Published August 1, 2011
| Version v1
Journal article
Covariant model for the γN→N(1535) transition at high momentum transfer
Creators
- 1. CFTP, Instituto Superior Tecnico, Universidade Tecnica de Lisboa, Av. Rovisco Pais, 1049-001 Lisboa (Portugal)
- 2. Dep. Fisica, Instituto Superior Tecnico, Universidade Tecnica de Lisboa, Av. Rovisco Pais, 1049-001 Lisboa (Portugal)
Description
A relativistic constituent quark model is applied to the γN→N(1535) transition. The N(1535) wave function is determined by extending the covariant spectator quark model, previously developed for the nucleon, to the S11 resonance. The model allows us to calculate the valence quark contributions to the γN→N(1535) transition form factors. Because of the nucleon and N(1535) structure the model is valid only for Q2>2.3 GeV2. The results are compared with the experimental data for the electromagnetic form factors F1* and F2* and the helicity amplitudes A1/2 and S1/2, at high Q2.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.84.033007;
- arXiv
- arXiv:1105.2223v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 84
- Journal Issue
- 3
- Journal Page Range
- p. 033007-033007.17
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43079613
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- ELECTROMAGNETIC FORM FACTORS; MOMENTUM TRANSFER; N-1535 BARYONS; NUCLEONS; PHOTON-NUCLEON INTERACTIONS; QUARK MODEL; QUARKS; RELATIVISTIC RANGE; RESONANCE; WAVE FUNCTIONS
- Descriptors DEC
- BARYONS; BASIC INTERACTIONS; COMPOSITE MODELS; DIMENSIONLESS NUMBERS; ELECTROMAGNETIC INTERACTIONS; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; FORM FACTORS; FUNCTIONS; HADRONS; INTERACTIONS; MATHEMATICAL MODELS; N BARYONS; N*BARYONS; PARTICLE INTERACTIONS; PARTICLE MODELS; PARTICLE PROPERTIES; PHOTON-BARYON INTERACTIONS; PHOTON-HADRON INTERACTIONS
Optional Information
- Notes
- (c) 2011 American Institute of Physics