Classical Stringy Black Holes Modify the Thermal Spectrum

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dc.creatorHarms, B.
dc.creatorLeblanc, Y.
dc.date1993-05-14
dc.date.accessioned2026-07-07T04:19:25Z
dc.date.available2026-07-07T04:19:25Z
dc.descriptionNon-local (alpha prime) corrections to Schwarzschild black holes are shown to invalidate the thermodynamical interpretation of black holes. In particular, the canonical and Bekenstein-Hawking temperatures are not equal. The particle number density of fields quantized in the (alpha prime modified) black hole background is no longer thermal. In the non-perturbative region (alpha prime going to infinity or mass going to zero), an analytic continuation to the number density is shown to vanish exponentially.
dc.description8 pages, REVTEX
dc.identifierhttps://arxiv.org/abs/hep-th/9305065
dc.identifierhttp://arxiv.org/abs/hep-th/9305065
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/53544
dc.subjectHigh Energy Physics - Theory
dc.titleClassical Stringy Black Holes Modify the Thermal Spectrum
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