Baryonic strangeness and related susceptibilities in QCD
Creators
- 1. Department of Physics, Duke University, Durham, North Carolina 27708-0305 (United States)
Description
The ratios of off-diagonal to diagonal conserved charge susceptibilities, e.g., χBS/χS,χQS/χS, related to the quark flavor susceptibilities, have proven to be discerning probes of the flavor carrying degrees of freedom in hot strongly interacting matter. Various constraining relations between the different susceptibilities are derived based on the Gell-Mann-Nishijima formula and the assumption of isospin symmetry. Using generic models of deconfined matter and results from lattice quantum chromodynamics, it is demonstrated that the flavor-carrying degrees of freedom at a temperature above 1.5Tc are quarklike quasiparticles. A new observable related by isospin symmetry to CBS=-3χBS/χS and equal to it in the baryon free regime is identified. This new observable, which is blind to neutral and nonstrange particles, carries the potential of being measured in relativistic heavy-ion collisions
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.74.054901;
- arXiv
- arXiv:nucl-th/0605079v1;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 74
- Journal Issue
- 5
- Journal Page Range
- p. 054901-054901.11
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38032618
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- BARYONS; DEGREES OF FREEDOM; FLAVOR MODEL; HEAVY ION REACTIONS; ISOSPIN; QUANTUM CHROMODYNAMICS; QUARKS; QUASI PARTICLES; RELATIVISTIC RANGE; STRANGENESS; SYMMETRY
- Descriptors DEC
- COMPOSITE MODELS; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; FIELD THEORIES; HADRONS; MATHEMATICAL MODELS; NUCLEAR REACTIONS; PARTICLE MODELS; PARTICLE PROPERTIES; QUANTUM FIELD THEORY; QUARK MODEL
Optional Information
- Notes
- (c) 2006 The American Physical Society