Solar Neutrino Session

Tuesday, 17 December 1996, 4:15-6:15 pm

Preliminary Program

Chair: V. Berezinsky (Gran Sasso)

If you have any queries or comments on the program please email: berezinsky@lngs.infn.it

Speakers

4:15 D.Cowen (Sudbury Neutrino Observatory) The Design and Status of the Sudbury Neutrino Observatory (15 min)
4:30 J.Christensen-Dalsgaard (Aarhus University, Denmark), Helioseismology and Solar Neutrinos (20 min)
4:50 S.Vauclair (Obsevatoire Midi- Pyrenees, France) Solar Models Including Element Diffusion and Partial Mixing: the Helioseismic Constraints on the Solar Neutrino Fluxes (10 min)
5:00 T.Stanev (Bartol Research Institute) Time Variation of Solar Neutrino Flux and its Correlation with Solar phenomena (20 min)
5:20 M.Lissia (University of Cagliari, Italy) Is there a time variation of the Homestake neutrino flux? (10 min)
5:30 G.Fiorentini (University of Ferrara, Italy) Progress in Standard Solar Models (15 min)

Posters

C.Y.Cardall (UCSD), Can a natural three generation neutrino mixing scheme satisfy everything?
J.Weber (Maryland), Observations of the solar neutrinos with a coherent scattering detector
J.Beacom (Wisconsin), Semiclassical treatment of matter enhanced neutrino oscillations for an arbitrary density profile
N.J.Shaviv (Caltech) and G.Shaviv , Extremely significant corrections to the plasma screening of nuclear reactions