Supported by
- National Science Foundation
- SUPA
- IOP Gravitational Physics Group
- Institute for Gravitational Research, University of Glasgow
- Center for Relativistic Astrophysics, Georgia Tech
Useful links
Program
Monday 28th May
Gamma-Ray Bursts
| Time | Speaker | Title |
|---|---|---|
| 8:45-9:00 | Laguna | Opening Remarks |
| 9:00-10:00 | Kobayashi & Tanvir | Mano-a-Mano |
| 10:00-10:30 | Break | |
| 10:30-10:50 | O'Brien | Are Gamma-Ray Bursts powered by magnetars? |
| 10:50-11:10 | Sutton | Searching for GWs Associated with GRBs |
| 11:10-11:30 | Kobayashi | Short GRBS: Observational links to stellar mergers or/and as EM counter parts |
| 11:30-12:00 | O'Brien | Summary Discussion |
| 12:00-2:00 | Lunch |
Modeling Compact Object Binaries
| 2:00-3:00 | Shoemaker & Liebling | Mano-a-Mano |
| 3:00-3:30 | Break | |
| 3:30-3:50 | Bernuzzi | Gravitational waves from binary neutron star mergers: tidal signatures and accuracy of the simulations |
| 3:50-4:10 | Johnson-McDaniel | Numerical simulations of eccentric neutron star binaries |
| 4:10-4:30 | Favata | Gravitational-wave bursts with memory |
| 4:30-5:00 | Neilsen | Summary Discussion |
Tuesday 29th May
Data Analysis & Instrumentation
| Time | Speaker | Title |
|---|---|---|
| 9:00-10:00 | Cadonati & Finn | Mano-a-Mano Discussion |
| 10:00-10:30 | Break | |
| 10:30-10:50 | Klimenko | Inverse problem for transient gravitational waves |
| 10:50-11:10 | Rodriguez | Fisher Matrix Usefulness in the advanced-detector era |
| 11:10-11:30 | Hild | Sensitivity scenarios and calibration accuracy of future GW detectors |
| 11:30-12:00 | Marka | Summary Discussion |
| 12:00-2:00 | Lunch | |
| 2:00-5:00 | Distillery Tour | |
| 6:30-late | Banquet |
Wednesday 30th May
Isolated Neutron Stars
| Time | Speaker | Title |
|---|---|---|
| 9:00-10:00 | Andersson & Kokkotas | Mano-a-Mano Discussion |
| 10:00-10:30 | Break | |
| 10:30-10:50 | Clark | Gravitational Waves From F-modes in Rotating Neutron Stars: Morphology & Parameter Space |
| 10:50-11:10 | Santiago-Prieto | Transient GWs at r-mode frequencies associated with pulsar glitches and super bursts in millisecond pulsars |
| 11:10-11:30 | ||
| 11:30-12:00 | Heng | Summary Discussion |
| 12:00-1:00 | Lunch |
Core-collapse Supernova
| 1:00-2:00 | Sutton & Reisswig | Mano-a-Mano Discussion |
| 2:00-2:30 | Break | |
| 2:30-2:50 | Reisswig | Neutrino and GW Signatures of Stellar Core Collapse |
| 2:50-3:10 | Logue | Inferring Core-Collapse Supernova Physics with GWs |
| 3:10-3:30 | Cerda-Duran | Gravitational waves in the Fully Constrained Formalism |
| 3:30-4:00 | Summary Discussion | |
| 4:00-4:15 | Laguna | Final Remarks |
Contact us by email at gwb-soc [at] gwbursts.org