GWADW2016 - Impact of Recent Discoveries on Future Detector Design

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Sessions*

Plenary 7 - Future detectors requirements, goals, possibilities

Plenary 6 - Enhanced interferometers near term (<12 years)

Plenary 9 - Workshop summaries

Plenary 8 - IFO configurations & squeezing

Summary

Plenary 10 - Future plans

Coordination of Future Development of Large Detectors

Plenary 2 - Science case for future Detectors

Plenary 1

Plenary 4 - Cryogenics

Plenary 3 - Workshop goals

Low frequency workshop

Plenary 5 - LISA Pathfinder

Thermal noise & coatings workshop

Controls Workshop

Poster Session

Include materials from selected sessions

Contributions*

A high-isolation, low-loss, in-vacuum, thermally-controlled Faraday isolator (in session "Poster Session")

A study of contamination in gravitational wave detectors (in session "Poster Session")

A Tunable Resonant Detector for Low Frequency Gravitational Waves (in session "Poster Session")

A. Low frequency (in session "Plenary 3 - Workshop goals")

Ambient Seismic Noise (in session "Low frequency workshop")

Ambient seismic noise and its potential use in seismic exploration and monitoring (in session "Poster Session")

Amorphous dielectric coatings (in session "Thermal noise & coatings workshop")

Amorphous optical coatings for gravitational-wave interferometers (in session "Thermal noise & coatings workshop")

Amorphous silicon as low loss, high refractive index material for dielectric mirror coatings (in session "Poster Session")

Angular control of Advanced Virgo suspended benches (in session "Controls Workshop")

Angular control of Advanced Virgo suspended benches (in session "Poster Session")

Angular loop consideration (in session "Controls Workshop")

Atmospheric NN modeling (in session "Low frequency workshop")

Atom Interferometer GW Detectors (in session "Plenary 8 - IFO configurations & squeezing")

Atomic structure investigations of amorphous coatings (in session "Thermal noise & coatings workshop")

B. Introduction to thermal noise workshop and goals (in session "Plenary 3 - Workshop goals")

Balanced homodyne readout (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

Brief description of next gen concepts (in session "Controls Workshop")

C. Controls (in session "Plenary 3 - Workshop goals")

Characterisation of the aLIGO monolithic suspensions (in session "Poster Session")

Coating - What's available now and in the 5-10 years (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

Coatings Thermal noise workshop discussion points (in session "Thermal noise & coatings workshop")

Coil-Coil Actuator for reduction of magnetic noise (in session "Poster Session")

Comparison of ring-Sagnac and sloshing-Sagnac interferometer (in session "Poster Session")

Controls (in session "Plenary 9 - Workshop summaries")

Cryogenic mechanical loss of IBS silica (in session "Poster Session")

Cryogenics Round Table (in session "Plenary 4 - Cryogenics")

Cyogenics session overview (in session "Plenary 4 - Cryogenics")

Define inputs and outputs (in session "Controls Workshop")

Developing a squeezed light source at Virgo site (in session "Poster Session")

Development of ultra-low optical and mechanical loss aSi coatings using novel ECR ion beam deposition (in session "Thermal noise & coatings workshop")

Development of ultra-low optical and mechanical loss aSi coatings using novel ECR ion beam deposition (in session "Poster Session")

Discussion (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

Discussion (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

Discussion (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

Discussion (in session "Thermal noise & coatings workshop")

Discussion (in session "Thermal noise & coatings workshop")

Discussion (in session "Thermal noise & coatings workshop")

Discussion (in session "Controls Workshop")

Discussion (in session "Controls Workshop")

Discussion (in session "Controls Workshop")

Discussion (in session "Controls Workshop")

Dynamics of Fiber Amplifiers in the Context of Gravitational Wave Detectors’ Laser Sources (in session "Poster Session")

Electromagnetic Derivation of Thermal Noise in Grating Reflectors (in session "Poster Session")

Environment at the underground GW detector KAGRA (in session "Poster Session")

Factors pertaining to the strength of four-fiber monolithic silica test mass suspensions. (in session "Poster Session")

Feedforward control for arm cavities (in session "Controls Workshop")

FINESSE 2.1 - with Multimode Squeezing (in session "Poster Session")

Fitting tools (in session "Controls Workshop")

Global Network of 2G+ and 3G Detectors (in session "Plenary 2 - Science case for future Detectors")

GWADW 2016 Summary (in session "Summary")

Heterogeneous detector networks discussion (in session "Plenary 7 - Future detectors requirements, goals, possibilities")

High and Low Frequency Sensitivity Improvements (in session "Plenary 1")

High power fibered electro-optics components (in session "Poster Session")

Hopes and Dreams: One Transfer Func4on Fi6ng Program to Rule Them All (in session "Controls Workshop")

How to use the earthquakes arrival predictor to put the IFO in robust mode (in session "Controls Workshop")

Indium bond research for crystalline cryogenic suspensions (in session "Poster Session")

Installation of Input Mode Cleaner of iKAGRA (in session "Poster Session")

Intracavity Squeezing I (in session "Plenary 8 - IFO configurations & squeezing")

Intracavity Squeezing II (in session "Plenary 8 - IFO configurations & squeezing")

Introduction (in session "Plenary 8 - IFO configurations & squeezing")

Investigation of Suspension Upgrades for the Advanced LIGO Gravitational Wave Detector (in session "Poster Session")

Large band low frequency sensors based on Watt’s linkage for future generations of interferometric detectors (in session "Poster Session")

Laser power stabilization for future gravitational wave detectors (in session "Poster Session")

Learning Methods for Interferometers (in session "Controls Workshop")

