McGill.CA / Science / Department of Physics

Joint Astrophysics Colloquium

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.

Tuesday, March 22nd 2011, 16:00
Ernest Rutherford Physics Building, R.E. Bell Conference Room (room 103)