Density dependent B- parameter model of relativistic strange stars in the framework of f(R, T) gravity
We investigate a spherically symmetric, isotropic model of strange stars in the context of modified gravity, considering the functional form f(R,T)=R+2βT, where R is the Ricci scalar, T the trace of the energy-momentum tensor, and β a coupling constant. To obtain the gravitational field equations, a...
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| Autors principals: | , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Elsevier
2026-02-01
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| Col·lecció: | Physics Letters B |
| Matèries: | |
| Accés en línia: | http://www.sciencedirect.com/science/article/pii/S0370269325008950 |
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