2020
DOI: 10.1088/1367-2630/ab83cf
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Non-equilibrium effects in a relativistic plasma sheath model

Abstract: Plasma sheaths characterized by electrons with relativistic energies and far from thermodynamic equilibrium are governed by a rich and largely unexplored physics. A reliable kinetic description of relativistic non-equilibrium plasma sheaths-besides its interest from a fundamental point of view-is crucial to many application, from controlled nuclear fusion to laser-driven particle acceleration. Sheath models proposed in the literature adopt either relativistic equilibrium distribution functions or non-relativis… Show more

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Cited by 6 publications
(4 citation statements)
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References 53 publications
(81 reference statements)
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“…T h is related to the electron energy E DLT with a functional dependence determined by the shape of the hot electron distribution function. While different kinds of distribution functions can be plugged into the quasi-static TNSA model 52 , here we consider a perfectly exponential spectrum, by which we have T h = E DLT (d nc ). To calculate n h0 we assume that the electrons are spread uniformly in a 'cylinder' with volume of V DÀ1 w DÀ1 0 d s , where d s is the substrate thickness:…”
Section: Resultsmentioning
confidence: 99%
“…T h is related to the electron energy E DLT with a functional dependence determined by the shape of the hot electron distribution function. While different kinds of distribution functions can be plugged into the quasi-static TNSA model 52 , here we consider a perfectly exponential spectrum, by which we have T h = E DLT (d nc ). To calculate n h0 we assume that the electrons are spread uniformly in a 'cylinder' with volume of V DÀ1 w DÀ1 0 d s , where d s is the substrate thickness:…”
Section: Resultsmentioning
confidence: 99%
“…According to the capacitor model [39] or the relativistic, selfconsistent sheath model [40], the number density of fast electrons can then be expressed as n e = n 0 exp(−(E k + eϕ s )/T e ). That is, the form of the fast electron spectrum is not influenced by the static potential while the number of electrons escaping the potential decreases.…”
Section: Simulations and Discussionmentioning
confidence: 99%
“…for E p ≤ E p,max . Here T eff is the electron temperature, a quantity that can be estimated as the average electron energy T e even far from thermodynamic equilibrium [60].…”
Section: A Experimental and Modeling Of Proton Acceleration With Dltsmentioning
confidence: 99%