Coy dark matter and the anomalous magnetic moment

Andi Hektor and Luca Marzola
Phys. Rev. D 90, 053007 – Published 11 September 2014

Abstract

Coy dark matter removes the tension between the traditional WIMP paradigm of dark matter and the latest exclusion bounds from direct detection experiments. In this paper we present a leptophilic coy dark matter model that, on top of explaining the spatially extended 1–5 GeV γ-ray excess detected at the galactic center, reconciles the measured anomalous magnetic moment of muon with the corresponding standard model prediction. The annihilation channel of dark matter is χχττ¯ with the dark matter mass mχ=9.43(0.52+.063stat)(±1.2sys)GeV given by best-fit of the γ-ray excess. Fitting the measured anomalous magnetic moment of the muon requires instead a pseudoscalar mediator with a minimal mass ma=123+7GeV.

  • Figure
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  • Received 23 May 2014

DOI:https://doi.org/10.1103/PhysRevD.90.053007

© 2014 American Physical Society

Authors & Affiliations

Andi Hektor

  • National Institute of Chemical Physics and Biophysics, Akadeemia tee 23, 12618 Tallinn, Estonia

Luca Marzola

  • Laboratory of Theoretical Physics, Institute of Physics, University of Tartu; Tähe 4, 51010 Tartu, Estonia

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Issue

Vol. 90, Iss. 5 — 1 September 2014

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