STRUCTURE SCALARS IN CHARGED PLANE SYMMETRY
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Publication:4913331
DOI10.1142/S0217732312501416zbMath1260.83049arXiv1310.8495OpenAlexW2090898624MaRDI QIDQ4913331
M. Zaeem Ul Haq Bhatti, Muhammad Sharif
Publication date: 5 April 2013
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1310.8495
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)
Related Items (17)
Charged adiabatic LTB gravitational collapse in \(f(R)\) gravity ⋮ Dynamics of dissipative viscous cylindrical collapse with full causal approach in \(f(R)\) gravity ⋮ Role of bulk viscosity and electromagnetic field on the stability of collapsing cylinder ⋮ Electromagnetic effects on the inhomogeneity of planar symmetry ⋮ Dynamics and stability of charged spherical star with tilted and non-tilted congruences ⋮ Study of charged anisotropic spherical collapse in f(𝒢) gravity ⋮ Binding energy in self-gravitating charged plane symmetric systems ⋮ Role of anisotropy in the expansion-free plane gravitational collapse ⋮ Structure scalars in dissipative axial system in \(f(R)\) gravity ⋮ EVOLUTION OF EXPANSION-FREE SELF-GRAVITATING FLUIDS AND PLANE SYMMETRY ⋮ Effects of some physical factors on the stability of collapsing stars ⋮ Electromagnetic effect on scalar field collapse in higher curvature gravity ⋮ Stability of the charged radiating cylinder ⋮ Self-gravitating spherically symmetric fluid models in Brans-Dicke gravity ⋮ Spherically symmetric spacetime with radiating fluids in f(𝒢, T) gravity ⋮ Dynamics of relativistic fluids with structure scalars and \(\epsilon R^2\) cosmology ⋮ Effects of some physical factors on the inhomogeneity in planar symmetry
Cites Work
- Dynamics of charged plane symmetric gravitational collapse
- Charged cylindrical collapse of anisotropic fluid
- Junction conditions and consequences of quasi-spherical space-time with electro-magnetic field and Vaidya metric
- EFFECTS OF ELECTROMAGNETIC FIELD ON GRAVITATIONAL COLLAPSE
- Evolution of the density contrast in inhomogeneous dust models
- PHYSICAL CAUSES OF ENERGY DENSITY INHOMOGENIZATION AND STABILITY OF ENERGY DENSITY HOMOGENEITY IN RELATIVISTIC SELF-GRAVITATING FLUIDS
- On Massive Neutron Cores
- On the stability of the shear-free condition
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