Multistrange baryon production in Au-Au collisions at root s(NN)=130 GeV

Bonner, BE; Sanchez, MCD; Dubey, AK; Gonzalez, JE; Jones, PG; Lansdell, CL; Marx, JN; Miller, ML; Romero, JL; Tribble, RE; Underwood, DG; Wang, XL; Wang, ZM; Zhang, ZP; STAR Collaboration

Abstract

The transverse mass spectra and midrapidity yields for Xis and Omegas are presented. For the 10% most central collisions, the (Xi) over bar (+)/h(-) ratio increases from the Super Proton Synchrotron to the Relativistic Heavy Ion Collider energies while the Xi(-)/h(-) stays approximately constant. A hydrodynamically inspired model fit to the Xi spectra, which assumes a thermalized source, seems to indicate that these multistrange particles experience a significant transverse flow effect, but are emitted when the system is hotter and the flow is smaller than values obtained from a combined fit to pi, K, p, and Lambdas.

Más información

Título según WOS: ID WOS:000221277900015 Not found in local WOS DB
Título de la Revista: PHYSICAL REVIEW LETTERS
Volumen: 92
Número: 18
Editorial: AMER PHYSICAL SOC
Fecha de publicación: 2004
DOI:

10.1103/PhysRevLett.92.182301

Notas: ISI