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Hybrid Charged Stellar Model Via Embedding and Gravitational Decoupling.
- Source :
- Brazilian Journal of Physics; Oct2021, Vol. 51 Issue 5, p1371-1405, 35p
- Publication Year :
- 2021
-
Abstract
- In this paper, we present a new exact anisotropic charged version of Pant's interior solution [Astrophys. Space Sci. 331, 633 (2011)] by employing the embedding class I condition and the gravitational decoupling via minimal geometric decoupling (MGD) approach. We successfully integrate the coupled Einstein–Maxwell field equations within the MGD and generate a family of new charged anisotropic solutions describing compact stellar objects. The matching of the interior to the exterior Reissner–Nordstrom solution help fix the arbitrary constants. For a chosen parameter space we subject our model to rigorous tests in order to validate its physical viability as a realistic self-gravitating, compact object. We show that the deformation parameter σ is intrinsically connected to key features such as compactness, mass-to-radius ratio and surface redshift for compact star candidates such as Her X-1, EXO 1785-248, PSR J1614-2230 and SAX J1808.4-3658. [ABSTRACT FROM AUTHOR]
Details
- Language :
- English
- ISSN :
- 01039733
- Volume :
- 51
- Issue :
- 5
- Database :
- Complementary Index
- Journal :
- Brazilian Journal of Physics
- Publication Type :
- Academic Journal
- Accession number :
- 152013875
- Full Text :
- https://doi.org/10.1007/s13538-021-00942-3