Axial N→Δ(1232) and N→N*(1440) transition form factors
- 1. Grupo de Fisica Nuclear, Departamento de Fisica Fundamental e IUFFyM, Facultad de Ciencias, E-37008 Salamanca (Spain)
- 2. Institut fuer Theoretische Physik, Universitaet Tuebingen, Auf der Morgenstelle 14, D-72076 Tuebingen (Germany)
Description
We calculate the axial N→Δ(1232) and N→N*(1440) transition form factors in a chiral constituent quark model. As required by the partial conservation of axial current (PCAC) condition, we include one- and two-body axial exchange currents. We compare the axial N→Δ(1232) form factors with previous quark model calculations that use only one-body axial currents, and with experimental analyses. The paper provides the first calculation of all weak axial N→N*(1440) form factors. Our main result is that exchange currents are very important for certain axial transition form factors. In addition to improving our understanding of nucleon structure, the present results are relevant to the neutrino-nucleus scattering cross section predictions needed in the analysis of neutrino mixing experiments
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.75.065203;
- arXiv
- arXiv:0705.3297v3;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 75
- Journal Issue
- 6
- Journal Page Range
- p. 065203-065203.11
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39027620
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CHIRALITY; COMPARATIVE EVALUATIONS; CROSS SECTIONS; CURRENTS; FORECASTING; FORM FACTORS; NEUTRINOS; NUCLEONS; QUARK MODEL; TWO-BODY PROBLEM
- Descriptors DEC
- BARYONS; COMPOSITE MODELS; DIMENSIONLESS NUMBERS; ELEMENTARY PARTICLES; EVALUATION; FERMIONS; HADRONS; LEPTONS; MANY-BODY PROBLEM; MASSLESS PARTICLES; MATHEMATICAL MODELS; PARTICLE MODELS; PARTICLE PROPERTIES
Optional Information
- Notes
- (c) 2007 The American Physical Society