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Michelson interferometer can be applied to not only the building block of the fundamental research of physics, but also the precise measurement, such as the direct observation of gravity wave signal. Therefore, high performance Michelson interferometer is the key step towards the implementation of direct observation of weak gravity wave signal. Recently, the vacuum noise was reduced by injecting squeezed vacuum into the unused port of Michelson interferomter, and the phase signal optical field in Mach-Zender interferometer is amplified based on the four-wave mixing in hot Rubidium atom. Here we study high sensitivity quantum Michelson interferometer. In the Michelson interferometer, the linear optical beam splitter is replaced by a non-degenerated optical parametric amplifier to realize the splitting and combining of optical fields, and the squeezed vacuum is also injected into the unused port of interferomter, so that the high signal-to-noise ratio and high sensitivity of phase measurement can be realized. Due to the inevitable optical losses, the losses inside and outside the Michelson interferometer are considered in our theoretical model. We investigate the influences of the losses inside and outside the Michelson interferometer on the sensitivity of phase measurement. By theoretical calculation, we analyze the dependence of sensitivity of phase measurement on system parameters, such as intensity of optical fields for phase sensing, gain factor of non-degenerated optical parametric amplifier, the losses inside and outside the Michelson interferometer, and the squeezing parameter of input squeezed vacuum, and thus the condition of high sensitivity nonlinear Michelson interferometer can be obtained. In a broad system parametric range, the quantum Michaleson interferometer can surpass standard quantum limit, and the nonlinear Michaleson interferometer with squeezed state injection can provide the optimal sensitivity for phase measurement. The nonlinear Michelson interferometer with squeezed state is suitable for weak signal measurement. While the gain factor of non-degenerated optical parametric amplifier is large enough, the nonlinear Michelson interferometer without injecting the squeezed vacuum can still reach the optimal sensitivity, which reduces the use of quantum resources. When the phase sensing optical field is strong, the linear Michelson interferometer with injecting the squeezed vacuum can also reach the optimal sensitivity, and the sensitivity is robust for both losses inside and outside the interferometer. All the kinds of interferometers are more sensitive to the loss inside the interferometer than outside the interferometer, and the sensitivity of phase measurement can be improved by reducing the loss inside the interferometer. Our result provides direct reference of experimental implementation of high performance interferometer for high precision quantum metrology.
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Keywords:
- Michelson interferometer /
- squeezed state /
- non-degenerated optical parametric amplifier /
- sensitivity
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[39] Ou Z Y 1997 Phys. Rev. A 55 2598
[40] Tian X D, Liu Y M, Cui C L, Wu J H 2015 Phys. Rev. A 92 063411
[41] Ding D S, Zhang W, Zhou Z Y, Shi S, Shi B S, Guo G C 2015 Nature Photon. 9 332
[42] Xin J, Jian Q, Jing J T 2017 Opt. Lett. 42 366
[43] Jing J T, Liu C J, Zhou Z F, Ou Z Y, Zhang W P 2011 Appl. Phys. Lett. 99 011110
[44] Hudelist F, Kong J, Liu C J, Jing J T, Zhou Z F, Ou Z Y, Zhang W P 2014 Nature Commun. 5 3049
[45] Xin J, Liu J M, Jing J T 2017 Opt. Express 25 1350
[46] Xin J, Wang H L, Jing J T 2016 Appl. Phys. Lett. 109 051107
[47] Wang H L, Marino A M, Jing J T 2015 Appl. Phys. Lett. 107 121106
[48] Kong J, Jing J T, Wang H L, Hudelist F, Liu C J, Zhang W P 2013 Appl. Phys. Lett. 102 011130
[49] Liu S S, Jin J T 2017 Opt. Express 25 15854
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[1] Einstein A 1916 Ann. Phys. 49 769
[2] Sathyaprakash B S, Schutz B F 2009 Living Rev. Relativ. 2 1
