Cesium lead bromide
(CsPbBr3) perovskite has recently
gained significance owing to its rapidly increasing performance when
used for light-emitting devices. In this study, we used density functional
theory to determine the structural, electronic, and optical properties
of the cubic, tetragonal, and orthorhombic temperature-dependent phases
of CsPbBr3 perovskite using the full-potential linear augmented
plane wave method. The electronic properties of CsPbBr3 perovskite have been investigated by evaluating their changes upon
exerting spin-orbit coupling (SOC). The following exchange potentials
were used: the local density approximation (LDA), Perdew–Burke–Ernzerhof
generalized gradient approximation (PBE-GGA), Engel–Vosko GGA
(EV-GGA), Perdew–Burke–Ernzerhof GGA revised for solids
(PBEsol-GGA), modified Becke–Johnson GGA (mBJ-GGA), new modified
Becke–Johnson GGA (nmBJ-GGA), and unmodified Becke–Johnson
GGA (umBJ-GGA). Our band structure results indicated that the cubic,
tetragonal, and orthorhombic phases have direct energy bandgaps. By
including the SOC effect in the calculations, the bandgaps computed
with mBJ-GGA and nmBJ-GGA were found to be in good agreement with
the experimental results. Additionally, despite the large variations
in their lattice constants, the three CsPbBr3 phases possessed
similar optical properties. These results demonstrate a wide temperature
range of operation for CsPbBr3.