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- W2953462680 abstract "We discuss the potential of detecting thermal neutrinos from matter-rich binary mergers, via a decades-long multi-messenger campaign involving a Mt-scale water Cherenkov neutrino detector and one or more next generation gravitational wave detectors, capable of observing mergers up to redshift $zsim 2$. The search of neutrinos in time-coincidence with gravitational wave detections will allow to identify single neutrinos from individual mergers above the background, and to study their distributions in energy, redshift and type (double neutron-star or neutron-star-black hole merger) of the candidate sources. We find that, for merger rates consistent with current LIGO-Virgo constraints, and for a $100~{rm Mtcdot yr}$ exposure, between ${mathcal O(10^{-1})}$ and ${mathcal O(10)}$ neutrino events are expected. For extreme cases of mergers with more than $10^{52}$ ergs emitted in $mathrel{{bar nu}_e}$, the number of events can be as large as $sim 100$, with sensitivity to mergers up to redshift $zsim 0.5$ or so. Such scenarios can already be tested with a $10~{rm Mtcdot yr}$ exposure, resulting in constraints on the post-merger evolution of the systems being considered." @default.
- W2953462680 created "2019-07-12" @default.
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- W2953462680 date "2020-01-29" @default.
- W2953462680 modified "2023-10-14" @default.
- W2953462680 title "Observing cosmological binary mergers with next generation neutrino and gravitational wave detectors" @default.
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- W2953462680 doi "https://doi.org/10.1103/physrevd.101.023016" @default.
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