Secondary CMB Anisotropy

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Scattering Secondaries 100 ∆T (µK) 10 1 Doppler suppression density–mod linear ion-mod SZ 0.1 10 100 1000 l
Gravitational Secondaries 100 ∆T (µK) 10 1 0.1 ISW lensing Moving Halo 10 100 1000 l un– lensed
Page 1 and 2: Secondary CMB Anisotropy I: Reioniz
Page 3 and 4: Outline Cabo Lectures (not all incl
Page 5: Physics of Secondary Anisotropies P
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: Doppler Effect in Limber Approximat
Page 21 and 22: Modulated Doppler Effect Reionizati
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: WMAP 3yr Data 100.00 WMAP 3yr: Page
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 and 58:
Large Angle Anomalies • Low plana
Page 59 and 60:
Polarization Bumps • If features
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Secondary CMB Anisotropy

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