From the early to the late time universe within \(f(T,\mathcal{T})\) gravity

In this paper we perform the reconstruction scheme of the gravitational action within \(f(T,\mathcal{T})\) gravity, where \(T\) and \(\mathcal{T}\) denote the torsion scalar and the trace of the energy momentum tensor, respectively. We particularly focus our attention on the case where the algebraic...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:arXiv.org 2015-06
Hauptverfasser: Nassur, S B, Houndjo, M J S, Kpadonou, A V, Rodrigues, M E, Tossa, J
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Nassur, S B
Houndjo, M J S
Kpadonou, A V
Rodrigues, M E
Tossa, J
description In this paper we perform the reconstruction scheme of the gravitational action within \(f(T,\mathcal{T})\) gravity, where \(T\) and \(\mathcal{T}\) denote the torsion scalar and the trace of the energy momentum tensor, respectively. We particularly focus our attention on the case where the algebraic function \(f(T,\mathcal{T})\) is decomposed as a sum of two functions \(f_1(T)\) and \(f_2(\mathcal{T})\), i.e, \(f(T,\mathcal{T})=f_{1}(T)+f_{2}(\mathcal{T})\). The description is essentially based on the scale factor and then, we consider two interesting and realistic expressions of this parameter and reconstruct the action corresponding to each phase of the universe. Our results show that some \(f(T,\mathcal{T})\) models are able to describe the evolution of the universe from the inflation phase to the late time dark energy dominated phase.
doi_str_mv 10.48550/arxiv.1506.09161
format Article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2078576991</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2078576991</sourcerecordid><originalsourceid>FETCH-proquest_journals_20785769913</originalsourceid><addsrcrecordid>eNqNik0LgjAAQEcQJOUP6DboopC2TTf1HEmHjh4FGTFz4kdt05LovxfRD-j0eLwHwBojP4wpRTuuHnL0MUXMRwlmeAYsEgTYi0NCFsDWukYIERYRSgMLnFLVt9BUAgqumgma_isNNwIa2Qo4dHIUSgt4l6aSHcyd0sm2ectNdebNM3u5uQsvio_STCswL3mjhf3jEmzSQ7Y_elfV3wahTVH3g-o-qSAoimnEkgQH_11v_lZC5A</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2078576991</pqid></control><display><type>article</type><title>From the early to the late time universe within \(f(T,\mathcal{T})\) gravity</title><source>Free E- Journals</source><creator>Nassur, S B ; Houndjo, M J S ; Kpadonou, A V ; Rodrigues, M E ; Tossa, J</creator><creatorcontrib>Nassur, S B ; Houndjo, M J S ; Kpadonou, A V ; Rodrigues, M E ; Tossa, J</creatorcontrib><description>In this paper we perform the reconstruction scheme of the gravitational action within \(f(T,\mathcal{T})\) gravity, where \(T\) and \(\mathcal{T}\) denote the torsion scalar and the trace of the energy momentum tensor, respectively. We particularly focus our attention on the case where the algebraic function \(f(T,\mathcal{T})\) is decomposed as a sum of two functions \(f_1(T)\) and \(f_2(\mathcal{T})\), i.e, \(f(T,\mathcal{T})=f_{1}(T)+f_{2}(\mathcal{T})\). The description is essentially based on the scale factor and then, we consider two interesting and realistic expressions of this parameter and reconstruct the action corresponding to each phase of the universe. Our results show that some \(f(T,\mathcal{T})\) models are able to describe the evolution of the universe from the inflation phase to the late time dark energy dominated phase.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1506.09161</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Astronomical models ; Dark energy ; Gravitation ; Tensors ; Universe</subject><ispartof>arXiv.org, 2015-06</ispartof><rights>2015. