“…[
32,33 ] Therefore, P2 and P3 can be attributed to the first‐order phonon replicas (FX‐1LO) and second‐order phonon replicas (FX‐2LO) of the free‐exciton (FX) principal zero phonon line (ZPL), respectively, revealing the role of exciton‐phonon coupling in light emission of CsPbBr 3 microwires. In addition, another important characteristic of temperature‐dependent PL spectra is the dramatically decreasing of emission intensity with the increasing of temperature, which can be attributable to the thermally activated non‐radiative recombination process, [
34 ] Figure 2c shows the dependence of PL emission intensity on temperature, which can be fitted by the Arrhenius equation of
, where I 0 represents the PL emission intensity at 0 K, A is the proportional coefficient, E b is the exciton binding energy, and k b is the Boltzmann constant. In this case, the exciton binding energy E b is extracted as 33.15 meV through fitting, which is higher than the thermal ionization energy of room temperature (≈26 meV).…”