Secondary CMB Anisotropy I: Reionization - Wayne Hu's Tutorials

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Polarization Tests • Matching polarization anomalies if cosmological Dvorkin, Peiris, Hu (2007)
Polarization Bumps • If features in the temperature spectrum reflect features in the power spectrum (inflationary potential), reflected in polarization with little ambiguity from reionization Mortonson et al (2009) Covi et al (2006) ionization adjusted to max/min feature
Page 1 and 2:
Secondary CMB Anisotropy I: Reioniz
Page 3 and 4:
Outline Cabo Lectures (not all incl
Page 5 and 6:
Physics of Secondary Anisotropies S
Page 7 and 8: ∆T (µK) 100 10 1 0.1 Gravitation
Page 9 and 10: Across the Horizon Hu & White (2004
Page 11 and 12: Why Are Secondaries So Smalll? •
Page 13 and 14: Integral Solution • Projection ke
Page 15 and 16: Reionization Suppression • Rescat
Page 17 and 18: Doppler Effect
Page 19 and 20: (2l+1)j l (100) Doppler Effect in L
Page 21 and 22: Reionization Surface Modulated Dopp
Page 23 and 24: Inhomogeneous Ionization • As rei
Page 25 and 26: Patchy Reionization Aghanim et al (
Page 27 and 28: WMAP Correlation • Reionization p
Page 29 and 30: Polarization from Thomson Scatterin
Page 31 and 32: Whence Quadrupoles? • Temperature
Page 33 and 34: Whence Polarization Anisotropy? •
Page 35 and 36: Modulation by Plane Wave • Amplit
Page 37 and 38: l(l+1)/2π Cl (µK 2 ) WMAP 3yr Dat
Page 39 and 40: Locally Transparent • Presently,
Page 41 and 42: Polarization Anisotropy • Electro
Page 43 and 44: Instantaneous Reionization • WMAP
Page 45 and 46: Distance Predicts Growth • With s
Page 47 and 48: Distinguishable History • Same op
Page 49 and 50: Principal Components • Eigenvecto
Page 51 and 52: Representation in Modes • Truncat
Page 53 and 54: Total Optical Depth • Optical dep
Page 55 and 56: Model-Independent Reionization •
Page 57: Large Angle Anomalies • Low plana
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Secondary CMB Anisotropy I: Reionization - Wayne Hu's Tutorials

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