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作者单位:Megandhren Govender (1) Robert Bogadi (2) Ranjan Sharma (3) Shyam Das (3)
1. Department of Mathematics, Faculty of Applied Sciences, Durban University of Technology, Durban, 4000, South Africa 2. Astrophysics and Cosmology Research Unit, School of Mathematical Sciences, University of KwaZulu Natal, Durban, 4041, South Africa 3. Department of Physics, P. D. Women’s College, Jalpaiguri, 735101, India
刊物类别:Physics and Astronomy
刊物主题:Physics Astronomy
出版者:Springer Netherlands
ISSN:1572-946X
文摘
We investigate the dynamical nature of the collapse process of a spherically symmetric star undergoing dissipative collapse. The star collapses from an initial static configuration by dissipating energy in the form of a radial heat flux. The perturbation in the density and pressure profiles are such that the star is always close to hydrostatic equilibrium. The temperature profiles are studied using a causal heat transport equation.