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This article is cited in 1 scientific paper (total in 1 paper)
FIELDS, PARTICLES, AND NUCLEI
Production of positrons by cosmic rays
I. M. Dremin, D. O. Chernyshov Lebedev Physical Institute, Russian Academy of Sciences, Moscow, 119991 Russia
Abstract:
It is shown that electromagnetic interactions of cosmic ray protons provide a noticeable contribution to positrons production. This is due to a combination of low energy threshold of electron–positron pair creation compared to the thresholds of pion creation in strong interactions and rapid decrease of the cosmic rays energy spectrum. Moreover, the electromagnetically produced positrons are very soft, therefore their annihilation with background electrons directly produces the observed 511 keV gamma-line.
Received: 30.05.2024 Revised: 14.06.2024 Accepted: 20.06.2024
Citation:
I. M. Dremin, D. O. Chernyshov, “Production of positrons by cosmic rays”, Pis'ma v Zh. Èksper. Teoret. Fiz., 120:2 (2024), 79–82; JETP Letters, 120:2 (2024), 79–82
Linking options:
https://www.mathnet.ru/eng/jetpl7273 https://www.mathnet.ru/eng/jetpl/v120/i2/p79
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