Improving a radiative plus collisional energy loss model for application to RHIC and LHC

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dc.creatorWicks, Simon
dc.creatorGyulassy, Miklos
dc.date2007-01-29
dc.date2007-06-20
dc.date.accessioned2026-07-07T11:44:26Z
dc.date.available2026-07-07T11:44:26Z
dc.descriptionWith the QGP opacity computed perturbatively and with the global entropy constraints imposed by the observed dNch/dy~1000, radiative energy loss alone cannot account for the observed suppression of single non-photonic electrons. Collisional energy loss is comparable in magnitude to radiative loss for both light and heavy jets. Two aspects that significantly affect the collisional energy loss are examined: the role of fluctuations, and the effect of introducing a running QCD coupling as opposed to the fixed alpha_s=0.3 used previously.
dc.descriptionPrepared for 19th International Conference on Ultra-Relativistic Nucleus-Nucleus Collisions: Quark Matter 2006 (QM2006), Shanghai, China, 14-20 Nov 2006
dc.identifierhttps://arxiv.org/abs/nucl-th/0701088
dc.identifierhttp://arxiv.org/abs/nucl-th/0701088
dc.identifierJ.Phys.G34:S989-S993,2007
dc.identifierdoi:10.1088/0954-3899/34/8/S141
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201602
dc.subjectNuclear Theory
dc.titleImproving a radiative plus collisional energy loss model for application to RHIC and LHC
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