Signatures of primordial black hole dark matter at DUNE and THEIA

被引:9
|
作者
De Romeri, Valentina [1 ]
Martinez-Mirave, Pablo
Tortola, Mariam
机构
[1] Univ Valencia, Dept Fis Teor, Paterna 46980, Spain
关键词
dark matter theory; neutrino experiments; primordial black holes; PARTICLE-EMISSION RATES; NEUTRINO OSCILLATION EXPERIMENTS; GLUON-JET EMISSION; MASSLESS PARTICLES; QUARK-JET; SIMULATION; DENSITY;
D O I
10.1088/1475-7516/2021/10/051
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Primordial black holes (PBHs) are a potential dark matter candidate whose masses can span over many orders of magnitude. If they have masses in the 10(15)-10(17) g range, they can emit sizeable fluxes of MeV neutrinos through evaporation via Hawking radiation. We explore the possibility of detecting light (non-)rotating PBHs with future neutrino experiments. We focus on two next generation facilities: the Deep Underground Neutrino Experiment (DUNE) and THEIA. We simulate the expected event spectra at both experiments assuming different PBH mass distributions and spins, and we extract the expected 95% C.L. sensitivities to these scenarios. Our analysis shows that future neutrino experiments like DUNE and THEIA will be able to set competitive constraints on PBH dark matter, thus providing complementary probes in a part of the PBH parameter space currently constrained mainly by photon data.
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页数:21
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