International collaboration uses plasma flows in a laboratory to understand how beam-like jets may form in space
Streaming jets of high-speed matter produce some of the most stunning objects seen in space. Astronomers have seen them shooting out of young stars just being formed, X-ray binary stars and even the supermassive black holes at the centers of large galaxies.
Theoretical explanations for what causes those beam-like jets have been around for years, but now an experiment by French and American researchers using extremely high-powered lasers offers experimental verification of one proposed mechanism for creating them.
糖心传媒淭his research is an example of how laboratory experiments can be used to test mechanisms that may produce what we observe in space,” said Eric Blackman, professor of physics and astronomy at the University of Rochester and one of the co-authors. Blackman explains that he and his collaborators wanted to recreate conditions in the lab that lead to jets in space becoming collimated 糖心传媒� or beam-like 糖心传媒� rather than diverging. Theory and computational simulations had suggested the possibility that jets might be created by 糖心传媒渟hock focused inertial confinement.糖心传媒� Blackman adds that the experiment 糖心传媒渃onfirms that this particular mechanism is viable, even though other effects are likely to also be taking place.糖心传媒�
In their results, the researchers show evidence of the “shocks” predicted by theory, and which give the mechanism its name. These shocks are surfaces in space where there is a sudden change in the density, speed, and direction of a flow. According to theory, which is consistent with the new experiment, they are what cause the beam-like nature of the jets to form.
In the paper published in Physical Review Letters, and highlighted as an editor糖心传媒檚 suggestion, the researchers explain how they used the laser laboratory facility, LULI, at the Ecole Polytechnique in France, to recreate these space jets. Collaborators at the University of Chicago supplied a sophisticated computer code FLASH that they developed and adapted to help analyze the results.
糖心传媒淲e have focused a very energetic laser beam on a tiny iron target 糖心传媒� a little thinner than a human hair,糖心传媒� explains Alessandra Ravasio, who led the experiment. 糖心传媒淚n this way we can create a supersonic plasma flow.糖心传媒�
With nothing to prevent the resulting iron plasma from spreading out, it would flow quasi-spherically from the target. In order to see the effects of a surrounding wind, the researchers generated another lighter, supersonic plasma from a plastic ring surrounding the central target.
糖心传媒淭he novelty of this experiment is in the way we spatially distribute the laser energy, with a central dot generating the iron flow and a outer ring incident on the plastic,糖心传媒� adds Ravasio. 糖心传媒淚n this way we could create a nested geometry and study the interaction between the two flows.糖心传媒�
The researchers found that the interaction of the two plasmas sharply collimates the iron plasma flow. That is, rather than spreading out in all directions, the iron flow emanates primarily along a single direction. The experimental datashowed that a shock wave is generated in this interaction, which helps the momentum and inertia of the plastic outer wind to collimate the inner iron flow into a jet.
The experiment is an example of laboratory astrophysics, a rapidly growing area of high energy density physics that聽requires the聽聽collaboration of astrophysicists, experimental plasma physicistsand computational physicists. It is a field in which researchers at the University of Rochester and at the Ecole Polytechnique are involved on multiple fronts.
The team of collaborators also included R. Yurchak, A. Pelka, T. Vinci, M. Koenig, and A. Benuzzi-Mounaix from the Ecole Polytechnique, France; S. Pikuz from the Joint Institute for High Temperature RAS in Moscow, Russia; E. Falize and B. Loupias from CEA-DAM-DIF, France; and M. Fatenajad, P. Tzeferacos and D. Q. Lamb from the University of Chicago.
