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Alexander Khalaidovski, Henning Vahlbruch, Hartmut Grote, Harald Lück, Benno Willke, Karsten Danzmann and Roman Schnabel STATUS OF THE GEO HF SQUEEZED LIGHT SOURCE LSC-Virgo March 2009 Meeting Pasadena, March 18th 2009 AEI Hannover LIGO-G0900232
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1 IN A NUTSHELL
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EXPERIMENTAL LAYOUT SCHEME I 2 2-COLOR LASER
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EXPERIMENTAL LAYOUT SCHEME I 3
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SECOND HARMONIC GENERATOR 4 Hemilithic cavity Nonlinear medium: Singly resonant at 1064 nm Coupling mirror: R = 90% Compact design 1 1.5 10 mm PPKTP crystal Finesse ≈ 60 High intrinsic mechanical x x stability
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SHG/SQUEEZER DESIGN 5
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EFFICIENT SHG 6
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7 inferred conversion efficiency > 90%
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EFFICIENT SHG 8 inferred conversion efficiency > 90% PRELIMINARY
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EXPERIMENTAL LAYOUT SCHEME II 9
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EXPERIMENTAL LAYOUT SCHEME III 10
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EXPERIMENTAL LAYOUT SCHEME IV 11
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EXPERIMENTAL LAYOUT SCHEME V 12
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GEO SQUEEZING BREADBOARD Breadboard: 113x135 cm Main Laser: InnoLight Mephisto > 120 opt. components Aux. Lasers: Mephisto OEM total weight ≈ 120 kg 13 Optics: ATF (superpolished) Nonlinear medium: PPKTP Beam height: 50mm Compact design
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STATUS OF THE EXPERIMENT I 14
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STATUS OF THE EXPERIMENT II 15
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STATUS OF THE EXPERIMENT II 16
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STATUS OF THE EXPERIMENT II 17
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STATUS OF THE EXPERIMENT II 18
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ELECTRONIC CONTROL Analog electronics for high Digitally interfaced Real time LINUX Operation in bandwidth control loops control system (EPICS) 24 h/day, 7 days/week self- relocking mode 19
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TIMELINE AND SUMMARY Assembling started! Squeezed light injection TIMELINE Spring/Summer 2009 into GEO 600: GOAL Squeezing-improved sensitivity for GEO 600 Test of squeezing as standard tool for future GW detectors 20
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THANK YOU
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SPARE SLIDES
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AUTO-ALIGNMENT SCHEME
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LOSS BUDGET 5%2%5% 1% 2% Total loss: 20%
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LOSS BUDGET II Goal: 6 dB detected squeezing
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SHOT NOISE (DARK FRINGE OPERATION)
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BACK-ACTION NOISE (SQL) Shot noise Radiation pressure noise [Unruh 1982] [Jaekel, Reynaud 1990] QND- Regime Squeezed Light Input (8dB)
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