Introduction

Quantum correlation shared between multiple quantum correlated beams is important for fundamental quantum mechanics1 and significant applications in quantum information technologies2. The relationship between the quantum correlation shared by the multiple quantum correlated beams and the pairwise correlations (PCs) of the multiple beams remains an open question. For example, ref. 3 discusses the trade-off between A’s correlation with B and its correlation with C in a three qubits (A, B and C) system; ref. 4 reviews the properties of the PCs in many-body systems; refs 5, 6 and ref. 7 give the classification of three-qubit correlation and four-qubit correlation respectively which both involve the consideration of PCs. ref. 8 have formalized and extended the operational classification and quantification of multipartite correlated states related to the PCs. Therefore, the characterization of PCs existed in the multiple quantum correlated beams is worth investigating for both the classification and application of quantum states.

Four-wave mixing (FWM) process in a hot rubidium (Rb) vapor9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24 has several advantages of practical implementations, e.g., no need of cavity due to strong nonlinearity of the system, natural spatial separation of the generated non-classical beams, etc. Our group has experimentally demonstrated the generation of strong quantum correlation between the three bright beams from a cascaded FWM process25. Under that experimental condition, there doesn’t exist any quantum correlation between any two of the three beams, i. e., no PC with quantum correlation has been shown in our previous work. Therefore, the dependence of the PCs on the system operating condition of the cascaded FWM processes is very interesting and worth studying. In this letter, based on two different cascaded FWM processes, i. e., asymmetrical cascaded scheme and symmetrical cascaded scheme, we theoretically characterize the performance of the PCs of the multiple quantum correlated beams and analyze their dependences on the system intensity gains Gk (k = 1, 2). The theoretical predictions can give a rough estimation of the obtained experimental results.

Results

Single FWM scheme

Firstly, we give a simple description of the single FWM scheme. FWM is a nonlinear process in which two pump photons can convert to one signal photon and one idler photon, or vice versa. In the cell1 of Fig. 1(a), an intense pump beam and a much weaker signal beam are crossed in the center of the Rb vapor cell with a slight angle. Then the signal beam is amplified as and a new beam called idler beam is generated as on the other side of the pump beam at the same time. The signal beam and idler beam have different frequencies. The input-output relation of the single FWM scheme shown in Fig. 1(a) is given by

Figure 1
figure 1

(a) Asymmetrical cascaded scheme. is coherent input signal, and are vacuum inputs, G1 and G2 are the power gains of cell1 and cell2 respectively. is the output signal beam from the first FWM, , and are the triple output beams. P1 and P2 are the pump beams for the Cell1 and Cell2 respectively. (b) The region plot of Eq. (8), Eq. (9) and Eq. (10). The green region (1, 2) is the region of , the red line (1, 3) is the region of (G2 = 2 − 1/G1), the magenta region (2, 3) is the region of . The black point (2.9, 2.1) is the experimental gain point. The blank region is the region in which , and . In all region, .

where G1 is the power gain of the FWM process. is the vacuum input and is the coherent input. Following the expressions of the creation and annihilation operators, the optical intensities ( (i = 1, 2’)) for the beams and can be given by

where . Then the PC for the two beams and can be quantified by the degree of intensity difference squeezing (DS), i. e., the ratio of the variance of the correlated beams to the variance at the standard quantum limit (SQL)26

here and . Here the superscript and subscript for the represent the kth (k = 1, 2, 3) scheme (we have three schemes throughout the whole discussion, i. e., the single FWM scheme (1), the asymmetrical cascaded scheme (2) and the symmetrical cascaded scheme (3), the ith (i = 1, 2, 3) beam and the jth (j = 2′, 2, 3, 4) beam in the scheme. Var (A) = 〈A2〉 − 〈A2 denotes the variance of A. demonstrates the presence of PC with quantum correlation between the two beams from the FWM process. Since G1 is always larger than 1, the PC with quantum correlation of the two beams can be easily obtained in the experiment. However, the DSs of the single beams and are given by

This corresponds to a linear increase in the noise on both the signal and idler beams as gain is increased. Thus the beams and in the FWM process are both in thermal states.

