Complexity and Simplicity of Self–Gravitating Fluids

Herrera, L.

doi:10.1007/978-981-97-1172-7_8

Springer Series in Astrophysics and Cosmology

2024

DOI: 10.1007/978-981-97-1172-7_8

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Complexity and Simplicity of Self–Gravitating Fluids

L. Herrera

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2024

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Cited by 2 publications

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Energetic Interaction between Einstein’s Universe and a Source like-Tolman IV Complexity Factor

Andrade,

Santana

2024

Int J Theor Phys

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Energetic Interaction between Einstein’s Universe and a Source like-Tolman IV Complexity Factor

Andrade,

Santana

2024

Int J Theor Phys

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Anisotropic extension of the Kohler–Chao–Tikekar cosmological solution with like Wyman IIa complexity factor

Siza,

Andrade,

Santana

et al. 2024

Eur. Phys. J. C

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We construct a new stellar compact object model in the regime of anisotropic pressure using the framework of gravitational decoupling via minimal geometric deformation, with the particularity that the seed solution used is the known Kohler–Chao–Tikekar cosmological solution. As an extra condition to close the Einstein’s field equations resulting for this construction, we use a generalised complexity factor for self-gravitating spheres to the well-known Wyman IIa solution. The resulting model fulfils the fundamental physical acceptability stellar conditions for a compactness factor of a pulsar SMC X-1. The stability of the model is also investigated.

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Complexity and Simplicity of Self–Gravitating Fluids

Cited by 2 publications

References 126 publications

Energetic Interaction between Einstein’s Universe and a Source like-Tolman IV Complexity Factor

Energetic Interaction between Einstein’s Universe and a Source like-Tolman IV Complexity Factor

Anisotropic extension of the Kohler–Chao–Tikekar cosmological solution with like Wyman IIa complexity factor

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