Discussion of GWIC 3G Report: acceptance and follow-up actions

Slides:



Advertisements
Similar presentations
Alan Edwards European Commission 5 th GEO Project Workshop London, UK 8-9 February 2011 * The views expressed in these slides may not in any circumstances.
Advertisements

Beyond the ALCPG David B. MacFarlane Associate Laboratory Director for PPA.
CHIPP Workshop on Detector R&D June - University of Geneva Common R&D for astroparticle physics: Activities of ApPEC and ASPERA Bernard Revaz and.
1 Research Infrastructures in FP7 EUDET Annual Meeting 19 October 2006, Munich Dr. Gerburg Larsen European Commission, RTD-B.3 - Research Infrastructures.
Regional Integration Cluster Olivier Hartmann - SSATP.
Towards a European network for digital preservation Ideas for a proposal Mariella Guercio, University of Urbino.
© Crown copyright Met Office Requirements, objectives and desired outcomes for the Workshop Stuart Goldstraw, CBS IOS ET-SBO Chair, 24 th April 2013.
LIGO-G M Summary Remarks: Management of LIGO Gary Sanders California Institute of Technology NRC Committee on Organization and Management of Research.
1 Direction scientifique Networks of Excellence objectives  Reinforce or strengthen scientific and technological excellence on a given research topic.
1 ASTRONET Coordinating strategic planning for European Astronomy.
LIGO-G M Organization and Budget Gary Sanders NSF Operations Review Caltech, February 26, 2001.
Consultant Advance Research Team. Outline UNDERSTANDING M&E DATA NEEDS PEOPLE, PARTNERSHIP AND PLANNING 1.Organizational structures with HIV M&E functions.
LIGO-G M Overview of LIGO R&D and Planning for Advanced LIGO Detectors Gary Sanders NSF R&D Review Caltech, January 29, 2001.
LIGO-G M Overview of the LIGO Continuing Operations (FY FY2006) Proposal Gary Sanders LIGO PAC9 Meeting December 2000.
Under construction SPANISH PRESIDENCY OF THE EU 2010 FRAMEWORK CONDITIONS ROADMAP 4-May-2010.
Section 4.9 Work Group Members Kris Hafner, Chair, Board Member Rob Kondziolka, MAC Chair Maury Galbraith, WIRAB Shelley Longmuir, Governance Committee.
Working Group II Terms of Reference Presented to CGMS Plenary and Working Group II CGMS-44 CGMS-WP-30.
Lessons to be learned from the ET design study Michele Punturo INFN Perugia ET-0005A-16 Dawn Meeting
Incoming Themes for 2017 Frank Kelly, USGS
Bow Basin Watershed Management Plan Revised Terms of Reference
ARIES WP2 Task 2.2 kick-off Coordination, support and enhancement of communication/outreach activities for accelerators in Europe Jennifer Toes (CERN),
The Quest for Gravitational Waves: a global strategy
Update from the Faster Payments Task Force
Dawn II, July 8, 2016 GaTech Organizing the international community: issues, open questions, opportunities Dave Reitze LIGO Laboratory, Caltech LIGO Laboratory.
CILIP Performance Framework – Business metrics & KPI
GW Policy: The Future: G3 Detectors
Achievements in 2016 Data Integration Linked Open Metadata
System Planning To Programming
Open and inclusive budgeting: Working beyond boundaries
Updating the Regulation for the JINR Programme Advisory Committees
New gTLD Auction Proceeds CCWG Status Update
Ground-based Gravitational-wave Detectors: Beyond 2030
Influencing the Progress of Advanced Core Technologies
The ESS vision, ESSnets and SDMX
Programme Board 6th Meeting May 2017 Craig Larlee
Goal of the workshop To define an international roadmap towards colliders based on advanced accelerator concepts, including intermediate milestones, and.
CERN LVC workshop roundtable (what’s coming next?)
Title Goes Here Name (s), Organization, CEOS Affiliation CEOS SIT-33
CEOS Status/Overview Steven Hosford WGCapD-7 Agenda Item #6
IT Governance Planning Overview
Support for the AASHTO Committee on Planning (COP) and its Subcommittees in Responding to the AASHTO Strategic Plan Prepared for NCHRP 8-36, TASK 138.
WMO Global Multi-Hazard Alert System
Stan Whitcomb LSC meeting Livingston 21 March 2005
Knowledge Translation
WP4 Positioning European Astroparticle Physics in the world-wide context WP leader CNRS Partners: FOM, IFIN-HH, FRS-FNRS/FWO, FCT Total work: 22 months.
Scanning the environment: The global perspective on the integration of non-traditional data sources, administrative data and geospatial information Sub-regional.
Review of Chair Priorities
Update RDA Strategy Discussion
Jozsef Szlezak & Pawel Kazmierczyk (EEA)
AMICI WP1 – Management, coordination and dissemination
Helene Skikos DG Education and Culture
The United Nations’ Legal Identity Agenda: Fulfilling the promise to Leave No One Behind Presented by, Kristen Wenz, Focal Point for the UN Legal Identity.
NERC Reliability Standards Development Plan
Finance & Planning Committee of the San Francisco Health Commission
Update RDA Strategy Discussion
Project proposal BRENTFORD SUSTAINABLE COMMUNITY STRATEGY
The MSK-HQ Developing a generic Musculoskeletal Patient Reported Outcome Measure Policy & Public Affairs Team, Arthritis Research UK e.
ASTRONET Coordinating strategic planning for European Astronomy
IMPROVING PUBLIC INFORMATION
7th EU Research FP has ten themes defined in order:
EU Marine Strategy DG Environment B.1.
NERC Reliability Standards Development Plan
Fitness Check EU Water Policy
Preliminary Project Execution Plan
League of Advanced European Neutron Sources
Next steps APPEC Gravitational Waves Job de Kleuver
Umbrella Organisation A proposal for Discussion
Getting Knowledge into Action for Healthcare Quality
- Kick-off meeting - ERANET Cofund BlueBio WP4 (Leader: AEI)
Draft Charter Community of Practice for Direct Access Entities
Presentation transcript:

Discussion of GWIC 3G Report: acceptance and follow-up actions Sheila Rowan GWIC Chair Dawn V Cascina, 26 - 27th May 2019

Charge, progress and draft recommendations of the draft 3G study Next steps.

