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

  • E. Falize
  • , B. Loupias
  • , S. Bouquet
  • , C. Michaut
  • , M. Koenig
  • , N. Woolsey
  • , C. Gregory
  • , J. Howe
  • , A. Bennuzzi-Mounaix
  • , N. Ozaki
  • Département de Physique Théorique et Appliquée
  • Centre d'Etudes de Limeil-Valenton
  • LUTH - Laboratoire de l'Univers et de ses Theories
  • CEA/UVSQ/CNRS
  • Department of Physics
  • University of York
  • Graduate School of Engineering
  • Osaka University

Research output: Contribution to journal › Conference article › peer-review

6 Citations (Scopus)

Abstract

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.

Original languageEnglish
Article number042015
JournalJournal of Physics: Conference Series
Volume112
Issue numberPart 4
DOIs
Publication statusPublished - 12 Jun 2008
Externally publishedYes
Event5th International Conference on Inertial Fusion Sciences and Applications, IFSA 2007 - Kobe, Japan
Duration: 9 Sept 2007 → 14 Sept 2007

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