2020
DOI: 10.1103/physreva.102.022809
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Nonlinear Compton scattering of polarized photons in plane-wave backgrounds

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Cited by 53 publications
(32 citation statements)
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“…Thus we expect the formalism to be very well-suited for future calculations of non-linear Compton scattering [44][45][46][47][48][49][50], including at higher orders, as well as its crossed process, multiple photon Bremsstrahlung (see, for example, [51][52][53][54][55][56][57][58]) and electron-positron annihilation into several photons [59][60][61][62]. This will, of course, require a computer algebra implementation, which is in progress.…”
Section: Discussionmentioning
confidence: 99%
“…Thus we expect the formalism to be very well-suited for future calculations of non-linear Compton scattering [44][45][46][47][48][49][50], including at higher orders, as well as its crossed process, multiple photon Bremsstrahlung (see, for example, [51][52][53][54][55][56][57][58]) and electron-positron annihilation into several photons [59][60][61][62]. This will, of course, require a computer algebra implementation, which is in progress.…”
Section: Discussionmentioning
confidence: 99%
“…[50,51]. The extension of this technique into nonlinear regime is possible [47,[52][53][54]. In the extreme nonlinear regime, it will allow us to obtain circularly polarized brilliant γ rays via nonlinear Compton scattering from longitudinally spin-polarized electrons [49], highly sought in detecting schemes of vacuum birefringence in ultrastrong laser fields [55][56][57].…”
mentioning
confidence: 99%
“…Althouth the ICS spectrum is at a considerably lower than the maximum energy achievable with a bremsstrahlung source, the ICS photons are mono-energetic and highly linearly polarised (above 75 %), (see also Refs. [120,121]). The quantum energy parameter is η γ 0.1 (for a head-on collision at the strong-field IP).…”
Section: Inverse Compton Sourcementioning
confidence: 99%