Solar neutrino detection sensitivity in DARWIN via electron scattering

dc.contributor.authorDARWIN Collaboration
dc.contributor.authorOstrovskiy, I.
dc.contributor.otherOskar Klein Centre
dc.contributor.otherStockholm University
dc.contributor.otherUniversity of Bologna
dc.contributor.otherIstituto Nazionale di Fisica Nucleare (INFN)
dc.contributor.otherCentre National de la Recherche Scientifique (CNRS)
dc.contributor.otherCNRS - National Institute of Nuclear and Particle Physics (IN2P3)
dc.contributor.otherUDICE-French Research Universities
dc.contributor.otherSorbonne Universite
dc.contributor.otherUniversite Paris Cite
dc.contributor.otherJohannes Gutenberg University of Mainz
dc.contributor.otherUniversity of Munster
dc.contributor.otherUniversidade de Coimbra
dc.contributor.otherFOM National Institute for Subatomic Physics
dc.contributor.otherUniversity of Amsterdam
dc.contributor.otherUniversity of Belgrade
dc.contributor.otherColumbia University
dc.contributor.otherWeizmann Institute of Science
dc.contributor.otherHelmholtz Association
dc.contributor.otherKarlsruhe Institute of Technology
dc.contributor.otherUniversity of Zurich
dc.contributor.otherUniversity of Freiburg
dc.contributor.otherUniversite Paris Saclay
dc.contributor.otherRensselaer Polytechnic Institute
dc.contributor.otherMax Planck Society
dc.contributor.otherPurdue University System
dc.contributor.otherPurdue University
dc.contributor.otherPurdue University West Lafayette Campus
dc.contributor.otherIMT - Institut Mines-Telecom
dc.contributor.otherIMT Atlantique
dc.contributor.otherNantes Universite
dc.contributor.otherUniversity of L'Aquila
dc.contributor.otherGran Sasso Science Institute (GSSI)
dc.contributor.otherRuprecht Karls University Heidelberg
dc.contributor.otherUniversity of Chicago
dc.contributor.otherUniversity of California System
dc.contributor.otherUniversity of California San Diego
dc.contributor.otherUniversity of Melbourne
dc.contributor.otherUniversity of Alabama Tuscaloosa
dc.contributor.otherRice University
dc.contributor.otherImperial College London
dc.contributor.otherTechnische Universitat Dresden
dc.contributor.otherUniversity of Banja Luka (UNIBL)
dc.contributor.otherUtrecht University
dc.contributor.otherInternational School for Advanced Studies (SISSA)
dc.date.accessioned2022-08-02T15:11:22Z
dc.date.available2022-08-02T15:11:22Z
dc.date.issued2020
dc.description.abstractWe detail the sensitivity of the proposed liquid xenon DARWIN observatory to solar neutrinos via elastic electron scattering. We find that DARWIN will have the potential to measure the fluxes of five solar neutrino components: pp, \({}^{7}\)Be, \({}^{13}\)N, \({}^{15}\)O and pep. The precision of the \({}^{13}\)N, \({}^{15}\)O and pep components is hindered by the double-beta decay of \({}^{136}\)Xe and, thus, would benefit from a depleted target. A high-statistics observation of pp neutrinos would allow us to infer the values of the electroweak mixing angle, \({sin}^{2}{\theta }_{w}\), and the electron-type neutrino survival probability, \({P}_{\mathrm{ee}}\), in the electron recoil energy region from a few keV up to 200 keV for the first time, with relative precision of 5% and 4%, respectively, with 10 live years of data and a 30 tonne fiducial volume. An observation of \(pp\) and \({}^{7}\)Be neutrinos would constrain the neutrino-inferred solar luminosity down to 0.2%. A combination of all flux measurements would distinguish between the high- (GS98) and low-metallicity (AGS09) solar models with 2.1–2.5\(\sigma \) significance, independent of external measurements from other experiments or a measurement of \({}^{8}\)B neutrinos through coherent elastic neutrino-nucleus scattering in DARWIN. Finally, we demonstrate that with a depleted target DARWIN may be sensitive to the neutrino capture process of \({}^{131}\)Xe.en_US
dc.format.mimetypeapplication/pdf
dc.identifier.citationAalbers, J., Agostini, F., Maouloud, S. E. M. A., Alfonsi, M., Althueser, L., Amaro, F. D., Angevaare, J., Antochi, V. C., Antunovic, B., Aprile, E., Arazi, L., Arneodo, F., Balzer, M., Baudis, L., Baur, D., Benabderrahmane, M. L., Biondi, Y., Bismark, A., … Zuber, K. (2020). Solar neutrino detection sensitivity in DARWIN via electron scattering. In The European Physical Journal C (Vol. 80, Issue 12). Springer Science and Business Media LLC. https://doi.org/10.1140/epjc/s10052-020-08602-7
dc.identifier.doi10.1140/epjc/s10052-020-08602-7
dc.identifier.orcidhttps://orcid.org/0000-0003-4939-0225
dc.identifier.urihttps://ir.ua.edu/handle/123456789/8656
dc.languageEnglish
dc.language.isoen_US
dc.publisherSpringer
dc.rights.urihttps://creativecommons.org/licenses//by/4.0
dc.subjectXENON
dc.subjectPhysics, Particles & Fields
dc.subjectPhysics
dc.titleSolar neutrino detection sensitivity in DARWIN via electron scatteringen_US
dc.typetext
dc.typeArticle
Files
Original bundle
Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
Aalbers2020.pdf
Size:
626.23 KB
Format:
Adobe Portable Document Format