English

Collisional and radiative energy loss in small systems

Nuclear Theory 2025-05-13 v2 High Energy Physics - Phenomenology

Abstract

We present an energy loss model which includes small system size corrections to both the radiative and elastic energy loss. Our model is used to compute the nuclear modification factor RABR_{AB} of light and heavy flavor hadrons, averaged over realistic collision geometries for central and peripheral A+AA+A and central p/d/3He+Ap / d / {}^3\text{He} + A collisions at LHC and RHIC. We find that the predicted suppression in small systems is almost entirely due to elastic energy loss. Our results are keenly sensitive to the crossover between elastic energy loss calculated with hard thermal loop propagators and vacuum propagators, respectively, which leads to a large theoretical uncertainty. We find that the RABR_{AB} is largely insensitive to the form of the elastic energy loss distribution - Gaussian or Poisson - surprisingly so in small systems where the central limit theorem is inapplicable. We present an expansion of the RABR_{AB} in terms of the moments of the energy loss probability distribution, which allows for a rigorous understanding of the dependence of the RABR_{AB} on the underlying energy loss distribution.

Keywords

Cite

@article{arxiv.2408.14426,
  title  = {Collisional and radiative energy loss in small systems},
  author = {Coleridge Faraday and W. A. Horowitz},
  journal= {arXiv preprint arXiv:2408.14426},
  year   = {2025}
}

Comments

33 pages, 34 figures. Updated to be consistent with published version. Numerical bug in pion hadronization was fixed, resulting in ~10% increase in pion RAB at high-pT compared to previous version; the conclusions of the manuscript are unchanged