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The influence of initial conditions during dissipative collapse

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Publication:2832077
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DOI10.1142/S0218271816500929zbMath1348.85002arXiv1602.02874MaRDI QIDQ2832077

M. Govender, Nolene F. Naidu

Publication date: 7 November 2016

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

Full work available at URL: https://arxiv.org/abs/1602.02874


zbMATH Keywords

dissipationhydrostatic equilibriumshear-free condition


Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)


Related Items (7)

Dynamical forces and the influence of an equation of state on gravitational collapse ⋮ What makes a shear-free spherical perfect fluid be inhomogeneous with tidal effects? ⋮ Non-adiabatic gravitational collapse in f(R,T) gravity with Karmarkar condition for anisotropic fluid ⋮ Shear-free radiating collapse model via Karmarkar condition in f(R) gravity ⋮ A charged anisotropic well-behaved Adler–Finch–Skea solution satisfying Karmarkar condition ⋮ Dissipative collapse of a Karmarkar star ⋮ Gravitational collapse for a radiating anisotropic fluid




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