Mirror Coating Research and Developments for Current and Future Gravitational-Wave Detectors

Alex Amato*, Michele Magnozzi, Janis Wohler

*Corresponding author for this work

Research output: Contribution to journalArticleAcademicpeer-review

Abstract

In current and future gravitational-wave detectors, thermal noise from mirror coatings limits the sensitivity of the detectors. To reduce the coating thermal noise, coatings with excellent optical and mechanical properties are needed. In this review, an overview of postdeposition coating treatments and the latest worldwide research activities on coatings with low mechanical loss and low optical absorption are reported. A brief overview of coating design optimization, including innovative solutions such as multimaterial coatings and nanolayers, is also discussed.
Original languageEnglish
Number of pages14
JournalAdvanced Photonics Research
DOIs
Publication statusPublished - 1 Mar 2025

Keywords

  • gravitational-wave detectors
  • internal friction
  • loss angle
  • optical absorption
  • optical coatings
  • refractive index
  • thermal noise
  • HFO2 THIN-FILMS
  • MECHANICAL LOSS
  • OPTICAL-ABSORPTION
  • AMORPHOUS-SILICON
  • ATOMIC-STRUCTURE
  • THERMAL NOISE
  • INTERNAL-FRICTION
  • CRYSTALLIZATION
  • REDUCTION
  • NITRIDE

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