Self-similar evolution of astrophysical and laboratory jets: expansion and collimation

Details Self-similar evolution of astrophysical and laboratory jets: expansion and collimation Self-similar evolution of astrophysical and laboratory jets: expansion and collimation

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jphcs.112d2015f&link_type=abstract

Journal of Physics: Conference Series, Volume 112, Issue 4, pp. 042015 (2008).

Physics

3

Scientific paper

In this paper, we deal theoretically with expansion, collimation or collapse of radiating fluids and jets, especially. Firstly, we consider a case in which radiation can be neglected in the modeling. Secondly, radiative losses are introduced. Finally, we compare, on the one hand, hydrodynamics self-similar solutions to laboratory jet experiments and, on the other hand, self-similiar solutions with radiation losses to numerical simulations.

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