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We demonstrate a femtosecond Ti: sapphire oscillator with ultralow repetition rate and ultrahigh peak power by inserting a specially designed Herriott telescope to increase the length of the cavity.By analyzing the intra-cavity dispersion and optimizing the extra-cavity compressor, stable pulses with repetition rate of 11 MHz and single pulse energy higher than 72nJ was obtained under 532 nm pump laser with average power of 8.2 W.The peak power of the pulses from the novel cavity is much higher than that from the original oscillators.
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Keywords:
- femtosecond laser /
- Ti: sapphire laser /
- low repetition rate /
- MW
[1] [1] Spence D E, Kean P N, Sibbett W 1991 Opt. Lett. 16 42
[2] [2]Bartels A, Dekorsy T, Kurz H 1999 Opt. Lett. 24 996
[3] [3]Foggi P, Bussotti L, Neiuwahl F V R 2001 Int. J. Photoenergy 3 103
[4] [4]Liu Q M, He X, Gan F X, Qian S X 2009 Acta Phys. Sin. 58 1002 (in Chinese) [刘启明、何漩、干福熹、钱世雄 2009 58 1002]
[5] [5]Kowalevicz A M, Sharma V, Ippen E P, Fujimoto J G, Minoshima K 2005 Opt. Lett. 30 964
[6] [6]Osellame R, Chiodo N, Maselli V, Yin A, Zavelani-Rossi M, Cerullo G, Laporta P 2005 Opt. Express 13 612
[7] [7]Yu B H, Dai N L, Wang Y, Li Y H, Ji L L, Zheng Q G, Lu P X 2007 Acta Phys. Sin. 56 5821 (in Chinese)[于本海、戴能利、王英、李玉华、季玲玲、郑启光、陆培祥 2007 56 5821]
[8] [8]Beddard T, Sibbett W, Reid D T, Garduno-Mejia J, Jamasbi N, Mohebi M 1999 Opt. Lett. 24 163
[9] [9]Zhou X, Kapteyn H, Murnane M 2007 Springer. Ser. Chem. Phys. 88 104
[10] ]Brabec Th, Krausz K 2000 Rev. Mod. Phys. 72 545
[11] ]Nejadmalayeri A H, Herman P R, Burghoff J, Will M, Nolte S T?nnermann A 2005 Opt. Lett. 30 964
[12] ]Takeshima N, Narita Y, Tanaka S, Kuroiwa Y, Hirao K 2005 Opt. Lett. 30 352
[13] ]Sanner N, Huot N, Audouard E, Larat C, Laporte P, Huignard J P 2005 Appl. Phys. B80 27
[14] ]Naumov S, Fernandez A, Graf R, Dombi P, Krausz F, Apolonski A 2005 New. J. Phys. 7 216
[15] ]Sennaroglu A, Fujimoto J G 2003 Opt. Express 11 1106
[16] ]Zhao Y Y, Han H N, Teng H, Wei Z Y 2009 Acta Phys. Sin. 58 1709 (in Chinese)[赵研英、韩海年、滕浩、魏志义 2009 58 1709]
[17] ]Kalashnikov V L, Podivilov E, Chernykh A, Naumov S, Fernandez A, Graf R, Apolonski A 2005 New. J. Phys. 7 217
[18] ]Wolf E 2004 Prog. Opt. 46 55
[19] ]Backus S, Durfee III C G, Murnane M M, Kapteyn H C 1998 Rev. Sci. Instrum. 69 1207
[20] ]Fork R L, Martinez O E, Gordon J P 1984 Opt. Lett. 9 150
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[1] [1] Spence D E, Kean P N, Sibbett W 1991 Opt. Lett. 16 42
[2] [2]Bartels A, Dekorsy T, Kurz H 1999 Opt. Lett. 24 996
[3] [3]Foggi P, Bussotti L, Neiuwahl F V R 2001 Int. J. Photoenergy 3 103
[4] [4]Liu Q M, He X, Gan F X, Qian S X 2009 Acta Phys. Sin. 58 1002 (in Chinese) [刘启明、何漩、干福熹、钱世雄 2009 58 1002]
[5] [5]Kowalevicz A M, Sharma V, Ippen E P, Fujimoto J G, Minoshima K 2005 Opt. Lett. 30 964
[6] [6]Osellame R, Chiodo N, Maselli V, Yin A, Zavelani-Rossi M, Cerullo G, Laporta P 2005 Opt. Express 13 612
[7] [7]Yu B H, Dai N L, Wang Y, Li Y H, Ji L L, Zheng Q G, Lu P X 2007 Acta Phys. Sin. 56 5821 (in Chinese)[于本海、戴能利、王英、李玉华、季玲玲、郑启光、陆培祥 2007 56 5821]
[8] [8]Beddard T, Sibbett W, Reid D T, Garduno-Mejia J, Jamasbi N, Mohebi M 1999 Opt. Lett. 24 163
[9] [9]Zhou X, Kapteyn H, Murnane M 2007 Springer. Ser. Chem. Phys. 88 104
[10] ]Brabec Th, Krausz K 2000 Rev. Mod. Phys. 72 545
[11] ]Nejadmalayeri A H, Herman P R, Burghoff J, Will M, Nolte S T?nnermann A 2005 Opt. Lett. 30 964
[12] ]Takeshima N, Narita Y, Tanaka S, Kuroiwa Y, Hirao K 2005 Opt. Lett. 30 352
[13] ]Sanner N, Huot N, Audouard E, Larat C, Laporte P, Huignard J P 2005 Appl. Phys. B80 27
[14] ]Naumov S, Fernandez A, Graf R, Dombi P, Krausz F, Apolonski A 2005 New. J. Phys. 7 216
[15] ]Sennaroglu A, Fujimoto J G 2003 Opt. Express 11 1106
[16] ]Zhao Y Y, Han H N, Teng H, Wei Z Y 2009 Acta Phys. Sin. 58 1709 (in Chinese)[赵研英、韩海年、滕浩、魏志义 2009 58 1709]
[17] ]Kalashnikov V L, Podivilov E, Chernykh A, Naumov S, Fernandez A, Graf R, Apolonski A 2005 New. J. Phys. 7 217
[18] ]Wolf E 2004 Prog. Opt. 46 55
[19] ]Backus S, Durfee III C G, Murnane M M, Kapteyn H C 1998 Rev. Sci. Instrum. 69 1207
[20] ]Fork R L, Martinez O E, Gordon J P 1984 Opt. Lett. 9 150
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