Studying the squeezing effect and phase space distribution of single-photonadded coherent state using postselected von Neumann measurement
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Studying the squeezing effect and phase space distribution of single- photon- added coherent state using postselected von Neumann measurement Wen Jun Xu, Taximaiti Yusufu and Yusuf Turek∗ School of Physics and Electronic Engineering, Xinjiang Normal University, Urumqi, Xinjiang 830054, China (Dated: September 15, 2021) In this paper, ordinary and amplitude-squared squeezing as well as Wigner functions of single- photon-added coherent state after postselected von Neumann measurements are investigated. The analytical results show that the von Neumann type measurement which is characterized by post- selection and weak value can significantly change the squeezing feature of single-photon-added co- herent state. It is also found that the postselected measurement can increase the nonclassicality of the original state in strong measurement regimes. It is anticipated that this work could may provide an alternate and effective methods to solve state optimization problems based on the postselected arXiv:2109.05423v2 [quant-ph] 14 Sep 2021 von Neumann measurement technique. PACS numbers: 42.50.-p, 03.65.-w, 03.65.Ta I. INTRODUCTION quantum digital signature [51], the optimization for this state is worthy of study, in particular, it may provide new States which possess nonclassical features are an im- methods to the implementations related processes. On portant resources for quantum information processing the other hand, the weak signal amplification technique and the investigation of fundamental problems in quan- proposed in 1988 [52] by Aharonov, Albert, and Vaidman tum theory. It has been shown that squeezed states of is widely used in state optimization and precision mea- radiation fields has been can be considered truly quan- surement problems [53–59]. Most recently, one of the tum [1]. In recent years studies concerning squeezing authors of this paper investigated the effects of postse- especially quadrature squeezing of radiation fields has lected von Neumann measurement on the properties of seen considerable attention as it may have applcaition single-mode radiation fields [58, 59] and found that post- in optical communication and information theory [2–13], selected von Neumann measurement changed the photon gravitatioanl wave detection [14], quantum teleportation statistics and quadrature squeezing of radiation fields for [14–22], dense coding [23], resonance fluorscence [24], different anomalous weak values and coupling strengths. and quantum cryptography [25]. Furthermore, with the However, to the best of our knowledge, the effects of rapid development of the techniques for making higher- postselected von Neumann measurement on higher-order order correlation measurements in quantum optics and squeezing and phase-space distribution of SPACS have laser physics, the high-order squeezing effects of radiation not been previously investigated. fields have also became a hot topic in state optimization In this work, motivated by our prior work [56, 58, 59], researches. Higher-order squeezing of radiation fields was we study the squeezing and Wigner function of SPACS first introduced by Hong and Manel [26] in 1985, and Hil- after postselected von Neumann measurement. In this ley [27, 28] defined another type higher-order squeezing, work, we take the spatial and polarization degrees of named amplitude- squared squeezing (ASS) of the elec- freedom of SPACS as a measuring device (pointer) and tromagnetic field in 1987. Following this work the highe- system, respectively, and consider all orders of the time squeezing of radiation fields has been investigated across evolution operator. Following determination of the final many fields of research. [29–45]. state of the pointer, we check the criteria for existence Squeezing is an inherent feature of nonclassical states, of squeezing of SPACS, and found that the postselected and its improvement requires optimization. Some states measurement has positve effects on squeezing of SPACS do not initially possess squeezing, but after undergoing in the weak measurement regime. Furthermore, we in- an optimization process, they may possess a pronounced vestigate the state-distance and the Wigner function of squeezing effect, The single-photon-added coherent state the SPACS after measurement. We found that with in- (SPACS) is a typical example. SPACAS are created by creasing coupling strength, the original SPACS spoiled adding the creation operator a† to the coherent state, and significantly, and the state exhibited more pronounced this optimization changes the coherent state from semi- negative areas as well as interference structures in phase classical to a new quantum state which possess squeez- space after postselected measurement. We observed that ing. Since this state has wide application across many the postselected von Neumann measurement has posi- quantum information processes including quantum com- tive effects on its nonclassicality including squeezing ef- munication [46], quantum key distribution [47–50], and fects especially in the weak measurement regime. These results can be considered a result of weak value amplifi- cation of the weak measurement technique. This paper is organized as follows. In Sec. II, we in- ∗ yusufu1984@hotmail.com troduce the main concepts of our scheme and derive the
