A JUNO-like reactor neutrino detector could reach a 90% confidence sensitivity of about 2.4 antineutrino events in a 1000-second gravitational-wave coincidence window, implying fluence limits of order 10^8 cm^-2 and detectable distances of 1 to 3 Mpc.
Search for High-energy Neutrinos from Gravitational Wave Event GW151226 and Candidate LVT151012 with ANTARES and IceCube
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abstract
The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find 2 and 4 neutrino candidates detected by IceCube, and 1 and 0 detected by ANTARES, within $\pm500$ s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use non-detection to constrain isotropic-equivalent high-energy neutrino emission from GW151226 adopting the GW event's 3D localization, to less than $2\times 10^{51}-2\times10^{54}$ erg.
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The determination capability of potential neutrinos from gravitational wave sources and contributions of extra detector at the future reactor neutrino experiment
A JUNO-like reactor neutrino detector could reach a 90% confidence sensitivity of about 2.4 antineutrino events in a 1000-second gravitational-wave coincidence window, implying fluence limits of order 10^8 cm^-2 and detectable distances of 1 to 3 Mpc.