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Fermi LAT Search for Dark Matter in Gamma-ray Lines and the Inclusive Photon Spectrum

Dark matter particle annihilation or decay can produce monochromatic gamma-ray lines and contribute to the diffuse gamma-ray background. Flux upper limits are presented for gamma-ray spectral lines from 7 to 200 GeV and for the diffuse gamma-ray background from 4.8 GeV to 264 GeV obtained from two y... Full description

Journal Title: arXiv.org May 12, 2012
Main Author: Ackermann, M
Other Authors: Ajello, M , Albert, A , Baldini, L , Barbiellini, G , Bechtol, K , Bellazzini, R , Berenji, B , Blandford, R , Bloom, E , Bonamente, E , Borgland, A , Brigida, M , Buehler, R , Buson, S , Caliandro, G , Cameron, R , Caraveo, P , Casandjian, J , Cecchi
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: DOI: 10.1103/PhysRevD.86.022002
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title: Fermi LAT Search for Dark Matter in Gamma-ray Lines and the Inclusive Photon Spectrum
format: Article
creator:
  • Ackermann, M
  • Ajello, M
  • Albert, A
  • Baldini, L
  • Barbiellini, G
  • Bechtol, K
  • Bellazzini, R
  • Berenji, B
  • Blandford, R
  • Bloom, E
  • Bonamente, E
  • Borgland, A
  • Brigida, M
  • Buehler, R
  • Buson, S
  • Caliandro, G
  • Cameron, R
  • Caraveo, P
  • Casandjian, J
  • Cecchi
subjects:
  • Dark Matter
  • Gamma Rays
  • Dark Matter
  • Background Radiation
  • Particle Decay
  • Cosmic Rays
  • Gamma Rays
  • Line Spectra
  • High Energy Astrophysical Phenomena
  • Cosmology and Nongalactic Astrophysics
ispartof: arXiv.org, May 12, 2012
description: Dark matter particle annihilation or decay can produce monochromatic gamma-ray lines and contribute to the diffuse gamma-ray background. Flux upper limits are presented for gamma-ray spectral lines from 7 to 200 GeV and for the diffuse gamma-ray background from 4.8 GeV to 264 GeV obtained from two years of Fermi Large Area Telescope data integrated over most of the sky. We give cross section upper limits and decay lifetime lower limits for dark matter models that produce gamma-ray lines or contribute to the diffuse spectrum, including models proposed as explanations of the PAMELA and Fermi cosmic-ray data.
language: eng
source:
identifier: DOI: 10.1103/PhysRevD.86.022002
fulltext: fulltext_linktorsrc
url: Link


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titleFermi LAT Search for Dark Matter in Gamma-ray Lines and the Inclusive Photon Spectrum
creatorAckermann, M ; Ajello, M ; Albert, A ; Baldini, L ; Barbiellini, G ; Bechtol, K ; Bellazzini, R ; Berenji, B ; Blandford, R ; Bloom, E ; Bonamente, E ; Borgland, A ; Brigida, M ; Buehler, R ; Buson, S ; Caliandro, G ; Cameron, R ; Caraveo, P ; Casandjian, J ; Cecchi
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ispartofarXiv.org, May 12, 2012
identifierDOI: 10.1103/PhysRevD.86.022002
subjectDark Matter ; Gamma Rays ; Dark Matter ; Background Radiation ; Particle Decay ; Cosmic Rays ; Gamma Rays ; Line Spectra ; High Energy Astrophysical Phenomena ; Cosmology and Nongalactic Astrophysics
descriptionDark matter particle annihilation or decay can produce monochromatic gamma-ray lines and contribute to the diffuse gamma-ray background. Flux upper limits are presented for gamma-ray spectral lines from 7 to 200 GeV and for the diffuse gamma-ray background from 4.8 GeV to 264 GeV obtained from two years of Fermi Large Area Telescope data integrated over most of the sky. We give cross section upper limits and decay lifetime lower limits for dark matter models that produce gamma-ray lines or contribute to the diffuse spectrum, including models proposed as explanations of the PAMELA and Fermi cosmic-ray data.
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titleFermi LAT Search for Dark Matter in Gamma-ray Lines and the Inclusive Photon Spectrum
authorAckermann, M ; Ajello, M ; Albert, A ; Baldini, L ; Barbiellini, G ; Bechtol, K ; Bellazzini, R ; Berenji, B ; Blandford, R ; Bloom, E ; Bonamente, E ; Borgland, A ; Brigida, M ; Buehler, R ; Buson, S ; Caliandro, G ; Cameron, R ; Caraveo, P ; Casandjian, J ; Cecchi
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96Snyder, A
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100...
atitleFermi LAT Search for Dark Matter in Gamma-ray Lines and the Inclusive Photon Spectrum
jtitlearXiv.org
risdate20120512
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abstractDark matter particle annihilation or decay can produce monochromatic gamma-ray lines and contribute to the diffuse gamma-ray background. Flux upper limits are presented for gamma-ray spectral lines from 7 to 200 GeV and for the diffuse gamma-ray background from 4.8 GeV to 264 GeV obtained from two years of Fermi Large Area Telescope data integrated over most of the sky. We give cross section upper limits and decay lifetime lower limits for dark matter models that produce gamma-ray lines or contribute to the diffuse spectrum, including models proposed as explanations of the PAMELA and Fermi cosmic-ray data.
copIthaca
pubCornell University Library, arXiv.org
doi10.1103/PhysRevD.86.022002
urlhttp://search.proquest.com/docview/2082766088/
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date2012-05-12