@article{e862ed8761ce445690b0ed398bc0e80b,
title = "Search for Coherent Elastic Scattering of Solar B 8 Neutrinos in the XENON1T Dark Matter Experiment",
abstract = "We report on a search for nuclear recoil signals from solar B8 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 B8 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.",
author = "{(XENON Collaboration)} and E. Aprile and J. Aalbers and F. Agostini and {Ahmed Maouloud}, S. and M. Alfonsi and L. Althueser and Amaro, {F. D.} and S. Andaloro and Antochi, {V. C.} and E. Angelino and Angevaare, {J. R.} and F. Arneodo and L. Baudis and B. Bauermeister and L. Bellagamba and Benabderrahmane, {M. L.} and A. Brown and E. Brown and S. Bruenner and G. Bruno and R. Budnik and C. Capelli and Cardoso, {J. M.R.} and D. Cichon and B. Cimmino and M. Clark and D. Coderre and Colijn, {A. P.} and J. Conrad and J. Cuenca and Cussonneau, {J. P.} and Decowski, {M. P.} and A. Depoian and {Di Gangi}, P. and {Di Giovanni}, A. and {Di Stefano}, R. and S. Diglio and A. Elykov and Ferella, {A. D.} and W. Fulgione and P. Gaemers and R. Gaior and M. Galloway and F. Gao and L. Grandi and C. Hils and K. Hiraide and L. Hoetzsch and J. Howlett and M. Iacovacci",
note = "Funding Information: We would like to thank Matthew Szydagis and Ekaterina Kozlova for useful discussions concerning the NEST model. We gratefully acknowledge support from the National Science Foundation, Swiss National Science Foundation, German Ministry for Education and Research, Max Planck Gesellschaft, Deutsche Forschungsgemeinschaft, Helmholtz Association, Netherlands Organisation for Scientific Research (NWO), Weizmann Institute of Science, ISF, Fundacao para a Ciencia e a Tecnologia, Rgion des Pays de la Loire, Knut and Alice Wallenberg Foundation, Kavli Foundation, JSPS Kakenhi in Japan and Istituto Nazionale di Fisica Nucleare. This project has received funding or support from the European Unions Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Grant Agreements No. 690575 and No. 674896, respectively. Data processing is performed using infrastructures from the Open Science Grid, the European Grid Initiative, and the Dutch national e-infrastructure with the support of SURF Cooperative. We are grateful to Laboratori Nazionali del Gran Sasso for hosting and supporting the XENON project. Publisher Copyright: {\textcopyright} 2021 authors.",
year = "2021",
month = mar,
day = "1",
doi = "10.1103/PhysRevLett.126.091301",
language = "English (US)",
volume = "126",
journal = "Physical Review Letters",
issn = "0031-9007",
publisher = "American Physical Society",
number = "9",
}