2 final pointer state after postselected measurement which and will be used throughout the study. In Sec. III, we give ϕ ϕ the details of ordinary squeezing and ASS effects of the |ψi i = cos |Hi + eiδ sin |V i, (4) 2 2 final pointer state. In Sec. IV, we investigate the state distance and the Wigner function SPACS after measure- respectively. Here, α = reiθ and δ ∈ [0, 2π] and ϕ ∈ ment. A conclusion is given in Sec. V. [0, π). Here, we are reminded that in weak measurement theory, the interaction strength between the system and measurement is weak, and it is enough to only consider II. MODEL AND THEORY the evolution of the unitary operator up to its first or- der. However, if we want to connect the weak and strong measurement and investigate the measurement feedback In this section, we introduce the basic concepts of post- of postselected weak measurement, and analyze experi- selected von Neumann measurement and give the expres- mental results obtained in non-ideal measurements, the sion of the final pointer state which we use in this paper. full-order evolution of the unitary operator is needed [61– We know that every measurement problems consists of 63], We call this kind of measurement a postselected von three main parts including a pointer(measuring device), Neumann measurement. Thus, the evolution operator of measuring system and the environment. In the current this total system corresponding to the interaction Hamil- work, we take the spatial and polarization degrees of free- tonian, Eq. (1), is evaluated as dom of SPACS as the pointer and system, respectively. In general, in measurement problems we want to deter- 1 ˆ s 1 s mine the system information of interest by comparing the e−ig0 σx ⊗P = I + σ̂x ⊗D + Iˆ − σ̂x ⊗D − 2 2 2 2 state-shifts of the pointer after measurement finishes, and (5) we do not consider spoiling of the pointer in the entire sinceσ̂x2 = 1. Here,s = gσ0 is the ratio between the cou- measurement process. Here, contrary to the standard pling strength and beam width, and it can characterize goal of the measurement, we investigate the effects of pre- the measurement types i.e. the measurement is consid- and post-selected measurement taken on a beam’s po- ered a weak measurement (strong measurement) if s < 1 larization(measured system) on the inherent properties (s > 1). D( 2s ) is the displacement operator defined as of a beam’s spatial component (pointer). In the mea- † ∗ D(α) = eαâ −α â . The results of our current research surement process, the system and pointer Hamiltonians are valid for weak and strong measurement regimes since doesn’t effect the final read outs, so it is sufficient to only we take into account the all orders of the time evolution consider their interaction Hamiltonian for our purposes. operator, Eq. (5). In the above calculation we use the According to standard von Neumann measurement the- definition of the momentum operator represented in Fock ory, the interaction Hamiltonian between the system and space in terms of an annihilation (creation) operator â the pointer takes the form [60] (↠), i.g., i a† − a P̂ = (6) Ĥ = g(t) ⊗ P̂ . (1) 2σ where σ is the width of the beam. Thus, the total state Here,  is the system observable we want to measure, and of the system, |ψi i⊗|φi, after the time evolution becomes P̂ is the momentum operator h of the i pointer conjugated with the position operator, X̂, P̂ = i. g(t) is the cou- |Ψi = e−ig0 σx ⊗P |ψi i ⊗ |φi pling strength function between the system and pointer 1 ˆ s ˆ −s and it is assumed exponentially small except during a = I + σ̂x ⊗ D + I − σ̂x ⊗ D |ψi i ⊗ |φi 2 2 2 period of interaction time of order T , and is normalized (7) R +∞ RT according to −∞ g(t)dt = 0 g(t)dt = g0 . In this work, we assume that the system observable A is Pauli x ma- After we take a strong projective measurement of the trix, i.e., polarization degree of the beam with posts-elected state |ψf i = |Hi, the above total system state gives us the 0 1 final state of the pointer, and its normalized expression  = σ̂x = |HihV | + |V ihH| = (2) reads as 1 0 κ h s s i Here, |Hi ≡ (1, 0)T and |V i ≡ (0, 1)T represent the hori- |Φi = √ (1 + hσx iw ) D + (1 − hσx iw ) D − |φi. 2 2 2 zontal and vertical polarization of the beam, respectively. (8) We also assume that in our scheme the pointer and mea- Here, surement system are initially prepared to s2 κ−2 = 1 +|hσx i|2 + γ 2 e− 2 Re[(1 + hσx i∗w )(1 −hσx iw )× † 1 |φi = γa |αi, γ=p (3) (γ −2 − s2 + αs − α∗ s)e2si=(α) ] (9) 1 + |α|2
