DAWN III Workshop: What’s Next for Gravitational Wave Astronomy?

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Presentation transcript:

DAWN III Workshop: What’s Next for Gravitational Wave Astronomy? Barry C Barish LIGO Laboratory 6-July-2017 Strategic Issues

Context of G3: Where will we be? 6-July-17 DAWN III G3 Workshop - Syracuse

Context of G3: Where will we be? KAGRA Kamioka Mine Cryogenic Mirror Underground Technologies crucial for next-generation detectors; KAGRA can be regarded as a 2.5-generation detector.

DAWN III G3 Workshop - Syracuse Context of G3: Where will we be? 6-July-17 DAWN III G3 Workshop - Syracuse

DAWN III G3 Workshop - Syracuse The advanced GW detector network: 2015-2025 Context of G3: Where will we be? Advanced LIGO Hanford 2015 GEO600 (HF) 2011 KAGRA 2017 Advanced LIGO Livingston 2015 Advanced Virgo 2016 LIGO-India 2022 5 5 6-July-17 DAWN III G3 Workshop - Syracuse

Localization of the Source future: more precise Context of G3: Where will we be? 2016-17 2017-18 2019+ 2022+ Adding Virgo will break the annulus As sensitivity progresses, so does the localization. In the design LIGO-Virgo network, GW150914 could have been localized to less than 20 deg2 LIGO India will lead to a further impressive improvement 6-July-17 DAWN III G3 Workshop - Syracuse

DAWN III G3 Workshop - Syracuse G3: Some Big Issues Science Motivations and Goals GWIC Committee (must be done in the context of projected G2) Science Goals  Technical Performance Frequency vs Sensitivity Goals? Network Performance Goals (e.g. Pointing Accuracy)? Strategic Issues How many G3 Detectors are required? G3 Detectors: Identical or Different? How Internationally Organized/Funded/Implemented? Present GW Model: “Collaboration of Collaborations?” Globally Organized, like ILC, SKA? Global w/ Strong Host, like CERN LHC, DUNE? ‘Limited’ Partnerships, like ALMA, LSST, TMT? 6-July-17 DAWN III G3 Workshop - Syracuse