{"title":"紧凑型恒星中的暗物质","authors":"Joseph Bramante , Nirmal Raj","doi":"10.1016/j.physrep.2023.12.001","DOIUrl":null,"url":null,"abstract":"<div><p><span><span>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 </span>fermion degeneracies, low temperatures, </span>nucleon<span><span> superfluidity, strong magnetic fields, high rotational regularity, and significant </span>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.</span></p></div>","PeriodicalId":404,"journal":{"name":"Physics Reports","volume":"1052 ","pages":"Pages 1-48"},"PeriodicalIF":23.9000,"publicationDate":"2023-12-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"4","resultStr":"{\"title\":\"Dark matter in compact stars\",\"authors\":\"Joseph Bramante , Nirmal Raj\",\"doi\":\"10.1016/j.physrep.2023.12.001\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p><span><span>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 </span>fermion degeneracies, low temperatures, </span>nucleon<span><span> superfluidity, strong magnetic fields, high rotational regularity, and significant </span>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.</span></p></div>\",\"PeriodicalId\":404,\"journal\":{\"name\":\"Physics Reports\",\"volume\":\"1052 \",\"pages\":\"Pages 1-48\"},\"PeriodicalIF\":23.9000,\"publicationDate\":\"2023-12-08\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"4\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physics Reports\",\"FirstCategoryId\":\"4\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0370157323004064\",\"RegionNum\":1,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"PHYSICS, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics Reports","FirstCategoryId":"4","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0370157323004064","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
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.
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.
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