  We present the results of SiO (2-1) and SO2 (12-13) line observations of Sgr
B2(N) made with the Atacama Large Millimeter/submillimeter Array (ALMA) at an
angular resolution of ~2arcsec. Our analysis of the SiO and SO2 line emission
reveals a bipolar molecular outflow in an east-west direction whose driving
source is located at K2. In addition, SO2 line core shows a north-south
velocity gradient most probably indicating a hot core of molecular gas rotating
around K2. Fractional abundances of SO2 and SiO (X(SO2) and X(SiO),
respectively) in the outflowing molecular gas are derived from comparisons with
the C18O emission. Assuming an excitation temperature of 100+-50 K, we
calculate X(SO2) = 2.3X10^-8 and X(SiO) = 1.2X10^-9. The outflow from SgrB2(N)
K2 is characterized as a young (5X10^3yr) and massive (~2000Msun), but
moderately collimated (~60deg) outflow. We also report a possible detection of
the SiO (v=2, J=2-1) maser emission from the position of K2. If confirmed, it
would make Sgr B2(N) the 4th star forming region associated with SiO masers.
