Year: 2009
Type: article
Abstract: We explain the PAMELA positron excess and the PPB-BETS/ATIC e + + e − data using a simple two component dark sector model (2CDS). The two particle species in the dark matter sector are assumed to be in thermal equilibrium in the early universe. While one particle is stable and is the present day dark matter, the second one is metastable and decays after the universe is 10 −8 s old. In this model it is simple to accommodate the large boost factors required to explain the PAMELA positron excess without the need for large spikes in the local dark matter density. We provide the constraints on the parameters of the model and comment on possible signals at future colliders.
Authors: Malcolm Fairbairn, Jure Zupan
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Funder: European Commission
Award: G415857248
OpenAlex ID: W1992216203
