Charged Polytropic Models on Finch-Skea Spacetime

TL;DR

This paper investigates static, charged, spherically symmetric relativistic models using polytropic equations of state on Finch-Skea spacetime, analyzing physical viability through various plots.

Contribution

It introduces charged polytropic models on Finch-Skea spacetime considering two polytropic indices, expanding the understanding of relativistic stellar structures.

Findings

Models satisfy causality conditions

Density and pressure profiles are physically acceptable

Models are suitable for describing relativistic polytropes

Abstract

The static, charged, spherically symmetric matter distribution have been studied by considering polytropic equation of state. Two polytropic indices have been considered for study. The plots of density, radial pressure, tangential pressure, anisotropy and causality condition indicates the models are suitable to describe the relativistic polytropes.