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A cosmological solution of Einstein’s equations
An exact solution of the equations of general relativity is given which tends to Einstein–de Sitter at late times. The energy density is inhomogeneous at early times, and is singular on two spherical surfaces which may be related to the ‘‘bubbles’’ typical of inflationary universe models.
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Published in: | Journal of mathematical physics 1984-11, Vol.25 (11), p.3297-3298 |
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Main Author: | |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | An exact solution of the equations of general relativity is given which tends to Einstein–de Sitter at late times. The energy density is inhomogeneous at early times, and is singular on two spherical surfaces which may be related to the ‘‘bubbles’’ typical of inflationary universe models. |
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ISSN: | 0022-2488 1089-7658 |
DOI: | 10.1063/1.526078 |