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

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Galaxies appear simpler than expected M. J. Dysney, et. al. Vol 455(2008)1082 R90 ∝ R50 Lg ∝ R 3 50 MHI ∝ R 2 50 Md ∝ Lg Σ = Lg/R 2 50 ∝ L 1/3 g Whereas Lg/R 3 50 Md/R 3 50 ∝ R50 are independent of the size of the galaxy
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Problems and Alternatives to Lambda
Page 3 and 4:
• Space-time: FLRW • Matter: DM
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The Standard Model of Cosmology: LC
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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 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 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 101 and 102: Pamela Constrains 43
Page 103 and 104: DM lifetime [s] 10 27 10 26 10 25 1
Page 108 and 109: Extra Symmetries A. de la Macorra,
Page 110 and 111: Extra Symmetries Cosmological Scala
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Extra Symmetries 47
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SM Extentions GR Extentions • Sel
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Repulsive, Fuzzy and Scalar Field D
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Ideas Matos-Guzman 2000 P. J. E. Pe
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Bose-Einstein Condensates ☐☐☐
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The Cosmology Φ 2 as Dark Matter.
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Linear regime of perturbations
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Linear regime of perturbations δ
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Linear regime of perturbations δ
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Galactic Collapse of Scalar Field D
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Weak Field Limit A. Bernal, et. al.
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Density Profiles T. Harko & C. G. B
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Density Profiles LSB Galaxies
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Hydrodinamical version of the Linea
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Hydrodinamical version of the Linea
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SFDM
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Page 171 and 172:
MOND and MOND+ R. H. Sanders. The A
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EG = 1 β Υgm Υgg MOND and MOND+
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Page 186:
f(R) Yong-Seon Song, Hiranya Peiris
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T. Damour & Esposito-Farèse. PRL 7
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Hidden Brane Visible Brane Scalar F
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Conclusion • We are in the thresh
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