LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
M. Ruiz-Granda, P. Diego-Palazuelos, C. Gimeno-Amo, P. Vielva, A. I. Lonappan, T. Namikawa, R. T. G\'enova-Santos, M. Lembo, R. Nagata, M. Remazeilles, D. Adak, E. Allys, A. Anand, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, R. B. Barreiro, N. Bartolo, S. Basak

TL;DR
This paper forecasts that combining LiteBIRD and Planck data will significantly enhance full-sky gravitational lensing maps, leading to better cosmological constraints and improved delensing capabilities for future CMB studies.
Contribution
It introduces an improved method for reconstructing the CMB lensing potential by combining LiteBIRD and Planck data, nearly doubling the sensitivity of previous measurements.
Findings
Enhanced lensing detection significance (49-58σ with LiteBIRD alone)
Combined data will achieve 72-78σ detection, nearly doubling Planck's sensitivity
Improved constraints on cosmological parameters, including a factor of 2 better S8 and 6% improvement in tensor-to-scalar ratio
Abstract
Cosmic microwave background (CMB) photons are deflected by large-scale structure through gravitational lensing. This secondary effect introduces higher-order correlations in CMB anisotropies, which are used to reconstruct lensing deflections. This allows mapping of the integrated matter distribution along the line of sight, probing the growth of structure, and recovering an undistorted view of the last-scattering surface. Gravitational lensing has been measured by previous CMB experiments, with 's detection being the current best full-sky lensing map. We present an enhanced lensing map by extending the CMB multipole range and including the minimum-variance estimation, leading to a to detection over of the sky, depending on the final complexity of polarized Galactic emission. The combination of …
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