The Origin of Cosmic Ray Electrons and Positrons
- 1 September 2004
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 612 (1) , 262-267
- https://doi.org/10.1086/422514
Abstract
The direct measurements of electrons and positrons over the last 30 years, corrected for the solar effect in the force-field approximation, are considered. The resulting overall electron spectrum may be fitted with a single power law above few GeV with spectral index ($gamma_{-} = 3.41 pm 0.02$), consistent with the spectral index of the positron spectrum ($gamma_{+} = 3.40 pm 0.06$), therefore suggesting a common acceleration process for both species. We propose that the engine was a shock wave originating from the last supernova explosion among those that formed the local bubble. In addition, at low energy, the electron spectrum measured during the last $A+$ solar phase is damped, whereas the positron spectrum is well represented by a single power law down to the lowest inferred local interstellar energy (0.8 GeV). We suggest that this difference arises from a time- and charge-dependent effect of the solar modulation that is not taken into account by the force-field approximation.Comment: 10 pages, 9 figures, 1 table. OBSOLETE: please refer to ApJ 612 (2004) 262-267, that is the final version of this wor
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This publication has 47 references indexed in Scilit:
- The Alpha Magnetic Spectrometer (AMS) on the International Space Station: Part I – results from the test flight on the space shuttlePhysics Reports, 2002
- Evidence for Nearby Supernova ExplosionsPhysical Review Letters, 2002
- Measurements of Cosmic-Ray Low-Energy Antiproton and Proton Spectra in a Transient Period of Solar Field ReversalPhysical Review Letters, 2002
- Cosmic protonsPhysics Letters B, 2000
- Leptons in near earth orbitPhysics Letters B, 2000
- The Cosmic‐Ray Electron and Positron Spectra Measured at 1 AU during Solar Minimum ActivityThe Astrophysical Journal, 2000
- Antiprotons at Solar MaximumPhysical Review Letters, 1999
- Balloon measurements of cosmic ray muon spectra in the atmosphere along with those of primary protons and helium nuclei over midlatitudePhysical Review D, 1999
- The Cosmic‐Ray Proton and Helium Spectra between 0.4 and 200 GVThe Astrophysical Journal, 1999
- Electrons and positrons in the galactic cosmic raysPhysical Review D, 1995