagoya Univ.) ⌧௦♫఍࡜⛉Ꮫ࢖ࣥࣇ࢛࣮࣐࣑࣮ࣝࢸ࢕ࣥࢢ ఍㆟ᐊ ḟୡ௦䝅䝇䝔䝮ㄪᰝ᳨ウWG䛸䛾ពぢ஺᥮఍ (ཧຍ⮬⏤)T.
Kobayashi (Tokyo)͆ࣄࢵࢢࢫ⢏Ꮚ͇ࡢⓎぢ࡜௒ᚋࡢᒎᮃ

18:00-19:30

࢖ࣥࣇ࢛࣮࣐࣑࣮ࣝࢸ࢕ࣥࢢ ఍㆟ᐊ

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ḟୡ௦䝅䝇䝔䝮ㄪᰝ᳨ウWG䛸䛾ពぢ஺᥮఍ (ཧຍ⮬⏤)Sunday, December 16
09:00-10:40
SessionSunday,December
16 XI

09:00-09:30
09:00-10:40
09:30-09:50
09:00-09:30
09:50-10:20
09:30-09:50
10:20-10:40
09:50-10:20
10:40-11:10
10:20-10:40
11:10-12:30
10:40-11:10
11:10-11:40
11:10-12:30
11:10-11:40
11:40-12:10

J. W. LeeXI(KEK)
SessionYamada(KEK)
J.N.W.
Lee (KEK)
M.Yamada
Kimura (KEK)(Hokkaido)N.
A. Kimura
Umeya (Hokkaido)
(NIT)
M.
Break
A.
Umeya (NIT)
Session XIIBreakK. Nakazato
SessionXII (Tokyo Sci.)
K.
(TokyoSci.)
K.Nakazato
Sumiyoshi(Numazu)

11:40-12:10
12:10-12:30
12:30-14:00
12:10-12:30
14:00-14:45
12:30-14:00
14:45-14:55
14:00-14:45
15:00
14:45-14:55

K.
(Numazu)
A.Sumiyoshi
Mizuta (KEK)
Lunch
A.
Mizuta (KEK)
Poster Award (3 talks)
Lunch
Closing
Address
PosterAward(3 talks)
AdjournAddress
Closing

15:00

Adjourn

Chair: S. Ejiri (Niigata)
Large Nc
theory and chiral random matrix theory
Chair:
S. gauge
Ejiri (Niigata)
Exploring
manytheory
flavorand
QCD
on thelatticematrix theory
Large
Nc gaugechiralrandom0RGLI\LQJDQG3URELQJ1XFOHDU6WUXFWXUHE\ȁ3DUWLFOH
Exploring
many flavor QCD on the lattice
Lambda Hypernuclei of He isotope with TOSM + UCOM0RGLI\LQJDQG3URELQJ1XFOHDU6WUXFWXUHE\ȁ3DUWLFOH

Lambda Hypernuclei of He isotope with TOSM + UCOM
Chair: K. Hashimoto (Osaka)
Stellar Core
Collapse andExotic Matter
Chair:
K. Hashimoto(Osaka)Numerical modeling of core-collapse supernovae with progress in nuclear physics andStellar Core Collapse and Exotic Mattersupercomputing
Numerical modeling of core-collapse supernovae with progress in nuclear physics and
Jet Opening angle of gamma-ray burst outflows
supercomputing
Jet Opening angle of gamma-ray burst outflows
Chair: S. Aoki (Tsukuba)
Chair: S. Aoki (Tsukuba)

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09:00-10:20
SessionSaturday,December
15 VIII

09:00-09:40
09:00-10:20
09:40-10:20
09:00-09:40
10:20-10:50
09:40-10:20
10:50-12:20
10:20-10:50
10:50-11:20
10:50-12:20
11:20-11:50
10:50-11:20
11:50-12:20
11:20-11:50
12:20-13:50
11:50-12:20
13:50-15:20
12:20-13:50
13:50-14:20
13:50-15:20
14:20-14:50
13:50-14:20
14:20-14:50
14:50-15:20

K. Makishima
Session
VIII (Tokyo/RIKEN)
T.Makishima
Iijima (Nagoya)
K.
(Tokyo/RIKEN)
BreakT. Iijima (Nagoya)
Session IX
BreakT. Yamazaki
Session
IX (Nagoya)
K.Yamazaki
Nagata (Hirosima)
T.
(Nagoya)
Y.Nagata
Suwa (YITP)K.
(Hirosima)
Lunch
Y.
Suwa (YITP)
Session X
Lunch
S.W. KimX(Osaka)
Session
S. Motoki
(KEK)
S.W.
Kim (Osaka)
S.A.Motoki(KEK)
Imakura(Tsukuba)

Chair: T. Oonogi (Osaka)
PhysicsT.and
Astrophysics
of Compact Stars
Chair:
Oonogi(Osaka)Hadronandspectroscopy
withofa Compact
variety ofStars
flavors
Physics
Astrophysics

