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Two-mode entangled state is an important quantum resource for quantum information. In this paper, the amplification of a single mode of two-mode entangled state (single-mode amplification scheme) and two modes of two-mode entangled state (two-mode amplification scheme) are theoretically proposed. Here, the optical beam splitter model is used to simulate the vacuum noise introduced by the loss in the optical transmission process. By utilizing the positivity under partial transpose criterion, we analyze the effect of the gain of the four-wave mixing process on the entanglement degree of the initial two-mode entangled state in two different amplification schemes. In these two schemes, we set the gain of the initial two-mode entangled state generation process to be 1.5, 2.5 and 50.0 respectively, and then change the gain of the amplification process in a certain range. We also set the transmission efficiency of the amplified beams for each of the two schemes to be a definite value. The results show that the entanglement of the initial two-mode entangled state decreases with the gain increasing under the condition of specific transmission loss in two schemes. When the gain does not exceed a certain value, the entanglement of the initial two-mode entangled state can be maintained. Then, with the increase of the gain, the entanglement of the initial two-mode entangled state will disappear. Moreover, the entanglement of the initial two-mode entangled state of the two-mode amplification scheme disappears faster than that of the single-mode amplification scheme. Our theoretical results pave the way for the experimental realization of the amplification of two-mode entangled state based on four-wave mixing process.
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Keywords:
- four-wave mixing /
- quantum entanglement /
- two-mode entangled state /
- optical parametric amplifier
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[19] McCormick C F, Marino A M, Boyer V, Lett P D 2008 Phys. Rev. A 78 043816Google Scholar
[20] MacRae A, Brannan T, Achal R, Lvovsky A I 2012 Phys. Rev. Lett. 109 033601Google Scholar
[21] Pooser R C, Lawrie B 2015 Optica 2 393Google Scholar
[22] Marino A M, Trejo N V C, Lett P D 2012 Phys. Rev. A 86 023844Google Scholar
[23] Li T, Anderson B E, Horrom T, Jones K M, Lett P D 2016 Opt. Express 24 19871Google Scholar
[24] Marino A M, Pooser R C, Boyer V, Lett P D 2009 Nature 457 859Google Scholar
[25] Fan W J, Lawrie B J, Pooser R C 2015 Phys. Rev. A 92 053812Google Scholar
[26] Li Z P, Wang X L, Li C Y, Zhang Y F, Wen F, Ahmed I, Zhang Y P 2016 Laser Phys. Lett. 13 025402Google Scholar
[27] Abdisa G, Ahmed I, Wang X X, Liu Z C, Wang H X, Zhang Y P 2016 Phys. Rev. A 94 023849Google Scholar
[28] Li C B, Jiang Z H, Zhang Y Q, Zhang Z Y, Wen F, Chen H X, Zhang Y P, Xiao M 2017 Phys. Rev. Appl. 7 014023Google Scholar
[29] Li C B, Li W, Zhang D, Zhang Z Y, Gu B L, Li K K, Zhang Y P 2019 Laser Phys. Lett. 17 015401Google Scholar
[30] Pooser R C, Marino A M, Boyer V, Jones K M, Lett P D 2009 Phys. Rev. Lett. 103 010501Google Scholar
[31] Werner R F, Wolf M M 2001 Phys. Rev. Lett. 86 3658Google Scholar
