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A Scenario for Strong Gravity without Extra Dimensions

D. G. Coyne
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Abstract

A different reason for the apparent weakness of the gravitational interaction is advanced, and its consequences for Hawking evaporation of a Schwarzschild black hole are investigated. A simple analytical formulation predicts that evaporating black holes will undergo a type of phase transition resulting in variously long-lived objects of reasonable sizes, with normal thermodynamic properties and inherent duality characteristics. Speculations on the implications for particle physics and for some recently-advanced new paradigms are explored.

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D. G. Coyne. 2006-02-19. A Scenario for Strong Gravity without Extra Dimensions. https://arxiv.org/abs/hep-th/0602183

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