Stellar models with like--Tolman IV complexity factor

Abstract

In this work, we construct stellar models ba-\break sed on the complexity factor as a supplementary condition which allows to close the system of differential equations arising from the Gravitational Decoupling. The assumed complexity is a generalization of the one obtained from the well known Tolman IV solution. We use Tolman IV, Wyman IIa, Durgapal IV and Heintzmann IIa as seeds solutions. Reported compactness parameters of SMC X-1 and Cen X-3 are used to study the physical acceptability of the models. Some aspects related to the density ratio are also discussed.

arXiv commentReferences updated. Some new references added. arXiv admin note: text overlap with arXiv:2108.10311

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• Complexity and Isotropization based Extended Models in the context of Electromagnetic Field: An Implication of Minimal Gravitational Decoupling
• Role of gravitational decoupling on isotropization and complexity of self-gravitating system under complete geometric deformation approach
• Effect of Extended Gravitational Decoupling on Isotropization and Complexity in f(\mathbb{R},\mathbb{T}) Theory
• Effects of Charge and Gravitational Decoupling on Complexity and Isotropization of Anisotropic Models
• Anisotropic stars made of exotic matter within the complexity factor formalism
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• Possible Existence of Ghost Stars in the context of Electromagnetic Field
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