 ![Constraints on the nightmare scenario from WMAP, Xenon000 first data, and CDMS II experiments. Higgs mass is fixed to be 000 GeV in left three figures, while 000 GeV in right three figures. Expected sensitivities to detect the signal of the dark matter at XMASS, SuperCDMS, Xenon000, and LHC experiments are also shown in these figures. See the text for the detail of the region painted by dark syan (light gray).[]{data-label="fig:results"}](S000fD.eps "fig:") ![Constraints on the nightmare scenario from WMAP, Xenon000 first data, and CDMS II experiments. Higgs mass is fixed to be 000 GeV in left three figures, while 000 GeV in right three figures. Expected sensitivities to detect the signal of the dark matter at XMASS, SuperCDMS, Xenon000, and LHC experiments are also shown in these figures. See the text for the detail of the region painted by dark syan (light gray).[]{data-label="fig:results"}](S000fD.eps "fig:")\ ![Constraints on the nightmare scenario from WMAP, Xenon000 first data, and CDMS II experiments. Higgs mass is fixed to be 000 GeV in left three figures, while 000 GeV in right three figures. Expected sensitivities to detect the signal of the dark matter at XMASS, SuperCDMS, Xenon000, and LHC experiments are also shown in these figures. See the text for the detail of the region painted by dark syan (light gray).[]{data-label="fig:results"}](F000fD.eps "fig:") ![Constraints on the nightmare scenario from WMAP, Xenon000 first data, and CDMS II experiments. Higgs mass is fixed to be 000 GeV in left three figures, while 000 GeV in right three figures. Expected sensitivities to detect the signal of the dark matter at XMASS, SuperCDMS, Xenon000, and LHC experiments are also shown in these figures. See the text for the detail of the region painted by dark syan (light gray).[]{data-label="fig:results"}](F000fD.eps "fig:")\ ![Constraints on the nightmare scenario from WMAP, Xenon000 first data, and CDMS II experiments. Higgs mass is fixed to be 000 GeV in left three figures, while 000 GeV in right three figures. Expected sensitivities to detect the signal of the dark matter at XMASS, SuperCDMS, Xenon000, and LHC experiments are also shown in these figures. See the text for the detail of the region painted by dark syan (light gray).[]{data-label="fig:results"}](V000fD.eps "fig:") ![Constraints on the nightmare scenario from WMAP, Xenon000 first data, and CDMS II experiments. Higgs mass is fixed to be 000 GeV in left three figures, while 000 GeV in right three figures. Expected sensitivities to detect the signal of the dark matter at XMASS, SuperCDMS, Xenon000, and LHC experiments are also shown in these figures. See the text for the detail of the region painted by dark syan (light gray).[]{data-label="fig:results"}](V000fD.eps "fig:") 