Photoluminescence spectra of cubic GaN grown on a GaAs substrate by mo
lecular beam epitaxy have been studied as a function of hydrostatic pr
essure at 10 K. The spectra are abundant in emission structures arisin
g from a variety of radiative recombination processes, such as free-el
ectron-bound-hole and donor-acceptor pair transitions. These emission
peaks shift to higher energy with increasing pressure, providing a mea
sure of the pressure coefficient of the band gap of cubic GaN. In addi
tion, a spectral feature, which is superimposed on the other emission
peaks and not observable at atmospheric pressure, becomes gradually re
solvable as pressure increases. The difference of pressure dependence
of this emission from the others suggests that it is associated with a
deep center.