Physically valid black-hole interior models

Abstract

New, simple models of ``black hole interiors'', namely spherically symmetric solutions of the Einstein field equations in matter matching the Schwarzschild vacuum at spacelike hypersurfaces ``R<2M'' are constructed. The models satisfy the weak energy condition and their matter content is specified by an equation of state of the elastic type.

6 pages, TeX format

References in corpus (3)

• Regular Black Holes and Topology Change
• Open and Closed Universes, Initial Singularities and Inflation
• The 2m <= r property of spherically symmetric static spacetimes

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• The Atmosphere of a Black Hole