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Experimental Astroparticle Physics

Experimental Astroparticle Physics. IceCube (Wisconsin) 4 faculty (Evenson, Gaisser , Seckel, Stanev), 1 senior scientist (Clem), 2 Associate Scientists (Bai, Tilav), 2 “LTR” (Stoyanov, Niessen) , 1 GS (Swarnkar), 3 technical staff (Shulman, Roth, McDermott)

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Experimental Astroparticle Physics

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  1. Experimental Astroparticle Physics • IceCube (Wisconsin) • 4 faculty (Evenson, Gaisser, Seckel, Stanev), 1 senior scientist (Clem), 2 Associate Scientists (Bai, Tilav), 2 “LTR” (Stoyanov, Niessen) , 1 GS (Swarnkar), 3 technical staff (Shulman, Roth, McDermott) • HE Neutrino Astronomy (100 GeV – 100 PeV) • SPASE (UD-BRI) • Bai, Evenson, Gaisser, Stanev, Tilav • Cosmic Ray Composition (w/AMANDA) • AMANDA • Bai, Gaisser, Stanev, Tilav • HE Neutrino Astronomy • ANITA (Hawaii) • Clem, Evenson, Seckel • UHE Neutrino Astronomy (> 10 PeV) • RICE (Kansas) • Seckel • UHE Neutrino Astronomy

  2. Surface Array: IceTop Where’s the n muon ? Deep Array: InIce ~15 m To DAQ Drill Hole Two DOMs: 10” PMT LG HG HG LG IceCube (IceTop) • IceCube Science Astrophysical n’s New Physics (100 GeV - 10 PeV) Detection Muons & Cascades 5000 PMTs Program 22 instiutions $ 300M (250 US) 7 + 5 yr • IceTop Science Surface Veto/Tag Calibration Cos-ray science Detection Muons & Showers 80 stations Program Integral part of IceCube UD-BRI lead ~ $1M/yr

  3. 600 m Radio: ANITA & RICE • ANITA: Pathfinding mission for balloon-borne neutrino telescope • NASA SR&T start 2003, LDB launch in 2006-07 • Survey Flight ANITA-Lite 2003-04 • RICE – Antenna array located in AMANDA holes GZK neutrinos

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