Abstract
We present a global approach to nondissipative physics. Based on symplectic mechanics, this technique allows us to obtain the solution of a very large class of problems in terms of a Taylor expansion. We apply this method to the problem of gravitational instability, and we obtain a general expression of the gravitational potential, solution of the Vlasov-Poisson system, as a function of time in the context of Newtonian dust cosmology.
| Original language | English |
|---|---|
| Pages (from-to) | 54-63 |
| Number of pages | 10 |
| Journal | Astrophysical Journal |
| Volume | 465 |
| Issue number | 1 PART I |
| DOIs | |
| Publication status | Published - 1 Jan 1996 |
| Externally published | Yes |
Keywords
- Cosmology: theory
- Dust, extinction
- Hydrodynamics
- Instabilities