arXiv · 0811.0477
High-energy Cosmic-Ray Positrons from Hidden-Gauge-Boson Dark Matter
Abstract
We provide a scenario in which a hidden U(1) gauge boson constitutes dark matter of the Universe and decays into the standard-model particles through a kinetic mixing with an $U(1)_{B-L}$ gauge boson. Interestingly, our model can naturally account for the steep rise in the positron fraction recently reported by PAMELA. Moreover, we find that due to the charge assignment of $U(1)_{B-L}$, only a small amount of antiprotons are produced in the decay, which is also consistent with the PAMELA and other observational data.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Chuan-Ren Chen, Fuminobu Takahashi, T. T. Yanagida. 2009-07-02. High-energy Cosmic-Ray Positrons from Hidden-Gauge-Boson Dark Matter. https://doi.org/10.1016/j.physletb.2009.02.046
Cite the original work for its findings. Save a collection to share your selection of sources.