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- W93487192 abstract "We consider the question, what topologies of space-time are permitted by Einstein's equations as models of nonsingular stars. A number of results from the literature on singularity theorems are drawn together here to give a clear answer to this question. If a star evolves from nearly Newtonian initial conditions, of low densities and small space-time curvatures, to a nonsingular final state, then the topology of the space-time representing the star must be R4. We also discuss some topological constraints on models that are not nearly Newtonian in the past, but may have evolved directly from the initial cosmic singularity." @default.
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- W93487192 date "1980-01-01" @default.
- W93487192 modified "2023-09-27" @default.
- W93487192 title "Comments on the Topology of Nonsingular Stellar Models" @default.
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- W93487192 doi "https://doi.org/10.1016/b978-0-12-691380-4.50008-3" @default.
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