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Anisotropic stars made of exotic matter within the complexity factor formalism
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We investigate exotic stars composed of dark energy within the context of Einstein's General Relativity, by applying an extended Chaplygin gas equation-of-state. To account for anisotropies, we utilize a formalism based on the complexity factor to obtain numerical solutions. By applying well-established criteria, we demonstrate that the solutions are physically valid and well-behaved. In addition, a comparison with a more conventional approach is also conducted.
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Cited by 2 Pith papers
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On Modeling Anisotropic Quark Stars: The Role of Anisotropy in Radial Oscillation Spectra
Radial oscillation spectra of an anisotropic strange quark star model of Cen X-3 are computed for three anisotropy prescriptions and differ by up to 40 percent between models.
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Radial Oscillations of the HESS J1731-347 Compact Object via the Karmarkar Condition in Gravity
A Karmarkar-based anisotropic stellar model fits HESS J1731-347's mass and radius and predicts radial oscillation frequencies about 20-30% higher than the isotropic Tolman IV model.
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