Non-adiabatic gravitational collapse in f(R,T) gravity with Karmarkar condition for anisotropic fluid
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Publication:5113738
DOI10.1142/S0217732320501035zbMath1435.83117OpenAlexW3004880610MaRDI QIDQ5113738
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Publication date: 16 June 2020
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0217732320501035
Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15)
Cites Work
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- Dynamical instability and the expansion-free condition
- \(f(R)\) theories
- Dynamics of Bianchi \(I\) universe with magnetized anisotropic dark energy
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
- Some new solutions for shear-free fluid spheres with heat flow
- The influence of initial conditions during dissipative collapse
- EFFECTS OF ELECTROMAGNETIC FIELD ON THE DYNAMICS OF BIANCHI TYPE VI0UNIVERSE WITH ANISOTROPIC DARK ENERGY
- A causal model of radiating stellar collapse
- RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
- Charged perfect fluid gravitational collapse in f(R, T) gravity
- Relativistic modeling of Vela X-1 using the Karmarkar condition
- Analysis of charged compact stars in modified gravity
- Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
- SPHERICAL COLLAPSE WITH HEAT FLOW AND WITHOUT HORIZON
- Interaction of viscous modified Chaplygin gas with f(R, T) gravity
- Causal solutions for radiating stellar collapse
- On the stability of the shear-free condition
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