1983
DOI: 10.1103/physreva.28.609
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Connection between the bremsstrahlung tip and direct radiative recombination: Angular distributions and polarization correlations

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1984
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Cited by 16 publications
(10 citation statements)
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“…Radiative recombination itself is related to its time-reversed processes, namely, photoionization and electron-positron pair production, by the principle of detailed balance [5,[11][12][13]. By comparing bremsstrahlung and radiative recombination it was shown theoretically that at the threshold dividing the two cases, i.e., the case of a finally free electron with negligibly low kinetic energy in the continuum E f 0 and the case E f 0 resulting in a finally bound electron captured into a high-lying Rydberg state n → ∞, both processes show comparable features in the differential cross sections and thus show a smooth transition from one process to the other [5,9,[14][15][16].…”
Section: Introductionmentioning
confidence: 89%
“…Radiative recombination itself is related to its time-reversed processes, namely, photoionization and electron-positron pair production, by the principle of detailed balance [5,[11][12][13]. By comparing bremsstrahlung and radiative recombination it was shown theoretically that at the threshold dividing the two cases, i.e., the case of a finally free electron with negligibly low kinetic energy in the continuum E f 0 and the case E f 0 resulting in a finally bound electron captured into a high-lying Rydberg state n → ∞, both processes show comparable features in the differential cross sections and thus show a smooth transition from one process to the other [5,9,[14][15][16].…”
Section: Introductionmentioning
confidence: 89%
“…The SM calculations are done for the differential cross sections [24,31] and P 1 [9] up to 15 MeV. The partial-wave results also concern the differential cross sections [8,33,34,31] and P 1 [8,34] at energies mostly below 2 MeV. In [35,36,34] another noticable advantage of the SWL was explored, the smooth transition between bremsstrahlung at threshold and radiative recombination (RR) of a free electron into infinitely high-lying Rydberg states of the target.…”
Section: Introductionmentioning
confidence: 99%
“…Strong effects of the spin-orbital interaction were observed via left-right asymmetry of bremsstrahlung from transversally spinoriented electrons [4]. This high energy tip region might also be considered as the Rydberg series limit of radiative recombination (RR) [5,6] and therefore it also describes the spin dynamics of the fundamental process of photoionization in time reversal [7]. Relativistic theories predict that more differential studies of linear polarization of photons emitted by polarized electrons, with a particular emphasis on the angle of polarization, should reveal significantly finer details of the spin dynamics of electrons in strong fields [3,8].…”
mentioning
confidence: 99%
“…To evaluate c for this particular energy we have extrapolated the results of the RR polarization calculations towards the continuum threshold. Such a computational approach has been justified for the tip region in a number of works (see, for example, [6] and references therein). In the present contribution, the polarization of the RR photons emitted due to the recombination of longitudinally polarized electrons into bound high-n states has been calculated within the fully relativistic theory.…”
mentioning
confidence: 99%