Problems and Alternatives to Lambda Cold Dark Matter - Berkeley ...

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Voids are too empty P. J. E. Peebles & A. Nusser, Nature 465(2010)565 In short, the general insensitivity of galaxies to their environments is not expected in standard ideas. It would help if galaxies were more rapidly assembled, as they could then evolve as more nearly isolated island universes. 28
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Problems and Alternatives to Lambda
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• Space-time: FLRW • Matter: DM
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The Standard Model of Cosmology: LC
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z=18.3 The Standard Model of Cosmol
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z=1.4 The Standard Model of Cosmolo
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Page 17 and 18: The Standard Model of Cosmology: LC
Page 19 and 20: Candidates: Axions Sterile neutrino
Page 22 and 23: Dama/Libra 8
Page 24 and 25: But a light WIMP, (10-100GeV, CoGeN
Page 26: IceCube Neutrino Telescope in Antar
Page 29 and 30: ANTARES -Telescopio de Neutrinos en
Page 31: Telescopio HESS, Namibia (2004) γ
Page 34 and 35: SuperCDMS 1TG Lux (3 T liq Xe) Xeno
Page 37 and 38: The Standard Model of Cosmology: Pr
Page 39 and 40: Galaxy´s density Observed Theory
Page 41 and 42: W. J. G. de Blok, Stacy S. McGaugh,
Page 43 and 44: Galaxy’s Center: Observations Jos
Page 45 and 46: Galaxy’s Center: Simulations
Page 47 and 48: Galaxy’s Center: Simulations F. G
Page 49 and 50: Galaxy’s Center: Simulations F. G
Page 52 and 53: Stellar Mass Predictions Till Sawal
Page 55 and 56: Velocity predictions Jesús Zavala,
Page 58 and 59: Missing Satellites Problem
Page 60 and 61: Missing Satellites Problem 26
Page 63 and 64: Galaxies appear simpler than expect
Page 66 and 67: Voids are too empty P. J. E. Peeble
Page 70 and 71: Early assembly of the most massive
Page 72 and 73: Pieter G. van Dokkum et. al. NATURE
Page 74 and 75: Early Galaxies Compactness Pieter G
Page 76 and 77: Clusters Collisons Mastropietro, C.
Page 78 and 79: MACS J0025.4-1222 2008 Clusters Col
Page 80 and 81: MACS J0025.4-1222 2008 Clusters Col
Page 82: Large scale structure anomaly Shaun
Page 85 and 86: • Self-Interacting DM • Warm DM
Page 87 and 88: SM Extentions GR Extentions • Sel
Page 89: SM Extentions GR Extentions • Sel
Page 92 and 93: Self-Interacting and Warm DM Rachel
Page 94 and 95: Self-Interacting and Warm DM Rachel
Page 101 and 102: Pamela Constrains 43
Page 103 and 104: DM lifetime [s] 10 27 10 26 10 25 1
Page 108 and 109: Extra Symmetries A. de la Macorra,
Page 110 and 111: Extra Symmetries Cosmological Scala
Page 113 and 114: Extra Symmetries 47
Page 115 and 116: SM Extentions GR Extentions • Sel
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Repulsive, Fuzzy and Scalar Field D
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Ideas Matos-Guzman 2000 P. J. E. Pe
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Bose-Einstein Condensates ☐☐☐
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The Cosmology Φ 2 as Dark Matter.
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Linear regime of perturbations
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Linear regime of perturbations δ
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Linear regime of perturbations δ
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Galactic Collapse of Scalar Field D
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Weak Field Limit A. Bernal, et. al.
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Density Profiles T. Harko & C. G. B
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Density Profiles LSB Galaxies
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Hydrodinamical version of the Linea
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Hydrodinamical version of the Linea
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SFDM
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SM Extentions GR Extentions • Sel
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MOND and MOND+ R. H. Sanders. The A
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EG = 1 β Υgm Υgg MOND and MOND+
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SM Extentions GR Extentions • Sel
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f(R) Yong-Seon Song, Hiranya Peiris
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T. Damour & Esposito-Farèse. PRL 7
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Hidden Brane Visible Brane Scalar F
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Conclusion • We are in the thresh
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