2015
DOI: 10.1088/1367-2630/17/5/053025
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Longitudinal and transverse cooling of relativistic electron beams in intense laser pulses

Abstract: With the emergence in the next few years of a new breed of high power laser facilities, it is becoming increasingly important to understand how interacting with intense laser pulses affects the bulk properties of a relativistic electron beam. A detailed analysis of the radiative cooling of electrons indicates that, classically, equal contributions to the phase space contraction occur in the transverse and longitudinal directions. In the weakly quantum regime, in addition to an overall reduction in beam cooling… Show more

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Cited by 44 publications
(65 citation statements)
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References 26 publications
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“…The solutions (23), (24) are consistent with those made by Joffe et al [19]. When the RR is negligible (formally τ r → 0), the function h (φ, ρ 0 ) tends to 1 and the electron motion reduces to the standard solution of the Lorentz equation in a plane wave [21].…”
Section: Analytical Model For the Radiating Electron Sourcesupporting
confidence: 85%
See 2 more Smart Citations
“…The solutions (23), (24) are consistent with those made by Joffe et al [19]. When the RR is negligible (formally τ r → 0), the function h (φ, ρ 0 ) tends to 1 and the electron motion reduces to the standard solution of the Lorentz equation in a plane wave [21].…”
Section: Analytical Model For the Radiating Electron Sourcesupporting
confidence: 85%
“…This opposite behavior is due to the stochasticity of photon emission, which becomes dominant in the full quantum regime, at the expense of the incoherent emission of multiple photons in the classical regime. These results have been confirmed by a similar study in reference [19].…”
Section: Introductionsupporting
confidence: 84%
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“…In the decades since its introduction it has become the dominant description of radiation reaction, and has been applied to electron dynamics [21][22][23][24][25][26][27][28], ion acceleration [29][30][31], and high-energy synchrotron radiation [32]. However, its provenance as an approximation to an unphysical equation questions its validity.…”
Section: Introductionmentioning
confidence: 99%
“…As quantum effects become more important, classical theories overestimate the amount of radiation emitted [16,7] which is accounted for by a rescaling of the characteristic time τ → τ g(χ) in equation (1), where the quantum nonlinearity parameter χ = eh F ab F acẋbẋ c /m 2 e and we use the approximation g(χ) = (1 + 12χ + 31χ 2 + 3.7χ…”
Section: Introductionmentioning
confidence: 99%