Published December 2002
| Version v1
Journal article
K*(892)0 production in relativistic heavy ion collisions at √(sNN)=130 GeV
Creators
- 1. University of Frankfurt, Frankfurt (Germany)
- 2. Purdue University, West Lafayette, Indiana 47907 (United States)
- 3. Indiana University, Bloomington, Indiana 47408 (United States)
Description
We report the first observation of K*(892)0→πK in relativistic heavy ion collisions. The transverse momentum spectrum of (K*0+K-bar*0)/2 from central Au+Au collisions at √(sNN)=130 GeV is presented. The ratios of the K*0 yield derived from these data to the yields of negative hadrons, charged kaons, and φ mesons have been measured in central and minimum bias collisions and compared with model predictions and comparable e+e-, pp, and p-barp results. The data indicate no dramatic reduction of K*0 production in relativistic heavy ion collisions despite expected losses due to rescattering effects
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.66.061901;
- arXiv
- arXiv:nucl-ex/0205015v2;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 66
- Journal Issue
- 6
- Journal Page Range
- p. 061901-061901.6
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36012795
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- COMPARATIVE EVALUATIONS; GEV RANGE 100-1000; GOLD 197 REACTIONS; GOLD 197 TARGET; HADRONIC PARTICLE DECAY; K*-892 MESONS; KAONS MINUS; KAONS PLUS; NUCLEAR REACTION YIELD; PARTICLE PRODUCTION; PHI-1020 MESONS; RELATIVISTIC RANGE; RESCATTERING; TRANSVERSE MOMENTUM
- Descriptors DEC
- BOSONS; DECAY; ELEMENTARY PARTICLES; ENERGY RANGE; EVALUATION; GEV RANGE; HADRONS; HEAVY ION REACTIONS; KAONS; LINEAR MOMENTUM; MESONS; NUCLEAR REACTIONS; PARTICLE DECAY; PSEUDOSCALAR MESONS; QUARKONIUM; SCATTERING; STRANGE MESONS; STRANGE PARTICLES; STRANGEONIUM; TARGETS; VECTOR MESONS; YIELDS
Optional Information
- Notes
- (c) 2002 The American Physical Society
- Collaborations
- STAR Collaboration