String cosmological model in the presence of a magnetic flux
Bijan Saha, Mihai Visinescu
TL;DR
This paper explores a Bianchi type I string cosmological model incorporating magnetic flux, providing exact solutions under specific assumptions to understand the universe's anisotropic evolution.
Contribution
It introduces a new exact analytical solution for a string cosmological model with magnetic flux in Bianchi type I spacetime, under plausible parametrizations.
Findings
Derived exact solutions for the model
Analyzed the impact of magnetic flux on anisotropy
Provided insights into early universe dynamics
Abstract
A Bianchi type I string cosmological model in the presence of a magnetic flux is investigated. A few plausible assumptions regarding the parametrization of the cosmic string and magneto-fluid are introduced and some exact analytical solutions are presented.
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