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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4472

Title: PeV gamma rays from interactions of ultra high energy cosmic rays in the Milky Way
Authors: Gupta, Nayantara
Issue Date: Mar-2012
Publisher: Elsevier B.V.
Citation: Astroparticle Physics, 2012, Vol.35, p503
Abstract: The PeV gamma ray background produced in the interactions of ultra high energy cosmic rays with the ambient matter and radiations during their propagation in the Milky Way has been calculated in this paper. If the primary ultra high energy cosmic rays are produced from Galactic point sources then those point sources are also emitting PeV gamma rays. We discuss that the detection of galactocentric PeV gamma rays in the future would be a signature of the presence of EeV cosmic accelerators in the Milky Way.
Description: Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)
URI: http://hdl.handle.net/2289/4472
ISSN: 0927-6505
Alternative Location: http://adsabs.harvard.edu/abs/2012APh....35..503G
http://arxiv.org/abs/1110.5257
http://dx.doi.org/10.1016/j.astropartphys.2011.11.002
Copyright: 2012 Elsevier B.V.
Appears in Collections:Research Papers (A&A)

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