Influence of modification of gravity on the complexity factor of static spherical structures
ABSTRACT The aim of this paper is to generalize the definition of complexity for the static self-gravitating structure in f (R, T, Q) gravitational theory, where R is the Ricci scalar, T is the trace part of energy–momentum tensor, and Q ≡ RαβT αβ. In this context, we have considered locally anisotr...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2020, Vol.495 (4), p.4334-4346 |
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creator | Yousaf, Z Khlopov, Maxim Yu Bhatti, M Z Naseer, T |
description | ABSTRACT
The aim of this paper is to generalize the definition of complexity for the static self-gravitating structure in f (R, T, Q) gravitational theory, where R is the Ricci scalar, T is the trace part of energy–momentum tensor, and Q ≡ RαβT αβ. In this context, we have considered locally anisotropic spherical matter distribution and calculated field equations and conservation laws. After the orthogonal splitting of the Riemann curvature tensor, we found the corresponding complexity factor with the help of structure scalars. It is seen that the system may have zero complexity factor if the effects of energy density inhomogeneity and pressure anisotropy cancel the effects of each other. All of our results reduce to general relativity on assuming f (R, T, Q) = R condition. |
doi_str_mv | 10.1093/mnras/staa1470 |
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The aim of this paper is to generalize the definition of complexity for the static self-gravitating structure in f (R, T, Q) gravitational theory, where R is the Ricci scalar, T is the trace part of energy–momentum tensor, and Q ≡ RαβT αβ. In this context, we have considered locally anisotropic spherical matter distribution and calculated field equations and conservation laws. After the orthogonal splitting of the Riemann curvature tensor, we found the corresponding complexity factor with the help of structure scalars. It is seen that the system may have zero complexity factor if the effects of energy density inhomogeneity and pressure anisotropy cancel the effects of each other. All of our results reduce to general relativity on assuming f (R, T, Q) = R condition.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1093/mnras/staa1470</identifier><language>eng</language><publisher>Oxford University Press</publisher><subject>General Relativity and Quantum Cosmology ; High Energy Physics - Theory ; Physics</subject><ispartof>Monthly notices of the Royal Astronomical Society, 2020, Vol.495 (4), p.4334-4346</ispartof><rights>2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society 2020</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c373t-f380a779a836d4a9c86a9207dc59a7bdba2eb16a2c471798bb36a6842ebace2a3</citedby><cites>FETCH-LOGICAL-c373t-f380a779a836d4a9c86a9207dc59a7bdba2eb16a2c471798bb36a6842ebace2a3</cites><orcidid>0000-0002-6286-1135 ; 0000-0001-8227-2621</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,1604,4024,27923,27924,27925</link.rule.ids><linktorsrc>$$Uhttps://dx.doi.org/10.1093/mnras/staa1470$$EView_record_in_Oxford_University_Press$$FView_record_in_$$GOxford_University_Press</linktorsrc><backlink>$$Uhttps://hal.science/hal-02863112$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Yousaf, Z</creatorcontrib><creatorcontrib>Khlopov, Maxim Yu</creatorcontrib><creatorcontrib>Bhatti, M Z</creatorcontrib><creatorcontrib>Naseer, T</creatorcontrib><title>Influence of modification of gravity on the complexity factor of static spherical structures</title><title>Monthly notices of the Royal Astronomical Society</title><description>ABSTRACT
The aim of this paper is to generalize the definition of complexity for the static self-gravitating structure in f (R, T, Q) gravitational theory, where R is the Ricci scalar, T is the trace part of energy–momentum tensor, and Q ≡ RαβT αβ. In this context, we have considered locally anisotropic spherical matter distribution and calculated field equations and conservation laws. After the orthogonal splitting of the Riemann curvature tensor, we found the corresponding complexity factor with the help of structure scalars. It is seen that the system may have zero complexity factor if the effects of energy density inhomogeneity and pressure anisotropy cancel the effects of each other. All of our results reduce to general relativity on assuming f (R, T, Q) = R condition.</description><subject>General Relativity and Quantum Cosmology</subject><subject>High Energy Physics - Theory</subject><subject>Physics</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNqFkL1PwzAUxC0EEqWwMmdlSOuPxHbGqgJaqRILbEjWi-NQoySObKei_z0J5WNkerqf7u5Jh9AtwQuCC7ZsOw9hGSIAyQQ-QzPCeJ7SgvNzNMOY5akUhFyiqxDeMcYZo3yGXrdd3Qym0yZxddK6ytZWQ7Sum_Sbh4ONx2RUcW8S7dq-MR8TqUFH5yfP-DBanYR-b_wYbUbgBx0Hb8I1uqihCebm-87Ry8P983qT7p4et-vVLtVMsJjWTGIQogDJeJVBoSWHgmJR6bwAUVYlUFMSDlRngohCliXjwGU2UtCGApuju1PvHhrVe9uCPyoHVm1WOzUxTCVnhNADGb2Lk1d7F4I39W-AYDXtqL52VD87_pW7of_P-wm8rng7</recordid><startdate>2020</startdate><enddate>2020</enddate><creator>Yousaf, Z</creator><creator>Khlopov, Maxim Yu</creator><creator>Bhatti, M Z</creator><creator>Naseer, T</creator><general>Oxford University Press</general><general>Oxford University Press (OUP): Policy P - Oxford Open Option A</general><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0002-6286-1135</orcidid><orcidid>https://orcid.org/0000-0001-8227-2621</orcidid></search><sort><creationdate>2020</creationdate><title>Influence of modification of gravity on the complexity factor of static spherical structures</title><author>Yousaf, Z ; Khlopov, Maxim Yu ; Bhatti, M Z ; Naseer, T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c373t-f380a779a836d4a9c86a9207dc59a7bdba2eb16a2c471798bb36a6842ebace2a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>General Relativity and Quantum Cosmology</topic><topic>High Energy Physics - Theory</topic><topic>Physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Yousaf, Z</creatorcontrib><creatorcontrib>Khlopov, Maxim Yu</creatorcontrib><creatorcontrib>Bhatti, M Z</creatorcontrib><creatorcontrib>Naseer, T</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Yousaf, Z</au><au>Khlopov, Maxim Yu</au><au>Bhatti, M Z</au><au>Naseer, T</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Influence of modification of gravity on the complexity factor of static spherical structures</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>2020</date><risdate>2020</risdate><volume>495</volume><issue>4</issue><spage>4334</spage><epage>4346</epage><pages>4334-4346</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>ABSTRACT
The aim of this paper is to generalize the definition of complexity for the static self-gravitating structure in f (R, T, Q) gravitational theory, where R is the Ricci scalar, T is the trace part of energy–momentum tensor, and Q ≡ RαβT αβ. In this context, we have considered locally anisotropic spherical matter distribution and calculated field equations and conservation laws. After the orthogonal splitting of the Riemann curvature tensor, we found the corresponding complexity factor with the help of structure scalars. It is seen that the system may have zero complexity factor if the effects of energy density inhomogeneity and pressure anisotropy cancel the effects of each other. All of our results reduce to general relativity on assuming f (R, T, Q) = R condition.</abstract><pub>Oxford University Press</pub><doi>10.1093/mnras/staa1470</doi><tpages>13</tpages><orcidid>https://orcid.org/0000-0002-6286-1135</orcidid><orcidid>https://orcid.org/0000-0001-8227-2621</orcidid></addata></record> |
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subjects | General Relativity and Quantum Cosmology High Energy Physics - Theory Physics |
title | Influence of modification of gravity on the complexity factor of static spherical structures |
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