[3] Hinderer T J, Lackey B D, Lang R N, Read J S 2010 Phys. Rev. D 81 123016
[4] Vines J, Flanagan E E, Hinderer T J 2011 Phys. Rev. D 83 084051
[5] Bauswein A, Janka H T 2012 Phys. Rev. Lett. 108 011101
[6] Abramovici A, Althouse W E, Drever R W P, Grsel Y, Kawamura S, Raab F J, Shoemaker D, Sievers L, Spero R E, Thorne K S, Vogt R E, Weiss R, Whitcomb S E, Zucker M E 1992 Science 256 5055
[7] Aasi J, Abbott B P, Abbott R, et al. 2015 Class. Quant. Grav. 32 074001
[8] Grote H 2010 Class. Quant. Grav. 27 084003
[9] Acernese F, Agathos M, Agatsuma K, et al. 2015 Class. Quant. Grav. 32 024001
[10] Arai K, Takahashi R, Tastumi D, et al. 2009 Class. Quant. Grav. 26 204020
[11] Barriga P, Blair G D, Coward D, et al. 2010 Class. Quant. Grav. 27 084005
[12] Punturo M, Abernathy M, Acernese F, et al. 2010 Class. Quant. Grav. 27 084007
[13] Abbott B P, Abbott R, Abbott T D, et al. 2016 Phys. Rev. Lett. 116 061102
[14] Abbott B P, Abbott R, Abbott T D, et al. 2017 Phys. Rev. Lett. 119 161101
[15] Hou Z B, Zhu H J, Xiang G Y, Li C F, Guo G C 2016 npj Quantum Information 2 16001
[16] Liu F, Zhou Y Y, Yu J, Guo J L, Wu Y, Xiao S X, Wei D, Zhang Y, Jia X J, Xiao M 2017 Appl. Phys. Lett. 110 021106
[17] Walls D F 1983 Nature 306 141
[18] Zhang M Z 2015 Quantum Optics (Beijing: Science Press) pp72-75 (in Chinese) 张智明 2015 量子光学 (北京:科学出版社) 第7275页
[19] Caves C M 1980 Phys. Rev. Lett. 45 75
[20] Caves C M 1981 Phys. Rev. D 23 1693
[21] Sun H X, Liu K, Zhang J X, Gao J R 2015 Acta Phys. Sin. 64 234210 (in Chinese) [孙恒信, 刘奎, 张俊香, 郜江瑞 2015 物理学报 64 234210]
[22] Slusher R E, Hollberg L W, Yurke B, Mertz J C, Valley J F 1985 Phys. Rev. Lett. 55 2409
[23] Wu L A, Kimble H J, Hall J L, Wu H F 1986 Phys. Rev. Lett. 57 2520
[24] Henning V, Moritz M, Karsten D, Schnabel R 2016 Phys. Rev. Lett. 117 110801
[25] Wan Z J, Feng J X, Sun Z N, Yao L T, Zhang K S 2014 Acta Sin. Quantum Opt. 20 271 (in Chinese) [万振菊, 冯晋霞, 孙志妮, 要立婷, 张宽收 2014 量子光学学报 20 271]
[26] Sun Z N, Feng J X, Wan Z J, Zhang K S 2016 Acta Phys. Sin. 65 044203 (in Chinese) [孙志妮, 冯晋霞, 万振菊, 张宽收 2016 物理学报 65 044203]
[27] McKenzie K, Grosse N, Bowen W P, Whitcomb S E, Gray M B, McClelland D E, Lam P K 2004 Phys. Rev. Lett. 93 161105
[28] Vahlbruch H, Chelkowski S, Hage B, Franzen A, Danzmann K, Schnabel R 2006 Phys. Rev. Lett. 97 011101
[29] Yan Z H, Sun H X, Cai C X, Ma L, Liu K, Gao J R 2017 Acta Phys. Sin. 66 114205 (in Chinese) [闫子华, 孙恒信, 蔡春晓, 马龙, 刘奎, 郜江瑞 2017 物理学报 66 114205]
[30] Goda K, Miyakawa O, Mikhailov E E, Saraf S, Adhikari R, McKenzie K, Ward R, Vass S, Weinstein A J, Mavalvala N 2008 Nature Phys. 4 472
[31] Schnabel R, Mavalvala N, McClelland D E, Lam P K 2010 Nature Commun. 1 121
[32] Abadie J, Abbott B P, Abbott R, et al. 2011 Nature Phys. 7 962
[33] Aasi J, Abadie J, Zweizi J, et al. 2013 Nature Photon. 7 613
[34] Liu Y C, Xiao Y F, Chen Y L, Yu X C, Gong Q H 2013 Phys. Rev. Lett. 111 083601
[35] Wang X L, Chen L K, Li W, Huang H L, Liu C, Chen C, Luo Y H, Su Z E, Wu D, Li Z D, Lu H, Hu Y, Jiang X, Peng C Z, Li L, Liu N L, Chen Y A, Lu C Y, Pan J W 2016 Phys. Rev. Lett. 117 210502
[36] Deng X W, Xiang Y, Tian C X, Adesso G, He Q Y, Gong Q H, Su X L, Xie C D, Peng K C 2017 Phys. Rev. Lett. 118 230501
[37] Yurke B, McCall S L, Klauder J R 1986 Phys. Rev. A 33 4033
[38] Plick W N, Dowling J P, Agarwal 2010 New J. Phys. 12 083014
[39] Ou Z Y 1997 Phys. Rev. A 55 2598
[40] Tian X D, Liu Y M, Cui C L, Wu J H 2015 Phys. Rev. A 92 063411
[41] Ding D S, Zhang W, Zhou Z Y, Shi S, Shi B S, Guo G C 2015 Nature Photon. 9 332
[42] Xin J, Jian Q, Jing J T 2017 Opt. Lett. 42 366
[43] Jing J T, Liu C J, Zhou Z F, Ou Z Y, Zhang W P 2011 Appl. Phys. Lett. 99 011110
[44] Hudelist F, Kong J, Liu C J, Jing J T, Zhou Z F, Ou Z Y, Zhang W P 2014 Nature Commun. 5 3049
[45] Xin J, Liu J M, Jing J T 2017 Opt. Express 25 1350
[46] Xin J, Wang H L, Jing J T 2016 Appl. Phys. Lett. 109 051107
[47] Wang H L, Marino A M, Jing J T 2015 Appl. Phys. Lett. 107 121106
[48] Kong J, Jing J T, Wang H L, Hudelist F, Liu C J, Zhang W P 2013 Appl. Phys. Lett. 102 011130
[49] Liu S S, Jin J T 2017 Opt. Express 25 15854
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