GWADW 2011 - Gravitational Waves Advanced Detectors Workshop - Progress Towards the Next Generation of Gravitational Wave Detectors

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Workshop Summary

Squeezed Light I

Novel Approaches to GW Detectors

Optical Configurations

Simulations (continued)

Squeezed Light II

Cryogenics in the Future

Future of GWADW

Simulations

Control Systems

Space Detectors

Inertial Sensors and Environmental Disturbance Removal

Lessons Learned

Setting the Stage

LCGT

Lessons Learned (continued)

Light Sources

Mitigating Newtonian Noise

Ways to Bring Down Thermal Noise

Enhanced 2nd Generation Detectors

ET

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Contributions*

AdVirgo Design (in session "Simulations")

An Updated Crash Course in Newtonian Noise (in session "Mitigating Newtonian Noise")

ANU Squeezing Progress (in session "Squeezed Light I")

Atom Interferometry for Gravitational Wave Detectors (in session "Novel Approaches to GW Detectors")

Central Heating Radius of Curvature Compensation System Used in Virgo (in session "Control Systems")

CLIO (in session "Lessons Learned (continued)")

Cryogenic Mirrors: the State of the Art in Interferometric GW Detectors (in session "Cryogenics in the Future")

DECIGO (in session "Space Detectors")

Detector Configuration and Control Scheme for LCGT (in session "LCGT")

Diffractive Optics Topologies (in session "Optical Configurations")

Digitally Enhanced Interferometry (in session "Optical Configurations")

Discussion to identify what are missing in the existing simulation tools, and to assign who will work on what (in session "Simulations (continued)")

Experimental Results on Cryogenic Strength of Silicon (in session "Cryogenics in the Future")

Feed-Forward Noise Reduction (in session "Control Systems")

Force Isolation at 1 mHz (in session "Space Detectors")

General Status (in session "ET")

GEO (in session "Lessons Learned")

Heterodyne Detection Method to Monitor Thermal Distortions in Mirrors (in session "Control Systems")

High Power Lasers for Third Generation Gravitational Wave Detectors (in session "Light Sources")

Interferometry over 5 Million Km (in session "Space Detectors")

Laser Sources for LTP and LISA (in session "Light Sources")

LCGT-SAS Design and R&D (in session "LCGT")

LIGO (in session "Lessons Learned")

LIGO H1 Squeezing Progress (in session "Squeezed Light I")

LISA (in session "Space Detectors")

LISA Pathfinder. Commissioning a GW Detector 1 Million Km away (in session "Space Detectors")

Materials 1 (in session "Ways to Bring Down Thermal Noise")

Materials 2 (in session "Ways to Bring Down Thermal Noise")

Modeling and Measuring Puzzling Effects of GAS Blades (in session "Inertial Sensors and Environmental Disturbance Removal")

Modeling Thermal Effects in aLIGO Using SIS (in session "Simulations (continued)")

New Beam Shape with Low Thermal Noise (in session "Simulations")

Newtonian Noise Predictions for Underground Environment (in session "Mitigating Newtonian Noise")

Open Discussion (in session "Future of GWADW")

Optical Design in ET (in session "ET")

Optical Techniques for Reducing/Detection Thermal Noise (in session "Ways to Bring Down Thermal Noise")

Opto-Mechnical Coupling for Quantum Experiments (in session "Optical Configurations")

Other Ideas for Reducing Thermal Noise (in session "Ways to Bring Down Thermal Noise")

Payloads at Cryogenic Temperature for Third Generation GW Detectors: Issues and Open Problems (in session "Cryogenics in the Future")

Ponderomotive Squeezing (in session "Squeezed Light I")

Present Design of LCGT Cryogenic Payload (in session "LCGT")

Real Controls with a Simulated Plant (in session "Simulations")

Refrigerator and Cryogenic Suspension (in session "Cryogenics in the Future")

Review of Folded Pendulum Seismometers, Accelerometers and Tiltmeters (in session "Inertial Sensors and Environmental Disturbance Removal")

Second Generation Interferometer Optics Requirements (in session "Simulations")

Seismic Scattering and/or aLIGO Newtonian Noise (in session "Mitigating Newtonian Noise")

Selective Cooling in Advanced Detectors (in session "Novel Approaches to GW Detectors")

Setting the Stage (in session "Setting the Stage")

Sharing Simulation Tools (in session "Simulations (continued)")

SOC Noise and Advanced Hinge Tiltmeters (in session "Inertial Sensors and Environmental Disturbance Removal")

Squeezing in GEO600 (in session "Lessons Learned (continued)")

Squeezing Progress (in session "Squeezed Light I")

Squeezing workshop: Issues and Directions (in session "Squeezed Light II")

Summary (in session "Workshop Summary")

Suspensions and Cryogenics (in session "ET")

Testing Optical Configurations with the Glasgow 10m Prototype (in session "Optical Configurations")

The High Power Light Source for LCGT (in session "Light Sources")

The STAR Program: Science and Advanced Clock Technology on Small Satellites (in session "Novel Approaches to GW Detectors")

Thermal Coating Noise Interferometer at UF (in session "Ways to Bring Down Thermal Noise")

Thermal Noise Related Plans for the AEI Prototype in Hannover (in session "Ways to Bring Down Thermal Noise")

TOBA (Torsion-bar antenna) to Observe Low-Frequency Gravitational Waves (in session "Novel Approaches to GW Detectors")

Underground Infrastructures (in session "ET")

Virgo (in session "Lessons Learned (continued)")

Welcome (in session "Setting the Stage")

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Events scheduled on*

5/22/11

5/23/11

5/24/11

5/25/11

5/26/11

5/27/11

5/28/11

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