A Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark Energy

The possibility of strange stars mixed with dark energy to be one of the candidates for dark energy stars is the main issue of the present study. Our investigation shows that quark matter atcs as dark energy after a certain yet unknown critical condition inside the quark stars. Our proposed model re...

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Autores principales:	Theophanes Grammenos, Farook Rahaman, Saibal Ray, Debabrata Deb, Sourav Roy Chowdhury
Formato:	article
Lenguaje:	EN
Publicado:	Hindawi Limited 2021
Materias:	Physics QC1-999
Acceso en línea:	https://doaj.org/article/545a7f5d16804a74ba5f2ab30a0d19a8
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spelling	oai:doaj.org-article:545a7f5d16804a74ba5f2ab30a0d19a82021-11-22T01:10:20ZA Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark Energy1687-736510.1155/2021/6966689https://doaj.org/article/545a7f5d16804a74ba5f2ab30a0d19a82021-01-01T00:00:00Zhttp://dx.doi.org/10.1155/2021/6966689https://doaj.org/toc/1687-7365The possibility of strange stars mixed with dark energy to be one of the candidates for dark energy stars is the main issue of the present study. Our investigation shows that quark matter atcs as dark energy after a certain yet unknown critical condition inside the quark stars. Our proposed model reveals that strange stars mixed with dark energy feature a physically acceptable stable model and mimic characteristics of dark energy stars. The plausible connections are shown through the mass-radius relation as well as the entropy and temperature. We particularly note that a two-fluid distribution is a major reason for the anisotropic nature of the spherical stellar system.Theophanes GrammenosFarook RahamanSaibal RayDebabrata DebSourav Roy ChowdhuryHindawi LimitedarticlePhysicsQC1-999ENAdvances in High Energy Physics, Vol 2021 (2021)
institution	DOAJ
collection	DOAJ
language	EN
topic	Physics QC1-999
spellingShingle	Physics QC1-999 Theophanes Grammenos Farook Rahaman Saibal Ray Debabrata Deb Sourav Roy Chowdhury A Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark Energy
description	The possibility of strange stars mixed with dark energy to be one of the candidates for dark energy stars is the main issue of the present study. Our investigation shows that quark matter atcs as dark energy after a certain yet unknown critical condition inside the quark stars. Our proposed model reveals that strange stars mixed with dark energy feature a physically acceptable stable model and mimic characteristics of dark energy stars. The plausible connections are shown through the mass-radius relation as well as the entropy and temperature. We particularly note that a two-fluid distribution is a major reason for the anisotropic nature of the spherical stellar system.
format	article
author	Theophanes Grammenos Farook Rahaman Saibal Ray Debabrata Deb Sourav Roy Chowdhury
author_facet	Theophanes Grammenos Farook Rahaman Saibal Ray Debabrata Deb Sourav Roy Chowdhury
author_sort	Theophanes Grammenos
title	A Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark Energy
title_short	A Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark Energy
title_full	A Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark Energy
title_fullStr	A Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark Energy
title_full_unstemmed	A Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark Energy
title_sort	relativistic compact stellar model of anisotropic quark matter mixed with dark energy
publisher	Hindawi Limited
publishDate	2021
url	https://doaj.org/article/545a7f5d16804a74ba5f2ab30a0d19a8
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A Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark Energy

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