| Literature DB >> 33750173 |
E Aprile1, J Aalbers2, F Agostini3, S Ahmed Maouloud4, M Alfonsi5, L Althueser6, F D Amaro7, S Andaloro8, V C Antochi2, E Angelino9, J R Angevaare10, F Arneodo11, L Baudis12, B Bauermeister2, L Bellagamba3, M L Benabderrahmane11, A Brown12, E Brown13, S Bruenner10, G Bruno11, R Budnik14, C Capelli12, J M R Cardoso7, D Cichon15, B Cimmino16, M Clark17, D Coderre18, A P Colijn10, J Conrad2, J Cuenca19, J P Cussonneau20, M P Decowski10, A Depoian17, P Di Gangi3, A Di Giovanni11, R Di Stefano16, S Diglio20, A Elykov18, A D Ferella21,22, W Fulgione9,22, P Gaemers10, R Gaior4, M Galloway12, F Gao1,23, L Grandi24, C Hils5, K Hiraide25, L Hoetzsch15, J Howlett1, M Iacovacci16, Y Itow26, F Joerg15, N Kato25, S Kazama26, M Kobayashi1, G Koltman14, A Kopec17, H Landsman14, R F Lang17, L Levinson14, S Liang8, S Lindemann18, M Lindner15, F Lombardi7, J Long24, J A M Lopes7, Y Ma27, C Macolino28, J Mahlstedt2, A Mancuso3, L Manenti11, A Manfredini12, F Marignetti16, T Marrodán Undagoitia15, K Martens25, J Masbou20, D Masson18, S Mastroianni16, M Messina22, K Miuchi29, K Mizukoshi29, A Molinario22, K Morå1, S Moriyama25, Y Mosbacher14, M Murra6, J Naganoma22, K Ni27, U Oberlack5, K Odgers13, J Palacio15,20, B Pelssers2, R Peres12, M Pierre20, J Pienaar24, V Pizzella15, G Plante1, J Qi27, J Qin17, D Ramírez García18, S Reichard19, A Rocchetti18, N Rupp15, J M F Dos Santos7, G Sartorelli3, J Schreiner15, D Schulte6, H Schulze Eißing6, M Schumann18, L Scotto Lavina4, M Selvi3, F Semeria3, P Shagin8, E Shockley24,27, M Silva7, H Simgen15, A Takeda25, C Therreau20, D Thers20, F Toschi18, G Trinchero9, C Tunnell8, K Valerius19, M Vargas6, G Volta12, Y Wei27, C Weinheimer6, M Weiss14, D Wenz5, C Wittweg6, T Wolf15, Z Xu1, M Yamashita26, J Ye1,27, G Zavattini3, Y Zhang1, T Zhu1, J P Zopounidis4.
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 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 neutrinolike excess is found in an exposure of 0.6 t×y. For the first time, we use the nondetection of solar neutrinos to constrain the light yield from 1-2 keV nuclear recoils in liquid xenon, as well as nonstandard neutrino-quark interactions. Finally, we improve upon world-leading constraints on dark matter-nucleus interactions for dark matter masses between 3 and 11 GeV c^{-2} by as much as an order of magnitude.Entities:
Year: 2021 PMID： 33750173 DOI： 10.1103/PhysRevLett.126.091301
Source DB: PubMed Journal: Phys Rev Lett ISSN： 0031-9007 Impact factor: 9.161