期刊
ASTROPHYSICS AND SPACE SCIENCE
卷 361, 期 1, 页码 -出版社
SPRINGER
DOI: 10.1007/s10509-015-2616-9
关键词
Gravitational collapse; Exact solutions; Einstein's field equations; Radiating star model; Extended irreversible thermodynamics
资金
- Inter University Centre for Astronomy and Astrophysics (IUCAA), Pune, India under Visiting Research Associateship Programme
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.
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