Jan 29, 2007 LIGO Excomm, G070006-00-R 1 Goal: Experimental Demonstration of a Squeezing-Enhanced Laser-Interferometric Gravitational Wave Detector in.

Slides:



Advertisements
Similar presentations
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut) HOMODYNE AND HETERODYNE READOUT OF A SIGNAL- RECYCLED GRAVITATIONAL WAVE DETECTOR.
Advertisements

G v1Squeezed Light Interferometry1 Squeezed Light Techniques for Gravitational Wave Detection July 6, 2012 Daniel Sigg LIGO Hanford Observatory.
Koji Arai – LIGO Laboratory / Caltech LIGO-G v2.
1 Experimental Demonstration of a Squeezing-Enhanced Laser-Interferometric Gravitational-Wave Detector Keisuke Goda Quantum Measurement Group, LIGO Massachusetts.
G v1 Squeezer Update Review August 25, 2009 H1 Squeezer Experiment ANU, AEI, MIT, CIT and LHO collaboration.
TeV Particle Astrophysics August 2006 Caltech Australian National University Universitat Hannover/AEI LIGO Scientific Collaboration MIT Corbitt, Goda,
Generation of squeezed states using radiation pressure effects David Ottaway – for Nergis Mavalvala Australia-Italy Workshop October 2005.
Jan 29, 2007 LIGO Excomm, G R 1 Status and Future of the Caltech 40m Lab Jan 29, 2007 the 40m team: Rana Adhikari, Ben Abbott, Rich Abbott, Rolf.
Ponderomotive Squeezing & Opto-mechanics Adam Libson and Thomas Corbitt GWADW 2015 G
Recent Developments toward Sub-Quantum-Noise-Limited Gravitational-wave Interferometers Nergis Mavalvala Aspen January 2005 LIGO-G R.
Quantum Noise Measurements at the ANU Sheon Chua, Michael Stefszky, Conor Mow-Lowry, Sheila Dwyer, Ben Buchler, Ping Koy Lam, Daniel Shaddock, and David.
Interferometer Topologies and Prepared States of Light – Quantum Noise and Squeezing Convenor: Roman Schnabel.
Experiments towards beating quantum limits Stefan Goßler for the experimental team of The ANU Centre of Gravitational Physics.
Test mass dynamics with optical springs proposed experiments at Gingin Chunnong Zhao (University of Western Australia) Thanks to ACIGA members Stefan Danilishin.
Generation and Control of Squeezed Light Fields R. Schnabel  S.  Chelkowski  A.  Franzen  B.  Hage  H.  Vahlbruch  N. Lastzka  M.  Mehmet.
SPECTROSCOPY LABORATORY MASSACHUSETTS INSTITUTE OF TECHNOLOGY Application of LIGO Technology to Biomedical Optics Keisuke Goda Quantum Measurement Group.
LIGO-G D Enhanced LIGO Kate Dooley University of Florida On behalf of the LIGO Scientific Collaboration SESAPS Nov. 1, 2008.
R·I·TR·I·T Rochester Institute of Technology -Proposal to join the LSC- Shally Saraf Rochester Institute of Technology Quantum Electronics Group (RITQEG)
SQL Related Experiments at the ANU Conor Mow-Lowry, G de Vine, K MacKenzie, B Sheard, Dr D Shaddock, Dr B Buchler, Dr M Gray, Dr PK Lam, Prof. David McClelland.
Squeezed light and GEO600 Simon Chelkowski LSC Meeting, Hannover.
Enhanced LIGO with squeezing: Lessons Learned for Advanced LIGO and beyond.
LIGO- G R Amaldi7 July 14 th, 2007 R. Ward, Caltech 1 DC Readout Experiment at the Caltech 40m Laboratory Robert Ward Caltech Amaldi 7 July 14.
Eighth Edoardo Amaldi Conference on Gravitational Waves Sheon Chua, Michael Stefszky, Conor Mow-Lowry, Daniel Shaddock, Ben Buchler, Kirk McKenzie, Sheila.
Advanced Virgo Optical Configuration ILIAS-GW, Tübingen Andreas Freise - Conceptual Design -
Frequency Dependent Squeezing Roadmap toward 10dB
S. ChelkowskiSlide 1WG1 Meeting, Birmingham 07/2008.
LIGO-G R Quantum Noise in Gravitational Wave Interferometers Nergis Mavalvala PAC 12, MIT June 2002 Present status and future plans.
Opto-mechanics with a 50 ng membrane Henning Kaufer, A. Sawadsky, R. Moghadas Nia, D.Friedrich, T. Westphal, K. Yamamoto and R. Schnabel GWADW 2012,
LIGO- G R LSC meeting at LSU, August Caltech 40m Lab Update LSC meeting at LSU Aug 16, 2006 Robert Ward, Caltech and the 40m team: Rana.
LSC March Meeting LIGO Hanford Observatory, March 22, 2006
Generation of Spurious Signals in Nonlinear Frequency Conversion Tyler Brewer, Russell Barbour, Zeb Barber.
Alexander Khalaidovski, Henning Vahlbruch, Hartmut Grote, Harald Lück, Benno Willke, Karsten Danzmann and Roman Schnabel STATUS OF THE GEO HF SQUEEZED.
SQL Related Experiments at the ANU Conor Mow-Lowry, G de Vine, K MacKenzie, B Sheard, Dr D Shaddock, Dr B Buchler, Dr M Gray, Dr PK Lam, Prof. David McClelland.
The road to 10 dB Kate Dooley, Emil Schreiber GWADW, Girdwood, May LIGO-G
G R Interferometer Sensing & Control P Fritschel 8 Oct 02.
GEO Status and Prospects Harald Lück ILIAS / ETmeeting Cascina November 2008.
Carmen Porto Supervisor: Prof. Simone Cialdi Co-Supervisor: Prof. Matteo Paris PhD school of Physics.
H1 Squeezing Experiment: the path to an Advanced Squeezer
Interferometer configurations for Gravitational Wave Detectors
Squeezing in Gravitational Wave Detectors
Quantum noise reduction using squeezed states in LIGO
Demonstration of lock acquisition and optical response on
Quantum Opportunities in Gravitational Wave Detectors
New directions for terrestrial detectors
Reaching the Advanced LIGO Detector Design Sensitivity
The Quantum Limit and Beyond in Gravitational Wave Detectors
Progress toward squeeze injection in Enhanced LIGO
Interferometric speed meter as a low-frequency gravitational-wave detector Helge Müller-Ebhardt Max-Planck-Institut für Gravitationsphysik (AEI) and Leibniz.
Nergis Mavalvala Aspen January 2005
MIT Corbitt, Goda, Innerhofer, Mikhailov, Ottaway, Pelc, Wipf Caltech
Generation of squeezed states using radiation pressure effects
Nergis Mavalvala (age 47)
Homodyne readout of an interferometer with Signal Recycling
Quantum Noise in Advanced Gravitational Wave Interferometers
Quantum Noise in Gravitational Wave Interferometers
Quantum effects in Gravitational-wave Interferometers
Nergis Mavalvala Aspen February 2004
Ponderomotive Squeezing Quantum Measurement Group
Australia-Italy Workshop October 2005
Quantum Optics and Macroscopic Quantum Measurement
Squeezed states in GW interferometers
Quantum studies in LIGO Lab
Detection Of High Frequency Gravitational Waves At LIGO W. Butler , A
Optical Squeezing For Next Generation Interferometric Gravitational Wave Detectors Michael Stefszky, Sheon Chua, Conor Mow-Lowry, Ben Buchler, Kirk McKenzie,
LIGO Quantum Schemes NSF Review, Oct
Nergis Mavalvala MIT December 2004
Squeezed Input Interferometer
Squeezed Light Techniques for Gravitational Wave Detection
Advanced Optical Sensing
Measurement of radiation pressure induced dynamics
Presentation transcript:

