Hydrogen recombination kinetics in the presence of low-mass primordial black holes

Details Hydrogen recombination kinetics in the presence of low-mass primordial black holes Hydrogen recombination kinetics in the presence of low-mass primordial black holes

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..387n&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, Sept.-Oct. 1978, p. 387-392.) Soviet Astronomy Letters, vol. 4, Sept.-Oct. 1978, p.

Astronomy and Astrophysics

Astronomy

12

Astronomical Models, Black Holes (Astronomy), Hydrogen Recombinations, Reaction Kinetics, Adiabatic Conditions, Energy Dissipation, Galactic Evolution, Relativistic Particles

Scientific paper

An analysis is given of the distortion of the dynamics of hydrogen recombination that would be introduced into a standard model universe by the evaporation of low-mass (mass less than 10 to the 17th g) primordial black holes. Limits are placed on the density distribution of these objects; they are consistent with the parameters of the adiabatic theory of galaxy formation.

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