Neutron stars, supernova explosions and the transition to quark matter

被引：0

作者：

Drago, A ^{[1
]}

机构：

[1] Univ Ferrara, Dipartmento Fis, I-44100 Ferrara, Italy

[2] Ist Nazl Fis Nucl, Sezione Ferrara, I-44100 Ferrara, Italy

来源：

NUCLEAR PHYSICS A | 1999年 / 661卷

关键词：

D O I：

10.1016/S0375-9474(99)00537-0

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

The structure of a hybrid star is discussed using both the MIT bag model and the Color Dielectric Model to describe the quark matter phase. A finite temperature equation of state is introduced to discuss the possibility that the transition to quark matter takes place during the pre-supernova collapse.

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页码：633C / 636C

页数：4

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