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The universe: Planck 2013 Planck 2013 XVI (Table 2 ff): Term “dark matter” due to Oort (1933) The sum of all Ωs very close to unity, critical density: “flat” geometry, like a perfect tabletop: ΩΛ = 0.692 ± 0.010 Ωdm = 0.2582 ± 0.0047 Ωb = 0.0482 ± 0.00076 Ωk = 1 − ΩΛ − Ωdm − Ωb = −0.0005 ± 0.0066 H0 = 67.8 ± 0.77 km/s/Mpc Assuming gradual re-ionization zre−ion,init > ∼ 20 Thomson depth: τT = 0.092 ± 0.013 The age of the universe: t0 = (13.798 ± 0.037) · 109 yr 6 80 years: what is dark matter?
Supersymmetry! Evidence? • Supersymmetric massive particles decay and might explain many observations • Upturn in CR-e + /CR-e− ratio and CR-e− in cosmic rays (Pamela, Fermi, ATIC, AMS) • Fermi haze/bubble; 511 keV + 130 GeV line: Galactic Center region synchrotron and IC 7 • Cygnus cocoon spectrum • WMAP + Planck haze spectra • IceCube high energy neutrino background
Page 1 and 2: ASTROPHYSICS OF WARM DARK MATTER Pe
Page 3 and 4: AMS positron fraction: data 2013 3
Page 5: CR positron fraction: prediction 20
Page 9 and 10: Cosmic ray knee: paper CR-IV, 1993
Page 11 and 12: 130 GeV line interpreted ? • Rece
Page 13 and 14: Summary cosmic ray particles • Qu
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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