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Missing energy signatures of inelastic magnetic dipole DM at NA64e

Sergei N. Gninenko1,2,3, N. V. Krasnikov1,2, I. V. Voronchikhin1,4, and D. V. Kirpichnikov1,*

  • *Contact author: dmbrick@gmail.com

Phys. Rev. D 113, 115055 – Published 22 June, 2026

DOI: https://doi.org/10.1103/w86p-8mj9

Abstract

Some extensions of the Standard Model consider inelastic dark matter (iDM) as an attractive candidate for sub-GeV DM of thermal origin that could be detected at modern accelerators. In the present paper, we calculate the production rate of iDM pairs χ1χ¯0 interacting with the ordinary photon via dipole magnetic moment in the reaction of high-energy electron scattering on nuclei, e−N→e−Nχ1χ¯0, in the NA64e experiment at the CERN Super Proton Synchrotron (SPS). We derive the projected sensitivity of NA64e to such particles assuming ≃1013 100 GeV electrons on target. We also show, that incorporating heavy vector meson decays, γ*N→NV(→χ1χ¯0), alongside bremsstrahlunglike emission of inelastic dark matter pairs, e−N→e−Nγ*(→χ1χ¯0), will allow NA64e to probe previously unexplored regions of the iDM parameter space, in particular for modest mass splittings, Δ≃5×10−2, and relatively light masses, mχ0≲100  MeV.

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