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• W2029342642 abstract "We consider the evolution of primordial black holes formed during the high energy phase of the braneworld scenario. We show that the effect of accretion from the surrounding radiation bath is dominant compared to evaporation for such black holes. This feature lasts till the onset of matter (or black hole) domination of the total energy density which could occur either in the high energy phase or later. We find that the black hole evaporation times could be significantly large even for black holes with small initial mass to survive until several cosmologically interesting eras." @default.
• W2029342642 created "2016-06-24" @default.
• W2029342642 creator A5064209588 @default.
• W2029342642 date "2003-01-24" @default.
• W2029342642 modified "2023-10-17" @default.
• W2029342642 title "Domination of Black Hole Accretion in Brane Cosmology" @default.
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• W2029342642 doi "https://doi.org/10.1103/physrevlett.90.031303" @default.
• W2029342642 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/12570481" @default.
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