http://arxiv.org/abs/2205.07966
Anisotropic neutrino emission from a core-collapse supernova (CCSN) causes a permanent change in the local space-time metric, called the gravitational wave (GW) memory. Long considered unobservable, this effect will be detectable in the near future, at deci-Hertz GW interferometers. I will present a novel idea, where observations of the neutrino GW memory from CCSNe will enable time-triggered searches of supernova neutrinos at megaton (Mt) scale detectors, which will open a new avenue to studying supernova neutrinos.
M. Mukhopadhyay
Wed, 18 May 22
54/66
Comments: 6 pages, 3 figures. Contribution to the 2022 Electroweak session of the 56th Rencontres de Moriond
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