研究者情報 | 神奈川大学

ヒラノ　シンゴ Hirano Shingo 平野　信吾所属神奈川大学工学部応用物理学科職種助教
言語種別	英語
発行・発表の年月	2012/12
形態種別	学術雑誌
査読	査読あり
標題	WEAKLY INTERACTING MASSIVE PARTICLE DARK MATTER AND FIRST STARS: SUPPRESSION OF FRAGMENTATION IN PRIMORDIAL STAR FORMATION
執筆形態	共著
掲載誌名	ASTROPHYSICAL JOURNAL
出版社・発行元	IOP PUBLISHING LTD
巻・号・頁	761(2),pp.154-167
国際共著	国際共著
著者・共著者	◎Rowan J. Smith,Fabio Iocco,Simon C. O. Glover,Dominik R. G. Schleicher,Ralf S. Klessen,Shingo Hirano,Naoki Yoshida
概要	We present the first three-dimensional simulations to include the effects of dark matter annihilation feedback during the collapse of primordial minihalos. We begin our simulations from cosmological initial conditions and account for dark matter annihilation in our treatment of the chemical and thermal evolution of the gas. The dark matter is modeled using an analytical density profile that responds to changes in the peak gas density. We find that the gas can collapse to high densities despite the additional energy input from the dark matter.
DOI	10.1088/0004-637X/761/2/154
ISSN	0004-637X
ORCIDのPut Code	31843103
PermalinkURL	http://orcid.org/0000-0002-4317-767X