CONSTRAINTS ON THE NUCLEAR EOS FROM NEUTRON STAR OBSERVABLES

被引：2

作者：

Blaschke, D. ^{[1
,2
]}

Klahn, T. ^{[3
]}

Weber, F. ^{[4
]}

机构：

[1] Uniwersytet Wroclawski, Inst Fizyki Teoretycznej, Pl M Borna 9, PL-50204 Wroclaw, Poland

[2] JINR, Bogoliubov Lab Theoret Phys, Dubna 141980, Russia

[3] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA

[4] San Diego State Univ, Dept Phys, San Diego, CA 92182 USA

来源：

ASTRONOMY AND RELATIVISTIC ASTROPHYSICS: NEW PHENOMENA AND NEW STATES OF MATTER IN THE UNIVERSE (IWARA07) | 2010年

基金：

美国国家科学基金会;

关键词：

Nuclear matter; quark matter; equation of state; neutron stars; pulsars; EQUATION-OF-STATE; QUARK MATTER; 1122; HZ; STRANGE STARS; DENSE MATTER; OSCILLATIONS; MASS; INERTIA; PHYSICS; MOMENT;

D O I：

10.1142/9789814304887_0003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Depending on the density reached in the cores of neutron stars, such objects may contain stable phases of novel matter found nowhere else in the Universe. This article gives a brief overview of these phases of matter and discusses astrophysical constraints on the high-density equation of state associated with ultra-dense nuclear matter.

引用

页码：31 / 46

页数：16

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