Entropy of Intermediate-Mass Black Holes

Details Entropy of Intermediate-Mass Black Holes Entropy of Intermediate-Mass Black Holes

2009-05-15

arxiv.org/abs/0905.2535v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

aastex. 8 pages, 1 figure

Scientific paper

Observational 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.

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