- 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 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 38 and 39: The Standard Model of Cosmology: Pr
- Page 40 and 41: Galaxy’s Density Galaxy´s densit
- Page 42 and 43: Galaxy’s Center: Observations W.
- Page 44 and 45: NFW Galaxy’s Center: Observations
- Page 46 and 47: Galaxy’s Center: Simulations F. G
- Page 48 and 49: Galaxy’s Center: Simulations F. G
- Page 50: No evidence for internal features o
- Page 53: Stellar Mass Predictions Till Sawal
- Page 56: Velocity predictions Jesús Zavala,
- Page 59 and 60: Missing Satellites Problem
- Page 61: Missing Satellites Problem 26
- Page 64: Galaxies appear simpler than expect
- Page 67 and 68: 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 96:
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
- Page 156:
Hydrodinamical version of the Linea
- Page 164 and 165:
SFDM
- Page 166 and 167:
SM Extentions GR Extentions • Sel
- Page 171 and 172:
MOND and MOND+ R. H. Sanders. The A
- Page 174 and 175:
EG = 1 β Υgm Υgg MOND and MOND+
- Page 180 and 181:
SM Extentions GR Extentions • Sel
- Page 186:
f(R) Yong-Seon Song, Hiranya Peiris
- Page 191:
T. Damour & Esposito-Farèse. PRL 7
- Page 200:
Hidden Brane Visible Brane Scalar F
- Page 203:
Conclusion • We are in the thresh