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Aprile, E.; Abe, K.; Ahmed Maouloud, S.; Angelino, E.; Angevaare, J. R.; Antón Martin, D.; Arneodo, F.; Baudis, L.; Bazyk, M.; Bismark, A.; Brookes, E. J.; Brown, A.; Bruenner, S.; Budnik, R.; Bui, T. K.; Cai, C.; Cimental Chavez, A. P.; Colijn, A. P.; Conrad, J.; Cuenca-García, J. J.; D’Andrea, V.; Decowski, M. P.; Diglio, S.; Eitel, K.; Elykov, A.; Ferella, A. D.; Ferrari, C.; Fischer, H.; Flierman, M.; Fulgione, W.; Fuselli, C.; Galloway, M.; Gao, F.; Glade-Beucke, R.; Grandi, L.; Guida, M.; Higuera, A.; Itow, Y.; Joerg, F.; Kavrigin, P.; Kazama, S.; Kobayashi, M.; Koltman, G.; Lang, R. F.; Layos Carlos, D. G.; Li, I.; Liang, S.; Lindemann, S.; Lombardi, F.; Mahlstedt, J.; Manenti, L.; Marignetti, F.; Marrodán Undagoitia, T.; Masson, D.; Mastroianni, S.; Messina, M.; Moriyama, S.; Ni, K.; Oberlack, U.; Palacio, J.; Pellegrini, Q.; Peres, R.; Peters, C.; Pienaar, J.; Pierre, M.; Qi, J.; Ramírez García, D.; Singh, R.; Sanchez, L.; dos Santos, J. M. F.; Sartorelli, G.; Schreiner, J.; Schulte, D.; Schulte, P.; Schulze Eißing, H.; Schumann, M.; Scotto Lavina, L.; Selvi, M.; Semeria, F.; Shockley, E.; Silva, M.; Simgen, H.; Thers, D.; Trinchero, G.; Tunnell, C.; Tönnies, F.; Valerius, K.; Weinheimer, C.; Wenz, D.; Wittweg, C.; Wolf, T.; Wu, V. H. S.; Xing, Y.; Xu, D.; Xu, Z.; Yamashita, M.; Yang, L.; Ye, J.; Zhong, M.; Zhu, T.
Physical review. D, 10/2023, Letnik: 108, Številka: 7Journal 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 and electronic recoil channels within ±500 seconds of observations of the gravitational-wave signals GW170104, GW170729, GW170817, GW170818, and GW170823. We use this null result to constrain monoenergetic neutrinos and axion-like 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 the 90% confidence level. Furthermore, we constrain the product of the coincident fluence and cross section of axion-like particles to be less than 10 −29 cm 2 /cm 2 in the 5.5–210 keV energy range at the 90% confidence level.
