Gravitational Model of Compact Spherical Reissner-Nordström-Type Star Under f(R, T) Gravity
DOI10.1080/1726037X.2021.1965705zbMath1503.83004OpenAlexW3201817743MaRDI QIDQ5029652
Publication date: 14 February 2022
Published in: Journal of Dynamical Systems and Geometric Theories (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1080/1726037x.2021.1965705
Diffraction, scattering (78A45) Spectrum, resolvent (47A10) Electromagnetic fields in general relativity and gravitational theory (83C50) Gravitational energy and conservation laws; groups of motions (83C40) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Conformal structures on manifolds (53C18)
Cites Work
- Rogue wave in Titan's atmosphere
- New class of regular and well behaved exact solutions in general relativity
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
- General Relativistic Fluid Spheres
- Static charged fluid in (2 + 1)-dimensions admitting conformal Killing vectors
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
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