  We present the analysis of the absorption troughs of six outflows observed in
quasar SDSS J1130+0411 ($z \approx 3.98$) with radial velocities ranging from
$-2400$ to $-15,400$ km s$^{-1}$. These spectra were taken with the Very Large
Telescope/Ultraviolet and Visual Echelle Spectrograph over the rest frame
wavelength range of $1135-1890$ \r{A}. In the main outflow system ($v \approx
-3200$ km s$^{-1}$), we identify Fe II and several Fe II* absorption troughs as
well as Si II and Si II* troughs, which we use to determine the electron number
density $\log n_e = 2.6_{-0.7}^{+0.8}$ cm$^{-3}$. Using the column densities of
these and other ions, we determine a photoionization solution with hydrogen
column density $\log N_H = 21.44_{-0.33}^{+0.24}$ cm$^{-2}$ and ionization
parameter $\log U_H = -1.75_{-0.45}^{+0.28}$. From these values we derive the
distance $R = 16_{-11}^{+23}$ kpc, the average mass flow rate $\dot{M} =
4100_{-2400}^{+6600}$ $M_{\odot}$ yr$^{-1}$, and the kinetic luminosity $\log
\dot{E}_k = 46.13_{-0.37}^{+0.41}$ erg s$^{-1}$. This $\dot{E}_k$ is
$1.4_{-0.8}^{+2.2}$% of the quasar's Eddington luminosity, and therefore
contributes significantly to AGN feedback.
