Flavor structure of the cosmic-ray electron/positron excesses at DAMPE
Abstract
The Dark Matter Particle Explorer (DAMPE) satellite detector announced its first result for measuring the cosmic-ray electron/positron (CRE) energy spectrum up to 4.6 TeV, including a tentative peak-like event excess at (1.3-1.5) TeV. In this work, we uncover a significant hidden excess in the DAMPE CRE spectrum over the energy range (0.6-1.1) TeV, which has a non-peak-like structure. We propose a new mechanism to explain this excess by a set of 1.5 TeV μ± events with subsequent decays into e± plus neutrinos. For explaining this new excess together with the peak excess around 1.4 TeV, we demonstrate that the flavor structure of the original lepton final-state produced by dark matter (DM) annihilations (or other mechanism) should have a composition ratio Ne : (Nμ + 1/6 Nτ) = 1 : y, with y ≃ 2.6- 10.8. For lepton portal DM models, this puts nontrivial constraint on the lepton-DM-mediator couplings λe : (λμ 4 + 1/6 λτ4)1/4 = 1 :y 1/4 with a narrow range y 1/4 ≃ 1.3- 1.8.
- Publication:
-
Physics Letters B
- Pub Date:
- June 2018
- DOI:
- 10.1016/j.physletb.2018.03.065
- arXiv:
- arXiv:1712.02744
- Bibcode:
- 2018PhLB..781...88G
- Keywords:
-
- High energy cosmic ray;
- Muon decay;
- Dark matter annihilation;
- Astrophysics - High Energy Astrophysical Phenomena;
- High Energy Physics - Experiment;
- High Energy Physics - Phenomenology
- E-Print:
- PLB journal version, 10 pages, 3 Figs and 1 Table. All conclusions un-changed, only fixed minor typos