Combining power spectrum and bispectrum measurements to detect oscillatory features
arXiv:1410.5114 · doi:10.1103/PhysRevD.91.023502
Abstract
The simplest inflationary models present us with few observable parameters to discriminate between them. A detection of features in the spectra of primordial density perturbations could provide valuable insights and lead to stringent tests of models of the early Universe. So far, searches for oscillatory features have not produced statistically significant results. In this work we consider a combined search for features in the power spectrum and bispectrum. We show that possible dependencies between the estimates of feature model amplitudes based on the two- and three-point correlators are largely statistically independent under the assumption of the null hypothesis of a nearly Gaussian featureless CMB. Building on this conclusion we propose an optimal amplitude estimator for a combined search and study the look-elsewhere effect in feature model surveys. In particular we construct analytic models for the distribution of amplitude estimates that allow for a reliable assessment of the significance of potential findings. We also propose a well-behaved integrated statistic that is designed to detect evidence for models exhibiting features at multiple frequencies.
v1: 20 pages, 14 figures; v2: references added, typos corrected, minor changes in introduction; v3: minor changes to match the published version
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- Untangling features in the primordial spectra
- Primordial Non-Gaussianity
- Searching for Cosmological Collider in the Planck CMB Data
- An optimal estimator for resonance bispectra in the CMB
- A Cosmological Bootstrap for Resonant Non-Gaussianity
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- Primordial feature constraints from BOSS+eBOSS
- High-resolution CMB bispectrum estimator with flexible modal basis
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- Investigating the Constraints on Primordial Features with Future Cosmic Microwave Background and Galaxy Surveys
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