Home

Stability of hydrodynamical relativistic planar jets. I. Linear evolution and saturation of Kelvin-Helmholtz modes

Repozytorium Uniwersytetu Mikołaja Kopernika

Pokaż prosty rekord

dc.contributor.author Perucho, Manuel
dc.contributor.author Hanasz, Michał
dc.contributor.author Marti, Jose-Maria
dc.contributor.author Sol, Helene
dc.date.accessioned 2012-12-19T09:06:13Z
dc.date.available 2012-12-19T09:06:13Z
dc.date.issued 2004-07-27
dc.identifier.citation Astron.Astrophys. 427 (2004) 415-429
dc.identifier.other doi:10.1051/0004-6361:20040349
dc.identifier.uri http://repozytorium.umk.pl/handle/item/248
dc.description.abstract The effects of relativistic dynamics and thermodynamics in the development of Kelvin-Helmholtz instabilities in planar, relativistic jets along the early phases (namely linear and saturation phases) of evolution has been studied by a combination of linear stability analysis and high-resolution numerical simulations for the most unstable first reflection modes in the temporal approach. Three different values of the jet Lorentz factor (5, 10 and 20) and a few different values of specific internal energy of the jet matter (from 0.08 to $60.0 c^2$) have been considered. Figures illustrating the evolution of the perturbations are also shown.
dc.language.iso eng
dc.relation.uri http://arxiv.org/abs/astro-ph/0407548
dc.rights info:eu-repo/semantics/openAccess
dc.subject Astrophysics
dc.title Stability of hydrodynamical relativistic planar jets. I. Linear evolution and saturation of Kelvin-Helmholtz modes
dc.type info:eu-repo/semantics/article


Pliki:

Należy do następujących kolekcji

Pokaż prosty rekord