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Schwarzschild Interior Solution in an Isotropic Coordinate System
Phys. Rev. 70, 74 – Published 1 July, 1946
DOI: https://doi.org/10.1103/PhysRev.70.74
Abstract
The relativistic equations for the case of a sphere of perfect fluid of constant density are solved when an isotropic coordinate system is used. It is again found that a sphere of given density has upper bounds on its mass and radius but that these upper bounds are smaller than those given by the ordinary Schwarzschild solution.
References (4)
- R. C. Tolman, Relativity, Thermodynamics and Cosmology (Clarendon Press, Oxford, 1934), pp. 245-247
- A. S. Eddington, Mathematical Theory of Relativity (Cambridge University Press. New York, 1923), pp. 93-95
- R. C. Tolman, [1], pp. 242-243
- A. S. Eddington, [2], p. 170