Search
Menu
Gentec Electro-Optics Inc   - Measure With Gentec Accuracy LB

Tabletop Accelerator Successfully Simulated

Facebook X LinkedIn Email
Full 3-D simulations of a tabletop laser-plasma wakefield accelerator were achieved in just a few hours of supercomputing time.

As conventional accelerators like CERN's Large Hadron Collider grow ever more vast and expensive, the best hope for the high-energy machines of the future may lie in tabletop accelerators like the Berkeley Lab Laser Accelerator (BELLA), now being built by the LOASIS program at the US Department of Energy's Lawrence Berkeley National Laboratory. In just one meter, a single BELLA stage will accelerate an electron beam to 10 billion electron volts, one-fifth the energy achieved by the two-mile-long linear accelerator at the SLAC National Accelerator Laboratory.


Like a speedboat leaving a wake that a surfer can ride, a laser pulse in a laser-plasma wakefield accelerator creates a wake in the plasma that an electron beam "surfs" to high energy. The ridges at bottom right are the laser pulse, which drives the wake as it speeds through the plasma. Colors in the wake represent intense electric fields: the decelerating fields (orange) and accelerating fields (blue) drive the electrons (white) to high energy. (Images: Lawrence Berkeley National Laboratory. Original boat-surfing photo by Sean C. Fulton.)

Jean-Luc Vay of Berkeley Lab's Accelerator and Fusion Research Division (AFRD) and his colleagues Cameron Geddes of AFRD, Estelle Cormier-Michel of the Tech-X Corp. in Denver and David Grote of Lawrence Livermore National Laboratory borrowed a page from Einstein to perfect a revolutionary new method for calculating what happens when a laser pulse plows through a plasma in an accelerator like BELLA. Using its "boosted frame" method, Vay's team achieved full 3-D simulations of a BELLA stage.

Not only are the recent BELLA calculations tens of thousands of times faster than conventional methods, they overcome problems that plagued previous attempts to achieve the full capacity of the boosted-frame method, such as violent numerical instabilities.

Space, time, and complexity

The boosted-frame method, first proposed by Vay in 2007, exploits Einstein's Theory of Special Relativity to overcome difficulties posed by the huge range of space and time scales in many accelerator systems. Vast discrepancies of scale are what made simulating these systems too costly.

"Most researchers assumed that since the laws of physics are invariable, the huge complexity of these systems must also be invariable," said Vay. "But what are the appropriate units of complexity? It turns out to depend on how you make the measurements."


A simulation of laser-plasma acceleration in the laboratory frame. The wavefronts of laser light are the red and blue disks at right; the fields in the wake are colored from pale blue (accelerating) to orange (decelerating). Electrons accelerated by the first of many buckets in the wake are shown in white at right. Both the laser and the wakefield buckets must be resolved over the entire domain of the plasma, requiring many cells and many time steps.

Researchers often use a simulation window that moves with the pulse, but this is not a true transformation of frame and reduces only the multitude of cells, not the multitude of time steps. Laser-plasma wakefield accelerators are particularly challenging: They send a very short laser pulse through a plasma measuring a few centimeters or more, many orders of magnitude longer than the pulse itself (or the even-shorter wavelength of its light). In its wake, as with a speedboat on water, the laser pulse creates waves in the plasma. These alternating waves of positively and negatively charged particles set up intense electric fields. Bunches of free electrons, shorter than the laser pulse, "surf" the waves and are accelerated to high energies.

"The most common way to model a laser-plasma wakefield accelerator in a computer is by representing the electromagnetic fields as values on a grid, and the plasma as particles that interact with the fields," said Geddes. "Since you have to resolve the finest structures – the laser wavelength, the electron bunch – over the relatively enormous length of the plasma, you need a grid with hundreds of millions of cells."

The laser period must also be resolved in time and calculated over millions of time steps. As a result, while much of the important physics of BELLA is three-dimensional, direct 3-D simulation was initially impractical. Just a one-dimensional simulation of BELLA required 5000 hours of supercomputer processor time at Berkeley Lab's National Energy Research Scientific Computing Center (NERSC).

