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Generation of attosecond X-ray pulse of wavelength below 0.4 nm from the interaction of ultra-relativistic intense lasers with thin foil targets

Bai Yi-Ling Zhang Qiu-Ju Tian Mi Cui Chun-Hong

Generation of attosecond X-ray pulse of wavelength below 0.4 nm from the interaction of ultra-relativistic intense lasers with thin foil targets

Bai Yi-Ling, Zhang Qiu-Ju, Tian Mi, Cui Chun-Hong
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  • By one-dimensional particle-in-cell simulations, the relativistic electron sheets generated by interaction between the ultra-relativistic intense laser pulse with intensity above 1022 W/cm2 and the thin foil target, as well as the attosecond X-ray pulses induced by Thomson backscattering from electron bunch are studied in this paper. The results indicate that increasing the intensity of the driving laser, reducing the density and thickness of foil target corresponding make the longitudinal momentum of the electrons enhanced and the wavelength of X-ray radiation reduced. Attosecond X-ray pulse with wavelength 1.168 nm can be obtained through optimizing correlated parameters. Especially, using probing laser pulse with doubling frequency and optimizing parameters of the drive light and thin film target can make the wavelength of coherent attosecond X-ray radiation reduced obviously, even below 0.4 nm, and the energy of the scattered photons can achieve more than 2 keV.
    • Funds: Project supported by the National Natural Science Foundation of China (Grant No. 11104168).
    [1]

    Drescher M, Hentschel M, Kienberger R, Tempea G, Spielmann C, Reider G A, Corkum P B, Krausz F 2001 Science 291 1923

    [2]

    Hentschel M, Kienberger R, Spielmann C, Reider G A, Milosevie N, BrabecT, Corkum P, Heinzmann U, Drescher M, Krausz F 2001 Nature 414 509

    [3]

    Zeng Z N, Li R X, Xie X H, Xu Z Z 2004 Acta Phys. Sin. 53 2316 (in Chinese) [曾志男, 李儒新, 谢新华, 徐至展 2004 物理学报 53 2316]

    [4]

    Wang Q, Chen J X, Xia Y Q, Chen D Y 2003 Chin. Phys. 12 524

    [5]

    Lan P F, Lu P X, Cao W, Wang X L 2005 Phys. Rev. E 72 066501

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    Lan P F, Lu P X, Cao W, Wang X L 2006 Phys. Plasmas 13 013106

    [7]

    Zheng J, Sheng Z M, Zhang J, Wei Z Y, Yu W 2005 Acta Phys. Sin. 54 1018 (in Chinese) [郑 君, 盛政明, 张 杰, 魏志义, 余 玮 2005物理学报 54 1018]

    [8]

    Zhang P, Song Y R, Zhang Z G 2006 Acta Phys. Sin. 55 6208 (in Chinese) [张 鹏, 宋晏蓉, 张志刚 2006物理学报 55 6208]

    [9]

    Kaplan A K 1994 Phys. Rev. Lett. 73 1243

    [10]

    Esarey E, Ride S K, Sprangle P 1993 Phys. Rev. E 48 3003

    [11]

    Schoenlein R W, Leemans W P, Chin A H, Volfbeyn P, Glover T E, Balling P, Zolotorev M, Kim K J, Chattopadhyay S, Shank C V 1996 Science 274 236

    [12]

    Wang F C, Shen B F, Zhang X M, Li X M, Jin Z Y 2007 Phys. Plasmas 14 083102

    [13]

    Kulagin V V, Vladimir A 2007 Phys. Rev. Lett. 99 124801

    [14]

    Leemans W P, Schoenlein R W, Volfbeyn P, Chin A H, Glover T E, Balling P, Zolotorev M, Kim K J, Chattopadhyay S, Shank C V 1997 J. Quan. Elec. 33 1925

    [15]

    Pogorelsky I V, Ben-Zvi I, Hirose T, Kashiwagi S, Yakimenkol V, Kuschel K, Siddonsl P, Skaritkal J, Kumita T, Tsunemi A, Omori T, Urakawa T, Washio M, Yokoya K, Okugi T, Liu Y, He P, Cline D 2000 Phys. Rev. ST Accel. Beams 3 090702

