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gr-qc2020
Adiabatic index for relativistic stars as a coefficient of non-thermal dissipation
Seema Satin
The adiabatic index of a relativistic star (modeled by a perfect fluid) is shown to act as a dissipation constant due to considerations of mesoscopic scale stochastic effects. This…
gr-qc2020
A Fluctuation Dissipation Relation for Relativistic stars
Seema Satin
A fluctuation-dissipation relation for perturbed configuration of a relativistic star is obtained. The stochastic fluctuations of the classical stress tensor comprising the matter…