GWADW 2013 - Gravitational Wave Detectors for the Next Decade Workshop

Name: GWADW 2013 - Gravitational Wave Detectors for the Next Decade Workshop
Start: 2013-05-19T17:00:00+02:00
End: 2013-05-25T19:00:00+02:00
Location: No location set

May 19 – 25, 2013

Europe/Rome timezone

Overview
The Workshop
The Travel
The Accommodation
Registration
Timetable
Timetable and Posters
Participant List

E-mail

gwadw@pi.infn.it

Material Package

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Sessions*

3 am brain session

Atom Interferometry

Pulsar Timing

Mitigating Thermal Noise I

Simulations

Setting the Stage

Early Lessons and Challenges in the Commissioning of Advanced Detectors

Future Interferometric Detectors

Astrophysical GW Sources

Mitigating Thermal Noise II

Plans for GWADW 2014 and discussion about GWADW 2015 - Open Discussion

Space Antennae

Cryogenics

Light sources and Interferometer Topologies

Workshop Adjourn

Workshop Summary

Poster session

Poster

Poster session

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Contributions*

"Introductory Talk": Light Sources Interferometer Topologies (in session "Light sources and Interferometer Topologies")

A double pendulum for lab testing of free fall on 2 DoFs (in session "Space Antennae")

A polarizing Sagnac topology with DC readout for future gravitational wave detectors (in session "Light sources and Interferometer Topologies")

A review of optical simulation techniques (in session "Simulations")

Active thermal lensing elements for spherical and astigmatic mode matching (in session "Poster")

aLigo analysis pipelines using simulated data (in session "Simulations")

Alternative configurations for Space-based GW detectors (in session "Space Antennae")

Anomalous Dynamical Back-Action in Michelson Interferometers (in session "Light sources and Interferometer Topologies")

Atomic gravitational wave sensors (in session "Atom Interferometry")

Bonding (in session "Poster session")

Broadband Sagnac Interferometer with short Filter Cavities (in session "Light sources and Interferometer Topologies")

Building up a commissioning network (in session "Early Lessons and Challenges in the Commissioning of Advanced Detectors")

Bulk silicon mechanical loss for estimates of thermal noise-what do know/need to know? (in session "Mitigating Thermal Noise II")

Challenges waiting in commissioning and preparations (in session "Simulations")

Characterization and direct thermal noise measurement of coatings (in session "Mitigating Thermal Noise I")

Chasing excess noise, focusing on diffused light (in session "Early Lessons and Challenges in the Commissioning of Advanced Detectors")

Coating modelling (in session "Poster session")

Coping with aberrations (in session "Early Lessons and Challenges in the Commissioning of Advanced Detectors")

Cosmology (in session "Astrophysical GW Sources")

Cryogenic properties of sapphire fibres (in session "Poster session")

Cryogenic Silicon Research for the Future of LIGO (in session "Cryogenics")

Design and expected thermal noise of the KAGRA sapphire suspensions (in session "Mitigating Thermal Noise II")

Detecting chirping gravitational waves in real time and its astrophysical implications (in session "Astrophysical GW Sources")

Electronical Absorption of Silicon at Cryogenic Temperatures (Julius Konna, Friedrich-Schiller University Jena) (in session "Poster")

eLISA and L2 process. Submission of White paper (in session "Space Antennae")

ET Overview (in session "Future Interferometric Detectors")

ET Seismic surveys (in session "Future Interferometric Detectors")

Experiences and lessons learned from interferometer simulations at GEO (in session "Simulations")

Experimental results on the thermal noise of oscillators in non equilibrium steady states (in session "Mitigating Thermal Noise I")

First Lessons from the aLIGO Commissioning (in session "Early Lessons and Challenges in the Commissioning of Advanced Detectors")

Geodesic reference performance limits for space gravitational wave missions (in session "Space Antennae")

Gravitational Reference Sensor Technology Advancements (in session "Poster session")

Gravitational Reference Sensor Technology Advancements (in session "Space Antennae")

How does cryogenics improve the sensitivity of interferometers? (in session "Cryogenics")

