About: Chromo–Weibel instability

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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.

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  • 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. (en)
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  • 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. (en)
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  • Chromo–Weibel instability (en)
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