Nucleon form factors to next-to-leading order with light-cone sum rules
Creators
- 1. Theoretical Physics Division, Rudjer Boskovic Institute, P.O. Box 180, HR-10002 Zagreb (Croatia)
- 2. Institut fuer Theoretische Physik, Universitaet Regensburg, D-93040 Regensburg (Germany)
Description
We have calculated the leading-twist next-to-leading order (NLO), i.e., O(αs), correction to the light-cone sum rules prediction for the electromagnetic form factors of the nucleon. We have used the Ioffe nucleon interpolation current and worked in MN=0 approximation, with MN being the mass of the nucleon. In this approximation, only the Pauli form factor F2 receives a correction and the calculated correction is quite sizable (ca. 60%). The numerical results for the proton form factors show the improved agreement with the experimental data. We also discuss the problems encountered when going away from MN=0 approximation at NLO, as well as gauge invariance of the perturbative results. This work presents the first step towards the NLO accuracy in the light-cone sum rules for baryon form factors.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.78.033009;
- arXiv
- arXiv:0805.1758v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 78
- Journal Issue
- 3
- Journal Page Range
- p. 033009-033009.36
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41001928
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- APPROXIMATIONS; BARYONS; COMPUTERIZED SIMULATION; CORRECTIONS; ELECTROMAGNETIC FORM FACTORS; FORECASTING; GAUGE INVARIANCE; INTERPOLATION; LIGHT CONE; MASS; PAULI FORM FACTORS; PROTONS; SUM RULES
- Descriptors DEC
- BARYONS; CALCULATION METHODS; DIMENSIONLESS NUMBERS; ELEMENTARY PARTICLES; EQUATIONS; FERMIONS; FORM FACTORS; HADRONS; INVARIANCE PRINCIPLES; MATHEMATICAL SOLUTIONS; NUCLEONS; NUMERICAL SOLUTION; PARTICLE PROPERTIES; SIMULATION; SPACE-TIME
Optional Information
- Notes
- (c) 2008 The American Physical Society