1. WORKING GROUP I: PHYSICS Convenors: O. Yasuda, M.Messier, P.Hernández

2.  The usual subjects: completing the 3 scenario Where do we stand ? The next 5 years … The race for precision lepton-flavour physics  Beyond the standard 3 scenario  Neutrinos and dark matter The WG1 agenda

3. Where do we stand ?

4. The next 5 years… First generation Superbeams Reactor experiments:

5. The race for precision neutrino flavour physics T2KK WBB LAr TPC Iron Scintillator

6. Hadron production experiments and beam-systematics

7. Beyond the standard 3  scenario Searching for non-standard neutrino interactions: model independent parametrizations, prospects in present and future neutrino oscillation experiments…

8. News on models of neutrino masses Testing the “standard” see-saw model experimentally ? Synergies with precise measurements of SUSY particle spectrum at LHC, ILC…

9. Neutrinos and dark matter Maybe a rather simple extension of the SM with three singlet Majorana neutrino could explain dark and visible matter ? Spectra from annihilation of dark matter particles in Earth/Sun