Auger North - Fermilab Center for Particle Astrophysics

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Determine Source Distribution! Type of Sources – acceleration models! Brightest Source Spectrum – acc. models! Test shower properties of primaries ! > 100 TeV (>335 TeV): Protons? Iron? ! Predict Cosmogenic (GZK) HE Neutrino & Photon Flux – test interactions > 1 TeV! Constrain Cosmic Magnetic Fields !
Exposure Evolution
Page 1 and 2: The Pierre Auger Observatory Auger
Page 3 and 4: To Discover UHECR Sources ! need:!
Page 5 and 6: Auger South!
Page 7 and 8: Auger South! Observed the GZK featu
Page 9 and 10: Attenuation length! e + e - π Atte
Page 11 and 12: Horizons:! 10 19 eV ~ 1 Gpc! 100 Mp
Page 14 and 15: Recent Auger Spectrum!
Page 18 and 19: Auger VCV correlation! 27 events te
Page 20 and 21: First 27 events!
Page 22 and 23: UHE neutrino limit!
Page 26 and 27: Composition observable: ! shower ma
Page 28 and 29: Puzzling Composition! Unexpected As
Page 30 and 31: Neutrino Fluxes!
Page 32 and 33: Above 60 EeV: ! either Protons or I
Page 34 and 35: If Correlated with sources ! < 10 o
Page 36 and 37: Hadronic Interactions ! Parameters
Page 40 and 41: Auger North - 10 yr Auger South - 1
Page 42 and 43: FD disentangle Composition !
Page 44 and 45: Galactic Plane!
Page 48 and 49: Lindsleys Exposure Evolution - Line
Page 50 and 51: Auger North Objectives! Obtain the
Page 52 and 53: State of Colorado Auger North: 4000
Page 54 and 55: Features of Auger North Fluorescenc
Page 56 and 57: Communications System Campus Area M
Page 58 and 59: Argentina " "Netherlands! Australia
Page 60 and 61: Estimated Construction Cost! WBS Ac
Page 62 and 63: Funding! Auger South ($54M):! Europ
Page 64 and 65: US Auger Groups! Argonne National L
Page 66 and 67: The Pierre Auger Observatory Auger
Page 68 and 69: Auger North Auger South Auger North

Auger North - Fermilab Center for Particle Astrophysics

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