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Measurement of the Cosmic Raye++e−Spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope

Measurement of the Cosmic Raye++e−Spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope
Designed as a high-sensitivity gamma-ray observatory, the Fermi Large Area Telescope is also an electron detector with a large acceptance exceeding 2m^2 sr at 300 GeV. Building on the gamma-ray analysis, we have developed an efficient electron detection strategy which provides sufficient background rejection for measurement of the steeply-falling electron spectrum up to 1 TeV. Our high precision data show that the electron spectrum falls with energy as E^(-3.0) and does not exhibit prominent spectral features. Interpretations in terms of a conventional diffusive model as well as a potential local extra component are briefly discussed.
6 pages, 3 figures - submitted to Physical Review Letters on March 19, published online on May 4 - contact authors: L. Latronico, A. Moiseev
- Spanish National Research Council Spain
- University of Maryland, Baltimore United States
- Tokyo Institute of Technology Japan
- INFN Sezione di Roma III Italy
- INFN Sezione di Genova Italy
[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], and other elementary particles; cosmic rays, 95.85.Ry, FOS: Physical sciences, Electrons, [PHYS.ASTR.HE] Physics/Astrophysics/High Energy Astrophysical Phenomena, Astrophysics, High Energy Physics - Experiment, 98.70.Sa, [SDU.ASTR.HE] Sciences of the Universe/Astrophysics/High Energy Astrophysical Phenomena, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), muon, Hepph, Neutrino, Dark matter, Electron Detection, Cosmic rays, Accuracy, 96.50.sb, High Energy Astrophysical Phenomena (astro-ph.HE), Cosmology And Astronomy, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], pion, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Hepex, 96.50.sb; 95.35.+d; 95.85.Ry; 98.70.Sa, energy spectra and interactions, Telescopes Astrophysics, Experiment-Hep, 520, High Energy Physics - Phenomenology, Phenomenology-Hep,Astro, 95.35.+d, [ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics - High Energy Astrophysical Phenomena, 79 Astrophysics, Composition
[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], and other elementary particles; cosmic rays, 95.85.Ry, FOS: Physical sciences, Electrons, [PHYS.ASTR.HE] Physics/Astrophysics/High Energy Astrophysical Phenomena, Astrophysics, High Energy Physics - Experiment, 98.70.Sa, [SDU.ASTR.HE] Sciences of the Universe/Astrophysics/High Energy Astrophysical Phenomena, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), muon, Hepph, Neutrino, Dark matter, Electron Detection, Cosmic rays, Accuracy, 96.50.sb, High Energy Astrophysical Phenomena (astro-ph.HE), Cosmology And Astronomy, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], pion, [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Hepex, 96.50.sb; 95.35.+d; 95.85.Ry; 98.70.Sa, energy spectra and interactions, Telescopes Astrophysics, Experiment-Hep, 520, High Energy Physics - Phenomenology, Phenomenology-Hep,Astro, 95.35.+d, [ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics - High Energy Astrophysical Phenomena, 79 Astrophysics, Composition
5 Research products, page 1 of 1
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