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- W2963353204 abstract "Singularities associated with an incomplete space-time (S) are not uniquely defined until a boundary is attached to it. [The resulting space-time-with-boundary will be termed a total space-time (TST).] Since an incomplete space-time is compatible with a variety of boundaries, it follows that S does not represent a unique universe but instead corresponds to a family of universes, one for each of the distinct TSTs. It is shown here that the boundary attached to the Reissner-Nordstrom space-time for a point charge is invalid for q^2 < m^2. When the correct boundary is used, the resulting TST is inextendible. This implies that the Graves-Brill black hole cannot be produced by gravitational collapse. The same is true of the Kruskal-Fronsdal black hole for the point mass, and for those black holes which reduce to the latter for special values of their parameters." @default.
- W2963353204 created "2019-07-30" @default.
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- W2963353204 date "2001-02-12" @default.
- W2963353204 modified "2023-09-27" @default.
- W2963353204 title "The Total Space-Time of a Point Charge and Its Consequences for Black Holes" @default.
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