Brightness of a micro-black hole as dark matter candidate

Details Brightness of a micro-black hole as dark matter candidate Brightness of a micro-black hole as dark matter candidate

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008menda..48...61s&link_type=abstract

The Memoirs of the National Defense Academy, Vol. 48, p. 61-67

Computer Science

Dark Matter, Back Hole, Relativity

Scientific paper

In our universe there is plenty of dark matter, even in our solar system. By its existence we can explain the structure and formation of the universe. That is why it has such an important role. However, we do not know its components. By assuming that dark matter is an ensemble of Micro Black Holes (MBH), in this paper we examine its observational properties to check if this MBH ensemble is a possible candidate for a dark matter component. According to our estimate, they should pass through our solar system quite often. They also glow in the band of gamma-ray. Because MBH are sufficiently bright and pass across the sky in ˜1000 seconds, we may observe them as bright lines on pictures taken with future gamma-ray telescopes that have good angular resolution.

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