APC, Paris - February 13-15, 2008
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Scientific Program
Scientific program
February 13, 2008 | ||
|---|---|---|
| Morning session (09:00-12:00) | ||
| 09:00-09:10 (10') | D. Semikoz | "Welcome" |
| Particle physics candidates | ||
| 09:10-09:45 (30'+5') | L. Roszkowski | "Particle physics candidates for Cold DM" |
| 09:45-10:20 (30'+5') | M. Shaposhnikov | "Particle physics candidates for Warm DM" |
| 10:20-10:40 | Coffee break | |
| Numerical simulations | ||
| 10:40-11:15 (30'+5') | C. Frenk | "Dark matter at small scales: N-body simulations" |
| 11:15-12:00 (40'+5') | S. Colombi J. Devriend |
"CDM versus the rest of the world : what can we believe from cosmological simulations?" |
| 12:00-13:30 | Lunch | |
| Afternoon session (13:30-19:00) | ||
| Numerical simulations | ||
| 13:30-14:10 (35'+5') | A. Maccio' | "WDM simulations" |
| 14:10-14:50 (35'+5') | S. Kazantzidis | "Dark Matter Halo Substructure and Galactic Disks" |
| 14:50-15:25 (30'+5') | L. Gao | "First stars in CDM and WDM" |
| 15:25-15:45 | Coffee break | |
| 15:45-16:25 (35'+5') | T. Naab | "How baryons can change the galaxy formation picture coming from N-body simulations" |
| 16:25-17:00 (30'+5') | M. Joyce | "Discreteness effects in cosmological simulations" |
| 17:00-17:35 (30'+5') | M. Vogelsberger | "Fine-grained phase-space structure of CDM halos" |
| 17:35-19:05 | Discussion | |
| 20:00 | Workshop Dinner
We made reservation in the one of well known Paris restaurants "La Rotonde" for all participants who want to come for common dinner. Please register on the registration page BEFORE February 10 and indicate, if you want to participate in the dinner. Price is 45 Euro per person to be payed in CASH at the registration. | |
February 14, 2008 | ||
| Morning session (09:00-12:00) | ||
| Local halo observations | ||
| 09:00-09:35 (30'+5') | G. Gilmore | "Some observed properties of Dark matter" |
| 09:35-10:10 (30'+5') | M. Walker | "Detailed mass profile studies of dwarf spheroidals" |
| 10:10-10:30 | Coffee break | |
| 10:30-11:05 (30'+5') | E. Lokas | "Mass modelling of dwarf spheroidal galaxies" |
| 11:05-11:40 (30'+5') | S. Koposov | "Luminosity function determination vs. predictions" |
| 11:40-12:15 (30'+5') | V. Belokurov | "Galaxy halo sub-structure" |
| 12:15-14:00 | Lunch | |
| Afternoon session (14:00-19:00) | ||
| Observations | ||
| 14:00-14:35 (30'+5') | L. Strigari | "The Dark Matter Content of Milky Way Satellites" |
| 14:35-15:10 (30'+5') | W. Evans | "Existence of streams - dynamics expectations" |
| 15:10-15:30 | Coffee break | |
| 15:30-16:05 (30'+5') | F. Bournaud | "Do the observation of TDG challenge the standard CDM paradigm?" |
| 16:05-16:40 (30'+5') | M. Capaccioli | "Dark matter content of early-type galaxies" |
| 16:40-17:15 (30'+5') | J. Silk | "Can CDM and galaxy formation be reconciled?" |
| 17:15-18:45 | Discussion | |
February 15, 2008 | ||
| Morning session (09:00-12:00) | ||
| 09:00-09:35 (30'+5') | A. Refregier | "Can the weak lensing discriminate between CDM and WDM?" |
| 09:35-10:10 (30'+5') | L. Bergstrom | "Can gamma-ray probe the nature of dark matter?" |
| 10:10-10:30 | Coffee break | |
| 10:30-11:05 (30'+5') | G. Mamon | "The dark matter content of elliptical galaxies and groups of galaxies" |
| 11:05-11:40 (30'+5') | A. Boyarsky O. Ruchayskiy |
"Constraints on decaying DM" |
| 11:40-12:00 | Discussion | |
| 12:00-14:00 | Lunch | |
| Afternoon session (14:00-19:00) | ||
| Lyman-alpha forest | ||
| 14:00-14:45 (40'+5') | T. Theuns | "Measuring the Lya flux power spectrum: observational status and uncertainties." |
| 14:45-15:30 (40'+5') | M. Viel | "From the flux power spectrum to the linear power spectrum: methods and uncertainties." |
| 15:30-15:50 | Coffee break | |
| 15:50-16:35 (40'+5') | J. Lesgourgues | "Constraining WDM observables with Lyman-alpha" |
| 16:35-18:00 | Discussion and concluding remarks | |
