1987
DOI: 10.1063/1.866343
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Relativistic fluid equations for intense electron beams

Abstract: Experimental and theoretical study of the equation of state of carbon using an intense beam of relativistic electrons

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Cited by 12 publications
(11 citation statements)
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“…We will assume a "warm" plasma such that the distribution f has a small momentum spread about its mean [14][15][16][17]. We make no additional assumptions concerning the specific form of f .…”
mentioning
confidence: 99%
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“…We will assume a "warm" plasma such that the distribution f has a small momentum spread about its mean [14][15][16][17]. We make no additional assumptions concerning the specific form of f .…”
mentioning
confidence: 99%
“…Note that ǫ is a Lorentz invariant and ǫ 2 ≪ 1 is satisfied if the local rest frame temperature of the plasma is nonrelativistic. We consider the ratio λ = n p /h [14,16], where n p = (J µ J µ ) 1/2 is the proper density, and introduce (λΓ, λΓw)…”
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confidence: 99%
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“…The space-time metric tensor g µν for the following covariant formulation has the convention g µν = diag(1, −1, −1, −1). Following previous relativistic fluid formulations [21][22][23][24], consider the following moments of the phase-space distribution:…”
Section: Relativistic Fluid Equationsmentioning
confidence: 99%
“…24,29 By assuming that the plasma is "warm", such that the phase-space distribution has a small momentum spread about its mean, allows the hierarchy of moment equations to be treated asymptotically. [29][30][31][32][33] No additional assumptions concerning the specific form of the distribution are required for closure of the fluid equations. Assuming the quasi-static approximation, 34 i.e., the plasma wave driver and fluid quantities are assumed to be functions only of the co-moving variable ξ = z − β ϕ ct (where z is the driver propagation direction), the fluid equations can be combined to yield the evolution equation for the nonlinear 1D plasma response 24…”
Section: Warm Wavebreakingmentioning
confidence: 99%