The plan is to have two sessions, from 15h - 19h, with one coffee/tea intermission, and about 1/4 to 1/3 of the entire time for discussion. Now we have a quantitative proposal of what dark matter is, and the challenge is to work through the consequences, for particle physics and cosmology, for large scale structure formation, for galaxy formation and galaxy structure, for the first stars, for supernova physics, the interstellar medium, the growth of black holes and active galactic nuclei, primordial magnetic fields, and other aspects. The session will address these questions. |
![]() ![]() |
The list of confirmed speakers is (status on June 8, 2006): Fred Baganoff (Cambridge, US) Peter L. Biermann (Bonn, Germany) George Fuller*(San Diego, US) Laszlo Gergely (Szeged, HU) Gerry Gilmore (Cambridge, UK) Philipp P. Kronberg (Toronto, Canada) Michela Mapelli (Trieste, Italy) Faustin Munyaneza (London, UK) Signe Riemer-Sorensen (Copenhagen, DK) Emanuele Ripamonti (Groningen, NL) Oleg Ruchayskiy (Bures-sur-Yvette, France) Ina Sarcevic*(Arizona, US) Mikhail Shaposhnikov (Lausanne, Switzerland) Anze Slosar (Ljubljana, Slovenia) Jaroslaw Stasielak (Cracow, Poland) Casey R. Watson (Ohio, US) |