Gravitational collapse and dark universe with LTB geometry
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Publication:4976089
DOI10.1142/S0218271817500456zbMath1367.83082MaRDI QIDQ4976089
Z. Yousaf, M. Zaeem Ul Haq Bhatti
Publication date: 27 July 2017
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Relativistic cosmology (83F05) Electromagnetic fields in general relativity and gravitational theory (83C50) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (15)
Various phases of irregular energy density in charged spheres ⋮ Role of modified scalar variables in the modeling of spherical fluids ⋮ Quasi static evolution of compact objects in modified gravity ⋮ Energy conditions in higher derivative f(R,□R,T) gravity ⋮ Some anisotropic planar stellar models ⋮ Stability analysis of stellar radiating filaments ⋮ Anisotropic Stellar Systems in f(R)$f(R)$ Connected Static Spacetime ⋮ Influence of modification of gravity on spherical wormhole models ⋮ Electromagnetic effects on cylindrical gravastar-like strings in f(R, T, RσηTση) gravity ⋮ Measure of complexity for dynamical self-gravitating structures ⋮ Evolution of the charged dynamical radiating spherical structures ⋮ Effects of non-minimally coupled \(f(R, T)\) gravity on the stability of a self-gravitating spherically symmetric fluid ⋮ Energy conditions in modified \(f(G)\) gravity ⋮ Role of f(G,T) gravity on the evolution of relativistic stars ⋮ Energy content of a collapsing sphere with f(R) gravity
Cites Work
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- The effect of pressure gradients on luminosity distance–redshift relations
- Cosmological constraints on f(R) gravity theories within the Palatini approach
- Matching spherical dust solutions to construct cosmological models
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