Impact of a variable cosmological constant on stellar matter configurations in Finch-Skea spacetime.

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Title: Impact of a variable cosmological constant on stellar matter configurations in Finch-Skea spacetime.
Authors: Ilyas, M.1 (AUTHOR) ilyas_mia@yahoo.com, Maha2 (AUTHOR) maha.official00@gmail.com, Nawaz, Salma1 (AUTHOR) salma_nawaz53@yahoo.com, Sher, Falak3 (AUTHOR) falaks2@illinois.edu, Khan, Fawad1 (AUTHOR) fawad.ccms@gmail.com
Source: Astrophysics & Space Science. May2025, Vol. 370 Issue 5, p1-11. 11p.
Subjects: Stellar structure, Cosmological constant, Compact objects (Astronomy), Stars, Spacetime
Abstract: In this study, a variable cosmological constant model is created for anisotropic star structures, which satisfies the remaining physical requirements, and validates the required energy conditions (Ecs), and TOV equations. First, the Finch-Skea spacetime solution is taken into account as a static spherically symmetric metric. Moreover, external Schwarzschild geometry is taken into account to correlate our internal stellar structure and determine the values of the constants used in the Finch-Skea spacetime solution. Finally, in this paper, multiple aspects are discussed, such as the radius, compactness, stresses, stability, density profile, and masses under the variable cosmological constant model in f (R , T) gravity for various stars. [ABSTRACT FROM AUTHOR]
Copyright of Astrophysics & Space Science 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.)
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  Data: Impact of a variable cosmological constant on stellar matter configurations in Finch-Skea spacetime.
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  Data: <searchLink fieldCode="AR" term="%22Ilyas%2C+M%2E%22">Ilyas, M.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> ilyas_mia@yahoo.com</i><br /><searchLink fieldCode="AR" term="%22Maha%22">Maha</searchLink><relatesTo>2</relatesTo> (AUTHOR)<i> maha.official00@gmail.com</i><br /><searchLink fieldCode="AR" term="%22Nawaz%2C+Salma%22">Nawaz, Salma</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> salma_nawaz53@yahoo.com</i><br /><searchLink fieldCode="AR" term="%22Sher%2C+Falak%22">Sher, Falak</searchLink><relatesTo>3</relatesTo> (AUTHOR)<i> falaks2@illinois.edu</i><br /><searchLink fieldCode="AR" term="%22Khan%2C+Fawad%22">Khan, Fawad</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> fawad.ccms@gmail.com</i>
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  Data: <searchLink fieldCode="JN" term="%22Astrophysics+%26+Space+Science%22">Astrophysics & Space Science</searchLink>. May2025, Vol. 370 Issue 5, p1-11. 11p.
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  Data: <searchLink fieldCode="DE" term="%22Stellar+structure%22">Stellar structure</searchLink><br /><searchLink fieldCode="DE" term="%22Cosmological+constant%22">Cosmological constant</searchLink><br /><searchLink fieldCode="DE" term="%22Compact+objects+%28Astronomy%29%22">Compact objects (Astronomy)</searchLink><br /><searchLink fieldCode="DE" term="%22Stars%22">Stars</searchLink><br /><searchLink fieldCode="DE" term="%22Spacetime%22">Spacetime</searchLink>
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  Label: Abstract
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  Data: In this study, a variable cosmological constant model is created for anisotropic star structures, which satisfies the remaining physical requirements, and validates the required energy conditions (Ecs), and TOV equations. First, the Finch-Skea spacetime solution is taken into account as a static spherically symmetric metric. Moreover, external Schwarzschild geometry is taken into account to correlate our internal stellar structure and determine the values of the constants used in the Finch-Skea spacetime solution. Finally, in this paper, multiple aspects are discussed, such as the radius, compactness, stresses, stability, density profile, and masses under the variable cosmological constant model in f (R , T) gravity for various stars. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of Astrophysics & Space Science 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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      – Type: doi
        Value: 10.1007/s10509-025-04435-6
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      – Code: eng
        Text: English
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        PageCount: 11
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      – SubjectFull: Stellar structure
        Type: general
      – SubjectFull: Cosmological constant
        Type: general
      – SubjectFull: Compact objects (Astronomy)
        Type: general
      – SubjectFull: Stars
        Type: general
      – SubjectFull: Spacetime
        Type: general
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      – TitleFull: Impact of a variable cosmological constant on stellar matter configurations in Finch-Skea spacetime.
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            – D: 01
              M: 05
              Text: May2025
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              Y: 2025
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