Strength of hydroxide catalysis bonds between sapphire, silicon, and fused silica as a function of time

Margot Phelps, Mariela Masso Reid, Rebecca Douglas, Anna-Maria van Veggel, Valentina Mangano, Karen Haughian, Arjen Jongschaap, Meghan Kelly, James Hough, and Sheila Rowan
Phys. Rev. D 98, 122003 – Published 10 December 2018

Abstract

Hydroxide catalysis bonds have formed an integral part of ground-based gravitational wave (GW) observatories since the 1990s. By allowing the creation of quasimonolithic fused silica mirror suspensions in detectors such as GEO600 and Advanced LIGO, their use was crucial to the first ever direct detection of gravitational waves. Following these successes, this bonding technique has been included in advanced next generation cryogenic detector designs. Currently, they are used to create quasimonolithic crystalline sapphire suspensions in the KAGRA detector. They are also planned for use in silicon suspensions of future detectors such as the Einstein Telescope. In this paper we report how the strength of hydroxide catalysis bonds evolves over time, and compare the curing rates of bonds as they form between fused silica substrates to those between sapphire to sapphire and silicon to silicon substrates. For bonds between all three types of substrate material we show that newly formed bonds exhibit slightly higher breaking stresses than bonds cured for longer periods of time. We find that the strength stabilizes at 15MPa for bonds cured for up to 30 weeks (7 months). This finding is important to future cryogenic GW detector design as it is crucial to ensure the long term integrity of the suspension interfaces. Monitoring the strength of bonds that have been allowed to cure for shorter lengths of time can also shed light on the chemistry of bond formation.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Received 5 October 2018

DOI:https://doi.org/10.1103/PhysRevD.98.122003

© 2018 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Margot Phelps1, Mariela Masso Reid2, Rebecca Douglas2, Anna-Maria van Veggel2, Valentina Mangano2, Karen Haughian2, Arjen Jongschaap3, Meghan Kelly2, James Hough2, and Sheila Rowan2

  • 1Max Planck Institute for Gravitational Physics, Leibniz University, 30167 Hannover, Germany
  • 2SUPA, School of Physics and Astronomy, The University of Glasgow, Glasgow, G128QQ, United Kingdom
  • 3TU Delft Aerospace Faculty, Kluyverweg 1, 2629 HS Delft, Netherlands

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 98, Iss. 12 — 15 December 2018

Reuse & Permissions
Access Options
CHORUS

Article Available via CHORUS

Download Accepted Manuscript
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×