Developing techniques for solving
the initial value problem for astrophysically relevant initial data
(including compact binaries).
Formulating the evolution equations of general relativity in a manner that can facilitate the construction of stable numerical evolution schemes for spacetimes containing compact objects (and in particular black holes).
Organizers: Miguel Alcubierre, Bernd Bruegmann, Michael Holst, Luis Lehner, and Mark Scheel.
Quasi-adiabatic approximation techniques for evolving nearly circular compact binaries (binaries made of neutron stars and/or black holes).
Organizers: Thomas Baumgarte and Masaru Shibata.