6–8 May 2013
University of Pittsburgh
US/Eastern timezone

Cosmic-Ray and Gamma-Ray Line Constraints on Decaying Dark Matter

7 May 2013, 16:30
15m
Benedum Hall G31 (University of Pittsburgh)

Benedum Hall G31

University of Pittsburgh

Pittsburgh, PA 15260

Speaker

David Tran (University of Minnesota)

Description

We discuss aspects of indirect detection of decaying dark matter and present updated fits to the parameter space in light of the recent AMS-02 measurements of the positron fraction. Leptonic dark matter decay modes can induce higher-order decays involving monoenergetic photons, which may be observed as gamma-ray lines. We examine the resulting interplay between cosmic-ray and gamma-ray constraints and compare observational sensitivities. We also discuss constraints on hadronic decay modes based on earlier measurements of the antiproton/proton ratio by PAMELA.

Author

David Tran (University of Minnesota)

Co-authors

Alejandro Ibarra (Technical University of Munich) Christoph Weniger (GRAPPA Institute) Mathias Garny (DESY)

Presentation materials