Time-bin-encoding-based remote states generation of nitrogen-vacancy centers through noisy channels*
Su Shi-Leia), Chen Lib), Guo Qia), Wang Hong-Fuc), Zhu Ai-Dongc), Zhang Shoua),c)†
Department of Physics, Harbin Institute of Technology, Harbin 150001, China
Department of Physics, School of Science, Changchun University, Changchun 130022, China
Department of Physics, College of Science, Yanbian University, Yanji 133002, China

Corresponding author. E-mail: szhang@ybu.edu.cn

Project supported by the National Natural Science Foundation of China (Grant Nos. 11264042, 61465013, 11465020, and 11165015), the Program for Chun Miao Excellent Talents of Jilin Provincial Department of Education (Grant No. 201316), and the Talent Program of Yanbian University of China (Grant No. 950010001).

Abstract

We design proposals to generate a remote Greenberger–Horne–Zeilinger (GHZ) state and a W state of nitrogen-vacancy (NV) centers coupled to microtoroidal resonators (MTRs) through noisy channels by utilizing time-bin encoding processes and fast-optical-switch-based polarization rotation operations. The polarization and phase noise induced by noisy channels generally affect the time of state generation but not its success probability and fidelity. Besides, the above proposals can be generalized to n-qubit between two or among n remote nodes with success probability unity under ideal conditions. Furthermore, the proposals are robust for regular noise-changeable channels for the n-node case. This method is also useful in other remote quantum information processing tasks through noisy channels.

Keyword: 03.67.Pp; 03.67.Mn; 42.50.Dv; Greenberger–Horne–Zeilinger state; W state; nitrogen-vacancy centers; noisy channel; time-bin encoding
1. Introduction

Quantum entanglement lies at the heart of quantum information science and technology and is thought to be the key resource to realize quantum computation and quantum information processing (QIP) tasks, [14] such as quantum cryptography, [1] quantum teleportation, [3] quantum secure direct communication, [5] quantum cloning machine, [6] and so on. For the case of a tripartite system, it is well known that there are two kinds of entanglement, one is the Greenberger– Horne– Zeilinger (GHZ) state,

the other is the W state,

The GHZ state is non-equivalent to W state owing to the fact that they cannot be converted to each other by local operations and classical communication. Great efforts have been taken to research both the GHZ and W states since these two states have been shown to have valuable applications in quantum information science.[712] Lots of theoretical and experiment schemes have been proposed and reported to generate these two states.[1323]

Generating remote entanglement is critical for constructing a quantum communication network and realizing long-range quantum information processing.[24, 25] Many meaningful schemes have been proposed to generate remote entangled states[26] or implement quantum computation[27, 28] in distant participants. For the theoretical long distance quantum information processing case, the noise is not seriously considered in general. But it is one of the most important problems in experiments and practical applications since the quantum system would inevitably couple with its environment. This interaction will decrease the reliability of the quantum channel or even cause the quantum states to be changed.[29, 30] Some schemes, such as entanglement purification, [3134] error correction, [3538] and quantum repeaters[39, 40] have been proposed to solve this problem. In contrast to the above schemes, Song et al. proposed a robust scheme[41] to generate a remote atomic W state in a polarization noisy channel through an interesting method, i.e. time-bin encoding, which was first proposed by Brendel et al.[42] and used widely in QIP tasks.[4353] The polarization noise in their scheme had no influence on the fidelity of generating the intended state but it would reduce the total success probability to (1/2)n– 1 for n nodes. In addition, Huang et al. proposed a fault tolerant quantum secure direct communication against collective noise.[54] Wu et al. also proposed three quantum dialogue protocols under the condition of collection noise.[55]

Recently, a novel solid-state QIP system, the NV center in diamond, has been examined intensively[56] because it has optical controllability and good long-lived spin triplets, even at room temperature.[57] To generate entanglement, the NV center is always designed to couple to one of the following resonators, i.e. nanomechanical resonators (NAMRs)[58] and MTRs[59, 60] with a quantized whispering-gallery mode (WGM), [19, 61] or embed in cavities.[62, 63] During these apparatus, the NV center coupled to MTRs with a quantized WGM is highly competitive because the required Q factor of the MTR can be surely degraded when it couples to a fiber, which allows the photons to be inputted and outputted on demand through fibers. This feature enables researchers to deterministically generate entanglement of different NV centers in a scalable fashion. Experimentally, by using microspheres, [64, 65] diamond-GaP microdisks, [66] and SiN photonic crystals, [67] a strong coupling has been demonstrated between the NV center and the WGM. Besides, MTRs or MTRs-like equipment have been paid more attention since single-photon input– output process with the MTR coupling to atom has been reported.[59] Moreover, the quantum non-demolition measurement for the electronic spin state of diamond NV centers has been proposed[68] and experimentally demonstrated.[69] These works have shown that an NV center coupled to MTR is a suitable platform for QIP tasks.

Inspired by the above researches, we propose to generate remote an n-qubit GHZ state and a W state of NV centers coupled to MTRs through noisy channels by using time-bin encoding processes and fast optical switches. The polarization and phase noise induced by noisy channels generally affect the time of state generation but not its success probability and fidelity. The structure of this paper is arranged as follows. In Section 2, we briefly introduce the rationale of the basic model. In Section 3, we describe the process to generate the four-qubit GHZ state and W state through a noisy channel in two nodes. In Section 4, the method to generalize the proposals to n-qubit is given through regular noise-changeable channels among n nodes. A discussion and conclusion are given in Section 5.

