Charged compact stars in %$f({\mathcal {G}})%$ gravity

Abstract This work is devoted to investigate some of the interior configuration of static anisotropic spherical stellar charged structures in the regime of %$f({\mathcal {G}})%$ gravity, where %${\mathcal {G}}%$ is the Gauss Bonnet invariant. The structure of particular charged stars is analyzed wit...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Ilyas, M. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2018

Übergeordnetes Werk:	Enthalten in: The European physical journal - Berlin : Springer, 1998, 78(2018), 9 vom: 20. Sept.
Übergeordnetes Werk:	volume:78 ; year:2018 ; number:9 ; day:20 ; month:09

Links:	Volltext

DOI / URN:	10.1140/epjc/s10052-018-6232-z

Katalog-ID:	SPR008373949

Internformat


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520			\|a Abstract This work is devoted to investigate some of the interior configuration of static anisotropic spherical stellar charged structures in the regime of %$f({\mathcal {G}})%$ gravity, where %${\mathcal {G}}%$ is the Gauss Bonnet invariant. The structure of particular charged stars is analyzed with the help of solution obtained by Krori and Barua under different viable models in %$f({\mathcal {G}})%$ gravity theory. The behavior of some physical aspects is investigated with the help of plots and the viability of our modeling is analyzed through different energy conditions. We have also studied some behavior of these realistic charged compact stars and discuss some aspects like density variation, evolution of stresses, different forces, stability of these stars, measure of anisotropy, equation of state parameters and the distribution of charges.
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Indexfelder

