- Page 1 and 2: 1 Cosmic-ray physics and Auger late
- Page 3 and 4: 3 Cosmic rays: “CRs” ■ Key su
- Page 5: Cosmic ray physics started one cent
- Page 9 and 10: 9 Then a long story began… ■
- Page 11 and 12: 11 CR-induced atmospheric showers P
- Page 13 and 14: Schism… and ecumenism! 13 study o
- Page 15 and 16: A remarkably coherent, though myste
- Page 17 and 18: [CR flux] x E 3 17 ■ Essentially
- Page 19 and 20: 19 The way out of the mist ■ Anal
- Page 21 and 22: 21 Propagation: a “3-space” pro
- Page 23 and 24: 23 Angular distribution ■ Isotrop
- Page 25 and 26: Interaction with B inhomogeneities
- Page 27 and 28: Reaching the diffusive regime 27 <
- Page 29 and 30: Diffusive transport and GCR confine
- Page 31 and 32: GCR large angular scale anisotropy
- Page 33 and 34: larger energy 33 Paris, 9 th June 2
- Page 35 and 36: still larger energy 35 “Ballistic
- Page 37 and 38: 37 Propagation: a “3-space” pro
- Page 39 and 40: Energy losses and nuclear interacti
- Page 41 and 42: Pion production in interstellar med
- Page 43 and 44: Nuclear interactions in ISM 43 Pari
- Page 45 and 46: Composition: CR vs solar system 45
- Page 47 and 48: Secondary/primary ratios 47 Strong
- Page 49 and 50: 49 Some results ■ ■ ■ ■ Sec
- Page 51 and 52: 51 Cosmic-ray clocks 54 Mn/Mn 36 Cl
- Page 53 and 54: 53 Antiprotons Strong & Moskalenko
- Page 55 and 56: Search for dark matter: positron fr
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57 High energy CR propagation ■
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59 [cross section] x [inelasticity]
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61 "Propagated" spectrum z = 0.01,
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63 10 Spectre propagé (source uniq
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UHE Nuclei propagation 65 2D nuclea
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Fe interaction and energy loss leng
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Fit of the spectrum with a “pure
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Are there nuclei among EGCRs? 71 Pu
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73 The Pierre Auger Observatory Nor
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High-energy CR detection 75 • com
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Hexagonal array (1.5 km spacing, 30
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Aerial view of Los Leones fluoresce
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One of the fluorescence eyes 81 440
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83 Independent analyses of stereo e
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Atmospheric depth of shower maximum
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Energy reconstruction with surface
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Cross-calibration of the detectors
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Energy spectrum from SD showers wit
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Energy spectrum 93 Paris, 9 th June
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Auger main anisotropy result 95 ■
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Auger main anisotropy result 97 3 f
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Significance of the anisotropy resu
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101 Auger main anisotropy result Th
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Summary of Auger results 103 compos
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Galactic/Extragalactic transition 1
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Toy model: holistic scenario 107
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What is at stake 109 ■ Major disc
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111 Extra slides Paris, 9 th June 2
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Photon flux limit 113 astro-ph/0712
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Neutrino detection with Auger "GZK
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Selection criteria 117 young shower
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Horizontal showers 119 Example of a
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LiBeB nucleosynthesis 121 ■ Li, B
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HE photon emission from GCR interac