2. Basic model

The NV centers considered here are negatively charged with six electrons from the nitrogen and three carbons surrounding the vacancy. The ground state are electronic spin triplet states | 0⟩ (ms = 0), | + 1⟩ (ms = 1), and | − 1⟩ (ms = − 1). The six excited states are recorded as | A1⟩ , | A2⟩ , | Ex⟩ , | Ey⟩ , | E1⟩ , and | E2⟩ .[61, 70] Ground states | 0⟩ and | ± 1⟩ are split with a gap of 2.87 GHz as a result of spin– spin interactions. The excited states are eigenvectors of the full Hamiltonian, which consists of a spin– spin interaction and a spin– orbit interaction without any perturbation. The pair (A1, A2) is split from the others at about 5.5 GHz owing to the spin– orbit interaction. The gap between states | A1 and | A2 would be increased to 3.3 GHz through the spin– spin interaction. Consequently, state | A2 would decay to sublevels | − 1⟩ and | + 1⟩ with emitting left (L) and right (R) polarization photons because state | A2 is robust with the stable symmetric properties in the limit of low strain, which has been demonstrated in Ref. [70]. With the aim of detecting ground state information conveniently and obtaining appropriate state transformation process, an external magnetic field B0 along the NV center symmetry axis should be introduced to the split states | − 1⟩ and | + 1⟩ . The effective energy levels of the NV centers used throughout our proposal are | A2, | + 1⟩ , and | – ⟩ , respectively. A sketch drawing is shown in Fig. 1. Considering a process where a single-photon pulse with frequency ω in inputs in an MTR cavity with the cavity mode frequency ω c, and interacts with the NV center through input– output process. Because the qubits are encoded in states | − 1⟩ and | + 1⟩ , the weak excitation condition, i.e. ⟨ σ z⟩ = − 1, should be satisfied throughout this paper. By combining the Heisenberge motion equations of the NV center lowing operators (σ ) and cavity field operator (a), and the input– output relationship , we can achieve the reflection coefficients[61, 7173]

where ω 0, κ , γ , and g denote the transition frequency between states | A2⟩ and | − 1⟩ , cavity damping rate, NV center dipolar decay rate, and the coupling coefficient between cavity and NV center, respectively. Under the condition ω c = ω 0 = ω in, the reflection coefficients would be simplified to

Fig. 1. A schematic diagram of the single photon input– output process. (a) The NV center fixing on the exterior surface of MTR and interacting with the single photon through input– output process. (b) The effective configuration of the NV center. The transformation from state | − 1⟩ to | A2⟩ is driven resonantly by the input L-polarized single photon. The transformation from state | + 1⟩ to | A2⟩ will not happen in the present scheme due to large detuning caused by the level splitting. B0 is an external magnetic field along the NV center symmetry axis to split | ± 1⟩ state. γ e is the electron gyromagnetic ratio.

After choosing coupling strength , the reflection coefficient in Eq. (4a) is reduced to r(ω in) = 1. Based on the above analysis, the controlled phase flip gate could be realized between the input pulse and NV center energy levels, which could be expressed as

after applying a phase shifter with π phase on the output pulse.

3. Generating remote four-qubit GHZ and W states between two nodes through a noisy channel
3.1. GHZ state

We now describe the process of GHZ state generation through a noisy channel via time-bin encoding. The sketch of the whole process is shown in Fig. 2. Assuming that the input photon is prepared in the state and the four NV centers are prepared in state . For convenience, we introduce a usual encoding method, . The initial state of the whole system could be written as

After photon passing through PBS1, NV1, NV2, and PBS2, the state of the whole system is transformed to

where the subscripts L0 and L1 correspond to the possible paths L0 and L1, respectively. A similar representing method will be used in the following discussion. After the optical switches S1 and S2, the whole system state evolves to

It is important that the optical switches S1 and S2, transmitted when photon in path L0 passing through, are adjusted to reflect just before the photon in path L1 passes through. The corresponding sketch of the time control sequences is shown in Fig. 3. Equation (8) implies that the polarization state of the photon is in | R⟩ state before passing through the noisy channel. This merit enables the photon pulse to see the same noise in the noisy channel, which could be expressed as

in which eiφ and eiω are phase noise, μ and ν are polarization noise parameters and satisfy the relation | μ |2+ |ν |2 = 1. Then, the evolution of the whole system after the photon pulse passes through the noisy channel could be written as

After the photon passes through optical switches S3 and S4, the whole system state is changed to

It should be noted that the optical switches S3 and S4, which are always transmitting when the earlier photon pulse (L0, L) passes through, are adjusted to reflect just before the later photon pulse (L1, L) comes. The control sequences of switches S5 and S6, S7 and S8 are the same as S3 and S4. Then, the whole state evolves to

after the photon pulse goes through PBS3, S5S8. Immediately following, the photon pulse will go through PBS4– PBS8 and the system state is transformed to

From Eq. (13), we can see that photons in path c or d are by far synchronized because the effective path length they passed are both equal to L0+ L1+ L. After the subsequent delay line LD in path d, optical switch S9, PBS9, NV3, and NV4 work, and the state of the system evolves to

