Xi production at AGS energies
arXiv:nucl-th/0211020 · doi:10.1016/j.physletb.2004.06.045
Abstract
A relativistic transport model is used to study Xi- production in 2-11A GeV Au+Au collisions. Introducing the strangeness-exchange reactions between antikaons and hyperons as the sources for Xi-, we find that the cascade yield in these collisions is in reasonable agreement with the data. Although the Xi- abundance does not reach chemical equilibrium unless the cross section for strangeness-exchange reactions is enhanced by six times, it exhibits the strongest enhancement with increasing centrality of collision and with increasing beam energy.
Title changed, Modified version, 5 pages, RevTex
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Cited by in corpus (6)
- A Multi-Phase Transport Model for Relativistic Heavy Ion Collisions
- Statistical production of antikaon nuclear bound states in heavy ion collisions
- Probing high-density nuclear symmetry energy with ratio in heavy-ion collisions at GeV
- Baryon-antibaryon annihilation and reproduction in relativistic heavy-ion collisions
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