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The propagation of broadband pulse in a medium with electromagnetically induced transparency (EIT) was studied. The results show that if the carrier frequency of pulse is exactly tuned to the center of the transparency window, and the pulse spectrum is broader than transparency window, the pulse is temporally broadened and the delay effect is significant. If the carrier frequency of pulse the is exactly tuned to the region of absorption, and the pulse spectrum is wide with respect to the width of absorption line, the pulse begins to distort after a certain distance and is split into two parts at last. The peak value depends not only on the frequency and intensity of the coupling field, but also on the length of the sample. Under appropriate conditions, strong and time domain narrowed pulse can be obtained in the output light.
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Keywords:
- electromagnetically induced transparency(EIT) /
- shape distortion /
- time delay /
- coherent addition
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[2] Giacobino E 2008 Phys. Rev. Lett. 101 133601
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[25] Novikova I, Phillips N B, Gorshkov A V 2008 Phys. Rev. A 78 021802
[26] Bashkansky M, Beadie G, Dutton Z, Fatemi F K, Reintjes J, Steiner M 2005 Phys. Rev. A 72 033819
[27] Sun Q, Rostovtsev Y V, Dowling J P, Scully M O, Zubairy M S 2005 Phys. Rev. A 72 031802
[28] Yavuz D D 2007 Phys. Rev. A 75 031801
[29] Scully M O, Zubairy M S 1997 Quantum Optics(Cambridge: Cambridge University Press)p225
[30] Fleischhauer M, Imamo lu A, Marangos J P 2005 Rev. Mod. Phys. 77 633
[31] Mishina O S, Larionov N V, Sheremet A S, Sokolov I M, Kupriyanov D V 2008 Phys. Rev. A 78 042313
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[1] Harris S E, Field J E and Imamo lu A 1990 Phys. Rev. Lett. 64 1107
[2] Giacobino E 2008 Phys. Rev. Lett. 101 133601
[3] Boller K J, Imamo lu A, Harris S E 1991 Phys. Rev. Lett. 66 2593
[4] Harris S E 1997 Phys. Today 50 36
[5] Hau L V, Harris S E, Dutton Z, Behroozi C H 1999 Nature 397 594
[6] Wang B, Li S J, Chang H, Wu H B, Xie C D, Wang H 2005 Acta Phys. Sin. 54 4136 (in Chinese)[王 波、李淑静、常 宏、武海斌、谢常德、王 海 2005 54 4136]
[7] Liu C, Dutton Z, Behroozi C H, Hau L V 2001 Nature 409 490
[8] Phillips D F, Fleischhauer A, Mair A, Walsworth R L 2001 Phys. Rev. Lett. 86 783
[9] Eisaman M D, André A, Massou F, Fleischhauer M, Zibrov A S, Lukin M D 2005 Nature 438 837
[10] Chanelière T, Matsukevich D N, Jenkins S D, Lan S Y, Kennedy T A B, Kuzmich A 2005 Nature 438 833
[11] Huang S G, Gu W Y, Ma H Q 2004 Acta Phys. Sin. 53 4211 (in Chinese)[黄善国、顾畹仪、马海强 2004 53 4211]
[12] Wang L R, Zhao Y T, Ma J, Zhao J M, Xiao L T, Jia S T 2006 Chin. Phys. 15 365
[13] Wang F Y, Shi B S, Lu X S, Guo G C 2008 Chin. Phys. B 17 1798
[14] Gorshkov A V, André A, Fleischhauer M, Srensen A S, Lukin M D 2007 Phys. Rev. Lett. 98 123601
[15] Gorshkov A V, André A, Lukin M D, Srensen A S 2007 Phys. Rev. A 76 033805
[16] Choi K S, Deng H, Laurat J, Kimble H J 2008 Nature 452 67
[17] Cviklinski J, Ortalo J, Laurat J, Bramati A, Pinard M,
[18] Yang L J, Zhang L S, Li X L, Li X W, Guo Q L, Han L, Fu G S 2006 Acta Phys. Sin. 55 5206(in Chinese)[杨丽君、张连水、李晓莉、李晓苇、郭庆林、韩 理、傅广生 2006 55 5206]
[19] Zhang L S, Li X L, Wang J, Yang L J, Feng X M, Li X W, Fu G S 2008 Acta Phys. Sin. 57 4921 (in Chinese)[张连水、李晓莉、王 健、杨丽君、冯晓敏、李晓苇、傅广生 2008 57 4921]
[20] Payne M G, Deng L 2001 Phys. Rev. A 64 031802
[21] Du D, Hu X M 2006 Acta Phys. Sin. 55 5232 (in Chinese) [杜 丹、胡响明 2006 55 5232]
[22] Chen Y F, Kao Y M, Lin W H, Yu T A 2006 Phys. Rev. A 74 063807
[23] Kiffner M, Dey T N 2009 Phys. Rev. A 79 023829
[24] Patnaik A K, Kien F L, Hakuta K 2004 Phys. Rev. A 69 035803
[25] Novikova I, Phillips N B, Gorshkov A V 2008 Phys. Rev. A 78 021802
[26] Bashkansky M, Beadie G, Dutton Z, Fatemi F K, Reintjes J, Steiner M 2005 Phys. Rev. A 72 033819
[27] Sun Q, Rostovtsev Y V, Dowling J P, Scully M O, Zubairy M S 2005 Phys. Rev. A 72 031802
[28] Yavuz D D 2007 Phys. Rev. A 75 031801
[29] Scully M O, Zubairy M S 1997 Quantum Optics(Cambridge: Cambridge University Press)p225
[30] Fleischhauer M, Imamo lu A, Marangos J P 2005 Rev. Mod. Phys. 77 633
[31] Mishina O S, Larionov N V, Sheremet A S, Sokolov I M, Kupriyanov D V 2008 Phys. Rev. A 78 042313
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