Meadowlark Optics - Building system MR 7/23

Choosing the right frame

The key to reducing complexity and cost lies in choosing the right point of view, or "reference frame." When Albert Einstein was 16 years old, he imagined riding along in a frame moving with a beam of light – a thought experiment that, 10 years later, led to his Theory of Special Relativity, which establishes that there is no privileged reference frame. Observers moving at different velocities may experience space and time differently and even see things happening in a different order, but calculations from any point of view can recover the same physical result.


A simulation of the same system in the boosted frame of the wake, moving at near light speed. Space has contracted, so that the laser wavelengths and the buckets in the wake have similar proportions. Time has stretched, so that first the laser interacts with the plasma, then the buckets are formed one at a time, and finally the electron beam is accelerated. Because of the separation of events in time, the laser has already left the plasma (in yellow rectangle) when the bucket accelerates the beam. Relatively few time steps are needed to model the events, which means less computer time.

Among the consequences are that the speed of light in a vacuum is always the same; compared to a stationary observer's experience, time moves more slowly, while space contracts for an observer traveling near light speed. These different points of view are called Lorentz frames, and changing one for another is called a Lorentz transformation. The "boosted frame" of the laser pulse is the key to enabling calculations of laser-plasma wakefield accelerators that otherwise would be inaccessible.

A laser pulse pushing through a tenuous plasma moves only a little slower than light through a vacuum. An observer in the stationary laboratory frame sees it as a rapid oscillation of electromagnetic fields moving through a very long plasma, whose simulation requires high resolution and many time steps. But for an observer moving with the pulse, time slows, and the frequency of the oscillations is greatly reduced; meanwhile, space contracts, and the plasma becomes much shorter. Thus, relatively few time steps are needed to model the interaction between the laser pulse, the plasma waves formed in its wake, and the bunches of electrons riding the wakefield through the plasma. Fewer steps mean less computer time.

Eliminating instability

Early attempts to apply the boosted-frame method to laser-plasma wakefield simulations encountered numerical instabilities that limited how much the calculation frame could be boosted. Calculations could still be speeded up tens or even hundreds of times, but the full promise of the method could not be realized.

Vay's team showed that using a particular boosted frame, that of the wakefield itself — in which the laser pulse is almost stationary — realizes near-optimal speedup of the calculation. And it fundamentally modifies the appearance of the laser in the plasma. In the laboratory frame, the observer sees many oscillations of the electromagnetic field in the laser pulse; in the frame of the wake, the observer sees just a few at a time.

Not only is speedup possible because of the coarser resolution, but at the same time, numerical instabilities due to short wavelengths can be suppressed without affecting the laser pulse. Combined with special techniques for interpreting the data between frames, this allows the full potential of the boosted-frame principle to be reached.

"We produced the first full multidimensional simulation of the 10 billion-electron-volt design for BELLA," said Vay. "We even ran simulations all the way up to a trillion electron volts, which establishes our ability to model the behavior of laser-plasma wakefield accelerator stages at varying energies. With this calculation, we achieved the theoretical maximum speedup of the boosted-frame method for such systems — a million times faster than similar calculations in the laboratory frame."

Simulations will still be challenging, especially those needed to tailor applications of high-energy laser-plasma wakefield accelerators to such uses as free-electron lasers for materials and biological sciences, or for homeland security or other research. But the speedup achieves what might otherwise have been virtually impossible: It puts the essential high-resolution simulations within reach of new supercomputers.

For more information, visit: www.lbl.gov

Published: March 2011
Glossary
einstein
A unit of energy equal to the amount of energy absorbed by one molecule of material undergoing a photochemical reaction, as determined by the Stark-Einstein law.
electron beam
A stream of electrons emitted by a single source that move in the same direction and at the same speed.
AmericasBasic ScienceBELLABerkeley Lab Laser Acceleratorboosted-frameCaliforniaCameron GeddesCERNs Large Hadron ColliderDavid GrotedefenseEinsteinelectron beamenergyEstelle Cormier-MichelEuropefree-electron lasersJean-Luc Vaylaser wavelengthlaser-plasma wakefield acceleratorLawrence Berkeley National LaboratoryLOASISNational Energy Research Scientific Computing Centernumerical instabilitiesResearch & TechnologySLAC National Accelerator Laboratorysupercomputingtabletop acceleratorTheory of Special RelativityUS Department of EnergyLasers

We use cookies to improve user experience and analyze our website traffic as stated in our Privacy Policy. By using this website, you agree to the use of cookies unless you have disabled them.