The Chalonge School 16th Paris Cosmology Colloquium 2012,The New Standard Model of the Universe:Lambda Warm Dark Matter.Theory and Observations.

The Chalonge School 16th Paris Cosmology Colloquium 2012,The New Standard Model of the Universe:Lambda Warm Dark Matter.Theory and Observations. The Chalonge School 16th Paris Cosmology Colloquium 2012,The New Standard Model of the Universe:Lambda Warm Dark Matter.Theory and Observations.
  • Contact

    Professor Dr Norma G. Sanchez
    Ecole Daniel Chalonge, Observatoire de Paris & CNRS
    LERMA, 77, Avenue Denfert Rochereau, 75014 Paris, 75014 Paris, FRANCE, 75 0 14
    phone: 00 33 1 40 51 20 07
    fax: 00 33 1 40 51 20 02

  • Working language

    English

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  • Observational and theoretical progress on the nature of dark matter : keV scale warm dark matter
  • Cored density profiles in agreement with observations.
  • Large and small scale structure formation in agreement with observations at large scales and small (galactic) scales.
  • Warm (keV scale) dark matter from theory and observations.
  • Warm (keV scale) dark matter N-body simulations in agreement with observations.
  • Neutrinos in astrophysics and cosmology.
  • The new serious dark matter candidate: Sterile neutrinos at the keV scale.
  • Neutrinos mass bounds from cosmological data and from high precision beta decay experiments.
  • Dark energy: cosmological constant: the quantum energy of the cosmological vacuum.
  • The analysis of the CMB+LSS+SN data with the effective (Ginsburg-Landau) effective theory of inflation: New Inflation (double well inflaton potential) strongly favored by the CMB + LSS + SN data.
  • The presence of the lower bound for the primordial gravitons (non vanishing tensor to scalar ratio r) with the present CMB+LSS+SN data.
  • CMB news and polarization. Forecasts and Planck results.
  • and Other Topics.

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