Asymmetrical cascaded FWM scheme

Secondly, compared to the above mentioned single FWM scheme, here we construct the asymmetrical cascaded scheme in Fig. 1(a). We take the signal beam from the first FWM process (cell1) as the seed for the second FWM process (cell2) in Fig. 1(a)25. , and are three newly-generated beams in the output stage of the cascaded processes. In our previous work25, we have shown the generation of strong quantum correlation between the three bright beams but not the PCs with quantum correlation for any pair of the three beams. Here we will study all the PCs of the triple beams , and in Fig. 1(a) and look for the possibilities for the existence of PCs with quantum correlation. The input-output relation of the asymmetrical cascaded scheme in Fig. 1(a) can be written as

where G1 and G2 are the power gains for the cell1 and cell2 respectively. The optical intensities ( (i = 1, 2 and 3)) for the individual beams , and can be given by

where . Here the second-order vacuum terms are omitted. It should be noted that the DS of the triple beams (, and ) is given by

where G1 and G2 are the power gains for the two FWM processes. Compared with Eq. (3), Eq. (7) means that the cascaded FWM process can enhance the quantum correlation of the system. The symmetrical dependence of the on the gains is shown in Fig. 2(a) and can be enhanced with the increasing of the gains G1 and G2. The quantum correlation shared by the triple beams is present if G1G2 > 1, i. e., G1 > 1 or G2 > 1.

Figure 2
figure 2

The contour plot of (a) ; (b) ; (c) and (d) .

Next we analyze all the possible PCs using the DS criterion. PC between and can be quantified by

Eq. (8) will be reduced to 2G2 − 1 and 1/(2G1 − 1) when we set G1 = 1 and G2 = 1 respectively, corresponding to the cases of Eq. (4) and Eq. (3) respectively. These phenomena can be understood as follows. When we set G1 = 1, the PC between the thermal states and translates into the one between the vacuum state and the thermal state , i. e., . When we set G2 = 1, the PC between the thermal states and translates into the one between the twin beams from the first FWM process, i. e., . The region in which , i. e., there exists quantum correlation between beams and , is shown in green denoted as (1, 2) in Fig. 1(b). The value of G2 on the boundary (see the boundary given by in Fig. 1(b)) of that region reaches its maximal value of 1.33 when G1 = 3 and it decreases when G1 > 3 and will eventually reaches at the value of 1. To clearly see how the depends on the gains G1 and G2, the contour plot of it is shown in Fig. 2(b). The larger G1 and smaller G2 are preferred for achieving . The study of presented above is actually the question of how to preserve the quantum correlation between beams and under the introduction of a second FWM which brings the deterioration effect to the quantum correlation by the quantum amplification of one of the beams (). The results shown in Figs 1(b) and 2(b) actually shows the value of G2 on the boundary below which the quantum correlation can always be preserved as the value of G1 increases. That is to say, in the low gain regime (G1 < 3), the stronger the quantum correlation between beams and is, the more robust to the deterioration effect from the quantum amplification of the second FWM it becomes. More interestingly, in the high gain regime (G1 > 3), the stronger the quantum correlation between beams and is, the more fragile to the deterioration effect from the quantum amplification of the second FWM it becomes.

PC between and can be quantified by

Eq. (9) is equal to 1 when G2 = 2 − 1/G1, meaning that the quantum fluctuation of intensity difference of two thermal states can be equal to the one of two coherent states with equal powers. Except that, is always larger than 1, i. e., there is no quantum correlation between beams and . The region in which (G2 = 2 − 1/G1) is shown as the red line denoted as (1, 3) in Fig. 1(b). The contour plot of is also shown in Fig. 2(c) in which the value of all the region is more than or equal to 1 for any G1, G2 > 1. In this sense, there isn’t any quantum correlation between beams and for any value of G1 and G2 since is always more than or equal to 1.