    [16]

    Zheng J, Sheng Z M, Zhang J 2005 Acta Phys. Sin. 54 2638 (in Chinese) [郑 君, 盛政明, 张 杰 2005 物理学报 54 2638]

    [17]

    Uesaka M, Kotaki H, Nakajima K, Harono H, Kinoshita K, Watanable T, Ueda T, Yoshii K, Kadno M, Dewa H, Kondo S, Sakai F 2000 Nucl. Instrum. Methods Phys. Res. A 455 90

    [18]

    Li Y, Huang Z, Borland M D, Milton S 2003 Phys. Rev. ST Accel. Beams 5 044701

    [19]

    Anderson S G, Barty C P J, Betts S M, Brown W J, Crane J K, Cross R R, Fittinghoff D N, Gibson D J, Hartemann F V, Kuba J, Lesage G P, Rosenzweig J B, Slaughter D R, Springer D T, Tremaine A M 2004 Appl. Phys. B 78 891

    [20]

    Meyer-ter-Vehn J, Wu H C 2009 Eur. Phys. J. D 55 433

    [21]

    Yan C Y, Zhang Q J, Luo M H 2011 Acta Phys. Sin. 60 035202 (in Chinese) [闫春燕, 张秋菊, 罗牧华 2011 物理学报 60 035202]

    [22]

    Wu H C, Meyer-ter-Vehn J, Fernández J, Hegelich B M 2010 Phys. Rev. Lett. 104 234801

    [23]

    Wu H C, Meyer-ter-Vehn J, Hegelich B M, Fernández J 2011 Phys. Rev. ST Accel. Beams 14 070702

    [24]

    Wu H C, Meyer-ter-Vehn J 2012 Nature 6 304

    [25]

    Jia Q Q, Wang W M, Dong Q L, Sheng Z M 2012 Acta Phys. Sin. 61 015203 (in Chinese) [贾倩倩, 王伟民, 董全力, 盛政明2012物理学报 61 015203]

  • [1]

    Drescher M, Hentschel M, Kienberger R, Tempea G, Spielmann C, Reider G A, Corkum P B, Krausz F 2001 Science 291 1923

    [2]

    Hentschel M, Kienberger R, Spielmann C, Reider G A, Milosevie N, BrabecT, Corkum P, Heinzmann U, Drescher M, Krausz F 2001 Nature 414 509

    [3]

    Zeng Z N, Li R X, Xie X H, Xu Z Z 2004 Acta Phys. Sin. 53 2316 (in Chinese) [曾志男, 李儒新, 谢新华, 徐至展 2004 物理学报 53 2316]

    [4]

    Wang Q, Chen J X, Xia Y Q, Chen D Y 2003 Chin. Phys. 12 524

    [5]

    Lan P F, Lu P X, Cao W, Wang X L 2005 Phys. Rev. E 72 066501

    [6]

    Lan P F, Lu P X, Cao W, Wang X L 2006 Phys. Plasmas 13 013106

    [7]

    Zheng J, Sheng Z M, Zhang J, Wei Z Y, Yu W 2005 Acta Phys. Sin. 54 1018 (in Chinese) [郑 君, 盛政明, 张 杰, 魏志义, 余 玮 2005物理学报 54 1018]

    [8]

    Zhang P, Song Y R, Zhang Z G 2006 Acta Phys. Sin. 55 6208 (in Chinese) [张 鹏, 宋晏蓉, 张志刚 2006物理学报 55 6208]

    [9]

    Kaplan A K 1994 Phys. Rev. Lett. 73 1243

    [10]

    Esarey E, Ride S K, Sprangle P 1993 Phys. Rev. E 48 3003

    [11]

    Schoenlein R W, Leemans W P, Chin A H, Volfbeyn P, Glover T E, Balling P, Zolotorev M, Kim K J, Chattopadhyay S, Shank C V 1996 Science 274 236

    [12]

