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:	Mardi, le 22 mars 2011
Heure:	16:00
Lieu:	Université McGill
	Ernest Rutherford Physics Building, R.E. Bell Conference Room (room 103)
Contact:	Robert Rutledge