Excluded volume effects on cold neutron star phenomenology

IF 1.7 4区 物理与天体物理 Q2 PHYSICS, NUCLEAR Nuclear Physics A Pub Date : 2024-07-10 DOI:10.1016/j.nuclphysa.2024.122928
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Abstract

Observable properties of neutron stars are studied within a hadronic equation of state derived from the quark level. The effect of short-range repulsion is incorporated within the excluded volume framework. It is found that one can sustain neutron stars with masses as large as 2.2M even including hyperons in β equilibrium, while producing radii and tidal deformabilities consistent with current constraints.

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冷中子星现象学的排除体积效应
在从夸克水平导出的强子状态方程中研究了中子星的可观测特性。短程斥力的影响被纳入了排除体积框架。研究发现,我们可以维持质量高达 2.2M⊙ 的中子星,甚至包括处于 β 平衡的超子,同时产生与当前约束相一致的半径和潮汐变形。
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来源期刊
Nuclear Physics A
Nuclear Physics A 物理-物理:核物理
CiteScore
3.60
自引率
7.10%
发文量
113
审稿时长
61 days
期刊介绍: Nuclear Physics A focuses on the domain of nuclear and hadronic physics and includes the following subsections: Nuclear Structure and Dynamics; Intermediate and High Energy Heavy Ion Physics; Hadronic Physics; Electromagnetic and Weak Interactions; Nuclear Astrophysics. The emphasis is on original research papers. A number of carefully selected and reviewed conference proceedings are published as an integral part of the journal.
期刊最新文献
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