Desktop Supernova

Prof Bob Bingham

Laser beams 60,000 billion times more powerful than a laser pointer have been used to recreate scaled supernova explosions in the laboratory as a way of investigating one of the most energetic events in the Universe. Research published in Nature Physics investigated how expanding shock waves created by a powerful laser become turbulent, amplifying magnetic fields in the process. Study co-author Professor Bob Bingham, of the University of Strathclyde's Department of Physics, said:

"Supernovae explosions are the largest in the universe since the Big Bang. They occur on average about once every 100 years in a galaxy and not easy to study. Being able to re-create supernova conditions in the laboratory is a big step in being able to understand how they shape the interstellar medium and the origin of magnetic fields in the universe."

Supernova explosions, triggered when the fuel within a star reignites or its core collapses, launch a detonation shock wave that sweeps through a few light years of space from the exploding star in just a few hundred years. But not all such explosions are alike and some, such as Cassiopeia A, show puzzling irregular shapes made of knots and twists.

To investigate what may cause these peculiar shapes, an international team of scientists devised a method of studying supernova explosions in the laboratory instead of observing them in space.

Professor Gianluca Gregori, of Oxford University's Department of Physics, who led the study, said: “It may sound surprising that a table-top laboratory experiment that fits inside an average room can be used to study astrophysical objects that are light years across.

“In reality, the laws of physics are the same everywhere, and physical processes can be scaled from one to the other in the same way that waves in a bucket are comparable to waves in the ocean. So our experiments can complement observations of events such as the Cassiopeia A supernova explosion.”

The Cassiopeia A supernova explosion was first spotted about 300 years ago in the Cassiopeia constellation 11,000 light years away and its light has taken this long to reach us. The optical images of the explosion reveal irregular 'knotty' features and associated with these are intense radio and X-ray emissions.

Whilst no one is sure what creates these phenomena one possibility is that the blast passes through a region of space that is filled with dense clumps or clouds of gas. To recreate a supernova explosion in the laboratory the team used the Vulcan laser facility at the UK's Science and Technology Facilities Council's Rutherford Appleton Lab.

Ms Jena Meinecke an Oxford University graduate student, who headed the experimental efforts, said: “Our team began by focusing three laser beams onto a carbon rod target, not much thicker than a strand of hair, in a low density gas-filled chamber.” The enormous amount of heat generated more than a few million degrees Celsius by the laser caused the rod to explode creating a blast that expanded out through the low density gas.

In the experiments the dense gas clumps or gas clouds that surround an exploding star were simulated by introducing a plastic grid to disturb the shock front. Professor Gregori said: “The experiment demonstrated that as the blast of the explosion passes through the grid it becomes irregular and turbulent just like the images from Cassiopeia.

“'We found that the magnetic field is higher with the grid than without it. Since higher magnetic fields imply a more efficient generation of radio and X-ray photons, this result confirms that the idea that supernova explosions expand into uniformly distributed interstellar material isn't always correct and it is consistent with both observations and numerical models of a shockwave passing through a 'clumpy' medium.”

Don Lamb, the Robert A. Millikan Distinguished Service Professor in Astronomy & Astrophysics at the University of Chicago, said: “Magnetic fields are ubiquitous in the universe. We're pretty sure that the fields didn't exist at the beginning, at the Big Bang.

“So there’s this fundamental question: how did magnetic fields arise?”

The study authors say the results are significant because they help to piece together a story for the creation and development of magnetic fields in our Universe, and provide the first experimental proof that turbulence amplifies magnetic fields in the tenuous interstellar plasma.

The advance was made possible by the extraordinarily close cooperation between the teams performing the experiments and the computer simulations. Study co-author Petros Tzeferacos, of the University of Chicago, said: “The experimentalists knew all the physical variables at a given point.

“They knew exactly the temperature, the density, the velocities. This allows us to benchmark the code against something that we can see.”

Such benchmarking – called validation – showed that the simulations can reproduce the experimental data. The simulations consumed 20 million processing hours on supercomputers at Argonne National Laboratory, in the USA.

A report of the research, entitled 'Turbulent amplification of magnetic fields in laboratory laser-produced shock waves', by the team including researchers from the University of Oxford, the University of Chicago, ETH Zurich, the Queen’s University Belfast, the Science and Technology Facilities Council, the University of York, the University of Michigan, Ecole Polytechnique, Osaka University, the University of Edinburgh, the University of Strathclyde and the Lawrence Livermore National Laboratory, is published in Nature Physics.

Funding for this research was provided by the European Research Council, the UK’s Science and Technology Facilities Council, and the US Department of Energy through the Innovative and Novel Computational Impact on Theory and Experiment program.

4th June 2014

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