Parametrization and applications of the low- Q2 nucleon vector form factors

Kaushik Borah, Richard J. Hill, Gabriel Lee, Oleksandr Tomalak

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48 Scopus citations

Abstract

We present the proton and neutron vector form factors in a convenient parametric form that is optimized for momentum transfers few GeV2. The form factors are determined from a global fit to electron scattering data and precise charge radius measurements. A new treatment of radiative corrections is applied. This parametric representation of the form factors, uncertainties, and correlations provides an efficient means to evaluate many derived observables. We consider two classes of illustrative examples: neutrino-nucleon scattering cross sections at GeV energies for neutrino oscillation experiments and nucleon structure corrections for atomic spectroscopy. The neutrino-nucleon charged current quasielastic cross section differs by 3%-5% compared to commonly used form factor models when the vector form factors are constrained by recent high-statistics electron-proton scattering data from the A1 Collaboration. Nucleon structure parameter determinations include: the magnetic and Zemach radii of the proton and neutron, [rMp,rMn]=[0.739(41)(23),0.776(53)(28)] fm and [rZp,rZn]=[1.0227(94)(51),-0.0445(14)(3)] fm; the Friar radius of nucleons, [(rFp)3,(rFn)3]=[2.246(58)(2),0.0093(6)(1)] fm3; the electric curvatures, [r4Ep,r4En]=[1.08(28)(5),-0.33(24)(3)] fm4; and bounds on the magnetic curvatures, [r4Mp,r4Mn]=[-2.0(1.7)(0.8),-2.3(2.1)(1.1)] fm4. The first and dominant uncertainty is propagated from the experimental data and radiative corrections, and the second error is due to the fitting procedure.

Original languageEnglish
Article number074012
JournalPhysical Review D
Volume102
Issue number7
DOIs
StatePublished - Oct 20 2020

Bibliographical note

Publisher Copyright:
© 2020 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

R. J. H. and G. L. thank J. Arrington and Z. Ye for many discussions and collaboration on Refs. which inspired the present work. Similarly, R. J. H. thanks M. Betancourt, R. Gran, and A. Meyer for discussion and collaboration on Ref. . The research of K. B., R. J. H., and O. T. is supported by the U.S. Department of Energy, Office of Science, Office of High Energy Physics, under Award No. DE-SC0019095. Fermilab is operated by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy. G. L. acknowledges support by the Samsung Science & Technology Foundation under Project No. SSTF-BA1601-07, a Korea University Grant, and the support of the U.S. National Science Foundation through Grant No. PHY-1719877. G. L. is grateful to the Technion–Israel Institute of Technology, the Fermilab theory group, and the Mainz Institute for Theoretical Physics (MITP) for hospitality and partial support during completion of this work. O. T. acknowledges the Fermilab theory group and the theory group of Institute for Nuclear Physics at Johannes Gutenberg-Universität Mainz for warm hospitality and support. The work of O. T. is supported by the Visiting Scholars Award Program of the Universities Research Association. The research of K.B., R.J.H., and O.T. is supported by the U.S. Department of Energy, Office of Science, Office of High Energy Physics, under Award No. DE-SC0019095. Fermilab is operated by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy. G.L. acknowledges support by the Samsung Science & Technology Foundation under Project No. SSTF-BA1601-07, a Korea University Grant, and the support of the U.S. National Science Foundation through Grant No. PHY-1719877. G.L. is grateful to the Technion-Israel Institute of Technology, the Fermilab theory group, and the Mainz Institute for Theoretical Physics (MITP) for hospitality and partial support during completion of this work. O.T. acknowledges the Fermilab theory group and the theory group of Institute for Nuclear Physics at Johannes Gutenberg-Universit?t Mainz for warm hospitality and support. The work of O.T. is supported by the Visiting Scholars Award Program of the Universities Research Association.

FundersFunder number
Fermi Research Alliance, LLCDE-AC02-07CH11359
Technion - Israel Institute of Technology
Universities Space Research Association
U.S. Department of Energy Chinese Academy of Sciences Guangzhou Municipal Science and Technology Project Oak Ridge National Laboratory Extreme Science and Engineering Discovery Environment National Science Foundation National Energy Research Scientific Computing Center National Natural Science Foundation of ChinaPHY-1719877
U.S. Department of Energy Chinese Academy of Sciences Guangzhou Municipal Science and Technology Project Oak Ridge National Laboratory Extreme Science and Engineering Discovery Environment National Science Foundation National Energy Research Scientific Computing Center National Natural Science Foundation of China
U.S. Department of Energy Oak Ridge National Laboratory U.S. Department of Energy National Science Foundation National Energy Research Scientific Computing Center
Kavli Institute for Theoretical Physics, University of California, Santa Barbara
National Science Foundation Office of International Science and Engineering
Department of Energy offices of High Energy Physics and Nuclear PhysicsDE-SC0019095
Department of Energy offices of High Energy Physics and Nuclear Physics
Korea University
Technion - Israel Institute of Technology
Samsung Science and Technology FoundationSSTF-BA1601-07
Samsung Science and Technology Foundation

    ASJC Scopus subject areas

    • Nuclear and High Energy Physics

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