In order to reveal the origin of the ultra-fast outflows (UFOs) that are frequently observed in active galactic nuclei (AGNs), we perform two-dimensional radiation hydrodynamics simulations of the line-driven disk winds, which are accelerated by the radiation force due to the spectral lines. The line-driven winds are successfully launched for the range of $M_{\rm BH}=10^{6-9}M_\odot\varepsilon$=0.1-0.5, and the resulting mass outflow rate (), momentum flux (), and kinetic luminosity () are in the region containing 90% of the posterior probability distribution in the - plane, - plane, and - plane shown in Gofford et al., where is the black hole mass, is the Eddington ratio, and is the bolometric luminosity. The best-fitting relations in Gofford et al., $d\log\dot{M_{\rm w}}/d\log{L_{\rm bol}}\sim 0.9d\log\dot{p_{\rm w}}/d\log{L_{\rm bol}}\sim 1.2d\log\dot{E_{\rm w}}/d\log{L_{\rm bol}}\sim 1.5$, are roughly consistent with our results, , , and $d\log\dot{E_{\rm w}}/d\log{L_{\rm bol}}\sim 11/8$. In addition, our model predicts that no UFO features are detected for the AGNs with , since the winds do not appear. Also, only AGNs with exhibit the UFOs when . These predictions nicely agree with the X-ray observations (Gofford et al.). These results support that the line-driven disk wind is the origin of the UFOs.

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