Then, the photon pulse in paths e and f will be delivered into path g and h through a 50:50 beam splitter, whose function could be expressed as[74]

And after the photon pulse passes through HWP5 and HWP6, the relevant system state is converted into

in which

and

and subscripts Di (i = 1, 2, 3, 4) of the polarization state mean that this polarization state will be detected by the detector Di. From Eq. (16), we can see the following results. (i) The phase noise produced in channel has no influence on the state generation because it has been converted to a collective phase which has no observable effects. (ii) Polarization noise μ and ν can influence the time of the desired state generation rather than the success probability and fidelity of the state generation because the state would be transformed to the maximum entangled GHZ state after any one of the four detectors clicks at the time (L0+ L1+ L)/c or (L0+ L1+ L+ LD)/c. If detector D1 clicks at time (L0+ L1+ L)/c, then the system state will collapse to state | GHZ1, while if detector D2 clicks at time (L0+ L1+ L)/c, then the system state will collapse to state | GHZ2. The other six cases and the corresponding GHZ states could be achieved analogously.

Fig. 2. A schematic diagram for GHZ state generation through noisy channel. Numbers 1– 11 denote the polarization beam splitters (PBS), whose function is to translate R polarization light and reflect L polarization light. The role of the half wave plate 1 (HWP1)– HWP4 is to perform σ x operation (| R⟩ ↔ | L⟩ ) on photon state, while the function of HWP5 and HWP6 can be represented as . The photon flying time difference between length L0 and L1 (L1> L0) is big enough to make the optical switch transmit or reflect. Nevertheless, this time difference should be taken to be much less than the photon fluctuation time L/c in the noisy channel to ensure that the noise has the same effect on the photon coming from path L0 or L1. The action of LD, which has a similar length to L1, is to delay the photon pulse in the lower path. The lengths of paths without labelling L0, L1, L, and LD are much less than L1L0 and can be ignored.

Fig. 3. Time control sequences of optical switches from S1 to S9. T and R mean that the optical switches are transmitted and reflected, respectively. Δ T is the photon pulse width, which should be far more less than the interval (L1L0)/c. Thus, Δ t≃ (L1L0)/c, and Δ t1LD/c. The time between S3 and S6 or between S3 and S8 should be much less than Δ t and have been ignored.

3.2. W state

We now describe the process for four-qubit W state generation between two nodes. The sketch is shown in Fig. 4. The control sequences of optical switches are shown in Fig. 3. Assuming that the initial photon pulse is in state | R⟩ and the four NV centers are all in state | + ⟩ . Thus, the initial system state could be represented as

which would be transformed to

after HWP1, NV1, PBS1, HWP2, and NV2 work. After the photon pulse passes through the time-bin encoding apparatus and optical switches S1 and S2, the system state will evolve to

Suppose the influence on photon pulse induced by noisy channel is same as Eq. (9), and would change system state to

Then from Fig. 4, the system has the following process

The component of the photon pulse in path d would go through an extra delay line LD and the state would be transformed to

Fig. 4. A sketch of W state generation. H1, H2, H3, and H4 denote the HWP with the action on the photon pulse, respectively. The role of the HWP1, HWP2, HWP3, HWP4 is to perform a σ x operation (| R⟩ ↔ | L⟩ ) on the photon. The optical control sequences and requirement of delay lines are the same as GHZ state generation.

The system state will have the following evolving process after the photon pulse interacts with the rest devices

It is easy to see that the polarization noise and phase noise have no influence on the state generation. If detector D2 clicks at time (L1+ L+ L0)/c or (L1+ L+ L0+ LD)/c, then the state of the four NV centers would both collapse to W state determinately.

4. Generating n-Qubit entanglement among n nodes through regular noise-changeable channels

Next, we shift our attention to illustrate the principle for generalizing the above proposals to n-qubit among two nodes or n (n !⩾ 3) nodes. For the case of n (n ⩾ 3) nodes, the proposals are robust for the regular changeable noise. This merit enables our proposals to have broadened applications in large scale QIP through noisy channels.

4.1. GHZ state

In this subsection, we illustrate the process of n-qubit GHZ state generation among n nodes, which are schematically drawn in Fig. 5. The case to generate n-qubit GHZ states between two nodes can be easily derived by following the process in Subsection 3.1 by adding NV centers behind NV 2 or NV 4 in Fig. 2. Thus, we will focus on describing the n nodes case in this subsection.

Fig. 5. A schematic diagram to generalize GHZ state generation to n-qubit case among n nodes. The role of HWP1-HWP4n− 4 is to perform a σ x operation on the photon pulse, while the role of HWP4n− 3 and HWP4n− 2 is to realize the transformation . The control sequences of optical switches are shown in Fig. 7. Subscript k denotes the sequence number of the node where the optical switches are located. It should be noted that the optical path and the elements from node 2 to node n − 1 are all same, except the the delay lines (marked with green boxes) under the optical switches S9k− 9, whose length is designed as LDj = 2j− 1LD(1 ⩽ jn− 1).

