Astronomy and astrophysics Definition
Zel'dovich approximation
Builds on Lagrangian and Eulerian descriptionJacobian determinant
Definition
Consider pressureless matter in an expanding universe, described in comoving coordinates. Label each mass element by its initial (Lagrangian) position . Let be its comoving (Eulerian) position at time , as in the Lagrangian and Eulerian description. Let be the growing mode of linear perturbation theory, and let be a potential such that the linear density contrast is . The Zel'dovich approximation is the trajectory The density then follows from conservation of mass: where is the Jacobian determinant. Here are the eigenvalues of the deformation tensor at .
Remarks
To first order in , the density formula gives , so the approximation agrees with linear theory. The formula holds while the map is one to one; the first time is called shell crossing.
Example: in one dimension take with . Then and , so . At the density becomes infinite when . For plane-parallel motion such as this one, the approximation is exact up to shell crossing.
Non-example: after shell crossing the map folds over and several streams overlap at one point. The formula then makes particles pass freely through each other, while real gravity binds them into a structure, so it no longer describes the dynamics.
Reading path
To understand this page from the ground up, read these 9 pages in order. The foundations come first.
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- no evidence level
- Euclidean space object
- Function concept
- Lagrangian and Eulerian description concept
- Total derivative concept
- Function of several variables concept
- Partial derivative concept
- Jacobian matrix concept
- Jacobian determinant concept
- Zel'dovich approximation definition
Further reading
About this page
| Tag | Z0PVBZC8KX |
|---|---|
| URI | m2://Z0PVBZC8KX |
| Kind | definition |
| Writing | W0 stub |
| MSC | 85A40, 85A05 |
| Defines | Zel'dovich approximation |
| Uses | Lagrangian and Eulerian description, Jacobian determinant |
| Changed | 3 November 2026 |
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