PlanetPhysics/Plasma Wave Excitation
Electron Acceleration by Non-linear Plasma Wave Excitation
Consider an electron pulse (or "bunch") of average density and average bunch [[../Velocity/|velocity]] in a surrounding [[../PlasmaDisplayPanel/|plasma]] of average electron density . One is interested in deriving the propagation equations for plasma [[../CosmologicalConstant2/|waves]] with relativistic phase velocities. A simplifying assumption is the presence of relatively slow moving ions at a very small fraction of the [[../CosmologicalConstant/|speed of light]] {\mathbf c} which is realistic for plasma ion temperatures of less than 10,000 K. One may also neglect in a first approximation the influence of the excited wake-field that affects the time-evolution of the electron pulse shape. Furthermore, one can consider the configuration of a cylindrical plasma in the absence of external [[../NeutrinoRestMass/|magnetic fields]]; along the plasma containing tube - axis one has a one-dimensional [[../SimilarityAndAnalogousSystemsDynamicAdjointnessAndTopologicalEquivalence/|system]] for which [[../FluorescenceCrossCorrelationSpectroscopy/|Maxwell's equations]] can be written in the following simplified form for the [[../FluorescenceCrossCorrelationSpectroscopy/|electrical field]] , average electron velocity in plasma , [[../Charge/|charge]] density , current density and perturbed electron density : and .
The equation of [[../CosmologicalConstant/|motion]] of a plasma electron with [[../Momentum/|momentum]] in the wake of a relativistic electron bunch of average velocity can be then written as:
Because the driving electron pulse has a relativistic average velocity one can expect solutions of the equations of motion to be of the form of travelling waves:
.
Molecular dynamics experiments or [[../AAT/|computer simulations]] that include these equations provide results in the form of numerical data that are consistent with such travelling wave solutions.