Exciting gauge unstable modes of the quark-gluon plasma by relativistic jets

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

6 pages, 2 figures, contributed to 2007 Europhysics Conference on High Energy Physics, Manchester, England 19-25 July 2007

Scientific paper

10.1088/1742-6596/110/3/032012

We present a study of the properties of the collective modes of a system composed by a thermalized quark-gluon plasma traversed by a relativistic jet of partons. We find that when the jet traverses the system unstable gauge field modes are excited and grow on very short time scales. The aim is to provide a novel mechanism for the description of the jet quenching phenomenon, where the jet crossing the plasma loses energy exciting colored unstable modes. In order to simplify the analysis we employ a linear response approximation, valid for short time scales. We assume that the partons in the jet can be described with a tsunami-like distribution function, whereas we treat the quark-gluon plasma employing two different approaches. In the first approach we adopt a Vlasov approximation for the kinetic equations, in the second approach we solve a set of fluid equations. In both cases we derive the expressions of the dispersion law of the collective unstable modes and compare the results obtained.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Exciting gauge unstable modes of the quark-gluon plasma by relativistic jets does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Exciting gauge unstable modes of the quark-gluon plasma by relativistic jets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Exciting gauge unstable modes of the quark-gluon plasma by relativistic jets will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-481830

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.