Hadron spectroscopy with a variety of flavors
Chair: T. Doi (RIKEN)
Calculationof light
nuclei from lattice QCD
Chair:
T. Doi(RIKEN)
Finite density
latticenuclei
QCDfrom
at lowtemperature
Calculationof light
lattice
QCD
PhysicalIngredientsin Core-Collapse
Supernova Explosion Mechanism
Finitedensitylattice QCD
at low temperature

14:50-15:20
16:00-18:00
16:00-16:50
16:00-18:00
17:00-17:50
16:00-16:50
18:00-19:30
17:00-17:50

Physical Ingredients in Core-Collapse Supernova Explosion Mechanism
Chair: K. Sumiyoshi (Numazu)
Cosmologicalsolutions (Numazu)in the Lorentzian matrix model
Chair:
K. Sumiyoshi
Common codesolutions
system for
the Lorentzian
lattice QCDmatrix
simulations
Cosmologicalin themodel
Aparametertuningtechniqueofaweighted
Jacobi-type
Common code system for the lattice QCD simulations preconditioner and its
application to supernova simulations
A parameter tuning technique of a weighted Jacobi-type preconditioner and its
A.
ImakuraSession(Tsukuba)
SpecialChair: S. Aoki (Tsukuba)
application to supernova simulations
T. Maskawa(KMI, Nagoya Univ.) Chair:⌧௦♫఍࡜⛉ᏛSpecialSessionS. Aoki (Tsukuba)
T.Maskawa
Kobayashi(KMI,(Tokyo)͆ࣄࢵࢢࢫ⢏Ꮚ͇ࡢⓎぢ࡜௒ᚋࡢᒎᮃ
T.
Nagoya Univ.) ⌧௦♫఍࡜⛉Ꮫ࢖ࣥࣇ࢛࣮࣐࣑࣮ࣝࢸ࢕ࣥࢢ ఍㆟ᐊ ḟୡ௦䝅䝇䝔䝮ㄪᰝ᳨ウWG䛸䛾ពぢ஺᥮఍ (ཧຍ⮬⏤)T.
Kobayashi (Tokyo)͆ࣄࢵࢢࢫ⢏Ꮚ͇ࡢⓎぢ࡜௒ᚋࡢᒎᮃ

18:00-19:30

࢖ࣥࣇ࢛࣮࣐࣑࣮ࣝࢸ࢕ࣥࢢ ఍㆟ᐊ

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ḟୡ௦䝅䝇䝔䝮ㄪᰝ᳨ウWG䛸䛾ពぢ஺᥮఍ (ཧຍ⮬⏤)Sunday, December 16
09:00-10:40
SessionSunday,December
16 XI

09:00-09:30
09:00-10:40
09:30-09:50
09:00-09:30
09:50-10:20
09:30-09:50
10:20-10:40
09:50-10:20
10:40-11:10
10:20-10:40
11:10-12:30
10:40-11:10
11:10-11:40
11:10-12:30
11:10-11:40
11:40-12:10

J. W. LeeXI(KEK)
SessionYamada(KEK)
J.N.W.
Lee (KEK)
M.Yamada
Kimura (KEK)(Hokkaido)N.
A. Kimura
Umeya (Hokkaido)
(NIT)
M.
Break
A.
Umeya (NIT)
Session XIIBreakK. Nakazato
SessionXII (Tokyo Sci.)
K.
(TokyoSci.)
K.Nakazato
Sumiyoshi(Numazu)

11:40-12:10
12:10-12:30
12:30-14:00
12:10-12:30
14:00-14:45
12:30-14:00
14:45-14:55
14:00-14:45
15:00
14:45-14:55

K.
(Numazu)
A.Sumiyoshi
Mizuta (KEK)
Lunch
A.
Mizuta (KEK)
Poster Award (3 talks)
Lunch
Closing
Address
PosterAward(3 talks)
AdjournAddress
Closing

15:00

Adjourn

Chair: S. Ejiri (Niigata)
Large Nc
theory and chiral random matrix theory
Chair:
S. gauge
Ejiri (Niigata)
Exploring
manytheory
flavorand
QCD
on thelatticematrix theory
Large
Nc gaugechiralrandom0RGLI\LQJDQG3URELQJ1XFOHDU6WUXFWXUHE\ȁ3DUWLFOH
Exploring
many flavor QCD on the lattice
Lambda Hypernuclei of He isotope with TOSM + UCOM0RGLI\LQJDQG3URELQJ1XFOHDU6WUXFWXUHE\ȁ3DUWLFOH

Lambda Hypernuclei of He isotope with TOSM + UCOM
Chair: K. Hashimoto (Osaka)
Stellar Core
Collapse andExotic Matter
Chair:
K. Hashimoto(Osaka)Numerical modeling of core-collapse supernovae with progress in nuclear physics andStellar Core Collapse and Exotic Mattersupercomputing
Numerical modeling of core-collapse supernovae with progress in nuclear physics and
Jet Opening angle of gamma-ray burst outflows
supercomputing
Jet Opening angle of gamma-ray burst outflows
Chair: S. Aoki (Tsukuba)
Chair: S. Aoki (Tsukuba)

Enjoy the symposium. Thank you.

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