Secondary CMB Anisotropy

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Secondary CMB Anisotropy III: Cosmic Acceleration Wayne Hu Cabo, January 2009
Physics of Secondary Anisotropies Primary Anisotropies recombination z~1000 Doppler Vishniac Lensing Patchy rei. reionization z~10 SZ ISW acceleration z~1
Page 1: Secondary CMB Anisotropy III: Cosmi
Page 5 and 6: Gravitational Secondaries 100 ∆T
Page 7 and 8: ISW Effect • Gravitational bluesh
Page 9 and 10: Smooth Energy Density & Potential D
Page 11 and 12: ISW Spatial Modes • ISW effect co
Page 13 and 14: Smooth Energy Density & Potential D
Page 15 and 16: Dark Energy • Peaks measure dista
Page 17 and 18: Dark Energy Clustering • ISW effe
Page 19 and 20: ISW-Galaxy Correlation • ~4σ joi
Page 21 and 22: Galaxy Cross Correlation • Cross
Page 23 and 24: Dark Energy Smoothness • More rob
Page 25 and 26: Low Quadrupole Models • Required
Page 27 and 28: ISW & Modified Gravity
Page 29 and 30: DGP Braneworld Acceleration • Bra
Page 31 and 32: DGP CMB Large-Angle Excess • Extr
Page 33 and 34: CMB in DGP • Adding cut off as an
Page 35 and 36: PPF f(R) Description • Metric and
Page 37 and 38: PPF f(R) Description • Metric and
Page 39 and 40: Parameterized Post-Friedmann • Pa
Page 41 and 42: Moving Halo Effect
Page 43 and 44: SZ Effect
Page 45 and 46: Thermal SZ Effect Large Scale Struc
Page 47 and 48: Beyond Thomson Limit • Thomson sc
Page 49 and 50: Recoil Effect • Since −1 ≤ co
Page 51 and 52: Thermalization • For a thermal di
Page 53 and 54:
Kompaneets Equation • The Kompane
Page 55 and 56:
Spectral Distortion • Compton ups
Page 57 and 58:
Amplitude of Fluctuations
Page 59 and 60:
Power Spectrum Present
Page 61 and 62:
SPT Discovered Clusters • Previou
Page 63 and 64:
Fully Calibrated • Given a comple
Page 65 and 66:
Joint Self-Calibration • Both cou
Page 67 and 68:
Modified Gravity f(R) Simulations
Page 69 and 70:
Summary: Lecture III • Differenti
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