Model of the effect of collisions on QCD plasma instabilities
- 1. Institut fuer Theoretische Physik, Johann Wolfgang Goethe-Universitaet Frankfurt, Max-von-Laue-Strasse 1, D-60438 Frankfurt (Germany)
- 2. Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universitaet Frankfurt, Max-von-Laue-Strasse 1, D-60438 Frankfurt (Germany)
- 3. Max-Planck-Institute for Extraterrestrial Physics, P.O. Box 1312, 85741 Garching (Germany)
Description
We study the effect of including a Bhatnagar-Gross-Krook (BGK) collisional kernel on the collective modes of a QCD plasma which has a hard-particle distribution function which is anisotropic in momentum space. We calculate dispersion relations for both the stable and unstable modes and show that the addition of hard-particle collisions slows the rate of growth of QCD plasma unstable modes. We also show that for any anisotropy there is an upper limit on the collisional frequency beyond which no instabilities exist. Estimating a realistic value for the collisional frequency for αs∼0.2-0.4 we find that for the large-anisotropy case which is relevant for the initial state of matter generated by free streaming in heavy-ion collisions that the collisional frequency is below this critical value
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.73.125004;
- arXiv
- arXiv:hep-ph/0603029v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 73
- Journal Issue
- 12
- Journal Page Range
- p. 125004-125004.12
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37078498
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ANISOTROPY; DISPERSION RELATIONS; DISTRIBUTION FUNCTIONS; HEAVY ION REACTIONS; QUANTUM CHROMODYNAMICS; QUARK MATTER
- Descriptors DEC
- FIELD THEORIES; FUNCTIONS; MATTER; NUCLEAR REACTIONS; QUANTUM FIELD THEORY
Optional Information
- Notes
- (c) 2006 The American Physical Society