Desperately Seeking Intermediate-Mass Black Holes

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dc.creatorFrampton, Paul H.
dc.date2009-04-20
dc.date2009-04-21
dc.date.accessioned2026-07-07T13:06:19Z
dc.date.available2026-07-07T13:06:19Z
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.descriptionTwo typos
dc.identifierhttps://arxiv.org/abs/0904.2934
dc.identifierhttp://arxiv.org/abs/0904.2934
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/227744
dc.subjectHigh Energy Physics - Theory
dc.titleDesperately Seeking Intermediate-Mass Black Holes
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