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Low-frequency gravitational wave telescopes

Latham Boyle

Perimeter Institute

The gravitational waves sought by LIGO represent the high-frequency tip of the expected astrophysical gravitational wave spectrum. Many of the most interesting gravitational wave signals will be at much lower frequencies. I will explain several ideas related to the design and scientific application of lower frequency gravitational wave telescopes.

Date: Tuesday, 22 March 2011
Time: 16:00
Where: McGill University
  Ernest Rutherford Physics Building, R.E. Bell Conference Room (room 103)
Contact: Robert Rutledge

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