Abstract
It is argued that the relativistic Vlasov–Maxwell equations of the kinetic theory of plasma approximately describe a relativistic system of N charged point particles interacting with the electromagnetic Maxwell fields in a Bopp–Landé–Thomas–Podolsky (BLTP) vacuum, provided the microscopic dynamics lasts long enough. The purpose of this work is not to supply an entirely rigorous vindication, but to lay down a conceptual road map for the microscopic foundations of the kinetic theory of special-relativistic plasma, and to emphasize that a rigorous derivation seems feasible. Rather than working with a BBGKY-type hierarchy of n-point marginal probability measures, the approach proposed in this paper works with the distributional PDE of the actual empirical 1-point measure, which involves the actual empirical 2-point measure in a convolution term. The approximation of the empirical 1-point measure by a continuum density, and of the empirical 2-point measure by a (tensor) product of this continuum density with itself, yields a finite-N Vlasov-like set of kinetic equations which includes radiation-reaction and nontrivial finite-N corrections to the Vlasov–Maxwell–BLTP model. The finite-N corrections formally vanish in a mathematical scaling limit \(N\rightarrow \infty \) in which charges \(\propto 1/\surd {N}\). The radiation-reaction term vanishes in this limit, too. The subsequent formal limit sending Bopp’s parameter \(\varkappa \rightarrow \infty \) yields the Vlasov–Maxwell model.
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Notes
Of historical interest, perhaps, is that Vlasov himself considered the relativistic Vlasov theory as more fundamental [104]. Needless to say that his view never caught on.
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The authors thank Holly Carley, Markus Kunze, and Shadi Tahvildar-Zadeh for helpful discussions. They also thank the two referees and the editor, Herbert Spohn, for their comments.
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Appendix
Appendix
1.1 A The Radiation-Reaction Force Term
In this appendix we collect the pertinent formulas needed to compute the radiation-reaction force terms.
We write \(\varvec{\Pi }^{\mathrm{field}}_{\alpha ,n}(t,{\varvec{{ s}} })\) as a sum of three terms, sorted by their singularities,
where the suffix \(\varvec{\xi }_n^\alpha \) indicates the vector function \(t\mapsto \varvec{\xi }_n^\alpha (t) \equiv ({\varvec{{ q}} }_n^\alpha ,{\varvec{{ v}} }_n^\alpha ,\varvec{{ a}} _n^\alpha )(t)\). Here, and now dropping \({}_n\) and \({}^\alpha \) indices,
with the abbreviations \(\mathrm {K}_{\varvec{\xi }}, \mathbf {K}_{\varvec{\xi }}\) defined as in (2.19) and (2.24), and where \(\big |_\mathrm {ret}\) means that \({\varvec{{ q}} }(\tilde{t})\), \({\varvec{{ v}} }(\tilde{t})\), and \(\varvec{{ a}} (\tilde{t})\) are evaluated with \(\tilde{t} = {t^\mathrm {ret}_{\varvec{\xi }}}(t,{\varvec{{ s}} })\).
With \(\overline{\varvec{\xi }}\equiv ({\overline{\varvec{{ q}} }},{\varvec{{ v}} }_{\!0},\varvec{{ 0}} )\), we thus have
Note that the acceleration \(t\mapsto \varvec{{ a}} _n(t)\) only features linearly, in the \(k=1\) term.
To carry out the integrations at r.h.s. (A.5) we in [54] switch to “retarded spherical co-ordinates” with the colatitude \(\vartheta \) defined with respect to \({\varvec{{ s}} }- {\varvec{{ q}} }(t^{\mathrm {r}})\). Let \(\mathrm {d}\omega _r({\varvec{{ s}} })\) denote the uniform measure on \(\partial B_r\left( {\varvec{{ q}} }(t^{\mathrm {r}})\right) \). For any \({\mathfrak {C}}^{1,1}\) map \(t^{\mathrm {r}}\mapsto {\varvec{{ q}} }(t^{\mathrm {r}})\) with \({{\dot{{\varvec{{ q}} }}}}(t^{\mathrm {r}})=:{\varvec{{ v}} }(t^{\mathrm {r}})\) we then have
This gives us
Next we register the following important facts about the angular integrations over the spheres \(\partial B_r\left( {\varvec{{ q}} }(t^{\mathrm {r}})\right) \) (where \({\varvec{{ q}} }\) stands for either \({\varvec{{ q}} }_n\) or \({\overline{\varvec{{ q}} }}_n\); \({\varvec{{ v}} }\) and \(\varvec{{ a}} \) similarly):
-
on \(\partial B_{r}({\varvec{{ q}} }(t^{\mathrm{r}}))\) the retarded time \(t^{\mathrm{r}}_{{\varvec{{ q}} }}(t,{\varvec{{ s}} }) = t-\frac{1}{c} r = t^{\mathrm{r}}\) is constant;
-
the vectors \({\varvec{{ q}} }(t^{\mathrm{r}})\), \({\varvec{{ v}} }(t^{\mathrm{r}})\), and \(\varvec{{ a}} (t^{\mathrm{r}})\) are constant during the integration over \(\partial B_{r}({\varvec{{ q}} }(t^{\mathrm{r}}))\);
-
for \({\varvec{{ s}} }\in \partial B_{r}({\varvec{{ q}} }(t^{\mathrm{r}}))\), we have \({\varvec{{ s}} }= r\, {\varvec{{ n}} }({\varvec{{ q}} }(t^{\mathrm{r}}),{\varvec{{ s}} }) + {\varvec{{ q}} }\big (t^{\mathrm{r}}\big )\);
-
for \({\varvec{{ s}} }\in \partial B_{r}({\varvec{{ q}} }(t^{\mathrm{r}}))\) the unit vector \({\varvec{{ n}} }({\varvec{{ q}} }(t^{\mathrm{r}}),{\varvec{{ s}} })=\big (\sin \vartheta \cos \varphi , \sin \vartheta \sin \varphi , \cos \vartheta \big )\).
