Spontaneous Generation of Electromagnetic Waves in Plasmas with Electron Thermal Flux

Nonlocal Electron Heat Transport in Magnetized Dense Plasmas

“…The temperature profile for strongly magnetized plasma, where the strength of the magnetic field is 10 MG, 2) Assuming τ = τ 0 v 3 , effective mean free path can be written as τ 0 v 4 /(1 + ω 2 τ 2 0 v 6 ). The derivative of this value with respect to v becomes zero and the effective mean free path takes a maximum value at ωτ = √ 2.…”

“…In laser produced plasmas, a magnetic field will be important because it implicates transport and nonuniformities. Spontaneously generated magnetic fields in laserproduced plasmas have been experimentally observed and theoretically demonstrated [1][2][3][4][5][6][7][8][9][10][11]. However, to directly detect the magnetic field B is difficult in collisional overdense plasma.…”

Interplay of Kinetic Plasma Instabilities

“…2 a) the two branches of the transverse modes (Eq. 15) are also symmetric and will be described by the same dispersion relation (Okada et al;1977;2009c) ( ) …”

Quasi Exact Model for the Anisotropy Driven Weibel Instability all over Fourier Space

“…This instability has been investigated in details, including for Maxwellian [1,11,12] and relativistic [13,14] plasmas. Basic equations are usually derived from the Maxwell-Vlasov system, although an interesting variation of the concept using the moments of the Vlasov equation has recently been used [15].…”

“…Considering therefore the plasma isotropic in the (x, y) plan, we set k = (k z , k x ) (see Figure 1). Using the Vlasov equation together with Maxwell equations, one derives the dispersion equation for the Weibel instability as [11,16],…”