1989
DOI: 10.1007/bf00774083
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Black holes without singularities

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Cited by 22 publications
(14 citation statements)
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“…For instance, choose any (D − 1)-dimensional proper Riemannian manifold containing a minimal surface S and take its direct product with (IR, −dt 2 ). A more sophisticated yet explicit example for non-static spacetimes was presented by Newman in [15] for the famous Gödel spacetime (see also [9], pp.393-405).…”
Section: Remarksmentioning
confidence: 99%
“…For instance, choose any (D − 1)-dimensional proper Riemannian manifold containing a minimal surface S and take its direct product with (IR, −dt 2 ). A more sophisticated yet explicit example for non-static spacetimes was presented by Newman in [15] for the famous Gödel spacetime (see also [9], pp.393-405).…”
Section: Remarksmentioning
confidence: 99%
“…Yet it is non-singular [1]. This escape from a singularity occurs because there are bad causality violations in the spacetime [17,19].…”
Section: Open-universe Singularity Theoremsmentioning
confidence: 99%
“…Some form of causality assumption is necessary for the topology-change argument of this paper to go through. If no such assumption is made, there are scenarios possible, based on the Gödel solution, that neither possess singularities nor change topology [24][25][26].…”
mentioning
confidence: 99%