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Investigation of tunable coherent XUV light source by high harmonics generation using intense femtosecond laser pulses in Ne

Lu Fa-Ming Xia Yuan-Qin Zhang Sheng Chen De-Ying

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Investigation of tunable coherent XUV light source by high harmonics generation using intense femtosecond laser pulses in Ne

Lu Fa-Ming, Xia Yuan-Qin, Zhang Sheng, Chen De-Ying
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  • The buleshift properties of high-harmonic generation with phase matching of different filling pressures and laser intensities are experimentally investigated in this paper. The laser buleshift generated in gas cell, with about 0.13 nm in plateau and 0.07 nm in cutoff is obtained. The buleshift is influenced by simply changing the filling pressure and laser intensity, namely, by varying the density of free electrons in gas cell.
    • Funds: Project supported by the National Natural Science Foundation of China (Grant No. 10774033).
    [1]

    Protopapas M, Keitel C H, Knight P L 1997 Rep. Prog. Phys. 60 389

    [2]

    Hasegawa H, Takahashi E J, Navekawa Y, Ishikawa K L, Midorikawa K 2005 Phys. Rev. A 71 023407

    [3]

    Itatani J, Zeidler D, Levesque J, Spanner M, Villeneuve D M, Corkum P B 2004 Nature 432 867

    [4]

    Wagner N L, West A, Christov I P, Popmintchev T, Zhou X B, Murnane M M, Kapteyn H C 2006 Proc. Natl. Acad. Sci. 103 13279

    [5]

    Baker S, Robinson J S, Haworth C A, Teng H, Smith R A, Chirilă C C, Lein M, Tisch J W G, Marangos J P 2006 Science 312 424

    [6]

    Corkum P B 1993 Phys. Rev. Lett. 71 1994

    [7]

    Lewenstein M, Balcou Ph, Ivanov M Yu, Huillier A L', Corkum P B 1994 Phys. Rev. A 49 2117

    [8]

    Wahlström C G, Larsson J, Persson A, Starczewaki T, Svanberg S 1993 Phys. Rev. A 48 4709

    [9]

    Kan C, Capjack C E, Rankin R 1995 Phys. Rev. A 52 R4336

    [10]

    Shin H J, Lee D G, Cha Y H, Hong K H, Nam C H 1999 Phys. Rev. Lett. 83 2544

    [11]

    Altucci C, Bruzzese R, Lisio C de, Nisoli M, Stagira S, Silvestri S De, Svelto O, Boscolo A, Ceccherini P, Poletto L, Tondello G, Villoresi P 1999 Phys. Rev. A 61 021801-1

    [12]

    Reitze D H, Kazamias S, Weihe F, Mullot G, Douillet D, Augé F, Albert O, Ramanathan V, Chambaret J P, Hulin D, Balcou P 2004 Opt. Lett. 29 86

  • [1]

    Protopapas M, Keitel C H, Knight P L 1997 Rep. Prog. Phys. 60 389

    [2]

    Hasegawa H, Takahashi E J, Navekawa Y, Ishikawa K L, Midorikawa K 2005 Phys. Rev. A 71 023407

    [3]

    Itatani J, Zeidler D, Levesque J, Spanner M, Villeneuve D M, Corkum P B 2004 Nature 432 867

    [4]

    Wagner N L, West A, Christov I P, Popmintchev T, Zhou X B, Murnane M M, Kapteyn H C 2006 Proc. Natl. Acad. Sci. 103 13279

    [5]

    Baker S, Robinson J S, Haworth C A, Teng H, Smith R A, Chirilă C C, Lein M, Tisch J W G, Marangos J P 2006 Science 312 424

    [6]

    Corkum P B 1993 Phys. Rev. Lett. 71 1994

    [7]

    Lewenstein M, Balcou Ph, Ivanov M Yu, Huillier A L', Corkum P B 1994 Phys. Rev. A 49 2117

    [8]

    Wahlström C G, Larsson J, Persson A, Starczewaki T, Svanberg S 1993 Phys. Rev. A 48 4709

    [9]

    Kan C, Capjack C E, Rankin R 1995 Phys. Rev. A 52 R4336

    [10]

    Shin H J, Lee D G, Cha Y H, Hong K H, Nam C H 1999 Phys. Rev. Lett. 83 2544

    [11]

    Altucci C, Bruzzese R, Lisio C de, Nisoli M, Stagira S, Silvestri S De, Svelto O, Boscolo A, Ceccherini P, Poletto L, Tondello G, Villoresi P 1999 Phys. Rev. A 61 021801-1

    [12]

    Reitze D H, Kazamias S, Weihe F, Mullot G, Douillet D, Augé F, Albert O, Ramanathan V, Chambaret J P, Hulin D, Balcou P 2004 Opt. Lett. 29 86

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Publishing process
  • Received Date:  05 June 2012
  • Accepted Date:  19 July 2012
  • Published Online:  05 January 2013

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