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Spacetimes Admitting Concircular Curvature Tensor in f(R) Gravity
The main object of this paper is to investigate spacetimes admitting concircular curvature tensor in f ( R ) gravity theory. At first, concircularly flat and concircularly flat perfect fluid spacetimes in f R gravity are studied. In this case, the forms of the isotropic pressure p and the energy den...
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Published in: | Frontiers in physics 2022-01, Vol.9 |
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container_title | Frontiers in physics |
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creator | De, Uday Chand Shenawy, Sameh Abu-Donia, H. M. Turki, Nasser Bin Alsaeed, Suliman Syied, Abdallah Abdelhameed |
description | The main object of this paper is to investigate spacetimes admitting concircular curvature tensor in
f
(
R
) gravity theory. At first, concircularly flat and concircularly flat perfect fluid spacetimes in
f
R
gravity are studied. In this case, the forms of the isotropic pressure
p
and the energy density
σ
are obtained. Next, some energy conditions are considered. Finally, perfect fluid spacetimes with divergence free concircular curvature tensor in
f
(
R
) gravity are studied; amongst many results, it is proved that if the energy-momentum tensor of such spacetimes is recurrent or bi-recurrent, then the Ricci tensor is semi-symmetric and hence these spacetimes either represent inflation or their isotropic pressure and energy density are constants. |
doi_str_mv | 10.3389/fphy.2021.800060 |
format | article |
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f
(
R
) gravity theory. At first, concircularly flat and concircularly flat perfect fluid spacetimes in
f
R
gravity are studied. In this case, the forms of the isotropic pressure
p
and the energy density
σ
are obtained. Next, some energy conditions are considered. Finally, perfect fluid spacetimes with divergence free concircular curvature tensor in
f
(
R
) gravity are studied; amongst many results, it is proved that if the energy-momentum tensor of such spacetimes is recurrent or bi-recurrent, then the Ricci tensor is semi-symmetric and hence these spacetimes either represent inflation or their isotropic pressure and energy density are constants.</description><identifier>ISSN: 2296-424X</identifier><identifier>EISSN: 2296-424X</identifier><identifier>DOI: 10.3389/fphy.2021.800060</identifier><language>eng</language><publisher>Frontiers Media S.A</publisher><subject>concircular curvature tensor ; energy conditions in modified gravity ; energy-momentum tensor ; f (R) gravity theory ; perfect fluid</subject><ispartof>Frontiers in physics, 2022-01, Vol.9</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c1960-ea9bba7e505fd4793e5913ac4712cfd45db6447c01d21e21af3894d46b039cdd3</citedby><cites>FETCH-LOGICAL-c1960-ea9bba7e505fd4793e5913ac4712cfd45db6447c01d21e21af3894d46b039cdd3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>De, Uday Chand</creatorcontrib><creatorcontrib>Shenawy, Sameh</creatorcontrib><creatorcontrib>Abu-Donia, H. M.</creatorcontrib><creatorcontrib>Turki, Nasser Bin</creatorcontrib><creatorcontrib>Alsaeed, Suliman</creatorcontrib><creatorcontrib>Syied, Abdallah Abdelhameed</creatorcontrib><title>Spacetimes Admitting Concircular Curvature Tensor in f(R) Gravity</title><title>Frontiers in physics</title><description>The main object of this paper is to investigate spacetimes admitting concircular curvature tensor in
f
(
R
) gravity theory. At first, concircularly flat and concircularly flat perfect fluid spacetimes in
f
R
gravity are studied. In this case, the forms of the isotropic pressure
p
and the energy density
σ
are obtained. Next, some energy conditions are considered. Finally, perfect fluid spacetimes with divergence free concircular curvature tensor in
f
(
R
