Deadline: 15-12-2008

Note: Attendance will be limited to about 80 participants who are supposed to arrange their accommodation by themselves. (take a look to hotel list at accommodation link).

Contact:

The conference will be devoted to the discussion of new data and ideas associated with astrophysical and cosmological evidence for Dark Matter. Several key questions on dark matter will be discussed: Does the dark matter match the appropriate relic density? Is it cold or hot ? Is it neutral? Is it consistent with Big Bang Nucleosynthesis ? Is it compatible with constraints on self-interactions ? Is it consistent with direct DM searches? Is it compatible with gamma-ray constraints? Is it compatible with other astrophysical bounds? Can it be probed experimentally? What is the mass of the neutrino and how many neutrinos or relativistic particles do we have in our universe ? More specifically, several talks will review the current status of cosmological and astrophysical evidence for dark matter. In particular, we will focus on new lensing observations, galaxy clustering, X-rays, gamma-rays, antimatter with space-borne detectors and direct DM detection in low background underground experiments. We plan to address the main theoretical extensions of the standard model which allow to explain dark matter and the corresponding predictions for future searches. Special attention will be given on the requirements for collider tests of dark matter candidates at LHC. Constraints on neutrino physics can be obtained from cosmological data. During the workshop, we aim to summarize the latest bounds on neutrino physics and discuss future experiments sensitive to neutrino masses into the sub-eV range.