FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4220854312> ?p ?o ?g. }

• W4220854312 endingPage "055004" @default.
• W4220854312 startingPage "055004" @default.
• W4220854312 abstract "Abstract This paper investigates some particular anisotropic star models in <?CDATA $f({ mathcal R },{ mathcal T },{ mathcal Q })$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mi>f</mml:mi> <mml:mo stretchy=false>(</mml:mo> <mml:mi mathvariant=italic></mml:mi> <mml:mo>,</mml:mo> <mml:mi mathvariant=italic></mml:mi> <mml:mo>,</mml:mo> <mml:mi mathvariant=italic></mml:mi> <mml:mo stretchy=false>)</mml:mo> </mml:math> gravity, where <?CDATA ${ mathcal Q }={{ mathcal R }}_{omega alpha }{{ mathcal T }}^{omega alpha }$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mi mathvariant=italic></mml:mi> <mml:mo>=</mml:mo> <mml:msub> <mml:mrow> <mml:mi mathvariant=italic></mml:mi> </mml:mrow> <mml:mrow> <mml:mi>ω</mml:mi> <mml:mi>α</mml:mi> </mml:mrow> </mml:msub> <mml:msup> <mml:mrow> <mml:mi mathvariant=italic></mml:mi> </mml:mrow> <mml:mrow> <mml:mi>ω</mml:mi> <mml:mi>α</mml:mi> </mml:mrow> </mml:msup> </mml:math> . We adopt a standard model <?CDATA $f({ mathcal R },{ mathcal T },{ mathcal Q })={ mathcal R }+varpi { mathcal Q }$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mi>f</mml:mi> <mml:mo stretchy=false>(</mml:mo> <mml:mi mathvariant=italic></mml:mi> <mml:mo>,</mml:mo> <mml:mi mathvariant=italic></mml:mi> <mml:mo>,</mml:mo> <mml:mi mathvariant=italic></mml:mi> <mml:mo stretchy=false>)</mml:mo> <mml:mo>=</mml:mo> <mml:mi mathvariant=italic></mml:mi> <mml:mo>+</mml:mo> <mml:mi>ϖ</mml:mi> <mml:mi mathvariant=italic></mml:mi> </mml:math> , where ϖ indicates a coupling constant. We take spherically symmetric spacetime and develop solutions to the modified field equations corresponding to different choices of the matter Lagrangian by applying ‘embedding class-one’ scheme. For this purpose, we utilize <?CDATA ${mathbb{MIT}}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mi mathvariant=double-struck>MIT</mml:mi> </mml:math> bag model equation of state and investigate some physical aspects of compact models such as RXJ 1856-37, 4U 1820-30, Cen X-3, SAX J 1808.4-3658 and Her X-I. We use masses and radii of these stars and employ the vanishing radial pressure condition at the boundary to calculate the value of their respective bag constant <?CDATA ${{mathfrak{B}}}_{{mathfrak{c}}}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msub> <mml:mrow> <mml:mi mathvariant=fraktur>B</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant=fraktur>c</mml:mi> </mml:mrow> </mml:msub> </mml:math> . Further, we fix ϖ = ± 4 to analyze the behavior of resulting state variables, anisotropy, mass, compactness, surface redshift as well as energy bounds through graphical interpretation for each star model. Two different physical tests are performed to check the stability of the developed solutions. We conclude that ϖ = −4 is more suitable choice for the considered modified model to obtain stable structures of the compact bodies." @default.
• W4220854312 created "2022-04-03" @default.
• W4220854312 creator A5010593762 @default.
• W4220854312 creator A5053960718 @default.
• W4220854312 date "2022-04-04" @default.
• W4220854312 modified "2023-10-14" @default.
• W4220854312 title "Effects of non-minimal matter-geometry coupling on embedding class-one anisotropic solutions" @default.
• W4220854312 cites W1485308145 @default.
• W4220854312 cites W1489032667 @default.
• W4220854312 cites W1751982145 @default.
• W4220854312 cites W1958232190 @default.
• W4220854312 cites W1964597263 @default.
• W4220854312 cites W1972268597 @default.
• W4220854312 cites W1976100082 @default.
