05/07/2001
A. Bettini 2001
1
Summary
1. History and present status
2. Status of the (new) neutrino physics
3. How LNGS contributed
4. How LNGS can contribute in the future?
Neutrinos from artificial sources
Neutrinos from the atmosphere
Neutrinos from the Sun
Neutrinos from Supernovae
5. Neutrino mass
6. Search for non baryonic dark matter
7. Other European Facilities
LSM
LSC
Boulby
CUPP
8. Interactions with the environment
9. Conclusions 
Snowmass Workshop
 A. Bettini July 3 2001
Status and Perspective of the (new) Physics ay Gran Sasso National Laboratory and in the other European Underground Facilities