Sign on

SAO/NASA ADS Astronomy Abstract Service


· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· References in the article
· Citations to the Article (7) (Citation History)
· Refereed Citations to the Article
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
ACIGA's high optical power test facility
Authors:
Ju, L.; Aoun, M.; Barriga, P.; Blair, D. G.; Brooks, A.; Burman, R.; Burston, R.; Chin, X. T.; Chin, E. J.; Lee, C. Y.; Coward, D.; Cusack, B.; de Vine, G.; Degallaix, J.; Dumas, J. C.; Garoi, F.; Gras, S.; Gray, M.; Hosken, D.; Howell, E.; Jacob, J. S.; Kelly, T. L.; Lee, B.; Lee, K. T.; Lun, T.; McClelland, D.; Mow-Lowry, C.; Mudge, D.; Munch, J.; Schediwy, S.; Scott, S.; Searle, A.; Sheard, B.; Slagmolen, B.; Veitch, P.; Winterflood, J.; Woolley, A.; Yan, Z.; Zhao, C.
Affiliation:
AA(School of Physics, University of Western Australia, Perth, Australia ), AB(Computer and Information Science, Edith Cowan University, Perth, Australia ), AC(School of Physics, University of Western Australia, Perth, Australia ), AD(School of Physics, University of Western Australia, Perth, Australia ), AE(Department of Physics and Mathematical Physics, Adelaide University, Adelaide, Australia ), AF(School of Physics, University of Western Australia, Perth, Australia ), AG(School of Mathematical Science, Monash University, Melbourne, Australia ), AH(School of Physics, University of Western Australia, Perth, Australia ), AI(School of Physics, University of Western Australia, Perth, Australia ), AJ(Computer and Information Science, Edith Cowan University, Perth, Australia ), AK(School of Physics, University of Western Australia, Perth, Australia ), AL(Department of Physics, Australian National University, Canberra, Australia), AM(Department of Physics, Australian National University, Canberra, Australia), AN(School of Physics, University of Western Australia, Perth, Australia ), AO(School of Physics, University of Western Australia, Perth, Australia ), AP(School of Physics, University of Western Australia, Perth, Australia ), AQ(School of Physics, University of Western Australia, Perth, Australia ), AR(Department of Physics, Australian National University, Canberra, Australia), AS(Department of Physics and Mathematical Physics, Adelaide University, Adelaide, Australia ), AT(School of Physics, University of Western Australia, Perth, Australia ), AU(School of Physics, University of Western Australia, Perth, Australia ), AV(Department of Physics and Mathematical Physics, Adelaide University, Adelaide, Australia ), AW(School of Physics, University of Western Australia, Perth, Australia ), AX(School of Physics, University of Western Australia, Perth, Australia ), AY(School of Mathematical Science, Monash University, Melbourne, Australia ), AZ(Department of Physics, Australian National University, Canberra, Australia), BA(Department of Physics, Australian National University, Canberra, Australia), BB(Department of Physics and Mathematical Physics, Adelaide University, Adelaide, Australia ), BC(Department of Physics and Mathematical Physics, Adelaide University, Adelaide, Australia ), BD(School of Physics, University of Western Australia, Perth, Australia ), BE(Department of Physics, Australian National University, Canberra, Australia), BF(Department of Physics, Australian National University, Canberra, Australia), BG(Department of Physics, Australian National University, Canberra, Australia), BH(School of Physics, University of Western Australia, Perth, Australia ), BI(Department of Physics and Mathematical Physics, Adelaide University, Adelaide, Australia ), BJ(School of Physics, University of Western Australia, Perth, Australia ), BK(School of Physics, University of Western Australia, Perth, Australia ), BL(School of Physics, University of Western Australia, Perth, Australia ), BM(Computer and Information Science, Edith Cowan University, Perth, Australia )
Publication:
Classical and Quantum Gravity, Volume 21, Issue 5, pp. S887-S893 (2004).
Publication Date:
03/2004
Origin:
IOP
DOI:
10.1088/0264-9381/21/5/077
Bibliographic Code:
2004CQGra..21S.887J

Abstract

Advanced laser interferometer detectors utilizing more than 100 W of laser power and with ~106 W circulating laser power present many technological problems. The Australian Consortium for Interferometric Gravitational Astronomy (ACIGA) is developing a high power research facility in Gingin, north of Perth, Western Australia, which will test techniques for the next generation interferometers. In particular it will test thermal lensing compensation and control strategies for optical cavities in which optical spring effects and parametric instabilities may present major difficulties.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)

   

Find Similar Abstracts:

Use: Authors
Title
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints