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arXiv · 0705.0904

String Cosmological Model in Cylindrically Symmetric Inhomogeneous Universe with Electromagnetic Field

Anirudh Pradhan·Anju Rai·Raj Bali
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Abstract

Cylindrically symmetric inhomogeneous string cosmological models in presence of electromagnetic field is investigated. We have assumed that $F_{12}$ is the only non-vanishing component of $F_{ij}$. The Maxwell's equations require that $F_{12}$ is the function of $x$ and $t$ both and the magnetic permeability is the function of $x$ and $t$ both. To get the deterministic solution, it has been assumed that the expansion ($θ$) in the model is proportional to the eigen value $σ^{1}_{1}$ of the shear tensor $σ^{i}_{j}$. The derived model represents the inflationary scenario as the proper volume increases exponentially with cosmic time. It is observed that the model has a point type singularity. The physical and geometric aspects of the model are also discussed.

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Anirudh Pradhan, Anju Rai, Raj Bali. 2014-05-04. String Cosmological Model in Cylindrically Symmetric Inhomogeneous Universe with Electromagnetic Field. https://arxiv.org/abs/0705.0904

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