Lenses and wedges – Do these make sense for long arms? (in session "Plenary 7 - Future detectors requirements, goals, possibilities")

LIGO: the A+ upgrade (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

LISA in the post detection and post LISA Pathfinder era (in session "Plenary 5 - LISA Pathfinder")

LISA Pathfinder scientific operations (in session "Plenary 5 - LISA Pathfinder")

Low Frequency (in session "Plenary 9 - Workshop summaries")

Low Frequency Noise Impact - Summary (in session "Plenary 7 - Future detectors requirements, goals, possibilities")

Low-frequency seismic sensors (in session "Low frequency workshop")

MEMS sensor development (in session "Low frequency workshop")

MIMO damping (in session "Controls Workshop")

Minimizing test mass thermal noise with crystalline coatings (in session "Thermal noise & coatings workshop")

Modeling coating thermal noise for gravitational wave detectors (in session "Thermal noise & coatings workshop")

Multimessenger Astronomy (in session "Plenary 2 - Science case for future Detectors")

Need for coordinated R&D: the ET perspective (in session "Coordination of Future Development of Large Detectors")

Need for coordinated R&D: the LIGO perspective (in session "Coordination of Future Development of Large Detectors")

New OSEM results using a displacement-doubling prism-based flag (in session "Poster Session")

New results on losses correlation with structure (in session "Thermal noise & coatings workshop")

New Topology Speedmeter (in session "Plenary 8 - IFO configurations & squeezing")

Newtonian Seismic Array at LHO (in session "Low frequency workshop")

NN modeling for MIGA (in session "Low frequency workshop")

Optical absorption of amorphous silicon coatings(included in previous slides) (in session "Thermal noise & coatings workshop")

Optical levitation of a mirror (in session "Poster Session")

Overview of the 20 K configuration (in session "Plenary 4 - Cryogenics")

Overview of the 120 K configuration (in session "Plenary 4 - Cryogenics")

Photoelasticity of Silicon and its temperature dependence (in session "Poster Session")

Possible models for GWIC’s role (in session "Coordination of Future Development of Large Detectors")

Present and future of superattenuator control system (in session "Controls Workshop")

Quantum dense metrology (in session "Plenary 8 - IFO configurations & squeezing")

Radiation pressure induced instability (in session "Controls Workshop")

Reduction of quantum noise for gravitational wave detector KAGRA (I) (in session "Poster Session")

Reduction of quantum noise for gravitational wave detector KAGRA (II) (in session "Poster Session")

Reduction of Seismic Coupling Noise for TOBA (in session "Poster Session")

Reduction of Virgo Low Frequency environmental magnetic noise (in session "Poster Session")

Scattering, technical noise and alignment, stability (in session "Plenary 7 - Future detectors requirements, goals, possibilities")

Science targets for future detectors (in session "Plenary 7 - Future detectors requirements, goals, possibilities")

Seismic rotational measurements (in session "Low frequency workshop")

Sensitivity limits of atom interferometry gravity gradiometers and strainmeters (in session "Low frequency workshop")

Sensor development and characterization at Nikhef (in session "Low frequency workshop")

Setting the stage (in session "Plenary 1")

Silicate bonding extends to the photonics industry (in session "Poster Session")

Some thoughts on controls challenges, considerations for discussion (in session "Controls Workshop")

Squeezing at 1064nm (in session "Plenary 8 - IFO configurations & squeezing")

Squeezing at 1550nm and across the wavelengths (in session "Plenary 8 - IFO configurations & squeezing")

Squeezing with long filter cavities (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

Summary of science goals (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

Suspending 400kg mirrors (in session "Plenary 7 - Future detectors requirements, goals, possibilities")

Synergy between space and terrestrial detectors (in session "Plenary 7 - Future detectors requirements, goals, possibilities")

The input optics for iKAGRA (in session "Poster Session")

Thermal conductivity of bonded materials for future generation gravitational wave observatories (in session "Poster Session")

Thermal noise & Coatings (in session "Plenary 9 - Workshop summaries")

Thermo-refractive noise measurement in the Advanced Virgo Output Mode Cleaner (in session "Poster Session")

Thermoelastic damping in silicon and metallic discs: the mode shape dependent branching effect (in session "Thermal noise & coatings workshop")

Thermoelastic damping in silicon and metallic discs: the mode-dependent branching effect (in session "Poster Session")

TOBA: a Low-frequency Gravitational-Wave Antenna (in session "Poster Session")

TOBA: a Low-frequency Gravitational-Wave AntennaMasaki (in session "Low frequency workshop")

Toward LISA in the USA (in session "Plenary 5 - LISA Pathfinder")

Towards Low Frequency Gravitational Force Sensing (in session "Low frequency workshop")

Trade-offs for squeezed light injection in a non-perfect world (in session "Poster Session")

Triangles vs Ls (in session "Plenary 7 - Future detectors requirements, goals, possibilities")

Twin Signal Recycling for the Einstein Telescope (in session "Poster Session")

Ultra-quiet Mirror Suspensions for the Glasgow Sagnac Speed Meter (in session "Poster Session")

Vibration Isolation System for KAGRA: Overview and Results in the First Operation (in session "Poster Session")

Virgo upgrade plans (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

Voyager: Pros and cons of the cryo-silicon-2micron idea (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

Welcome (in session "Plenary 1")

What Binary Black Holes Teach (in session "Plenary 1")

What environmental changes or instrument drifts require re-tuning (in session "Controls Workshop")

What if we are stuck with the coatings I (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

What if we are stuck with the coatings II (in session "Plenary 6 - Enhanced interferometers near term (<12 years)")

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