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Delensing of Cosmic Microwave Background Polarization with Machine Learning
Ist Teil von
The Astrophysical journal. Supplement series, 2023-07, Vol.267 (1), p.2
Ort / Verlag
Saskatoon: The American Astronomical Society
Erscheinungsjahr
2023
Quelle
Free E-Journal (出版社公開部分のみ)
Beschreibungen/Notizen
Abstract
Primordial
B
-mode detection is one of the main goals of next-generation cosmic microwave background (CMB) experiments. Primordial
B
-modes are a unique signature of primordial gravitational waves (PGWs). However, the gravitational interaction of CMB photons with large-scale structures will distort the primordial E modes, adding a lensing
B
-mode component to the primordial
B
-mode signal. Removing the lensing effect (“delensing”) from observed CMB polarization maps will be necessary to improve the constraint of PGWs and obtain a primordial
E
-mode signal. Here, we introduce a deep convolutional neural network model named multi-input multi-output U-net (MIMO-UNet) to perform CMB delensing. The networks are trained on simulated CMB maps with size 20° × 20°. We first use MIMO-UNet to reconstruct the unlensing CMB polarization (
Q
and
U
) maps from observed CMB maps. The recovered
E
-mode power spectrum exhibits excellent agreement with the primordial EE power spectrum. The recovery of the primordial
B
-mode power spectrum for noise levels of 0, 1, and 2
μ
K-arcmin is greater than 98% at the angular scale of
ℓ
< 150. We additionally reconstruct the lensing B map from observed CMB maps. The recovery of the lensing
B
-mode power spectrum is greater than roughly 99% at the scales of
ℓ
> 200. We delens the observed
B
-mode power spectrum by subtracting the reconstructed lensing
B
-mode spectrum. The recovery of tensor
B
-mode power spectrum for noise levels of 0, 1, and 2
μ
K-arcmin is greater than 98% at the angular scales of
ℓ
< 120. Even at
ℓ
= 160, the recovery of tensor
B
-mode power spectrum is still around 71%.