radio lobe sound disk t p optical light cone The Vision *) see e.g. A. Ringwald ,ARENA 2005 Build ~100 km 3 hybrid detector to: Confirm GZK cutoff ! Do physics with extremely high energy cosmic neutrinos *) - astrophysics - E > 10 16 eV : study origin of cosmic rays - (AGN’s, black holes, GZK cutoff, …) - particle physics - E > 10 18 eV : study neutrino cross section (sphalerons, mini BH, strong ,…) - cosmology - E > 10 21 eV : study relic neutrino background radiation (UHE absorption at CBR )
~ km. sound disk. p. t. radio lobe. The Vision. Build ~100 km 3 hybrid detector to: Confirm GZK cutoff ! Do physics with extremely high energy cosmic neutrinos *) - astrophysics - E > 10 16 eV : study origin of cosmic rays - (AGN’s, black holes, GZK cutoff, …) - PowerPoint PPT Presentation
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radio lobe
sound disk
t
p
optical light cone
The Vision
*) see e.g. A. Ringwald ,ARENA 2005
Build ~100 km3 hybrid detector to:
Confirm GZK cutoff !
Do physics with extremelyhigh energy cosmic neutrinos*)
- astrophysics - E > 1016eV : study origin of cosmic rays - (AGN’s, black holes, GZK cutoff, …)
- particle physics - E > 1018eV :study neutrino cross section (sphalerons, mini BH, strong,…)
- cosmology - E > 1021eV : study relic neutrino background radiation (UHE absorption at CBR )
Acoustic R&D in IceCube 2002 2003 2004 2005 2006 2007