Artist representation of laboratory astrophysics experiments. By mimicking fundamental physics aspects in the lab, researchers hope to better understand violent cosmic phenomena. Credit: SLAC National Accelerator Laboratory
Conditions in the vast universe can be quite extreme: Violent collisions scar the surfaces of planets. Nuclear reactions in bright stars generate tremendous amounts of energy. Gigantic explosions catapult matter far out into space. But how exactly do processes like these unfold? And could their power be harnessed? To find out, researchers from the Department of Energy’s SLAC National Accelerator Laboratory perform sophisticated experiments and computer simulations that recreate violent cosmic conditions on a small scale in the lab.
3 recent studies shine light on meteor impacts, the cores of giant planets and cosmic particle accelerators a million times more powerful than the Large Hadron Collider.
High pressure can turn graphite into an extremely hard form of carbon, diamond. Could the same thing happen when a meteor hits graphite in the ground? Scientists predicted that it could, and that these impacts might be powerful enough to produce a form of diamond, called lonsdaleite, harder than regular diamond. “The existence of lonsdaleite has been disputed, but we’ve now found compelling evidence for it,” says Glenzer.
The team heated the surface of graphite with a powerful optical laser pulse that set off a shock wave inside the sample and rapidly compressed it. By shining bright, ultrafast X-rays from SLAC’s X-ray laser Linac Coherent Light Source (LCLS) through the sample, the researchers were able to see how the shock changed the graphite’s atomic structure. “We saw that lonsdaleite formed for certain graphite samples within a few billionths of a second and at a pressure of about 200 gigapascals” says Dominik Kraus. “These results strongly support the idea that violent impacts can synthesize this form of diamond, and that traces of it in the ground could help identify meteor impact sites.”
A second study looked at another peculiar transformation that might occur inside giant gas planets like Jupiter, whose interior is largely made of liquid hydrogen: At high pressure and temperature, this material is believed to switch from its “normal,” electrically insulating state into a metallic, conducting one. “Understanding this process provides new details about planet formation and the evolution of the solar system,” says Glenzer.
They used the high-power Janus laser to rapidly compress and heat a sample of liquid deuterium, a heavy form of hydrogen, and to create a burst of X-rays that probed subsequent structural changes in the sample.
The team saw that above a pressure of 250,000 atmospheres and a temperature of 7,000 F, deuterium indeed changed from a neutral, insulating fluid to an ionized, metallic one. “Computer simulations suggest that the transition coincides with the separation of the 2 atoms normally bound together in deuterium molecules,” says Paul Davis. “It appears that as the pressure and temperature of the laser-induced shock wave rip the molecules apart, their electrons become unbound and are able to conduct electricity.” The study could also inform energy research aimed at using deuterium as nuclear fuel for fusion reactions that replicate analogous processes inside the sun and other stars.
In a 3rd example of the extreme universe, tremendously powerful cosmic particle accelerators – near supermassive black holes, for instance – propel streams of ionized gas, called plasma, hundreds of thousands of light-years into space. The energy stored in these streams and in their electromagnetic fields can convert into a few extremely energetic particles, which produce very brief but intense bursts of gamma rays that can be detected on Earth. Scientists want to know how these energy boosters work because it would help them better understand the universe. It could also give them fresh ideas for building better accelerators for physics and med. Researchers believe one of the main driving forces behind cosmic accelerators could be “magnetic reconnection” – a process in which the magnetic field lines in plasmas break and reconnect in a different way, releasing magnetic energy.
“Magnetic reconnection has been observed in the lab before, for instance in experiments with 2 colliding plasmas that were created with high-power lasers,” says Frederico Fiúza. “However, none of these laser experiments have seen non-thermal particle acceleration – an acceleration not just related to the heating of the plasma. But our work demonstrates that with the right design, current experiments should be able to see it.” His team ran a number of computer simulations that predicted how plasma particles would behave in such experiments. The most demanding calculations, with about 100 billion particles, took more than a million CPU hours and more than a terabyte of memory on Argonne National Lab’s Mira supercomputer.
“We determined key parameters for the required detectors, including the energy range they should operate in, the energy resolution they should have, and where they must be located in the experiment,” says Samuel Totorica. “Our results are a recipe for the design of future experiments that want to study how particles gain energy through magnetic reconnection.”
Meteor impacts, planetary science and cosmic accelerators are just three of a large number of laboratory astrophysics topics that will be discussed at the 11th International Conference on High Energy Density Laboratory Astrophysics (HEDLA2016), to be held May 16-20 at SLAC. https://www6.slac.stanford.edu/news/2016-04-15-slac-researchers-recreate-extreme-universe-lab.aspx
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