Resolving Experimental Raman Spectra of TiO<sub>2</sub>:GeO<sub>2</sub> via Atomistic Modeling and Simulations
ORAL
Abstract
TiO2:GeO2 thin film is the most promising candidate high-index mirror coating material for the LIGO gravitational wave detector. To gain a more in-depth understanding of structural changes/transformations during annealing processes, we investigated both experimental and calculated Raman spectra of TiO2:GeO2. Our calculated Raman spectra exhibited a remarkable agreement with the experimental Raman spectra of TiO2:GeO2 for as-deposited thin films, spanning a wide range of Ti concentrations, from 0% to 100%. This alignment reinforces the fidelity of our computational model compared with experimental observations. Subsequently, we focused our attention on the 44% TiO2:GeO2 composition. The evolution in the experimental Raman spectra on annealing these films at various doping concentrations was carefully scrutinized, shedding light on the underlying structural transformation.
*This work is supported by the NSF through grants PHY-2011776, PHY-2011770 and PHY-2309291. Computations were performed using the utilities of the National Energy Research Scientific Computing Center (NERSC) and the University of Florida Research Computing HiPerGator.
–
Presenters
-
Rui Zhang
- University of Florida