Measuring primordial anisotropic correlators with CMB spectral distortions
arXiv:1506.06670 · doi:10.1103/PhysRevD.92.083502
Abstract
We show that inflationary models with broken rotational invariance generate testable off-diagonal signatures in the correlation between the -type distortion and temperature fluctuations of the cosmic microwave background. More precisely, scenarios with a quadrupolar bispectrum asymmetry, usually generated by fluctuations of primordial vector fields, produce a nonvanishing - correlation when . Since spectral distortions are sensitive to primordial fluctuations up to very small scales, a cosmic variance limited spectral distortion experiment can detect such effects with a high signal-to-noise ratio.
9 pages, 3 figures. Accepted for publication in PRD
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- Exploring Cosmic Origins with CORE: Inflation
- Testing the Early Universe with Anisotropies of the Gravitational Wave Background
- Polypolar spherical harmonic decomposition of galaxy correlators in redshift space: Toward testing cosmic rotational symmetry
- Primordial trispectra and CMB spectral distortions
- Induced superhorizon tensor perturbations from anisotropic non-Gaussianity
- Violation of statistical isotropy and homogeneity in the 21-cm power spectrum
- Primordial non-Gaussianity with -type and -type spectral distortions: exploiting Cosmic Microwave Background polarization and dealing with secondary sources
- Correlating CMB Spectral Distortions with Temperature: what do we learn on Inflation?
- Angular dependence of primordial trispectra and CMB spectral distortions
- Primordial tensor bispectra in -CMB cross-correlations
- Leverage on small-scale primordial non-Gaussianity through cross-correlations between CMB -mode and -distortion anisotropies
- Testing the scale-dependent hemispherical asymmetry with the 21-cm power spectrum from the epoch of reionization
- Statistical anisotropy in CMB spectral distortions
- Testing kinetically coupled inflation models with CMB distortions
- CMB spectroscopy at third-order in cosmological perturbations