S. Kind et J. Ehlers, INITIAL-BOUNDARY VALUE-PROBLEM FOR THE SPHERICALLY SYMMETRICAL EINSTEIN EQUATIONS FOR A PERFECT FLUID, Classical and quantum gravity, 10(10), 1993, pp. 2123-2136
It is shown that for a given spherically symmetric distribution of a p
erfect fluid on a spacelike hypersurface with boundary and a given, ti
me-dependent boundary pressure. there exists a unique, local-in-time s
olution of the Einstein equations. A Schwarzschild spacetime can be at
tached to the fluid body if and only if the boundary pressure vanishes
. We assume a smooth equation of state for which the density and the s
peed of sound remain positive for vanishing pressure.