Stellar collapse with hadron-quark phase transition of hot and dense matter

Ken'ichiro Nakazato, Kohsuke Sumiyoshi, Shoichi Yamada

研究成果: Article査読

抄録

We construct an equation of state (EOS) including the hadron-quark phase transition by the Gibbs conditions for finite temperature. We adopt the EOS based on the relativistic mean field theory for the hadronic phase and the MIT bag model of the deconfined 3-flavor strange quark matter for the quark phase. Moreover, the gravitational collapse of massive stars with several masses is computed using our EOS and we find that the phase transition makes the interval time from the bounce to the black hole formation, namely the duration time of the neutrino emission, shorter for the model with a bounce. This fact implies that we may be able to probe observationally the EOS of hot and dense matter in future.

本文言語English
ページ(範囲)76-79
ページ数4
ジャーナルProgress of Theoretical Physics Supplement
174
DOI
出版ステータスPublished - 2008

ASJC Scopus subject areas

  • 物理学および天文学(その他)

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