We first consider the 3-node case, based on which the n-node case can be understood and derived. The initial state is . Assuming that the noisy channel 1 has the effect , and noisy channel 2 has the effect on the pulse with arriving time inside interval (2L0+ L1+ L)/c– (L0+ 2L1+ L)/c and on the pulse with arriving time inside interval (2L0+ L1+ L+ LD)/c– (L0+ 2L1+ L+ LD)/c, respectively. The control sequences of optical switches S1– S9 and S10– S18 are shown in Fig. 3 and Fig. 6, respectively. The state evolution process can be expressed as

where and . From the above expression (24), we can obtain the following information, that is, a | GHZ+ (| GHZ) state will be achieved if the detector D1 or D4 (D2 or D3) clicks at any one of the four following times, i.e., (2L0+ 2L1+ 2L)/c, (2L0+ 2L1+ 2L+ LD)/c, (2L0+ 2L1+ 2L+ 2LD)/c, and (2L0+ 2L1+ 2L+ 3LD)/c. That is to say, the steady noise introduced by the noisy channel 1 and the regular changeable noise introduced by the noisy channel 2 have no effect on the state generation.

Fig. 6. Control sequences of optical switches S10– S18. The channels following optical switch S11 should have the same influence on the photon with arriving time inside the red-dotted-line-formed rectangle, but can have a different influence on the photon with arriving time inside a different red-dotted-line-formed rectangle. The control sequences of optical switches S1– S9 are identical to Fig. 3. Δ t2⋍ (LD+ L0L1)/c.

Fig. 7. Time control sequences of optical switches for n-node (n⩾ 3) GHZ and W states generation. The regular noise-changeable channels following optical switch S9k– 7 should have the same influence on the photon with arriving time inside the red-dotted-line-formed rectangle but can have a different influence on the photon with arriving time inside a different red-dotted-line-formed rectangle.

We now discuss the n-node (n > 3) case. For simplicity, we assume that the noises in different channels are the same and can be expressed as | R⟩ → eiφ μ | R⟩ + eiω ν | L⟩ . Initially, suppose that the photon pulse is in state , and each of the NV centers is in state | + ⟩ . According to Fig. 5 and Fig. 7, the process of state evolution could be written as

From the last term in Eq. (25), one can see that if D4 clicks at the time [(n− 1)L0+ (n− 1)L1+ (n− 1)L+ (2n− 1− 1)LD]/c, then the n-qubit GHZ state would be generated. Similar results would be achieved if other detectors click at the time [(n− 1)L0+ (n− 1)L1+ (n− 1)L+ LD]/c ( is an integer which belongs to the interval [0, (2n− 1– 1)]).

4.2. W state

The case of the n-qubit W state is schematically drawn in Fig. 8. The case to generate a n-qubit W state between two nodes can be derived similarly according to Subsection 3.2 and Fig. 8(a). Thus, we focus on the case among n nodes. For simplicity, we first consider the three-node case, based on which the n-node case can be deduced. The initial state of the whole system is | ψ 1 = | R⟩ | + ⟩ 1| + ⟩ 2| + ⟩ 3. Assuming that the influence of noisy channels is the same as in Subsection 4.1, then we can have the following process

From Eq. (26), we can see that the steady noise caused by channel 1 and the regular changeable noise caused by channel 2 would influence the time of state generation but have no effect on the success probability and fidelity. The n-node case can also be derived in a similar way based on the sketch in Fig. 8(b) and the control sequences of the optical switches in Fig. 7.

We now discuss the n-node (n > 3) case. For simplicity, supposing that the noises in different channels are the same and can be expressed as | R⟩ → eiφ μ | R⟩ + eiω ν | L⟩ . Initially, the photon pulse is in state | R⟩ , and each of the NV centers is in state | + ⟩ . According to Fig. 7 and Fig. 8, the process of state evolution could be written as

From Eq. (27), one can see that the n-qubit W state can be generated if detector D2 clicks at any one of the times [(n– 1)L0+ (n– 1)L1+ (n– 1)L+ LD]/c ( is an integer which belongs to the interval [0, (2n– 1– 1)]). Moreover, the noises have no influence on state generation since the overall phase could be eliminated.

Fig. 8. A schematic diagram to generalize W state generation to n-qubit case. The photon pulses are both prepared in | R⟩ state and the NV centers are all prepared in | + ⟩ state. Hl denotes the HWP with the action and HWPk denotes the HWP with the action | R⟩ ↔ | L⟩ . (a) To generate n qubit W state between two nodes. The control sequences are the same as those in Fig. 3. (b) To generate an n qubit W state among n nodes. The control sequences are the same as those in Fig. 6. The optical path and elements from node 2 to node n – 1 are all the same, except for the delay lines (marked with green boxes) under the optical switches S9k– 9, whose length is designed as LDj = 2j– 1LD.

