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 language | English |
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Article number | 074012 |
Journal | Physical Review D |
Volume | 102 |
Issue number | 7 |
DOIs | |
State | Published - 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.
Funders | Funder number |
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Fermi Research Alliance, LLC | DE-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 China | PHY-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 Physics | DE-SC0019095 |
Department of Energy offices of High Energy Physics and Nuclear Physics | |
Korea University | |
Technion - Israel Institute of Technology | |
Samsung Science and Technology Foundation | SSTF-BA1601-07 |
Samsung Science and Technology Foundation |
ASJC Scopus subject areas
- Nuclear and High Energy Physics