DAMPE excess from decaying right-handed neutrino dark matter
Nobuchika Okada, Osamu Seto

TL;DR
This paper proposes that a decaying right-handed neutrino dark matter within a minimal gauged $U(1)_{B-L}$ model explains the DAMPE excess at 1.4 TeV, with testable predictions for gamma rays and collider searches.
Contribution
It introduces a specific decay mechanism of right-handed neutrino dark matter in a $U(1)_{B-L}$ model to explain the DAMPE excess, linking cosmic-ray data with collider and gamma-ray tests.
Findings
A 3 TeV right-handed neutrino dark matter can fit the DAMPE peak with a lifetime of about 10^{28} seconds.
The model predicts a $Z'$ boson around 6 TeV accessible at the LHC.
The parameter space is constrained by relic density, stability, and avoidance of Landau poles.
Abstract
The flux of high-energy cosmic-ray electrons plus positrons recently measured by the DArk Matter Particle Explorer (DAMPE) exhibits a tentative peak excess at an energy of around TeV. In this paper, we consider the minimal gauged model with a right-handed neutrino (RHN) dark matter (DM) and interpret the DAMPE peak with a late-time decay of the RHN DM into . We find that a DM lifetime s can fit the DAMPE peak with a DM mass TeV. This favored lifetime is close to the current bound on it by Fermi-LAT, our decaying RHN DM can be tested once the measurement of cosmic gamma ray flux is improved. The RHN DM communicates with the Standard Model particles through the gauge boson ( boson), and its thermal relic abundance is controlled by only three free parameters: , the gauge coupling…
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