5. Discussion and conclusion

The feasibility of our proposals mainly depends on the time-bin encoding and the performance of our NV center, it is thus essential to discuss the experimental feasibility of these two primary components. The accuracy of the time is seriously dependent on the length of the delay lines. Thus, the delay line lengths L0, L1, and LD are critical in our proposals. The time Δ t, Δ t1, and Δ t2 should be big enough to make sure that the status of optical switches has enough time to be changed, which can be achieved by adjusting the lengths of L0, L1, and LD. Meanwhile, the time interval Δ t should be less than L/c to ensure that the noisy channel has a steady influence on the photon pulse with arriving time inside the red-dotted-line-formed rectangle, as shown in Fig. 7. In addition, LD should have a similar value as L1 to ensure L0+ LD> L1, this is the prerequisite condition to unmix the pulses with different noises and arriving times. In addition, The reason why we have not considered the interaction time between photon pulses and NV centers is that it has a smaller level. Sometimes it may even be bigger than (L1L0)/c. Since the | L⟩ component of photon pulse with different noises and arriving time will inevitably interact with the NV centers, we can add extra delay lines in the paths which | R⟩ component passes through to make the two paths balanced. The only influence of these balanced paths is to shift the control sequences in Fig. 7 to the right for some definite distance, this is the reason why we have not considered the interaction time. Experimentally, time-bin encoding has been widely researched and demonstrated. Brendel et al. have demonstrated the time-bin encoding with time difference (L1L0)/c in ns orders of magnitude.[42, 43] Recently, Wang et al. have realized the high-speed tomography of time-bin-entangled photons with the time difference 21.3 ns[44] and Takeda et al. have demonstrated it in a time difference 242 ns.[45] Besides, time-bin encoding has been verified as interacting with semiconductor quantum wells, [46] quantum dots, [4749] collective atomic excitation in a rare-earth-doped solid, [50] and it has been realized in other QIP tasks.[45, 51] Furthermore, Humphreys et al. have recently demonstrated a robust heralded controlled-phase gate with higher fidelity by using single-spatial time-bin encoding.[52] Donohue et al. have recently reported an effective technique using a nonlinear interaction between chirped entangled time-bin photons and shaped laser pulses to perform projective measurements on arbitrary time-bin states with ps-scale separations to readout the information of time-bin encoding.[53] That is, recent advances in Refs. [52] and Ref. [53] have provided powerful supporting for time-bin-encoding-based QIP tasks.

On the other hand, many efforts have been paid to investigate the performance of the NV centers and the coupled resonators. Although the ideal coupling strength between the NV center and optical resonator is supposed to be on the order of hundreds of megahertz, it is inevitably diminished due to some out-out-control effects.[75] Research on composite microcavity systems where NV centers in bulk diamond couple evanescently to optical resonators[6567] makes it possible to retain the excellent properties of NV centers. The experiment in Ref. [66] provided the datum (g, κ , γ )/2π ≈ (0.3, 26, 0.0004) with a relative low-Q value 104. This datum is very close to the requirement of our proposal , which is the same as Ref. [61]. It deserves special mention that the NV centers used here can be replaced by any system which can realize a controlled phase flip gate.

The efficiency of our proposals is defined as the probability of the photons to be detected after the generation process. Thus, similar to the scheme proposed in Ref. [76], we use to denote the efficiency for GHZ state and W state, in which n denotes number of NV centers. The fidelity of the present proposal is defined as F = | ⟨ ψ ideal| ψ prac⟩ | 2, where | ψ ideal⟩ is the ideal final state of the quantum system after processing for state generation, and | ψ prac⟩ is the final state of the system by considering practical external reservoirs. In Fig. 9, we plot the efficiency of n-qubit state generation and fidelity of 4-qubit state generation, from which we can see that the fidelity would be higher than 92% if the condition g2/κ γ > 15 is satisfied. However, it should be noted that the fidelity would decrease as the number of NV centers grow. The efficiency would be higher than 90% if the cavity parameters g2/κ γ are greater than 50 and the number of NV centers is less than 10. Nevertheless, in practical experiments, the efficiency would also be influenced by other factors; such as, the photon loss induced by the fiber and the insensitivity of the photon detector.

Fig. 9. (a) Efficiency of n-qubit GHZ and W-states generation. (b) Fidelity of 4-qubit GHZ and W states generation.

In conclusion, we have designed theoretical proposals to generate GHZ and W states of NV centers coupled to microresonator through noisy channels with the help of time-bin encoding processes and optical switches. The polarization and phase noise induced by noisy channels generally affect the time of state generation but not its success probability and fidelity, which is a big progress compared with the success probability 1/2 in Ref. [41]. The proposals can also be generalized to n-qubit between two nodes or among n nodes with n – 1 different noisy channels. In addition, this proposal is robust for the regular changeable noise. For the n-qubit state generation, we here only consider the two extreme cases, i.e. two-node case and n-node case. In fact, the n-qubit state can also be generated in more than two and less than n nodes if the operators place more than one NV center in any node. In other words, our proposals provide an alternative avenue for remote large scale QIP through noisy channels via time-bin encoding.

