Radio interferometric experiments aim to constrain the reionization model
parameters by measuring the 21-cm signal statistics, primarily the power
spectrum. However the Epoch of Reionization (EoR) 21-cm signal is highly
non-Gaussian, and this non-Gaussianity encodes important information about this
era. The bispectrum is the lowest order statistic able to capture this inherent
non-Gaussianity. Here we are the first to demonstrate that bispectra for large
and intermediate length scales and for all unique $k$-triangle shapes provide
tighter constraints on the EoR parameters compared to the power spectrum or the
bispectra for a limited number of shapes of $k$-triangles. We use the Bayesian
inference technique to constrain EoR parameters. We have also developed an
Artificial Neural Network (ANN) based emulator for the EoR 21-cm power spectrum
and bispectrum which we use to remarkably speed up our parameter inference
pipeline. Here we have considered the sample variance and the system noise
uncertainties corresponding to $1000$ hrs of SKA-Low observations for
estimating errors in the signal statistics. We find that using all unique
$k$-triangle bispectra improves the constraints on parameters by a factor of
$2-4$ (depending on the stage of reionization) over the constraints that are
obtained using power spectrum alone.
Description
Improving constraints on the reionization parameters using 21-cm bispectrum
%0 Generic
%1 tiwari2021improving
%A Tiwari, Himanshu
%A Shaw, Abinash Kumar
%A Majumdar, Suman
%A Kamran, Mohd
%A Choudhury, Madhurima
%D 2021
%K library
%T Improving constraints on the reionization parameters using 21-cm
bispectrum
%U http://arxiv.org/abs/2108.07279
%X Radio interferometric experiments aim to constrain the reionization model
parameters by measuring the 21-cm signal statistics, primarily the power
spectrum. However the Epoch of Reionization (EoR) 21-cm signal is highly
non-Gaussian, and this non-Gaussianity encodes important information about this
era. The bispectrum is the lowest order statistic able to capture this inherent
non-Gaussianity. Here we are the first to demonstrate that bispectra for large
and intermediate length scales and for all unique $k$-triangle shapes provide
tighter constraints on the EoR parameters compared to the power spectrum or the
bispectra for a limited number of shapes of $k$-triangles. We use the Bayesian
inference technique to constrain EoR parameters. We have also developed an
Artificial Neural Network (ANN) based emulator for the EoR 21-cm power spectrum
and bispectrum which we use to remarkably speed up our parameter inference
pipeline. Here we have considered the sample variance and the system noise
uncertainties corresponding to $1000$ hrs of SKA-Low observations for
estimating errors in the signal statistics. We find that using all unique
$k$-triangle bispectra improves the constraints on parameters by a factor of
$2-4$ (depending on the stage of reionization) over the constraints that are
obtained using power spectrum alone.
@misc{tiwari2021improving,
abstract = {Radio interferometric experiments aim to constrain the reionization model
parameters by measuring the 21-cm signal statistics, primarily the power
spectrum. However the Epoch of Reionization (EoR) 21-cm signal is highly
non-Gaussian, and this non-Gaussianity encodes important information about this
era. The bispectrum is the lowest order statistic able to capture this inherent
non-Gaussianity. Here we are the first to demonstrate that bispectra for large
and intermediate length scales and for all unique $k$-triangle shapes provide
tighter constraints on the EoR parameters compared to the power spectrum or the
bispectra for a limited number of shapes of $k$-triangles. We use the Bayesian
inference technique to constrain EoR parameters. We have also developed an
Artificial Neural Network (ANN) based emulator for the EoR 21-cm power spectrum
and bispectrum which we use to remarkably speed up our parameter inference
pipeline. Here we have considered the sample variance and the system noise
uncertainties corresponding to $1000$ hrs of SKA-Low observations for
estimating errors in the signal statistics. We find that using all unique
$k$-triangle bispectra improves the constraints on parameters by a factor of
$2-4$ (depending on the stage of reionization) over the constraints that are
obtained using power spectrum alone.},
added-at = {2021-08-18T06:16:12.000+0200},
author = {Tiwari, Himanshu and Shaw, Abinash Kumar and Majumdar, Suman and Kamran, Mohd and Choudhury, Madhurima},
biburl = {https://www.bibsonomy.org/bibtex/2c8ada532af33f71b6f99aa06529d2d06/gpkulkarni},
description = {Improving constraints on the reionization parameters using 21-cm bispectrum},
interhash = {8d12244752c423f5ff63e2c3cb369786},
intrahash = {c8ada532af33f71b6f99aa06529d2d06},
keywords = {library},
note = {cite arxiv:2108.07279Comment: 13 pages, 9 figures, submitted to MNRAS, comments are welcome},
timestamp = {2021-08-18T06:16:12.000+0200},
title = {Improving constraints on the reionization parameters using 21-cm
bispectrum},
url = {http://arxiv.org/abs/2108.07279},
year = 2021
}