Cool dense matter and neutron star phenomenology

被引：0
|
作者：
Reddy, S. [1 ]
Steiner, A. W. [1 ]
机构：
[1] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA
来源：
NUCLEAR PHYSICS A | 2007年 / 785卷 / 1-2期
关键词：
D O I：
10.1016/j.nuclphysa.2006.11.130
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：
Neutron star observations offer a novel approach to exploring Quantum Chromodynamics (QCD) at high densities and low temperatures. We discuss how the physics of QCD affects the structure and evolution of neutron stars, paying particular attention to heterogeneous phases, quark matter, and neutrino transport. Afterwards, we discuss the status of several types of neutron star observations and what they mean for the physics of dense matter. © 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码：24C / 35C
页数：12
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