Improving the capabilities of localizing the sources of gravitational waves with the pulsar timing array(s): news and views from the PPTA (in session "Pulsar Timing")

Increasing the sensitivity of the NANOGrav PTA: recent improvements in backends and software (in session "Pulsar Timing")

Introductory Talk (in session "Simulations")

Japan 2014 (in session "Plans for GWADW 2014 and discussion about GWADW 2015 - Open Discussion")

Laser frequency noise immune gravitational wave detection using atom interferometry (in session "Atom Interferometry")

Lavender (in session "3 am brain session")

Lessons from commissioning cryogenic systems underground (in session "Early Lessons and Challenges in the Commissioning of Advanced Detectors")

LIGO3G (in session "Future Interferometric Detectors")

LISA 2020: An intermediate scale space gravitational wave observatory for this decade (in session "Space Antennae")

LOFAR: Building a Flexible and Responsive Radio Telescope for Pulsars and Transients (in session "Pulsar Timing")

Mechanical loss of amorphous thin films at low temperatures (in session "Poster session")

Modal simulation of dual recycled interferometers (in session "Simulations")

Multiple optical springs in coupled resonator systems (in session "Light sources and Interferometer Topologies")

MutiSAS + Control (in session "Future Interferometric Detectors")

New noise estimates in waveguide coatings (in session "Mitigating Thermal Noise I")

Newtonian noise effects in atom interferometers (in session "Atom Interferometry")

Newtonian Noise Substraction (in session "Future Interferometric Detectors")

Non-equilibrium thermal noise (in session "Poster session")

Novel alingnment sensing scheme with RF jitter modulation (in session "Poster")

Open questions re the use of crystalline coating materials (in session "Mitigating Thermal Noise I")

Optical measurements at cryogenic temperatures (in session "Cryogenics")

Optical techniques for reducing thermal noise (in session "Mitigating Thermal Noise II")

Optics for Future Detectors (in session "Future Interferometric Detectors")

Overview talk on advances and challenges in mitigating thermal noise (in session "Mitigating Thermal Noise I")

Properties of silicon and coatings for a low temperature detector (in session "Cryogenics")

Prospects and Progress in Crystalline coatings: AlGaAs (in session "Mitigating Thermal Noise I")

Prospects and Progress in Crystalline coatings: AlGaP (in session "Mitigating Thermal Noise I")

Pulsar timing perspectives with the new Sardinia Radio Telescope (in session "Pulsar Timing")

Sagnac Interferometer for GW Detection (in session "Light sources and Interferometer Topologies")

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

Silicon absorption (in session "Poster session")

Silicon suspensions (in session "Poster session")

Simulation of Sensitivity curves for dual recycled interferometers using DarkF (in session "Simulations")

Squeezing for future generation detectors (in session "Future Interferometric Detectors")

Status of activities on crystalline suspensions at Nikhef (in session "Cryogenics")

Strong field tests of GR (in session "Astrophysical GW Sources")

Summary (in session "Workshop Summary")

Suspensions for future GWDs (in session "Future Interferometric Detectors")

System for characterising Virgo/Advanced Virgo test mass Qs (in session "Mitigating Thermal Noise II")

The MAGIA Experiment: current status and future prospects (in session "Atom Interferometry")

The path to ultra broad band pulsar observations at the Effelsberg 100m and its impact on EPTA results (in session "Pulsar Timing")

Time domain simulation for the lock acquisition study of aLIGO (in session "Simulations")

UF-LIGO Cryogenic Test Bed (in session "Poster session")

Using the phase camera in advanced interferometers (in session "Simulations")

Verification of cooling time reduction of interferometric cryogenic gravitational wave detectors using high emissivity coating (in session "Cryogenics")

Very long baseline underground gravitation antenna with atom interferometry (in session "Atom Interferometry")

Welcome (in session "Setting the Stage")

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5/20/13

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5/22/13

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5/24/13

5/25/13

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GWADW 2013 - Gravitational Wave Detectors for the Next Decade Workshop

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