Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons

Abstract

High energy cosmic ray electrons plus positrons (CREs), which lose energy quickly during their propagation, provide an ideal probe of Galactic high-energy processes and may enable the observation of phenomena such as dark-matter particle annihilation or decay. The CRE spectrum has been directly measured up to $\sim 2$ TeV in previous balloon- or space-borne experiments, and indirectly up to $\sim 5$ TeV by ground-based Cherenkov $\gamma$-ray telescope arrays. Evidence for a spectral break in the TeV energy range has been provided by indirect measurements of H.E.S.S., although the results were qualified by sizeable systematic uncertainties. Here we report a direct measurement of CREs in the energy range $25\mathrm{GeV}-4.6\mathrm{TeV}$ by the DArk Matter Particle Explorer (DAMPE) with unprecedentedly high energy resolution and low background. The majority of the spectrum can be properly fitted by a smoothly broken power-law model rather than a single power-law model. The direct detection of a spectral break at $E\sim 0.9$ TeV confirms the evidence found by H.E.S.S., clarifies the behavior of the CRE spectrum at energies above 1 TeV and sheds light on the physical origin of the sub-TeV CREs.

arXiv comment18 pages, 6 figures, Nature in press, doi:10.1038/nature24475

References in corpus (23)

• Particle Dark Matter: Evidence, Candidates and Constraints
• Observation of an anomalous positron abundance in the cosmic radiation
• Dark Matter Candidates from Particle Physics and Methods of Detection
• Cosmic-ray propagation and interactions in the Galaxy
• Measurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope
• Detection of the Characteristic Pion-Decay Signature in Supernova Remnants
• Production and propagation of cosmic-ray positrons and electrons
• The energy spectrum of cosmic-ray electrons at TeV energies
• Boosted Decision Trees as an Alternative to Artificial Neural Networks for Particle Identification
• Pulsars as the Sources of High Energy Cosmic Ray Positrons
• Probing the ATIC peak in the cosmic-ray electron spectrum with H.E.S.S
• The cosmic-ray electron flux measured by the PAMELA experiment between 1 and 625 GeV
• The DArk Matter Particle Explorer mission
• The origin of the positron excess in cosmic rays
• The Most Likely Sources of High Energy Cosmic-Ray Electrons in Supernova Remnants
• Cosmic-ray electron+positron spectrum from 7 GeV to 2 TeV with the Fermi Large Area Telescope
• Dark matter interpretation of recent electron and positron data
• HAWC Observations Strongly Favor Pulsar Interpretations of the Cosmic-Ray Positron Excess
• $e^{\pm }$ Excesses in the Cosmic Ray Spectrum and Possible Interpretations
• The calibration and electron energy reconstruction of the BGO ECAL of the DAMPE detector
• Search for Cosmic-Ray Electron and Positron Anisotropies with Seven Years of Fermi Large Area Telescope Data
• A Parameterized Energy Correction Method for Electromagnetic Showers in BGO-ECAL of DAMPE
• Precision measurement of the (e${}^{+}$ + e${}^{-}$) flux in primary cosmic rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station

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