Physics:Chromo–Weibel instability

Short description: Instability in non-abelian plasmas

The Chromo–Weibel instability is a plasma instability present in homogeneous or nearly homogeneous non-abelian plasmas which possess an anisotropy in momentum space. In the linear limit it is similar to the Weibel instability in electromagnetic plasmas but due to non-linear interactions present in non-abelian plasmas the late development of this instability is characterized by a turbulent cascade of modes. This instability is relevant in the understanding of the early-time dynamics of the quark-gluon plasma as produced in heavy-ion collisions.

See also

• Weibel instability

References

• Mrówczyński, Stanisław; Schenke, Björn; Strickland, Michael (2017). "Color instabilities in the quark–gluon plasma". Physics Reports 682: 1–97. doi:10.1016/j.physrep.2017.03.003. Bibcode: 2017PhR...682....1M. 
• Mrówczyński, Stanisław (1994). "Color collective effects at the early stage of ultrarelativistic heavy-ion collisions". Physical Review C 49 (4): 2191–7. doi:10.1103/PhysRevC.49.2191. PMID 9969449. Bibcode: 1994PhRvC..49.2191M. 
• Strickland, Michael (2007). "The chromo-weibel instability". Brazilian Journal of Physics 37 (2c): 762–766. doi:10.1590/S0103-97332007000500021. Bibcode: 2007BrJPh..37..762S. 
• Arnold, Peter; Moore, Guy D (2006). "Turbulent spectrum created by non-Abelian plasma instabilities". Physical Review D 73 (2): 025013. doi:10.1103/PhysRevD.73.025013. Bibcode: 2006PhRvD..73b5013A. https://cds.cern.ch/record/886120.