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Experimental demonstration of an inertial collimation mechanism in nested outflows.
Yurchak, R; Ravasio, A; Pelka, A; Pikuz, S; Falize, E; Vinci, T; Koenig, M; Loupias, B; Benuzzi-Mounaix, A; Fatenejad, M; Tzeferacos, P; Lamb, D Q; Blackman, E G.
Afiliación
  • Yurchak R; LULI, Ecole Polytechnique, CNRS, CEA, UPMC, Route de Saclay, 91128 Palaiseau, France.
  • Ravasio A; LULI, Ecole Polytechnique, CNRS, CEA, UPMC, Route de Saclay, 91128 Palaiseau, France.
  • Pelka A; LULI, Ecole Polytechnique, CNRS, CEA, UPMC, Route de Saclay, 91128 Palaiseau, France.
  • Pikuz S; Joint Institute for High Temperatures RAS, 13-2 Izhorskaya street, Moscow 125412, Russia.
  • Falize E; CEA-DAM-DIF, F-91297 Arpajon, France.
  • Vinci T; LULI, Ecole Polytechnique, CNRS, CEA, UPMC, Route de Saclay, 91128 Palaiseau, France.
  • Koenig M; LULI, Ecole Polytechnique, CNRS, CEA, UPMC, Route de Saclay, 91128 Palaiseau, France.
  • Loupias B; CEA-DAM-DIF, F-91297 Arpajon, France.
  • Benuzzi-Mounaix A; LULI, Ecole Polytechnique, CNRS, CEA, UPMC, Route de Saclay, 91128 Palaiseau, France.
  • Fatenejad M; Flash Center for Computational Science, University of Chicago, Chicago, Illinois 60637, USA.
  • Tzeferacos P; Flash Center for Computational Science, University of Chicago, Chicago, Illinois 60637, USA.
  • Lamb DQ; Flash Center for Computational Science, University of Chicago, Chicago, Illinois 60637, USA.
  • Blackman EG; Department of Physics and Astronomy, University of Rochester, Rochester, New York 14627, USA.
Phys Rev Lett ; 112(15): 155001, 2014 Apr 18.
Article en En | MEDLINE | ID: mdl-24785042
ABSTRACT
Interaction between a central outflow and a surrounding wind is common in astrophysical sources powered by accretion. Understanding how the interaction might help to collimate the inner central outflow is of interest for assessing astrophysical jet formation paradigms. In this context, we studied the interaction between two nested supersonic plasma flows generated by focusing a long-pulse high-energy laser beam onto a solid target. A nested geometry was created by shaping the energy distribution at the focal spot with a dedicated phase plate. Optical and x-ray diagnostics were used to study the interacting flows. Experimental results and numerical hydrodynamic simulations indeed show the formation of strongly collimated jets. Our work experimentally confirms the "shock-focused inertial confinement" mechanism proposed in previous theoretical astrophysics investigations.
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Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2014 Tipo del documento: Article País de afiliación: Francia
Buscar en Google
Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2014 Tipo del documento: Article País de afiliación: Francia