Generation of Growing Modes in Cosmological Density Fluctuations by Black Hole Evapolation

Details Generation of Growing Modes in Cosmological Density Fluctuations by Black Hole Evapolation Generation of Growing Modes in Cosmological Density Fluctuations by Black Hole Evapolation

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pthph..68.1398k&link_type=abstract

Progress of Theoretical Physics, Vol. 68, No. 4, pp. 1398-1401

Physics

7

Scientific paper

We investigate the possibility that growing density fluctuations are
generated in the early universe by the evaporation of primordial black
holes whose distribution has small in-homogeneities on large scales. We
show that the growing modes are actually generated and their amplitudes
are independent of the temporal behavior of evaporation.

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