Secondary CMB Anisotropy - Wayne Hu's Tutorials

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Lensing-Galaxy Correlation • ~3σ+ joint detection of WMAP lensing reconstruction with large scale structure (galaxies) • Consistent with ΛCDM Smith et al (2007) [Hirata et al 2008]
∆P P Matter Power Spectrum • Measuring projected matter power spectrum to cosmic variance limit across whole linear regime 0.002< k < 0.2 h/Mpc ≈ −0.6 deflection power mtot eV 10 –7 10 –8 Hu & Okamoto (2001) Reference Linear 10 100 1000 L
Page 1 and 2: Secondary CMB Anisotropy II: B-Mode
Page 3 and 4: ∆ (µK) 100 10 1 0.1 0.01 Hu & Do
Page 5 and 6: Electric & Magnetic Polarization (a
Page 7 and 8: Quadrupoles from Gravitational Wave
Page 9 and 10: ∆B (µK) Energy Scale of Inflatio
Page 11 and 12: Slow Roll Consistency Relation •
Page 13 and 14: Modulated Polarization • Ionizati
Page 15 and 16: B-mode Contamination from Reionizat
Page 17 and 18: Example of CMB Lensing • Toy exam
Page 19 and 20: Lensing by a Gaussian Random Field
Page 21 and 22: Gravitational Lensing • Lensing i
Page 23 and 24: Flat-sky Treatment • Mode couplin
Page 25 and 26: • If ˜ C ΘΘ l Smoothing Power
Page 27 and 28: Generation of Power • On scales b
Page 29 and 30: Lensing Smoothing • Lensing smoot
Page 31 and 32: Polarization Lensing • Since E an
Page 33 and 34: Polarization Power Spectra • Carr
Page 35 and 36: Power Spectrum Measurements • Len
Page 37 and 38: Redshift Sensitivity • Lensing ob
Page 39 and 40: Lensing Observables • Lensing obs
Page 41 and 42: Lensing Reconstruction
Page 43 and 44: Quadratic Reconstruction • Matche
Page 45: High Signal-to-Noise B-modes • Co
Page 49 and 50: Tomography & Growth Rate • Cross
Page 51 and 52: Cross Correlation with Temperature
Page 53 and 54: (pixels) 1000 800 600 400 200 Recon
Page 55 and 56: (pixels) 1000 800 600 400 200 Recon
Page 57 and 58: ∂lnR/∂p 0 -0.05 -0.10 -0.15 0.3

Secondary CMB Anisotropy - Wayne Hu's Tutorials

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