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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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[1] |
Campbell E M, Hunt J T, Bliss E S, Speck D R and Drake R P 1986 Rev. Sci. Instrum. 57 2101
|
[2] |
Yamanaka C, Nakai S, Yamanaka T, Izawa Y, Kato Y, Mima K, Nishihara K, Mochizuki T, Yamanaka M, Nakatsuka M, Sasaki T, Yabe T, Yoshida K, Azechi H, Nishimura H, Norimatsu T, Ido S, Miyanaga N, Sakabe S, Takabe H, Jitsuno J and Takagi M 1987 Nucl. Fusion 27 19
|
[3] |
Boehly T R, McCrory R L, Verdon C P, Seka W, Loucks S J, Babushkin A, Bahr R E, Boni R, Bradley D K, Craxton R S, Delettrez J A, Donaldson W R, Epstein R, Harding D, Jaanimagi P A, Jacobs S D, Kearney K, Keck R L, Kelly J H, Kessler T J, Kremens R L, Knauer J P, Lonobile D J, Lund L D, Marshall F J, McKenty P W, Meyerhofer D D, Morse S F B, Okishev A, Papernov S, Pien G, Safford T, Schnittman J D, Short R, Shoup M J, Skeldon M, Skupsky S, Schmid A W, Smalyuk V A, Smith D J, Soures J M, Wittman M and Yaakobi B 1999 Fusion Eng. Des. 44 35
|
[4] |
Ryutov D D, Derzon M S and Matzen M K 2000 Rev. Mod. Phys. 72 167
|
[5] |
Lebedev S V, Chittenden J P, Beg F N, Bland S N, Ciardi A, Ampleford D, Hughes S, Haines M G, Frank A, Blackman E G and Gardiner T 2002 Astrophys. J. 564 113
|
[6] |
Ryutov D D, Drake R P, Kane J, Liang E, Remington B A and Wood-Vasey W M 1999 Astrophys. J. 518 821
|
[7] |
Ryutov D D, Remington B A and Robey H F 2001 Phys. Plasmas 8 1804
|
[8] |
Remington B A 2005 Plasma Phys. Control. Fusion 47 A191
|
[9] |
Treumann R A 2009 Astron Astrophys. Rev. 17 409
|
[10] |
Bykov A M and Treumann R A 2011 Astron Astrophys. Rev. 19 42
|
[11] |
Yamada M 2007 Phys. Plasmas 14 058102
|
[12] |
Zweibel E and Yamada M 2009 Annu. Rev. Astron. Astrophys. 47 291
|
[13] |
Mizuta A, Yamada S and Takabe H 2002 Astrophys. J. 567 635
|
[14] |
Farley D R, Estabrook K G, Glendinning S G, Glenzer S H, Remington B A, Shigemori K, Stone J M, Wallace R J, Zimmerman G B and Harte J A 1999 Phys. Rev. Lett. 83 1892
|
[15] |
Zhong J Y, Li Y T, Wang X G, Wang J Q, Dong Q L, Xiao C J, Wang S J, Liu X, Zhang L, An L, Wang F L, Zhu J Q, Gu Y, He X T, Zhao G and Zhang J 2010 Nat. Phys. 6 984
|
[16] |
Gregori G, Ravasio A, Murphy C D, Schaar K, Baird A, Bell A R, Benuzzi-Mounaix A, Bingham R, Constantin C, Drake R P, Edwards M, Everson E T, Gregory C D, Kuramitsu Y, Lau W, Mithen J, Niemann C, Park H S, Remington B A, Reville B, Robinson A P L, Ryutov D D, Sakawa Y, Yang S, Woolsey N C, Koenig M and Miniati F 2012 Nature 481 480
|
[17] |
Carley E P, Long D M, Byrne J P, Zucca P, Bloomfield D S, McCauley J and Gallagher P T 2013 Nat. Phys. 9 811
|
[18] |
Meinecke J, Doyle H W, Miniati F, Bell A R, Bingham R, Crowston R, Drake R P, Fatenejad M, Koenig M, Kuramitsu Y, Kuranz C C, Lamb D Q, Lee D, MacDonald M J, Murphy C D, Park H S, Pelka A, Ravasio A, Sakawa Y, Schekochihin A A, Scopatz A, Tzeferacos P, Wan W C, Woolsey N C, Yurchak R, Reville B and Gregori G 2014 Nat. Phys. 10 520
|
[19] |
Aharonian F A, Akhperjanian A G, Aye K M, et al. 2004 Nature 432 75
|
[20] |
Uchiyama Y, Aharonian F A, Tanaka T, Takahashi T and Maeda Y 2007 Nature 449 576
|
[21] |
Remington B A, Drake R P and Ryutov D D 2006 Rev. Mod. Phys. 78 755
|
[22] |
Takabe H, Nagatomo H, Sunahara A, Ohnishi N, Mahdy A I, Yoda Y, Naruo S, Azechi H, Nishimura H and Mima K 1999 Plasma Phys. Control. Fusion 41 A75
|
[23] |
Zhang J and Zhao G 2000 Physics 29 393 (in Chinese)
|
[24] |
Bamba A, Yamazaki R, Ueno M and Koyama K 2003 Astrophys. J. 589 827
|
[25] |
Kugland N L, Ross J S, Chang P Y, Drake R P, Fiksel G, Froula D H, Glenzer S H, Gregori G, Grosskopf M, Huntington C, Koenig M, Kuramitsu Y, Kuranz C, Levy M C, Liang E, Martinez D, Meinecke J, Miniati F, Morita T, Pelka A, Plechaty C, Presura R, Ravasio A, Remington B A, Reville B, Ryutov D D, Sakawa Y, Spitkovsky A, Takabe H and Park H S 2013 Phys. Plasmas 20 056313