It follows that on \(\partial B_{r}({\varvec{{ q}} }(t^{\mathrm{r}}))\) the vectors \(\varvec{\pi }_{\varvec{\xi }}^{[k]}\big (t,{\varvec{{ s}} }_{{\varvec{{ q}} }}(r,\vartheta ,\varphi )\big )\) are bounded continuous functions of \(\vartheta \) and \(\varphi \). Thus the angular integrations at r.h.s. (A.7) can be carried out to yield
The vector functions \(\widetilde{\mathbf {Z}}_{\varvec{\xi }}^{[k]}(t,r)\) depend on the maps \(t'\mapsto {\varvec{{ q}} }(t')\) and \(t'\mapsto {\varvec{{ v}} }(t')\) between \(t'=0\) and \(t'=t^{\mathrm{ret}}_{{\varvec{{ q}} }}(t,{\varvec{{ s}} })=t^{\mathrm{r}}\), through the \(\mathrm {d}{t'}\) integrals over the Bessel function kernels, through which they also depend on the initial data \({\varvec{{ q}} }(0)\) and \({\varvec{{ v}} }(0)\) (recall that the integrations over \(t'<0\) involve an unaccelerated auxiliary motion determined by the initial data \({\varvec{{ q}} }(0)\) and \({\varvec{{ v}} }(0)\)). They also depend on t and r, explicitly through the Bessel function kernels (2.24) and (2.19) (recall also the third bullet point above), and implicitly through the dependence on \(t^{\mathrm{r}} = t-r/c\) in: (a) the vectors \({\varvec{{ q}} }(t^{\mathrm{r}})\), \({\varvec{{ v}} }(t^{\mathrm{r}})\), and (when \(k=1\)) \(\varvec{{ a}} (t^{\mathrm{r}})\), and (b) the upper limit of integration of the integrals over the Bessel function kernels.
Next, by a change of integration variable from r to \(t^{\mathrm{r}}= t-r/c\) we eliminate the implicit t dependence from the integrands at r.h.s.(A.8). Writing \(\widetilde{\mathbf {Z}}_{\varvec{\xi }}^{[k]}\big (t,r\big ) = {\mathbf {Z}}_{\varvec{\xi }}^{[k]}\big (t,t^{\mathrm{r}}\big )\), this yields (2.25).
We thus arrive at the “self”-field force on the n-th point charge source of the MBLTP field equations, given for \(t>0\) by the negative t derivative of (2.25), viz.
Remark A.1
Thus the integrals in the second and third line at r.h.s.(A.9) are well defined Riemann integrals.
Remark A.2
Since \(t^{\mathrm {r}}\) is a mute integration variable at r.h.s.(A.9), the \(\frac{\partial }{\partial t}\) derivative in the third line at r.h.s(A.9) does not act on it. In particular, it does not act on \({\varvec{{ q}} }_n(t^\mathrm {r})\), \({\varvec{{ v}} }_n(t^\mathrm {r})\), or \(\varvec{{ a}} _n(t^\mathrm {r})\) in any of the \({\mathbf {Z}}_{\varvec{\xi }_n}^{[k]}\big (t,t^{\mathrm {r}}\big )\). This leads to the important observation that the “self” force does not involve higher-than-second-order time derivates of \(t\mapsto {\varvec{{ q}} }(t)\).
Remark A.3
The derivative \(\frac{\partial }{\partial t}\) also does not act on \({\varvec{{ q}} }_n(t^\prime )\) or \({\varvec{{ v}} }_n(t^\prime )\) in the kernels \(\mathbf {K}_{\varvec{\xi }}(t',t,{\varvec{{ s}} }_{\varvec{{ q}} })\) and \(\mathrm {K}_{\varvec{\xi }}(t',t,{\varvec{{ s}} }_{\varvec{{ q}} })\). Thus the acceleration enters the “self” force only linearly, as \(\varvec{{ a}} _n(t^{\mathrm {r}})\), through \({\mathbf {Z}}_{\varvec{\xi }_n}^{[1]}\big (t,t^{\mathrm {r}}\big )\) in the second, and \(\frac{\partial }{\partial t}{\mathbf {Z}}_{\varvec{\xi }_n}^{[1]}\big (t,t^{\mathrm {r}}\big )\) in the third line at r.h.s.(A.9). This gives rise to the Volterra integral equation for the accelerations, mentioned in 2.3.
There is no purely light-like contribution to the third line at r.h.s.(A.9). The \(\frac{\partial }{\partial t}\) in the third line at r.h.s.(A.9) acts only on the explicit t-dependence in \(\mathbf {K}_{\varvec{\xi }}\) and in \(\mathrm {K}_{\varvec{\xi }}\) in the mixed light- & time-like and purely time-like contributions to \({\mathbf {Z}}_{\varvec{\xi }_n}^{[k]}\big (t,t^{\mathrm {r}}\big )\). The identity
(see §10.6(ii) in [17]) yields these derivatives easily as
where \({\varvec{{ s}} }_{\varvec{{ q}} }= r{\varvec{{ n}} }+{\varvec{{ q}} }(t^\mathrm {r})\).
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Elskens, Y., Kiessling, M.KH. Microscopic Foundations of Kinetic Plasma Theory: The Relativistic Vlasov–Maxwell Equations and Their Radiation-Reaction-Corrected Generalization. J Stat Phys 180, 749–772 (2020). https://doi.org/10.1007/s10955-020-02519-x
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DOI: https://doi.org/10.1007/s10955-020-02519-x