In order to effectively test the evolution codes and their output two tasks have been defined:
- Task 1 - a few specific, fully identified, stellar cases are used to compare the evolution models. The comparison has to consider the physics used in the calculation in order to allow for a detailed comparison of the results and by how much the numerical implementation of the physics may affect the result in different codes.
- Task 3 - a few specific, fully identified, stellar cases are used to compare evolution models including diffusion.
As the activities progress, and the results become available, these will be made available here.
