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Primordial Black Hole Dark Matter and the LIGO/Virgo observations · Around

2020

Primordial Black Hole Dark Matter and the LIGO/Virgo observations

Jedamzik, Karsten

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The LIGO/Virgo collaboration have by now detected the mergers of ten black hole binaries via the emission of gravitational radiation.

The hypothesis that these black holes have formed during the cosmic QCD epoch and make up all of the cosmic dark matter, has been rejected by many authors reasoning that, among other constraints, primordial black hole (PBH) dark matter would lead to orders of magnitude larger merger rates than observed.
We revisit the calculation of the present PBH merger rate.
Solar mass PBHs form clusters at fairly high redshifts, which evaporate at lower redshifts.

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