Abstract
A model for a time-dependent relativistic “gas” sphere is given. Both pressurep and densityρ are positive inside the outer boundary of the sphere, and they both drop to zero at the boundary itself. Their respective gradients are negative. For expanding models the pressure and the density are decreasing, and for contracting models the pressure and the density are increasing. The adiabatic sound speed is thus real, and for the layers close to the surface of the sphere it is found that the adiabatic sound speed is less than the speed of light. For these layers the conditionρ>3p is also fulfilled. However, the area 4πR 2 for a sphere of constantr is not an increasing function of comoving radial coordinater.
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Knutsen, H. Nonstatic gas spheres in general relativity. Gen Relat Gravit 16, 777–788 (1984). https://doi.org/10.1007/BF00762915
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DOI: https://doi.org/10.1007/BF00762915