Stellar modeling with the Einstein-Maxwell field equations via gravitational decoupling
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Publication:6490588
DOI10.1016/J.CJPH.2020.06.020MaRDI QIDQ6490588
Ravindra Kishor Bisht, Neeraj Pant, Satyanarayana Gedela
Publication date: 23 April 2024
Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)
Einstein's field equationsgeneral relativitycompact starsKarmarkar conditionembedding class IMGD-decoupling
General relativity (83Cxx) Astronomy and astrophysics (85Axx) Unified, higher-dimensional and super field theories (83Exx)
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- Well behaved class of charge analogue of heintzmann's relativistic exact solution
- New class of well behaved exact solutions of relativistic charged white-dwarf star with perfect fluid
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
- Insufficiency of Karmarkar's condition
- The stability of relativistic stars and the role of the adiabatic index
- Decoupling gravitational sources in general relativity: the extended case
- Anisotropic spherical solutions by gravitational decoupling in \(f(R)\) gravity
- A class of charged analogues of Durgapal and Fuloria superdense star
- Some new exact solutions with finite central parameters and uniform radial motion of sound
- Classes of exact Einstein-Maxwell solutions
- Anisotropic relativistic stellar models
- Relativistic anisotropic models for compact star with equation of state p = f(ρ)
- Tikekar superdense stars in electric fields
- The minimal geometric deformation approach extended
- Static charged fluid surrounded by a black antihole: an enlarged Klein solution
- Anisotropic stars in general relativity
- REGULAR AND WELL-BEHAVED RELATIVISTIC CHARGED SUPERDENSE STAR MODELS
- Relativistic modeling of Vela X-1 using the Karmarkar condition
- Gravitational decoupling in 2 + 1 dimensional space-times with cosmological term
- Anisotropic ultracompact Schwarzschild star by gravitational decoupling
- Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
- SEARCHING EXACT SOLUTIONS FOR COMPACT STARS IN BRANEWORLD: A CONJECTURE
- The contraction of gravitating spheres
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
- Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity
- Using MGD Gravitational Decoupling to Extend the Isotropic Solutions of Einstein Equations to the Anisotropical Domain
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