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Anisotropic compact stars in f(R, A) gravity including charge with exterior Reissner-Nordstrom spacetime
The aim of this manuscript is to investigate the charged anisotropic compact stars in f ( R , A ) theory of gravity, namely Ricci-Inverse gravity. By employing the Karmarkar condition, we construct relativistic anisotropic static spherically symmetric solutions using a particular Adler model for the...
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| Published in: | International journal of theoretical physics 2023-11, Vol.62 (11), Article 243 |
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| Main Authors: | , , |
| Format: | Article |
| Language: | English |
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| container_issue | 11 |
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| container_title | International journal of theoretical physics |
| container_volume | 62 |
| creator | Malik, Adnan Arif, Amna Shamir, M. Farasat |
| description | The aim of this manuscript is to investigate the charged anisotropic compact stars in
f
(
R
,
A
)
theory of gravity, namely Ricci-Inverse gravity. By employing the
Karmarkar
condition, we construct relativistic anisotropic static spherically symmetric solutions using a particular
Adler
model for the
g
tt
metric potential (1974). The exterior geometry is derived following the
Reissner-Nordstrom
spacetime. A series of physical analysis, including
energy density
, pressure elements, and energy conditions, anisotropy, as well as
mass-radius relation
,
compactness
and
redshift
activity, are conducted to assess the viability of the
Ricci-Inverse
gravity model. Our paper discuss the effectiveness of the
f
(
R
,
A
)
gravity model in describing charged anisotropic compact stars provides significant support for massive stars and proves to be suitable for our chosen model. |
| doi_str_mv | 10.1007/s10773-023-05499-2 |
| format | article |
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f
(
R
,
A
)
theory of gravity, namely Ricci-Inverse gravity. By employing the
Karmarkar
condition, we construct relativistic anisotropic static spherically symmetric solutions using a particular
Adler
model for the
g
tt
metric potential (1974). The exterior geometry is derived following the
Reissner-Nordstrom
spacetime. A series of physical analysis, including
energy density
, pressure elements, and energy conditions, anisotropy, as well as
mass-radius relation
,
compactness
and
redshift
activity, are conducted to assess the viability of the
Ricci-Inverse
gravity model. Our paper discuss the effectiveness of the
f
(
R
,
A
)
gravity model in describing charged anisotropic compact stars provides significant support for massive stars and proves to be suitable for our chosen model.</description><identifier>ISSN: 1572-9575</identifier><identifier>EISSN: 1572-9575</identifier><identifier>DOI: 10.1007/s10773-023-05499-2</identifier><language>eng</language><publisher>New York: Springer US</publisher><subject>Elementary Particles ; Mathematical and Computational Physics ; Physics ; Physics and Astronomy ; Quantum Field Theory ; Quantum Physics ; Theoretical</subject><ispartof>International journal of theoretical physics, 2023-11, Vol.62 (11), Article 243</ispartof><rights>The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c291t-e7347383920a071e34e8c990bfd7a8b19cc3c05bf7d9e6a16bbea6a2635bbef23</citedby><cites>FETCH-LOGICAL-c291t-e7347383920a071e34e8c990bfd7a8b19cc3c05bf7d9e6a16bbea6a2635bbef23</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids></links><search><creatorcontrib>Malik, Adnan</creatorcontrib><creatorcontrib>Arif, Amna</creatorcontrib><creatorcontrib>Shamir, M. Farasat</creatorcontrib><title>Anisotropic compact stars in f(R, A) gravity including charge with exterior Reissner-Nordstrom spacetime</title><title>International journal of theoretical physics</title><addtitle>Int J Theor Phys</addtitle><description>The aim of this manuscript is to investigate the charged anisotropic compact stars in
f
(
R
,
A
)
theory of gravity, namely Ricci-Inverse gravity. By employing the
Karmarkar
condition, we construct relativistic anisotropic static spherically symmetric solutions using a particular
Adler
model for the
g
tt
metric potential (1974). The exterior geometry is derived following the
