Abstract

Although many astrophysical and cosmological observations point towards the existence of Dark Matter (DM), the nature of the DM particle has not been clarified to date. In this paper, we investigate a minimal model with a vector DM (VDM) candidate. Within this model, we compute the cross section for the scattering of the VDM particle with a nucleon. We provide the next-to-leading order (NLO) cross section for the direct detection of the DM particle. Subsequently, we study the phenomenological implications of the NLO corrections, in particular with respect to the sensitivity of the direct detection DM experi- ments. We further investigate more theoretical questions such as the gauge dependence of the results and the remaining theoretical uncertainties due to the applied approximations.

Highlights

  • Refer in most cases to particles belonging to some extension of the Standard Model (SM), and all experimental data from the different sources favour a weakly interacting massive particle (WIMP) with a velocity of the order of 200 km/s

  • In the following we present the leading order (LO) and next-to-leading order (NLO) results for the spin-independent direct detection cross section of the vector DM (VDM) model

  • We investigate the size of the NLO corrections and their phenomenological impact

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Summary

The vector dark matter model

The VDM model discussed in this work is an extension of the SM, where a complex SMgauge singlet S is added to the SM field content [14,15,16,17,18,19,20,21]. The dark gauge boson χμ and the scalar field S transform under the Z2 symmetry as follows χμ → −χμ and S → S∗ ,. The neutral component of the Higgs doublet H and the real part of the singlet field each acquire a vacuum expectation value (VEV) v and vS, respectively. The expansions around their VEVs can be written as. The CP-odd field components σH and σS do not acquire VEVs and are identified with the neutral SM-like Goldstone boson G0 and the Goldstone boson Gχ for the gauge boson χμ, respectively, while G± are the Goldstone bosons of the W bosons. The requirement of the potential to be bounded from below is translated into the following conditions λH > 0, λS > 0, κ > −2 λH λS

Renormalisation of the VDM model
Renormalisation of the dark gauge coupling gχ
Renormalisation of the scalar mixing angle α
Dark matter direct detection at tree level
Dark matter direct detection at one-loop order
Vertex corrections χχhi
Mediator corrections
Box corrections
The SI one-loop cross section
Numerical analysis
Results
The SI direct detection cross section at leading order
Gauge dependence
Renormalisation scheme dependence
Phenomenological impact of the NLO corrections on the xenon limit
Conclusions
A Nuclear form factors
B Feynman rules
Full Text
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