- 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 7 and 8: The Standard Model of Cosmology: LC
- Page 9 and 10: 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 15 and 16: The Standard Model of Cosmology: LC
- 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 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 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:
SM Extentions GR Extentions • Sel
- 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:
SM Extentions GR Extentions • Sel
- 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
- Page 133 and 134:
Linear regime of perturbations δ
- 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
- Page 160:
0.0001 9e-05 8e-05 7e-05 6e-05 5e-0
- Page 165 and 166:
SM Extentions GR Extentions • Sel
- Page 167:
M. Milgrom. Acta Phys.Polon.B32:361
- Page 172:
MOND and MOND+ J. D. Bekenstain. PH
- Page 175:
MOND and MOND+ S. Mendoza, X. Herna
- Page 181:
SM Extentions GR Extentions • Sel
- Page 188:
f(R) Dark matter as a geometric eff
- Page 199 and 200:
Extra Dimensions 81
- Page 202 and 203:
Conclusion