Working Group Form/Schedule

Note: "Round table" discussion means that various participants can have the floor, for, say, 5 minutes to push a given experiment, argue for a theory initiative, etc. Then the other participants should ask the hard questions, provide a reality check, etc.

"Discussion" resignates the final working group meeting in which the convenors and participants try to decide which experiments should be pushed now; which ones require more R&D and development, but are promising; etc. The goal should be to formulate a timeline and process that the DOE/NSF could adopt to "grow" and nurture this physics.

The sessions are staggered a bit to allow participants to attend more than one working group.

September 21	1:45-3:30	4:00-5:45
room A118	Solar Neutrinos Round Table Presentations	Solar Neutrinos Round Table Presentations
room C520	Supernova Neutrinos, the Supernova Mechanism, and Related Astrophysics Round Table Presentations	Underground Laboratories (including atmospheric and high energy neutrinos) Round Table Presentations
room C421	Reactor and Accelerator Neutrinos Round Table Presentations	Neutrino Mass Round Table Presentations
September 22	2:15-4:00	4:30-6:15
room A118	Supernova Neutrinos, the Supernova Mechanism, and Related Astrophysics Round Table Presentations	Solar Neutrinos Discussion
room C520	Reactor and Accelerator Neutrinos Discussion	Supernova Neutrinos, the Supernova Mechanism, and Related Astrophysics Discussion
room C421	Underground Laboratories (including atmospheric and high energy neutrinos) Discussion	Neutrino Mass Discussion

Schedule

September 21
8:15	Introduction: Wick Haxton and Hamish Robertson, Washington explosion of interest in neutrinos possible strategies for neutrinos and the LRP connections between RIA and neutrino physics intersections among NP, HEP, astrophysics funding profiles and manpower in neutrino physics
8:30	A. Baha Balantekin, Wisconsin: Status of the Neutrino Problems 25+10 min.
9:05	Bob Lanou, Brown: The Next Generation of Solar Neutrino Detectors 25+10 min.
9:40	Tony Mezzacappa, ORNL: Toward a Standard Model of Core-Collapse Supernovae 25+10 min.
10:15-10:40	Break
10:40	John Beacom, Fermilab: The Supernova Watch: Possibilities for Supernova Neutrino Observatories 25+10 min.
11:15	Petr Vogel, Caltech: Future Possibilities for Neutrinoless Double Beta Decay Measurements 25+10 min.
11:50	Christian Weinheimer, Mainz: Direct Neutrino Mass Measurements 25+10 min.
12:30-1:45	Lunch
1:45-5:45	Working groups
6:00 -	Dinner at Faculty Club
September 22
8:30	Bill Louis, LANL, Gerry Garvey, Los Alamos: Accelerator Neutrino Opportunities 25+10 min.
9:05	Frank Avignone, Univ. South Carolina/ORNL and Michael Strayer, ORNL: ORLAND 25+10 min.
9:40	Todd Haines, LANL: Underground Laboratories 35+10 min.
10:25-10:45	Break
10:45	Peter Parker, Yale: Astrophysics with RIA 25+10 min.
11:20	George Fuller, UCSD: Big Bang and Supernova Constraints on Neutrino Physics 25+10 min.
11:55	Chang Kee Jung, SUNY Stony Brook: UNO 20+10 min.
12:25	Bob Bernstein, FNAL: The Neutrino Factory 20+10 min.
1:00-2:15	Lunch
2:15-6:15	Working Groups
September 23
9-9:35	Hamish Robertson, Washington: Solar Neutrino Working Group conclusions
9:35-10:10	Ken Lande, Pennsylvania: Supernova Neutrinos, the Supernova Mechanism, and Related Astrophysics conclusions
10:10-10:45	Stuart Freedman, UC Berkeley/LBNL: Reactor and Accelerator Neutrinos conclusions
10:45-11:15	Break
11:15-11:50	Kevin Lesko, LBNL: Underground Laboratories (including atmospheric and high energy neutrinos) conclusions
11:50-12:25	Wick Haxton, Washington: Neutrino Mass conclusions
12:30-2:00	Break
2:00-3:00	Discussion of priorities and strategies (refer back to issues listed in introduction)
3:00-...	Convenors/Organizers meeting

Plenary Session Chairs
Sept. 21	8:30-10:15	Dave Arnett
	10:40-12:30	Alejandro Garcia
Sept. 22	8:30-10:25	Fred Bertrand
	10:45-1:00	Gerry Garvey
Sept. 23	9:00-10:45	Frank Calaprice
	11:15-12:25	Yong Qian