1995
DOI: 10.1103/physreve.52.5425
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Thomson scattering of intense lasers from electron beams at arbitrary interaction angles

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Cited by 141 publications
(120 citation statements)
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“…While the theory of Thomson backscattered radiation is well known and has been well documented [18][19][20][21][22][23][24], there remains a need to have a complete three-dimensional time resolved computational capability for the full determination of the temporally and spatially resolved spectra and intensity distributions produced from a Thomson interaction of arbitrary geometry. This capability is crucial for both the design of Thomson scattered x-ray sources, as well as future experiments and applications utilizing such sources.…”
Section: Introductionmentioning
confidence: 99%
“…While the theory of Thomson backscattered radiation is well known and has been well documented [18][19][20][21][22][23][24], there remains a need to have a complete three-dimensional time resolved computational capability for the full determination of the temporally and spatially resolved spectra and intensity distributions produced from a Thomson interaction of arbitrary geometry. This capability is crucial for both the design of Thomson scattered x-ray sources, as well as future experiments and applications utilizing such sources.…”
Section: Introductionmentioning
confidence: 99%
“…Neglecting higher harmonics, the energy of the emitted photons for the case of a near head-on collision of the laser pulse and a bunch of relativistic electrons is given by [27,28] …”
mentioning
confidence: 99%
“…For head-on collision and relativistic intensities of the colliding pulse the number of generated x-ray photons N X per shot is given by [27,28] …”
mentioning
confidence: 99%
“…This feature is physically understandable, if we take into account that the ultrarelativistic electron moves practically in phase with the copropagating component of the standing wave and experiences quickly oscillating force from the counterpropagating component. Thus, we can expect that the overall angular and spectral spread of the radiated photons shall generally obey distributions obtained in [14,15,19,20] for Compton (or Thomson) backscattering of a single laser beam on the relativistic electron beam. However, more detailed analysis may be necessary, especially for angular and frequency distributions of the radiation intensity that depend on the initial phase.…”
Section: Discussionmentioning
confidence: 99%