Abstract

The process of resonant high-energy electron–positron pair production by an ultrarelativistic electron colliding with the field of an X-ray pulsar is theoretically investigated. Resonant kinematics of the process is studied in detail. Under the resonance condition, the intermediate virtual photon in the X-ray pulsar field becomes a real particle. As a result, the initial process of the second order in the fine structure constant effectively reduces into two successive processes of the first order: X-ray-stimulated Compton effect and X-ray-stimulated Breit–Wheeler process. For a high-energy initial electron all the final ultrarelativistic particles propagate in a narrow cone along the direction of the initial electron momentum. The presence of threshold energy for the initial electron which is of order of 100 MeV for 1-KeV-frequency field is shown. At the same time, the energy spectrum of the final particles (two electrons and a positron) highly depends on their exit angles and on the initial electron energy. This result significantly distinguishes the resonant process from the non-resonant one. It is shown that the resonant differential probability significantly exceeds the non-resonant one.

Highlights

  • Resonant nonlinear effects of quantum electrodynamics (QED) can be observed in strong electromagnetic fields

  • To create such fields and ultrarelativistic particles special conditions are required. These conditions can be achieved near specific space objects, such as neutron stars, pulsars, magnetars or supernovae. It has been reported of anomalous high-energy positron abundance [1] in cosmic rays, which are suggested to be produced by pulsars [2]

  • In contrast to the works discussed above in this paper the resonant high-energy electron-positron pair production by an ultrarelativistic electron colliding with the field of an X-ray pulsar is theoretically investigated

Read more

Summary

Introduction

Resonant nonlinear effects of quantum electrodynamics (QED) can be observed in strong electromagnetic fields To create such fields and ultrarelativistic particles special conditions are required. These conditions can be achieved near specific space objects, such as neutron stars, pulsars, magnetars or supernovae. Several external field QED effects make contribution to production of high-energy positrons. In this paper resonant ultrarelativistic electron-positron pair production by high-energy electrons in the field of the X-ray pulsar is studied. The process of high-energy electron–positron pair production by an ultrarelativistic electron colliding with an external field is studied in works [23–27]. In contrast to the works discussed above in this paper the resonant high-energy electron-positron pair production by an ultrarelativistic electron colliding with the field of an X-ray pulsar is theoretically investigated. We aim to compare the differential probability of the process and the differential probability of the non-resonant one

External Field Description
Amplitude of Ultrarelativistic Electron–Positron Pair Production
Resonant Kinematics of Ultrarelativistic Electron–Positron Pair Production
Conclusions

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.