    Wang F C, Shen B F, Zhang X M, Li X M, Jin Z Y 2007 Phys. Plasmas 14 083102

    [13]

    Kulagin V V, Vladimir A 2007 Phys. Rev. Lett. 99 124801

    [14]

    Leemans W P, Schoenlein R W, Volfbeyn P, Chin A H, Glover T E, Balling P, Zolotorev M, Kim K J, Chattopadhyay S, Shank C V 1997 J. Quan. Elec. 33 1925

    [15]

    Pogorelsky I V, Ben-Zvi I, Hirose T, Kashiwagi S, Yakimenkol V, Kuschel K, Siddonsl P, Skaritkal J, Kumita T, Tsunemi A, Omori T, Urakawa T, Washio M, Yokoya K, Okugi T, Liu Y, He P, Cline D 2000 Phys. Rev. ST Accel. Beams 3 090702

    [16]

    Zheng J, Sheng Z M, Zhang J 2005 Acta Phys. Sin. 54 2638 (in Chinese) [郑 君, 盛政明, 张 杰 2005 物理学报 54 2638]

    [17]

    Uesaka M, Kotaki H, Nakajima K, Harono H, Kinoshita K, Watanable T, Ueda T, Yoshii K, Kadno M, Dewa H, Kondo S, Sakai F 2000 Nucl. Instrum. Methods Phys. Res. A 455 90

    [18]

    Li Y, Huang Z, Borland M D, Milton S 2003 Phys. Rev. ST Accel. Beams 5 044701

    [19]

    Anderson S G, Barty C P J, Betts S M, Brown W J, Crane J K, Cross R R, Fittinghoff D N, Gibson D J, Hartemann F V, Kuba J, Lesage G P, Rosenzweig J B, Slaughter D R, Springer D T, Tremaine A M 2004 Appl. Phys. B 78 891

    [20]

    Meyer-ter-Vehn J, Wu H C 2009 Eur. Phys. J. D 55 433

    [21]

    Yan C Y, Zhang Q J, Luo M H 2011 Acta Phys. Sin. 60 035202 (in Chinese) [闫春燕, 张秋菊, 罗牧华 2011 物理学报 60 035202]

    [22]

    Wu H C, Meyer-ter-Vehn J, Fernández J, Hegelich B M 2010 Phys. Rev. Lett. 104 234801

    [23]

    Wu H C, Meyer-ter-Vehn J, Hegelich B M, Fernández J 2011 Phys. Rev. ST Accel. Beams 14 070702

    [24]

    Wu H C, Meyer-ter-Vehn J 2012 Nature 6 304

    [25]

    Jia Q Q, Wang W M, Dong Q L, Sheng Z M 2012 Acta Phys. Sin. 61 015203 (in Chinese) [贾倩倩, 王伟民, 董全力, 盛政明2012物理学报 61 015203]

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  • Received Date:  14 September 2012
  • Accepted Date:  09 March 2013
  • Published Online:  20 June 2013

Generation of attosecond X-ray pulse of wavelength below 0.4 nm from the interaction of ultra-relativistic intense lasers with thin foil targets

  • 1. College of Physics and Electronics, Shandong Normal University, Jinan 250014, China
Fund Project:  Project supported by the National Natural Science Foundation of China (Grant No. 11104168).

Abstract: By one-dimensional particle-in-cell simulations, the relativistic electron sheets generated by interaction between the ultra-relativistic intense laser pulse with intensity above 1022 W/cm2 and the thin foil target, as well as the attosecond X-ray pulses induced by Thomson backscattering from electron bunch are studied in this paper. The results indicate that increasing the intensity of the driving laser, reducing the density and thickness of foil target corresponding make the longitudinal momentum of the electrons enhanced and the wavelength of X-ray radiation reduced. Attosecond X-ray pulse with wavelength 1.168 nm can be obtained through optimizing correlated parameters. Especially, using probing laser pulse with doubling frequency and optimizing parameters of the drive light and thin film target can make the wavelength of coherent attosecond X-ray radiation reduced obviously, even below 0.4 nm, and the energy of the scattered photons can achieve more than 2 keV.

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