Towards a Supersymmetric Description of the Fermi Galactic Center Excess
Matthew Cahill-Rowley, Jamie Gainer, JoAnne Hewett, and Tom Rizzo

TL;DR
This paper explores a supersymmetric model to explain the Fermi galactic gamma-ray excess, identifying a specific parameter space with a singlino dark matter candidate and a light CP-odd Higgs, and discusses the challenges in detecting such signals.
Contribution
It demonstrates that a supersymmetric explanation for the FGCE is feasible within the general NMSSM with specific parameters, highlighting the importance of a light CP-odd Higgs and singlino dark matter.
Findings
A particular NMSSM parameter space fits the FGCE data.
Detection of the light CP-odd Higgs at the LHC is challenging.
Indirect detection remains the most promising method for probing this scenario.
Abstract
We attempt to build a model that describes the {\it Fermi} galactic gamma-ray excess (FGCE) within a UV-complete Supersymmetric framework; we find this to be highly non-trivial. At the very least a successful Supersymmetric explanation must have several important ingredients in order to fit the data and satisfy other theoretical and experimental constraints. Under the assumption that a {\it single} annihilation mediator is responsible for both the observed relic density as well as the FGCE, we show that the requirements are not easily satisfied in many TeV-scale SUSY models, but can be met with some model building effort in the general NMSSM with parameters beyond the MSSM. We find that the data selects a particular region of the parameter space with a mostly singlino lightest Supersymmetric particle and a relatively light CP-odd Higgs boson that acts as the mediator for dark…
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