• W4220854312 cites W1978864258 @default.
• W4220854312 cites W1992753446 @default.
• W4220854312 cites W2018635598 @default.
• W4220854312 cites W2021937588 @default.
• W4220854312 cites W2033562931 @default.
• W4220854312 cites W2037195717 @default.
• W4220854312 cites W2039130581 @default.
• W4220854312 cites W2039142178 @default.
• W4220854312 cites W2066155353 @default.
• W4220854312 cites W2067915846 @default.
• W4220854312 cites W2070620588 @default.
• W4220854312 cites W2071725611 @default.
• W4220854312 cites W2071863200 @default.
• W4220854312 cites W2073220558 @default.
• W4220854312 cites W2074305322 @default.
• W4220854312 cites W2074818582 @default.
• W4220854312 cites W2080787731 @default.
• W4220854312 cites W2092350553 @default.
• W4220854312 cites W2096475520 @default.
• W4220854312 cites W2102716046 @default.
• W4220854312 cites W2109243620 @default.
• W4220854312 cites W2111626561 @default.
• W4220854312 cites W2115485026 @default.
• W4220854312 cites W2128752885 @default.
• W4220854312 cites W2132358705 @default.
• W4220854312 cites W2135414712 @default.
• W4220854312 cites W2136368343 @default.
• W4220854312 cites W2141978587 @default.
• W4220854312 cites W2145385926 @default.
• W4220854312 cites W2154422137 @default.
• W4220854312 cites W2163930464 @default.
• W4220854312 cites W2229552618 @default.
• W4220854312 cites W2235048890 @default.
• W4220854312 cites W2258743878 @default.
• W4220854312 cites W2281531506 @default.
• W4220854312 cites W2288758309 @default.
• W4220854312 cites W2314220888 @default.
• W4220854312 cites W2336937883 @default.
• W4220854312 cites W2499691194 @default.
• W4220854312 cites W2516724975 @default.
• W4220854312 cites W2569816558 @default.
• W4220854312 cites W2594787117 @default.
• W4220854312 cites W2764219617 @default.
• W4220854312 cites W2793164673 @default.
• W4220854312 cites W2980254384 @default.
• W4220854312 cites W3006999801 @default.
• W4220854312 cites W3013634084 @default.
• W4220854312 cites W3015486985 @default.
• W4220854312 cites W3022083082 @default.
• W4220854312 cites W3025250329 @default.
• W4220854312 cites W3026286413 @default.
• W4220854312 cites W3042261546 @default.
• W4220854312 cites W3048729889 @default.
• W4220854312 cites W3093829664 @default.
• W4220854312 cites W3098822838 @default.
• W4220854312 cites W3101087432 @default.
• W4220854312 cites W3102314660 @default.
• W4220854312 cites W3102949153 @default.
• W4220854312 cites W3103155918 @default.
• W4220854312 cites W3104121279 @default.
• W4220854312 cites W3104181435 @default.
• W4220854312 cites W3106539614 @default.
• W4220854312 cites W3118796946 @default.
• W4220854312 cites W3120476710 @default.
• W4220854312 cites W3126103825 @default.
• W4220854312 cites W3166121241 @default.
• W4220854312 cites W3185788806 @default.
• W4220854312 cites W3209208932 @default.
• W4220854312 cites W4205157729 @default.
• W4220854312 cites W4242783256 @default.
• W4220854312 doi "https://doi.org/10.1088/1402-4896/ac5ed4" @default.
• W4220854312 hasPublicationYear "2022" @default.
• W4220854312 type Work @default.
• W4220854312 citedByCount "12" @default.
• W4220854312 countsByYear W42208543122022 @default.
• W4220854312 countsByYear W42208543122023 @default.
• W4220854312 crossrefType "journal-article" @default.
• W4220854312 hasAuthorship W4220854312A5010593762 @default.
• W4220854312 hasAuthorship W4220854312A5053960718 @default.
• W4220854312 hasBestOaLocation W42208543122 @default.
• W4220854312 hasConcept C11413529 @default.
• W4220854312 hasConcept C121332964 @default.
• W4220854312 hasConcept C192562407 @default.
• W4220854312 hasConcept C41008148 @default.

• next