DUSEL and UNO - Stony Brook NN Group

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DUSEL Candidate Sites and Potential LBL/Superbeam Experiments J. Wilkes, 28 Oct '05 Homestake Henderson 1315 km 1500 km 2760 km 730 km 2560 km FNAL BNL 30
Why VLBL? J. Wilkes, 28 Oct '05 • Marciano pointed out that for HE neutrino beams, 2nd and 3rd oscillation dips can be very handy... neutrino, max CP δ antineutrino M. Diwan, B. Viren 31
Page 1 and 2: DUSEL (U.S. Deep Underground Scienc
Page 3 and 4: J. Wilkes, 28 Oct '05 DUSEL: Deep U
Page 5 and 6: J. Wilkes, 28 Oct '05 DUSEL Candida
Page 7 and 8: Henderson Underground Science/Engin
Page 9 and 10: J. Wilkes, 28 Oct '05 Henderson Min
Page 11 and 12: J. Wilkes, 28 Oct '05 Henderson Min
Page 13 and 14: J. Wilkes, 28 Oct '05 Deep Access C
Page 15 and 16: UNO Detector Concept Water Cherenko
Page 17 and 18: J. Wilkes, 28 Oct '05 UNO Collabora
Page 19 and 20: UNO Physics Goals J. Wilkes, 28 Oct
Page 21 and 22: J. Wilkes, 28 Oct '05 Supernovae UN
Page 23 and 24: J. Wilkes, 28 Oct '05 Diffuse super
Page 25 and 26: UNO Design and Construction Timelin
Page 27 and 28: J. Wilkes, 28 Oct '05 Aspen Center
Page 29: J. Wilkes, 28 Oct '05 SALTA’s und
Page 33: J. Wilkes, 28 Oct '05 Now and near

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