CRAQLow-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