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We study the properties of optomechanically induced transparency and normal mode splitting in an optical parametric amplifier (OPA) cavity. We find that the value of phase of the field driving the OPA and the nonlinear gain of the OPA will evidently affect the width of the optomechanically induced transparency window and the property of the normal mode splitting. In particular, when the coupling field works at the mechanical red sideband, narrower transparency window than the case of empty cavity (no OPA) can be realized by adjusting the value of phase of the field driving the OPA and the nonlinear gain of the OPA, accompanied by the steep dispersion curve. These results may be applied to the realization of fast/slow light, and light storage in optomechanical system.
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Keywords:
- optomechanics /
- optomechanically induced transparency /
- normal mode splitting /
- optical parametric amplifier
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[67] -
[1] Kippenberg T J, Vahala K J 2008 Science 321 1172
[2] [3] Marquardt F, Girvin S M 2009 Physics 2 40
[4] Verlot P, Tavernarakis A, Briant T, Cohadon P F, Heidmann A 2010 Phys. Rev. Lett. 104 133602
[5] [6] Mahajan S, Kumar T, Bhattacherjee A B, ManMohan 2013 Phys. Rev. A 87 013621
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[10] [11] Kippenberg T J, Vahala K J 2007 Opt. Express 15 17172
[12] Jiang X S, Lin Q, Rosenberg J, Vahala K, Painter O 2009 Opt. Express 17 20911
[13] [14] Ma R, Schliesser A, Del'Haye P, Dabirian A, Anetsberger G, Kippenberg T J 2007 Opt. Lett. 32 2200
[15] [16] Eichenfield M, Camacho R, Chan J, Vahala K J, Prainter O 2009 Nature 459 550
[17] [18] Eichenfield M, Chan J, Camacho R, Vahala K J, Prainter O 2009 Nature 462 78
[19] [20] [21] Brennecke F, Ritter S, Donner T, Esslinger T 2008 Science 322 235
[22] L X Y, Zhang W M, Ashhab S, Wu Y, Nori F 2013 Sci. Reports 3 2943
[23] [24] [25] Liu Y C, Xiao Y F, Chen Y L, Yu X C, Gong Q H 2013 Phys. Rev. Lett. 111 083601
[26] [27] Zhou L, Cheng J, Han Y, Zhang W P 2013 Phys. Rev. A 88 063854
[28] [29] Vitali D, Gigan S, Ferreira A, Bhm H R, Tombesi P, Guerreiro A, Vedral V, Zeilinger A, Aspelmeyer M 2007 Phys. Rev. Lett. 98 030405
[30] Barzanjeh S, Vitali D, Tombesi P, Milburn G J 2011 Phys. Rev. A 84 042342
[31] [32] Wang Y D, Clerk A A 2013 Phys. Rev. Lett. 110 253601
[33] [34] Mi X W, Bai J X, Li D J 2012 Chin. Phys. B 21 030303
[35] [36] [37] Li Y, Wu L A, Wang Z D 2011 Phys. Rev. A 83 043804
[38] Deng Z J, Li Y, Gao M, Wu C W 2012 Phys. Rev. A 85 025804
[39] [40] [41] Dantan A, Genes C, Vitali D, Pinard M 2008 Phys. Rev. A 77 011804(R)
[42] Liu Y C, Wen H Y, Wei W C, Xiao Y F 2013 Chin. Phys. B 22 114213
[43] [44] Huang S M, Agarwal G S 2009 Phys. Rev. A 79 013821
[45] [46] [47] Agarwal G S, Huang S M 2010 Phys. Rev. A 81 041803
[48] [49] Huang S M, Agarwal G S 2010 Phys. Rev. A 81 033830
[50] Shu J 2011 Chin. Phys. Lett. 28 104203
[51] [52] [53] Chen H J, Mi X W 2011 Acta Phys. Sin. 60 124206 (in Chinese) [陈华俊, 米贤武 2011 物理学报 60 124206]
[54] Han Y, Cheng J, Zhou L 2011 J. Phys. B 44 165505
[55] [56] [57] Zhang J Q, Li Y, Feng M, Xu Y 2012 Phys. Rev. A 86 053806
[58] Kronwald A, Marquardt F 2013 Phys. Rev. Lett. 111 133601
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[62] [63] Fiore V, Dong C H, Kuzyk M C, Wang H L 2013 Phys. Rev. A 87 023812
[64] [65] Weis S, Riviere R, Deleglise S, Gavartin E, Arcizet O, Schliesser A, Kippenberg T J 2010 Science 330 1520
[66] Grblacher S, Hammerer K, Vanner M, Aspelmeyer M 2009 Nature 460 724
[67] -
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