Conveners
W2-3 Gravity II (DTP) / Gravité II (DPT)
- Ariel Edery (Bishop's University)
                Prof.
    Nicolas Yunes
        
            (Montana State University)
            
        
                17/06/2015, 13:45
            
        
                    Theoretical Physics / Physique théorique (DTP-DPT)
                
            
                    Invited Speaker / Conférencier invité
                
            
        Einstein's theory has passed all tests to date in the quasi-stationary weak-field, where gravitational dynamics are weak and quadrupolar, while velocities are small relative to the speed of light. The highly non-linear and dynamical regime of the gravitational interaction, however, remains mostly unexplored. The imminent detection of gravitational waves will open a window into this regime that...
                
                
    Ingrid Stairs
        
            (UBC)
            
        
                17/06/2015, 14:15
            
        
                    Theoretical Physics / Physique théorique (DTP-DPT)
                
            
                    Invited Speaker / Conférencier invité
                
            
        Millisecond radio pulsars (MSPs) exhibit tremendous rotational stability and 
therefore provide a means to detect gravitational waves passing near the Earth. 
Three collaborations are using the world's largest radio telescopes to observe 
arrays of MSPs with the goal of making such a detection.  This talk will
review the expected gravitational-wave sources, the methodology and the...
                
                
    Michael Landry
        
            (LIGO Hanford Observatory/Caltech)
            
        
                17/06/2015, 14:45
            
        
                    Theoretical Physics / Physique théorique (DTP-DPT)
                
            
                    Invited Speaker / Conférencier invité
                
            
        Gravitational waves are distortions in the metric of space-time, the detection of which would provide key information on strong gravity and the astrophysical systems that produce them: supernovae, spinning compact stars, and the coalescence of compact binary systems (CBCs).
LIGO is a gravitational wave observatory composed to two 4km interferometric detectors separated by 3000km, in Hanford...
                