Turning point principle for relativistic stars
Mahir Hadzic, Zhiwu Lin

TL;DR
This paper proves the turning point principle for relativistic stars, linking stability changes to extrema in mass-radius curves, and describes the linearized dynamics, showing the number of unstable modes increases with central redshift.
Contribution
It rigorously establishes the turning point principle for Einstein-Euler systems and details the linearized stability analysis for relativistic stars.
Findings
Spectral stability changes only at mass extrema.
Number of growing modes increases with redshift.
Provides a detailed linearized dynamics description.
Abstract
Upon specifying an equation of state, spherically symmetric steady states of the Einstein-Euler system are embedded in 1-parameter families of solutions, characterized by the value of their central redshift. In the 1960's Zel'dovich [50] and Wheeler [22] formulated a turning point principle which states that the spectral stability can be exchanged to instability and vice versa only at the extrema of mass along the mass-radius curve. Moreover the bending orientation at the extrema determines whether a growing mode is gained or lost. We prove the turning point principle and provide a detailed description of the linearized dynamics. One of the corollaries of our result is that the number of growing modes grows to infinity as the central redshift increases to infinity.
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