Unified gravity mode and Rossby mode Analysis of Accreting White Dwarf Stars

This repository contains the files and related work directories used in the preparation of the paper "Unified g-mode and r-mode Analysis of Accreting White Dwarf Stars." This has mesa models including the inlists and the gyre input files. The cooled WD model is taken from "Gravity Modes on Rapidly Rotating Accreting White Dwarfs and Their Variation after Dwarf Novae." The requirements are MESA version: 15140 MESASDK version: 21.4.1 Proper environments, see MESA Documentation GYRE version: 7.0 (GYRE Documentation) The details of the steps on MESA models and GYRE input/output are provided in README.txt.