Published November 1982 | Version v1
Report Open

Study of Vlasov instabilities of a gravitational plasma in realistic cosmology

Description

A description is given of the cosmological model in which the perturbations will evolve and a bref survey relating to the evolution of the perturbations such as they have been described in recent works. The role of heavy neutrinos in the evolution of baryon perturbations is recalled. Vlasov's linearized system is established for a gravitational plasma. The classification of the gravitational field according to its components of helicity is given. The method of two timescales is introduced in order to solve Vlasov's linearized system. The standard solutions in helicity modes +-2, +-1, and 0 are studied successively

Availability note (English)

MF available from INIS under the Report Number.

Abstract (French)

On donne une description du modele cosmologique dans lequel les perturbations vont evoluer et un bref apercu relatif a l'evolution des perturbations telles qu'elles sont decrites dans les travaux recents. On rappelle le role des neutrinos massifs dans l'evolution des perturbations baryoniques. On etablit le systeme linearise de Vlasov pour un plasma gravitationnel. On donne la classification du champ de gravitation selon ses composantes d'helicite. On introduit la methode a deux echelles de temps pour resoudre le systeme linearise de Vlasov. On etudie successivement les solutions classees en modes d'helicite +-2, +-1 et 0

Files

16079361.pdf

Files (1.8 MB)

Name Size Download all
md5:deaa1b7297ea0c1e56431f62564a00c7
1.8 MB Preview Download

Additional details

Additional titles

Original title (French)
Etude des instabilites Vlasoviennes d'un plasma gravitationnel en cosmologie relativiste

Publishing Information

Imprint Pagination
113 p.
Report number
FRNC-TH--1927