2020
DOI: 10.1142/s0217732320500716
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Analytical model of dark energy stars

Abstract: In this article we study the structure and stability of compact astrophysical objects which are ruled by the dark energy equation of state (EoS). The existence of dark energy is important for explaining the current accelerated expansion of the universe. Exact solutions to Einstein field equations (EFE) have been found by considering particularized metric potential, Finch and Skea ansatz [1]. The obtained solutions are relevant to the explanation of compact fluid sphere. Further, we have observed at the junctio… Show more

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Cited by 14 publications
(5 citation statements)
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“…This article aims to discover the notion of 𝜕𝛩 * 𝐸𝐺𝑅𝑂 -detectability by means of the sensors selection [13][14][15]. The motive of studying conception, there are existent several problems in the real world need to be studied as in [16][17] and for another system types (see [18][19][20]). This means, one maybe devoted to the boundary gradient exponential problem of type detection in 𝜕𝛩 * (see Figure 1) [21].…”
Section: Introductionmentioning
confidence: 99%
“…This article aims to discover the notion of 𝜕𝛩 * 𝐸𝐺𝑅𝑂 -detectability by means of the sensors selection [13][14][15]. The motive of studying conception, there are existent several problems in the real world need to be studied as in [16][17] and for another system types (see [18][19][20]). This means, one maybe devoted to the boundary gradient exponential problem of type detection in 𝜕𝛩 * (see Figure 1) [21].…”
Section: Introductionmentioning
confidence: 99%
“…In this way, various models of DES were presented over time, most of them referring to the anisotropy parameter and stability of the star. In addition, other definable properties were also studied for it [14][15][16][17]. Of course, it was shown in Ref.…”
Section: Introductionmentioning
confidence: 99%
“…In this study, it is assumed that the pressure of the fluid is positive at the beginning of falling and then, where the star reaches its final stage of collapse, the negative pressure prevails in the system. By expressing the equations of motion in the presence of specific metric potentials Finch and Skea, Banerjee et al [20] were able to provide an exact solution for the dark energy star. The effects of slow rotation on the configuration of a dark energy star with the governing Chaplygin equation of state were investigated by Panotopoulos et al in Ref.…”
Section: Introductionmentioning
confidence: 99%