“…The FWHM of the luminescent band increases with increasing temperature. Boltzmann distribution is often used to explain this phenomenon
15,45 :
where k is Boltzmann constant; S is the Huang‐Rhys parameter; hv is the electronic transitions vibrate phonon energy, and it is the same for 5d and 4f of Eu 2+ . As the temperature rises, the interaction of electrons and phonons is dominant.…”