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

More documents

Recommendations

Info

The Cosmology Φ 2 as Dark Matter. T. Matos, A. Vázquez & J.A. Magaña. MNRAS, 389, (2009) 13957.
The Cosmology Φ 2 as Dark Matter. T. Matos, A. Vázquez & J.A. Magaña. MNRAS, 389, (2009) 13957.
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:
Page 9 and 10:
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:
Page 17 and 18:
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 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 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: The Cosmology
Page 129 and 130: 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 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
show all

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

Create successful ePaper yourself

Delete template?

Save as template?