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Through a Black Hole into a New Universe
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We show that an S-Brane which arises in the inside of the black hole horizon when the Weyl curvature reaches the string scale induces a continuous transition between the inside of the black hole and the beginning of a new universe. This provides a simultaneous resolution of both the black hole and Big Bang singularities. In this context, the black hole information loss problem is also naturally resolved.
Forward citations
Cited by 3 Pith papers
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Dynamical Formation of Regular Black Holes
In quasi-topological gravity, a collapsing thin shell bounces at small radius, producing a regular, geodesically complete black hole instead of a singularity.
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Regular black holes from thin-shell collapse
In D≥5 pure gravity with an infinite tower of higher-curvature terms, spherical thin-shell collapse generically produces regular black holes that bounce into new universes.
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Regular black holes from Oppenheimer-Snyder collapse
In quasi-topological gravities in D>=5 with infinite higher-curvature towers, Oppenheimer-Snyder dust collapse bounces at a finite minimum radius, yielding regular black holes and bouncing FLRW cosmologies.
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