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Title: Measurement of Separate Cosmic-Ray Electron and Positron Spectra with the Fermi Large Area Telescope

Journal Article · · Physical Review Letters
 [1]
  1. Deutsches Elektronen-Synchrotron (DESY), Hamburg (Germany); et al.

We measured separate cosmic-ray electron and positron spectra with the Fermi Large Area Telescope. Because the instrument does not have an onboard magnet, we distinguish the two species by exploiting the Earth’s shadow, which is offset in opposite directions for opposite charges due to the Earth’s magnetic field. We estimate and subtract the cosmic-ray proton background using two different methods that produce consistent results. We report the electron-only spectrum, the positron-only spectrum, and the positron fraction between 20 GeV and 200 GeV. We confirm that the fraction rises with energy in the 20–100 GeV range. The three new spectral points between 100 and 200 GeV are consistent with a fraction that is continuing to rise with energy.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Contributing Organization:
Fermi LAT Collaboration
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1356772
Alternate ID(s):
OSTI ID: 1098536
Journal Information:
Physical Review Letters, Vol. 108, Issue 1; ISSN 0031-9007
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 436 works
Citation information provided by
Web of Science

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Planck 2015 results : XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation journal September 2016
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Planck 2015 results : X. Diffuse component separation: Foreground maps journal September 2016
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Planck 2015 results : XVI. Isotropy and statistics of the CMB journal September 2016
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  • IX MEXICAN SCHOOL ON GRAVITATION AND MATHEMATICAL PHYSICS: COSMOLOGY FOR THE XXIST CENTURY: Gravitation and Mathematical Physics Division of the Mexican Physical Society (DGFM-SMF), AIP Conference Proceedings https://doi.org/10.1063/1.4817029
conference January 2013
Towards Understanding the Origin of Cosmic-Ray Positrons conference July 2019
Towards Understanding the Origin of Cosmic-Ray Electrons text January 2019
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IceCube Search for Dark Matter Annihilation in nearby Galaxies and Galaxy Clusters text January 2013
Dark Matter from Hidden Forces text January 2013
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Current Dark Matter Annihilation Constraints from CMB and Low-Redshift Data text January 2013
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Testing the dark matter scenario in the inert doublet model by future precision measurements of the Higgs boson couplings text January 2016
Late decaying 2-component dark matter scenario as an explanation of the AMS-02 positron excess text January 2016
Constraints on the Primordial Black Hole Abundance from the First Advanced LIGO Observation Run Using the Stochastic Gravitational-Wave Background text January 2016
HAWC Observations Strongly Favor Pulsar Interpretations of the Cosmic-Ray Positron Excess text January 2017
WIMP dark matter candidates and searches - current status and future prospects text January 2017
HelMod in the works: from direct observations to the local interstellar spectrum of cosmic-ray electrons text January 2018
Dark Matter in Anomaly-Free Gauge Extensions text January 2018
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Towards Understanding the Origin of Cosmic-Ray Positrons text January 2019

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