[32] Simon R 2000 Phys. Rev. Lett. 84 2726Google Scholar
[33] Jasperse M, Turner L D, Scholten R E 2011 Opt. Express 19 3765Google Scholar
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[1] Horodecki R, Horodecki P, Horodecki M, Horodecki K 2009 Rev. Mod. Phys. 81 865Google Scholar
[2] Braunstein S L, Look P van 2005 Rev. Mod. Phys. 77 513Google Scholar
[3] Weedbrook C, Pirandola S, García-Patrón R, Cerf N J, Ralph T C, Shapiro J H, Lloyd S 2012 Rev. Mod. Phys. 84 621Google Scholar
[4] Ekert A K 1991 Phys. Rev. Lett. 67 661Google Scholar
[5] Ralph T C 1999 Phys. Rev. A 61 010303Google Scholar
[6] Naik D S, Peterson C G, White A G, Berglund A J, Kwiat P G 2000 Phys. Rev. Lett. 84 4733Google Scholar
[7] Bennett C H, Wiesner S J 1992 Phys. Rev. Lett. 69 2881Google Scholar
[8] Zhang J, Peng K C 2000 Phys. Rev. A 62 064302Google Scholar
[9] Heaney L, Vedral V 2009 Phys. Rev. Lett. 103 200502Google Scholar
[10] Ou Z Y, Pereira S F, Kimble H J, Peng K C 1992 Phys. Rev. Lett. 68 3663Google Scholar
[11] Bouwmeester D, Pan J W, Mattle K, Eibl M, Weinfurter H, Zeilinger A 1997 Nature 390 575Google Scholar
[12] Furusawa A, Sørensen J L, Braunstein S L, Fuchs C A, Kimble H J, Polzik E S 1998 Science 282 706Google Scholar
[13] Li X Y, Pan Q, Jing J T, Zhang J, Xie C D, Peng K C 2002 Phys. Rev. Lett. 88 047904Google Scholar
[14] McCormick C F, Boyer V, Arimondo E, Lett P D 2007 Opt. Lett. 32 178Google Scholar
[15] Boyer V, Marino A M, Pooser R C, Lett P D 2008 Science 321 544Google Scholar
[16] Boyer V, Marino A M, Lett P D 2008 Phys. Rev. Lett. 100 143601Google Scholar
[17] Kumar P, Kolobov M I 1994 Opt. Commun. 104 374Google Scholar
[18] Qin Z Z, Jing J T, Zhou J, Liu C J, Pooser R C, Zhou Z F, Zhang W P 2012 Opt. Lett. 37 3141Google Scholar
[19] McCormick C F, Marino A M, Boyer V, Lett P D 2008 Phys. Rev. A 78 043816Google Scholar
[20] MacRae A, Brannan T, Achal R, Lvovsky A I 2012 Phys. Rev. Lett. 109 033601Google Scholar
[21] Pooser R C, Lawrie B 2015 Optica 2 393Google Scholar
[22] Marino A M, Trejo N V C, Lett P D 2012 Phys. Rev. A 86 023844Google Scholar
[23] Li T, Anderson B E, Horrom T, Jones K M, Lett P D 2016 Opt. Express 24 19871Google Scholar
[24] Marino A M, Pooser R C, Boyer V, Lett P D 2009 Nature 457 859Google Scholar
[25] Fan W J, Lawrie B J, Pooser R C 2015 Phys. Rev. A 92 053812Google Scholar
[26] Li Z P, Wang X L, Li C Y, Zhang Y F, Wen F, Ahmed I, Zhang Y P 2016 Laser Phys. Lett. 13 025402Google Scholar
[27] Abdisa G, Ahmed I, Wang X X, Liu Z C, Wang H X, Zhang Y P 2016 Phys. Rev. A 94 023849Google Scholar
[28] Li C B, Jiang Z H, Zhang Y Q, Zhang Z Y, Wen F, Chen H X, Zhang Y P, Xiao M 2017 Phys. Rev. Appl. 7 014023Google Scholar
[29] Li C B, Li W, Zhang D, Zhang Z Y, Gu B L, Li K K, Zhang Y P 2019 Laser Phys. Lett. 17 015401Google Scholar
[30] Pooser R C, Marino A M, Boyer V, Jones K M, Lett P D 2009 Phys. Rev. Lett. 103 010501Google Scholar
[31] Werner R F, Wolf M M 2001 Phys. Rev. Lett. 86 3658Google Scholar
[32] Simon R 2000 Phys. Rev. Lett. 84 2726Google Scholar
[33] Jasperse M, Turner L D, Scholten R E 2011 Opt. Express 19 3765Google Scholar
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