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

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EG = 1 β Υgm Υgg MOND and MOND+ R. Reyes, R. Mandelbaum, U. Seljak, T. Baldauf, J. E. Gunn, L. Lombriser & R. E. Smith. NATURE, Vol 464, 11 March 2010 74
MOND and MOND+ S. Mendoza, X. Hernandez, J.C. Hidalgo & T. Bernal. arXiv: 1006.5037 75
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
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z=1.4 The Standard Model of Cosmolo
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Page 17 and 18:
Page 19 and 20:
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
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ANTARES -Telescopio de Neutrinos en
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Telescopio HESS, Namibia (2004) γ
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SuperCDMS 1TG Lux (3 T liq Xe) Xeno
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The Standard Model of Cosmology: Pr
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Galaxy´s density Observed Theory
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W. J. G. de Blok, Stacy S. McGaugh,
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Galaxy’s Center: Observations Jos
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Galaxy’s Center: Simulations
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Galaxy’s Center: Simulations F. G
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Galaxy’s Center: Simulations F. G
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Stellar Mass Predictions Till Sawal
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Velocity predictions Jesús Zavala,
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Missing Satellites Problem
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Missing Satellites Problem 26
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Galaxies appear simpler than expect
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Voids are too empty P. J. E. Peeble
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Voids are too empty P. J. E. Peeble
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Early assembly of the most massive
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Early Galaxies Compactness Pieter G
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1E 0657-56, "Bullet Cluster” 2006
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The only way to fit the observation
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MACS J0025.4-1222 2008 Clusters Col
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Shaun A. Thomas, Filipe B. Abdalla,
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Some Alternatives SM Extentions GR
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• Self-Interacting DM • Warm DM
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SM Extentions GR Extentions • Sel
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Self-Interacting and Warm DM Rachel
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Self-Interacting and Warm DM Rachel
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pbar/p 1e-04 1e-05 Pamela Constrain
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DM lifetime [s] 10 27 10 26 10 25 1
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Page 107 and 108:
Extra Symmetries A. de la Macorra,
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Extra Symmetries 46
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L = 1 Extra Symmetries Cosmological
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35 30 25 20 15 10 5 0 4 Extra Symme
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Page 119 and 120:
Repulsive, Fuzzy and Scalar Field D
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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 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 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
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