Auger North - Fermilab Center for Particle Astrophysics

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The Pierre Auger Observatory Science Goals: Auger North! To Discover the Sources of Ultra High Energy Cosmic Rays To Study Particle Interactions above 100 TeV CM
To Discover UHECR Sources ! need:! Full Sky Distribution of events > 60 EeV! Much Higher Statistics > 60 EeV! To Probe >100 TeV scale, ! need:! Determine the Primary Composition > 60 EeV:! "Astrophysically AND thru Shower Properties! Detect UHE neutrinos and photons!
Page 1: The Pierre Auger Observatory Auger
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 46 and 47: Determine Source Distribution! Type
Page 48 and 49: Lindsleys Exposure Evolution - Line
Page 50 and 51: Auger North Objectives! Obtain the
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State of Colorado Auger North: 4000
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Features of Auger North Fluorescenc
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Communications System Campus Area M
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Argentina " "Netherlands! Australia
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Estimated Construction Cost! WBS Ac
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Funding! Auger South ($54M):! Europ
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US Auger Groups! Argonne National L
Page 66 and 67:
The Pierre Auger Observatory Auger
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Auger North Auger South Auger North
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Auger North - Fermilab Center for Particle Astrophysics

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