Universal bounds for SU(3) low energy constants
Creators
- 1. Departament de Fisica Teorica, IFIC, Universitat de Valencia-CSIC, Apt. Correus 22085, E-46071 Valencia (Spain)
Description
In this paper bounds for L1, L2, and L3 are obtained in chiral perturbation theory with three flavors. At the same time we test the compatibility of this theory with axiomatic principles. Following a recent paper we use dispersion relations to write positivity conditions that translate into bounds for the chiral low energy constants. As a first approach we consider the exact SU(3)V limit and notice that if a common mass of the order of that of the kaon is adopted for the octet of pseudo-Goldstone bosons the bounds have very large O(p6) corrections. Once the positivity conditions are adapted to account for different masses, we correct the previous bounds for a physical kaon mass and find that they tighten. We observe an overlap between the experimentally determined region and the first principles forbidden region, in the space of parameters.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.77.094020;
- arXiv
- arXiv:0801.3627v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 77
- Journal Issue
- 9
- Journal Page Range
- p. 094020-094020.6
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41001455
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CHIRALITY; COMPATIBILITY; CORRECTIONS; DISPERSION RELATIONS; FLAVOR; FLAVOR MODEL; GOLDSTONE BOSONS; GROUP CONSTANTS; KAONS; MASS; PERTURBATION THEORY; SPACE; SU-3 GROUPS
- Descriptors DEC
- BOSONS; COMPOSITE MODELS; CROSS SECTIONS; ELEMENTARY PARTICLES; HADRONS; LIE GROUPS; MATHEMATICAL MODELS; MESONS; ORGANOLEPTIC PROPERTIES; PARTICLE MODELS; PARTICLE PROPERTIES; POSTULATED PARTICLES; PSEUDOSCALAR MESONS; QUARK MODEL; STRANGE MESONS; STRANGE PARTICLES; SU GROUPS; SYMMETRY GROUPS
Optional Information
- Notes
- (c) 2008 The American Physical Society