Ashadul Halder, Shibaji Banerjee, S. Ghosh, S. Raha
{"title":"旋转夸克星的钱德拉塞卡极限","authors":"Ashadul Halder, Shibaji Banerjee, S. Ghosh, S. Raha","doi":"10.1103/PHYSREVC.103.035806","DOIUrl":null,"url":null,"abstract":"The limiting mass is a significant characteristic for compact exotic stars including quark stars and can be expressed in terms of fundamental constants and the Bag constant. In the present work, using bag model description, maximum mass of a rotating quark star is found to depend on the rotational frequency apart from other fundamental parameters. The analytical results obtained agrees with the result of several relevant numerical estimates as well as observational evidences.","PeriodicalId":8437,"journal":{"name":"arXiv: High Energy Astrophysical Phenomena","volume":"109 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2020-05-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Chandrasekhar limit for rotating quark stars\",\"authors\":\"Ashadul Halder, Shibaji Banerjee, S. Ghosh, S. Raha\",\"doi\":\"10.1103/PHYSREVC.103.035806\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The limiting mass is a significant characteristic for compact exotic stars including quark stars and can be expressed in terms of fundamental constants and the Bag constant. In the present work, using bag model description, maximum mass of a rotating quark star is found to depend on the rotational frequency apart from other fundamental parameters. The analytical results obtained agrees with the result of several relevant numerical estimates as well as observational evidences.\",\"PeriodicalId\":8437,\"journal\":{\"name\":\"arXiv: High Energy Astrophysical Phenomena\",\"volume\":\"109 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2020-05-29\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv: High Energy Astrophysical Phenomena\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1103/PHYSREVC.103.035806\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv: High Energy Astrophysical Phenomena","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1103/PHYSREVC.103.035806","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The limiting mass is a significant characteristic for compact exotic stars including quark stars and can be expressed in terms of fundamental constants and the Bag constant. In the present work, using bag model description, maximum mass of a rotating quark star is found to depend on the rotational frequency apart from other fundamental parameters. The analytical results obtained agrees with the result of several relevant numerical estimates as well as observational evidences.
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