• Open Access

Inelastic nuclear scattering from neutrinos and dark matter

Bhaskar Dutta, Wei-Chih Huang, Jayden L. Newstead, and Vishvas Pandey
Phys. Rev. D 106, 113006 – Published 21 December 2022

Abstract

Neutrinos with energy of order 10 MeV, such as from pion decay-at-rest sources, are an invaluable tool for studying low-energy neutrino interactions with nuclei—previously enabling the first measurement of coherent elastic neutrino-nucleus scattering. Beyond elastic scattering, neutrinos and dark matter in this energy range also excite nuclei to its low-lying nuclear states, providing an additional physics channel. Here, we consider neutral-current inelastic neutrino-nucleus and dark matter (DM)-nucleus scattering off Ar40, Cs133, and I127 nuclei that are relevant to a number of low-threshold neutrino experiments at pion decay-at-rest facilities. We carry out large scale nuclear shell model calculations of the inelastic cross sections considering the full set of electroweak multipole operators. Our results demonstrate that Gamow-Teller transitions provide the dominant contribution to the cross section and that the long-wavelength limit provides a reasonable approximation to the total cross section for neutrino sources. We show that future experiments will be sensitive to this channel, and thus these results provide additional neutrino and DM scattering channels to explore at pion decay-at-rest facilities.

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  • Received 26 June 2022
  • Accepted 1 December 2022

DOI:https://doi.org/10.1103/PhysRevD.106.113006

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsNuclear Physics

Authors & Affiliations

Bhaskar Dutta1,*, Wei-Chih Huang1,†, Jayden L. Newstead2,‡, and Vishvas Pandey3,4,§

  • 1Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
  • 2ARC Centre of Excellence for Dark Matter Particle Physics, School of Physics, University of Melbourne, Victoria 3010, Australia
  • 3Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
  • 4Department of Physics, University of Florida, Gainesville, Florida 32611, USA

  • *dutta@physics.tamu.edu
  • s104021230@tamu.edu
  • jnewstead@unimelb.edu.au
  • §vpandey@fnal.gov

Article Text

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Issue

Vol. 106, Iss. 11 — 1 December 2022

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