Amos V. Mathias, Jefta M. Sunzu, Jason M. Mkenyeleye
{"title":"具有玻色-爱因斯坦凝聚态内核和多向性包层的卡玛卡尔机制相对论星体","authors":"Amos V. Mathias, Jefta M. Sunzu, Jason M. Mkenyeleye","doi":"10.1007/s12648-024-03408-9","DOIUrl":null,"url":null,"abstract":"<p>A new anisotropic star model with core-envelope division is generated. The star is assumed to have the core composed of Bose–Einstein Condensate matter and polytropic envelope. The interior space-time is considered to be static and spherically symmetric in relativistic framework. We specify one of the gravitational potentials <span>\\(e^{\\lambda }\\)</span> and <span>\\(e^{\\nu }\\)</span> and then apply the Karmarkar condition to generate our model. The model formulated is free from central singularities and is verified by various stability tests and energy conditions. The equilibrium of the present model is examined by analysing TOV-equation. Stellar masses and radii of compact fluid spheres consistent with observations including Vela X-1, PSRJ1903+327, Cen X-3 and Her X-1 have been generated by using this model. The profiles for the matter variables in the present model are well behaved. It is entrancing to note that a multi-layered star model with core admitting Bose–Einstein condensate equation of state in embedding setting is missing in the previous studies.</p>","PeriodicalId":584,"journal":{"name":"Indian Journal of Physics","volume":null,"pages":null},"PeriodicalIF":1.6000,"publicationDate":"2024-09-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Relativistic star with Bose–Einstein condensate core and polytropic envelope in Karmarkar regime\",\"authors\":\"Amos V. Mathias, Jefta M. Sunzu, Jason M. Mkenyeleye\",\"doi\":\"10.1007/s12648-024-03408-9\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>A new anisotropic star model with core-envelope division is generated. The star is assumed to have the core composed of Bose–Einstein Condensate matter and polytropic envelope. The interior space-time is considered to be static and spherically symmetric in relativistic framework. We specify one of the gravitational potentials <span>\\\\(e^{\\\\lambda }\\\\)</span> and <span>\\\\(e^{\\\\nu }\\\\)</span> and then apply the Karmarkar condition to generate our model. The model formulated is free from central singularities and is verified by various stability tests and energy conditions. The equilibrium of the present model is examined by analysing TOV-equation. Stellar masses and radii of compact fluid spheres consistent with observations including Vela X-1, PSRJ1903+327, Cen X-3 and Her X-1 have been generated by using this model. The profiles for the matter variables in the present model are well behaved. It is entrancing to note that a multi-layered star model with core admitting Bose–Einstein condensate equation of state in embedding setting is missing in the previous studies.</p>\",\"PeriodicalId\":584,\"journal\":{\"name\":\"Indian Journal of Physics\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":1.6000,\"publicationDate\":\"2024-09-05\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Indian Journal of Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1007/s12648-024-03408-9\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"PHYSICS, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Indian Journal of Physics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1007/s12648-024-03408-9","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
Relativistic star with Bose–Einstein condensate core and polytropic envelope in Karmarkar regime
A new anisotropic star model with core-envelope division is generated. The star is assumed to have the core composed of Bose–Einstein Condensate matter and polytropic envelope. The interior space-time is considered to be static and spherically symmetric in relativistic framework. We specify one of the gravitational potentials \(e^{\lambda }\) and \(e^{\nu }\) and then apply the Karmarkar condition to generate our model. The model formulated is free from central singularities and is verified by various stability tests and energy conditions. The equilibrium of the present model is examined by analysing TOV-equation. Stellar masses and radii of compact fluid spheres consistent with observations including Vela X-1, PSRJ1903+327, Cen X-3 and Her X-1 have been generated by using this model. The profiles for the matter variables in the present model are well behaved. It is entrancing to note that a multi-layered star model with core admitting Bose–Einstein condensate equation of state in embedding setting is missing in the previous studies.
期刊介绍:
Indian Journal of Physics is a monthly research journal in English published by the Indian Association for the Cultivation of Sciences in collaboration with the Indian Physical Society. The journal publishes refereed papers covering current research in Physics in the following category: Astrophysics, Atmospheric and Space physics; Atomic & Molecular Physics; Biophysics; Condensed Matter & Materials Physics; General & Interdisciplinary Physics; Nonlinear dynamics & Complex Systems; Nuclear Physics; Optics and Spectroscopy; Particle Physics; Plasma Physics; Relativity & Cosmology; Statistical Physics.