Energy Dependence of Short and Long-Range Multiplicity Correlations in Au+Au Collisions from STAR

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dc.creatorTarnowsky, Terence
dc.date2007-02-26
dc.date.accessioned2026-07-07T11:23:52Z
dc.date.available2026-07-07T11:23:52Z
dc.descriptionA general overview of the measurement of long-range multiplicity correlations measured by the STAR experiment in Au+Au collisions at RHIC is presented. The presence of long-range correlations can provide insight into the early stages, and the type of matter produced in, these collisions. These measurements have been made in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 and 62.4 GeV. These results indicate a relatively large long-range correlation is produced in Au+Au collisions compared to a {\it pp} baseline at $\sqrt{s_{NN}}$ = 200 GeV. A weaker long-range correlation is seen as a function of incident energy. Further, comparison of the onset of the long-range correlation to the calculated percolation density parameter at $\sqrt{s_{NN}}$ = 200 GeV is presented.
dc.description8 pages, 6 figures, Conference Proceedings for the XI International Workshop on Correlation and Fluctuation in Multiparticle Production, Hangzhou, China, November 21-25, 2006
dc.identifierhttps://arxiv.org/abs/nucl-ex/0702056
dc.identifierhttp://arxiv.org/abs/nucl-ex/0702056
dc.identifierInt.J.Mod.Phys.E16:3363-3370,2008
dc.identifierdoi:10.1142/S0218301307009348
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195039
dc.subjectNuclear Experiment
dc.titleEnergy Dependence of Short and Long-Range Multiplicity Correlations in Au+Au Collisions from STAR
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