Formation of population III stars and galaxies with primordial planetary-mass black holes

Details Formation of population III stars and galaxies with primordial planetary-mass black holes Formation of population III stars and galaxies with primordial planetary-mass black holes

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...275..405f&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 275, Dec. 15, 1983, p. 405-412.

Astronomy and Astrophysics

Astronomy

30

Black Holes (Astronomy), Galactic Evolution, Stellar Evolution, Baryons, Big Bang Cosmology, Red Shift, Universe

Scientific paper

Primordial black holes in the mass range 1015g ⪉ mbh ⪉ 1033g are candidates for the nonbaryonic dark halo matter. This paper explores the evolution of perturbations associated with these planetary-mass black holes. Clusters of black holes and baryonic matter of mass 104M_sun; ⪉ M ⪉ 107M_sun; are shown to form at redshifts 5 ⪉ z ⪉ 100. Explosions of these objects may lead to galaxy formation via the Ostriker-Cowie mechanism. Thus the spontaneous generation of primordial planetary-mass black holes may subsequently produce galaxies.

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