Name | Organization | Talk | Begin | End | Student |
|
|
Breakfast and Registration |
8:00 |
8:55 |
|
Jim Isenberg |
University of Oregon |
Welcome and Announcements |
8:55 |
9:00 |
|
Detournay Stephane |
UC Santa Barbara |
Three-dimensional gravities and black hole entropy |
9:00 |
9:12 |
|
Sophie de Buyl |
UC Santa Barbara |
Asymptotic infinite dimensional symmetry of gravity duals for non-relativistic CFTs |
9:12 |
9:24 |
|
Tomas Andrade |
UC Santa Barbara |
Stability Analysis of Topologically Massive Gravity in three dimensions |
9:24 |
9:36 |
|
Derek Wise |
UC Davis |
Topologically Massive AdS Gravity |
9:36 |
9:48 |
|
Colin Cunliff |
UC Davis |
What happens in 3D gravity at the chiral point? |
9:48 |
10:00 |
|
Usama al-Binni |
University of Tennessee |
Particle emission from a black hole on a tense codimension-2 brane |
10:00 |
10:12 |
|
Matthew West |
Syracuse University |
eLIGO Photon Pressure Calibration |
10:12 |
10:24 |
|
|
|
Coffee Break |
10:24 |
11:00 |
|
Name | Organization | Talk | Begin | End | Student |
Harald Pfeiffer |
Caltech |
Comparing post-Newtonian binary black hole waveforms to numerical relativity simulations |
11:00 |
11:12 |
|
Tony Chu |
Caltech |
Simulations of Spinning (Non-Precessing) Binary Black Holes with SpEC |
11:12 |
11:24 |
|
Lee Lindblom |
Caltech |
Improved Gauge Drivers for the Generalized Harmonic Einstein Equations |
11:24 |
11:36 |
|
Bela Szilagyi |
Caltech |
Numerical Simulations of Binary Black Hole Mergers |
11:36 |
11:48 |
|
Jim Bardeen |
University of Washington |
Trumpet Boundary Conditions for CMC Black Hole IVPs |
11:48 |
12:00 |
|
Luisa T. Buchman |
Caltech |
Black hole initial data to future null infinity |
12:00 |
12:12 |
|
Charles Torre |
Utah State University |
Algebraic Computing Tools for Gravitational Physics |
12:12 |
12:24 |
|
Sydney Chamberlin |
Utah State University |
Algebraic Computing Tools in Gravitational Physics |
12:24 |
12:36 |
|
|
|
Lunch |
12:36 |
2:00 |
|
Name | Organization | Talk | Begin | End | Student |
Jeandrew Brink |
Caltech |
Whetting the appetite for understanding strong field Binary Collisions |
11:00 |
11:12 |
|
Mark Scheel (for Kip Thorne) |
Caltech |
Flat-Spacetime Field Theory and Momentum Flow in Black-Hole Binaries |
11:12 |
11:24 |
|
Jeff Kaplan |
Caltech |
Post-Newtonian Approximation in a Maxwell-Like Form for Use in Interpreting
Binary-Black-Hole Simulations |
11:24 |
11:36 |
|
David Nichols |
Caltech |
Momentum Flow in Black-Hole Binaries: Post-Newtonian Approximation |
11:36 |
11:48 |
|
Mark Scheel |
Caltech |
Momentum flow in binary black hole collisions: numerical results |
11:48 |
12:00 |
|
Keith D. Matthews |
Caltech |
Harmonic Initial Data for Post-Newtonian Comparison |
12:00 |
12:12 |
|
Tanja Hinderer |
Caltech |
Transition from inspiral to plunge:
Progress on an improved treatment |
12:12 |
12:24 |
|
|
|
Lunch |
12:24 |
1:48 |
|
Name | Organization | Talk | Begin | End | Student |
David Yeaton-Massey |
Caltech |
From IR to Green: Measuring Doubling Noise |
2:00 |
2:12 |
|
Nicolas Smith |
MIT |
Enhanced LIGO: Output Mode Cleaner and DC Interferormeter Locking |
2:12 |
2:24 |
|
Emelie Harstad |
University of Oregon |
An expanded search for GW bursts in association
with GRBs |
2:24 |
2:36 |
|
Tyson Littenberg |
Montana State University |
A Bayesian Approach to the Detection Problem in Gravitational Wave Astronomy |
2:36 |
2:48 |
|
Joey Key |
Montana State University |
Characterizing the Gravitational Wave Signature from Cosmic String Cusps |
2:48 |
3:00 |
|
Matthew Adams |
Montana State University |
Discriminating between a Stochastic Gravitational Wave Background and Instrument Noise |
3:00 |
3:12 |
|
Joseph Plowman |
Montana State University |
Constraining the Black Hole Mass Spectrum with Gravitational Wave Observations |
3:12 |
3:24 |
|
Michael Cohen |
Caltech |
Mock Lisa Data Challenge 3 - Finding Cosmic Strings with Markov Chain Monte Carlo Methods |
3:24 |
3:36 |
|
|
|
Coffee Break |
3:36 |
4:06 |
|