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Иш: Modeling of Finch-Skea hybrid neutron stars with complexity-free characteristics

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ABI
Anisotropic spheres with variable energy density in general relativity
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Charged anisotropic Starobinsky models admitting vanishing complexity
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On the propagation across the big bounce in an open quantum FLRW cosmology
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New definition of complexity for self-gravitating fluid distributions: The spherically symmetric, static case
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Collapsed Nuclei
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Neutron stars with an anisotropic equation of state: mass, redshift and stability.
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Сарлавҳасиз
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The mass of the compact object in the X-ray binary her X-1/HZ her
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A completely deformed anisotropic class one solution for charged compact star: a gravitational decoupling approach
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Physical characteristics and maximum allowable mass of hybrid star in the context of f(Q) gravity
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Complexity and isotropization based extended models in the context of electromagnetic field: an implication of minimal gravitational decoupling
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Gravitational waves at the first post-Newtonian order with the Weyssenhoff fluid in Einstein–Cartan theory
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A realistic stellar model based on an ansatz of Duorah and Ray
Michael R. Finch, J E F Skea
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Anisotropic interior models with Kohler–Chao–Tikekar-like complexity factor
Abeer M. Albalahi, Z. Yousaf, S. Khan +1
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The Nambu—Jona-Lasinio model of quantum chromodynamics
S. P. Klevansky
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Decoupled anisotropic Buchdahl’s relativistic models in <i>f</i>( <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>R</mml:mi> <mml:mo>,</mml:mo> <mml:mspace/> <mml:mi>T</mml:mi> </mml:math> ) theory
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Estimating the role of bag constant and modified theory on anisotropic stellar models
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Quasi-homologous evolution of self-gravitating systems with vanishing complexity factor
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Gravitational cracking and complexity in the framework of gravitational decoupling
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Мақола20214 иқтибос
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Isotropization and complexity shift of gravitationally decoupled charged anisotropic sources
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Isotropization and change of complexity by gravitational decoupling
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ABI
A simple protocol to construct solutions with vanishing complexity by Gravitational Decoupling
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Hybrid Stars that Masquerade as Neutron Stars
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Sharp Bounds on the Critical Stability Radius for Relativistic Charged Spheres
Håkan Andréasson
Мақола20084 иқтибос
ABI