6–7 Oct 2025
Leibniz-Insitut für Kristallzüchtung (IKZ)
Europe/Berlin timezone

Evolution Optical Coating Thin Films Following Thermal Annealing: IR Spectroscopic Ellipsometry and Raman Investigation

7 Oct 2025, 13:15
15m
Max-Born-Saal

Max-Born-Saal

Speaker

Shima Samandari (OptMatLab, Dipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146 Genova, Italy)

Description

The development of future gravitational wave observatories such as the Einstein Telescope requires the development of multilayer mirror coatings with low absorption and constant refractive indices [1]. These coatings, which are usually amorphous mixed oxides, are deposited by ion beam sputtering. Thermal annealing after deposition is used to enhance the performance of the coatings. However, the specific atomic-scale structural changes that control this tuning are not well understood, especially for promising germania-based systems. This study investigates the effects of thermal annealing at 600° on amorphous oxide coatings based on germanium oxide. We used a complementary approach using infrared spectroscopic ellipsometry (IRSE) to measure the complex dielectric function (ε = ε₁ + iε₂) and Raman spectroscopy to investigate the bond angle distribution and medium-range order in the oxide coatings [2, 3]. Our analysis shows a direct correlation between the annealing-induced structural relaxation [4] and the evolution of vibrational signatures in both the IR and Raman spectra. This study shows the effects of thermal processing to optimize the atomic structure and optical performance of germanium-based coatings for use in next-generation GWDs.

Acknowledgments:
We gratefully acknowledge the Project Einstein Telescope Infrastructure Consortium (ETIC)(IR0000004)-MUR call n. 3264 PNRR, Miss. 4-Comp. 2, Line 3.1.

Keywords: Optical coatings, thermal annealing, Infrared spectroscopic ellipsometry, Raman, GWD mirrors

References:
1. Amato, Alex, Michele Magnozzi, and Janis Wöhler. "Mirror Coating Research and Developments for Current and Future Gravitational‐Wave Detectors." Adv. Photon. Res. (2025): 2400117.
2. Yin, Shenwei, et al. "Preventing overfitting in infrared ellipsometry using temperature dependence: fused silica as a case study." Opt. Mater. Expr. 15.8 (2025): 1939-1948.
3. Micoulaut, Matthieu, L. Cormier, and G. S. Henderson. "The structure of amorphous, crystalline andliquid GeO2." J. Phys.: Cond. Matt.18.45 (2006): R753.
4. Suzuki, K., M. Misawa, and Y. Kobayashi. "What difference exists in the structure of SiO2 and GeO2 between melt-quenched bulk glass and sputter-deposited amorphous film." Le Journal de Physique Colloques 46.C8 (1985): C8-617.

Author

Shima Samandari (OptMatLab, Dipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146 Genova, Italy)

Co-authors

Dr Michele Magnozzi (INFN Sezione di Genova, Via Dodecaneso 33, 16146 Genova, Italy) Dr Valerie Martinez (Institut Lumière Matière, 10 rue Ada Byron, 69622 Villeurbanne, France) Prof. maurizio canepa (OptMatLab, Dipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146 Genova, Italy)

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