The relativistic equation of motion in turbulent jets

Abstract

The turbulent jets are usually described by classical velocities. The relativistic case can be treated starting from the conservation of the relativistic momentum. The two key assumptions which allow to obtain a simple expression for the relativistic trajectory and relativistic velocity are null pressure and constant density.

arXiv comment2 figures 7 pages

References in corpus (1)

• Self-similar imploding relativistic shock waves

Cited by in corpus (1)

• Classical and relativistic conservation of momentum flux in radio-galaxies