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Modeling the jet quenching in hot and dense QCD matter

2009/10/27 by I. P. Lokhtin, I. Lokhtin, L. Malinina +15
Physics and Astronomy · #Cosmology and Gravitation Theories #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #High-Energy Particle Collisions Research #Quantum Chromodynamics and Particle Interactions #hep-ph

paper · pdf · doi:10.48550/arxiv.0910.5129

Talk given at XXXIX International Symposium on Multiparticle Dynamics (Gomel, Belarus, September 4-9, 2009); 8 pages including 4 figures as EPS-files; prepared using LaTeX package for publication in the International Journal "Nonlinear Phenomena in Complex Systems"

arxiv created 2009/10/27 · openalex publication_date 2009/10/27 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

One of the important perturbative ("hard") probes of hot and dense QCD matter is the medium-induced energy loss of energetic partons, so called "jet quenching", which is predicted to be very different in cold nuclear matter and in QGP, and leads to a number of phenomena which are already seen in the RHIC data on the qualitative level. The inclusion of jet quenching and other important collective effects, such as radial and elliptic flows, in the existing Monte-Carlo models of relativistic heavy ion collisions is discussed. Some issues on the corresponding physical observables at RHIC and LHC energies obtained with HYDJET++ model are presented.

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