We present the first results of AKARI Infrared Camera near-infrared spectroscopic survey of the Large Magellanic Cloud ( LMC ) .
We detected absorption features of the H _ { 2 } O ice 3.05 \mu m and the CO _ { 2 } ice 4.27 \mu m stretching mode toward seven massive young stellar objects ( YSOs ) .
These samples are for the first time spectroscopically confirmed to be YSOs .
We used a curve-of-growth method to evaluate the column densities of the ices and derived the CO _ { 2 } /H _ { 2 } O ratio to be 0.45 \pm 0.17 .
This is clearly higher than that seen in Galactic massive YSOs ( 0.17 \pm 0.03 ) .
We suggest that the strong ultraviolet radiation field and/or the high dust temperature in the LMC may be responsible for the observed high CO _ { 2 } ice abundance .