) gravity are studied; amongst many results, it is proved that if the energy-momentum tensor of such spacetimes is recurrent or bi-recurrent, then the Ricci tensor is semi-symmetric and hence these spacetimes either represent inflation or their isotropic pressure and energy density are constants.</description><subject>concircular curvature tensor</subject><subject>energy conditions in modified gravity</subject><subject>energy-momentum tensor</subject><subject>f (R) gravity theory</subject><subject>perfect fluid</subject><issn>2296-424X</issn><issn>2296-424X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>DOA</sourceid><recordid>eNpNkEtLAzEUhYMoWGr3LrPUxdS8Z7Isg49CQdAK7kIed2pKO1OSaaH_3qkVcXUuh8sH50PolpIp55V-aHZfxykjjE4rQogiF2jEmFaFYOLz8t99jSY5r4cXyqSumBih2fvOeujjFjKehW3s-9iucN21Pia_39iE63062H6fAC-hzV3CscXN3ds9fk72EPvjDbpq7CbD5DfH6OPpcVm_FIvX53k9WxSeakUKsNo5W4Iksgmi1Bykptx6UVLmh0YGp4QoPaGBUWDUNsMwEYRyhGsfAh-j-ZkbOrs2uxS3Nh1NZ6P5Kbq0Mjb10W_AKOXBSedLKhqhpXQl6EoKpaDi4KAcWOTM8qnLOUHzx6PEnIyak1FzMmrORvk3A1Bplg</recordid><startdate>20220112</startdate><enddate>20220112</enddate><creator>De, Uday Chand</creator><creator>Shenawy, Sameh</creator><creator>Abu-Donia, H. M.</creator><creator>Turki, Nasser Bin</creator><creator>Alsaeed, Suliman</creator><creator>Syied, Abdallah Abdelhameed</creator><general>Frontiers Media S.A</general><scope>AAYXX</scope><scope>CITATION</scope><scope>DOA</scope></search><sort><creationdate>20220112</creationdate><title>Spacetimes Admitting Concircular Curvature Tensor in f(R) Gravity</title><author>De, Uday Chand ; Shenawy, Sameh ; Abu-Donia, H. M. ; Turki, Nasser Bin ; Alsaeed, Suliman ; Syied, Abdallah Abdelhameed</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c1960-ea9bba7e505fd4793e5913ac4712cfd45db6447c01d21e21af3894d46b039cdd3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>concircular curvature tensor</topic><topic>energy conditions in modified gravity</topic><topic>energy-momentum tensor</topic><topic>f (R) gravity theory</topic><topic>perfect fluid</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>De, Uday Chand</creatorcontrib><creatorcontrib>Shenawy, Sameh</creatorcontrib><creatorcontrib>Abu-Donia, H. M.</creatorcontrib><creatorcontrib>Turki, Nasser Bin</creatorcontrib><creatorcontrib>Alsaeed, Suliman</creatorcontrib><creatorcontrib>Syied, Abdallah Abdelhameed</creatorcontrib><collection>CrossRef</collection><collection>DOAJ Directory of Open Access Journals</collection><jtitle>Frontiers in physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>De, Uday Chand</au><au>Shenawy, Sameh</au><au>Abu-Donia, H. M.</au><au>Turki, Nasser Bin</au><au>Alsaeed, Suliman</au><au>Syied, Abdallah Abdelhameed</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Spacetimes Admitting Concircular Curvature Tensor in f(R) Gravity</atitle><jtitle>Frontiers in physics</jtitle><date>2022-01-12</date><risdate>2022</risdate><volume>9</volume><issn>2296-424X</issn><eissn>2296-424X</eissn><abstract>The main object of this paper is to investigate spacetimes admitting concircular curvature tensor in
f
(
R
) gravity theory. At first, concircularly flat and concircularly flat perfect fluid spacetimes in
f
R
gravity are studied. In this case, the forms of the isotropic pressure
p
and the energy density
σ
are obtained. Next, some energy conditions are considered. Finally, perfect fluid spacetimes with divergence free concircular curvature tensor in
f
(
R
) gravity are studied; amongst many results, it is proved that if the energy-momentum tensor of such spacetimes is recurrent or bi-recurrent, then the Ricci tensor is semi-symmetric and hence these spacetimes either represent inflation or their isotropic pressure and energy density are constants.</abstract><pub>Frontiers Media S.A</pub><doi>10.3389/fphy.2021.800060</doi><oa>free_for_read</oa></addata></record> |
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subjects | concircular curvature tensor energy conditions in modified gravity energy-momentum tensor f (R) gravity theory perfect fluid |
title | Spacetimes Admitting Concircular Curvature Tensor in f(R) Gravity |
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