2019
DOI: 10.31349/revmexfis.65.382
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A charged perfect fluid model with high compactness

Abstract: A relativistic, static and spherically symmetrical stellar model is presented, constituted by a perfect charged fluid. This represents a generalization to the case of a perfect neutral fluid, whose construction is made through the solution to the Einstein-Maxwell equations proposing a form of gravitational potential  $g_{tt}$ and the electric field. The choice of electric field implies that this model supports values of compactness$u=GM/c^2R\leq 0.5337972212$, values higher than the case without electric charg… Show more

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Cited by 21 publications
(14 citation statements)
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“…Solutions with given Δ, a 1 and l are discussed [41][42][43], where the mass is used instead of y, [44][45][46][47][48][49][50]. There are also solutions with Δ = 0 [51,52].…”
Section: The Tangential Pressure and The Anisotropic Factormentioning
confidence: 99%
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“…Solutions with given Δ, a 1 and l are discussed [41][42][43], where the mass is used instead of y, [44][45][46][47][48][49][50]. There are also solutions with Δ = 0 [51,52].…”
Section: The Tangential Pressure and The Anisotropic Factormentioning
confidence: 99%
“…Together, Eqs. (51,52) give another linear equation for y which depends only on a 1 and Δ. Solving it, we find y and then l 2 from any of Eqs.…”
Section: Solutions When the Charge Is Not Given Beforehandmentioning
confidence: 99%
“…Since σ = k R 2 B g > 0 this relation determines the values of the MIT Bag constant given ν. Replacing (31) in Eq. 30we arrive at the finding that the rate of compactness u for this model matches the one obtained for the case of a perfect fluid with (y, B), given by (22) and 21…”
Section: Analysis Of the Solutionmentioning
confidence: 99%
“…We know that its mass is M = 0.87M and its radius R = 7.866km, replacing this in (32) we obtain (ν = 0.51192), and replacing this value in Eq. (31) and since σ = k R 2 B g we determine the value of B g to be B g = 97.00476509 Mev fm 3 . The value that we obtained differs a little from the one obtained previously for the same star, considering a model without quintessence, which was B g = 99.7207866 Mev/fm 3 [66] .…”
Section: Graphical Representation Of the Solutionmentioning
confidence: 99%
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