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- W2088397314 abstract "It is possible that TeV γ rays can originate in the photo-deexcitation of a PeV nucleus following photodisintegration via the Giant Dipole Resonance in an environment rich in Lyman alpha photons. This mechanism is examined as a candidate explanation of the recently discovered HEGRA source. The ultra-violet photon background results from the rich O and B star environment of the CygnusOB2 association. A signature of the mechanism is the existence of a lower limit ~ 500 GeV on the γ-ray spectrum. The conditions for an measurable accompanying neutrino flux from neutron decay are assessed." @default.
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- W2088397314 date "2007-03-01" @default.
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- W2088397314 title "TeV γ-rays via nuclei de-excitation: HEGRA source" @default.
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- W2088397314 doi "https://doi.org/10.1088/1742-6596/60/1/041" @default.
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