Systematic long term simulations of spherical supernova explosions and their applications

Hideto Kikuchi; Hideyuki Suzuki; Ken'ichiro Nakazato; Shoichi Yamada; Kohsuke Sumiyoshi

doi:10.1063/1.4763432

Systematic long term simulations of spherical supernova explosions and their applications

Hideto Kikuchi^*, Hideyuki Suzuki, Ken'ichiro Nakazato, Shoichi Yamada, Kohsuke Sumiyoshi

^*Corresponding author for this work

School of Advanced Science and Engineering

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

Most of the sophisticated numerical simulations of the collapse-driven supernova explosions are performed until 1-2 seconds after bounce. On the other hand, we caluclate long term evolution of supernovae using spherical symmetric models and approximate neutrino transfer. We applied this scheme to the systematic study on evaluation of explosion energy E_exp.

Original language	English
Title of host publication	Origin of Matter and Evolution of Galaxies 2011
Pages	397-399
Number of pages	3
DOIs	https://doi.org/10.1063/1.4763432
Publication status	Published - 2012
Event	International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, Japan Duration: 2011 Nov 14 → 2011 Nov 17

Publication series

Name	AIP Conference Proceedings
Volume	1484
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Conference

Conference	International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
Country/Territory	Japan
City	Wako
Period	11/11/14 → 11/11/17

Keywords

explosion energy
neutrinos
supernovae

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1063/1.4763432

Cite this

Kikuchi, H, Suzuki, H, Nakazato, K, Yamada, S & Sumiyoshi, K 2012, Systematic long term simulations of spherical supernova explosions and their applications. in Origin of Matter and Evolution of Galaxies 2011. AIP Conference Proceedings, vol. 1484, pp. 397-399, International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011, Wako, Japan, 11/11/14. https://doi.org/10.1063/1.4763432

@inproceedings{82892bd691a84470b30c33ef3c0bd30a,

title = "Systematic long term simulations of spherical supernova explosions and their applications",

abstract = "Most of the sophisticated numerical simulations of the collapse-driven supernova explosions are performed until 1-2 seconds after bounce. On the other hand, we caluclate long term evolution of supernovae using spherical symmetric models and approximate neutrino transfer. We applied this scheme to the systematic study on evaluation of explosion energy Eexp.",

keywords = "explosion energy, neutrinos, supernovae",

author = "Hideto Kikuchi and Hideyuki Suzuki and Ken'ichiro Nakazato and Shoichi Yamada and Kohsuke Sumiyoshi",

year = "2012",

doi = "10.1063/1.4763432",

language = "English",

isbn = "9780735410961",

series = "AIP Conference Proceedings",

pages = "397--399",

booktitle = "Origin of Matter and Evolution of Galaxies 2011",

note = "International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 ; Conference date: 14-11-2011 Through 17-11-2011",

}

TY - GEN

T1 - Systematic long term simulations of spherical supernova explosions and their applications

AU - Kikuchi, Hideto

AU - Suzuki, Hideyuki

AU - Nakazato, Ken'ichiro

AU - Yamada, Shoichi

AU - Sumiyoshi, Kohsuke

PY - 2012

Y1 - 2012

N2 - Most of the sophisticated numerical simulations of the collapse-driven supernova explosions are performed until 1-2 seconds after bounce. On the other hand, we caluclate long term evolution of supernovae using spherical symmetric models and approximate neutrino transfer. We applied this scheme to the systematic study on evaluation of explosion energy Eexp.

AB - Most of the sophisticated numerical simulations of the collapse-driven supernova explosions are performed until 1-2 seconds after bounce. On the other hand, we caluclate long term evolution of supernovae using spherical symmetric models and approximate neutrino transfer. We applied this scheme to the systematic study on evaluation of explosion energy Eexp.

KW - explosion energy

KW - neutrinos

KW - supernovae

UR - http://www.scopus.com/inward/record.url?scp=84874523909&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84874523909&partnerID=8YFLogxK

U2 - 10.1063/1.4763432

DO - 10.1063/1.4763432

M3 - Conference contribution

AN - SCOPUS:84874523909

SN - 9780735410961

T3 - AIP Conference Proceedings

SP - 397

EP - 399

BT - Origin of Matter and Evolution of Galaxies 2011

T2 - International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011

Y2 - 14 November 2011 through 17 November 2011

ER -

Systematic long term simulations of spherical supernova explosions and their applications

Abstract

Publication series

Conference

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this