Entropy of Intermediate-Mass Black Holes

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dc.creatorFrampton, Paul H.
dc.date2009-05-15
dc.date.accessioned2026-07-07T13:15:37Z
dc.date.available2026-07-07T13:15:37Z
dc.descriptionObservational searches for Intermediate-Mass Black Holes (IMBHs), defined to have masses between 30 and 300,000 solar masses, provide limits which allow up to ten percent of what is presently identified as halo dark matter to be in the form of IMBHs. These concentrate entropy so efficiently that the halo contribution can be bigger than the core supermassive black hole. Formation of IMBHs is briefly discussed.
dc.descriptionaastex. 8 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/0905.2535
dc.identifierhttp://arxiv.org/abs/0905.2535
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/230527
dc.subjectAstrophysics of Galaxies
dc.subjectHigh Energy Astrophysical Phenomena
dc.titleEntropy of Intermediate-Mass Black Holes
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