Revisiting cosmic microwave background radiation using blackbody radiation inversion

Abstract Blackbody radiation inversion is a mathematical process for the determination of probability distribution of temperature from measured radiated power spectrum. In this paper a simple and stable blackbody radiation inversion is achieved by using an analytical function with three determinable...

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Autores principales: Koustav Konar, Kingshuk Bose, R. K. Paul
Formato: article
Lenguaje:EN
Publicado: Nature Portfolio 2021
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Acceso en línea:https://doaj.org/article/d794c720be9f4d788656105d2f5ec35a
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spelling oai:doaj.org-article:d794c720be9f4d788656105d2f5ec35a2021-12-02T14:12:10ZRevisiting cosmic microwave background radiation using blackbody radiation inversion10.1038/s41598-020-80195-32045-2322https://doaj.org/article/d794c720be9f4d788656105d2f5ec35a2021-01-01T00:00:00Zhttps://doi.org/10.1038/s41598-020-80195-3https://doaj.org/toc/2045-2322Abstract Blackbody radiation inversion is a mathematical process for the determination of probability distribution of temperature from measured radiated power spectrum. In this paper a simple and stable blackbody radiation inversion is achieved by using an analytical function with three determinable parameters for temperature distribution. This inversion technique is used to invert the blackbody radiation field of the cosmic microwave background, the remnant radiation of the hot big bang, to infer the temperature distribution of the generating medium. The salient features of this distribution are investigated and analysis of this distribution predicts the presence of distortion in the cosmic microwave background spectrum.Koustav KonarKingshuk BoseR. K. PaulNature PortfolioarticleMedicineRScienceQENScientific Reports, Vol 11, Iss 1, Pp 1-9 (2021)
institution DOAJ
collection DOAJ
language EN
topic Medicine
R
Science
Q
spellingShingle Medicine
R
Science
Q
Koustav Konar
Kingshuk Bose
R. K. Paul
Revisiting cosmic microwave background radiation using blackbody radiation inversion
description Abstract Blackbody radiation inversion is a mathematical process for the determination of probability distribution of temperature from measured radiated power spectrum. In this paper a simple and stable blackbody radiation inversion is achieved by using an analytical function with three determinable parameters for temperature distribution. This inversion technique is used to invert the blackbody radiation field of the cosmic microwave background, the remnant radiation of the hot big bang, to infer the temperature distribution of the generating medium. The salient features of this distribution are investigated and analysis of this distribution predicts the presence of distortion in the cosmic microwave background spectrum.
format article
author Koustav Konar
Kingshuk Bose
R. K. Paul
author_facet Koustav Konar
Kingshuk Bose
R. K. Paul
author_sort Koustav Konar
title Revisiting cosmic microwave background radiation using blackbody radiation inversion
title_short Revisiting cosmic microwave background radiation using blackbody radiation inversion
title_full Revisiting cosmic microwave background radiation using blackbody radiation inversion
title_fullStr Revisiting cosmic microwave background radiation using blackbody radiation inversion
title_full_unstemmed Revisiting cosmic microwave background radiation using blackbody radiation inversion
title_sort revisiting cosmic microwave background radiation using blackbody radiation inversion
publisher Nature Portfolio
publishDate 2021
url https://doaj.org/article/d794c720be9f4d788656105d2f5ec35a
work_keys_str_mv AT koustavkonar revisitingcosmicmicrowavebackgroundradiationusingblackbodyradiationinversion
AT kingshukbose revisitingcosmicmicrowavebackgroundradiationusingblackbodyradiationinversion
AT rkpaul revisitingcosmicmicrowavebackgroundradiationusingblackbodyradiationinversion
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