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Beams and plasmas

FEB 01, 2019
Progress in plasma physics and accelerator science research advances astrophysics, energy production, and many other scientific fields.

DOI: 10.1063/PT.3.4136

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Wim Leemans

Plasmas are being studied for applications such as magnetic and inertial confinement fusion and in astrophysical phenomena. And accelerators, with their ever-increasing performance, are enabling new generations of light sources and the exploration of the frontiers of particle physics. By connecting those two scientific disciplines, researchers have learned that plasmas can support extremely large electric fields, which may be exploited to accelerate particles. Those fields can be generated using either intense lasers or particle beams to drive collective density waves, much like how a motorboat generates a wake on a lake’s surface.

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The Alcator C-Mod tokamak at MIT uses a strong magnetic field to confine plasma for fusion energy applications. (Photo by Mike Garrett, CC BY 3.0 .)

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The successful combination of plasma and accelerator physics has resulted in the birth of new areas of research in which magnetized plasmas may be controlled to generate energy or in which light or particle beams are used to generate energetic particle beams, and those beams, in turn, are used to generate intense photon beams. In the past four decades, research with ever more intense laser and particle accelerator beams has increased our understanding of the interaction between ultra-intense light and matter. Those interactions arise from high-energy-density physics, nonlinear quantum electrodynamics, and radiation reaction forces, such as the creation of electron–positron pairs. The beams and plasma-physics section of Reviews of Modern Physics (RMP) has chronicled the key developments and, through its highly cited papers, has been an important partner in training the next generation of scientists.

Magnetized plasmas found in laboratory tokamak settings or as astrophysical plasmas in nature are rich in kinetic phenomena and particle-wave interactions. Researchers have been trying for a long time to harness the potential of controlled plasma fusion for energy production; the first experiments to use magnetized plasmas happened in the 1950s (see the article by David Pace, Bill Heidbrink, and Michael Van Zeeland, Physics Today, October 2015, page 34 ). To enable fusion reactions, the relatively low-density energetic plasmas must be confined for many seconds to several hours. Important topics that were covered in RMP include the physics of how electrons and ions behave in hot magnetized plasmas, the transport of energy and mass in a fusion reactor, 1 the excitation of waves, 2 and the heating of plasmas with driving currents. 3

How turbulence affects the magnetized plasma as it relaxes toward an equilibrium state continues to interest researchers (see the article by Richard Hazeltine and Stewart Prager, Physics Today, July 2002, page 30 ). Their understanding of complex behavior, such as magnetic reconnection 4 , 5 and nonlinear gyrokinetic theory, 6 is also fundamental for gaining control of the hot magnetized plasmas long enough to create a burning plasma suitable for generating copious amounts of energy.

Since the invention of the laser in 1960, nanosecond-duration laser pulses have progressed from containing tens of joules to megajoules of energy and have been used extensively to generate hot and dense plasmas. Scientists applied such technology to laser-driven, inertial confinement 7 and toward understanding astrophysically relevant, strongly coupled plasmas 8 in laboratory experiments 9 , 10 (see Physics Today, September 2015, page 16 ). Those breakthroughs have enabled the exploration of matter in states relevant to the physics of supernovae, supernova remnants, interstellar shock waves, photoevaporated molecular clouds, photoionized plasmas, and planetary interiors (see the article by Philipp Kronberg, Physics Today, December 2002, page 40 ).

The advent of ultra-intense femtosecond lasers has opened up access to new regimes of interaction between strong electromagnetic fields and plasma. 11 In the relativistic regime, the photon pressure exerted by the laser light can displace plasma electrons from ions. The resulting density waves that follow the laser pulse ripple through the plasma at velocities near the speed of light and support electric fields from a few to tens of gigavolts per meter; the electric fields can then accelerate electrons to high energies after they’ve traveled just a few centimeters 12 (see the article by Wim Leemans and Eric Esarey, Physics Today, March 2009, page 44 ). Researchers are using such laser plasma accelerators to develop ultracompact, mobile devices for scientific and societal applications, such as studying soil samples or art objects on location or destroying cancer cells in vivo. The generated ultrashort electron beams can be used to produce x rays and gamma rays 13 for imaging and spectroscopy with femtosecond time resolution. As such, they aim to complement the existing kilometer-scale, state-of-the-art conventional accelerators and are driving advances in scientific tools, such as free-electron lasers 14 for smaller-scale laboratory or industrial settings. In addition, the interaction of relativistically intense laser beams with solid materials has produced intense high-energy photons that are of higher-order harmonics than the incident laser photons. 15