|
[26] |
Buneman O 1959 Phys. Rev. 115 503
|
[27] |
Weibel E S 1959 Phys. Rev. Lett. 2 83
|
[28] |
Forslund D W and Shonk C R 1970 Phys. Rev. Lett. 25 1699
|
[29] |
Taylor R J, Baker D R and Ikezi H 1970 Phys. Rev. Lett. 24 206
|
[30] |
Kato T N and Takabe H 2008 Astrophys. J. 681 L93
|
[31] |
Fiuza F, Fonseca R A, Tonge J, Mori W B and Silva L O 2012 Phys. Rev. Lett. 108 235004
|
[32] |
Bell A R and Lucek S G 1996 Mon. Not. R. Astron. Soc. 283 1083
|
[33] |
Blandford R D and Ostriker J 1978 Astrophys. J. Lett. 221 L29
|
[34] |
Axford W I, Leer E and McKenzie J F 1982 Astron. Astrophys. 111 317
|
[35] |
Holman G D and Pesses M E 1983 Astrophys. J. 267 837H
|
[36] |
Drury L O'C 1983 Rep. Prog. Phys. 46 973
|
[37] |
Fermi E 1949 Phys. Rev. 75 1169
|
[38] |
Cosmic Particle Accelerators Identified 2013 Science 342 1438
|
[39] |
Takabe H, Kato T N, Sakawa Y, Kuramitsu Y, Morita T, Kadono T, Shigemori K, Otani K, Nagatomo H, Norimatsu T, Dono S, Endo T, Miyanishi K, Kimura T, Shiroshita A, Ozaki N, Kodama R, Fujioka S, Nishimura H, Salzman D, Loupias B, Gregory C, Koenig M, Waugh J N, Woolsey N C, Kato D, Li Y T, Dong Q L, Wang S J, Zhang Y, Zhao J, Wang F L, Wei H G, Shi J R, Zhao G, Zhang J Y, Wen T S, Zhang W H, Hu X, Liu S Y, Ding Y K, Zhang L, Tang Y J, Zhang B H, Zheng Z J, Sheng Z M and Zhang J 2008 Plasma Phys. Control. Fusion 50 124057
|
[40] |
Chenais-Popovics C, Renaudin P, Rancu O, Gilleron F, Gauthier J C, Larroche O, Peyrusse O, Dirksmöller M, Sondhauss P, Missalla T, Uschmann I, Förster E, Renner O and Krousky E 1997 Phys. Plasmas 4 190
|
[41] |
Kugland N L, Ryutov D D, Plechaty C, Ross J S and Park H S 2012 Rev. Sci. Instrum. 83 101301
|
[42] |
Borghesi M, Giulietti A, Giulietti D, Gizzi L A, Macchi A and Willi O 1996 Phys. Rev. E 54 6769
|
[43] |
Drake R P 2000 Phys. Plasmas 7 4690
|
[44] |
Courtois C, Grundy R A D, Ash A D, Chambers D M, Woolsey N C, Dendy R O and McClements K G 2004 Phys. Plasmas 11 3386
|
[45] |
Sorasio G, Marti M, Fonseca R and Silva L O 2006 Phys. Rev. Lett. 96 045005
|
[46] |
Kato T N and Takabe H 2010 Phys. Plasmas 17 032114
|
[47] |
Morita T, Sakawa Y, Kuramitsu Y, Dono S, Aoki H, Tanji H, Kato T N, Li Y T, Zhang Y, Liu X, Zhong J Y, Takabe H and Zhang J 2010 Phys. Plasmas 17 122702
|
[48] |
Liu X, Li Y T, Zhang Y, Zhong J Y, Zheng W D, Dong Q L, Chen M, Zhao G, Sakawa Y, Morita T, Kuramitsu Y, Kato T N, Chen L M, Lu X, Ma J L, Wang W M, Sheng Z M, Takabe H, Rhee Y J, Ding Y K, Jiang S E, Liu S Y, Zhu J Q and Zhang J 2011 New J. Phys. 13 093001
|
[49] |
Kuramitsu Y, Sakawa Y, Morita T, Gregory C D, Waugh J N, Dono S, Aoki H, Tanji H, Koenig M, Woolsey N and Takabe H 2011 Phys. Rev. Lett. 106 175002
|
[50] |
Kugland N L, Ryutov D D, Chang P Y, Drake R P, Fiksel G, Froula D H, Lenzer S H, Gregori G, Grosskopf M, Koenig M, Kuramitsu Y, Kuranz C, Levy M C, Liang E, Meinecke J, Miniati F, Morita T, Pelka A, Plechaty C, Presura R, Ravasio A, Remington B A, Reville B, Ross J S, Sakawa Y, Spitkovsky A, Takabe H and Park H S 2012 Nat. Phys. 8 809
|
[51] |
Li Y T, Sheng Z M, Chen L M, Lu X, Ma J L, Dong Q L, Wang Z H, Wei Z Y and Zhang J 2009 The 8th Pacific Rim Conference on Lasers and Electro-Optics August 30-September 3, 2009 Shanghai, China
|
[52] |
Yuan D W, Li Y T, Su L N, Liao G Q, Yin C L, Zhu B J and Zhang J 2013 Science China Phys. Mech. & Astro. 56 2381
|
[53] |
Kato T N 2005 Phys. Plasmas 12 080705
|
[54] |
Fox W, Fikse G, Bhattacharjee A, Chang P Y, Germaschewski K, Hu S X and Nilson P M 2013 Phys. Rev. Lett. 111 225002
|
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