Accurate and Unbiased Reconstruction of CMB B Mode using Deep Learning

Fuente: arXiv
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Auteurs principaux: Pal, Srikanta, Yadav, Sarvesh Kumar, Saha, Rajib, Souradeep, Tarun
Format: Preprint
Publié: 2024
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author Pal, Srikanta
Yadav, Sarvesh Kumar
Saha, Rajib
Souradeep, Tarun
author_facet Pal, Srikanta
Yadav, Sarvesh Kumar
Saha, Rajib
Souradeep, Tarun
contents An ingeniously designed autoencoder (PrimeNet) using simulated observations of future generation ECHO satellite mission recovers CMB B mode map, angular spectrum for multipoles $\ell \lesssim 9$ and tensor to scalar ratio $r$ {\it limited only by cosmic variance down to $r= 0.0001$ and below}. We use diverse, realistically complex and detailed foreground models. PrimeNet predicts accurate results even when data with $r=0$ are tested which were not used in training, implying robust and efficient predictive power. The work eliminates a major bottleneck of weak CMB B mode reconstruction and takes a leap forward for understanding fundamental physics of the primordial Universe.
format Preprint
id arxiv_https___arxiv_org_abs_2404_18100
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Accurate and Unbiased Reconstruction of CMB B Mode using Deep Learning
Pal, Srikanta
Yadav, Sarvesh Kumar
Saha, Rajib
Souradeep, Tarun
Cosmology and Nongalactic Astrophysics
An ingeniously designed autoencoder (PrimeNet) using simulated observations of future generation ECHO satellite mission recovers CMB B mode map, angular spectrum for multipoles $\ell \lesssim 9$ and tensor to scalar ratio $r$ {\it limited only by cosmic variance down to $r= 0.0001$ and below}. We use diverse, realistically complex and detailed foreground models. PrimeNet predicts accurate results even when data with $r=0$ are tested which were not used in training, implying robust and efficient predictive power. The work eliminates a major bottleneck of weak CMB B mode reconstruction and takes a leap forward for understanding fundamental physics of the primordial Universe.
title Accurate and Unbiased Reconstruction of CMB B Mode using Deep Learning
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2404.18100