53
520
521
523
524
52-1
52-6
41.00
29.35
29.31
29.33
29.27
29.05
03.06.01
03.05.01
03.04.03
2
223
614
6135
SCI004000
SCI005000
The interaction of the cosmological gamma-ray background photons with soft cosmological background with producing electron-positron pairs is considered. It is shown that the majority of positrons are produced with energies of 10 Gev - 1 TeV. However, the interaction of ``X-ray" cosmological background photons may produce the positrons with energies of 10-100 keV.
cosmology: cosmic background radiation; positrons
1. Ackermann M., Ajello M., Albert A., et al., 2015, Astrophysical Journal, 799, id. 86
2. Ajello M., Greiner J., Sato G., et al., 2008, Astrophysical Journal, 689, p. 666
3. Behroozi P., Wechsler R., and Conroy C., 2013, Astrophysical Journal, 770, id. 57
4. Cooray A., 2016, Royal Society Open Science, 3, p. 150555
5. Franceschini A., Rodighiero G., and Vaccari M., 2008, Astronomy and Astrophysics, 487, p. 837
6. Gould R. and Schreder G., 1967, Physical Review, 155, p. 1408
7. Grebenev S. and Sunyaev R., 2020, Astronomy Letters, 45, p. 791
8. Hill R., Masui K., and Scott D., 2018, Applied Spectroscopy, 72, p. 663
9. Nizamov B. and Pshirkov M., 2023, Astronomy Letters, 49, p. 9
10. Nizamov B. and Pshirkov M., 2024, Astronomy Letters, 50, p. 186
11. Popov A., Barsukov D., Ivanchik A., and Bobashev S., 2023, Technical Physics, 68, p. 1619