Heavy quark-philic scalar dark matter with a vector-like fermion portal

The absence of confirmed signal in dark matter (DM) direct detection (DD) may suggest weak interaction strengths between DM and the abundant constituents inside nucleon, i.e. gluons and valence light quarks. In this work we consider a real scalar dark matter S interacting only with SU(2)(L) singlet Up-type quarks U-i, = uR, c(R), t(R) via a vector like fermion 0 which has the same quantum number as U-i. The DM-nucleon scattering can proceed through both h-mediated Higgs portal (HP) and psi-mediated vector-like portal (VLP), in which HP can receive sizable radiative corrections through the new fermions. We first study the separate constraints on the new Yukawa couplings y(i) and find that the constraints of XENON1T results are strong on y(1) from VLP scattering and on y(3) from its radiative contributions to HP scattering. Since both DM-light quark interactions and HP have been well studied in the existing literature, we move forward to focus on DM heavy quark interactions. Since there is no valence c, t quark inside nucleons at mu(had) similar to 1 GeV, y(2), y(3) interactions are manifested in DM-gluon scattering at loop level. We find that renormalization group equation (RGE) and heavy quark threshold effects are important if one calculates the DM-nucleon scattering rate apsi at Mad 1 GeV while constructing the effective theory at mu(LEFT) similar to m(Z). For the benchmarks y(3) = 0.5, y(2) = 0.5,1, 3, combined results from Omega(DM)h(2) similar or equal to 0.12, XENON1T, Fermi-LAT, 13 TeV LHC data have almost excluded m(s) < m(t)/2 when only DM-{c, t} interactions are considered. FCNC of top quark can be generated at both tree level t -> psi(*),S -> cSS and loop level t -> c + gamma/g/Z, of which the branching fractions are typically below 10(-9) after passing the other constraints, which are still safe from the current top quark width measurements.