English

$Z^\prime_{BL}$ portal dark matter and LHC Run-2 results

High Energy Physics - Phenomenology 2017-02-07 v4 Cosmology and Nongalactic Astrophysics High Energy Physics - Experiment

Abstract

We consider a concise dark matter scenario in the minimal gauged BLB-L extension of the Standard Model (SM), where the global BLB-L (baryon number minus lepton number) symmetry in the SM is gauged, and three generations of right-handed neutrinos and a BLB-L Higgs field are introduced. Associated with the BLB-L gauge symmetry breaking by a VEV of the BLB-L Higgs field, the seesaw mechanism for generating the neutrino mass is automatically implemented after the electroweak symmetry breaking in the SM. In this model context, we introduce a Z2Z_2-parity and assign an odd parity for one right-handed neutrino while even parities for the other fields. Therefore, the dark matter candidate is identified as the right-handed Majorana neutrino with odd Z2Z_2 parity, keeping the minimality of the particle content intact. When the dark matter particle communicates with the SM particles mainly through the BLB-L gauge boson (ZBLZ^\prime_{BL} boson), its relic abundance is determined by only three free parameters, the BLB-L gauge coupling (αBL\alpha_{BL}), the ZBLZ^\prime_{BL} boson mass (mZm_{Z^\prime}) and the dark matter mass (mDMm_{DM}). With the cosmological upper bound on the dark matter relic abundance we find a lower bound on αBL\alpha_{BL} as a function of mZm_{Z^\prime}. On the other hand, we interpret the recent LHC Run-2 results on search for ZZ^\prime boson resonance to an upper bound on αBL\alpha_{BL} as a function of mZm_{Z^\prime}. Combining the two results we identify an allowed parameter region for this "ZBLZ^\prime_{BL} portal" dark matter scenario, which turns out to be a narrow window with the lower mass bound of mZ>2.5m_{Z^\prime} > 2.5 TeV.

Keywords

Cite

@article{arxiv.1601.07526,
  title  = {$Z^\prime_{BL}$ portal dark matter and LHC Run-2 results},
  author = {Nobuchika Okada and Satomi Okada},
  journal= {arXiv preprint arXiv:1601.07526},
  year   = {2017}
}

Comments

17 pages, 5 figures, typographical errors corrected