作者: G Govender , S D Maharaj , M Govender
DOI: 10.1088/1742-6596/484/1/012014
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摘要: We have constructed the general junction conditions on surface of a dissipating relativistic star. The stellar exterior is spacetime described by generalised Vaidya metric and two-fluid energy-momentum tensor, therefore, defines local atmosphere, which must be super-position standard null radiation fluid. highlighted briefly that our result will effect physics dissipation at boundary.