Charge Asymmetric Cosmic Ray Signals From Dark Matter Decay

TL;DR

This paper proposes that dark matter decay could produce a charge asymmetry in cosmic rays, offering a distinct signature that can be tested by current and future experiments like AMS-02, Fermi, and IceCube.

Contribution

It introduces the concept of charge asymmetry in cosmic rays from dark matter decay as a novel signature, distinct from astrophysical explanations.

Findings

Charge asymmetry can arise from relic asymmetry in dark matter.

Models predict observable gamma-ray and neutrino signals.

AMS-02 can effectively test charge asymmetry in cosmic rays.

Abstract

The PAMELA and Fermi measurements of the cosmic-ray electron and positron spectra have generated much interest over the past two years, because they are consistent with a significant component of the electron and positron fluxes between 20 GeV and 1 TeV being produced through dark matter annihilation or decay. However, since the measurements are also consistent with astrophysical interpretations, the message is unclear. In this paper, we point out that dark matter can have a more distinct signal in cosmic rays, that of a charge asymmetry. Such charge asymmetry can result if the dark matter's abundance is due to a relic asymmetry, allowing its decay to generate an asymmetry in positrons and electrons. This is analogous to the baryon asymmetry, where decaying neutrons produce electrons and not positrons. We explore benchmark scenarios where the dark matter decays into a leptophilic charged Higgs boson or electroweak gauge bosons. These models have observable signals in gamma rays and neutrinos, which can be tested by Fermi and IceCube. The most powerful test will be at AMS-02, given its ability to distinguish electron and positron charge above 100 GeV. Specifically, an asymmetry favoring positrons typically predicts a larger positron ratio and a harder (softer) high energy spectrum for positrons (electrons) than charge symmetric sources. We end with a brief discussion on how such scenarios differ from the leading astrophysical explanations.