PC between and can be quantified by

The simplified results, i. e., 1/(2G2 − 1) and 2G1 − 1 for Eq. (10) can be obtained when G1 and G2 are set to equal to 1 respectively, corresponding to the cases of Eq. (3) and Eq. (4) respectively. This is because when we set G1 = 1, the PC between the thermal states and translates into the one between the twin beams from the second FWM process, i. e., . When we set G2 = 1, the PC between the thermal states and translates into the one between the thermal state and the vacuum state , i. e., . The region in which (G1 < G2) is shown in magenta denoted as (2, 3) in Fig. 1(b), meanwhile, the contour plot of is also shown in Fig. 2(d) in which the region of G1 < G2 gives . Therefore, the PC with quantum correlation between beams and will be present for any G1 less than G2. This is not difficult to figure out if one looks at the functional form of Eq. (10). As we all know, in order to generate strong quantum correlation from FWM process, the shot noise limited seed beam, such as coherent state or vacuum state, is always preferred. From this point of view, the analysis presented above actually answers the question of how to produce quantum correlation with the seeding of a thermal state. Figs 1(b) and 2(d) actually gives the answer that the quantum correlation will be produced as long as the FWM gain for producing the quantum correlation is larger than the FWM gain for the thermal state generation. In such region (G1 < G2), the existence of quantum correlation between beams and eliminates the possibility of the one between beams and . In other words, beam can’t be simultaneously quantum correlated with beams and . In this sense, we could call this phenomena as repulsion effect of quantum correlation between the PCs in this cascaded FWM process. It can be explained as follows. The repulsion effect is actually the result of the competition between the correlation mechanism and decorrelation mechanism. As shown in Fig. 1(a), firstly, for the PC between beams and , obviously, cell1 will provide the correlation between them and cell2 will destroy their quantum correlation by adding extra vacuum noise, thus cell1 and cell2 can be viewed as the correlation mechanism provider and decorrelation mechanism provider respectively, thus the larger G1 and smaller G2 are preferred for the PC between beams and . Secondly, for the case of the PC between beams and , cell1 will generate a thermal state which will destroy their quantum correlation by adding extra vacuum noise into the system while the cell2 will make them quantum correlated through the FWM process. In this case, cell1 and cell2 can be viewed as the decorrelation mechanism provider and correlation mechanism provider respectively, thus the smaller G1 and larger G2 are preferred for the PC between beams and . Finally, the complete opposite dependence of the PC between beams and and the PC between beams and on the gains leads to the repulsion effect between the PCs of certain pairs. In the blank region of Fig. 1(b), all the PCs with quantum correlation are absent since , and , however, the quantum correlation between the triple beams is still present.

In order to give a summary of the theoretical predictions of Figs 1(b) and 2. We plot the dependence of (A) ; (B) ; (C) and (D) on the gain G2 when G1 = 2.9 (cell1 gain in the experiment) in Fig. 3. (trace A) can be enhanced with the increasing of G2 which is consistent with Fig. 2(a), the value of (trace B) will be larger than 1 as long as G2 > 1.33 which is consistent with the boundary of in Fig. 1(b), (trace C) will approach the SQL only G2 = 1.66 which is consistent with G2 = 2 − 1/G1 in Fig. 1(b), the value of (trace D) will be smaller than 1 as long as G2 > 2.9 which is consistent with Figs 1(b) and 2(d).

Figure 3: The dependence of (A) ; (B) ; (C) and (D) on the gain G2 when G1 = 2.9 (cell1 gain in the experiment).
figure 3

The black dashed line: SQL.

To verify these theoretical predictions, we apply them to the experimental results. The measured results are shown in Fig. 4, the traces A, B, C and D are the measured DSs between and , and , and and the triple beams respectively, the trace E is the corresponding normalized SQLs for traces A ~ D (See the methods). The experimental results show 10Log() = 7.0 ± 0.2 dB, 10Log() = 5.5 ± 0.1 dB, 10Log() = 1.0 ± 0.2 dB and 10Log() = −6.7 ± 0.4 dB at 1 MHz where the maximal degree of squeezing can be considered as the best choice to reflect the quantum properties of the system because there exist huge classical noise peaks at lower frequencies from the laser, the bandwidth limitation of the photodetector and even the bandwidth limitation of the squeezing generation. As we can see from Fig. 4, the noise power of the three beams increases quickly as the frequency increases. It also increases faster than the one of the two beams. We can understand this results as follows. Although the probe and idler beams in the single FWM scheme are generated almost simultaneously, there are still some time delay between them during their propagation through the cell27. This difference limits the squeezing bandwidth to some extent. This time delay induced squeezing bandwidth becomes narrower in the case of asymmetrical cascaded FWM scheme due to two of the three beams experiencing additional time delay in the second vapor cell. The faster increasing of the noise power of the three beams than the one of the two beams is due to that the number of beams of the three beams related to the time delay is more than the one of the two beams. For the experimental gains G1 ≈ 2.9 and G2 ≈ 2.1, our theoretical predictions give 10Log() = 5.9 dB, 10Log() = 2.2 dB, 10Log() = 1.8 dB and 10Log() = −10.5 dB in which the positive and negative values represent antisqueezing and squeezing respectively. As we can see, although these theoretical predictions do not perfectly agree with the experimental results at 1 MHz, they still give a rough estimation of the relationship between the obtained experimental noise power traces.

