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A model-free procedure to correct for volume fluctuations in E-by-E analyses of particle multiplicities

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arxiv 2211.14849 v1 pith:5653RJZG submitted 2022-11-27 nucl-th hep-phnucl-ex

classification nucl-thhep-phnucl-ex
keywords fluctuationsdistributionsprocedurevolumeaccountcontributionscumulantsexperimentally
verification ladder T0 review T1 audit T2 compute T3 formal
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We develop an innovative and unbiased procedure, based on event mixing, to account for unavoidable contributions from volume (or system size) fluctuations to experimentally measured moments of particle multiplicity distributions produced in relativistic nuclear collisions. Within the wounded-nucleon model they are characterized by fluctuations of the number of wounded nucleons, the latter usually referred to as participants. For the first time we extract participant fluctuations directly from the data used for the fluctuation analysis, i.e., without involving model calculations. To achieve this we constructed a dedicated event-mixing algorithm that eliminates all possible correlations between produced particles while preserving the volume fluctuations. The procedure provides direct access to the cumulants of wounded-nucleon distributions, which can be used to account for non-critical contributions to the experimentally measured cumulants of multiplicity distributions.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. To bin or not to bin: does binning in multiplicity reliably suppress unwanted volume fluctuations?

    nucl-th 2025-11 conditional novelty 7.0 of 10

    In a Poisson-plus-Gamma model, CBWC overcorrects and underestimates proton and net-proton cumulants whenever resonance-type correlations between multiplicity and proton number are sufficiently strong.

  2. Baselines for Abelian Charge Fluctuations in Nuclear Collisions:Theory and Comparison with Experimental Data

    nucl-th 2025-08 conditional novelty 6.0 of 10

    Exact global baryon number conservation alone cannot reproduce STAR BES-II and HADES proton factorial cumulants; adding repulsive proton pairs at high energies and attractive triplets at low energies does, but with pa...

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