'Interacting dark matter' presentation slideshows

La Cristalera, Spain June 2008

557 views • 55 slides

P. Belli INFN-Roma Tor Vergata

First results from DAMA/LIBRA. SLAC July 1st, 2008. P. Belli INFN-Roma Tor Vergata. Relic DM particles from primordial Universe. axion-like (light pseudoscalar and scalar candidate). SUSY (as neutralino or sneutrino In various scenarios). self-interacting dark matter.

665 views • 52 slides

P. Belli INFN-Roma Tor Vergata

First results from DAMA/LIBRA. FERMILAB June 27th, 2008. P. Belli INFN-Roma Tor Vergata. Roma2,Roma1,LNGS,IHEP/Beijing. + by-products and small scale expts.: INR-Kiev + neutron meas.: ENEA-Frascati + in some studies on bb decays (DST-MAE project): IIT Kharagpur, India.

649 views • 52 slides

NO-VE Int. Conf. Venezia, 15-17 Aprile 2008

635 views • 51 slides

NO-VE Int. Conf. Venezia, 15-17 Aprile 2008

515 views • 51 slides

Particle Dark Matter in the galactic halo

635 views • 50 slides

F. Nozzoli INFN-Univ. Roma Tor Vergata

Detection of Dark Matter and perspectives. F. Nozzoli INFN-Univ. Roma Tor Vergata. Matalasca ñ as September 2007. Relic DM particles from primordial Universe. Heavy candidates:. Light candidates:. In thermal equilibrium in the early stage of Universe Non relativistic at decoupling time:

576 views • 47 slides

The Cosmological Model: an overview and an outlook

The Cosmological Model: an overview and an outlook. Alan Heavens University of Edinburgh. The Standard Cosmological Model. Universe started with Big Bang Einstein gravity CDM, baryons, photons (++) Cosmological Constant Inflation adiabatic, near-gaussian fluctuations. Evidence.

817 views • 42 slides

Chandra Science Highlight

Chandra Science Highlight. Abell 2029: A cluster of galaxies one billion light years from Earth in the constellation Serpens.

203 views • 1 slides