Anisotropic compact star with Vaidya–Tikekar potential in f(Q) gravity.
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| Title: | Anisotropic compact star with Vaidya–Tikekar potential in f(Q) gravity. |
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| Authors: | AWAIS, M.1 (AUTHOR) mawaisarain181@gmail.com, AZAM, M.1 (AUTHOR) muhammadawais.maths@gmail.com |
| Source: | Journal of Astrophysics & Astronomy. 2/20/2026, Vol. 47 Issue 1, p1-12. 12p. |
| Subjects: | Compact objects (Astronomy), Gravitational potential, Schwarzschild metric, Fluids, Pulsars |
| Abstract: | The goal of this work is to develop physical models for spherically symmetric systems in the realm of f(Q) gravity. The field equations are set up for an anisotropic fluid, and formulate these equations using the physical ansatz of the Vaidya–Tikekar solution. The intrinsic constants of the model can be ascertained by matching the interior solution to the external Schwarzschild solution. The use of accessibility conditions helps to understand the physical viability of the obtained model. LMC X-4 pulsar is used as a toy model to test the viability of the model, and Mathematica software is used for deeper insights and visualisation of the physical parameters against fixed values of constants. [ABSTRACT FROM AUTHOR] |
| Copyright of Journal of Astrophysics & Astronomy is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.) | |
| Database: | Engineering Source |
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| Header | DbId: egs DbLabel: Engineering Source An: 191806333 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| Items | – Name: Title Label: Title Group: Ti Data: Anisotropic compact star with Vaidya–Tikekar potential in f(Q) gravity. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22AWAIS%2C+M%2E%22">AWAIS, M.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> mawaisarain181@gmail.com</i><br /><searchLink fieldCode="AR" term="%22AZAM%2C+M%2E%22">AZAM, M.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> muhammadawais.maths@gmail.com</i> – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Journal+of+Astrophysics+%26+Astronomy%22">Journal of Astrophysics & Astronomy</searchLink>. 2/20/2026, Vol. 47 Issue 1, p1-12. 12p. – Name: Subject Label: Subjects Group: Su Data: <searchLink fieldCode="DE" term="%22Compact+objects+%28Astronomy%29%22">Compact objects (Astronomy)</searchLink><br /><searchLink fieldCode="DE" term="%22Gravitational+potential%22">Gravitational potential</searchLink><br /><searchLink fieldCode="DE" term="%22Schwarzschild+metric%22">Schwarzschild metric</searchLink><br /><searchLink fieldCode="DE" term="%22Fluids%22">Fluids</searchLink><br /><searchLink fieldCode="DE" term="%22Pulsars%22">Pulsars</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: The goal of this work is to develop physical models for spherically symmetric systems in the realm of f(Q) gravity. The field equations are set up for an anisotropic fluid, and formulate these equations using the physical ansatz of the Vaidya–Tikekar solution. The intrinsic constants of the model can be ascertained by matching the interior solution to the external Schwarzschild solution. The use of accessibility conditions helps to understand the physical viability of the obtained model. LMC X-4 pulsar is used as a toy model to test the viability of the model, and Mathematica software is used for deeper insights and visualisation of the physical parameters against fixed values of constants. [ABSTRACT FROM AUTHOR] – Name: AbstractSuppliedCopyright Label: Group: Ab Data: <i>Copyright of Journal of Astrophysics & Astronomy is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.) |
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| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1007/s12036-025-10119-y Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 12 StartPage: 1 Subjects: – SubjectFull: Compact objects (Astronomy) Type: general – SubjectFull: Gravitational potential Type: general – SubjectFull: Schwarzschild metric Type: general – SubjectFull: Fluids Type: general – SubjectFull: Pulsars Type: general Titles: – TitleFull: Anisotropic compact star with Vaidya–Tikekar potential in f(Q) gravity. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: AWAIS, M. – PersonEntity: Name: NameFull: AZAM, M. IsPartOfRelationships: – BibEntity: Dates: – D: 20 M: 02 Text: 2/20/2026 Type: published Y: 2026 Identifiers: – Type: issn-print Value: 02506335 Numbering: – Type: volume Value: 47 – Type: issue Value: 1 Titles: – TitleFull: Journal of Astrophysics & Astronomy Type: main |
| ResultId | 1 |
