Logo

User Guide

  • Preliminaries
  • Quick Start
  • Example Walkthrough
  • Frontends
  • Numerical Methods
  • Interpreting Output Files
  • Understanding Grids
  • Working With Tags
  • Performance Tuning
  • Advanced Usage
  • Frequently Asked Questions
  • Troubleshooting

Reference Guide

  • Installation
  • Namelist Input Files
  • Output Files
  • Stellar Models
  • Oscillation Equations
    • Fluid Equations
    • Equilibrium State
    • Linearized Equations
    • Separated Equations
    • Boundary Conditions
    • Dimensionless Formulation
    • Rotation Effects
    • Convection Effects
    • Tidal Effects

Appendices

  • Composite Polytropes
  • Support Tools
GYRE
  • Oscillation Equations
  • View page source

Oscillation Equations

This chapter outlines how the oscillation equations solved by the GYRE frontends are obtained from the basic equations of stellar structure.

  • Fluid Equations
  • Equilibrium State
  • Linearized Equations
  • Separated Equations
  • Boundary Conditions
    • Inner Boundary
    • Outer Boundary
    • Internal Boundaries
  • Dimensionless Formulation
    • Variables
    • Oscillation Equations
    • Boundary Conditions
      • Inner Boundary
      • Outer Boundary
      • Internal Boundaries
    • Structure Coefficients
    • Physics Switches
  • Rotation Effects
    • Doppler Shift
    • Perturbative Coriolis Force Treatment
    • Non-Perturbative Coriolis Force Treatment
      • Solution Families
      • Implementing the TAR
  • Convection Effects
    • Frozen Convection
    • Turbulent Damping
  • Tidal Effects
    • Tidal Potential
    • Separated Equations
    • Boundary Conditions
Previous Next

© Copyright 2013-2026, Rich Townsend & The GYRE Team.

Built with Sphinx using a theme provided by Read the Docs.