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      Results from PHENIX at RHIC

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          Abstract

          Results from PHENIX at RHIC in p-p and Au+Au collisions are presented from the perspective of measurements in p-p collisions at the CERN ISR which serve as a basis for many of the techniques used. Notable results include the equality of the suppression of inclusive pi0 and direct electrons (from the decay of heavy quarks) in the range of transverse momentuum 4 < pT < 9 GeV/c in central Au+Au collisions. This result appears to strongly disfavor the explanation of suppression as due to radiative energy loss of partons traversing a Quark Gluon Plasma but opens up a fundamental discussion of how Fermions get mass, whether all six quarks are nearly massless in a QGP and how to test this.

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          Non-Abelian Energy Loss at Finite Opacity

          , , (2009)
          A systematic expansion in opacity, \(L/\lambda\), is used to clarify the non-linear behavior of induced gluon radiation in quark-gluon plasmas. The inclusive differential gluon distribution is calculated up to second order in opacity and compared to the zeroth order (factorization) limit. The opacity expansion makes it possible to take finite kinematic constraints into account that suppress jet quenching in nuclear collisions below RHIC (\(\sqrt{s}=200\) AGeV) energies.
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            Energy loss in perturbative QCD

            We review the properties of energetic parton propagation in hot or cold QCD matter, as obtained in recent works. Advances in understanding the energy loss - collisional and radiative - are summarized, with emphasis on the latter: it features very interesting properties which may help to detect the quark-gluon plasma produced in heavy ion collisions. We describe two different theoretical approaches, which lead to the same radiated gluon energy spectrum. The case of a longitudinally expanding QCD plasma is investigated. The energy lost by a jet with given opening angle is calculated in view of making predictions for the suppression (quenching) of hard jet production. Phenomenological implications for the difference between hot and cold matter are discussed. Numerical estimates of the loss suggest that it may be significantly enhanced in hot compared to cold matter.
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              Author and article information

              Journal
              03 June 2009
              Article
              0906.0745
              b623148f-020d-4b00-a405-0a358363a261

              http://arxiv.org/licenses/nonexclusive-distrib/1.0/

              History
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              Invited lecture at International School of Subnuclear Physics, 46th Course, Erice, Sicily, Italy, August 29-September 7, 2008. 15 pages, 11 figures
              nucl-ex

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