Ar transport and blister growth kinetics in titania-doped germania-based optical coatings

Emile Lalande, Aaron Davenport, Lory Marchand, Ashot Markosyan, Daniel Martinez, Annalisa Paolone, Michael Rezac, Marco Bazzan, Martin Chicoine, Julien Colaux, Matthieu Coulon, Martin M. Fejer, Alexandre W. Lussier, Ettore Majorana, Ludvik Martinu, Carmen Menoni, Christophe Michel, Fulvio Ricci, François Schiettekatte, Nikita ShcheblanovJoshua R. Smith, Julien Teillon, Guy Terwagne, Gabriele Vajente

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Abstract

Blistering is a phenomenon sometimes observed in sputtered-deposited thin films but seldom investigated in detail. Here, we consider the case of titania-doped germania (TGO)/silica multilayers deposited by ion beam sputtering. TGO is a candidate as high refractive index material in the Bragg mirrors for the next iteration of gravitational waves detectors. It needs to be annealed at 600 C for 100 h in order to reach the desired relaxation state. However under some growth conditions, in 52-layer TGO/silica stacks, blistering occurs upon annealing at a temperature near 500 C, which corresponds to the temperature where Ar desorbs from TGO. In order to better understand the blistering phenomenon, we measure the Ar transport in single layers of TGO and silica. In the case of < 1 µm-thick TGO layers, the Ar desorption is mainly limited by detrapping. The transport model also correctly predicts the evolution of the total amount of Ar in a 8.5 µm stack of TGO and silica layers annealed at 450 C, but in that case, the process is mainly limited by diffusion. Since Ar diffusion is an order of magnitude slower in TGO compared to silica, we observe a correspondingly strong accumulation of Ar in TGO. The Ar transport model is used to explain some regimes of the blisters growth, and we find indications that Ar accumulation is a driver for their growth in general, but the blisters nucleation remains a complex phenomenon influenced by several other factors including stress, substrate roughness, and impurities.

Original languageEnglish
Article number115013
JournalClassical and Quantum Gravity
Volume41
Issue number11
DOIs
Publication statusPublished - 6 Jun 2024

Funding

The work performed at UdeM and Polytechnique Montr\u00E9al was supported by the Natural Sciences and Engineering Research Council of Canada (NSERC), the Canadian foundation for innovation (CFI) and the Fonds de recherche Qu\u00E9bec, Nature et technologies (FQRNT) through the Regroupement Qu\u00E9b\u00E9cois sur les Mat\u00E9riaux de Pointe (RQMP), as well as a Projet de coop\u00E9ration Qu\u00E9bec-Wallonie-Bruxelles (Wallonie: #RECH-INNO-02, Qu\u00E9bec: #11.802). The authors thank Prof. S Roorda and F Debris from U Montr\u00E9al for fruitful discussions and technical support. Cal State Fullerton authors were supported by NSF Awards PHY-2207998 and PHY-1807069, the Dan Black Family Trust, and Nancy and Lee Begovich. The authors thank their colleagues within the LIGO Scientific Collaboration for advice and support. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation, and operates under cooperative Agreement PHY-0757058. Advanced LIGO was built under Award PHY-0823459. This paper has LIGO Document Number LIGO-P2300328.

FundersFunder number
Massachusetts Institute of Technology
Canada Foundation for Innovation
Fonds de recherche du Québec – Nature et technologies
Natural Sciences and Engineering Research Council of Canada
Dan Black Family Trust
Fonds Québécois de la Recherche sur la Nature et les Technologies
Nancy and Lee Begovich
National Science FoundationPHY-0823459, PHY-2207998, LIGO-P2300328, PHY-0757058, PHY-1807069
National Science Foundation
Regroupement Québécois sur les Matériaux de Pointe11.802, INNO-02

    Keywords

    • annealing
    • argon
    • blistering
    • bragg reflector
    • ion beam analysis
    • scatterometer
    • thermal desorption

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