重力崩壊型超新星およびコンパクト天体形成に関する研究会(3/19-21)


国際研究集会:Physics of Core-Collapse Supernovae and Compact Star Formations

日時:2018年3月19日〜21日
場所:早稲田大学西早稲田キャンパス
ホームページ:http://www.heap.phys.waseda.ac.jp/Conference_waseda_2018/about.html

Aim of Workshop

The aim of this workshop is to gather the latest knowledge on both macro- and microphysics
of relevance for core-collapse supernova explosions and ensuing compact-star formations.
It has been already some time since spatially 3-dimensional supernova simulations became
feasible and these days numerical schemes are getting more sophisticated and microphysics
incorporated in simulations are being scrutinized. In the wake of the first detection of
a neutron star merger via gravitational waves, on the other hand, interest in the equation
of state of hot and dense hadronic matter is very high. In this workshop we invite leading
researchers on the topics listed below and discuss the latest issues in a broad context of
compact-star formations.

Topics

EOS of hot and dense hadronic matter relevant for core-collapse supernovae and proto neutron stars
Supernova simulations with multi-dimensional neutrino transport
Weak interactions and neutrino emissions in core-collapse supernovae and proto neutron star cooling
Neutrino oscillations in core-collapse supernova cores and proto neutron stars
Neutron star mergers: gravitational waves, EOS and nucleosynthesis

Invited Speakers

Luca Baiotti (Osaka univ.)
Jinniu Hu (Nankai Univ.)
Oliver Just (RIKEN)
Jonas Lippuner (LANL)
David Radice (Princeton Univ.)
Luke F. Roberts (Michigan State Univ.)
Yu-ichiro Sekiguchi (Toho Univ.)
Hong Shen (Nankai Univ.)
Atsushi Tamii (Osaka Univ.)
Stefan Typel (GSI)
Maria C. Volpe (ACP)
Remco Zeger (NSCL)

Important dates

The deadline for contribution talks and travel supports: 19, February, 2018
The deadline for poster presentations and only admission (including banquet): 28, February, 2018
Workshop: 19-21, March, 2018

Organizers

山田章一、加藤ちなみ(早稲田大学)、長倉洋樹(Caltech)、住吉光介(沼津高専)

Sponsors

科研費基盤B「多次元一般相対論的輻射流体力学シミュレーションによる超新星爆発の研究」
新学術領域「重力波物理学・天文学:創世記」”Studying supernova explosions via their neutrino emissions”
科研費基盤C「6次元ボルツマン方程式により探る多次元超新星爆発メカニズム」

Supported by

計算基礎科学連携拠点(JICFuS)
ポスト「京」重点課題9「宇宙の基本法則と進化の解明」

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