Published November 2002
| Version v1
Journal article
Complete next-to-leading-order calculation for pion production in nucleon-nucleon collisions at threshold
Creators
- 1. Forschungszentrum Juelich, Institut fuer Kernphysik (Theorie), D-52425 Juelich (Germany)
- 2. Institut fuer Theoretische Physik, Physik Department T39, Technische Universitaet Muenchen, D-85747 Garching (Germany)
Description
Based on a counting scheme that explicitly takes into account the large momentum √(Mmπ) characteristic for pion production in nucleon-nucleon collisions we calculate all diagrams for the reaction NN→NNπ at threshold up to next-to-leading-order. At this order there are no free parameters and the size of the next-to-leading- order contributions is in line with the expectation from power counting. The sum of loop corrections at that order vanishes for the process pp→ppπ0 at threshold. The total contribution at next-to-leading-order from loop diagrams that include the delta degree of freedom vanishes at threshold in both reaction channels pp→ppπ0,pnπ+
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.66.054005;
- arXiv
- arXiv:nucl-th/0208050v1;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 66
- Journal Issue
- 5
- Journal Page Range
- p. 054005-054005.5
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36012734
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CHIRAL SYMMETRY; CORRECTIONS; DEGREES OF FREEDOM; FEYNMAN DIAGRAM; NUCLEAR FORCES; NUCLEAR MATTER; NUCLEAR REACTIONS; NUCLEON-NUCLEON INTERACTIONS; PARTICLE PRODUCTION; QUARK MODEL; THRESHOLD ENERGY
- Descriptors DEC
- BARYON-BARYON INTERACTIONS; COMPOSITE MODELS; DIAGRAMS; ENERGY; HADRON-HADRON INTERACTIONS; INFORMATION; INTERACTIONS; MATHEMATICAL MODELS; MATTER; PARTICLE INTERACTIONS; PARTICLE MODELS; SYMMETRY
Optional Information
- Notes
- (c) 2002 The American Physical Society