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Measurement of the axial vector form factor from antineutrino-proton scattering.
Cai, T; Moore, M L; Olivier, A; Akhter, S; Dar, Z Ahmad; Ansari, V; Ascencio, M V; Bashyal, A; Bercellie, A; Betancourt, M; Bodek, A; Bonilla, J L; Bravar, A; Budd, H; Caceres, G; Carneiro, M F; Díaz, G A; da Motta, H; Felix, J; Fields, L; Filkins, A; Fine, R; Gago, A M; Gallagher, H; Gilligan, S M; Gran, R; Granados, E; Harris, D A; Henry, S; Jena, D; Jena, S; Kleykamp, J; Klustová, A; Kordosky, M; Last, D; Le, T; Lozano, A; Lu, X-G; Maher, E; Manly, S; Mann, W A; Mauger, C; McFarland, K S; Messerly, B; Miller, J; Moreno, O; Morfín, J G; Naples, D; Nelson, J K; Nguyen, C.
Affiliation
  • Cai T; Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA. tejinc@yorku.ca.
  • Moore ML; Department of Physics and Astronomy, York University, Toronto, Ontario, Canada. tejinc@yorku.ca.
  • Olivier A; Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA.
  • Akhter S; Department of Physics, Stanford University, Stanford, CA, USA.
  • Dar ZA; Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA.
  • Ansari V; AMU Campus, Aligarh, India.
  • Ascencio MV; AMU Campus, Aligarh, India.
  • Bashyal A; Department of Physics, William & Mary, Williamsburg, VA, USA.
  • Bercellie A; AMU Campus, Aligarh, India.
  • Betancourt M; Sección Física, Departamento de Ciencias, Pontificia Universidad Católica del Perú, Lima, Peru.
  • Bodek A; Iowa State University, Ames, IA, USA.
  • Bonilla JL; Department of Physics, Oregon State University, Corvallis, OR, USA.
  • Bravar A; High Energy Physics/Center for Computational Excellence Department, Argonne National Laboratory, Lemont, IL, USA.
  • Budd H; Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA.
  • Caceres G; Fermi National Accelerator Laboratory, Batavia, IL, USA.
  • Carneiro MF; Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA.
  • Díaz GA; Campus León y Campus Guanajuato, Universidad de Guanajuato, Guanajuato, Mexico.
  • da Motta H; University of Geneva, Geneva, Switzerland.
  • Felix J; Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA.
  • Fields L; Centro Brasileiro de Pesquisas Físicas, Rio de Janeiro, Brazil.
  • Filkins A; Department of Physics and Astronomy, University of California at Davis, Davis, CA, USA.
  • Fine R; Department of Physics, Oregon State University, Corvallis, OR, USA.
  • Gago AM; Centro Brasileiro de Pesquisas Físicas, Rio de Janeiro, Brazil.
  • Gallagher H; Brookhaven National Laboratory, Upton, NY, USA.
  • Gilligan SM; Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA.
  • Gran R; Centro Brasileiro de Pesquisas Físicas, Rio de Janeiro, Brazil.
  • Granados E; Campus León y Campus Guanajuato, Universidad de Guanajuato, Guanajuato, Mexico.
  • Harris DA; Department of Physics, University of Notre Dame, Notre Dame, IN, USA.
  • Henry S; Department of Physics, William & Mary, Williamsburg, VA, USA.
  • Jena D; Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA.
  • Jena S; Los Alamos National Laboratory, Los Alamos, NM, USA.
  • Kleykamp J; Sección Física, Departamento de Ciencias, Pontificia Universidad Católica del Perú, Lima, Peru.
  • Klustová A; Physics Department, Tufts University, Medford, MA, USA.
  • Kordosky M; Department of Physics, Oregon State University, Corvallis, OR, USA.
  • Last D; Department of Physics, University of Minnesota - Duluth, Duluth, MN, USA.
  • Le T; Campus León y Campus Guanajuato, Universidad de Guanajuato, Guanajuato, Mexico.
  • Lozano A; Department of Physics and Astronomy, York University, Toronto, Ontario, Canada.
  • Lu XG; Fermi National Accelerator Laboratory, Batavia, IL, USA.
  • Maher E; Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA.
  • Manly S; Fermi National Accelerator Laboratory, Batavia, IL, USA.
  • Mann WA; Department of Physical Sciences, IISER Mohali, Mohali, India.
  • Mauger C; Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA.
  • McFarland KS; Department of Physics and Astronomy, University of Mississippi, Oxford, MS, USA.
  • Messerly B; The Blackett Laboratory, Imperial College London, London, UK.
  • Miller J; Department of Physics, William & Mary, Williamsburg, VA, USA.
  • Moreno O; Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA, USA.
  • Morfín JG; Physics Department, Tufts University, Medford, MA, USA.
  • Naples D; Centro Brasileiro de Pesquisas Físicas, Rio de Janeiro, Brazil.
  • Nelson JK; Department of Physics, University of Warwick, Coventry, UK.
  • Nguyen C; Department of Physics, University of Oxford, Oxford, UK.
Nature ; 614(7946): 48-53, 2023 02.
Article in En | MEDLINE | ID: mdl-36725994
ABSTRACT
Scattering of high energy particles from nucleons probes their structure, as was done in the experiments that established the non-zero size of the proton using electron beams1. The use of charged leptons as scattering probes enables measuring the distribution of electric charges, which is encoded in the vector form factors of the nucleon2. Scattering weakly interacting neutrinos gives the opportunity to measure both vector and axial vector form factors of the nucleon, providing an additional, complementary probe of their structure. The nucleon transition axial form factor, FA, can be measured from neutrino scattering from free nucleons, νµn → µ-p and [Formula see text], as a function of the negative four-momentum transfer squared (Q2). Up to now, FA(Q2) has been extracted from the bound nucleons in neutrino-deuterium scattering3-9, which requires uncertain nuclear corrections10. Here we report the first high-statistics measurement, to our knowledge, of the [Formula see text] cross-section from the hydrogen atom, using the plastic scintillator target of the MINERvA11 experiment, extracting FA from free proton targets and measuring the nucleon axial charge radius, rA, to be 0.73 ± 0.17 fm. The antineutrino-hydrogen scattering presented here can access the axial form factor without the need for nuclear theory corrections, and enables direct comparisons with the increasingly precise lattice quantum chromodynamics computations12-15. Finally, the tools developed for this analysis and the result presented are substantial advancements in our capabilities to understand the nucleon structure in the weak sector, and also help the current and future neutrino oscillation experiments16-20 to better constrain neutrino interaction models.

Full text: 1 Collection: 01-internacional Database: MEDLINE Type of study: Prognostic_studies Language: En Journal: Nature Year: 2023 Document type: Article Affiliation country:

Full text: 1 Collection: 01-internacional Database: MEDLINE Type of study: Prognostic_studies Language: En Journal: Nature Year: 2023 Document type: Article Affiliation country: