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Paper detail

Cosmic evolution during primordial black hole evaporation

Primordial black holes with a narrow mass range are regarded as a nonrelativistic fluid component with an equation of state for dust. The impact of the black hole evaporation on the dynamics of the early universe is studied by resorting to a two-fluid model. We find periods of intense radiation reheating in the initial and final stages of the evaporation.

preprint1998arXivOpen access
Winfried ZimdahlDiego Pavón
astro-phgr-qc
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Winfried ZimdahlDiego Pavón

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