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The Relativistic Vlasov Equation with current and charge density given by by Alec Johnson, January 2011 X X J = qpvpδxp σ = qpδxp I. Recitation of basic electrodynamics p p

X δxp X δxp = q p , = q γ ; A. Classical electrodynamics p p γ p p γ p p p p Classical electrodynamics is governed by Newton’s sec- here p (i.e. γ v ) is the proper velocity, where γ is the ond law (for particle motion), p p p p rate at which time t elapses with respect to the proper time τ of a clock moving with particle p. Dropping the particle mpdtvp = Fp, vp := dtxp, p index, (where p is particle index, t is time, mp is particle mass, γ := d t, and xp(t) is particle position, and Fp(t) is the force on the τ particle), the Lorentz force law, p := dτ x = (dτ t)dtx = γv.

Fp = qp (E + v × B) A concrete expression relating γ to (proper) velocity is (where E(t, x) = electric field, B(t, x) = magnetic field, and qp is particle charge), and Maxwell’s equations, γ2 = 1 + (p/c)2, i.e. (dividing by γ2), −2 2 ∂tB + ∇ × E = 0, ∇ · B = 0, 1 = γ + (v/c) , i.e. (solving for γ), 2 −1/2 ∂tE − c ∇ × B = −J/, ∇ · E = σ/, γ = 1 − (v/c)2 . with current and charge density given by II. Vlasov equation X X J := qpvpδxp , σ := qpδxp , The Vlasov equation asserts that particles are conserved p p in phase space and that the only force acting on particles is the electromagnetic force. where c is light speed, 0 is electric permittivity, J is net current density, σ is net charge density, δ (t, x) := δ(x − xp The Vlasov equation writes xp(t)) is the particle density function, and δ is the Dirac delta function (unit spike). ∂tfs + ∇x · (vfs) + ∇p · (asfs) = 0, (1)

B. Relativistic electrodynamics where fs(t, x, p) is the particle density function of species s and as = dtp = (qs/ms)(E+v ×B) is particle acceleration Newton’s second law is invariant under Galilean transfor- and we recall that v = dtx is velocity and p = γv is proper mations, but Maxwell’s equations are not (because they velocity. imply the existence of a light speed c). The Maxwell source terms are provided by the relations Einstein (and previously Lorentz) characterized the set of affine coordinate transformations, called Lorentz transfor- mations, which leave light speed constant and which satisfy X Z X Z J = q f vdp σ := q f dp the property that if system A has velocity v in system B s s s s then system B has velocity −v in system A. s s X Z dp X Z dp = q f p , = q f γ . s s γ s s γ Einstein then modified the laws of electrodynamics to make s s them Lorentz-invariant. To do so we replace velocity with proper velocity in Newton’s second law. So the laws of relativistic electrodynamics are: If we regard fs as a linear superposition of spike functions then the Vlasov system (1) with Maxwell’s equations is Newton’s second law, equivalent to the fundamental equations of electrodynam- ics written in terms of individual particles. mpdtpp = Fp, vp := dtxp, A. Lorentz-invariant form the Lorentz force law,

