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

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MACS J0025.4-1222 2008 Clusters Collisons J. Lee & E. Komatsu, ApJ, 718(2010)60 Gpc 3 /h 3 With a large-volume (27 ) cosmological N-body MICE simulation, the probability of finding 3000 km/s is between 3.3 x 10 <strong>and</strong> 3.6 x . −11 10 −9 33
Shaun A. Thomas, Filipe B. Abdalla, <strong>and</strong> Ofer Lahav. arXiv:1012.2272 . . . 0.55
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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:
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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
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 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: MACS J0025.4-1222 2008 Clusters Col
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 100 and 101: pbar/p 1e-04 1e-05 Pamela Constrain
Page 102 and 103: DM lifetime [s] 10 27 10 26 10 25 1
Page 107 and 108: Extra Symmetries A. de la Macorra,
Page 109 and 110: Extra Symmetries 46
Page 111: L = 1 Extra Symmetries Cosmological
Page 114 and 115: 35 30 25 20 15 10 5 0 4 Extra Symme
Page 116: SM Extentions GR Extentions • Sel
Page 119 and 120: Repulsive, Fuzzy and Scalar Field D
Page 121: Ideas Perez-Lorenzana-et. al. 2007
Page 125 and 126: The Cosmology
Page 127 and 128: The Cosmology Φ 2 as Dark Matter.
Page 129 and 130: Linear regime of perturbations δ
Page 131 and 132:
Linear regime of perturbations δ
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Linear regime of perturbations δ
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Scalar Field Fluctuation = Halo Gal
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T. Harko & C. G. Bhömer JCAP 0706:
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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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0.0001 9e-05 8e-05 7e-05 6e-05 5e-0
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SM Extentions GR Extentions • Sel
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M. Milgrom. Acta Phys.Polon.B32:361
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MOND and MOND+ J. D. Bekenstain. PH
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MOND and MOND+ S. Mendoza, X. Herna
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SM Extentions GR Extentions • Sel
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f(R) Dark matter as a geometric eff
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Extra Dimensions 81
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Conclusion
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