<i>f</i>(<i>T</i>, <i>B</i>) Cosmography for High Redshifts

<i>f</i>(<i>T</i>, <i>B</i>) Cosmography for High Redshifts

In light of the statistical performance of cosmological observations, in this work we present the cosmography in <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>f</mi><mo>(</mo>...

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Autores principales: Celia Escamilla-Rivera, Geovanny Rave-Franco, Jackson Levi-Said
Formato: article
Lenguaje:EN
Publicado: MDPI AG 2021
Materias:
<i>f</i>(<i>T</i>, <i>B</i>) gravity
teleparallel gravity
cosmography
Elementary particle physics
QC793-793.5
Acceso en línea:https://doaj.org/article/5246dc42d3a34d05a9a06449151826bf
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spelling oai:doaj.org-article:5246dc42d3a34d05a9a06449151826bf2021-11-25T19:09:49Z<i>f</i>(<i>T</i>, <i>B</i>) Cosmography for High Redshifts10.3390/universe71104412218-1997https://doaj.org/article/5246dc42d3a34d05a9a06449151826bf2021-11-01T00:00:00Zhttps://www.mdpi.com/2218-1997/7/11/441https://doaj.org/toc/2218-1997In light of the statistical performance of cosmological observations, in this work we present the cosmography in <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>f</mi><mo>(</mo><mi>T</mi><mo>,</mo><mi>B</mi><mo>)</mo></mrow></semantics></math></inline-formula> gravity. In this scenario we found a cosmological viable standard case that allows the reduction of the degeneracy between several <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>f</mi><mo>(</mo><mi>T</mi><mo>,</mo><mi>B</mi><mo>)</mo></mrow></semantics></math></inline-formula> models already proposed in the literature. Furthermore, we constrain this model using Pantheon SNeIa compilation, cosmic chronometers and a newly GRB calibrated data sample. We found that with an appropriate strategy for including the cosmographic parameter, we do produce a viable cosmology with our model within <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>f</mi><mo>(</mo><mi>T</mi><mo>,</mo><mi>B</mi><mo>)</mo></mrow></semantics></math></inline-formula> gravity.Celia Escamilla-RiveraGeovanny Rave-FrancoJackson Levi-SaidMDPI AGarticle<i>f</i>(<i>T</i>, <i>B</i>) gravityteleparallel gravitycosmographyElementary particle physicsQC793-793.5ENUniverse, Vol 7, Iss 441, p 441 (2021)
institution DOAJ
collection DOAJ
language EN
topic <i>f</i>(<i>T</i>, <i>B</i>) gravity
teleparallel gravity
cosmography
Elementary particle physics
QC793-793.5
spellingShingle <i>f</i>(<i>T</i>, <i>B</i>) gravity
teleparallel gravity
cosmography
Elementary particle physics
QC793-793.5
Celia Escamilla-Rivera
Geovanny Rave-Franco
Jackson Levi-Said
<i>f</i>(<i>T</i>, <i>B</i>) Cosmography for High Redshifts
description In light of the statistical performance of cosmological observations, in this work we present the cosmography in <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>f</mi><mo>(</mo><mi>T</mi><mo>,</mo><mi>B</mi><mo>)</mo></mrow></semantics></math></inline-formula> gravity. In this scenario we found a cosmological viable standard case that allows the reduction of the degeneracy between several <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>f</mi><mo>(</mo><mi>T</mi><mo>,</mo><mi>B</mi><mo>)</mo></mrow></semantics></math></inline-formula> models already proposed in the literature. Furthermore, we constrain this model using Pantheon SNeIa compilation, cosmic chronometers and a newly GRB calibrated data sample. We found that with an appropriate strategy for including the cosmographic parameter, we do produce a viable cosmology with our model within <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>f</mi><mo>(</mo><mi>T</mi><mo>,</mo><mi>B</mi><mo>)</mo></mrow></semantics></math></inline-formula> gravity.
format article
author Celia Escamilla-Rivera
Geovanny Rave-Franco
Jackson Levi-Said
author_facet Celia Escamilla-Rivera
Geovanny Rave-Franco
Jackson Levi-Said
author_sort Celia Escamilla-Rivera
title <i>f</i>(<i>T</i>, <i>B</i>) Cosmography for High Redshifts
title_short <i>f</i>(<i>T</i>, <i>B</i>) Cosmography for High Redshifts
title_full <i>f</i>(<i>T</i>, <i>B</i>) Cosmography for High Redshifts
title_fullStr <i>f</i>(<i>T</i>, <i>B</i>) Cosmography for High Redshifts
title_full_unstemmed <i>f</i>(<i>T</i>, <i>B</i>) Cosmography for High Redshifts
title_sort <i>f</i>(<i>t</i>, <i>b</i>) cosmography for high redshifts
publisher MDPI AG
publishDate 2021
url https://doaj.org/article/5246dc42d3a34d05a9a06449151826bf
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AT geovannyravefranco ifiitiibicosmographyforhighredshifts
AT jacksonlevisaid ifiitiibicosmographyforhighredshifts
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