1996
DOI: 10.1103/physrevlett.76.3116
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Observation of Nonlinear Effects in Compton Scattering

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Cited by 605 publications
(487 citation statements)
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“…One important reason is that in physical experiments one endeavors to define as exactly as possible the initial and/or final states of the systems being considered. Moreover experiments on laser-induced process in strong laser fields well be- * Electronic address: bouzid.manaut@laposte.net † Electronic address: attaourti@ucam.ac.ma yond the atomic field strength intensity of about 3.5 10 16 W/cm 2 have clearly given evidence of relativistic effects [5]. However, the search for spin-specific effects has been rare [6]- [7].…”
Section: Introductionmentioning
confidence: 99%
“…One important reason is that in physical experiments one endeavors to define as exactly as possible the initial and/or final states of the systems being considered. Moreover experiments on laser-induced process in strong laser fields well be- * Electronic address: bouzid.manaut@laposte.net † Electronic address: attaourti@ucam.ac.ma yond the atomic field strength intensity of about 3.5 10 16 W/cm 2 have clearly given evidence of relativistic effects [5]. However, the search for spin-specific effects has been rare [6]- [7].…”
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%
“…Though pair production has been demonstrated at SLAC (E144-experiment) [32] by the interaction of y-ray with an intense laser at intensities in the range of 10 18 W/cm 2 , the direct production of pairs by a high-intensity laser from vacuum remains elusive. The rule of thumb for threshold of pair production derives from the simple argument that it is the field necessary for a virtual electron to gain an energy 2raoc 2 during its lifetime §t , imposed by the Heisenberg uncertainty principle 8f =/?/raoc 2 , the energy gain length, c5t is the Compton length K c .…”
Section: Nonlinear Qed and Horizon Physicsmentioning
confidence: 99%