.. AGB Wind Model documentation master file ========================================================== Atmospheric Model for Asymptotic Giant Branch Stars ========================================================== This is the documentation of a self-consistent model for the **stationary, spherically symmetric, dust-driven wind of a carbon-rich asymptotic giant branch (AGB) star**. The code couples * a **spherical, frequency-dependent radiative transfer** solver using the Rybicki–Hummer variable-Eddington-factor moment method, * a **radiative-equilibrium temperature** determination (Unsöld–Lucy correction and a full-linearisation Newton corrector), * **equilibrium gas-phase chemistry** (FastChem), * **carbon-dust nucleation and growth** following Gail & Sedlmayr, using the moment method with self-consistent carbon depletion, and * a **stationary wind hydrodynamics** solver (Melia ``Φ`` transform with a mass-loss eigenvalue, plus an optional Henyey global-Newton structure solver), iterated to a self-consistent stationary outflow. .. note:: The model is research software and under active development. This documentation reflects the implementation on the ``main`` branch. The underlying radiative-transfer scheme and notation follow the diploma thesis of D. Kitzmann; equation numbers of the form *(2.59)*, *(3.64)*, … below refer to that thesis. .. toctree:: :maxdepth: 2 :caption: Getting started overview installation running configuration .. toctree:: :maxdepth: 2 :caption: Theory and modelling theory/index theory/governing_equations theory/radiative_transfer theory/temperature_correction theory/chemistry theory/dust theory/opacities theory/hydrodynamics theory/numerics .. toctree:: :maxdepth: 2 :caption: Implementation implementation/architecture implementation/modules implementation/io_formats .. toctree:: :maxdepth: 1 :caption: Appendix glossary references Indices and tables ================== * :ref:`genindex` * :ref:`search`