Positron Production Due to Interaction of Cosmological Background Photons

IF 1.1 4区物理与天体物理 Q4 PHYSICS, APPLIED

Technical Physics Pub Date : 2024-09-26 DOI:10.1134/S1063784224060343

A. N. Popov, D. P. Barsukov, A. V. Ivanchik, S. V. Bobashev

引用次数: 0

Abstract

The interaction of photons of the cosmological gamma-ray background radiation to photons of extragalactic background light with producing electron-positron pairs is considered. It is shown that the majority of positrons is produced with energy 10 GeV–1 TeV.

Abstract Image

查看原文本刊更多论文

宇宙背景光子相互作用导致的正电子产生

研究考虑了宇宙伽马射线背景辐射的光子与银河系外背景光的光子之间产生电子-正电子对的相互作用。结果表明，大部分正电子的能量为 10 GeV-1 TeV。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

求助全文

约1分钟内获得全文求助全文

来源期刊

Technical Physics 物理-物理：应用

CiteScore

1.30

自引率

14.30%

发文量

139

审稿时长

3-6 weeks

期刊介绍： Technical Physics is a journal that contains practical information on all aspects of applied physics, especially instrumentation and measurement techniques. Particular emphasis is put on plasma physics and related fields such as studies of charged particles in electromagnetic fields, synchrotron radiation, electron and ion beams, gas lasers and discharges. Other journal topics are the properties of condensed matter, including semiconductors, superconductors, gases, liquids, and different materials.