author_variant	m i mi
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allfields	10.1140/epjc/s10052-018-6232-z doi (DE-627)SPR008373949 (SPR)s10052-018-6232-z-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Ilyas, M. verfasserin aut Charged compact stars in %$f({\mathcal {G}})%$ gravity 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract This work is devoted to investigate some of the interior configuration of static anisotropic spherical stellar charged structures in the regime of %$f({\mathcal {G}})%$ gravity, where %${\mathcal {G}}%$ is the Gauss Bonnet invariant. The structure of particular charged stars is analyzed with the help of solution obtained by Krori and Barua under different viable models in %$f({\mathcal {G}})%$ gravity theory. The behavior of some physical aspects is investigated with the help of plots and the viability of our modeling is analyzed through different energy conditions. We have also studied some behavior of these realistic charged compact stars and discuss some aspects like density variation, evolution of stresses, different forces, stability of these stars, measure of anisotropy, equation of state parameters and the distribution of charges. Enthalten in The European physical journal Berlin : Springer, 1998 78(2018), 9 vom: 20. Sept. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:78 year:2018 number:9 day:20 month:09 https://dx.doi.org/10.1140/epjc/s10052-018-6232-z kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 78 2018 9 20 09
spelling	10.1140/epjc/s10052-018-6232-z doi (DE-627)SPR008373949 (SPR)s10052-018-6232-z-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Ilyas, M. verfasserin aut Charged compact stars in %$f({\mathcal {G}})%$ gravity 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract This work is devoted to investigate some of the interior configuration of static anisotropic spherical stellar charged structures in the regime of %$f({\mathcal {G}})%$ gravity, where %${\mathcal {G}}%$ is the Gauss Bonnet invariant. The structure of particular charged stars is analyzed with the help of solution obtained by Krori and Barua under different viable models in %$f({\mathcal {G}})%$ gravity theory. The behavior of some physical aspects is investigated with the help of plots and the viability of our modeling is analyzed through different energy conditions. We have also studied some behavior of these realistic charged compact stars and discuss some aspects like density variation, evolution of stresses, different forces, stability of these stars, measure of anisotropy, equation of state parameters and the distribution of charges. Enthalten in The European physical journal Berlin : Springer, 1998 78(2018), 9 vom: 20. Sept. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:78 year:2018 number:9 day:20 month:09 https://dx.doi.org/10.1140/epjc/s10052-018-6232-z kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 78 2018 9 20 09
allfields_unstemmed	10.1140/epjc/s10052-018-6232-z doi (DE-627)SPR008373949 (SPR)s10052-018-6232-z-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Ilyas, M. verfasserin aut Charged compact stars in %$f({\mathcal {G}})%$ gravity 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract This work is devoted to investigate some of the interior configuration of static anisotropic spherical stellar charged structures in the regime of %$f({\mathcal {G}})%$ gravity, where %${\mathcal {G}}%$ is the Gauss Bonnet invariant. The structure of particular charged stars is analyzed with the help of solution obtained by Krori and Barua under different viable models in %$f({\mathcal {G}})%$ gravity theory. The behavior of some physical aspects is investigated with the help of plots and the viability of our modeling is analyzed through different energy conditions. We have also studied some behavior of these realistic charged compact stars and discuss some aspects like density variation, evolution of stresses, different forces, stability of these stars, measure of anisotropy, equation of state parameters and the distribution of charges. Enthalten in The European physical journal Berlin : Springer, 1998 78(2018), 9 vom: 20. Sept. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:78 year:2018 number:9 day:20 month:09 https://dx.doi.org/10.1140/epjc/s10052-018-6232-z kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 78 2018 9 20 09
allfieldsGer	10.1140/epjc/s10052-018-6232-z doi (DE-627)SPR008373949 (SPR)s10052-018-6232-z-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Ilyas, M. verfasserin aut Charged compact stars in %$f({\mathcal {G}})%$ gravity 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract This work is devoted to investigate some of the interior configuration of static anisotropic spherical stellar charged structures in the regime of %$f({\mathcal {G}})%$ gravity, where %${\mathcal {G}}%$ is the Gauss Bonnet invariant. The structure of particular charged stars is analyzed with the help of solution obtained by Krori and Barua under different viable models in %$f({\mathcal {G}})%$ gravity theory. The behavior of some physical aspects is investigated with the help of plots and the viability of our modeling is analyzed through different energy conditions. We have also studied some behavior of these realistic charged compact stars and discuss some aspects like density variation, evolution of stresses, different forces, stability of these stars, measure of anisotropy, equation of state parameters and the distribution of charges. Enthalten in The European physical journal Berlin : Springer, 1998 78(2018), 9 vom: 20. Sept. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:78 year:2018 number:9 day:20 month:09 https://dx.doi.org/10.1140/epjc/s10052-018-6232-z kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 78 2018 9 20 09
allfieldsSound	10.1140/epjc/s10052-018-6232-z doi (DE-627)SPR008373949 (SPR)s10052-018-6232-z-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Ilyas, M. verfasserin aut Charged compact stars in %$f({\mathcal {G}})%$ gravity 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract This work is devoted to investigate some of the interior configuration of static anisotropic spherical stellar charged structures in the regime of %$f({\mathcal {G}})%$ gravity, where %${\mathcal {G}}%$ is the Gauss Bonnet invariant. The structure of particular charged stars is analyzed with the help of solution obtained by Krori and Barua under different viable models in %$f({\mathcal {G}})%$ gravity theory. The behavior of some physical aspects is investigated with the help of plots and the viability of our modeling is analyzed through different energy conditions. We have also studied some behavior of these realistic charged compact stars and discuss some aspects like density variation, evolution of stresses, different forces, stability of these stars, measure of anisotropy, equation of state parameters and the distribution of charges. Enthalten in The European physical journal Berlin : Springer, 1998 78(2018), 9 vom: 20. Sept. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:78 year:2018 number:9 day:20 month:09 https://dx.doi.org/10.1140/epjc/s10052-018-6232-z kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 78 2018 9 20 09
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author	Ilyas, M.
spellingShingle	Ilyas, M. ddc 530 bkl 33.50 Charged compact stars in %$f({\mathcal {G}})%$ gravity
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title	Charged compact stars in %$f({\mathcal {G}})%$ gravity
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title_full	Charged compact stars in %$f({\mathcal {G}})%$ gravity
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title_sort	charged compact stars in %$f({\mathcal {g}})%$ gravity
title_auth	Charged compact stars in %$f({\mathcal {G}})%$ gravity
abstract	Abstract This work is devoted to investigate some of the interior configuration of static anisotropic spherical stellar charged structures in the regime of %$f({\mathcal {G}})%$ gravity, where %${\mathcal {G}}%$ is the Gauss Bonnet invariant. The structure of particular charged stars is analyzed with the help of solution obtained by Krori and Barua under different viable models in %$f({\mathcal {G}})%$ gravity theory. The behavior of some physical aspects is investigated with the help of plots and the viability of our modeling is analyzed through different energy conditions. We have also studied some behavior of these realistic charged compact stars and discuss some aspects like density variation, evolution of stresses, different forces, stability of these stars, measure of anisotropy, equation of state parameters and the distribution of charges.
abstractGer	Abstract This work is devoted to investigate some of the interior configuration of static anisotropic spherical stellar charged structures in the regime of %$f({\mathcal {G}})%$ gravity, where %${\mathcal {G}}%$ is the Gauss Bonnet invariant. The structure of particular charged stars is analyzed with the help of solution obtained by Krori and Barua under different viable models in %$f({\mathcal {G}})%$ gravity theory. The behavior of some physical aspects is investigated with the help of plots and the viability of our modeling is analyzed through different energy conditions. We have also studied some behavior of these realistic charged compact stars and discuss some aspects like density variation, evolution of stresses, different forces, stability of these stars, measure of anisotropy, equation of state parameters and the distribution of charges.
abstract_unstemmed	Abstract This work is devoted to investigate some of the interior configuration of static anisotropic spherical stellar charged structures in the regime of %$f({\mathcal {G}})%$ gravity, where %${\mathcal {G}}%$ is the Gauss Bonnet invariant. The structure of particular charged stars is analyzed with the help of solution obtained by Krori and Barua under different viable models in %$f({\mathcal {G}})%$ gravity theory. The behavior of some physical aspects is investigated with the help of plots and the viability of our modeling is analyzed through different energy conditions. We have also studied some behavior of these realistic charged compact stars and discuss some aspects like density variation, evolution of stresses, different forces, stability of these stars, measure of anisotropy, equation of state parameters and the distribution of charges.
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title_short	Charged compact stars in %$f({\mathcal {G}})%$ gravity
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score	7.399289

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Charged compact stars in %$f({\mathcal {G}})%$ gravity

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