Steady states of the Vlasov-Maxwell system
Author:
Jack Schaeffer
Journal:
Quart. Appl. Math. 63 (2005), 619-643
MSC (2000):
Primary 35Q60; Secondary 86A25
DOI:
https://doi.org/10.1090/S0033-569X-05-00984-5
Published electronically:
September 22, 2005
MathSciNet review:
2187923
Full-text PDF Free Access
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Abstract: The Vlasov-Maxwell system models collisionless plasma. Solutions are considered that depend on one spatial variable, $x$, and two velocity variables, $v_1$ and $v_2$. As $x\rightarrow - \infty$ it is required that the phase space densities of particles approach a prescribed function, $F\left (v_1,v_2\right )$, and all field components approach zero. It is assumed that $F\left (v_1,v_2\right ) = 0$ if $v_1 \leq W_1$, where $W_1$ is a positive constant. An external magnetic field is prescribed and taken small enough so that no particle is reflected ($v_1$ remains positive). The main issue is to identify the large-time behavior; is a steady state approached and, if so, can it be identified from the time independent Vlasov-Maxwell system? The time-dependent problem is solved numerically using a particle method, and it is observed that a steady state is approached (on a bounded $x$ interval) for large time. For this steady state, one component of the electric field is zero at all points, the other oscillates without decay for $x$ large; in contrast the magnetic field tends to zero for large $x$. Then it is proven analytically that if the external magnetic field is sufficiently small, then (a reformulation of) the steady problem has a unique solution with $B \rightarrow 0$ as $x \rightarrow +\infty$. Thus the “downstream” condition, $B \rightarrow 0$ as $x\rightarrow + \infty$, is used to identify the large time limit of the system.
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[1]1 Batt, J. and Fabian, K., Stationary Solutions of the Relativistic Vlasov-Maxwell System of Plasma and Physics, Chin. Ann. of Math., 14B:3 (1993), 253-278.
[2]2 Bernstein, I., Greene, J., and Kruskal, M., Exact Nonlinear Plasma Oscillations, Phys. Rev., 108, 3 (1957), 546-550.
[3]3 Birdsall, C. K. and Langdon, A. B., Plasma Physics via Computer Simulation, McGraw Hill (1985).
[4]4 DiPerna, R. and Lions, P.-L., Global Solutions of Vlasov-Maxwell Systems, Comm. Pure Appl. Math, 42 (1989), 729-757.
[5]5 Glassey, R., The Cauchy Problem in Kinetic Theory, SIAM: Philadelphia (1996).
[6]6 Glassey, R. and Schaeffer, J., Global Existence of the Relativistic Vlasov-Maxwell System with Nearly Neutral Initial Data, Comm. Math. Phys., 119 (1988), 353-384.
[7]7 Glassey, R. and Schaeffer, J., On the One and One-Half Dimensional Relativistic Vlasov-Maxwell System, Math. Meth. Appl. Sci., 13 (1990), 169-179.
[8]8 Glassey, R. and Schaeffer, J., The Relativistic Vlasov-Maxwell System in Two Space Dimensions: Part I, Arch. Rat. Mech. Anal., 141 (1998), 331-354.
[9]9 Glassey, R. and Schaeffer, J., The Relativistic Vlasov-Maxwell System in Two Space Dimensions: Part II, Arch. Rat. Mech. Anal., 141 (1998), 355-374.
[10]10 Glassey, R. and Schaeffer, J., The Two and One-Half Dimensional Relativistic Vlasov-Maxwell System, Comm. Math. Phys., 185 (1997), 257-284.
[11]11 Glassey, R. and Schaeffer, J., Convergence of a Particle Method for the Relativistic Vlasov-Maxwell System, SIAM Journal on Numerical Analysis, 28(1) (1991), 1-25.
[12]12 Glassey R. and Strauss, W., Absence of Shocks in an Initially Dilute Collisionless Plasma, Comm. Math. Phys., 113 (1987), no. 2, 191-208.
[13]13 Glassey, R. and Strauss, W., Similarity Formation in a Collisionless Plasma Could Occur Only at High Velocities, Arch. Rat. Mech. Anal., 92 (1986), 59-90.
[14]14 Guo, Y., Stable Magnetic Equilibria in Collisionless Plasmas, Comm. Pure and Applied Math., 50 (1997), 891-933.
[15]15 Guo, Y. and Ragazzo, C. G., On Steady States in a Collisionless Plasma, Comm. Pure and Applied Math., 49 (1996), 1145-1174.
[16]16 Guo, Y. and Strauss, W., Instability of periodic BGK equilibria, Comm. Pure and Applied Math., 48 (1995), 861-846.
[17]17 Guo, Y. and Strauss, W., Nonlinear Instability of Double-Humped Equilibria, Ann. Inst. Henri Poincaré, 12 (1995), 339-352.
[18]18 Guo, Y. and Strauss, W., Unstable oscillatory-tail solutions, SIAM J. Math. Analysis, 30, no. 5 (1999), 1076-1114.
[19]19 Horst, E., On the asymptotic growth of the solutions of the Vlasov-Poisson system, Math. Meth. Appl. Sci. 16 (1993), 75-85.
[20]20 Lions, P.-L. and Perthame, B., Propogation of Moments and Regularity for the Three Dimensional Vlasov-Poisson System, Inventions Mathematical, 105 (1991), 415-430.
[21]21 Morawetz, C. S., Magnetohydrodynamical shock structure without collisions, Phys. Fluids, 4 (1961), 988-1006.
[22]22 Pfaffelmoser, K., Global Classical Solutions of the Vlasov-Poisson System in Three Dimensions for General Initial Data, J. Diff. Eqn., 95(2) (1992), 281-303.
[23]23 Rein, G., Nonlinear Stability for the Vlasov-Poisson system - the energy - Cashmir method, Math. Meth. in the Appl. Sci., 17 (1994), 1129-1140.
[24]24 Rein, G., Existence of Stationary Collisionless Plasmas on Bounded Domains, Math. Meth. in the Appl. Sci., 15 (1992), 365-374.
[25]25 Rein, G., Generic Global Solutions of the Relativistic Vlasov-Maxwell System of Plasma Physics, Comm. Math. Phys., 135 (1990), 41-78.
[26]26 Schaeffer, J., Global Existence of Smooth Solutions to the Vlasov-Poisson System in Three Dimensions, Comm. Part. Diff. Eqn., 16(8 and 9) (1991), 1313-1335.
[27]27 Schaeffer, J., Steady States for a One Dimensional Model of the Solar Wind, Quart. of Appl. Math., 59 (2001), 507-528.
[28]28 Schaeffer, J., The Classical Limit of the Relativistic Vlasov-Maxwell System, Commun. Math. Phys., 104 (1986), 403-421.
[29]29 Schaeffer, J., A Small Data Theorem for Collisionless Plasma that Includes High Velocity Particles, Indiana University Mathematics Journal 53, 1 (2004), 1-34.
[30]30 Tidman, D. and Krall, N., Shock Waves in Collisionless Plasmas, Wiley-Interscience (1971).
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Additional Information
Jack Schaeffer
Affiliation:
Department of Mathematical Sciences, Carnegie Mellon University, Pittsburgh, Pennsylvania 15213
Email:
js5m@andrew.cmu.edu
Received by editor(s):
October 13, 2004
Published electronically:
September 22, 2005
Article copyright:
© Copyright 2005
Brown University
The copyright for this article reverts to public domain 28 years after publication.