2015
DOI: 10.1016/j.physa.2015.08.010
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Stimulated Raman scattering in nonextensive statistics

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Cited by 4 publications
(3 citation statements)
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References 50 publications
(57 reference statements)
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“…The Tsallis statistics, with the use of q-parameter to evaluate the degree of nonextensivity of the system, has been proposed for the Stimulated Raman Scattering (SRS) in a collisionless plasma by Sharifi & Parvazian (2015). SRS involves a resonant decay of laser electromagnetic waves into scattered electromagnetic waves and electron plasma waves (EPW).…”
Section: Physical Reasonsmentioning
confidence: 99%
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“…The Tsallis statistics, with the use of q-parameter to evaluate the degree of nonextensivity of the system, has been proposed for the Stimulated Raman Scattering (SRS) in a collisionless plasma by Sharifi & Parvazian (2015). SRS involves a resonant decay of laser electromagnetic waves into scattered electromagnetic waves and electron plasma waves (EPW).…”
Section: Physical Reasonsmentioning
confidence: 99%
“…"Most of the studies for SRS are derived in the frame of a fluid description, a Maxwellian distribution function, or a relativistic Maxwellian distribution function. However, many space and laboratory plasmas show a non-Maxwellian behavior" (Sharifi & Parvazian, 2015). According to Sharifi and Parvazian, new statistical approaches based on the generalization of Boltzmann-Gibbs entropy, have been proposed, according to the works by Alfred Rényi (1955) and Constantino Tsallis (1988).…”
Section: Physical Reasonsmentioning
confidence: 99%
“…Suprathermal tails also exist in space plasmas, where the collisional effect is weak, and a stable superheat distribution or kappa distribution can be formed. [25][26][27][28][29] However, in the laserplasma environment, due to a relatively short time scale and the long-term impact of the collisional effect, a hot electron tail with Maxwellian distribution is commonly observed in experiments and simulations. [30][31][32][33] This hot Maxwellian tail is formed due to SRS or two-plasma decay instability, and the effective temperature is roughly approximated by T h ≈ 1 2 mv 2 φ where v φ is the phase velocity of the excited Langmuir wave.…”
Section: Introductionmentioning
confidence: 99%