A Scenario for Strong Gravity without Extra Dimensions

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dc.creatorCoyne, D. G.
dc.date2006-02-19
dc.date.accessioned2026-07-07T07:02:53Z
dc.date.available2026-07-07T07:02:53Z
dc.descriptionA 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.
dc.description49 pages, 13 figures, pdf. For a high resolution file contact me at coyne@scipp.ucsc.edu
dc.identifierhttps://arxiv.org/abs/hep-th/0602183
dc.identifierhttp://arxiv.org/abs/hep-th/0602183
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/108765
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA Scenario for Strong Gravity without Extra Dimensions
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