KeV scale new fermion from a hidden sector

preprint2020arXivOpen access

Abstract

We studied a simple model of hidden sector consists of a Dirac fermion χχ and a spontaneously broken U(1)sU(1)_s symmetry. The dark sector is connected to the Standard Model(SM) via three righthanded SM singlet neutrinos, NRN_R's, and the kinetic mixing between U(1)sU(1)_s and U(1)YU(1)_Y. A mixing between the scalar ϕϕ that breaks U(1)sU(1)_s and the SM Higgs boson, HH, is implemented via the term ϕ†ϕH†Hϕ^\dagger ϕH^\dagger H and this provides a third connection to the SM. Integrating out the NRN_R at a high scale not only gives the active neutrinos, νν, masses but generates effective Dirac type of couplings between νν and χχ. This changes the usual Type-I seesaw results for active neutrino masses and makes χχ behave like a sterile neutrino even though its origin is in the hidden sector. χχ is also split into a pair of Majorana fermions. The amount of splitting depends on the parameters. If the lighter of the pair has a mass around keV, its lifetime is longer than the age of the universe and it can be a warm dark matter candidate. Signatures of χχ in high precision Kurie plots of nuclei ββ decays and low energy neutrino nuclei coherent scatterings are discussed. The model also induces new invisible ZZ decay modes that can be searched for in future Z factories.

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