Abstract
We study a scenario in which a hidden gaugino dark matter decays into the standardmodel particles (and their supersymmetric partners) through a kinetic mixing with the gaugino of a U(1)B-L broken at a scale close to the grand unification scale. We show that the decay of the hidden gaugino can explain the excesses in cosmic-ray electrons and positrons observed by PAMELA and Fermi.
Original language | English |
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Pages (from-to) | 1277-1284 |
Number of pages | 8 |
Journal | Progress of Theoretical Physics |
Volume | 122 |
Issue number | 5 |
DOIs | |
Publication status | Published - 2009 Nov |
Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)