pith. sign in

arxiv: 1808.00903 · v1 · pith:KF5ZWCV7new · submitted 2018-08-01 · 🌀 gr-qc

Complexity Factor for Charged Spherical System

classification 🌀 gr-qc
keywords complexityfactorchargedfieldscalarssystemanisotropicastrophysical
0
0 comments X
read the original 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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Radial oscillations of quark stars in light of current astrophysical constraints: A comparative study

    gr-qc 2026-06 unverdicted novelty 3.0

    Comparative numerical study of radial modes in strange quark stars using CFL, interacting, and linear causal EOS shows all satisfy current mass-radius bounds and produce 4-7 kHz fundamental frequencies.