Gran Sasso Laboratory: present and future - LIGO

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ICARUS Imaging Cosmic and Rare Underground Signals First Unit T600 T1200 T1200 Liquid Argon (-176 °C) First half of T600 module successfully operated in Pavia Expect to install T600 in 2004 T3000 detector proposed as a series of five T600 modules •Wide physics program •ν τ and ν e appearance on CNGS • atmospheric neutrinos • supernova neutrinos • solar neutrinos • proton decay 17 m Collaboration: Italy, Poland, China Spain, Switzerland, USA
ICARUS T600 Dicember 3, 2004
Page 1 and 2: The Gran Sasso Underground Laborato
Page 4 and 5: 1400 m rock coverage cosmic µ redu
Page 6 and 7: External facilities Administration
Page 8 and 9: Underground Laboratories Canfranc S
Page 10 and 11: COBRA LUNA2 Occupancy LUNA CRESST2
Page 12 and 13: OPERA 2 super-modules 1800 t sensit
Page 16 and 17: GNO 101 tons Gallium Cloride soluti
Page 18 and 19: Borexino Inner vessel installation
Page 21 and 22: LVD Large Volume Detector Running s
Page 23 and 24: Direct Detection Methods Direct Det
Page 25 and 26: Neutrino masses and 0ν2β decay He
Page 29 and 30: Cella et al.
Page 31 and 32: Two-degrees of freedom roto-transla
Page 33: Burst event for a present bar: a mi
Page 37 and 38: D = 4.0 m; f 1 =380 Hz; f 2 =1200 H
Page 39 and 40: Dark Energy 73% (Cosmological Const

Gran Sasso Laboratory: present and future - LIGO

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