Effects of some physical factors on the stability of collapsing stars

DOI10.1142/S0218271814500850zbMath1310.83029OpenAlexW2132315806MaRDI QIDQ5176252

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Publication date: 3 March 2015

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0218271814500850

zbMATH Keywords

instabilityconservation lawsshear viscosityelectromagnetic fieldanisotropyheat fluxEinstein-Maxwell field equationsReissner-Nordström-Vaidya spacetime

Mathematics Subject Classification ID

Gravitational energy and conservation laws; groups of motions (83C40) Space-time singularities, cosmic censorship, etc. (83C75) Classical and relativistic thermodynamics (80A10) Galactic and stellar structure (85A15) Electromagnetic theory (general) (78A25) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Einstein-Maxwell equations (83C22)

Related Items (6)

Charged adiabatic LTB gravitational collapse in \(f(R)\) gravity ⋮ Binding energy in self-gravitating charged plane symmetric systems ⋮ Dynamical variables and evolution of the universe ⋮ Stability of anisotropic compact objects in f(T) gravity ⋮ Complexity factor for charged dissipative dynamical system ⋮ Dynamics of relativistic fluids with structure scalars and \(\epsilon R^2\) cosmology

Cites Work

• Dynamical instability and the expansion-free condition
• Structure scalars for charged cylindrically symmetric relativistic fluids
• Radiating spherical collapse with shear and heat flow
• Anisotropic stars. II: Stability
• Radiating shear-free gravitational collapse with charge
• Thermodynamical instabilities of perfect fluid spheres in General Relativity
• Dynamical instability for non-adiabatic spherical collapse
• STRUCTURE SCALARS IN CHARGED PLANE SYMMETRY
• The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
• Stability of the charged radiating cylinder

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