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Spherically symmetric false vacuum: no-go theorems and global structure

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arxiv gr-qc/0104092 v1 pith:CWJBCDN5 submitted 2001-04-27 gr-qc hep-th

classification gr-qchep-th
keywords fieldpossibleregularflatgeneralscalarschwarzschildsitter
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We enumerate all possible types of spacetime causal structures that can appear in static, spherically symmetric configurations of a self-gravitating, real, nonlinear, minimally coupled scalar field \phi in general relativity, with an arbitrary potential V(\phi), not necessarily positive-definite. It is shown that a variable scalar field adds nothing to the list of possible structures with a constant \phi field, namely, Minkowski (or AdS), Schwarzschild, de Sitter and Schwarzschild - de Sitter. It follows, in particular, that, whatever is V(\phi), this theory does not admit regular black holes with flat or AdS asymptotics. It is concluded that the only possible globally regular, asymptotically flat solutions are solitons with a regular center, without horizons and with at least partly negative potentials V(\phi). Extension of the results to more general field models is discussed.

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  1. Spherically symmetric black holes and wormholes in hybrid metric-Palatini gravity

    gr-qc 2019-08 conditional novelty 6.0 of 10

    In the massless sector of hybrid metric-Palatini gravity, exact spherical vacuum solutions are generically singular or wormhole-like, with special extremal black holes and an infinite-horizon geometry.

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