Tensors, non-Gaussianities, and the future of potential reconstruction

Abstract

We present projections for reconstruction of the inflationary potential expected from ESA's upcoming Planck Surveyor CMB mission. We focus on the effects that tensor perturbations and the presence of non-Gaussianities have on reconstruction efforts in the context of non-canonical inflation models. We consider potential constraints for different combinations of detection/null-detection of tensors and non-Gaussianities. We perform Markov Chain Monte Carlo and flow analyses on a simulated Planck-precision data set to obtain constraints. We find that a failure to detect non-Gaussianities precludes a successful inversion of the primordial power spectrum, greatly affecting uncertainties, even in the presence of a tensor detection. In the absence of a tensor detection, while unable to determine the energy scale of inflation, an observable level of non-Gaussianities provides correlations between the errors of the potential parameters, suggesting that constraints might be improved for suitable combinations of parameters. Constraints are optimized for a positive detection of both tensors and non-Gaussianities.

12 pages, 5 figures, LaTeX; V2: version submitted to JCAP

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• Bayesian Analysis of Inflation: Parameter Estimation for Single Field Models
• Constraining $\mathcal{N}=1$ supergravity inflationary framework with non-minimal Kähler operators
• Inflationary potentials in DBI models
• Optimizing future experimental probes of inflation
• Let Effective Field Theory of Inflation flow: stochastic generation of models with red/blue tensor tilt
• Identifying the inflaton with primordial gravitational waves
• B-modes and the sound speed of primordial fluctuations