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Special Issue:
TOPICAL REVIEW — Ultrafast intense laser science
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| TOPICAL REVIEW—Ultrafast intense laser science |
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Studies of collisionless shockwaves using high-power laser pulses in laboratories |
| Yuan Da-Wei (袁大伟), Li Yu-Tong (李玉同) |
| National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China |
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Abstract The remarkable experimental progress in the studies of collisionless shockwave (CS) in laboratories employing high-power lasers is briefly reviewed. The results show that CS can be generated in laser-produced plasmas due to the micro-turbulence associated with instabilities. CS is one of the most important astronomical phenomena. It has been found in supernova remnants (SNRs), Sun-Earth space, etc. This paper focuses on CS in ways relevant to SNRs. Laboratory astrophysics (LA), a new interdisciplinary frontier of astrophysics, plasma and laser physics, has developed rapidly in recent years. As an accessory to the astronomical observation, LA experimenters can closely study some astronomical events scaled-down to controllable phenomena.
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Received: 19 August 2014
Revised: 11 October 2014
Accepted manuscript online:
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PACS:
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52.35.Tc
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(Shock waves and discontinuities)
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52.35.Fp
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(Electrostatic waves and oscillations (e.g., ion-acoustic waves))
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52.35.Hr
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(Electromagnetic waves (e.g., electron-cyclotron, Whistler, Bernstein, upper hybrid, lower hybrid))
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| Fund: Project supported by the National Basic Research Program of China (Grant No. 2013CBA01501) and the National Natural Science Foundation of China (Grant No. 11135012). |
Corresponding Authors:
Li Yu-Tong
E-mail: ytli@iphy.ac.cn
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Cite this article:
Yuan Da-Wei (袁大伟), Li Yu-Tong (李玉同) Studies of collisionless shockwaves using high-power laser pulses in laboratories 2015 Chin. Phys. B 24 015204
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