Figure 4: Experimentally measured (A) ; (B) ; (C) ; (D) and (E) the corresponding SQLs of the traces A ~ D in the asymmetrical cascaded scheme.
figure 4

The vertical dashed line: 1 MHz.

Symmetrical cascaded FWM scheme

Finally, we construct the following symmetrical cascaded scheme as shown in Fig. 5(a). We take the signal beam from the first FWM process (cell1) as the seed for the second FWM process (cell2) and the idler beam as the seed for the third FWM process (cell3) in Fig. 5(a). , , and are the quadruple newly-generated beams in the output stage of the cascaded processes. We will also study all the PCs of the quadruple beams , , and in Fig. 5(a) and look for the possibilities for existence of the PCs with quantum correlation. The input-output relation of the symmetrical cascaded scheme in Fig. 5(a) can be written as

Figure 5
figure 5

(a) Symmetrical cascaded scheme. is coherent input signal, , and are vacuum inputs, G1 and G2 are the power gains of cell1 and cell2 (cell3) respectively. , , and are the output beams. P1, P2 and P3 are the pump beams for the Cell1, Cell2 and Cell3 respectively. (b) The region plot of Eq. (14), Eq. (15). The green region (1, 2) is the region of , the magenta region ((1, 4), (2, 3)) is the region of and . The black point (2.94, 2.85) is the experimental gain point. The blank region is the region of , , , , and , meaning that there is no PC with quantum correlation for any pair of the quadruple beams. In all region, .

where G1, G2 are the power gains of cell1, cell2 (cell3) respectively. Here we assume that the two FWM processes in the cell2 and cell3 have the same power gains for simplicity. The optical intensities ( (i = 1, 2, 3 and 4)) for the individual beams , , and can be given by

where . Here the second-order vacuum terms are omitted. It should be noted that the DS of the quadruple beams (, , and ) is given by

compared with Eq. (7), this cascaded scheme has also enhanced the quantum correlation of the system. The symmetrical dependence of the on the gains is shown in Fig. 6(a) and it can be enhanced with the increasing of the gains G1 and G2, similar to the case of . The quantum correlation shared by the quadruple beams is present if (2G1 − 1)(2G2 − 1) > 1, i. e., G1 > 1 or G2 > 1. Next let us analyze all the possible PCs in this scheme and the triple correlations can also be obtained from the expressions of the PCs in the asymmetrical cascaded FWM scheme, for example, the DS for the triple beams (, and ) can be expressed as . Therefore, we only focus on the PCs. PC between and can be quantified by

Figure 6
figure 6

The contour plot (a) ; (b) and (c) and .

The region in which is shown in green denoted as (1, 2) in Fig. 5(b), the contour plot of the dependence of on the gains G1 and G2 is shown in Fig. 6(b). With the increasing of G1, the value of G2 on the boundary always increases and eventually saturates at the value of 2 (see the boundary given by G2 = 2 − 1/G1 in Fig. 5(b)). This is different from the asymmetrical scheme discussed above, where the value of G2 on the boundary finally reaches 1. This is because here beams and from the first FWM process experience the same amount of amplification in the second and third FWM processes, which leads to their good noise balance, thus the performance of the PC with quantum correlation between beams and is not as sensitive to the G2 as the one in the asymmetrical cascaded FWM scheme, where only beam experiences the amplification, leading to noise unbalance. The study of presented above is actually the question of how to preserve the quantum correlation between beams and under the introduction of two FWMs which bring the deterioration effect to the quantum correlation by the quantum amplification of both the beams (, ). The results shown in Figs 5(b) and 6(b) actually shows the boundary for the values of G2 below which the quantum correlation can always be preserved as the value of G1 increases. More interestingly, any value of G2 more than 2 will eliminate the possibility of the existence of PC with quantum correlation between beams and regardless of the value of G1.

