Is Radiation of Quantized Black Holes Observable?

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dc.creatorKhriplovich, I. B.
dc.creatorProduit, N.
dc.date2006-04-01
dc.date2006-12-04
dc.date.accessioned2026-07-07T10:43:44Z
dc.date.available2026-07-07T10:43:44Z
dc.descriptionIf primordial black holes (PBH) saturate the present upper limit on the dark matter density in our Solar system and if their radiation spectrum is discrete, the sensitivity of modern detectors is close to that necessary for detecting this radiation. This conclusion is not in conflict with the upper limits on the PBH evaporation rate.
dc.description6 pages, 1 figure (reproduced properly in pdf file)
dc.identifierhttps://arxiv.org/abs/astro-ph/0604003
dc.identifierhttp://arxiv.org/abs/astro-ph/0604003
dc.identifierInt.J.Mod.Phys.D16:1243-1248,2007
dc.identifierdoi:10.1142/S0218271807010730
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/182347
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleIs Radiation of Quantized Black Holes Observable?
dc.typetext

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