Matches in SemOpenAlex for { <https://semopenalex.org/work/W2594787117> ?p ?o ?g. }
- W2594787117 abstract "We propose a unique stellar model under the $f(R,mathcal{T})$ gravity by using the conjecture of Mazur-Mottola [P. Mazur and E. Mottola, Report number: LA-UR-01-5067., P. Mazur and E. Mottola, Proc. Natl. Acad. Sci. USA 101, 9545 (2004)] which is known as gravastar and a viable alternative to the black hole as available in literature. This gravastar is described by the three different regions, viz., (I) Interior core region, (II) Intermediate thin shell, and (III) Exterior spherical region. The pressure within the interior region is equal to the constant negative matter density which provides a repulsive force over the thin spherical shell. This thin shell is assumed to be formed by a fluid of ultra relativistic plasma and the pressure, which is directly proportional to the matter-energy density according to Zel'dovich's conjecture of stiff fluid [Y.B. Zel'dovich, Mon. Not. R. Astron. Soc. 160, 1 (1972)], does counter balance the repulsive force exerted by the interior core region. The exterior spherical region is completely vacuum and assumed to be de Sitter spacetime which can be described by the Schwarzschild solution. Under this specification we find out a set of exact and singularity-free solution of the collapsing star which presents several other physically valid features within the framework of alternative gravity." @default.
- W2594787117 created "2017-03-16" @default.
- W2594787117 creator A5006886016 @default.
- W2594787117 creator A5023028401 @default.
- W2594787117 creator A5067823193 @default.
- W2594787117 creator A5076928889 @default.
- W2594787117 creator A5078783335 @default.
- W2594787117 creator A5084285757 @default.
- W2594787117 date "2017-06-06" @default.
- W2594787117 modified "2023-10-13" @default.
- W2594787117 title "Gravastars in <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mi>f</mml:mi><mml:mo stretchy=false>(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant=script>T</mml:mi><mml:mo stretchy=false>)</mml:mo></mml:math> gravity" @default.
- W2594787117 cites W1187216380 @default.
- W2594787117 cites W1637390811 @default.
- W2594787117 cites W1853767801 @default.
- W2594787117 cites W1878544655 @default.
- W2594787117 cites W1976030533 @default.
- W2594787117 cites W1976900091 @default.
- W2594787117 cites W1978943205 @default.
- W2594787117 cites W1992018634 @default.
- W2594787117 cites W1992690837 @default.
- W2594787117 cites W1992887596 @default.
- W2594787117 cites W1998388948 @default.
- W2594787117 cites W2000248272 @default.
- W2594787117 cites W2003279266 @default.
- W2594787117 cites W2004188331 @default.
- W2594787117 cites W2011317280 @default.
- W2594787117 cites W2012535746 @default.
- W2594787117 cites W2018370556 @default.
- W2594787117 cites W2021000304 @default.
- W2594787117 cites W2021214254 @default.
- W2594787117 cites W2026555370 @default.
- W2594787117 cites W2027875859 @default.
- W2594787117 cites W2029500034 @default.
- W2594787117 cites W2034388871 @default.
- W2594787117 cites W2034936981 @default.
- W2594787117 cites W2037867314 @default.
- W2594787117 cites W2046092404 @default.
- W2594787117 cites W2049032016 @default.
- W2594787117 cites W2051556588 @default.
- W2594787117 cites W2052862393 @default.
- W2594787117 cites W2057803783 @default.
- W2594787117 cites W2069042714 @default.
- W2594787117 cites W2073603601 @default.
- W2594787117 cites W2073832139 @default.
- W2594787117 cites W2077431724 @default.
- W2594787117 cites W2080253621 @default.
- W2594787117 cites W2085701313 @default.
- W2594787117 cites W2101862267 @default.
- W2594787117 cites W2102716046 @default.
- W2594787117 cites W2105927609 @default.
- W2594787117 cites W2107068964 @default.
- W2594787117 cites W2119220636 @default.
- W2594787117 cites W2127851281 @default.
- W2594787117 cites W2128752885 @default.
- W2594787117 cites W2135138933 @default.
- W2594787117 cites W2141141990 @default.
- W2594787117 cites W2145385926 @default.
- W2594787117 cites W2158917220 @default.
- W2594787117 cites W2212302519 @default.
- W2594787117 cites W2261682825 @default.
- W2594787117 cites W2293270763 @default.
- W2594787117 cites W2333825634 @default.
- W2594787117 cites W2343784889 @default.
- W2594787117 cites W2409764154 @default.
- W2594787117 cites W2461428575 @default.
- W2594787117 cites W2557376874 @default.
- W2594787117 cites W2759816459 @default.
- W2594787117 cites W2952210376 @default.
- W2594787117 cites W2952332536 @default.
- W2594787117 cites W3098008667 @default.
- W2594787117 cites W3098371892 @default.
- W2594787117 cites W3098931315 @default.
- W2594787117 cites W3100023005 @default.
- W2594787117 cites W3100246253 @default.
- W2594787117 cites W3100280251 @default.
- W2594787117 cites W3102763870 @default.
- W2594787117 cites W3103172379 @default.
- W2594787117 cites W3103299669 @default.
- W2594787117 cites W3103825464 @default.
- W2594787117 cites W3106257655 @default.
- W2594787117 cites W3123519702 @default.
- W2594787117 cites W3126103825 @default.
- W2594787117 cites W4232247040 @default.
- W2594787117 doi "https://doi.org/10.1103/physrevd.95.124011" @default.
- W2594787117 hasPublicationYear "2017" @default.
- W2594787117 type Work @default.
- W2594787117 sameAs 2594787117 @default.
- W2594787117 citedByCount "105" @default.
- W2594787117 countsByYear W25947871172017 @default.
- W2594787117 countsByYear W25947871172018 @default.
- W2594787117 countsByYear W25947871172019 @default.
- W2594787117 countsByYear W25947871172020 @default.
- W2594787117 countsByYear W25947871172021 @default.
- W2594787117 countsByYear W25947871172022 @default.
- W2594787117 countsByYear W25947871172023 @default.
- W2594787117 crossrefType "journal-article" @default.
- W2594787117 hasAuthorship W2594787117A5006886016 @default.
- W2594787117 hasAuthorship W2594787117A5023028401 @default.
- W2594787117 hasAuthorship W2594787117A5067823193 @default.
- W2594787117 hasAuthorship W2594787117A5076928889 @default.