Reference
1 Ekert A K 1991 Phys. Rev. Lett. 67 661 DOI:10.1103/PhysRevLett.67.661 [Cited within:2] [JCR: 7.943]
2 Bennett C H and Wiesner S J 1992 Phys. Rev. Lett. 69 2881 DOI:10.1103/PhysRevLett.69.2881 [Cited within:1] [JCR: 7.943]
3 Bennett C H, Brassard G, Crépeau C, Jozsa R, Peres A and Wootters W K 1993 Phys. Rev. Lett. 70 1895 DOI:10.1103/PhysRevLett.70.1895 [Cited within:1] [JCR: 7.943]
4 Bennett C H and DiVincenzo D P 2000 Nature 404 247 DOI:10.1038/35005001 [Cited within:1] [JCR: 38.597]
5 Zhu A D, Xia Y, Fan Q B and Zhang S 2006 Phys. Rev. A 73 022338 DOI:10.1103/PhysRevA.73.022338 [Cited within:1] [JCR: 3.042]
6 Deng F G and Long G L 2004 Phys. Rev. A 70 012311 DOI:10.1103/PhysRevA.70.012311 [Cited within:1] [JCR: 3.042]
7 Karlsson A and Bourennane M 1998 Phys. Rev. A 58 4394 DOI:10.1103/PhysRevA.58.4394 [Cited within:1] [JCR: 3.042]
8 Shi B S and Tomita A 2002 Phys. Lett. A 296 161 DOI:10.1016/S0375-9601(02)00257-8 [Cited within:1] [JCR: 1.11]
9 Cleve R, Gottesman D and Lo H K 1999 Phys. Rev. Lett. 83 648 DOI:10.1103/PhysRevLett.83.648 [Cited within:1] [JCR: 7.943]
10 Durkin G A, Simon C and Bouwmeester D 2002 Phys. Rev. Lett. 88 187902 DOI:10.1103/PhysRevLett.88.187902 [Cited within:1] [JCR: 7.943]
11 Gorbachev V N, Trubilko A I, Rodichkina A A and Zhiliba A I 2003 Phys. Lett. A 314 267 DOI:10.1016/S0375-9601(03)00906-X [Cited within:1] [JCR: 1.11]
12 Gisin N and Massar S 1997 Phys. Rev. Lett. 79 2153 DOI:10.1103/PhysRevLett.79.2153 [Cited within:1] [JCR: 7.943]
13 Zou X B, Pahlke K and Mathis W 2004 Phys. Rev. A 69 052314 DOI:10.1103/PhysRevA.69.052314 [Cited within:1] [JCR: 3.042]
14 Fidio C D and Vogel W 2003 J. Opt. B: Quantum Semiclass. Opt. 5 105 DOI:10.1088/1464-4266/5/1/314 [Cited within:1] [JCR: 1.813]
15 Duan L M and Kimble H J 2003 Phys. Rev. Lett. 90 253601 DOI:10.1103/PhysRevLett.90.253601 [Cited within:1] [JCR: 7.943]
16 Yamamoto T, Tamaki K, Koashi M and Imoto N 2002 Phys. Rev. A 66 064301 DOI:10.1103/PhysRevA.66.064301 [Cited within:1] [JCR: 3.042]
17 Yu C S, Yi X X, Song H S and Mei D 2007 Phys. Rev. A 75 044301 DOI:10.1103/PhysRevA.75.044301 [Cited within:1] [JCR: 3.042]
18 Zheng A S, Li J H, Yu R, X Y and Wu Y 2012 Opt. Express 20 16902 DOI:10.1364/OE.20.016902 [Cited within:1] [JCR: 3.546]
19 Cheng L Y, Wang H F, Zhang S and Yeon K H 2013 Opt. Express 21 5988 DOI:10.1364/OE.21.005988 [Cited within:1] [JCR: 3.546]
20 Eibl M, Kiesel N, Bourennane M, Kurtsiefer C and Weinfurter H 2004 Phys. Rev. Lett. 92 077901 DOI:10.1103/PhysRevLett.92.077901 [Cited within:1] [JCR: 7.943]
21 Leibfried D, Knill E, Seidelin S, Britton J, Blakestad R B, Chiaverini J, Hume D B, Itano W M, Jost J D, Langer C, Ozeri R, Reichle R and Wineland D J 2005 Nature 438 639 DOI:10.1038/nature04251 [Cited within:1] [JCR: 38.597]
22 Häffner H, Hänsel W, Roos C F, Benhelm J, Chekalkar D, Chwalla M, Körber T, Rapol U D, Riebe M, Schmidt P O, Becher C, Gühne O, Dür W and Blatt R 2005 Nature 438 643 DOI:10.1038/nature04279 [Cited within:1] [JCR: 38.597]
23 Rauschenbeutel A, Nogues G, Osnaghi S, Bertet P, Brune M, Raimond J M and Haroche S 2000 Science 288 2024 DOI:10.1126/science.288.5473.2024 [Cited within:1]
24 Cirac J I, Zoller P, Kimble H J and Mabuchi H 1997 Phys. Rev. Lett. 78 3221 DOI:10.1103/PhysRevLett.78.3221 [Cited within:1] [JCR: 7.943]
25 Browne D E, Plenio M B and Huelga S F 2003 Phys. Rev. Lett. 91 067901 DOI:10.1103/PhysRevLett.91.067901 [Cited within:1] [JCR: 7.943]
26 Stace T M, Milburn G J and Barnes C H W 2003 Phys. Rev. B 67 085317 DOI:10.1103/PhysRevB.67.085317 [Cited within:1]
