English

Light $Z^\prime$ and Dirac fermion dark matter in the $B-L$ model

High Energy Physics - Phenomenology 2022-10-19 v2 High Energy Physics - Experiment

Abstract

We consider a U(1)BLU(1)_{B-L} model with a ZZ^\prime portal Dirac fermion dark matter (DM) χ\chi of low mass which couples very weakly to the BLB - L gauge boson ZZ^\prime. An arbitrary BLB-L charge Q±1,±3Q\neq \pm1, \pm 3 of the DM χ\chi ensures its stability. Motivated by the sensitivity reach of forthcoming "Lifetime Frontier" experiments, we focus on the ZZ^\prime mass, mZm_{Z^\prime}, in the sub-GeV to few GeV range. To evaluate the DM relic abundance, we examine both the freeze-out and freeze-in DM scenarios. For the freeze-out scenario, we show that the observed DM abundance is reproduced near the ZZ^\prime resonance, mχmZ/2m_\chi \simeq m_{Z^\prime}/2, where mχm_\chi is the DM mass. For the freeze-in scenario, we focus on mχmZm_\chi \ll m_{Z^\prime}. We show that for a fixed value of mZm_{Z^\prime}, gBLg_{BL} values roughly scale as 1/Q1/Q to reproduce the observed DM abundance. For various QQ values in the range between 10610^{-6} and 10210^2, we show that the gauge coupling values gBLg_{BL} needed to reproduce the observed DM abundance lie in the search reach of future planned and/or proposed experiments such as FASER, Belle-II, LDMX, and SHiP. In the freeze-in case, the QQ values to realize observable gBLg_{BL} values are found to be much smaller than that in the freeze-out case.

Keywords

Cite

@article{arxiv.2112.08960,
  title  = {Light $Z^\prime$ and Dirac fermion dark matter in the $B-L$ model},
  author = {Newton Nath and Nobuchika Okada and Satomi Okada and Digesh Raut and Qaisar Shafi},
  journal= {arXiv preprint arXiv:2112.08960},
  year   = {2022}
}

Comments

14 pages, 3 figures, revised section III with new Figure 1