CR电子:走向更完整的空气-切伦科夫视图

Michele Palatiello
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引用次数: 0

摘要

甚高能量;E比;30 GeV)从太阳系外到达地球的宇宙射线电子和正电子(CRe−,e+)是我们银河系附近(1 - 2kpc)最近高能事件的重要示踪剂。这种辐射的光谱测量可能有助于检查CRe -, e+起源的标准天体物理情景(例如,脉冲星,信噪比)与奇异情景(例如,DM粒子湮灭)。Air-Cherenkov望远镜可以帮助测量CRe−,e+的VHE总通量。这将使我们能够通过ATIC, HESS, AMS-02和Fermi-LAT等整合相关结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
CR electrons: towards a more complete air-Cherenkov view

Very high energy (VHE; E > 30 GeV) cosmic-ray electrons and positrons (CRe, e+) reaching the Earth from beyond the solar system are important tracers of recent energetic events in our Galactic neighbourhood (1–2 kpc). Spectral measurements of this radiation may help checking standard astrophysical scenarios of CRe, e+ origin (e.g., pulsars, SNRs) versus exotic scenarios (e.g., DM particle annihilation). Air-Cherenkov telescopes can contribute to the measurement of the total VHE flux of CRe, e+. This will allow us to consolidate relevant results by, e.g., ATIC, HESS, AMS-02, and Fermi-LAT.

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