Neutrino physics with an opaque detector

Neutrino Physics Inside SK detector

The non-zero mass difference square of three generations of neutrino has already been verified in the K2K experiment conducted in Japan. But we still need more experimental data to have more accurate results about neutrinos. New generation of neutrino experiments are being built up in all over the world. Here I would like to present some Monte Carlo results using a special neutrino beam passing...

Neutrino physics and astrophysics with the MACRO detector

After a brief presentation of the MACRO detector we discuss the data on atmospheric neutrinos and neutrino oscillations, on high energy (Eν > 1 GeV) neutrino astronomy, on indirect searches for WIMPs and low energy (Eν > ∼ 7 MeV) stellar collapse neutrinos.

Neutrino Physics: an Update

We update our recent didactic survey of neutrino physics, including new results from the Sudbury Neutrino Observatory and KamLAND experiments, and recent constraints from WMAP and other cosmological probes.

Neutrino astronomy: physics goals, detector parameters, OECD workshop

Neutrino Physics: an Experimental Overview

Neutrinos are now known to have mass and to mix. It is still not known exactly how they fit into the theoretical picture, however. In the baseline Standard Model, neutrinos are massless, and extensions to the Standard Model are required to explain their small masses and the observed oscillation phenomena. These observations can be accommodated in GUTs, and perhaps more exotic scenarios such as ...