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>776,780,27902</link.rule.ids></links><search><creatorcontrib>Nassur, S B</creatorcontrib><creatorcontrib>Houndjo, M J S</creatorcontrib><creatorcontrib>Kpadonou, A V</creatorcontrib><creatorcontrib>Rodrigues, M E</creatorcontrib><creatorcontrib>Tossa, J</creatorcontrib><title>From the early to the late time universe within \(f(T,\mathcal{T})\) gravity</title><title>arXiv.org</title><description>In this paper we perform the reconstruction scheme of the gravitational action within \(f(T,\mathcal{T})\) gravity, where \(T\) and \(\mathcal{T}\) denote the torsion scalar and the trace of the energy momentum tensor, respectively. We particularly focus our attention on the case where the algebraic function \(f(T,\mathcal{T})\) is decomposed as a sum of two functions \(f_1(T)\) and \(f_2(\mathcal{T})\), i.e, \(f(T,\mathcal{T})=f_{1}(T)+f_{2}(\mathcal{T})\). The description is essentially based on the scale factor and then, we consider two interesting and realistic expressions of this parameter and reconstruct the action corresponding to each phase of the universe. Our results show that some \(f(T,\mathcal{T})\) models are able to describe the evolution of the universe from the inflation phase to the late time dark energy dominated phase.</description><subject>Astronomical models</subject><subject>Dark energy</subject><subject>Gravitation</subject><subject>Tensors</subject><subject>Universe</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNqNik0LgjAAQEcQJOUP6DboopC2TTf1HEmHjh4FGTFz4kdt05LovxfRD-j0eLwHwBojP4wpRTuuHnL0MUXMRwlmeAYsEgTYi0NCFsDWukYIERYRSgMLnFLVt9BUAgqumgma_isNNwIa2Qo4dHIUSgt4l6aSHcyd0sm2ectNdebNM3u5uQsvio_STCswL3mjhf3jEmzSQ7Y_elfV3wahTVH3g-o-qSAoimnEkgQH_11v_lZC5A</recordid><startdate>20150617</startdate><enddate>20150617</enddate><creator>Nassur, S B</creator><creator>Houndjo, M J S</creator><creator>Kpadonou, A V</creator><creator>Rodrigues, M E</creator><creator>Tossa, J</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20150617</creationdate><title>From the early to the late time universe within \(f(T,\mathcal{T})\) gravity</title><author>Nassur, S B ; Houndjo, M J S ; Kpadonou, A V ; Rodrigues, M E ; Tossa, J</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20785769913</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Astronomical models</topic><topic>Dark energy</topic><topic>Gravitation</topic><topic>Tensors</topic><topic>Universe</topic><toplevel>online_resources</toplevel><creatorcontrib>Nassur, S B</creatorcontrib><creatorcontrib>Houndjo, M J S</creatorcontrib><creatorcontrib>Kpadonou, A V</creatorcontrib><creatorcontrib>Rodrigues, M E</creatorcontrib><creatorcontrib>Tossa, J</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Nassur, S B</au><au>Houndjo, M J S</au><au>Kpadonou, A V</au><au>Rodrigues, M E</au><au>Tossa, J</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>From the early to the late time universe within \(f(T,\mathcal{T})\) gravity</atitle><jtitle>arXiv.org</jtitle><date>2015-06-17</date><risdate>2015</risdate><eissn>2331-8422</eissn><abstract>In this paper we perform the reconstruction scheme of the gravitational action within \(f(T,\mathcal{T})\) gravity, where \(T\) and \(\mathcal{T}\) denote the torsion scalar and the trace of the energy momentum tensor, respectively. We particularly focus our attention on the case where the algebraic function \(f(T,\mathcal{T})\) is decomposed as a sum of two functions \(f_1(T)\) and \(f_2(\mathcal{T})\), i.e, \(f(T,\mathcal{T})=f_{1}(T)+f_{2}(\mathcal{T})\). The description is essentially based on the scale factor and then, we consider two interesting and realistic expressions of this parameter and reconstruct the action corresponding to each phase of the universe. Our results show that some \(f(T,\mathcal{T})\) models are able to describe the evolution of the universe from the inflation phase to the late time dark energy dominated phase.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1506.09161</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2015-06
issn 2331-8422
language eng
recordid cdi_proquest_journals_2078576991
source Free E- Journals
subjects Astronomical models
Dark energy
Gravitation
Tensors
Universe
title From the early to the late time universe within \(f(T,\mathcal{T})\) gravity
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-28T17%3A30%3A10IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=From%20the%20early%20to%20the%20late%20time%20universe%20within%20%5C(f(T,%5Cmathcal%7BT%7D)%5C)%20gravity&rft.jtitle=arXiv.org&rft.au=Nassur,%20S%20B&rft.date=2015-06-17&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1506.09161&rft_dat=%3Cproquest%3E2078576991%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2078576991&rft_id=info:pmid/&rfr_iscdi=true