1993
DOI: 10.1103/physreve.48.3003
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Nonlinear Thomson scattering of intense laser pulses from beams and plasmas

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Cited by 438 publications
(439 citation statements)
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“…Using the betatron orbits given above, the radiation spectrum can be calculated with conventional techniques [36] - [38]. It is convenient to introduce spherical coordinates (r, θ, φ) and unit vectors (e r , e θ , e φ ), where x = r sin θ cos φ, y = r sin θ sin φ, z = r cos θ, and e r = sin θ cos φ e x + sin θ sin φ e y + cos θ e z ,…”
Section: Synchrotron Radiationmentioning
confidence: 99%
“…Using the betatron orbits given above, the radiation spectrum can be calculated with conventional techniques [36] - [38]. It is convenient to introduce spherical coordinates (r, θ, φ) and unit vectors (e r , e θ , e φ ), where x = r sin θ cos φ, y = r sin θ sin φ, z = r cos θ, and e r = sin θ cos φ e x + sin θ sin φ e y + cos θ e z ,…”
Section: Synchrotron Radiationmentioning
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%