ON THE ONE AND 1/2 DIMENSIONAL RELATIVISTIC VLASOV-MAXWELL SYSTEM

被引：79

作者：

GLASSEY, R ^{[1
]}

SCHAEFFER, J ^{[1
]}

机构：

[1] CARNEGIE MELLON UNIV,DEPT MATH,PITTSBURGH,PA 15213

来源：

MATHEMATICAL METHODS IN THE APPLIED SCIENCES | 1990年 / 13卷 / 02期

关键词：

D O I：

10.1002/mma.1670130207

中图分类号：

O29 [应用数学];

学科分类号：

070104 [应用数学];

摘要：

The time evolution of a collisionless plasma is studied in the case when the Viasov density ƒ is a function of the time, one space variable and two velocity variables. The electromagnetic fields E, B also have a special structure, and the magnetic field B is non‐trivial. It is shown that smooth, consistent initial values generate a uniquc smooth global solution. Copyright © 1990 John Wiley & Sons, Ltd

引用

页码：169 / 179

页数：11

共 12 条

[1]

GLOBAL SYMMETRIC SOLUTIONS OF INITIAL VALUE-PROBLEM OF STELLAR DYNAMICS [J].