On the linear stability of polytropic fluid spheres in $R^2$ gravity
Vladimir Dzhunushaliev, Vladimir Folomeev

TL;DR
This paper investigates the linear stability of polytropic fluid spheres in $R^2$ gravity, showing that the stability transition occurs at the maximum mass-central density point, similar to general relativity.
Contribution
It provides the first analysis of stability for polytropic spheres in $R^2$ gravity within the Jordan frame, extending stability criteria beyond general relativity.
Findings
Stability transition occurs at maximum mass-central density curve
Results align with general relativity stability criteria
Supports the applicability of classical stability analysis in $R^2$ gravity
Abstract
Within gravity, we study the linear stability of strongly gravitating spherically symmetric configurations supported by a polytropic fluid. All calculations are carried out in the Jordan frame. It is demonstrated that, as in general relativity, the transition from stable to unstable systems occurs at the maximum of the curve mass-central density of the fluid.
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