Figure 3. (a) Representative PL spectra under different excitation
energies at 15K base temperature. The PL spectra are renormalized and
shifted with respect to the spectral peak for comparison. The upper
halves of the PL lineshape (normalized PL> 0.5) are nearly
the same, and the lower parts of PL lineshape expand at the higher
excitation energy. The expansion weighs heavily at the higher energy
tails as magnified in the inset. (b) Representative PL spectra at
various cryostat temperature. The linewidth broadening owing to the
lattice temperature displays different pattern against that of exciton
temperature. The inset shows the linewidth from Lorentz fitting as a
function of the lattice temperature (c) Simulated PL spectra with the
mechanism of acoustic phonon assisted exciton emission, where the
lattice temperature is kept constant (\(T_{\text{lattice}}=15K\)) and
the exciton temperature is the sole variable. The high energy side tail
expands obviously accompanying with the linewidth broadening. The inset
shows the linewidth broadening as a function of the exciton temperature.
Simulation result of PL spectra with excitation energy of 2.31eV (d) and
2.75eV (e), the exciton temperature is estimated to be 39K and 55K
(~24K and 40K higher than the lattice temperature) under
the excitation energies of 2.31eV and 2.75eV, respectively.
Figure 3(a) shows the representative PL spectra under different
excitation energies. These PL spectra are renormalized and shifted with
respect to the PL energy peak for better comparison. Note that the top
halves of the PL spectra where the normalized intensity >
0.5 are nearly the same across the excitation energy range. Contrarily
the tail at the high energy side expands with the elevating excitation
energy as illustrated in the inset. This linewidth broadening has a
contrasting manner to the lattice temperature induced line shape
broadening (Figure 3(b)) which displays a whole line shape broadening
other than just an expansion in the tail. To simulate the
phonon-assisted PL we set the exciton temperature as the single variable
and keep lattice temperature as a constant (~15K).
Figure 3(c) shows the simulated PL spectrum of A1s exciton under
the acoustic phonon assisted photoluminescence mechanism with all
defined parameters from M. M. Glazov and B. Urbaszek’s
work28 (detailed in SI). The expansion at the higher
energy edge leads to the effective linewidth broadening (inset of
Fig.3(c)), remarkably reproducing the experimental features in Fig.2(d).
The simulation perfectly describes our experimental results and it
clearly indicates that the acoustic phonon assisted photoluminescence
process makes significant contribution to the whole PL spectrum in high
quality samples. Comparing our experimental (Figure 3(a)) with
simulation results (Fig.3(c)), we conclude that the higher excitation
energy leads to the higher exciton temperature and finally raises
non-Lorentz high energy tail. As demonstrated in the Fig.3(d) and (e),
the effective exciton temperature (\(T_{\text{exciton}}\)) is 24Khigher than the lattice temperature (\(T_{\text{lattice}}\)) when the
excitation is at 2.31eV and 40K higher at 2.75eV ,
respectively.