# Charged Perfect Fluid Distribution for Cosmological Universe Interacting With Massive Scalar Field in Brans-Dicke Theory

## TL;DR

This paper explores a non-static cosmological model in Brans-Dicke theory, analyzing perfect fluid interactions with scalar and electromagnetic fields, and finds electromagnetic fields cannot persist in flat models due to scalar field effects.

## Contribution

It provides exact solutions for a cosmological flat model with scalar and electromagnetic fields in Brans-Dicke theory, highlighting the influence of scalar fields on electromagnetic presence.

## Key findings

- Electromagnetic field cannot survive in the flat cosmological model.
- Exact solutions for the interacting fields are obtained.
- Scalar field significantly influences the electromagnetic field presence.

## Abstract

Considering a spherically-symmetric non-static cosmological flat model of Robertson-Walker universe we have investigated the problem of perfect fluid distribution interacting with the gravitational field in presence of massive scalar field and electromagnetic field in B-D theory. Exact solutions have been obtained by using a general approach of solving the partial differential equations and it has been observed that the electromagnetic field cannot survive for the cosmological flat model due to the influence caused by the presence of massive scalar field.

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Source: https://tomesphere.com/paper/1701.02997