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  • Search for events in XENON1T associated with Gravitational Waves
    Abe, K; S Ahmed Maouloud; Angelino, E; Angevaare, J R; Antochi, V C; Martin, D Antoń; Arneodo, F; Baudis, L; Baxter, A L; Bazyk, M; Bellagamba, L; Biondi, R; Brookes, E J; Brown, A; Bui, T K; Cardoso, J M R; Colijn, A P; Cuenca-García, J J; D'Andrea, V; Diglio, S; Eitel, K; Elykov, A; Ferella, A D; Fischer, H; Fulgione, W; Fuselli, C; Gaemers, P; Gaior, R; Galloway, M; Gao, F; Grandi, L; Guida, M; Hammann, R; Hils, C; Hoetzsch, L; Hood, N F; Howlett, J; Iacovacci, M; Itow, Y; Jakob, J; Joerg, F; Joy, A; Kara, M; Kavrigin, P; Kazama, S; Landsman, H; Lang, R F; Layos Carlos, D G; I Li; Liang, S; Lindemann, S; Liu, K; Loizeau, J; Long, J; Y Ma; Manenti, L; Marignetti, F; T Marrodán Undagoitia; Masbou, J; Masson, D; Masson, E; Messina, M; Moriyama, S; Morå, K; Mosbacher, Y; K Ni; Oberlack, U; Paetsch, B; Palacio, J; Pellegrini, Q; Peres, R; Pienaar, J; J Qi; Qin, J; Shi, J; Singh, R; Sanchez, L; J M F dos Santos; Sarnoff, I; Sartorelli, G; Schulte, D; Schulte, P; H Schulze Eißing; Schumann, M; L Scotto Lavina; Selvi, M; Semeria, F; Shi, S; P -L Tan; Terliuk, A; Toschi, F; Trinchero, G; Tunnell, C; Wenz, D; Wu, V H S; Xing, Y; D Xu; Yuan, L; Zavattini, G; Zhong, M

    arXiv (Cornell University), 10/2023
    Paper, Journal Article

    We perform a blind search for particle signals in the XENON1T dark matter detector that occur close in time to gravitational wave signals in the LIGO and Virgo observatories. No particle signal is observed in the nuclear recoil, electronic recoil, CE\(\nu\)NS, and S2-only channels within \(\pm\) 500 seconds of observations of the gravitational wave signals GW170104, GW170729, GW170817, GW170818, and GW170823. We use this null result to constrain mono-energetic neutrinos and Beyond Standard Model particles emitted in the closest coalescence GW170817, a binary neutron star merger. We set new upper limits on the fluence (time-integrated flux) of coincident neutrinos down to 17 keV at 90% confidence level. Furthermore, we constrain the product of coincident fluence and cross section of Beyond Standard Model particles to be less than \(10^{-29}\) cm\(^2\)/cm\(^2\) in the 5.5-210 keV energy range at 90% confidence level.

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