27 Serafini A, Mancini S and Bose S 2006 Phys. Rev. Lett. 96 010503 DOI:10.1103/PhysRevLett.96.010503 [Cited within:1] [JCR: 7.943]
28 Deng Z J, Zhang X L, Wei H, Gao K L and Feng M 2007 Phys. Rev. A 76 044305 DOI:10.1103/PhysRevA.76.044305 [Cited within:1] [JCR: 3.042]
29 Li X H, Deng F G and Zhou H Y 2007 Appl. Phys. Lett. 91 144101 DOI:10.1063/1.2794433 [Cited within:1] [JCR: 3.794]
30 Yamamoto T, Shimamura J, Oz̈demir Ş K, Koashi M and Imoto N 2005 Phys. Rev. Lett. 95 040503 DOI:10.1103/PhysRevLett.95.040503 [Cited within:1] [JCR: 7.943]
31 Bennett C H, Brassard G, Popescu S, Schumacher B, Smolin J A and Wootters W K 1996 Phys. Rev. Lett. 76 722 DOI:10.1103/PhysRevLett.76.722 [Cited within:1] [JCR: 7.943]
32 Sheng Y B, Zhou L, Cheng W W, Gong L Y, Zhao S M and Zheng B Y 2012 Chin. Phys. B 21 030307 DOI:10.1088/1674-1056/21/3/030307 [Cited within:1] [JCR: 1.148] [CJCR: 1.2429]
33 Zheng S B 2008 Chin. Phys. B 17 2969 DOI:10.1088/1674-1056/17/8/034 [Cited within:1] [JCR: 1.148] [CJCR: 1.2429]
34 Xue P 2011 Chin. Phys. B 20 100310 DOI:10.1088/1674-1056/20/10/100310 [Cited within:1] [JCR: 1.148] [CJCR: 1.2429]
35 Steane A M 1996 Phys. Rev. Lett. 77 793 DOI:10.1103/PhysRevLett.77.793 [Cited within:1] [JCR: 7.943]
36 Zhao F 2013 Acta Phys. Sin. 62 200303 (in Chinese) DOI:10.7498/aps.62.200303 [Cited within:1] [JCR: 1.016] [CJCR: 1.691]
37 Xiao F Y and Chen H W 2011 Acta Phys. Sin. 60 080303 (in Chinese) DOI:10.7498/aps.60.080303 [Cited within:1] [JCR: 1.016] [CJCR: 1.691]
38 Zhang Z R, Liu W T and Li C Z 2011 Chin. Phys. B 20 050309 DOI:10.1088/1674-1056/20/5/050309 [Cited within:1] [JCR: 1.148] [CJCR: 1.2429]
39 Briegel H J, Dür W, Cirac J I and Zoller P 1998 Phys. Rev. Lett. 81 5932 DOI:10.1103/PhysRevLett.81.5932 [Cited within:1] [JCR: 7.943]
40 Xue L, Nie M and Liu X H 2013 Acta Phys. Sin. 62 170305 (in Chinese) DOI:10.7498/aps.62.170305 [Cited within:1] [JCR: 1.016] [CJCR: 1.691]
41 Song J, Xia Y and Song H S 2008 Phys. Rev. A 78 024302 DOI:10.1103/PhysRevA.78.024302 [Cited within:2] [JCR: 3.042]
42 Brendel J, Mohler E and Martienssen W 1991 Phys. Rev. Lett. 66 1142 DOI:10.1103/PhysRevLett.66.1142 [Cited within:2] [JCR: 7.943]
43 Brendel J, Gisin N, Tittel W and Zbinden H 1999 Phys. Rev. Lett. 82 2594 DOI:10.1103/PhysRevLett.82.2594 [Cited within:2] [JCR: 7.943]
44 Wang S X, Chan C, Moraw P, Reilly D R, Altepeter J B and Kanter G S 2012 Phys. Rev. A 86 042122 DOI:10.1103/PhysRevA.86.042122 [Cited within:1] [JCR: 3.042]
45 Takeda S, Mizuta T, Fuwa M, Yoshikawa J I, Yonezawa H and Furusawa A 2013 Phys. Rev. A 87 043803 DOI:10.1103/PhysRevA.87.043803 [Cited within:2] [JCR: 3.042]
46 Heberle A P, Baumberg J J, Binder E, Kuhn T, Kohler K and Ploog K H 1996 IEEE J. Sel. Top. Quantum Electron. 2 769 DOI:10.1109/2944.571778 [Cited within:1] [JCR: 4.078]
47 Marie X, Le Jeune P, Amand T, Brousseau M, Barrau J, Paillard M and Planel R 1997 Phys. Rev. Lett. 79 3222 DOI:10.1103/PhysRevLett.79.3222 [Cited within:1] [JCR: 7.943]
48 Bonadeo N H, Erland J, Gammon D, Park D, Katzer D S and Steel D G 1998 Science 282 1473 DOI:10.1126/science.282.5393.1473 [Cited within:1]
49 Michaelis de Vasconcellos S, Gordon S, Bichler M, Meier T and Zrenner A 2010 Nat. Photon. 4 545 DOI:10.1038/nphoton.2010.124 [Cited within:1] [JCR: 27.254]
50 Riedmatten H D, Afzelius M, Staudt M U, Simon C and Gisin N 2008 Nature 456 773 DOI:10.1038/nature07607 [Cited within:1] [JCR: 38.597]
51 Takeda S, Mizuta T, Fuwa M, Loock P V and Furusawa A 2013 Nature 500 315 DOI:10.1038/nature12366 [Cited within:1] [JCR: 38.597]
