A set of nonlinear differential equations that describe moving relativistic
solitons is investigated analytically and solved numerically. The influenc
e of the ion motion on the soliton structure is investigated. It is demonst
rated that, depending on the propagation velocity, relativistic solitary wa
ves can occur in the form of bright solitons, dark solitons, or collisionle
ss electromagnetic shock waves. In the limit of a low propagation velocity,
a dark soliton can trap the ions and accelerate them. In the case of a bri
ght soliton, the effects of ion dynamics limit the soliton amplitude. The c
onstraint on the maximum amplitude is related to either the breaking of ion
motion or the intersection of electron trajectories. The soliton breaking
provides a new mechanism for ion and electron acceleration in the interacti
on of high-intensity laser pulses with plasmas. (C) 2001 MAIK "Nauka/Interp
eriodica".