GWIC Roadmap 2010

A strategic tool in planning for the development of capabilities and facilities needed to seize the tremendous scientific opportunities now on the horizon.

GWIC Roadmap 2010

In the coming decades, ultra-sensitive arrays of ground-based instruments and complementary spaced-based instruments will continue to observe the gravitational wave sky, inevitably discovering entirely unexpected phenomena while providing new insight into many of the most profound astrophysical phenomena known. This new window into the cosmos could revolutionize humanity’s understanding of the Universe in which we live.

The goal of this roadmap is to serve the international gravitational wave community and its stakeholders as a tool for the development of capabilities and facilities needed to address the exciting scientific opportunities on the intermediate and long-term horizons.

This roadmap will serve the international gravitational wave community and its stakeholders as a strategic tool in planning for the development of capabilities and facilities needed to seize the tremendous scientific opportunities now on the horizon. This material represents the consensus best judgment of GWIC following discussions with leaders in the gravitational-wave field and with other members of the gravitational physics and astrophysics communities, and with representatives of funding agencies.

GWIC Roadmap 2010 Committee

  • Karsten Danzmann, AEI Hannover, Germany
  • James Hough, University of Glasgow, UK (ex-officio)
  • Kazuaki Kuroda, Institute for Cosmic Ray Research, Tokyo, Japan
  • David McClelland, Australian National University, Australia
  • Jay Marx, Caltech, USA
  • Benoit Mours, LAPP Annecy, France
  • Sterl Phinney, Caltech, USA
  • Sheila Rowan, University of Glasgow, UK
  • Flavio Vetrano, University of Urbino, Italy
  • Stefano Vitale, University of Trento, Italy
  • Stan Whitcomb, Caltech, USA
  • Clifford Will, Washington University, St Louis, USA
  • Advisory Member: B. Sathyaprakash, Cardiff University, USA