Peter BIERMANN (.pdf)

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KASCADE, KASCADE-Grande and Auger 0.6 2.0 ) -2 -1.5 eV -1.2 -1 2.4 Sum sr -1 s 1.8 -2 He 24 10 H Ne-S CNO x dN/dE (m 3 Fe E 12 Cl-Mn 23 10 KASCADE QGSJet KASCADE Sibyll KASCADE Grande Auger 20 10 E (eV/nucleus) 19 10 18 10 17 10 16 10 15 10 Figure 5 KASCADE, KASCADE-Grande, and Auger data interpreted as arising from a combination of Galactic CRs plus galactic CRs from another active galaxy, shifted up in a relativistic kick (Gopal-Krishna et al. 2010 ApJL; PLB & de Souza 2012 ApJ). The numbers give (model - data)/(experimental error): this suggests a good fit beyond the knee, and a single extragalactic source, only Cen A: contrary to the expectation since 1966 (Greisen, Zatsepin, Kuzmin) there is no other extragalactic source population necessary.
Summary cosmic ray particles • Quantitative predictions from 1993: Tests since 2009 • Occam’s razor simplicity: CR-I to IV (1993) model suffices to explain the 2009 - 2013 data • Polar cap CRs of exploding stars with magnetic winds : CR positron fraction, Galactic haze, 511 keV line, γ-ray continuum and 130 GeV line • CR spectrum possibly explained with our Galaxy and radio galaxy Cen A 13 • Below GZK no other source population required by the data: magnetic horizon (Ryu et al. 2008+) • Can be falsified: very different abundances? magnetic wind of our Galaxy (Everett et al. 2008)? Neutrinos ?
Page 1 and 2: ASTROPHYSICS OF WARM DARK MATTER Pe
Page 3 and 4: AMS positron fraction: data 2013 3
Page 5 and 6: CR positron fraction: prediction 20
Page 7 and 8: Supersymmetry! Evidence? • Supers
Page 9 and 10: Cosmic ray knee: paper CR-IV, 1993
Page 11: 130 GeV line interpreted ? • Rece
Page 15 and 16: The sky in black holes > ∼108 M
Page 17 and 18: Massive and supermassive stars at v
Page 19 and 20: Stellar agglomeration conditions
Page 21 and 22: The radio background, Thomson depth
Page 23 and 24: The radio background, Thomson depth
Page 25 and 26: Energy density from ∼ 3 106 M⊙
Page 27 and 28: ? ? Weakly Interacting Neutrino = W
Page 29 and 30: 2 Abstract Dark matter has been fir
Page 31 and 32: pernova CR-contributions with pulsa
Page 33 and 34: massive black holes: they possibly
Page 35 and 36: HII regions and HNRs, and only a ve
Page 37 and 38: [11] Adulpravitchai, A., Gu, P.-H.,
Page 39 and 40: [19] Bringmann, T., et al., eprint
Page 41 and 42: Strom, Astron. & Astroph. 275, 659
Page 43 and 44: [34] Universality of galactic surfa

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