Reissner-Nordstrom
spacetime. A series of physical analysis, including
energy density
, pressure elements, and energy conditions, anisotropy, as well as
mass-radius relation
,
compactness
and
redshift
activity, are conducted to assess the viability of the
Ricci-Inverse
gravity model. Our paper discuss the effectiveness of the
f
(
R
,
A
)
gravity model in describing charged anisotropic compact stars provides significant support for massive stars and proves to be suitable for our chosen model.</description><subject>Elementary Particles</subject><subject>Mathematical and Computational Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Theoretical</subject><issn>1572-9575</issn><issn>1572-9575</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><recordid>eNp9kEtLAzEUhYMoWKt_wFWWCkbzmJlMlqX4gqJQdB0ymTszKZ2ZkqRq_72pdeHKxeUeLvccDh9Cl4zeMkrlXWBUSkEoT5NnShF-hCYsl5yoXObHf_QpOgthRSlVNCsnqJsNLozRjxtnsR37jbERh2h8wG7AzdXyBs-ucevNh4u7dLLrbe2GFtvO-Bbwp4sdhq8I3o0eL8GFMIAnL6OvQwrtcUiBEF0P5-ikMesAF797it4f7t_mT2Tx-vg8ny2I5YpFAlJkUpRCcWqoZCAyKK1StGpqacqKKWuFpXnVyFpBYVhRVWAKwwuRJ9VwMUX8kGv9GIKHRm-8643faUb1npU-sNKJlf5hpfcmcTCF9Dy04PVq3Poh9fzP9Q3QC27Q</recordid><startdate>20231113</startdate><enddate>20231113</enddate><creator>Malik, Adnan</creator><creator>Arif, Amna</creator><creator>Shamir, M. Farasat</creator><general>Springer US</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20231113</creationdate><title>Anisotropic compact stars in f(R, A) gravity including charge with exterior Reissner-Nordstrom spacetime</title><author>Malik, Adnan ; Arif, Amna ; Shamir, M. Farasat</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c291t-e7347383920a071e34e8c990bfd7a8b19cc3c05bf7d9e6a16bbea6a2635bbef23</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Elementary Particles</topic><topic>Mathematical and Computational Physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theory</topic><topic>Quantum Physics</topic><topic>Theoretical</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Malik, Adnan</creatorcontrib><creatorcontrib>Arif, Amna</creatorcontrib><creatorcontrib>Shamir, M. Farasat</creatorcontrib><collection>CrossRef</collection><jtitle>International journal of theoretical physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Malik, Adnan</au><au>Arif, Amna</au><au>Shamir, M. Farasat</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Anisotropic compact stars in f(R, A) gravity including charge with exterior Reissner-Nordstrom spacetime</atitle><jtitle>International journal of theoretical physics</jtitle><stitle>Int J Theor Phys</stitle><date>2023-11-13</date><risdate>2023</risdate><volume>62</volume><issue>11</issue><artnum>243</artnum><issn>1572-9575</issn><eissn>1572-9575</eissn><abstract>The aim of this manuscript is to investigate the charged anisotropic compact stars in
f
(
R
,
A
)
theory of gravity, namely Ricci-Inverse gravity. By employing the
Karmarkar
condition, we construct relativistic anisotropic static spherically symmetric solutions using a particular
Adler
model for the
g
tt
metric potential (1974). The exterior geometry is derived following the
Reissner-Nordstrom
spacetime. A series of physical analysis, including
energy density
, pressure elements, and energy conditions, anisotropy, as well as
mass-radius relation
,
compactness
and
redshift
activity, are conducted to assess the viability of the
Ricci-Inverse
gravity model. Our paper discuss the effectiveness of the
f
(
R
,
A
)
gravity model in describing charged anisotropic compact stars provides significant support for massive stars and proves to be suitable for our chosen model.</abstract><cop>New York</cop><pub>Springer US</pub><doi>10.1007/s10773-023-05499-2</doi></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1572-9575 |
| ispartof | International journal of theoretical physics, 2023-11, Vol.62 (11), Article 243 |
| issn | 1572-9575 1572-9575 |
| language | eng |
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| source | Springer Nature |
| subjects | Elementary Particles Mathematical and Computational Physics Physics Physics and Astronomy Quantum Field Theory Quantum Physics Theoretical |
| title | Anisotropic compact stars in f(R, A) gravity including charge with exterior Reissner-Nordstrom spacetime |
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