Jan 29, 2007 LIGO Excomm, G R 1 Goal: Experimental Demonstration of a Squeezing-Enhanced Laser-Interferometric Gravitational Wave Detector in the Advanced LIGO Configuration (or similar configurations) Squeezing 40m Keisuke Goda, Osamu Miyakawa, Eugeniy Mikhailov, Shailendhar Saraf, Steve Vass, Alan Weinstein, Nergis Mavalvala  The flipper mirror is inserted in between the SRM and OMC for squeezing measurements.  Squeezed vacuum is generated by the optical parametric oscillator (OPO) pumped by the MOPA laser.  The squeezed vacuum is injected into the dark port via the optical circulator (Faraday isolator and PBS).  Noise-locking technique is used to lock the squeeze angle so that broadband reduction of the IFO shot noise can be achieved. DRMI/RSE Quantum Noise Budget Input Power to BS = 700mW Homodyne Angle = 0 Squeeze Angle = π/2 Initial Squeezing Level = 5dB Injection Loss = 10% Detection Loss = 10%

Jan 29, 2007 LIGO Excomm, G R 2 Generation of Squeezed Vacuum in Optical Parametric Oscillation and Injection of Squeezing to the IFO  The OPO is a 2.2cm long cavity composed of a periodically poled KTP crystal with flat/flat AR/AR surfaces and two coupling mirrors (R = 99.95% at 1064/532nm and R = 92%/4% at 1064/532nm).  The OPO is pumped by 300 mW of second-harmonic light at 532nm.  Quasi-phase matching is used and both the seed and pump are polarized in the same direction.  Frequency-shifted, orthogonally polarized light is used to lock the OPO cavity so that a vacuum field at 1064nm can couple to the cavity and get squeezed by its nonlinear interaction with the pump field in a TEM00 mode.  The picomotor mirror can be inserted in or out for squeezing-enhanced IFO measurements.  Isolation of a GW signal from the injection of squeezing is done by Faraday isolation.  The squeezing-enhanced GW-signal/shot-noise ratio is measured by the DC PD with high quantum efficiency (93%). Coupling Mirrors PPKTP

Jan 29, 2007 LIGO Excomm, G R 3 Some Results & Future Work  About 6dB of scanned squeezing  About 4dB of phase-locked squeezing  Measured by the squeezing monitoring homodyne detector  Ready to be injected into the IFO in the next few weeks to demonstrate squeezing-enhanced IFO  Shot noise  Squeezed shot noise