Science case Charge: Commission a study of ground-based gravitational wave science from the global scientific community, investigating potential science vs architecture vs. network configuration vs. cost trade-offs, recognizing and taking into account existing studies for 3G projects (such as ET) as well as science overlap with the larger gravitational-wave spectrum Progress: Draft report leaves no doubt that there is a wealth of science to be delivered by detectors ~X10 more sensitive than the current ‘Advanced’ instruments Outcomes: Clear advantage with 3 x 3G detectors Global network delivers the optimum science

R&D Charge: Develop and facilitate coordination mechanisms among the current and future planned and anticipated ground-based GW projects, including identification of common technologies and R&D activities as well as comparison of the specific technical approaches to 3G detectors. Possible support for coordination of 2G observing and 3G construction schedules. Progress: Substantial evaluation of current status of technology and R&D and identification of specific areas of common global interest Recommendations: R1 An international 3G R&D coordination committee should be formed, with broad and inclusive membership representing GW groups across the world. A series of workshops on enabling technologies should be held in order to stimulate exchange of ideas and allowing (if deemed useful) for coordination of the person-power intensive experimental activities. Each of the major R&D tasks should generate a list of goals with quantitative metrics, timelines and required resources. Activities requiring global collaboration and coordination should be laid down and pathways identified.

R&D Recommendations: R2: International consortia should be formed to work on key issues with industry partners, establish a governance and organisational structure with teeth (i.e. controls purse strings) and seek funding through joint proposals submitted across funding agencies. R3: National funding agencies should increase funding (staff and instrumentation) to enable the required long-term research programmes at relevant laboratories and prototype interferometers. R4: Existing GW collaborations should integrate 3G R&D tasks and corresponding deliverables into their programs in order to ensure sufficient support for the long-term future of the field. In particular, over the next 5 years, mature 2G enabling technologies (e.g. 1064 nm laser, fused silica optics, coatings) should be demonstrated to be up-scaled and ready for application in 3G facilities.

Networking Charge: organize and facilitate links between planned global 3G projects and other relevant scientific communities, including organizing: town hall meetings to survey the community dedicated sessions in scientific conferences dedicated to GW physics and astronomy focused topical workshops within the relevant communities Progress: Regular activity in the above areas – reaching out to the astronomy, particle astrophysics and particle physics communities Co-ordinated submissions from or endorsed by GWIC to roadmapping and planning exercises over the last few years.

Agency Interfacing and Advocacy Charge: identify and establish a communication channel with funding agencies who currently or may in the future support ground-based GW detectors; communicate as needed to those agencies officially through GWIC on the scientific needs, desires, and constraints from the communities and 3G projects (collected via 1) – 3) above) structured in a coherent framework; serve as an advocacy group for the communities and 3G projects with the funding agencies. Progress (as an action based charge there is no written report - examples include): Formation of the Gravitational Wave Agencies Correspondents group Multiple presentations by GWIC to GWAC (2016, onwards) Joint meetings with GWAC and APPEC representatives at DAWN IV, V Presentation at APPEC General Assembly, Barcelona (Dec 2017) Upcoming invitation to GWIC to present to the ‘Group of Senior Officials’ meeting, (3rd June, Roscoff) Recommendations: This need continues to exists with GWIC currently still well placed to facilitate communication Future role tbd in the context of governance recommendations

Governance Evaluation Charge: By applying knowledge of the diverse structures of the global GW community, propose a sustainable governance model for the management of detector construction and joint working, to support planning of 3rd generation observatories. Progress: draft report delivered. Three example options for international governance models. Recommendations: Experience suggests arriving at a global governance model is an evolution process, emerging from sustained collaboration between project leaders and funding agencies. Phased approach proposed to walk down that path starting now.

Next steps on the report We are here May 26 - present major conclusions (in draft form) at the Dawn V workshop in Cascina for community discussion, feedback End of May - send out reports to a broad list of reviewers for feedback by June 30.  Also circulate broadly to relevant communities (LSC, Virgo, KAGRA, LISA, ..) for input/comment/feedback July 7 - present a mature draft of the report to GWIC, present at Amaldi August 30 - deliver final version of the report (Caveat: the GWIC 3G Committee may revise these dates.) Aim to reach a consensus on the contents of the report - tune and make complete.

Next steps on future planning – topics for discussion A common key recommendation is around a proposal for the continuation/change/end of the GWIC 3G committee Addressed to the field: Form an international (non-legal) umbrella organization Charge people to write the charter R&D as one first focus of this group    Advocacy: dedicated effort: team whose #1 priority is 3G - advocating, planning, seeking funding, standing up R&D programs, and coordinating across the globe ? in the early phase, before a common management/governance structure is still missing, should we include in the management team of each project a delegate of the other project(s)?

Next steps on future planning – topics for discussion Addressed to the Agencies Apportion resource/develop joint tools, and for funding R&D at an international or even global level Work with the community on advancing common governance structures Seek to lay placeholders within the available infrastructural resource models for relevant scale of future GW observatories