Constraint on the Mass of Primordial Black Holes from the Value of the Cosmological Constant
classification
🌀 gr-qc
keywords
holesblackprimordialconstantcosmologicalmassbeenchange
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In a recent propposal, the cosmological constant has been considered as as a new thermodynamical variable and its change is related to the radiation produced by black holes. Using this consideration and by modelling the primordial black holes as Schwarzschild-de Sitter holes,we have constrained the total mass of primordial black holes evaporated by now, giving an estimate of the order of 1.624x10^24 solar masses.
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