Do hyperons exist in the interior of neutron stars?

被引：181
作者：
Chatterjee, Debarati [1 ,2 ]
Vidana, Isaac [3 ]
机构：
[1] Univ Paris Diderot, CNRS, Observ Paris, LUTH, 5 Pl Jules Janssen, F-92190 Meudon, France
[2] ENSICAEN, Lab Phys Corpusculaire, 6 Blvd Marechal Juin, F-14050 Caen, France
[3] Univ Coimbra, Dept Phys, CFisUC, Rua Larga S-N, P-3004516 Coimbra, Portugal
来源：
EUROPEAN PHYSICAL JOURNAL A | 2016年 / 52卷 / 02期
关键词：
EQUATION-OF-STATE; LAMBDA LAMBDA-HYPERNUCLEI; MONTE-CARLO CALCULATIONS; NUCLEON INTERACTION; BULK VISCOSITY; QUARK MATTER; DENSE MATTER; FIELD THEORY; MASS; PULSAR;
D O I：
10.1140/epja/i2016-16029-x
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：
In this work we review the role of hyperons on the properties of neutron and proto-neutron stars. In particular, we revise the so-called "hyperon puzzle", go over some of the solutions proposed to tackle it, and discuss the implications that the recent measurements of unusually high neutron star masses have on our present knowledge of hypernuclear physics. We re-examine also the role of hyperons on the cooling properties of newly born neutron stars and on the so-called r-mode instability.
引用
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页码：1 / 18
页数：18
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