Slightly Non-Minimal Dark Matter in PAMELA and ATIC
Ann E. Nelson, Christopher Spitzer
TL;DR
This work introduces a nonminimal dark-matter framework in which a heavy stable particle $X$ annihilates to a light unstable mediator $Y$ that decays to Standard Model leptons, potentially explaining the PAMELA and ATIC lepton excesses without an antiproton surplus. The authors present a concrete scalar mediator model with a decoupled hidden sector, derive the relic abundance accounting for differences between hidden and visible sector temperatures via a factor $F$, and compute the galactic $e^\pm$ flux by solving a diffusion equation with a calibrated injection spectrum. They find that with $M \sim 700$–$800$ GeV and reasonable boost factors, the model can fit PAMELA/ATIC data and be compatible with Fermi within uncertainties, while predicting gamma-ray signals that distinguish scalar mediators from vector ones. The framework can be embedded in hidden-valley or unparticle theories, offering attractive indirect-detection prospects while keeping direct detection and collider signatures suppressed in the minimal realization.
Abstract
We present a simple model in which dark matter couples to the standard model through a light scalar intermediary that is itself unstable. We find this model has several notable features, and allows a natural explanation for a surplus of positrons, but no surplus of anti-protons, as has been suggested by early data from PAMELA and ATIC. Moreover, this model yields a very small nucleon coupling, well below the direct detection limits. In this paper we explore the effect of this model in both the early universe and in the galaxy.
