A Modal Approach to the Numerical Calculation of Primordial non-Gaussianities
arXiv:1211.3086 · doi:10.1088/1475-7516/2013/02/002
Abstract
We propose a new method to numerically calculate higher-order correlation functions of primordial fluctuations generated from any early-universe scenario. Our key-starting point is the realization that the tree-level In-In formalism is intrinsically separable. This enables us to use modal techniques to efficiently calculate and represent non-Gaussian shapes in a separable form well suited to data analysis. We prove the feasibility and the accuracy of our method by applying it to simple single-field inflationary models in which analytical results are available, and we perform non-trivial consistency checks like the verification of the single field consistency relation. We also point out that the i epsilon prescription is automatically taken into account in our method, preventing the need for ad-hoc tricks to implement it numerically.
18 pages, 6 figures
References in corpus (8)
- Observational Signatures and Non-Gaussianities of General Single Field Inflation
- Primordial Non-Gaussianities from Inflation Models
- Generation and Characterization of Large Non-Gaussianities in Single Field Inflation
- The shape of primordial non-Gaussianity and the CMB bispectrum
- Primordial non-Gaussianity and the CMB bispectrum
- A Statistical Approach to Multifield Inflation: Many-field Perturbations Beyond Slow Roll
- Nongaussianity from Particle Production During Inflation
- Optimal Trispectrum Estimators and WMAP Constraints
Cited by in corpus (9)
- Primordial fluctuations and non-Gaussianities in sidetracked inflation
- Numerical evaluation of the bispectrum in multiple field inflation
- Stability analysis of inflation with an SU(2) gauge field
- Transporting non-Gaussianity from sub to super-horizon scales
- General CMB bispectrum analysis using wavelets and separable modes
- Non-Gaussian signatures of general inflationary trajectories
- Anatomy of Parity-violating Trispectra in Galaxy Surveys
- Planck and WMAP constraints on generalised Hubble flow inflationary trajectories
- Probing Inflation with Precision Bispectra