scholarly journals High Power Lasers and Novel Optics for Laser Interferometric Gravitational Wave Detectors

1995 ◽  
Vol 48 (6) ◽  
pp. 999 ◽  
Author(s):  
PJ Veitch ◽  
J Munch ◽  
MW Hamilton ◽  
D Ottaway ◽  
A Greentree ◽  
...  

Research at Adelaide is directed towards the development of critical optical components for second generation long baseline gravitational wave interferometers. In particular, the development of high power, low noise lasers, and an investigation to determine the potential of holographic, diffractive and nonlinear optical components for solving some of the problems which could limit the sensitivity of second generation detectors. In this paper we will outline the proposed research and present some early results.

2003 ◽  
Author(s):  
Jean-Christophe Poncetta ◽  
Vincent Beau ◽  
Jerome Daurios ◽  
Gael Gaborit ◽  
Genevieve Chabassier

2011 ◽  
Vol 20 (10) ◽  
pp. 2043-2049 ◽  
Author(s):  
SHEON CHUA ◽  
MICHAEL STEFSZKY ◽  
CONOR MMOW-LOWRY ◽  
BEN C. BUCHLER ◽  
KIRK MCKENZIE ◽  
...  

Second generation ground-based gravitational wave detectors, scheduled to be operating by the middle of this decade, will be limited in sensitivity over much of their detection range by optical quantum noise. As they will be operating at power levels close to the tolerance of the optical components, significant further improvement in sensitivity will require the use of quantum optical techniques such as the injection of squeezed states. In this paper we briefly review squeezing and plans for its implementation into advanced gravitational wave detectors.


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