Abstract
The process of resonant high-energy electron–positron pairs production by electrons in an X-ray pulsar electromagnetic field is studied theoretically. Under the resonance conditions, the second-order process under consideration effectively reduces into two sequential first-order processes: X-ray-stimulated Compton effect and X-ray–stimulated Breit–Wheeler process. The kinematics of the process is studied in detail: the dependencies of the energy of the scattered electron on its outgoing angle and the energies of the particles of the pair on the outgoing angle of the scattered electron and the opening angle of the pair are obtained. The analysis of the number of different possible particles energies values in the entire range of the angles is also carried out, according to which the energies of the particles of the pair can take up to eight different values at a fixed outgoing angle of the scattered electron and opening angle of the pair. The estimate of the resonant differential probability per unit time of the process, which reaches the maximum value of 24 orders of the value of the non-resonant differential probability per unit time, is obtained. The angular distribution of the differential probability per unit time of the process is analyzed, particularly for the case of high-energy positrons presenting in pulsar radiation.
Highlights
Oleinik resonances [1,2] have been studied for quite a long time
Since the works of Oleinik, various resonant processes of quantum electrodynamics in an external electromagnetic field have been considered from different angles
In the monograph [5], the first-order external field quantum electrodynamics (QED) processes into which higher-order processes reduce in resonance are studied in detail and in the works [6–26], the resonant second-order external field QED
Summary
Oleinik resonances [1,2] (see reviews [3,4]) have been studied for quite a long time. May be produced by pulsars, in particular, in the process of resonant electron-positron pair production in collision of an electron with the electromagnetic field of a pulsar. The process of electron–positron pairs production in collision of electrons with an electromagnetic wave ( non-linear trident pair production, NTPP) was studied in [29–34]. The NTPP process was studied in [23], but resonant kinematics of the process was not studied in sufficient detail, and only an estimate of the resonant differential probability was given.
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