紧凑型恒星中的暗物质

IF 23.9 1区物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY

Physics Reports Pub Date : 2023-12-08 DOI:10.1016/j.physrep.2023.12.001

Joseph Bramante , Nirmal Raj

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引用次数: 4

摘要

在寻找暗物质的过程中，WD 和中子星是意义深远的多面实验室。我们回顾了对类波、微粒、宏观和黑洞暗物质的探测前景，这些暗物质利用了紧凑星的一些特殊性质，如超高密度、深度费米子退行性、低温、核子超流、强磁场、高旋转规则性和显著的引力波发射率。本文件首次明确提出的基础课题包括 "推进器阶段 "对中子星重子吸积的影响，以及奥杰和库珀对断裂效应对中子星暗物质俘获加热的贡献。

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Dark matter in compact stars

WDs and neutron stars are far-reaching and multi-faceted laboratories in the hunt for dark matter. We review detection prospects of wave-like, particulate, macroscopic and black hole dark matter that make use of several exceptional properties of compact stars, such as ultra-high densities, deep fermion degeneracies, low temperatures, nucleon superfluidity, strong magnetic fields, high rotational regularity, and significant gravitational wave emissivity. Foundational topics first made explicit in this document include the effect of the “propellor phase” on neutron star baryonic accretion, and the contribution of Auger and Cooper pair breaking effects to neutron star heating by dark matter capture.

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来源期刊

Physics Reports 物理-物理：综合

CiteScore

56.10

自引率

0.70%

发文量

102

审稿时长

9.1 weeks

期刊介绍： Physics Reports keeps the active physicist up-to-date on developments in a wide range of topics by publishing timely reviews which are more extensive than just literature surveys but normally less than a full monograph. Each report deals with one specific subject and is generally published in a separate volume. These reviews are specialist in nature but contain enough introductory material to make the main points intelligible to a non-specialist. The reader will not only be able to distinguish important developments and trends in physics but will also find a sufficient number of references to the original literature.