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Influence of Initial Pulse Chirp on Rainbow-Like Supercontinuum Generation from Filamentation in Air

Influence of Initial Pulse Chirp on Rainbow-Like Supercontinuum Generation from Filamentation in Air
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摘要 Supereontinuum (SC) generation from laser filamentation in air is found to depend strongly on the pulse duration. Rainbow-like SC generation is observed only for a pulse of appropriate negative chirp that agrees with the predictions put forward by Golubtsov et al. [Quantum Electron. 33 (2003) 525]. The conversion efficiency of an 800-nm laser light to rainbow-like SC is found to be the highest for 257fs pulses with an initial negative chirp. A larger chirp will lead to filamentation surviving at longer distance. Supereontinuum (SC) generation from laser filamentation in air is found to depend strongly on the pulse duration. Rainbow-like SC generation is observed only for a pulse of appropriate negative chirp that agrees with the predictions put forward by Golubtsov et al. [Quantum Electron. 33 (2003) 525]. The conversion efficiency of an 800-nm laser light to rainbow-like SC is found to be the highest for 257fs pulses with an initial negative chirp. A larger chirp will lead to filamentation surviving at longer distance.
出处 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第4期1365-1367,共3页 中国物理快报(英文版)
基金 Supported by the National Natural Science Foundation of China under Grant Nos 10634020, 10390161, 60621063, and 10734130, the National Basic Research Programme of China Grant No 2007CB815100, and the National Hi-Tech ICF Project.
关键词 supernova explosion proto-neutron star shock wave supernova explosion, proto-neutron star, shock wave
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参考文献22

  • 1Braun A, Korn G, Liu X, Du D, Squier J and Mourou G 1995 Opt. Lett. 20 73
  • 2Xi T T, Lu X and Zhang J 2006 Phys. Rev. Lett. 96 025003
  • 3Woste L, Wedekind C, Wille H, Rairoux P, Stein B, Nikolov S, Werner C, Niedermeier S, Ronneberger F, Schillinger H and Sauerbrey R 1997 Las. Optoelektron. 29 51
  • 4Tzortzakis S, Franco M A, Andre Y B, Chiron A, Lamouroux B, Prade B S and Mysyrowicz A 1999 Phys. Rev. E 60 3505
  • 5Zhang Z, Zhang J, Li Y T, Hao Z Q, Zheng Z Y, Yuan X H and Wang Z H 2007 Acta Phys. Sin. 55 357
  • 6Liu J S, Schroeder H, Chin S L, Li R X and Xu Z Z, 2005 Appl. Phys. Lett. 87 161105
  • 7Kasparian J, Sauerbrey R, Mondelain D, Niedermeier S, Yu J, Wolf J P, Andre Y B, Franco M, Prade B, Tzortzakis S, Mysyrowicz A, Rodriguez M, Wille H and Woste L 2000 Opt. Lett. 25 1397
  • 8Hao Z Q, Zhang J, Zhang Z, Yuan X H, Zheng Z Y, Lu X, Jin Z, Wang Z H, Zhong J Y and Liu Y Q 2006 Phys. Rev. E 74 066402
  • 9Kasparian J, Rodriguez M, Mejean G, Yu J, Salmon E, Wille H, Bourayou R, Frey S, Andre Y B, Mysyrowicz A, Sauerbrey R, Wolf J P and WSste L 2003 Science 301 61
  • 10Hao Z Q, Zhang J, Lu X, Xi T T, Li Y T, Yuan X H, Zheng Z Y, Wang Z H, Ling W J and Wei Z Y 2006 Opt. Express 14 773

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