C. Spiering Hamburg, March 20, 2007 - Desy

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� Radio detection of air showers � Radio detection of showers at the moon � Radio detection of neutrinos in ice or salt � Acoustic detection of neutrinos in water and ice � Detection of cosmic ray & neutrino interactions from space (by fluorescence) � Wide angle Gamma detection � New photosensors � ….
� Ground based Interferometers (here: VIRGO) 10 Hz – 10 kHz � Resonant antennas: ~ 1 kHz � Space based interferometer (LISA): < mHz - 1 Hz
Page 1 and 2: C. Spiering Hamburg, March 20, 2007
Page 3 and 4: � Steering Committee (Funding Age
Page 5 and 6: � February 2007: . „PHASE-I“
Page 8 and 9: IceCube Charged Cosmic Rays GeV-TeV
Page 10 and 11: Interferometers (Geo-600, VIRGO) In
Page 12: - Dark matter: WIMPS direct and ind
Page 15 and 16: - effect from movement through WIMP
Page 17 and 18: Cross section (pb) 10 -4 10 -6 10 -
Page 19 and 20: Spectrum endpoint and ββ , oscill
Page 21 and 22: (A,Z) → (A,Z+2) + 2e - � Neutri
Page 23 and 24: proof/disprove Klapdor test inverte
Page 25 and 26: now 2005 2006 2007 2008 2009 2010 2
Page 27: Soon: Borexino Soon: Borexino ≥ 2
Page 30 and 31: Large Detectors for SN Neutrinos SN
Page 32 and 33: Large Detectors for SN Neutrinos SN
Page 34 and 35: Balloons, PAMELA AMS Kascade-Grande
Page 37 and 38: � Site: Colorado � Estimated co
Page 39 and 40: Not to scale ! Beyond H.E.S.S. and
Page 41 and 42: Distance Pulsed emission Microquasa
Page 43: �Need larger detectors: IceCube,
Page 46 and 47: now 2005 2006 2007 2008 2009 2010 2
Page 51: 3-1000 0.01-3 10 3 -10 5
Page 55 and 56: 2007 2008 2009 2010 2011 2012 2013
Page 57: �From infancy to maturity: the pa
Page 61 and 62: Field/ Experiment Properties of neu
Page 63 and 64: Field/ Experiment High Energy Univ.
Page 65 and 66: Ionization WIMP Smoking guns: Heat
Page 67 and 68: Noble liquids TPC Ionization DRIFT
Page 69 and 70: � Radio detection of air showers:

C. Spiering Hamburg, March 20, 2007 - Desy

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