  We explore the singlet scalar dark matter (DM) from direct detections and
high energy neutrino signals generated by the solar DM annihilation. Two
singlet scalar DM models are discussed, one is the real singlet scalar DM model
as the simple extension of the standard model (SSDM-SM) with a discrete Z_2
symmetry, and another is the complex singlet scalar DM model as the simple
extension of the left-right symmetric two Higgs bidoublet model (SSDM-2HBDM)
with $P$ and CP symmetries. To derive the Sun capture rate, we consider the
uncertainties in the hadronic matrix elements and calculate the
spin-independent DM-nucleon elastic scattering cross section. We find that the
predicted neutrino induced upgoing muon fluxes in the region 3.7 GeV < m_D <
4.2 GeV slightly exceed the Super-Kamiokande limit in the SSDM-SM. However,
this exceeded region can be excluded by the current DM direct detection
experiments. For the SSDM-2HBDM, one may adjust the Yukawa couplings to avoid
the direct detection limits and enhance the predicted muon fluxes. For the
allowed parameter space of the SSDM-SM and SSDM-2HBDM, the produced muon fluxes
in the Super-Kamiokande and muon event rates in the IceCube are less than the
experiment upper bound and atmosphere background, respectively.
