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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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The Standard Model of Cosmology: LC
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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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The Standard Model of Cosmology: LC
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The Standard Model of Cosmology: LC
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Candidates: Axions Sterile neutrino
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Dama/Libra 8
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But a light WIMP, (10-100GeV, CoGeN
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IceCube Neutrino Telescope in Antar
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ANTARES -Telescopio de Neutrinos en
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Telescopio HESS, Namibia (2004) γ
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SuperCDMS 1TG Lux (3 T liq Xe) Xeno
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The Standard Model of Cosmology: Pr
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Galaxy´s density Observed Theory
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W. J. G. de Blok, Stacy S. McGaugh,
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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 68: Voids are too empty P. J. E. Peeble
- Page 71 and 72: Early assembly of the most massive
- Page 73 and 74: Early Galaxies Compactness Pieter G
- Page 75 and 76: 1E 0657-56, "Bullet Cluster” 2006
- Page 77 and 78: The only way to fit the observation
- Page 79 and 80: MACS J0025.4-1222 2008 Clusters Col
- Page 81 and 82: Shaun A. Thomas, Filipe B. Abdalla,
- Page 84 and 85: Some Alternatives SM Extentions GR
- Page 86 and 87: • Self-Interacting DM • Warm DM
- Page 88 and 89: SM Extentions GR Extentions • Sel
- Page 91 and 92: Self-Interacting and Warm DM Rachel
- Page 93 and 94: Self-Interacting and Warm DM Rachel
- Page 95: SM Extentions GR Extentions • Sel
- Page 101 and 102: Pamela Constrains 43
- Page 103 and 104: DM lifetime [s] 10 27 10 26 10 25 1
- Page 105: SM Extentions GR Extentions • Sel
- 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
- Page 118 and 119: Repulsive, Fuzzy and Scalar Field D
- Page 120 and 121: Ideas Matos-Guzman 2000 P. J. E. Pe
- Page 123: Bose-Einstein Condensates ☐☐☐
- Page 126 and 127: The Cosmology Φ 2 as Dark Matter.
- Page 128 and 129: Linear regime of perturbations
- Page 130 and 131: Linear regime of perturbations δ
- Page 132 and 133: Linear regime of perturbations δ
- Page 134 and 135: Galactic Collapse of Scalar Field D
- Page 137 and 138: Weak Field Limit A. Bernal, et. al.
- Page 139 and 140: Density Profiles T. Harko & C. G. B
- Page 141 and 142: Density Profiles LSB Galaxies
- Page 144: 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