Quantum Gravity and Black Hole Entropy

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dc.creatorMoffat, J. W.
dc.date1998-08-14
dc.date1998-09-18
dc.date.accessioned2026-07-07T04:24:57Z
dc.date.available2026-07-07T04:24:57Z
dc.descriptionThe basic features of a quantum field theory which is Poincaré invariant, gauge invariant, finite and unitary to all orders of perturbation theory are reviewed. Quantum gravity is finite and unitary to all orders of perturbation theory. The Bekenstein-Hawking entropy formula for a black hole is investigated in a conical Rindler space approximation to a black hole event horizon. A renormalization of the gravitational coupling constant is performed leading to a finite Bekenstein-Hawking entropy at the horizon.
dc.description11 pages. Plaintex. Corrections to text
dc.identifierhttps://arxiv.org/abs/hep-th/9808091
dc.identifierhttp://arxiv.org/abs/hep-th/9808091
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/55609
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleQuantum Gravity and Black Hole Entropy
dc.typetext

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