Cosmic-kite: Auto-encoding the cosmic microwave background

Detalhes bibliográficos
Autor(a) principal: De Los Rios, Martín [UNESP]
Data de Publicação: 2022
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1093/mnras/stac393
http://hdl.handle.net/11449/230665
Resumo: In this work, we present the results of the study of the cosmic microwave background temperatureerature power spectrum through auto-encoders in which the latent variables are the cosmological parameters. This method was trained and calibrated using a data set composed of 80 000 power spectra from random cosmologies computed numerically with the camb code. Due to the specific architecture of the auto-encoder, the encoder part is a model that estimates the maximum-likelihood parameters from a given power spectrum. On the other hand, the decoder part is a model that computes the power spectrum from the cosmological parameters and can be used as a forward model in a fully Bayesian analysis. We show that the encoder is able to estimate the true cosmological parameters with a precision varying from ≈ 0.004 per cent to ≈ 0.2 per cent (depending on the cosmological parameter), while the decoder computes the power spectra with a mean percentage error of ≈ 0.0018 per cent for all the multipole range. We also demonstrate that the decoder recovers the expected trends when varying the cosmological parameters one by one, and that it does not introduce any significant bias on the estimation of cosmological parameters through a Bayesian analysis. These studies gave place to the cosmic-kite python software, which is publicly available and can be downloaded and installed from https://github.com/Martindelosrios/cosmic-kite. Although this algorithm does not improve the precision of the measurements compared with the traditional methods, it reduces significantly the computation time and represents the first attempt towards forcing the latent variables to have a physical interpretation.
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spelling Cosmic-kite: Auto-encoding the cosmic microwave backgroundCosmic background radiationMethods: data analysisMethods: statisticalIn this work, we present the results of the study of the cosmic microwave background temperatureerature power spectrum through auto-encoders in which the latent variables are the cosmological parameters. This method was trained and calibrated using a data set composed of 80 000 power spectra from random cosmologies computed numerically with the camb code. Due to the specific architecture of the auto-encoder, the encoder part is a model that estimates the maximum-likelihood parameters from a given power spectrum. On the other hand, the decoder part is a model that computes the power spectrum from the cosmological parameters and can be used as a forward model in a fully Bayesian analysis. We show that the encoder is able to estimate the true cosmological parameters with a precision varying from ≈ 0.004 per cent to ≈ 0.2 per cent (depending on the cosmological parameter), while the decoder computes the power spectra with a mean percentage error of ≈ 0.0018 per cent for all the multipole range. We also demonstrate that the decoder recovers the expected trends when varying the cosmological parameters one by one, and that it does not introduce any significant bias on the estimation of cosmological parameters through a Bayesian analysis. These studies gave place to the cosmic-kite python software, which is publicly available and can be downloaded and installed from https://github.com/Martindelosrios/cosmic-kite. Although this algorithm does not improve the precision of the measurements compared with the traditional methods, it reduces significantly the computation time and represents the first attempt towards forcing the latent variables to have a physical interpretation.Instituto de Física Teórica Universidad Autónoma de Madrid UAM-CSIC, c/Nicolá Cabrera 13-15, CantoblancoDepartamento de Física Teórica Universidad Autónoma de MadridIctp South American Institute for Fundamental Research Instituto de Física Teórica Universidade Estadual Paulista, São Paulo-SPIctp South American Institute for Fundamental Research Instituto de Física Teórica Universidade Estadual Paulista, São Paulo-SPUAM-CSICUniversidad Autónoma de MadridUniversidade Estadual Paulista (UNESP)De Los Rios, Martín [UNESP]2022-04-29T08:41:25Z2022-04-29T08:41:25Z2022-04-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article5525-5535http://dx.doi.org/10.1093/mnras/stac393Monthly Notices of the Royal Astronomical Society, v. 511, n. 4, p. 5525-5535, 2022.1365-29660035-8711http://hdl.handle.net/11449/23066510.1093/mnras/stac3932-s2.0-85127419017Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengMonthly Notices of the Royal Astronomical Societyinfo:eu-repo/semantics/openAccess2022-04-29T08:41:25Zoai:repositorio.unesp.br:11449/230665Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-06T00:14:33.332838Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Cosmic-kite: Auto-encoding the cosmic microwave background
title Cosmic-kite: Auto-encoding the cosmic microwave background
spellingShingle Cosmic-kite: Auto-encoding the cosmic microwave background
De Los Rios, Martín [UNESP]
Cosmic background radiation
Methods: data analysis
Methods: statistical
title_short Cosmic-kite: Auto-encoding the cosmic microwave background
title_full Cosmic-kite: Auto-encoding the cosmic microwave background
title_fullStr Cosmic-kite: Auto-encoding the cosmic microwave background
title_full_unstemmed Cosmic-kite: Auto-encoding the cosmic microwave background
title_sort Cosmic-kite: Auto-encoding the cosmic microwave background
author De Los Rios, Martín [UNESP]
author_facet De Los Rios, Martín [UNESP]
author_role author
dc.contributor.none.fl_str_mv UAM-CSIC
Universidad Autónoma de Madrid
Universidade Estadual Paulista (UNESP)
dc.contributor.author.fl_str_mv De Los Rios, Martín [UNESP]
dc.subject.por.fl_str_mv Cosmic background radiation
Methods: data analysis
Methods: statistical
topic Cosmic background radiation
Methods: data analysis
Methods: statistical
description In this work, we present the results of the study of the cosmic microwave background temperatureerature power spectrum through auto-encoders in which the latent variables are the cosmological parameters. This method was trained and calibrated using a data set composed of 80 000 power spectra from random cosmologies computed numerically with the camb code. Due to the specific architecture of the auto-encoder, the encoder part is a model that estimates the maximum-likelihood parameters from a given power spectrum. On the other hand, the decoder part is a model that computes the power spectrum from the cosmological parameters and can be used as a forward model in a fully Bayesian analysis. We show that the encoder is able to estimate the true cosmological parameters with a precision varying from ≈ 0.004 per cent to ≈ 0.2 per cent (depending on the cosmological parameter), while the decoder computes the power spectra with a mean percentage error of ≈ 0.0018 per cent for all the multipole range. We also demonstrate that the decoder recovers the expected trends when varying the cosmological parameters one by one, and that it does not introduce any significant bias on the estimation of cosmological parameters through a Bayesian analysis. These studies gave place to the cosmic-kite python software, which is publicly available and can be downloaded and installed from https://github.com/Martindelosrios/cosmic-kite. Although this algorithm does not improve the precision of the measurements compared with the traditional methods, it reduces significantly the computation time and represents the first attempt towards forcing the latent variables to have a physical interpretation.
publishDate 2022
dc.date.none.fl_str_mv 2022-04-29T08:41:25Z
2022-04-29T08:41:25Z
2022-04-01
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1093/mnras/stac393
Monthly Notices of the Royal Astronomical Society, v. 511, n. 4, p. 5525-5535, 2022.
1365-2966
0035-8711
http://hdl.handle.net/11449/230665
10.1093/mnras/stac393
2-s2.0-85127419017
url http://dx.doi.org/10.1093/mnras/stac393
http://hdl.handle.net/11449/230665
identifier_str_mv Monthly Notices of the Royal Astronomical Society, v. 511, n. 4, p. 5525-5535, 2022.
1365-2966
0035-8711
10.1093/mnras/stac393
2-s2.0-85127419017
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Monthly Notices of the Royal Astronomical Society
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 5525-5535
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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