We report on low temperature measurements of the pressure dependence o
f the photoluminescence (PL) associated with Co2+ in ZnSe performed in
a diamond anvil cell. Two sharp emission peaks at similar to 2.36 eV,
labeled L and L', show a weak redshift under pressure with rapidly de
creasing peak intensities. These results, together with the excitation
energy and temperature dependence of the PL at 1 bar, allow for a cri
tical examination of previous models proposed for these optical transi
tions. The PL data are discussed within the framework of conventional
crystal-field theory based on the Racah and crystal-field parameters B
, C, and Delta(=10Dq). From this analysis, the normalized energy E/B i
s determined as a function of the normalized crystal field parameter D
q/B. Thus quantitative estimates for the enhancement in the p-d hybrid
ization with pressure (evident in the line-shape profiles of the spect
ra) are deduced. The energy separation between L and L' decreases cont
inuously for modest pressures (similar to 1 GPa), and raises questions
about the role of spin-orbit coupling in accounting for the splitting
of this emission doublet.