Stability of Relativistic Hydrodynamical Planar Jets: Linear and Nonlinear Evolution of Kelvin-Helmholtz Modes

Details Stability of Relativistic Hydrodynamical Planar Jets: Linear and Nonlinear Evolution of Kelvin-Helmholtz Modes Stability of Relativistic Hydrodynamical Planar Jets: Linear and Nonlinear Evolution of Kelvin-Helmholtz Modes

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.293..139m&link_type=abstract

Astrophysics and Space Science, v. 293, Issue 1, p. 139-147 (2004).

Astronomy and Astrophysics

Astrophysics

1

Astrophysical Jets, Relativistic Hydrodynamics, Instabilities

Scientific paper

Some aspects about the stability of relativistic flows against
Kelvin-Helmholtz (KH) perturbations are studied by means of
relativistic, hydrodynamical simulations. In particular, we analyze the
transition to the fully nonlinear regime and the long-term evolution of
two jet models with different specific internal energies.

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