Energetic interaction between Einstein's universe and a source like-Tolman IV complexity factor

Cites Work

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Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
Cracking of homogeneous self-gravitating compact objects induced by fluctuations of local anisotropy
The stability of relativistic stars and the role of the adiabatic index
Decoupling gravitational sources in general relativity: the extended case
Anisotropic stars: Exact solutions
Anisotropic star models in the context of vanishing complexity
Beyond Einstein gravity. The minimal geometric deformation approach in the brane-world
A class of charged analogues of Durgapal and Fuloria superdense star
Brane-world stars from minimal geometric deformation, and black holes
Static solutions of Einstein's field equations for spheres of fluid.
The minimal geometric deformation approach extended
Some models of anisotropic spheres in general relativity
Anisotropic stars in general relativity
Gravitational decoupled solutions of axial string cosmology
Energy conditions in general relativity and quantum field theory
Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
SEARCHING EXACT SOLUTIONS FOR COMPACT STARS IN BRANEWORLD: A CONJECTURE
Dynamical laws of superenergy in general relativity
Exact Space-Times in Einstein's General Relativity
A Static and Spherically Symmetric Hairy Black Hole in the Framework of the Gravitational Decoupling
Complexity‐Free Anisotropic Solution of Buchdahl's Model and Energy Exchange Between Relativistic Fluids by Extended Gravitational Decoupling
Finch-Skea dark energy stars with vanishing complexity factor

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