Scaled laboratory experiments explain the kink behaviour of the Crab Nebula jet

نویسندگان

  • C. K. Li
  • P. Tzeferacos
  • D. Lamb
  • G. Gregori
  • P. A. Norreys
  • M. J. Rosenberg
  • R. K. Follett
  • D. H. Froula
  • M. Koenig
  • F. H. Seguin
  • J. A. Frenje
  • H. G. Rinderknecht
  • H. Sio
  • A. B. Zylstra
  • R. D. Petrasso
  • P. A. Amendt
  • H. S. Park
  • B. A. Remington
  • D. D. Ryutov
  • S. C. Wilks
  • R. Betti
  • A. Frank
  • S. X. Hu
  • T. C. Sangster
  • P. Hartigan
  • R. P. Drake
  • C. C. Kuranz
  • S. V. Lebedev
  • N. C. Woolsey
چکیده

The remarkable discovery by the Chandra X-ray observatory that the Crab nebula's jet periodically changes direction provides a challenge to our understanding of astrophysical jet dynamics. It has been suggested that this phenomenon may be the consequence of magnetic fields and magnetohydrodynamic instabilities, but experimental demonstration in a controlled laboratory environment has remained elusive. Here we report experiments that use high-power lasers to create a plasma jet that can be directly compared with the Crab jet through well-defined physical scaling laws. The jet generates its own embedded toroidal magnetic fields; as it moves, plasma instabilities result in multiple deflections of the propagation direction, mimicking the kink behaviour of the Crab jet. The experiment is modelled with three-dimensional numerical simulations that show exactly how the instability develops and results in changes of direction of the jet.

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عنوان ژورنال:

دوره 7  شماره 

صفحات  -

تاریخ انتشار 2016