Primordial Black Hole Dark Matter evaporating on the Neutrino Floor

30 Aug 2021, 17:10
Talk in parallel session Neutrino physics and astrophysics Discussion Panel Neutrinos 2


Roberta Calabrese (Università degli studi di Napoli "Federico II")


Primordial black holes hypothetically generated in the first instants of life of the Universe are potential dark matter candidates. Focusing on Primordial Black Holes masses in the range $[5 \times10^{14} - 5 \times 10^{15}]$g, we point out that the neutrinos emitted by Primordial Black Holes evaporation can interact through the coherent elastic neutrino-nucleus scattering producing an observable signal in multi-ton Dark Matter direct detection experiments. We show that with the high exposures envisaged for the next-generation facilities, it will be possible to set bounds on the fraction of Dark Matter composed by Primordial Black Holes improving the existing neutrino limits obtained with Super-Kamiokande. We also quantify to what extent a signal originating from a small fraction of Dark Matter in the form of Primordial Black Holes would modify the so-called "neutrino floor", the well-known barrier towards detection of weakly interacting massive particles as the dominant Dark Matter component.

Reference to paper (DOI or arXiv)

Primary authors

Roberta Calabrese (Università degli studi di Napoli "Federico II") Stefano Morisi (University of Naples "Federico II") Antonio Palazzo (AHEP Group, Institut de Fisica Corpuscular, CSIC/Universitat de Valencia) Prof. Gennaro Miele Damiano Francesco Giuseppe Fiorillo

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