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v7.0

User Guide

  • Preliminaries
  • Quick Start
  • Example Walkthrough
  • Frontends
  • Numerical Methods
  • Interpreting Output Files
  • Understanding Grids
  • Working With Tags
  • 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
    • Dimensionless Formulation
    • Rotation Effects
  • Tidal Equations

Appendices

  • Composite Polytropes
  • Building POLY Models
  • Evaluating Tidal Eigenvalues
GYRE
  • Oscillation Equations
  • Edit on GitHub

Oscillation Equations

This chapter outlines how the oscillation equations (solved by the gyre frontend) are obtained from the basic equations of stellar structure.

  • Fluid Equations
  • Equilibrium State
  • Linearized Equations
  • Separated Equations
  • Dimensionless Formulation
    • Variables
    • Oscillation Equations
    • Boundary Conditions
      • Inner Boundary
      • Outer Boundary
    • Jump Conditions
    • Structure Coefficients
    • Physics Switches
  • Rotation Effects
    • Doppler Shift
    • Coriolis Force
      • The Traditional Approximation of Rotation
      • Solution Families
      • Incorporating the TAR
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© Copyright 2023, Rich Townsend & The GYRE Team. Revision a0e66906.

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