{"title":"有暗物质的德西特时空中的强宇宙审查","authors":"Shun Jiang , Jie Jiang","doi":"10.1016/j.physletb.2024.139035","DOIUrl":null,"url":null,"abstract":"<div><div>After imposing the weak energy condition on dark matter, we find that even in the absence of charge, a spherically symmetric de Sitter black hole with perfect fluid dark matter may still possess a Cauchy horizon. This paper investigates the stability of the Cauchy horizon in such a black hole under perturbations from a massless scalar field. Through numerical calculations of the massless scalar field's quasinormal modes, we discover that in this spacetime, when the black hole approaches extremality, i.e., when the dark-matter parameter <em>b</em> approaches its maximum value <span><math><msub><mrow><mi>b</mi></mrow><mrow><mtext>max</mtext></mrow></msub></math></span>, the Strong Cosmic Censorship (SCC) conjecture may be violated. This is the first instance of classical SCC violation observed in a spherically symmetric, uncharged black hole. Additionally, we explore the region of SCC violation within the parameter space <span><math><mi>Λ</mi><msup><mrow><mi>M</mi></mrow><mrow><mn>2</mn></mrow></msup><mo>−</mo><mi>b</mi><mo>/</mo><msub><mrow><mi>b</mi></mrow><mrow><mtext>max</mtext></mrow></msub></math></span>. Our findings indicate that as the cosmological constant increases, the violation region initially expands and then contracts.</div></div>","PeriodicalId":20162,"journal":{"name":"Physics Letters B","volume":"858 ","pages":"Article 139035"},"PeriodicalIF":4.3000,"publicationDate":"2024-09-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S0370269324005938/pdfft?md5=b3eaf78f97227f31e303e42123618dca&pid=1-s2.0-S0370269324005938-main.pdf","citationCount":"0","resultStr":"{\"title\":\"Strong cosmic censorship in de Sitter spacetimes with dark matter\",\"authors\":\"Shun Jiang , Jie Jiang\",\"doi\":\"10.1016/j.physletb.2024.139035\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>After imposing the weak energy condition on dark matter, we find that even in the absence of charge, a spherically symmetric de Sitter black hole with perfect fluid dark matter may still possess a Cauchy horizon. This paper investigates the stability of the Cauchy horizon in such a black hole under perturbations from a massless scalar field. Through numerical calculations of the massless scalar field's quasinormal modes, we discover that in this spacetime, when the black hole approaches extremality, i.e., when the dark-matter parameter <em>b</em> approaches its maximum value <span><math><msub><mrow><mi>b</mi></mrow><mrow><mtext>max</mtext></mrow></msub></math></span>, the Strong Cosmic Censorship (SCC) conjecture may be violated. This is the first instance of classical SCC violation observed in a spherically symmetric, uncharged black hole. Additionally, we explore the region of SCC violation within the parameter space <span><math><mi>Λ</mi><msup><mrow><mi>M</mi></mrow><mrow><mn>2</mn></mrow></msup><mo>−</mo><mi>b</mi><mo>/</mo><msub><mrow><mi>b</mi></mrow><mrow><mtext>max</mtext></mrow></msub></math></span>. Our findings indicate that as the cosmological constant increases, the violation region initially expands and then contracts.</div></div>\",\"PeriodicalId\":20162,\"journal\":{\"name\":\"Physics Letters B\",\"volume\":\"858 \",\"pages\":\"Article 139035\"},\"PeriodicalIF\":4.3000,\"publicationDate\":\"2024-09-20\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://www.sciencedirect.com/science/article/pii/S0370269324005938/pdfft?md5=b3eaf78f97227f31e303e42123618dca&pid=1-s2.0-S0370269324005938-main.pdf\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physics Letters B\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0370269324005938\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics Letters B","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0370269324005938","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Strong cosmic censorship in de Sitter spacetimes with dark matter
After imposing the weak energy condition on dark matter, we find that even in the absence of charge, a spherically symmetric de Sitter black hole with perfect fluid dark matter may still possess a Cauchy horizon. This paper investigates the stability of the Cauchy horizon in such a black hole under perturbations from a massless scalar field. Through numerical calculations of the massless scalar field's quasinormal modes, we discover that in this spacetime, when the black hole approaches extremality, i.e., when the dark-matter parameter b approaches its maximum value , the Strong Cosmic Censorship (SCC) conjecture may be violated. This is the first instance of classical SCC violation observed in a spherically symmetric, uncharged black hole. Additionally, we explore the region of SCC violation within the parameter space . Our findings indicate that as the cosmological constant increases, the violation region initially expands and then contracts.
期刊介绍:
Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.