THE TELEGRAPH EQUATION IN CHARGED-PARTICLE TRANSPORT

被引:48
作者
GOMBOSI, TI [1 ]
JOKIPII, JR [1 ]
KOTA, J [1 ]
LORENCZ, K [1 ]
WILLIAMS, LL [1 ]
机构
[1] UNIV ARIZONA,DEPT PLANETARY SCI,LUNAR & PLANETARY LAB,TUCSON,AZ 85721
关键词
ACCELERATION OF PARTICLES; COSMIC RAYS; DIFFUSION;
D O I
10.1086/172209
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a new derivation of the telegraph equation which modifies its coefficients. First, an infinite-order partial differential equation is obtained for the velocity-space solid angle-averaged phase-space distribution of particles which underwent at least a few collisions. It is shown that in the lowest order asymptotic expansion this equation simplifies to the well-known diffusion equation. The second-order asymptotic expansion for isotropic small-angle scattering results in a modified telegraph equation with a signal propagation speed of v(5/11)1/2 instead of the usual v/3(1/2). Our derivation of a modified telegraph equation follows from an expansion of the Boltzmann equation in the relevant smallness parameters and not from a truncation of an eigenfunction expansion. This equation is consistent with causality. It is shown that under steady state conditions in a convecting plasma the telegraph equation may be regarded as a diffusion equation with a modified transport coefficient, which describes a combination of diffusion and cosmic-ray inertia. This modified transport coefficient becomes negative for particles with random velocities less than the critical velocity, v(c). This negative value is a consequence of the second time derivative term in the telegraph equation and it is closely related to causality.
引用
收藏
页码:377 / 384
页数:8
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