Relativistic compact stars with dark matter density profile
Abstract In this article, we are proposing a model of anisotropic compact star possessing density profile of pseudo-isothermal dark matter satisfying a linear equation of state (EoS). The stellar system supported by this density profile is physically possible and in equilibrium fulfilling all the en...
Main Authors: | , , , |
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Format: | Article |
Language: | English |
Published: |
SpringerOpen
2020-03-01
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Series: | European Physical Journal C: Particles and Fields |
Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-020-7803-3 |
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author | Nayan Sarkar Susmita Sarkar Ksh. Newton Singh Farook Rahaman |
author_facet | Nayan Sarkar Susmita Sarkar Ksh. Newton Singh Farook Rahaman |
author_sort | Nayan Sarkar |
collection | DOAJ |
description | Abstract In this article, we are proposing a model of anisotropic compact star possessing density profile of pseudo-isothermal dark matter satisfying a linear equation of state (EoS). The stellar system supported by this density profile is physically possible and in equilibrium fulfilling all the energy conditions including the TOV-equation. The solution also satisfies the causality condition, static stability criterion, Abreu’s stability and Bondi’s criteria. The fulfillment of Rhoades–Ruffini criterion makes our solution more physically viable as well. The M–R curve is plotted for $$b=12.55$$ b=12.55 km and $$B_g=60$$ Bg=60 MeV/fm$$^3$$ 3 . |
first_indexed | 2024-12-24T13:07:21Z |
format | Article |
id | doaj.art-0b472ec0c3eb46b3bbe9d8ac609498dd |
institution | Directory Open Access Journal |
issn | 1434-6044 1434-6052 |
language | English |
last_indexed | 2024-12-24T13:07:21Z |
publishDate | 2020-03-01 |
publisher | SpringerOpen |
record_format | Article |
series | European Physical Journal C: Particles and Fields |
spelling | doaj.art-0b472ec0c3eb46b3bbe9d8ac609498dd2022-12-21T16:53:58ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-03-0180311310.1140/epjc/s10052-020-7803-3Relativistic compact stars with dark matter density profileNayan Sarkar0Susmita Sarkar1Ksh. Newton Singh2Farook Rahaman3Department of Mathematics, Jadavpur UniversityDepartment of Mathematics, Jadavpur UniversityDepartment of Mathematics, Jadavpur UniversityDepartment of Mathematics, Jadavpur UniversityAbstract In this article, we are proposing a model of anisotropic compact star possessing density profile of pseudo-isothermal dark matter satisfying a linear equation of state (EoS). The stellar system supported by this density profile is physically possible and in equilibrium fulfilling all the energy conditions including the TOV-equation. The solution also satisfies the causality condition, static stability criterion, Abreu’s stability and Bondi’s criteria. The fulfillment of Rhoades–Ruffini criterion makes our solution more physically viable as well. The M–R curve is plotted for $$b=12.55$$ b=12.55 km and $$B_g=60$$ Bg=60 MeV/fm$$^3$$ 3 .http://link.springer.com/article/10.1140/epjc/s10052-020-7803-3 |
spellingShingle | Nayan Sarkar Susmita Sarkar Ksh. Newton Singh Farook Rahaman Relativistic compact stars with dark matter density profile European Physical Journal C: Particles and Fields |
title | Relativistic compact stars with dark matter density profile |
title_full | Relativistic compact stars with dark matter density profile |
title_fullStr | Relativistic compact stars with dark matter density profile |
title_full_unstemmed | Relativistic compact stars with dark matter density profile |
title_short | Relativistic compact stars with dark matter density profile |
title_sort | relativistic compact stars with dark matter density profile |
url | http://link.springer.com/article/10.1140/epjc/s10052-020-7803-3 |
work_keys_str_mv | AT nayansarkar relativisticcompactstarswithdarkmatterdensityprofile AT susmitasarkar relativisticcompactstarswithdarkmatterdensityprofile AT kshnewtonsingh relativisticcompactstarswithdarkmatterdensityprofile AT farookrahaman relativisticcompactstarswithdarkmatterdensityprofile |