PC between and ( and ) can be quantified by

Eq. (15) is similar to the case of Eq. (10). The region in which () is shown in magenta denoted as ((1, 4), (2, 3)) in Fig. 5(b) and the contour plot is shown in Fig. 6(c). Therefore, beams () and () are quantum correlated within the magenta region (G1 < G2) in Fig. 5(b).

PC between and ( and ) can be quantified by

Eq. (16) is always larger than 1 for any value of G1, G2 > 1 as shown in the contour plot of and in Fig. 7(a) and (b). In this sense, there isn’t any quantum correlation between beams and ( and ) since () is always larger than 1 for any value of G1, G2 > 1. The absence of () here compared with the red line in Fig. 1(b) is due to that both the beams and ( and ) are amplified by the second and the third FWM processes independently.

Figure 7
figure 7

The contour plot of (a) ; (b) and (c) .

PC between and can be quantified by

The PC with quantum correlation between beams and will be absent because G2 is always more than or equal to 1. This can be easily found if one looks at the functional form of Eq. (17). Its contour plot is shown in Fig. 7(c) in which the value of all the region is more than 1 for any G1, G2 > 1. As discussed above, for this symmetric cascaded scheme, there are three possible PCs with quantum correlation, namely , and . In addition, the existence of quantum correlation between beams and eliminates the possibility of the one between beams () and (). In other words, beam () can’t be simultaneously quantum correlated with beam () and (). These effects in this symmetric scheme are similar to the above mentioned repulsion effect of quantum correlation between the PCs in the asymmetrical cascaded FWM process. Firstly, for the PC between beams and , clearly, cell1 will provide the correlation between them while cell2 and cell3 will destroy their quantum correlation by adding extra vacuum noise, thus cell1, cell2 (cell3) can be viewed as the correlation mechanism provider and decorrelation mechanism provider respectively, thus the larger G1 and smaller G2 are preferred for the PC between beams and . Secondly, for the case of the PC between and ( and ), cell1 will generate two thermal states which will destroy their quantum correlation by adding extra vacuum noise into the system while the cell3 (cell2) will make them quantum correlated through the FWM processes. In this case, cell1, cell3 (cell2) can be viewed as the decorrelation mechanism provider and correlation mechanism provider respectively, thus the smaller G1 and larger G2 are preferred for the PC between beams and ( and ). Finally, the complete opposite dependence of the PC between beams and and the PC between beams and ( and ) on the gains results in the repulsion effect between the PCs of certain pairs. In the blank region of Fig. 5(b), all of the PCs have no quantum correlation since , , , , and , however, the quantum correlation between the quadruple beams is still present.

Here we also give a summary of the theoretical predictions of Figs 5(b), 6 and 7. We plot the dependence of the (A) ; (B) ; (C) ; (D) and ; (E) and (F) on the gain G2 when G1 = 2.94 (cell1 gain in the experiment) in Fig. 8. (trace A) can be enhanced with the increasing of G2 which is consistent with Fig. 6(a), the value of (trace B) will be larger than 1 as long as G2 > 1.67 which is consistent with the boundary (G2 = 2 − 1/G1) in Fig. 5(b), the value of and (trace D) will be smaller than 1 as long as G2 > 2.9 which is consistent with Figs 5(b) and 6(c). In addition, (trace C), (trace E) and (trace F) are also consistent with Fig. 7(a–c) respectively.

Figure 8: The dependence of (A) ; (B) ; (C) ; (D) and ; (E) and (F) on the gain G2 when G1 = 2.94 (cell1 gain in the experiment).
figure 8

The black dashed line: SQL.

