Chalonge de Vega Meudon Workshop 2016

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Ecole Internationale Daniel Chalonge - Héctor de Vega Chalonge de Vega Meudon Workshop 2016 Warm Dark Matter Astrophysics in agreement with observations and kev Sterile neutrinos Observatoire de Paris, CIAS Château de Meudon, Meudon campus, 15, 16 and 17 JUNE 2016 All Sessions of the Workshop take place in the historic Castle building (CIAS, Château de Meudon) Observatoire de Meudon ENTRY: 5 Place Jules Janssen, 92195 Meudon. Entry for cars: 11 Avenue Marcelin Berthelot, 92195 Meudon

Sessions start at the indicated times sharp 1 HOUR = 45 minutes lecture + 15 minutes discussions WEDNESDAY 15 JUNE MORNING 8.00 9.30: URANIA HALL (in the Château building) REGISTRATION, badges, lunch tickets for the Observatoire Restaurant, copies of the full Time Table with Lectures and Lecturers. «SALLE DE CONFERENCES DU CHATEAU» 9.45 10:00 Welcome Address 10.00 11.00 Peter BIERMANN (MPI-Bonn, Germany & Univ of Alabama, Tuscaloosa, USA) Warm Dark Matter, Supermassive black holes and black hole mergers 11.00 11.30 COFFEE-TEA BREAK at URANIA HALL, in Château building 11.30 12.30 Work with Héctor J. DE VEGA on Warm Dark Matter Norma G. SANCHEZ (CNRS LERMA Observatoire de Paris, Paris, France) 12.30 14.00 LUNCH at the Observatoire Restaurant (Meudon campus around the lac near the Château building)

WEDNESDAY 15 JUNE AFTERNOON 14.00 15.00 Sinziana PADUROIU (Observatoire de Geneve, Switzerland) Warm Dark Matter Cosmology: Numerical Simulations on Structure Formation 15.00 16.00 Thierry LASSERRE (CEA, IRFU-Saclay, France) A Status Report on Sterile Neutrino experiments and the kev case 16.00 17.00 COFFEE-TEA BREAK at URANIA HALL, 17.00 18.00 Anton HUBER (KIT, Karlsruhe Institute of Technology, Karlsruhe, Germany) The Status of the kev-scale sterile neutrino search with KATRIN

THURSDAY 16 JUNE MORNING 10.00 11.00 Eloisa MENEGONI (University of Roma I, Rome, Italy) Constraints on fundamental physics from CMB data and galaxy clustering 11.00 11.30 COFFEE TEA BREAK at URANIA HALL 11.30 12.30 Daniel MAIER (Service d'astrophysique CEA-Saclay, Gif-sur-Yvette, FRANCE) X-Ray Astronomy and the search for kev sterile neutrino signatures 12.30 14.00 LUNCH at the Observatoire Restaurant (Meudon campus around the lac, near the Château building)

THURSDAY 16 JUNE AFTERNOON 14.00 15.00 Nicola MENCI (INAF, Osservatorio di Roma, Roma, Italy) Warm Dark Matter Astrophysics: Galaxy and Star formation and kev sterile neutrino mass constraints 15.00 16.00 Pier-Stefano CORASANITI (CNRS LUTH Observatoire de Paris, Meudon, France) Non-linear small scale structure formation in non-standard cosmologies 16.00 17.00 COFFEE-TEA BREAK at URANIA HALL 17.00 18.00 Loredana GASTALDO (Kirchhoff Institute for Physics KIP, Univ Heidelberg, Germany) The Status of the ECHO experiment for the investigation of kev sterile neutrinos. 18.00 19.00 Isabella P. CARUCCI (SISSA- Astrophysics, Trieste, Italy) Exploiting the 21cm power spectrum: forecasts for SKA on the Warm Dark Matter

FRIDAY 17 JUNE MORNING 10.00 11.00 Marco LOMBARDI (Dept. of Physics, University of Milano, Italy) Dark Matter Searches with Gravitational Lensing 11.00 11.30 COFFEE TEA BREAK at URANIA HALL in Château building PHOTO OF THE GROUP (in the Urania Hall facade) 11.30 12.30 Paolo SALUCCI (SISSA-Astrophysics, Trieste, Italy) The observed structural properties of Galaxies and cored density profiles lead to Warm Dark Matter 12.30 14.00 LUNCH BREAK at the Observatoire Restaurant (Meudon campus around the lac, near the Château building)

FRIDAY 17 JUNE AFTERNOON «SALLE DE CONFERENCES DU CHATEAU» 14.00 15.00 Norma G. SANCHEZ (CNRS LERMA Observatoire de Paris,Paris, France) Warm Dark Matter 15.00 16.00 All participants: General Discussion on the present and future of the scientific research on Dark Matter and Galaxies 16.00 16.30 The Héctor J. de Vega Medal 16.30 17.00 COFFEE-TEA- BREAK at URANIA HALL 17.00 18.00 Visit inside the Chateau building 18.00 20.00 APERITIF/COCKTAIL at URANIA HALL in Château building for all participants and accompanying persons. All Lecturers and participants are expected to remain untill the end of the Workshop END OF THE WORKSHOP