Neutrino trapping effects on β-stable neutron star matter

被引：4

作者：

Vidaña, I

Bombaci, I

Polls, A

Ramos, A

机构：

[1] Univ Pisa, Dipartimento Fis Enrico Fermi, I-56127 Pisa, Italy

[2] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy

[3] Univ Barcelona, Dept Estructura & Constituents Mat, E-08028 Barcelona, Spain

来源：

NUCLEAR PHYSICS A | 2003年 / 719卷

关键词：

D O I：

10.1016/S0375-9474(03)00913-8

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：

We investigate in the framework of the Brueckner-Hartree-Fock approximation, the influence of neutrino trapping on the composition, equation of state, and structure of neutron stars immediately after birth. We explore also the consequences of neutrino trapping on the early evolution of a neutron star and on the final remnant left by the supernova explosion.

引用

页码：173C / 176C

页数：4

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