Gingin High Optical Power Test Facility

Chunnong Zhao, David Blair, Pablo Barrigo, Jerome Degallaix, Jean-Charles Dumas, Yaohui Fan, Slawomir Gras, Li Ju, B.H. Lee, Sascha Schediwy, Z. Yan, D.E. Mcclelland, S.M. Scott, M.B. Gray, A.C. Searle, S. Gossler, B.J.J. Slagmolen, J. Dickson, K. Mckenzie, C. Mow-LowryA. Moylan, D. Rabeling, J. Cumpston, K. Wette, J. Munch, P.J. Veitch, D. Mudge, A. Brooks, D. Hosken

    Research output: Contribution to journalArticle

    15 Citations (Scopus)

    Abstract

    The Australian Consortium for Gravitational Wave Astronomy (ACIGA) in collaboration with LIGO is developing a high optical power research facility at the AIGO site, Gingin, Western Australia. Research at the facility will provide solutions to the problems that advanced gravitational wave detectors will encounter with extremely high optical power. The problems include thermal lensing and parametric instabilities. This article will present the status of the facility and the plan for the future experiments.
    Original languageEnglish
    Pages (from-to)368-373
    JournalJournal of Physics: Conference Series
    Volume32
    DOIs
    Publication statusPublished - 2006

    Fingerprint Dive into the research topics of 'Gingin High Optical Power Test Facility'. Together they form a unique fingerprint.

  • Cite this

    Zhao, C., Blair, D., Barrigo, P., Degallaix, J., Dumas, J-C., Fan, Y., ... Hosken, D. (2006). Gingin High Optical Power Test Facility. Journal of Physics: Conference Series, 32, 368-373. https://doi.org/10.1088/1742-6596/32/1/056