Equations of state for supernovae and compact stars

被引：904

作者：

Oertel, M. ^{[1
]}

Hempel, M. ^{[2
]}

Klahn, T. ^{[3
]}

Typel, S. ^{[4
,5
]}

机构：

[1] Univ Paris Diderot, PSL Res Univ, Sorbonne Paris Cite, Lab Univ & Theories,CNRS,Observ Paris, 5 Pl Jules Janssen, F-92195 Meudon, France

[2] Univ Basel, Dept Phys, Klingelbergstr 82, CH-4056 Basel, Switzerland

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

[4] Tech Univ Darmstadt, Inst Kernphys, Schlossgartenstr 9, D-64289 Darmstadt, Germany

[5] GSI Helmholtzzentrum Schwerionenforsch, Planckstr 1, D-64291 Darmstadt, Germany

来源：

REVIEWS OF MODERN PHYSICS | 2017年 / 89卷 / 01期

基金：

瑞士国家科学基金会;

关键词：

NUCLEAR SYMMETRY ENERGY; EFFECTIVE-FIELD THEORY; HEAVY-ION COLLISIONS; SELF-CONSISTENT CALCULATIONS; CORE-COLLAPSE SUPERNOVAE; BLACK-HOLE FORMATION; MONTE-CARLO CALCULATIONS; NEUTRON SKIN THICKNESS; GAS PHASE-TRANSITION; GAUGE VECTOR-MESONS;

D O I：

10.1103/RevModPhys.89.015007

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A review is given of various theoretical approaches for the equation of state (EoS) of dense matter, relevant for the description of core-collapse supernovae, compact stars, and compact star mergers. The emphasis is put on models that are applicable to all of these scenarios. Such EoS models have to cover large ranges in baryon number density, temperature, and isospin asymmetry. The characteristics of matter change dramatically within these ranges, from a mixture of nucleons, nuclei, and electrons to uniform, strongly interacting matter containing nucleons, and possibly other particles such as hyperons or quarks. As the development of an EoS requires joint efforts from many directions, different theoretical approaches are considered and relevant experimental and observational constraints which provide insights for future research are discussed. Finally, results from applications of the discussed EoS models are summarized.

引用

页数：68

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