Higher moments of net-proton multiplicity distributions in a heavy-ion event pile-up scenario

P. Garg and D. K. Mishra
Phys. Rev. C 96, 044908 – Published 20 October 2017

Abstract

High-luminosity modern accelerators, like the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory (BNL) and Large Hadron Collider (LHC) at European Organization for Nuclear Research (CERN), inherently have event pile-up scenarios which significantly contribute to physics events as a background. While state-of-the-art tracking algorithms and detector concepts take care of these event pile-up scenarios, several offline analytical techniques are used to remove such events from the physics analysis. It is still difficult to identify the remaining pile-up events in an event sample for physics analysis. Since the fraction of these events is significantly small, it may not be as serious of an issue for other analyses as it would be for an event-by-event analysis. Particularly when the characteristics of the multiplicity distribution are observable, one needs to be very careful. In the present work, we demonstrate how a small fraction of residual pile-up events can change the moments and their ratios of an event-by-event net-proton multiplicity distribution, which are sensitive to the dynamical fluctuations due to the QCD critical point. For this study, we assume that the individual event-by-event proton and antiproton multiplicity distributions follow Poisson, negative binomial, or binomial distributions. We observe a significant effect in cumulants and their ratios of net-proton multiplicity distributions due to pile-up events, particularly at lower energies. It might be crucial to estimate the fraction of pile-up events in the data sample while interpreting the experimental observable for the critical point.

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  • Received 19 June 2017
  • Revised 11 September 2017

DOI:https://doi.org/10.1103/PhysRevC.96.044908

©2017 American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsNuclear Physics

Authors & Affiliations

P. Garg1,* and D. K. Mishra2,†

  • 1Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
  • 2Nuclear Physics Division, Bhabha Atomic Research Center, Mumbai 400085, India

  • *prakhar@rcf.rhic.bnl.gov
  • dkmishra@barc.gov.in

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Vol. 96, Iss. 4 — October 2017

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