Abstract
Precision measurements of antineutrino elastic scattering on hydrogen from future neutrino experiments offer a unique opportunity to access the low-energy structure of protons and neutrons. We discuss the determination of the nucleon axial-vector form factor and radius from antineutrino interactions on hydrogen that can be collected at the future Long-Baseline Neutrino Facility and study the sources of theoretical and experimental uncertainties. The projected accuracy would improve existing measurements by 1 order of magnitude and be competitive with contemporary lattice-QCD determinations, potentially helping to resolve the corresponding tension with measurements from (anti)neutrino elastic scattering on deuterium. We find that the current knowledge of the nucleon vector form factors could be one of the dominant sources of uncertainty. We also evaluate the constraints that can be simultaneously obtained on the absolute ν¯μ flux normalization.
| Original language | English |
|---|---|
| Article number | L051301 |
| Journal | Physical Review D |
| Volume | 109 |
| Issue number | 5 |
| DOIs | |
| State | Published - Mar 1 2024 |
Bibliographical note
Publisher Copyright:© 2024 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/"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.
Funding
O. T. acknowledges useful discussions with Aaron Meyer, Kevin McFarland, and Clarence Wret. Research of R. J. H. is supported by the U.S. Department of Energy, Office of Science, Office of High Energy Physics, under Award No. DE-SC0019095. This work is supported by the U.S. Department of Energy through the Los Alamos National Laboratory. Los Alamos National Laboratory is operated by Triad National Security, LLC, for the National Nuclear Security Administration of U.S. Department of Energy (Award No. 89233218CNA000001). This research is funded by LANL’s Laboratory Directed Research and Development (LDRD/PRD) program under projects 20210968PRD4, 20210190ER, and 20240127ER. R. P. is thankful for support from the CERN neutrino platform. This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics. For facilitating portions of this research, O. T. wishes to acknowledge the Center for Theoretical Underground Physics and Related Areas (CETUP*), The Institute for Underground Science at Sanford Underground Research Facility (SURF), and the South Dakota Science and Technology Authority for hospitality and financial support.
| Funders | Funder number |
|---|---|
| Fermi Research Alliance, LLC | DE-AC02-07CH11359 |
| South Dakota Science and Technology Authority | |
| U.S. Department of Energy EPSCoR | |
| Office of Science Programs | |
| Institute for High Energy Physics | DE-SC0019095 |
| Laboratory Directed Research and Development | 20210968PRD4, 20210190ER, 20240127ER |
| Los Alamos National Laboratory | |
| CERN |
ASJC Scopus subject areas
- Nuclear and High Energy Physics
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