52 Humphreys P C, Metcalf B J, Spring J B, Moore M, Jin X M, Barbieri M, Kolthammer W S and Walmsley I A 2013 Phys. Rev. Lett. 111 150501 DOI:10.1103/PhysRevLett.111.150501 [Cited within:2] [JCR: 7.943]
53 Donohue J M, Agnew M, Lavoie J and Resch K J 2013 Phys. Rev. Lett. 111 153602 DOI:10.1103/PhysRevLett.111.153602 [Cited within:3] [JCR: 7.943]
54 Huang W, Wen Q Y, Jia H Y, Qin S J and Gao F 2012 Chin. Phys. B 21 100308 DOI:10.1088/1674-1056/21/10/100308 [Cited within:1] [JCR: 1.148] [CJCR: 1.2429]
55 Wu G T, Zhou N R, Gong L H and Liu S Q 2014 Acta Phys. Sin. 63060302 (in Chinese) DOI:10.7498/aps.63.060302 [Cited within:1] [JCR: 1.016] [CJCR: 1.691]
56 Neumann P, Mizuochi N, Rempp F, Hemmer P, Watanabe H, Yamasaki S, Jacques V, Gaebel T, Jelezko F and Wrachtrup J 2008 Science 320 1326 DOI:10.1126/science.1157233 [Cited within:1]
57 Childress L, Gurudev Dutt M V, Taylor J M, Zibrov A S, Jelezko F, Wrachtrup J, Hemmer P R and Lukin M D 2006 Science 314 281 DOI:10.1126/science.1131871 [Cited within:1]
58 Xu Z Y, Hu Y M, Yang W L, Feng M and Du J F 2009 Phys. Rev. A 80 022335 DOI:10.1103/PhysRevA.80.022335 [Cited within:1] [JCR: 3.042]
59 Dayan B, Parkins A S, Aoki T, Ostby E P, Vahala K J and Kimble H J 2008 Science 319 1062 DOI:10.1126/science.1152261 [Cited within:2]
60 Cao C, Liu G, Zhang R and Wang C 2014 Chin. Phys. B 23 040304 DOI:10.1088/1674-1056/23/4/040304 [Cited within:1] [JCR: 1.148] [CJCR: 1.2429]
61 Chen Q, Yang W L, Feng M and Du J F 2011 Phys. Rev. A 83 054305 DOI:10.1103/PhysRevA.83.054305 [Cited within:4] [JCR: 3.042]
62 Lim Y L, Beige A and Kwek L C 2005 Phys. Rev. Lett. 95 030505 DOI:10.1103/PhysRevLett.95.030505 [Cited within:1] [JCR: 7.943]
63 Yang W L, Yin Z Q, Xu Z Y, Feng M and Du J F 2010 Appl. Phys. Lett. 96 241113 DOI:10.1063/1.3455891 [Cited within:1] [JCR: 3.794]
64 Park Y S, Cook A K and Wang H L 2006 Nano Lett. 6 2075 DOI:10.1021/nl061342r [Cited within:1] [JCR: 13.025]
65 Barbour R J, Dinyari K N and Wang H L 2010 Opt. Express 18 18968 DOI:10.1364/OE.18.018968 [Cited within:2] [JCR: 3.546]
66 Barclay P E, Fu K M C, Santori C and Beausoleil R G 2009 Appl. Phys. Lett. 95 191115 DOI:10.1063/1.3262948 [Cited within:2] [JCR: 3.794]
67 McCutcheon M W and Loncar M 2008 Opt. Express 16 19136 DOI:10.1364/OE.16.019136 [Cited within:2] [JCR: 3.546]
68 Young A, Hu C Y, Marseglia L, Harrison J P, O’Brien J L and Rarity J G 2009 New J. Phys. 11 013007 DOI:10.1088/1367-2630/11/1/013007 [Cited within:1] [JCR: 4.063]
69 Buckley B B, Fuchs G D, Bassett L C and Awschalom D D 2010 Science 330 1212 DOI:10.1126/science.1196436 [Cited within:1]
70 Togan E, Chu Y, Trifonov A S, Jiang L, Maze J, Childress L, Dutt M V G, Sørensen A S, Hemmer P R, Zibrov A S and Lukin M D 2010 Nature 466 730 DOI:10.1038/nature09256 [Cited within:2] [JCR: 38.597]
71 An J H, Feng M and Oh C H 2009 Phys. Rev. A 79 032303 DOI:10.1103/PhysRevA.79.032303 [Cited within:1] [JCR: 3.042]
72 Hu C Y, Young A, OBrien J L, Munro W J and Rarity J G 2008 Phys. Rev. B 78 085307 DOI:10.1103/PhysRevB.78.085307 [Cited within:1]
73 Su S L, Guo Q, Zhu L, Wang H F and Zhang S 2012 J. Opt. Soc. Am. B 29 2827 DOI:10.1364/JOSAB.29.002827 [Cited within:1] [JCR: 2.21]
74 Pavičić M 2011 Phys. Rev. Lett. 107 080403 DOI:10.1103/PhysRevLett.107.080403 [Cited within:1] [JCR: 7.943]
75 Barclay P E, Santori C, Fu K M, Beausoleil R G and Painter O 2009 Opt. Express 17 8081 DOI:10.1364/OE.17.008081 [Cited within:1] [JCR: 3.546]
76 Ren B C and Deng F G 2014 Sci. Rep. 4 4623 DOI:10.1038/srep04623 [Cited within:1] [JCR: 15.333]