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waynehu

Professor, Department of Astronomy and Astrophysics
University of Chicago

Group Contact CV Computing SnapShots
CMB Introduction '96   Intermediate '01   Polarization Intro '01   Cosmic Symphony '04   Polarization Primer '97   Review '02   Power Animations   Lensing   Power Prehistory   Legacy Material '96   PhD Thesis '95 Baryon Acoustic Oscillations Cosmic Shear Clusters
Transfer Function WMAP Likelihood Reionization PPF for CAMB Halo Mass Conversion Cluster Abundance
Advanced CMB [448] Cosmology [321] Current Topics [282] Galaxies and Universe [242] Radiative Processes [305] Research Preparation [307] Inflationary Perturbations [408]

Damping Tail

The damping tail is predicted by the same parameters that control the first three peaks in the standard model (usual particle species and power law initial fluctuations). Any deviation from these predictions indicates that more exotic physics may be at work. Conversely, consistency is proof against such missing physics.