With recent advances in laser technology we have seen laser intensities reach the order of
10^22 W/cm2, with higher intensities anticipated in the near future. This thesis concerns a
classical approach to the simulation of laser matter interactions for intensities above the
relativistic threshold of 10^18 W/cm2. A pulsed plane wave model is used to simulate the
laser fields. In particular this thesis aims to determine the effect of radiation reaction on
relativistic interactions as well as proposing an effective method of vacuum laser acceleration
from rest. We consider the equations of motion accounting for radiative effects
and present their analytic plane wave solution. A novel numerical scheme to solve the
equations of motion for arbitrary field configurations is presented. The method is manifestly
covariant and exact for constant fields. Radiative reaction effects are explored using
the numerical method and we find that the electron gains energy from the radiation field
produced by its acceleration. Methods of vacuum laser acceleration are studied and we
predict a significant acceleration using two co-propagating lasers where the frequency of
the two lasers differ significantly. We also look at analytic and numerical solutions of the
radiation spectrum, observing an increase in oscillations in the spectrum for larger intensities.
We see more photons radiated when we include radiative terms in our calculations.
Date of Award | 2013 |
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Original language | English |
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Awarding Institution | |
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Supervisor | Kurt Langfeld (Other Supervisor) |
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Simulating Relativistic Laser Matter Interactions
Iji, N. (Author). 2013
Student thesis: PhD