Group transformation for phase space fluids - Archive ouverte HAL Accéder directement au contenu
Rapport (Rapport De Recherche) Année : 1977

Group transformation for phase space fluids

(1, 2) , (1) , (1) , (1) , (1, 2)
1
2

Résumé

We want to study the time behaviour of Systems where long distances forces are predominant. Such is the case of plasmas, accelerator beam (where we are dealing with Coulomb forces plus electromagnetic confinning external fields) and self gravitating gas (galaxy, cluster of stars etc...) where the Newtonian attraction compete against the thermal (ballistic)expansion. In many cases we can disregard the small irregularities due to the grain structure of the matter (with grain as big as a star in a galaxy) and describe the interaction through a continuous field obtained by the solution of the Poisson equation. This is the well known Vlasov Poisson structure where the global description is obtained by considering the distribu- tion function f (x,v, t) in the 6 dimensional phase space in contradiction to a regular gas where we can usually deal with the first moments of f with respect to v (particles density, momentum, energy density etc...). Consequently we call phase space fluids such Systems. A discussion of the relative properties of these a priori very différent fluids is given in 111 and 121. From the model's maker point of view adopted hère they présent great similarities.
Fichier principal
Vignette du fichier
RP_182-22.pdf (3.37 Mo) Télécharger le fichier
Origine : Fichiers produits par l'(les) auteur(s)
Loading...

Dates et versions

hal-02191403 , version 1 (23-07-2019)

Identifiants

  • HAL Id : hal-02191403 , version 1

Citer

J.R. Burgan, J. Guttierez, A. Munier, E. Fijalkow, M.R. Feix. Group transformation for phase space fluids. [Research Report] Note technique CRPE n° 47, Centre de recherches en physique de l'environnement terrestre et planétaire (CRPE). 1977, 50 p. ⟨hal-02191403⟩
44 Consultations
108 Téléchargements

Partager

Gmail Facebook Twitter LinkedIn More