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

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The Standard Model of Cosmology: Problems • Cuspy central density profiles • Missing Satellites Problem • No-fit of the early assembly of galaxies • Galaxies seems to be simpler • Voids are too empty • No-detection of DM • etc.
Galaxy´s density Observed Theory ρNFW = 1 x ρNFW ∼ 1 x ρ ∼ 1 x α 0 < α < 1 δ0ρ0 (1 + x) 2 17
Page 1 and 2: Problems and Alternatives to Lambda
Page 3 and 4: • Space-time: FLRW • Matter: DM
Page 5 and 6: The Standard Model of Cosmology: LC
Page 11 and 12: z=18.3 The Standard Model of Cosmol
Page 13 and 14: z=1.4 The Standard Model of Cosmolo
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: The Standard Model of Cosmology: Pr
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 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 and 96:
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 104 and 105:
Page 107 and 108:
Extra Symmetries A. de la Macorra,
Page 109 and 110:
Extra Symmetries 46
Page 111:
L = 1 Extra Symmetries Cosmological
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35 30 25 20 15 10 5 0 4 Extra Symme
Page 116:
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:
Page 133 and 134:
Page 135:
Scalar Field Fluctuation = Halo Gal
Page 138 and 139:
T. Harko & C. G. Bhömer JCAP 0706:
Page 140 and 141:
Density Profiles LSB Galaxies
Page 142:
Hydrodinamical version of the Linea
Page 154:
Hydrodinamical version of the Linea
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0.0001 9e-05 8e-05 7e-05 6e-05 5e-0
Page 165 and 166:
Page 167:
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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f(R) Dark matter as a geometric eff
Page 199 and 200:
Extra Dimensions 81
Page 202 and 203:
Conclusion
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