Higher-Order Cumulants and Correlation Functions of Proton Multiplicity Distributions in $\sqrt{s_{\mathrm{NN}}}$ = 3 GeV Au+Au Collisions at the RHIC STAR Experiment
STAR Collaboration: M. S. Abdallah, B. E. Aboona, J. Adam, L., Adamczyk, J. R. Adams, J. K. Adkins, I. Aggarwal, M. M. Aggarwal, Z. Ahammed,, D. M. Anderson, E. C. Aschenauer, J. Atchison, V. Bairathi, W. Baker, J. G., Ball Cap, K. Barish, R. Bellwied, P. Bhagat, A. Bhasin

TL;DR
This paper measures higher-order cumulants and correlation functions of proton multiplicity distributions in 3 GeV Au+Au collisions, revealing a dominance of hadronic interactions at this energy through suppressed cumulant ratios.
Contribution
It provides the first detailed analysis of proton cumulants up to sixth order at this energy, including systematic corrections and comparisons with theoretical models.
Findings
Proton cumulant ratio C4/C2 is negative in central collisions.
Strong suppression of C4/C2 compared to higher energy collisions.
Results suggest hadronic interactions dominate at 3 GeV.
Abstract
We report a measurement of cumulants and correlation functions of event-by-event proton multiplicity distributions from fixed-target Au+Au collisions at = 3 GeV measured by the STAR experiment. Protons are identified within the rapidity () and transverse momentum () region and GeV/ in the center-of-mass frame. A systematic analysis of the proton cumulants and correlation functions up to sixth-order as well as the corresponding ratios as a function of the collision centrality, , and are presented. The effect of pileup and initial volume fluctuations on these observables and the respective corrections are discussed in detail. The results are compared to calculations from the hadronic transport UrQMD model as well as a hydrodynamic model. In the most central 5\% collisions, the value of proton cumulant…
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