2005, Vol.8, No.3, pp.308-312
It is shown that collisions of particles of
cosmological background should be taken into consideration to
adequately describe accretion onto primordial black holes (PBHs)
in braneworld cosmologies. When the particle collisions are really
important, accretion of radiation dominated cosmological
background is described by approximation of continuous matter which
accretion rate, evaluated here for the first time, considerably
exceeds the one obtained earlier in free particle approximation
and gives footing to reconsider the possible observational
consequences of extra dimensions. A new procedure of evaluation of
intensive PBH accretion mass growth on the high-energy phase of
Randall-Sundrum Type II braneworld cosmology is given.
Key words:
black hole, braneworld cosmologies, accretion
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