Issue |
EPJ Web Conf.
Volume 191, 2018
XXth International Seminar on High Energy Physics (QUARKS-2018)
|
|
---|---|---|
Article Number | 08011 | |
Number of page(s) | 6 | |
Section | Cosmology and Astroparticle Physics | |
DOI | https://doi.org/10.1051/epjconf/201819108011 | |
Published online | 31 October 2018 |
https://doi.org/10.1051/epjconf/201819108011
Photon splitting in strongly magnetized medium with taking into account positronium influence
1
Division of Physics, Yaroslavl Higher Military School of Air Defense, Moscow Prospect 28, 150001 Yaroslavl, Russian Federation
2
Division of Theoretical Physics, Department of Physics, Yaroslavl State P. G. Demidov University, Sovietskaya 14, 150000 Yaroslavl, Russian Federation
* e-mail: anik-roman@mail.ru
** e-mail: mch@uniyar.ac.ru
*** e-mail: rda@uniyar.ac.ru
**** e-mail: allen_caleb@rambler.ru 1We use the natural units c = ħ = k = 1, m is the electron mass, e > 0 is the elementary charge.
Published online: 31 October 2018
The process of the photon splitting, γ → γγ, is investigated in strongly magnetized vacuum with taking into account positronium influence. The dispersion properties of photons and the new polarization selection rules are obtained. The absorption rate of the leading photon splitting channels are calculated with taking account of the photon dispersion and wave function renormalization.
© The Authors, published by EDP Sciences, 2018
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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