Black Holes from Blue Spectra

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dc.creatorLidsey, James E.
dc.creatorCarr, B. J.
dc.creatorGilbert, J. H.
dc.date1994-06-09
dc.date.accessioned2026-07-07T02:19:13Z
dc.date.available2026-07-07T02:19:13Z
dc.descriptionBlue primordial power spectra with a spectral index $n>1$ can lead to a significant production of primordial black holes in the very early Universe. The evaporation of these objects leads to a number of observational consequences and a model independent upper limit of $n \approx 1.4$. In some cases this limit is strengthened to $n=1.3$. Such limits may be employed to define the boundary to the region of parameter space consistent with generalized inflationary predictions. [To appear in Proceedings of the CASE WESTERN CMB WORKSHOP, April 22-24 1994. Figures available on request from J.H.Gilbert@qmw.ac.uk]
dc.description9 pages, LaTex
dc.identifierhttps://arxiv.org/abs/astro-ph/9406028
dc.identifierhttp://arxiv.org/abs/astro-ph/9406028
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9781
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBlack Holes from Blue Spectra
dc.typetext

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