Search for inelastic scattering of WIMP dark matter in XENON1T

Search for inelastic scattering of WIMP dark matter in XENON1T

XENON Collaboration;XENON Collaboration;Aprile, E.;Aprile, E.;Aalbers, J.;Aalbers, J.;Agostini, F.;Agostini, F.;Alfonsi, M.;Alfonsi, M.;Althueser, L.;Althueser, L.;Amaro, F. D.;Amaro, F. D.;Andaloro, S.;Andaloro, S.;Angelino, E.;Angelino, E.;Angevaare, J. R.;Angevaare, J. R.;Antochi, V. C.;Antochi, V. C.;Arneodo, F.;Arneodo, F.;Baudis, L.;Baudis, L.;Bauermeister, B.;Bauermeister, B.;Bellagamba, L.;Bellagamba, L.;Benabderrahmane, M. L.;Benabderrahmane, M. L.;Brown, A.;Brown, A.;Brown, E.;Brown, E.;Bruenner, S.;Bruenner, S.;Bruno, G.;Bruno, G.;Budnik, R.;Budnik, R.;Capelli, C.;Capelli, C.;Cardoso, J. M. R.;Cardoso, J. M. R.;Cichon, D.;Cichon, D.;Cimmino, B.;Cimmino, B.;Clark, M.;Clark, M.;Coderre, D.;Coderre, D.;Colijn, A. P.;Colijn, A. P.;Conrad, J.;Conrad, J.;Cuenca, J.;Cuenca, J.;Cussonneau, J. P.;Cussonneau, J. P.;Decowski, M. P.;Decowski, M. P.;Depoian, A.;Depoian, A.;Di Gangi, P.;Di Gangi, P.;Di Giovanni, A.;Di Giovanni, A.;Di Stefano, R.;Di Stefano, R.;Diglio, S.;Diglio, S.;Elykov, A.;Elykov, A.;Ferella, A. D.;Ferella, A. D.;Fulgione, W.;Fulgione, W.;Gaemers, P.;Gaemers, P.;Gaior, R.;Gaior, R.;Galloway, M.;Galloway, M.;Gao, F.;Gao, F.;Grandi, L.;Grandi, L.;Hils, C.;Hils, C.;Hiraide, K.;Hiraide, K.;Hoetzsch, L.;Hoetzsch, L.;Howlett, J.;Howlett, J.;Iacovacci, M.;Iacovacci, M.;Itow, Y.;Itow, Y.;Joerg, F.;Joerg, F.;Kato, N.;Kato, N.;Kazama, S.;Kazama, S.;Kobayashi, M.;Kobayashi, M.;Koltman, G.;Koltman, G.;Kopec, A.;Kopec, A.;Landsman, H.;Landsman, H.;Lang, R. F.;Lang, R. F.;Levinson, L.;Levinson, L.;Liang, S.;Liang, S.;Lin, Q.;Lin, Q.;Lindemann, S.;Lindemann, S.;Lindner, M.;Lindner, M.;Lombardi, F.;Lombardi, F.;Long, J.;Long, J.;Lopes, J. A. M.;Lopes, J. A. M.;Ma, Y.;Ma, Y.;Macolino, C.;Macolino, C.;Mahlstedt, J.;Mahlstedt, J.;Mancuso, A.;Mancuso, A.;Manenti, L.;Manenti, L.;Manfredini, A.;Manfredini, A.;Marignetti, F.;Marignetti, F.;Marrodán Undagoitia, T.;Marrodán Undagoitia, T.;Martens, K.;Martens, K.;Masbou, J.;Masbou, J.;Masson, D.;Masson, D.;Mastroianni, S.;Mastroianni, S.;Messina, M.;Messina, M.;Miuchi, K.;Miuchi, K.;Mizukoshi, K.;Mizukoshi, K.;Molinario, A.;Molinario, A.;Morå, K.;Morå, K.;Moriyama, S.;Moriyama, S.;Mosbacher, Y.;Mosbacher, Y.;Murra, M.;Murra, M.;Naganoma, J.;Naganoma, J.;Ni, K.;Ni, K.;Oberlack, U.;Oberlack, U.;Odgers, K.;Odgers, K.;Palacio, J.;Palacio, J.;Pelssers, B.;Pelssers, B.;Peres, R.;Peres, R.;Pienaar, J.;Pienaar, J.;Pierre, M.;Pierre, M.;Pizzella, V.;Pizzella, V.;Plante, G.;Plante, G.;Qi, J.;Qi, J.;Qin, J.;Qin, J.;Ramírez García, D.;Ramírez García, D.;Reichard, S.;Reichard, S.;Rocchetti, A.;Rocchetti, A.;Rupp, N.;Rupp, N.;dos Santos, J. M. F.;dos Santos, J. M. F.;Sartorelli, G.;Sartorelli, G.;Šarčević, N.;Šarčević, N.;Scheibelhut, M.;Scheibelhut, M.;Schreiner, J.;Schreiner, J.;Schulte, D.;Schulte, D.;Schulze Eißing, H.;Schulze Eißing, H.;Schumann, M.;Schumann, M.;Scotto Lavina, L.;Scotto Lavina, L.;Selvi, M.;Selvi, M.;Semeria, F.;Semeria, F.;Shagin, P.;Shagin, P.;Shockley, E.;Shockley, E.;Silva, M.;Silva, M.;Simgen, H.;Simgen, H.;Takeda, A.;Takeda, A.;Therreau, C.;Therreau, C.;Thers, D.;Thers, D.;Toschi, F.;Toschi, F.;Trinchero, G.;Trinchero, G.;Tunnell, C.;Tunnell, C.;Valerius, K.;Valerius, K.;Vargas, M.;Vargas, M.;Volta, G.;Volta, G.;Wei, Y.;Wei, Y.;Weinheimer, C.;Weinheimer, C.;Weiss, M.;Weiss, M.;Wenz, D.;Wenz, D.;Wittweg, C.;Wittweg, C.;Wolf, T.;Wolf, T.;Xu, Z.;Xu, Z.;Yamashita, M.;Yamashita, M.;Ye, J.;Ye, J.;Zavattini, G.;Zavattini, G.;Zhang, Y.;Zhang, Y.;Zhu, T.;Zhu, T.;Zopounidis, J. P.;Zopounidis, J. P.;
Physical review / D 2021 Vol. 103 pp. 063028-
167
collaboration2021physicalsearch

Abstract

We report the results of a search for the inelastic scattering of weakly interacting massive particles (WIMPs) in the XENON1T dark matter experiment. Scattering off 129Xe is the most sensitive probe of inelastic WIMP interactions, with a signature of a 39.6 keV deexcitation photon detected simultaneously with the nuclear recoil. Using an exposure of 0.83 tonne-years, we find no evidence of inelastic WIMP scattering with a significance of more than 2σ. A profile-likelihood ratio analysis is used to set upper limits on the cross section of WIMP-nucleus interactions. We exclude new parameter space for WIMPs heavier than 100  GeV/c2, with the strongest upper limit of 3.3×10−39  cm2 for 130  GeV/c2 WIMPs at 90% confidence level.

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