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• W2016501653 abstract "In light of the recent observation of the Fermi-LAT 130 GeV gamma-ray line, we suggest a model of scalar dark matter in hidden sector, which can decay into two (hidden) photons. The process is radiatively induced by a GUT scale fermion in the loop, which is charged under a hidden sector U(1), and the kinetic mixing ($sim epsilon F^{munu}F'_{munu}$) enables us to fit the required decay width for the Fermi-LAT peak. The model does not allow any dangerous decay channels into light standard model particles." @default.
• W2016501653 created "2016-06-24" @default.
• W2016501653 creator A5020503634 @default.
• W2016501653 creator A5075736412 @default.
• W2016501653 date "2013-01-01" @default.
• W2016501653 modified "2023-10-17" @default.
• W2016501653 title "Radiatively decaying scalar dark matter through U(1) mixings and the Fermi 130 GeV gamma-ray line" @default.
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• W2016501653 doi "https://doi.org/10.1016/j.physletb.2012.12.035" @default.
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