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11/07/2006, 08:30After a brief summary of the evolution of cosmological perturbation in the Friedmann universe, I will show why neutrinos are expected to leave a signature in the spectrum of CMB anisotropies and in the distribution of large scale structures. I will present current cosmological bounds on neutrino physics, based on various types of cosmological observations. Finally, I will intruduce the...Go to contribution page
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11/07/2006, 10:45The quest for the very fundamental mysteries of nature by exploring the smallest scales and highest energies at particle colliders requires a huge technological and intellectual effort. While many people think this is a purely intellectual exercise for some crazy super-brains without any impact on society, the spin-offs from High Energy Physics research actually has and will have a...Go to contribution page
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