Complexity Factor for Charged Spherical System

Abstract

In this paper, we study the complexity factor for a charged anisotropic self-gravitating object. We formulate the Einstein-Maxwell field equations, Tolman-Opphenheimer-Volkoff equation, and the mass function. We form the structure scalars by the orthogonal splitting of the Riemann tensor and then find the complexity factor with the help of these scalars. Finally, we investigate some astrophysical objects for the vanishing of complexity condition. It is found that the presence of the electromagnetic field decreases the complexity of the system.

16 pages, no figure, to appear in EPJC

References in corpus (6)

• All static spherically symmetric anisotropic solutions of Einstein's equations
• New definition of complexity for self-gravitating fluid distributions: The spherically symmetric, static case
• Gravitational Decoupled Charged Anisotropic Spherical Solutions
• Statistical complexity, Fisher-Shannon information, and Bohr orbits in the H-atom
• Complexity and neutron stars structure
• Electromagnetic Effects on Cracking of Anisotropic Polytropes

Cited by in corpus (27)

• Definition of complexity for dynamical spherically symmetric dissipative self-gravitating fluid distributions
• Isotropization and change of complexity by gravitational decoupling
• Complexity factors for axially symmetric static sources
• Quasi-homologous evolution of self-gravitating systems with vanishing complexity factor
• Uncharged and charged anisotropic like--Durgapal stellar model with vanishing complexity
• Gravitational cracking and complexity in the framework of gravitational decoupling
• Complexity of the Bondi metric
• Complexity analysis of Cylindrically Symmetric Self-gravitating Dynamical System in $f(R,T)$ Theory of Gravity
• Role of gravitational decoupling on isotropization and complexity of self-gravitating system under complete geometric deformation approach
• Complexity Factor for Static Sphere in Self-interacting Brans-Dicke Gravity
• Charged Anisotropic Models with Complexity-free Condition
• Anisotropic stars made of exotic matter within the complexity factor formalism
• Complexity of Dynamical Dissipative Cylindrical System in Non-minimally Coupled Theory
• Possibility of the Traversable Wormholes in the Galactic Halos within $4D$ Einstein-Gauss-Bonnet Gravity
• Anisotropic Quark Stars with an Interacting Quark Equation of State within the Complexity Factor Formalism
• Complexity factor of spherically anisotropic polytropes from gravitational decoupling
• Complexity for Dynamical Anisotropic Sphere in f(G,T) Gravity
• Complexity factor Parametrization for Traversable Wormholes
• Complexity of Charged Dynamical Spherical System in Modified Gravity
• Radial Oscillations of the HESS J1731-347 Compact Object via the Karmarkar Condition in Gravity
• Gaussian curvature of spherical shells: A geometric measure of complexity
• Configurational entropy and stability conditions of fermion and boson stars
• Stellar modeling via the Tolman IV solution: The cases of the massive pulsar J0740+6620 and the HESS J1731-347 compact object
• The spacetime geodesy of perfect fluid spheres
• Radial oscillations of quark stars in light of current astrophysical constraints: A comparative study
• Statistical complexity as a probe of mass and phase structure in compact objects
• On Modeling Anisotropic Quark Stars: The Role of Anisotropy in Radial Oscillation Spectra