Published August 2009
| Version v1
Journal article
Exclusive photoproduction of f1(1285) meson off the proton in kinematics available at the Jefferson Laboratory experimental facilities
Creators
- 1. Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna, RU-141980 Moscow region (Russian Federation)
- 2. Istituto Nazionale di Fisica Nucleare, I-16146 Genova (Italy)
Description
We calculated the exclusive f1(1285) meson photoproduction cross section at an energy of a few GeV within the Regge approach. The calculation shows that the cross section is sizable, being in the range of 100 nb, and much larger than the expected cross section of the η(1295) meson photoproduction at the same energy. These two facts make it possible to use this reaction to study the poor known properties of the f1(1285) meson in the JLab kinematics.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.80.025201;
- arXiv
- arXiv:0903.5369v2;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 80
- Journal Issue
- 2
- Journal Page Range
- p. 025201-025201.4
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41037464
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CEBAF ACCELERATOR; COMPUTERIZED SIMULATION; CROSS SECTIONS; ETA-1295 MESONS; F1-1285 MESONS; GEV RANGE 01-10; NIOBIUM 100; PHOTOPRODUCTION; PROTONS
- Descriptors DEC
- ACCELERATORS; AXIAL VECTOR MESONS; BARYONS; BASIC INTERACTIONS; BETA DECAY RADIOISOTOPES; BETA-MINUS DECAY RADIOISOTOPES; BOSONS; ELECTROMAGNETIC INTERACTIONS; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; GEV RANGE; HADRONS; INTERACTIONS; INTERMEDIATE MASS NUCLEI; ISOTOPES; LINEAR ACCELERATORS; MESONS; NIOBIUM ISOTOPES; NUCLEI; NUCLEONS; ODD-ODD NUCLEI; PARTICLE INTERACTIONS; PARTICLE PRODUCTION; PSEUDOSCALAR MESONS; RADIOISOTOPES; SECONDS LIVING RADIOISOTOPES; SIMULATION
Optional Information
- Notes
- (c) 2009 The American Physical Society