We have also applied these theoretical predictions to the experimental results of the symmetrical cascaded scheme as shown in Fig. 9, the traces A, B, C, D and E are the measured DSs between and , and , and , and and the quadruple beams respectively, the trace F is the corresponding normalized SQLs for traces A ~ E (See the methods). The experimental results show 10Log() = 5.9 ± 0.3 dB, 10Log() = 3.8 ± 0.6 dB, 10Log() = 0.1 ± 0.4 dB, 10Log() = −0.2 ± 0.7 dB and 10Log() = −8.2 ± 0.5 dB at 0.6 MHz. For the experimental gains G1 ≈ 2.94 and G2 ≈ 2.85, the theoretical predictions give 10Log() = 5.1 dB, 10Log() = 3.9 dB, 10Log() = 0.2 dB, 10Log() = 0.2 dB and 10Log() = −13.6 dB. As we can see, although these theoretical predictions do not perfectly agree with the experimental results at 0.6 MHz, they still give a rough estimation of the relationship between the obtained experimental noise power traces.

Figure 9: Experimentally measured (A) ; (B) ; (C) ; (D) ; (E) and (F) the corresponding SQLs of the traces A ~ E in the symmetrical cascaded scheme.
figure 9

The vertical dashed line: 0.6 MHz.

Discussion

The PCs existed in the asymmetrical cascaded scheme and symmetrical cascaded scheme are both studied. We found that the symmetrical cascaded scheme has the following distinctions compared with the asymmetrical cascaded scheme: (1) Quantum enhancement. The DS of the quadruple beams in the symmetrical cascaded scheme (Eq. 13) has quantum enhancement compared with the one of the triple beams in the asymmetrical cascaded scheme (Eq. 7) with the same gains; (2) Boundary effect. The boundary of the PC with quantum correlation between beams and in the asymmetrical cascaded FWM scheme shown in Fig. 1(b) is obviously different from the one of the symmetrical cascaded FWM scheme shown in Fig. 5(b). This is because here beams and from the first FWM process experience the same amount of amplification in the second and third FWM processes, which leads to their good noise balance, thus the performance of the PC with quantum correlation between beams and is not as sensitive to the G2 as the one in the asymmetrical cascaded FWM scheme, where only beam experiences the amplification, leading to noise unbalance. (3) SQL Approaching. The PC between beams and in the asymmetrical cascaded FWM scheme is clearly different from the one in the symmetrical cascaded FWM scheme. The PC between beams and in the asymmetrical cascaded FWM scheme can approach its corresponding SQL (see the trace C in Fig. 3), while the PC between beams and in the symmetrical cascaded FWM scheme is always much higher than its corresponding SQL (see the trace C in Fig. 8). This is because in the asymmetrical cascaded FWM scheme only one beam is amplified by the second FWM process, while in the symmetrical cascaded FWM scheme both of the beams and are amplified by the second and third FWM processes independently.

In summary, we have theoretically characterized the performance of the PCs from the multiple quantum correlated beams and analyzed the dependence of all the PCs on the system intensity gains based on two different cascaded FWM processes. For both cases, we have theoretically predicted the so called repulsion effect of quantum correlation between the PCs of the cascaded systems. Our results presented here can be applied to the classification and application of the quantum states generated from the cascaded FWM processes.

Methods

Experimental measurements of PCs

The output beams (i = 1, 2, 3, and 4) from the cascaded FWM processes are sent to the photodetectors and their noise power values Ni (i = 1, 2, 3, and 4) are measured. One beam is subtracted from the other beam in the pairwise beams and thus the intensity-difference squeezing shared by the pairwise beams is measured. In addition, the SQL of the measured pairwise beams can be measured in this way by using a beam in a coherent state with a power equal to the total power of the measured pairwise beams impinging on the photodetectors. We then split it with a 50/50 beamsplitter, direct the obtained beams into two photodetectors. and record the noise power of the differential photocurrent. This balanced detection system makes it possible to cancel all the sources of classical noise and obtain a measure of the SQL.

Additional Information

How to cite this article: Wang, H. et al. Characterization of Pairwise Correlations from Multiple Quantum Correlated Beams Generated from Cascaded Four-Wave Mixing Processes. Sci. Rep. 7, 40410; doi: 10.1038/srep40410 (2017).

Publisher's note: Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.