The effective geometry of the $n=1$ uniformly rotating self-gravitating polytrope
Donato Bini, Christian Cherubini, Simonetta Filippi, Andrea Geralico

TL;DR
This paper explores the geometric properties of perturbations in a rotating, self-gravitating fluid modeled as a polytrope with index n=1, using an effective geometry approach to analyze acoustic metrics and null geodesics.
Contribution
It introduces an analytical study of the effective acoustic geometry of a rotating polytrope with n=1, highlighting its null geodesics and light cone structure.
Findings
Analysis of null geodesics in the acoustic metric
Characterization of the effective light cone structure
Insights into the geometrical properties of rotating fluid perturbations
Abstract
The \lq\lq effective geometry" formalism is used to study the perturbations of a perfect barotropic Newtonian self-gravitating rotating and compressible fluid coupled with gravitational backreaction. The case of a uniformly rotating polytrope with index is investigated, due to its analytical tractability. Special attention is devoted to the geometrical properties of the underlying background acoustic metric, focusing in particular on null geodesics as well as on the analog light cone structure.
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