1. fs is a scalar. Fp = qp (E + v × B) , (In this section without loss of generality we take c = 1.) and Maxwell’s equations, The particle density function fs(t, x, p) is a scalar. This means that it remains invariant under the transforma- ∂tB + ∇ × E = 0, ∇ · B = 0, 2 tion of phase space that is implied by a Lorentz trans- ∂tE − c ∇ × B = −J/, ∇ · E = σ/, formation (i.e. a relativistic inertial transformation). It 2 takes a little work to see this. By definition, the quantity This confirms that the Vlasov equation (1) is indeed phys- 3 3 dfs := fs(t, x, p)d x ∧ d p counts the number of particles ical and Lorentz-invariant. 3 3 in a region (x0 +d x, p0 +d p) in phase space. (Note that d3x ∧ d3p denotes an infinitesimal surface of simultaneous B. Moments points in (t, x, p)-space.) We argue that dfs is a scalar, then argue that d3x ∧ d3p is a scalar, and then conclude Let χ(p) be a generic moment to evaluate: that fs is a scalar. The essence of the argument is to con- Z 3  µ k d p sider a Lorentz boost which transforms into the reference χ ∂xµ (p fs) + γ∇pk (as fs) = Cs . 3 3 3 3 0 γ frame of d x∧d p (i.e. which transforms p0 +d p to d p , p so that the transformed range of velocities is centered on Integrate by parts to get zero). Z 3 Z 3 Z 3  µ d p k  d p d p ∂ µ χp f = f a ∇ k χ + C χ . x s γ ses p γ s γ To see that such a boost leaves dfs invariant, consider p p p the particle event paths (“world lines”) that intersect 3 3 d x ∧ d p. The transformed region of phase space will Use p⊗n := ⊗np to denote the nth tensor power. In be intersected by exactly the same particles. Although case χ = p⊗n = Sym (p⊗n), we have (at least for spa- the transformed region of phase space is not simultane- tial indices, and then by tensoriality of the expression for ous, orthogonal projection to make it simultaneous does k ⊗n−1 temporal indices as well): aes ∇pk χ = n Sym (p aes) = not change the number of particles intersecting it because qs n Sym (F•p⊗n), where I adopt the notation (F•p)µ = ms their velocity is approximately zero. µν qs F pν and use that as = F• p, where F is the electro- e ms magnetic four-tensor with components To see that the same boost leaves d3x ∧ d3p invariant, 3 3  0 −ET /c note that orthogonality of d x and d p is invariant under F µν := . the boost, that the simultaneous region d3x is mapped E/c B × I 3 to a (nonsimultaneous) region of size γ0d x (where γ0 is 3 computed from the boost velocity), and that d p is shrunk So for χ = p⊗n (n ≥ 1) we have by a factor of γ because it is transformed to a region where 2 Z 3 Z 3 dγ = 0 (because γdγ = p · dp (because γ = 1 + p · p)  ⊗n µ d p qs  ⊗n d p 0 ∂xµ fsp p = n Sym F• fsp and p0 = 0 post-transformation). Again, projecting onto p γ ms p γ 3 simultaneous points does not change d x. In summary, Z 3 3 3 ⊗n d p we have argued that γ0d x and d p/γ0 are scalars, and + Csp . therefore their product d3x ∧ d3p is a scalar. p γ

2. Lorentz-invariant form For χ = 1 we get balance of particle four-flow: Z 3 Z 3 µ  µ d p d p Observe that ∂tfs + ∇x · (vfs) = ∂xµ (v fs), which would ∂xµ p fs = Cs . be Lorentz-invariant if we replaced vµ with γvµ = pµ. p γ p γ This indicates that to put the Vlasov equation (1) in a Separating time and space derivatives, manifestly Lorentz-invariant form we need to multiply it  Z   Z  Z d3p by γ. Then we have ∂ f + ∇ · f v = C . ct s s s γ µ k p p p ∂xµ (p fs) + γ∇pk (as fs) = 0; the first term is manifestly Lorentz-invariant; for the sec- More generally, for χ = p⊗n, separating time and space ond term we rewrite ∇pk in terms of derivatives with re- derivatives reveals a moment hierarchy: µ 0 k spect to the four-vector p by regarding γ = p and p as Z Z independent quantities (that is, we extend the definition of ∂ct fsχ + ∇· fsvχ all quantities (arbitrarily) beyond the quadratic manifold p p 2 2 Z Z γ = 1 + p ). Then the chain rule for partial derivatives qs  χ χ = n Sym F• fs + Cs . says ms p γ p γ ∂γ pk ∂ k 7→ ∂ + ∂ k = ∂ + ∂ k , p ∂pk γ p γ γ p Explicitly, omitting the collision term, the moment hierar- so chy is: Z Z Z  k  qs  χ  k p k k χ :∂ct fsχ + ∇· fsvχ = n Sym F• fs γ∇ k (a f ) 7→ γ ∂ (a f ) + ∇ k (a f ) . ms γ p s s γ γ s s p s s p p p  Z   Z  Let a := d p = γa be the proper acceleration. Then 1 : ∂ct fs + ∇· fsv = 0, es τ s p p p · a = p · d p = γd γ = γa0, that is, p · a = a0, so the Z Z Z e τ τ e s e qs   acceleration term can indeed be cast into the form appear- p : ∂ct fsp + ∇· fsvp = F• fsv , p p ms p ing in the following manifestly Lorentz-invariant version of Z Z Z qs   the Vlasov equation, pp : ∂ct fspp + ∇· fsvpp = 2 Sym F• fsvp , p p ms p µ µ ∂xµ (p fs) + ∂pµ (aes fs) = 0; ... 3

