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Search for Coherent Elastic Scattering of Solar $^8$B Neutrinos in the XENON1T Dark Matter Experiment

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arxiv 2012.02846 v2 pith:H3BN4BWR submitted 2020-12-04 hep-ex

E. Aprile , J. Aalbers , F. Agostini , S. Ahmed Maouloud , M. Alfonsi , L. Althueser , F. D. Amaro , S. Andaloro
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V. C. Antochi E. Angelino J. R. Angevaare F. Arneodo L. Baudis B. Bauermeister L. Bellagamba M. L. Benabderrahmane A. Brown E. Brown S. Bruenner G. Bruno R. Budnik C. Capelli J. M. R. Cardoso D. Cichon B. Cimmino M. Clark D. Coderre A. P. Colijn J. Conrad J. Cuenca J. P. Cussonneau M. P. Decowski A. Depoian P. Di Gangi A. Di Giovanni R. Di Stefano S. Diglio A. Elykov A. D. Ferella W. Fulgione P. Gaemers R. Gaior M. Galloway F. Gao L. Grandi C. Hils K. Hiraide L. Hoetzsch J. Howlett M. Iacovacci Y. Itow F. Joerg N. Kato S. Kazama M. Kobayashi G. Koltman A. Kopec H. Landsman R. F. Lang L. Levinson S. Liang S. Lindemann M. Lindner F. Lombardi J. Long J. A. M. Lopes Y. Ma C. Macolino J. Mahlstedt A. Mancuso L. Manenti A. Manfredini F. Marignetti T. Marrodán Undagoitia K. Martens J. Masbou D. Masson S. Mastroianni M. Messina K. Miuchi K. Mizukoshi A. Molinario K. Mor{aa} S. Moriyama Y. Mosbacher M. Murra J. Naganoma K. Ni U. Oberlack K. Odgers J. Palacio B. Pelssers R. Peres M. Pierre J. Pienaar V. Pizzella G. Plante J. Qi J. Qin D. Ramírez García S. Reichard A. Rocchetti N. Rupp J. M. F. dos Santos G. Sartorelli J. Schreiner D. Schulte H. Schulze Ei{ss}ing M. Schumann L. Scotto Lavina M. Selvi F. Semeria P. Shagin E. Shockley M. Silva H. Simgen A. Takeda C. Therreau D. Thers F. Toschi G. Trinchero C. Tunnell K. Valerius M. Vargas G. Volta Y. Wei C. Weinheimer M. Weiss D. Wenz C. Wittweg T. Wolf Z. Xu M. Yamashita J. Ye G. Zavattini Y. Zhang T. Zhu J. P. Zopounidis
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classification hep-ex
keywords darkneutrinossolarinteractionsmatternuclearscatteringsearch
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We report on a search for nuclear recoil signals from solar $^8$B neutrinos elastically scattering off xenon nuclei in XENON1T data, lowering the energy threshold from 2.6 keV to 1.6 keV. We develop a variety of novel techniques to limit the resulting increase in backgrounds near the threshold. No significant $^8$B neutrino-like excess is found in an exposure of 0.6 t $\times$ y. For the first time, we use the non-detection of solar neutrinos to constrain the light yield from 1-2 keV nuclear recoils in liquid xenon, as well as non-standard neutrino-quark interactions. Finally, we improve upon world-leading constraints on dark matter-nucleus interactions for dark matter masses between 3 GeV/c$^2$ and 11 GeV/c$^2$ by as much as an order of magnitude.

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