At even higher laser intensities, the radiation pressure can result in ion motion and the generation of high-energy ion beams from dense target materials. 16 At laser intensities exceeding 1023 W/cm2, nonlinear quantum electrodynamics phenomena emerge with electron–positron pair production and a breakdown of the vacuum when the field strengths approach the Schwinger field limit. 11 , 17

This brief summary does not mention several topics in plasma physics and its intersections with other branches of physics, including Penning traps that have been used in antihydrogen production, plasmas for nanoassembly processing, and laser manipulation and acceleration of electrons. 18 As knowledge of plasma physics and the progress in laser- and particle-beam technology advances to open new frontiers, we foresee a continuing presence of exciting topics in beams and plasmas in the pages of RMP.

References

  1. 1. F. L. Hinton, R. D. Hazeltine, Rev. Mod. Phys. 48, 239 (1976). https://doi.org/10.1103/RevModPhys.48.239

  2. 2. W. Horton, Rev. Mod. Phys. 71, 735 (1999). https://doi.org/10.1103/RevModPhys.71.735

  3. 3. N. J. Fisch, Rev. Mod. Phys. 59, 175 (1987). https://doi.org/10.1103/RevModPhys.59.175

  4. 4. J. B. Taylor, Rev. Mod. Phys. 58, 741 (1986). https://doi.org/10.1103/RevModPhys.58.741

  5. 5. M. Yamada, R. Kulsrud, H. Ji, Rev. Mod. Phys. 82, 603 (2010). https://doi.org/10.1103/RevModPhys.82.603

  6. 6. A. J. Brizard, T. S. Hahm, Rev. Mod. Phys. 79, 421 (2007). https://doi.org/10.1103/RevModPhys.79.421

  7. 7. K. A. Brueckner, S. Jorna, Rev. Mod. Phys. 46, 325 (1974). https://doi.org/10.1103/RevModPhys.46.325

  8. 8. S. Ichimaru, Rev. Mod. Phys. 54, 1017 (1982). https://doi.org/10.1103/RevModPhys.54.1017

  9. 9. B. A. Remington, R. P. Drake, D. D. Ryutov, Rev. Mod. Phys. 78, 755 (2006). https://doi.org/10.1103/RevModPhys.78.755

  10. 10. S. H. Glenzer, R. Redmer, Rev. Mod. Phys. 81, 1625 (2009). https://doi.org/10.1103/RevModPhys.81.1625

  11. 11. G. A. Mourou, T. Tajima, S. V. Bulanov, Rev. Mod. Phys. 78, 309 (2006). https://doi.org/10.1103/RevModPhys.78.309

  12. 12. E. Esarey, C. B. Schroeder, W. P. Leemans, Rev. Mod. Phys. 81, 1229 (2009). https://doi.org/10.1103/RevModPhys.81.1229

  13. 13. S. Corde et al., Rev. Mod. Phys. 85, 1 (2013). https://doi.org/10.1103/RevModPhys.85.1

  14. 14. C. Pellegrini, A. Marinelli, S. Reiche, Rev. Mod. Phys. 88, 015006 (2016). https://doi.org/10.1103/RevModPhys.88.015006

  15. 15. U. Teubner, P. Gibbon, Rev. Mod. Phys. 81, 445 (2009). https://doi.org/10.1103/RevModPhys.81.445

  16. 16. A. Macchi, M. Borghesi, M. Passoni, Rev. Mod. Phys. 85, 751 (2013). https://doi.org/10.1103/RevModPhys.85.751

  17. 17. M. Marklund, P. K. Shukla, Rev. Mod. Phys. 78, 591 (2006). https://doi.org/10.1103/RevModPhys.78.591

  18. 18. R. J. England et al., Rev. Mod. Phys. 86, 1337 (2014). https://doi.org/10.1103/RevModPhys.86.1337

More about the Authors

Wim Leemans now directs the accelerator division at DESY (German Electron Synchrotron) in Hamburg, after more than 27 years of research at Lawrence Berkeley National Laboratory in Berkeley, California.

This Content Appeared In
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Volume 72, Number 2

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