The first woman to be appointed as Vice-Chancellor of the University of Oxford will be honoured by Queen’s University today (Thursday 2 July). Professor Louise Richardson, a renowned scholar on ...
Read July 2012's Press releases
Read June 2012's Press releases
Read May 2012's Press releases
Read April 2012's Press releases
Read March 2012's Press releases
Read February 2012's Press releases
Read January 2012's press releases
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.
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 led by Queen’s University and Oxford University scientists has devised a method of studying supernovae explosions in the laboratory instead of observing them in space. A report by the team is published in Nature Physics.
Dr Brian Reville from Queen’s University Physics and Astronomy said: “This is a very important result, as it opens a new window into the complex processes occurring in some of our Galaxy’s most fascinating objects, supernovae.”
‘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,’ said Professor Gianluca Gregori of Oxford University’s Department of Physics, who led the study. ‘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 spotted about 300 years ago in the Cassiopeia constellation 11,000 light years away. 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 Rutherford Appleton Laboratory. ‘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,’ said Jena Meinecke, an Oxford University graduate student, who headed the experimental efforts. 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.
‘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,’ said Professor Gregori. ‘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 supernovae 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.’
These results are significant because they help to piece together a story for the creation and development of magnetic fields in our Universe, and provides the first experimental proof that turbulence amplifies magnetic fields in the tenuous interstellar plasma.
The Oxford team included the groups of Professor Gregori and Professor Bell in Atomic and Laser Physics and Professor Schekochihin in Theoretical Physics alongside researchers from the University of Chicago, ETH Zurich, 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.