Motion of primordial black holes in the early universe and their likely distribution today

Details Motion of primordial black holes in the early universe and their likely distribution today Motion of primordial black holes in the early universe and their likely distribution today

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980gregr..12..881i&link_type=abstract

General Relativity and Gravitation, vol. 12, Nov. 1980, p. 881-893.

Astronomy and Astrophysics

Astronomy

Black Holes (Astronomy), Spatial Distribution, Stellar Motions, Energy Dissipation, Galactic Evolution, Halos, Quantum Mechanics

Scientific paper

The effects which slow down holes of mass approximately 10 to the 15th g and affect their spatial distribution today are examined in detail. In particular effects caused by the charge fluctuations of the hole which results from quantum-mechanical processes are treated. The dominant energy-loss mechanism for the holes is the expansion of the universe, which leaves them virtually at rest at the time of galaxy formation. The resultant violent relaxation should concentrate roughly half of them in present-day galaxies and their halos.

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