Abstract

We present a study of singlet-doublet vector-like leptonic dark matter (DM) in the framework of two Higgs doublet model (2HDM), where the dark sector is comprised of one doublet and one singlet vectorlike fermions (VLFs). The DM, that arises as an admixture of the neutral components of the VLFs, is stabilized by an imposed discrete symmetry $\mathcal{Z}_2^{'}$ . We test the viability of the model in the light of observations from PLANCK and recent limits on spin-independent direct detection experiments, and search for its possible collider signals. In addition, we also look for the stochastic gravitational wave (GW) signatures resulting from strong first order phase transition due to the presence of the second Higgs doublet. The model thus offers a viable parameter space for a stable DM candidate that can be probed from direct search, collider and GW experiments.

Highlights

  • Despite strong evidence of the existence of dark matter (DM) from several astrophysical and cosmological observations like rotation curves of spiral galaxies [1,2], the bullet cluster [3], gravitational lensing [4], etc., the particle nature of DM is unknown to date

  • We present a study of singlet-doublet vectorlike leptonic dark matter (DM) in the framework of the twoHiggs-doublet model (2HDM), where the dark sector is comprised of one doublet and one singlet vectorlike fermion (VLF)

  • We have proposed a singlet-doublet fermionic DM model, where the lightest fermion, emerging as a singletdoublet admixture of VLFs, can be a viable DM candidate (ψ1)

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Summary

INTRODUCTION

Despite strong evidence of the existence of dark matter (DM) from several astrophysical and cosmological observations like rotation curves of spiral galaxies [1,2], the bullet cluster [3], gravitational lensing [4], etc., the particle nature of DM is unknown to date. As we shall see, due to the presence of the second Higgs doublet, the bound from a direct search is less stringent. This is possible due to some destructive interference between the scalar-mediated direct search diagrams. Even in the absence of such destructive interference, a small direct search cross section is still conceivable due to the suppression coming from the heavy Higgs mass and small scalar mixing. This provides some freedom of choosing a moderate sin θ.

Fields and interactions
Mixing in the scalar sector
Mixing in the VLF sector
CONSTRAINTS ON THE MODEL PARAMETERS
Vacuum stability
Perturbativity
Constraints from phase transition
Collider bounds
Invisible decay constraints
DARK MATTER PHENOMENOLOGY
Relic abundance of the dark matter
Direct detection of the dark matter
COLLIDER PHENOMENOLOGY
Object reconstruction and simulation details
Event rates and signal significance
STRONG FIRST-ORDER ELECTROWEAK PHASE TRANSITION AND GRAVITATIONAL
Finite temperature effective potential
Gravitational wave from SFOPT
CONCLUSIONS
Findings
Invisible Higgs and Z decay
Full Text
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