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- W2046863360 abstract "In this paper, we present an exact model of a spherically symmetric star undergoing dissipative collapse in the form of a radial heat flux. The interior of the star is matched smoothly to the generalized Vaidya line element representing a two-fluid atmosphere comprising null radiation and a string fluid. The influence of the string density on the thermal behavior of the model is investigated by employing a causal heat transport equation of Maxwell–Cattaneo form." @default.
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- W2046863360 date "2013-06-01" @default.
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- W2046863360 title "NONADIABATIC SPHERICAL COLLAPSE WITH A TWO-FLUID ATMOSPHERE" @default.
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- W2046863360 doi "https://doi.org/10.1142/s0218271813500491" @default.
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