6–11 Dec 2010
CNR headquarter
Europe/Rome timezone

Session

Cosmology and astroparticles, dark matter (2)

9 Dec 2010, 17:00
CNR headquarter

CNR headquarter

Piazzale Aldo Moro, 7 00185 Roma

Presentation materials

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  1. Dr Roberta Sparvoli (University of Rome ”Tor Vergata”, and INFN Section of Rome ”Tor Vergata”, Rome, Italy)
    09/12/2010, 17:00
    After four years of data taking in space, the experiment PAMELA is showing very interesting features in cosmic rays that might change our basic vision of their mechanisms of production, acceleration and propagation in the galaxy. In addition, PAMELA measurements of cosmic antimatter fluxes are setting strong constraints to the nature of Dark Matter. In this talk PAMELA main results will be...
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  2. Prof. Isabella Masina (Ferrara University and CP3-Origins)
    09/12/2010, 17:25
    Cosmology and astroparticles, dark matter searches
    We introduce new sum rules allowing to determine universal properties of the unknown component of the cosmic rays and show how they can be used to predict the positron fraction at energies not yet explored by current experiments and to constrain specific models.
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  3. Prof. Federico Palmonari (INFN and University, Bologna)
    09/12/2010, 17:50
    Cosmology and astroparticles, dark matter searches
    The growing observational evidence for Dark Matter from astrophysical observations gives a solid base to the Cosmological Standar Model. On the other side, the Standard Model of particles and interactions has no answer on DM nature. Experimental evidence of DM from underground experiments is under scrutiny while recent results from space experiments have no clear interpretation. The...
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  4. Dr Maurice LALOUM (retired CNRS/IN2P3/LPNHE Paris)
    09/12/2010, 18:15
    Cosmology and astroparticles, dark matter searches
    Many essential paradoxes in the mechanical balance of the Galaxy are highlighted. We propose a unique and synthetic interpretation, including a cosmological theory of the origin of the observed cosmic rays, especially at the highest energies. It involves MATTER-ANTIMATTER ANNIHILATION in the median plane of the Milky Way, as a source of "DARK MATTER". We discuss the structure and balance of...
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