New equations of state constrained by nuclear physics, observations, and QCD calculations of high-density nuclear matter

被引：61

作者：

Huth, S. ^{[1
,2
]}

Wellenhofer, C. ^{[1
,2
]}

Schwenk, A. ^{[1
,2
,3
]}

机构：

[1] Tech Univ Darmstadt, Dept Phys, D-64289 Darmstadt, Germany

[2] GSI Helmholtzzentrum Schwerionenforsch GmbH, ExtreMe Matter Inst EMMI, D-64291 Darmstadt, Germany

[3] Max Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany

来源：

PHYSICAL REVIEW C | 2021年 / 103卷 / 02期

基金：

美国国家科学基金会;

关键词：

MULTI-MESSENGER OBSERVATIONS; NEUTRON-STAR; OF-STATE; MAXIMUM MASS; NICER VIEW; SUPERNOVA; ENERGY; HOT;

D O I：

10.1103/PhysRevC.103.025803

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 present new equations of state for applications in core-collapse supernova and neutron star merger simulations. We start by introducing an effective mass parametrization that is fit to recent microscopic calculations up to twice saturation density. This is important to capture the predicted thermal effects, which have been shown to determine the proto-neutron star contraction in supernova simulations. The parameter range of the energy-density functional underlying the equation of state is constrained by chiral effective field theory results at nuclear densities as well as by functional renormalization group computations at high densities based on QCD. We further implement observational constraints from measurements of heavy neutron stars, the gravitational wave signal of GW170817, and from the recent NICER results. Finally, we study the resulting allowed ranges for the equation of state and for properties of neutron stars, including the predicted ranges for the neutron star radius and maximum mass.

引用

页数：19

共 91 条

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