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Born-regulated gravity in four dimensions

James FeigenbaumEnrico Fermi Institute and Department of Physics, The University of Chicago, Chicago, Illinois 60637
1998en
ABI

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Previous work involving Born-regulated gravity theories in two dimensions is extended to four dimensions. The action we consider has two dimensionful parameters. Black hole solutions are studied for typical values of these parameters. For masses above a critical value determined in terms of these parameters, the event horizon persists. For masses below this critical value, the event horizon disappears, leaving a ``bare mass,'' though of course no singularity.

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