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• W3214156927 endingPage "14" @default.
• W3214156927 startingPage "1" @default.
• W3214156927 abstract "The main aim of our study is to explore some relativistic configurations of compact object solution in the background of <math xmlns=http://www.w3.org/1998/Math/MathML id=M2> <mi>f</mi> <mfenced open=( close=)> <mrow> <mi>R</mi> </mrow> </mfenced> </math> gravity, by adopting the Krori-Barua spacetime. In this regard, we establish the field equations for spherically symmetric spacetime along with charged anisotropic matter source by assuming the specific form of the metric potentials, i.e., <math xmlns=http://www.w3.org/1998/Math/MathML id=M3> <mi>ν</mi> <mfenced open=( close=)> <mrow> <mi>r</mi> </mrow> </mfenced> <mo>=</mo> <mi>B</mi> <msup> <mrow> <mi>r</mi> </mrow> <mrow> <mn>2</mn> </mrow> </msup> <mo>+</mo> <mi>C</mi> </math> and <math xmlns=http://www.w3.org/1998/Math/MathML id=M4> <mi>λ</mi> <mfenced open=( close=)> <mrow> <mi>r</mi> </mrow> </mfenced> <mo>=</mo> <mi>A</mi> <msup> <mrow> <mi>r</mi> </mrow> <mrow> <mn>2</mn> </mrow> </msup> </math> . Further, to calculate the constant values, we consider the Bardeen model as an exterior spacetime at the surface boundary. To ensure the viability of the <math xmlns=http://www.w3.org/1998/Math/MathML id=M5> <mi>f</mi> <mfenced open=( close=)> <mrow> <mi>R</mi> </mrow> </mfenced> </math> gravity model, the physical characteristics including energy density, pressure components, energy bonds, equilibrium condition, Herrera cracking concept, mass-radius relation, and adiabatic index are analyzed in detail. It is observed that all the outcomes by graphical exploration and tabular figures show that the Bardeen black hole model describes the physically realistic stellar structures." @default.
• W3214156927 created "2021-11-22" @default.
• W3214156927 creator A5029116825 @default.
• W3214156927 creator A5053086418 @default.
• W3214156927 creator A5064333061 @default.
• W3214156927 date "2021-11-17" @default.
• W3214156927 modified "2023-10-18" @default.
• W3214156927 title "Physical Attributes of Bardeen Stellar Structures in f R Gravity" @default.
• W3214156927 cites W1145642073 @default.
• W3214156927 cites W1485308145 @default.
• W3214156927 cites W1964461841 @default.
• W3214156927 cites W1964597263 @default.
• W3214156927 cites W1965657937 @default.
• W3214156927 cites W1970329710 @default.
• W3214156927 cites W1972268597 @default.
• W3214156927 cites W1972357349 @default.
• W3214156927 cites W1974832459 @default.
• W3214156927 cites W1979584221 @default.
• W3214156927 cites W1981305761 @default.
• W3214156927 cites W1983131591 @default.
• W3214156927 cites W1990620034 @default.
• W3214156927 cites W1992753446 @default.
• W3214156927 cites W2003636313 @default.
• W3214156927 cites W2004058932 @default.
• W3214156927 cites W2004493956 @default.
• W3214156927 cites W2005633297 @default.
• W3214156927 cites W2006350945 @default.
• W3214156927 cites W2007479791 @default.
• W3214156927 cites W2012139916 @default.
• W3214156927 cites W2012535746 @default.
• W3214156927 cites W2013062057 @default.
• W3214156927 cites W2014571316 @default.
• W3214156927 cites W2023126263 @default.
• W3214156927 cites W2024441041 @default.
• W3214156927 cites W2027052805 @default.
• W3214156927 cites W2027933892 @default.
• W3214156927 cites W2029403139 @default.
• W3214156927 cites W2030489439 @default.
• W3214156927 cites W2033562931 @default.
• W3214156927 cites W2034158615 @default.
• W3214156927 cites W2036662279 @default.
• W3214156927 cites W2037195717 @default.
• W3214156927 cites W2039130581 @default.
• W3214156927 cites W2041664594 @default.
• W3214156927 cites W2041766951 @default.
• W3214156927 cites W2044912559 @default.
• W3214156927 cites W2048446165 @default.
• W3214156927 cites W2050551135 @default.
• W3214156927 cites W2052080007 @default.
• W3214156927 cites W2058562197 @default.
• W3214156927 cites W2058734209 @default.
• W3214156927 cites W2063936939 @default.
• W3214156927 cites W2064074968 @default.
• W3214156927 cites W2065626203 @default.
• W3214156927 cites W2066155353 @default.
• W3214156927 cites W2069017641 @default.
• W3214156927 cites W2070540953 @default.
• W3214156927 cites W2070854247 @default.
• W3214156927 cites W2071863200 @default.
• W3214156927 cites W2078125471 @default.
• W3214156927 cites W2079674788 @default.
• W3214156927 cites W2081318224 @default.
• W3214156927 cites W2081691279 @default.
• W3214156927 cites W2085610153 @default.
• W3214156927 cites W2086567204 @default.
• W3214156927 cites W2094740723 @default.
• W3214156927 cites W2099192770 @default.
• W3214156927 cites W2100641107 @default.
• W3214156927 cites W2102716046 @default.
• W3214156927 cites W2103355709 @default.
• W3214156927 cites W2105364155 @default.
• W3214156927 cites W2106127715 @default.
• W3214156927 cites W2109243620 @default.
• W3214156927 cites W2111042150 @default.
• W3214156927 cites W2115623495 @default.
• W3214156927 cites W2119220636 @default.
• W3214156927 cites W2120371558 @default.
• W3214156927 cites W2127521893 @default.
• W3214156927 cites W2131839868 @default.
• W3214156927 cites W2139440433 @default.
• W3214156927 cites W2143114981 @default.
• W3214156927 cites W2145568712 @default.
• W3214156927 cites W2147088395 @default.
• W3214156927 cites W2154748230 @default.
• W3214156927 cites W2168527615 @default.
• W3214156927 cites W2209377845 @default.
• W3214156927 cites W2225468140 @default.
• W3214156927 cites W2258743878 @default.
• W3214156927 cites W2500302874 @default.
• W3214156927 cites W2593232323 @default.
• W3214156927 cites W2657866703 @default.
• W3214156927 cites W2735931983 @default.
• W3214156927 cites W2964048743 @default.
• W3214156927 cites W2998664116 @default.
• W3214156927 cites W3000177939 @default.
• W3214156927 cites W3020648868 @default.
• W3214156927 cites W3022804291 @default.
• W3214156927 cites W3034606379 @default.

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