Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/10161
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dc.contributor.authorTiwari, Himanshuen_US
dc.contributor.authorMajumdar, Sumanen_US
dc.contributor.authorKamran, Mohden_US
dc.contributor.authorChoudhury, Madhurimaen_US
dc.date.accessioned2022-05-26T15:09:14Z-
dc.date.available2022-05-26T15:09:14Z-
dc.date.issued2022-
dc.identifier.citationTiwari, H., Shaw, A. K., Majumdar, S., Kamran, M., & Choudhury, M. (2022). Improving constraints on the reionization parameters using 21-cm bispectrum. Journal of Cosmology and Astroparticle Physics, 2022(04), 045. https://doi.org/10.1088/1475-7516/2022/04/045en_US
dc.identifier.issn1475-7516-
dc.identifier.otherEID(2-s2.0-85129920504)-
dc.identifier.urihttps://doi.org/10.1088/1475-7516/2022/04/045-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/10161-
dc.description.abstractRadio 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. © 2022 IOP Publishing Ltd and Sissa Medialab.en_US
dc.language.isoenen_US
dc.publisherInstitute of Physicsen_US
dc.sourceJournal of Cosmology and Astroparticle Physicsen_US
dc.subjectBayesian reasoningen_US
dc.subjectMachine learningen_US
dc.subjectnon-gaussianityen_US
dc.subjectreionizationen_US
dc.titleImproving constraints on the reionization parameters using 21-cm bispectrumen_US
dc.typeJournal Articleen_US
dc.rights.licenseAll Open Access, Green-
Appears in Collections:Department of Astronomy, Astrophysics and Space Engineering

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