sary for all the flux moments and not just the highest flux moment). Note that (1) the evolved moments are not tensorial (be- dp To separate space and time components of vectors, use that cause γ , not dp, is tensorial) and (2) the fluxes are not identical to the evolved moments (so closures are neces- v = (1, v) and that p = (γ, p); then the moment hierarchy is:

  ⊗n R ⊗n R ⊗n qs −1 R ⊗n−1 R ⊗n−1 p : ∂ct p fs + ∇ · vp fs = n Sym c E p fs + vp fs × B p p ms p p   ⊗n−1 R ⊗n−1 R ⊗n qs −1 R ⊗n−1 γp : ∂ct γp fs + ∇ · p fs = n Sym c E · vp fs p p ms p R R 1 : ∂ct pfs + ∇· pvfs = 0,   R R qs −1 R R p : ∂ct pfs + ∇· vpfs = c E fs + vfs × B , p p ms p p

R R qs −1 R γ : ∂ct γfs + ∇· pfs = c E · vfs, p p ms p   R R qs −1 R R pp : ∂ct fspp + ∇· fsvpp = 2 Sym c E · p + vpfs × B , p p ms p p   R R qs −1 R γp : ∂ct γpfs + ∇ · ppfs = 2 Sym c E · vpfs p p ms p ...

C. Moment closure Moveover, by scalability in ρ, the reduces P E to a function of a single variable: ρ = Pe( ρ ). For this section, assume that c = 1. For isotropic gas dynamics, one posits that there exists a reference frame Determining values of ρ, E, and the three velocity compo- in which the distribution fs is isotropic. In this reference nents of the Lorentz boost so as to match the five evolved frame, the invariant flux tensor for χ = 1 has a single moments is a nonlinear problem that is usually solved it- nonzero component: eratively. To determine the form of this system, we apply a Lorentz R boost Λ that transforms from quantities in the reference [1, v]fs = [ρ, 0] p frame of the fluid to a laboratory frame moving at proper velocity U and the invariant flux tensor for χ = p is diagonal: Γ U  Λ = , U + UU Z γ p  E 0  I Γ+1 f = ; p vp s 0 P p I where Γ2 = 1 + |U|2. the pressure P is related to the energy E and density ρ Applying this boost to the tensor for the density and flux by an equation of state that is determined by the assumed of mass says that distribution of particle velocities; usually the assumed dis- ρ Γρ tribution is defined to maximize some notion of . Λ · = , i.e., To see how the assumed distribution relates pressure to 0 Uρ energy, observe that pressure as well as energy is given by ρ0 = Γρ, integrating the assumed distribution against a function of γ: where ρ0 is mass density in laboratory coordinates.

Applying this boost to the tensor for the density and flux R vpf = R γ−1ppf p s I p s of energy and says that R −1 1 2 = I γ |p| fs p 3 E 0  Γ2E + |U|2P (E + P)ΓU Z 2 Λ · ; ·Λ = ; γ − 1 0 P (E + P)ΓU P( + UU) = I fs. I I p 3γ