CMB internal delensing with general optimal estimator for higher-order correlations
arXiv:1703.00169 · doi:10.1103/PhysRevD.95.103514
Abstract
We present a new method for delensing modes of the cosmic microwave background (CMB) using a lensing potential reconstructed from the same realization of the CMB polarization (CMB internal delensing). The -mode delensing is required to improve sensitivity to primary modes generated by, e.g., the inflationary gravitational waves, axion-like particles, modified gravity, primordial magnetic fields, and topological defects such as cosmic strings. However, the CMB internal delensing suffers from substantial biases due to correlations between observed CMB maps to be delensed and that used for reconstructing a lensing potential. We construct a realization-dependent (RD) estimator for correcting these biases by deriving a general optimal estimator for higher-order correlations. The RD estimator is less sensitive to simulation uncertainties. Compared to the previous methods, we find that the RD estimator corrects the biases without substantial degradation of the delensing efficiency.
18 pages, 8 figures, accepted for publication in PRD
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- Future cosmic microwave background delensing with galaxy surveys
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- Optimal constraints on primordial gravitational waves from the lensed CMB
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- CMB Mode Coupling with Isotropic Polarization Rotation
- A numerical study of observational systematic errors in lensing analysis of CMB polarization
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- The reconstructed CMB lensing bispectrum
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- LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data