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SPECIAL TOPIC — Celebrating the 100th Anniversary of Physics Discipline of Northwest University
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SPECIAL TOPIC—Celebrating the 100th Anniversary of Physics Discipline of Northwest University |
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Absorption spectra and enhanced Kerr nonlinearity in a four-level system |
Hao-Jie Huangfu(皇甫浩杰)1, Ying-Jie Du(杜英杰)1,2,†, and Ai-Hua Gao(高爱华)1 |
1 School of Physics, Northwest University, Xi'an 710069, China; 2 Collaborative Innovation Center of Extreme Optics, Shanxi University, Taiyuan 030006, China |
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Abstract In a coherent system, enhanced nonlinearity can be reached via far-detuned coupling fields in the presence of Autler-Townes splitting. We explore the absorption spectra and the Kerr nonlinearity of the coherent system via the interaction between a four-level atomic system and triple fields. We obtain the absorption spectra with double, triple and even quadruple peaks which depend on both the magnitude and the difference of the coupling fields. The Kerr nonlinearity always remains reversely correlated with the absorption spectra. We find that the large coupling detunings can lead to a significant growth of the Kerr nonlinearity and the degenerate four-wave mixing. Both the Kerr nonlinearity and the four-wave mixing can be managed by adjusting the detunings of the coupling fields.
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Received: 19 June 2023
Revised: 23 October 2023
Accepted manuscript online: 24 October 2023
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PACS:
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42.50.Gy
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(Effects of atomic coherence on propagation, absorption, and Amplification of light; electromagnetically induced transparency and Absorption)
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32.80.Qk
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(Coherent control of atomic interactions with photons)
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42.65.-k
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(Nonlinear optics)
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Fund: Project supported by the Open Subject of the State Key Laboratory of Quantum Optics and Quantum Optics Devices (Grant No. KF202209). |
Corresponding Authors:
Ying-Jie Du
E-mail: yingjied@nwu.edu.cn
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Cite this article:
Hao-Jie Huangfu(皇甫浩杰), Ying-Jie Du(杜英杰), and Ai-Hua Gao(高爱华) Absorption spectra and enhanced Kerr nonlinearity in a four-level system 2023 Chin. Phys. B 32 114214
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[1] Zibrov A S, Lukin M D and Scully M O 1999 Phys. Rev. Lett. 83 4049 [2] Liang H, Niu Y, Deng L and Gong S 2017 Phys. Lett. A 381 3978 [3] Eckhardt G, Hellwarth R W, McClung F J, Schwarz S E, Weiner D and Woodbury E J 1962 Phys. Rev. Lett. 9 455 [4] Sinclair J, Angulo D, Lupu-Gladstein N, Bonsma-Fisher K and Steinberg A M 2019 Phys. Rev. Res. 1 033193 [5] Schmid D, Marshall K and James D F V 2017 J. Mod. Opt. 64 2306 [6] Nemoto K and Munro W J 2004 Phys. Rev. Lett. 93 250502 [7] Wan R G, Kou J, Jiang L, Jiang Y and Gao J Y 2011 Phys. Rev. A 83 033824 [8] Dey T N and Agarwal G S 2007 Phys. Rev. A 76 015802 [9] Wu Y and Yang X 2007 Phys. Rev. B 76 054425 [10] Harris S E 1997 Phys. Today 50 36 [11] Braje D A, Balić V, Yin G Y and Harris S E 2003 Phys. Rev. A 68 041801 [12] Cahuzac P and Vetter R 1976 Phys. Rev. A 14 270 [13] Autler S H and Townes C H 1955 Phys. Rev. 100 703 [14] Lezama A, Barreiro S and Akulshin A M 1999 Phys. Rev. A 59 4732 [15] Zhao J M, Zhao Y T, Huang T, Xiao L T and Jia S T 2005 Chin. Phys. 14 725 [16] Zhao S M and Zhuang P 2014 Chin. Phys. B 23 054203 [17] Zhang Y, Qu S and Gu S 2012 Opt. Express 20 6400 [18] Distante E, Padrón-Brito A, Cristiani M, Paredes-Barato D and de Riedmatten H 2016 Phys. Rev. Lett. 117 113001 [19] Harris S E, Field J E and Imamoğlu A 1990 Phys. Rev. Lett. 64 1107 [20] Wang H, Goorskey D and Xiao M 2002 Opt. Lett. 27 1354 [21] Michinel H, Paz-Alonso M J and Pérez-García V M 2006 Phys. Rev. Lett. 96 023903 [22] Carvalho S A and de Araujo L E E 2011 Phys. Rev. A 83 053825 [23] Wang H, Goorskey D and Xiao M 2001 Phys. Rev. Lett. 87 073601 [24] Gu Y, Sun Q and Gong Q 2003 Phys. Rev. A 67 063809 [25] Raczyński A, Rzepecka M, Zaremba J and Zielińska-Kaniasty S 2006 Opt. Commun. 260 73 [26] Li S, Yang X, Cao X, Zhang C, Xie C and Wang H 2008 Phys. Rev. Lett. 101 073602 [27] Asadpour S H, Hamedi H R and Sahrai M 2012 J. Lumin. 132 2188 [28] Ziemkiewicz D and Zielińska-Raczyńska S 2020 Entropy 22 160 [29] Alotaibi H M M and Sanders B C 2016 Phys. Rev. A 94 053832 [30] Kang H and Zhu Y 2003 Phys. Rev. Lett. 91 093601 [31] Sheng J, Yang X, Wu H and Xiao M 2011 Phys. Rev. A 84 053820 [32] Jia F D, Liu X B, Mei J, Yu Y H, Zhang H Y, Lin Z Q, Dong H Y, Zhang J, Xie F and Zhong Z P 2021 Phys. Rev. A 103 063113 [33] Pooser R C, Marino A M, Boyer V, Jones K M and Lett P D 2009 Opt. Express 17 16722 [34] Glorieux Q, Dubessy R, Guibal S, Guidoni L, Likforman J P, Coudreau T and Arimondo E 2010 Phys. Rev. A 82 033819 [35] Niu Y and Gong S 2006 Phys. Rev. A 73 053811 [36] Boyd R W, Raymer M G, Narum P and Harter D J 1981 Phys. Rev. A 24 411 [37] Taichenachev A V, Tumaikin A M and Yudin V I 1999 Phys. Rev. A 61 011802 |
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