Part 3
Initial Conditions

3.1 Introduction
3.2 Constraining inflation
 3.2.1 Primordial perturbations from inflation
 3.2.2 Forecast constraints on the power spectrum
3.3 Probing the early universe with non-Gaussianities
 3.3.1 Local non-Gaussianity
 3.3.2 Shapes: what do they tell us?
 3.3.3 Beyond shapes: scale dependence and the squeezed limit
 3.3.4 Beyond inflation
3.4 Primordial Non-Gaussianity and Large-Scale Structure
 3.4.1 Constraining primordial non-Gaussianity and gravity from 3-point statistics
 3.4.2 Non-Gaussian halo bias
 3.4.3 Number counts of nonlinear structures
 3.4.4 Forecasts for Euclid
 3.4.5 Complementarity
3.5 Isocurvature modes
 3.5.1 The origin of isocurvature perturbations
 3.5.2 Constraining isocurvature perturbations
3.6 Summary and outlook

  Go to previous page Go up Go to next page