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- W3025577551 abstract "Abstract In this work an analytic fluid sphere built on the well-known Tolman IV space–time is obtained. This toy model is sourced by an imperfect fluid distribution with a dark matter component. The anisotropic behavior is introduced into the system via gravitational decoupling by means of minimal geometric deformation. In this regard, the temporal component of the $$theta $$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mi>θ</mml:mi></mml:math> -sector has been interpreted as the dark side of the matter distribution. To validate the feasibility of the salient model a detailed graphical analysis is performed, supported by real observational data corresponding to some strange star candidates. Besides, the impacts of minimal geometric deformation approach on the main macro physical observables ı.e, the total mass M , compactness factor u and surface gravitational red-shift $$z_{s}$$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:msub><mml:mi>z</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:math> are discussed." @default.
- W3025577551 created "2020-05-21" @default.
- W3025577551 creator A5075250490 @default.
- W3025577551 date "2020-05-01" @default.
- W3025577551 modified "2023-09-27" @default.
- W3025577551 title "Minimally deformed anisotropic dark stars in the framework of gravitational decoupling" @default.
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