Suppr超能文献

地面探测来自雷暴云的电子-正电子湮没线。

On-ground detection of an electron-positron annihilation line from thunderclouds.

机构信息

Department of Physics, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan.

High Energy Astrophysics Laboratory, RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0193, Japan.

出版信息

Phys Rev E. 2016 Feb;93(2):021201. doi: 10.1103/PhysRevE.93.021201. Epub 2016 Feb 16.

Abstract

Thunderclouds can produce bremsstrahlung gamma-ray emission, and sometimes even positrons. At 00:27:00 (UT) on 13 January 2012, an intense burst of gamma rays from a thundercloud was detected by the GROWTH experiment, located in Japan, facing the Sea of Japan. The event started with a sharp gamma-ray flash with a duration of <300 ms coincident with an intracloud discharge, followed by a decaying longer gamma-ray emission lasting for ∼60 s. The spectrum of this prolonged emission reached ∼10 MeV, and contained a distinct line emission at 508±3(stat.)±5(sys.) keV, to be identified with an electron-positron annihilation line. The line was narrow within the instrumental energy resolution (∼80keV), and contained 520±50 photons which amounted to ∼10% of the total signal photons of 5340±190 detected over 0.1-10 MeV. As a result, the line equivalent width reached 280±40 keV, which implies a nontrivial result. The result suggests that a downward positron beam produced both the continuum and the line photons.

摘要

雷暴云可以产生韧致辐射伽马射线发射,有时甚至可以产生正电子。2012 年 1 月 13 日 00:27:00(UT),位于日本面向日本海的 GROWTH 实验探测到了来自雷暴云的强烈伽马射线爆发。该事件以持续时间<300ms 的强烈伽马射线闪光开始,与云内放电同时发生,随后是持续约 60s 的衰减较长的伽马射线发射。这次延长的发射光谱达到了约 10 MeV,并包含了一个在 508±3(统计)±5(系统)keV 处明显的线发射,被认为是电子-正电子湮没线。该线在仪器能量分辨率(约 80keV)内很窄,包含 520±50 个光子,占在 0.1-10 MeV 范围内探测到的 5340±190 个总信号光子的约 10%。因此,线等效宽度达到 280±40 keV,这意味着一个重要的结果。结果表明,一个向下的正电子束产生了连续谱和线光子。

文献AI研究员

20分钟写一篇综述,助力文献阅读效率提升50倍。

立即体验

用中文搜PubMed

大模型驱动的PubMed中文搜索引擎

马上搜索

文档翻译

学术文献翻译模型,支持多种主流文档格式。

立即体验