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Titania-doped tantala/silica coatings for gravitational-wave detection

  • Gregory M. Harry
  • , Matthew R. Abernathy
  • , Andres E. Becerra-Toledo
  • , Helena Armandula
  • , Eric Black
  • , Kate Dooley
  • , Matt Eichenfield
  • , Chinyere Nwabugwu
  • , Akira Villar
  • , D. R.M. Crooks
  • , Gianpietro Cagnoli
  • , Jim Hough
  • , Colin R. How
  • , Ian MacLaren
  • , Peter Murray
  • , Stuart Reid
  • , Sheila Rowan
  • , Peter H. Sneddon
  • , Martin M. Fejer
  • , Roger Route
  • Steven D. Penn, Patrick Ganau, Jean Marie MacKowski, Christophe Michel, Laurent Pinard, Alban Remillieux

Research output: Contribution to journalArticlepeer-review

242 Scopus citations

Abstract

Reducing thermal noise from optical coatings is crucial to reaching the required sensitivity in next generation interferometric gravitational-wave detectors. Here we show that adding TiO2 to Ta2O 5 in Ta2O5/SiO2 coatings reduces the internal friction and in addition present data confirming it reduces thermal noise. We also show that TiO2-doped Ta2O 5/SiO2 coatings are close to satisfying the optical absorption requirements of second generation gravitational-wave detectors. © 2007 IOP Publishing Ltd.
Original languageEnglish
Pages (from-to)405-415
Number of pages11
JournalClassical and Quantum Gravity
Volume24
Issue number2
DOIs
StatePublished - Jan 21 2007
Externally publishedYes

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