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The electromagnetic signature of jets

Charles Gale et al 2004 J. Phys. G: Nucl. Part. Phys. 30 S1013-S1016   doi: 10.1088/0954-3899/30/8/049  Help

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Charles Gale1, T C Awes2, Rainer J Fries3 and Dinesh K Srivastava4
1 Department of Physics, McGill University, 3600 University Street, Montreal, QC, H3A 2T8, Canada
2 Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
3 School of Physics & Astronomy, University of Minnesota, 116 Church Street S.E., Minneapolis, MN 55455, USA
4 Variable Energy Cyclotron Centre, 1/AF Bidhan Nagar, Kolkata 700 064, India

Abstract. Recent RHIC data have suggested an interesting scenario where jets, after being formed in the very first instants of the nuclear collision, interact strongly and are absorbed by the hot and dense matter subsequently created. In this respect, electromagnetic signals constitute another class of penetrating radiation. We first propose the study of large mass dileptons induced by the passage of high-energy quark jets through quark–gluon plasma. We find that the yield due to the jet–plasma interaction gets progressively larger as the collision energy increases: it is slightly less than the Drell–Yan contribution at RHIC energies, and it is a factor of 10 larger than Drell–Yan at the LHC. In a related investigation, we then propose to study dilepton-tagged jets. We estimate quantitatively the various background sources, and identify windows where those are sub-dominant.

Print publication: Issue 8 (August 2004)
Received 15 March 2004
Published 19 July 2004

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