<p>We consider the gauged U(1)<sub><i>B</i>−<i>L</i></sub> model and examine the situation where the sterile neutrino is a dark matter candidate produced by the freeze-in mechanism. In our model, the dark matter <i>N</i> is mainly produced by the decay of a U(1)<sub><i>B</i>−<i>L</i></sub> breaking scalar boson <i>ϕ</i>. We point out that the on-shell production of <i>ϕ</i> through annihilation of the U(1)<sub><i>B</i>−<i>L</i></sub> gauge boson <i>Z</i><sup>′</sup> plays an important role. We find that the single production of <i>Z</i><sup>′</sup> from the gluon bath in the early Universe can become the main production modes for <i>Z</i><sup>′</sup> in some parameter regions. To prevent <i>N</i> from being overproduced, we show that the U(1)<sub><i>B</i>−<i>L</i></sub> gauge coupling constant <i>g</i><sub><i>B</i>−<i>L</i></sub> must be as small as 10<sup>−16</sup>–10<sup>−10</sup>. We also consider the case where the decay of <i>ϕ</i> into <i>N</i> is kinematically forbidden. In this case, <i>N</i> is generated by the scattering of <i>Z</i><sup>′</sup> and the <i>g</i><sub><i>B</i>−<i>L</i></sub> takes values of 10<sup>−10</sup>–10<sup>−6</sup>, which can be explored in collider experiments like FASER and SHiP.</p>

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Freeze-in sterile neutrino dark matter in a feebly gauged BL model

  • Osamu Seto,
  • Takashi Shimomura,
  • Yoshiki Uchida

摘要

We consider the gauged U(1)BL model and examine the situation where the sterile neutrino is a dark matter candidate produced by the freeze-in mechanism. In our model, the dark matter N is mainly produced by the decay of a U(1)BL breaking scalar boson ϕ. We point out that the on-shell production of ϕ through annihilation of the U(1)BL gauge boson Z plays an important role. We find that the single production of Z from the gluon bath in the early Universe can become the main production modes for Z in some parameter regions. To prevent N from being overproduced, we show that the U(1)BL gauge coupling constant gBL must be as small as 10−16–10−10. We also consider the case where the decay of ϕ into N is kinematically forbidden. In this case, N is generated by the scattering of Z and the gBL takes values of 10−10–10−6, which can be explored in collider experiments like FASER and SHiP.