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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| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
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Wiley
2021-01-01
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| Series: | Advances in High Energy Physics |
| Online Access: | http://dx.doi.org/10.1155/2021/6966689 |
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| 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 |
| collection | DOAJ |
| 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 |
| id | doaj-art-545a7f5d16804a74ba5f2ab30a0d19a8 |
| institution | Kabale University |
| issn | 1687-7365 |
| language | English |
| publishDate | 2021-01-01 |
| publisher | Wiley |
| record_format | Article |
| series | Advances in High Energy Physics |
| spelling | doaj-art-545a7f5d16804a74ba5f2ab30a0d19a82025-02-03T01:04:24ZengWileyAdvances in High Energy Physics1687-73652021-01-01202110.1155/2021/6966689A Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark EnergyTheophanes Grammenos0Farook Rahaman1Saibal Ray2Debabrata Deb3Sourav Roy Chowdhury4Department of Civil EngineeringDepartment of MathematicsDepartment of PhysicsDepartment of PhysicsInstitute of PhysicsThe 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.http://dx.doi.org/10.1155/2021/6966689 |
| spellingShingle | Theophanes Grammenos Farook Rahaman Saibal Ray Debabrata Deb Sourav Roy Chowdhury A Relativistic Compact Stellar Model of Anisotropic Quark Matter Mixed with Dark Energy Advances in High Energy Physics |
| title | 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_short | 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 |
| url | http://dx.doi.org/10.1155/2021/6966689 |
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