Journal Article PUBDB-2025-00578

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High-Statistics Measurement of the Cosmic-Ray Electron Spectrum with H.E.S.S.

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2024
APS College Park, Md.

Physical review letters 133(22), 221001 () [10.1103/PhysRevLett.133.221001]
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Report No.: arXiv:2411.08189

Abstract: Owing to their rapid cooling rate and hence loss-limited propagation distance, cosmic-ray electrons and positrons (CRe) at very high energies probe local cosmic-ray accelerators and provide constraints on exotic production mechanisms such as annihilation of dark matter particles. We present a high-statistics measurement of the spectrum of CRe candidate events from 0.3 to 40 TeV with the High Energy Stereoscopic System, covering 2 orders of magnitude in energy and reaching a proton rejection power of better than 104. The measured spectrum is well described by a broken power law, with a break around 1 TeV, where the spectral index increases from Γ1=3.25±0.02(stat)±0.2(sys) to Γ2=4.49±0.04(stat)±0.2(sys). Apart from the break, the spectrum is featureless. The absence of distinct signatures at multi-TeV energies imposes constraints on the presence of nearby CRe accelerators and the local CRe propagation mechanisms.

Classification:

Note: Phys. Rev. Lett. 133, 221001 (2024). PhysRevLett.133.221001. main paper: 8 pages, 4 figures, supplemental material: 12 pages, 14 figures, accepted for publication in Physical Review Letters https://journals.aps.org/prl/

Contributing Institute(s):
  1. Gammaastronomie (Z_GA)
Research Program(s):
  1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
Experiment(s):
  1. High Energy Stereoscopic System

Appears in the scientific report 2024
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 Record created 2025-01-31, last modified 2025-07-15


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