3 is the normalization coefficient, and the weak value of the of the field mode amplitude can be defined by operators system observable σ̂x is given by Xθ and Yθ as [64] hψf |σx |ψi i ϕ 1 ae−iθ + a† eiθ hσx iw = = eiδ tan . (10) Xθ ≡ (11) hψf |ψi i 2 2 In general, the expectation value of σx is bounded −1 ≤ and hσx i ≤ 1 for any associated system state. However, as 1 2 −iθ + a†2 eiθ , we see in Eq. (10), the weak values of the observable σx Yθ ≡ a e (12) 2 can take arbitrary large numbers with small successful post-selection probability Ps = |hψf |ψi i|2 = cos2 ϕ2 . This respectively. For these operators, if 4Xθ ≡ Xθ − hXθ i, weak value feature is used to amplify very weak but useful 4Yθ ≡ Yθ − hYθ i, the minimum variances are [65] information on various of related physical systems. The state given in Eq. ( 8) is a spoiled version of 1 1 † h(4Xθ )2 imin = ha ai − |hai|2 − |ha2 i − hai2 | + SPACS after postselected measurement. In the next sec- 4 2 tions, we study squeezing effects, and nonclassicality fea- (13) tures characterized by the Wigner function. 1 h(4Yθ )2 imin = ha† a + i (14) 2 III. ORDINARY AND AMPLITUDE SQUARE 1 †2 2 ha a i − |ha2 i|2 − |ha4 i − ha2 i2 | SQUEEZING + 2 where a and a† are annihilation and creation operators In this section, we check the ordinary (first-order) and of the radiation field. If h(4Xθ )2 imin < 41 , Xθ is said to ASS (second order) squeezing effects of SPACS after be ordinary squeezed and if h(4Yθ )2 imin < ha† a + 21 i, Yθ postselected von Neumann measurement.The squeezing is said to be ASS. These conditions can be rewritten as effect is one of the non-classical phenomena unique to the quantum light field. The squeezing reflects the non- Sos = ha† ai − |hai|2 − |ha2 i − hai2 | < 0 (15) classical statistical properties of the optical field by a noise component lower than that of the coherent state. In other words, the noise of an orthogonal component of the squeezed light is lower than the noise of the corre- Sass = ha†2 a2 i − |ha2 i|2 − |ha4 i − ha2 i2 | < 0. (16) sponding component of the coherent state light field. In practice, if this component is used to transmit informa- Thus, the system characterized by any wave function may tion, a higher signal-to-noise ratio can be obtained than exhibit non-classical features if it satisfies Eqs. (15-16). that of the coherent state. Consider a single mode of To achieve our goal, we first have to calculate the above electromagnetic field of frequency ω with creation and related quantities and their explicit expressions under the annihilation operator a† ,a. The quadrature and square state |Φi.these are listed below. 1.The expectation value ha† ai under the state |Ψi is given by ∗ ha† ai = |κ|2 |1 + hσx iw |2 t1 (s) + |1 − hσx iw |2 t1 (−s) + 2Re[(1 − hσx iw ) (1 + hσx iw ) t3 (s)] (17) where s2 t1 (s) = γ 2 2 + |α|4 + s|α|2 Re(α) + 3αα∗ + 1 + 4 and 1 2 2isIm(α) − s2 t3 (s) = γ e e 2 (4|α|4 − 6sα|α|2 + 2(6αα∗ + sα∗2 (3α + s) 4 + sRe(α)(8 − 9sα − 3s2 )) + 11α2 s2 + s4 + 6αs3 − 5s2 − 16αs + 4) respectively. 2.The expectation value hai under the state |Ψi is given by
4 s s hai = |κ|2 γ 2 {|1 + hσx iw |2 2α + α|α|2 + 2 + |1 − hσx iw |2 2α + α|α|2 − 2 2γ 2γ ∗ ∗ + (1 − hσx iw ) (1 + hσx iw ) w1 (s) + + (1 + hσx iw ) (1 − hσx iw ) w1 (−s)]} (18) where 1 2isIm(α) − s2 e 2 4α + α∗ (s − 2α)(s − α) + 2α2 s + s3 − 3αs2 − 3s w1 (s) = e 2 3.The expectation value ha2 i under the state |Ψi is given by ∗ ha2 i = |κ|2 {|1 + hσx iw |2 q1 (s) + |1 − hσx iw |2 q1 (−s) + (1 − hσx iw ) (1 + hσx iw ) q2 (s) ∗ + (1 + hσx iw ) (1 − hσx iw ) q2 (−s)} (19) where 1 2 q1 (s) = γ (2α + s)(6α + |α|2 (2α + s) + s) 4 and 1 s2 q2 (s) = − e2isIm(α) e− 2 γ 2 (s − 2α)(6α + α∗ (s − 2α)(s − α) + 2α2 s + s3 − 3αs2 − 5s) 4 respectively. 4.The expectation value ha†2 a2 i under the state |Ψi is given by ∗ ha†2 a2 i = |κ|2 {|1 + hσx iw |2 f1 (s) + |1 − hσx iw |2 f2 (−s) + 2Re[(1 − hσx iw ) (1 + hσx iw ) f3 (s)]} (20) where 1 2 f1 (s) = γ (2|α|6 + s|α|2 ((s2 + 16)Re(α) + sRe(α2 )) + 2|α|4 (2sRe(α) + s2 + 5) 2 s4 + 8α∗ α + 6s2 α∗ α + (2s3 + 8s)Re(α) + 3s2 Re(α2 )) + + γ 2 s2 16 and 1 f3 (s) = − γ 2 (s − 2α) (2α∗ + s) 16 2 1 2 (α∗ ) (s − 2α)(s − α) + 20|α|2 + 3sα∗ (s − 2α)(s − α) + 28isIm(α) + s2 2α2 + s2 − 3αs − 9 + 16e− 2 s(s−4iIm[α]) respectively. 5.The expectation value ha4 i under the state |Ψi is given by ha4 i = |κ|2 {|1 + hσx iw |2 h1 (s) + |1 − hσx iw |2 h1 (−s) + (1 + hσx iw )∗ (1 − hσx iw )h2 (s) (21) ∗ + (1 + hσx iw ) (1 − hσx iw ) h2 (−s)} (22) where 1 h1 (s) = (8αγ 2 |α|2 (α + s)(2α2 + s2 + 2αs) + s4 + 8αγ 2 (10α3 + 2s3 + 9αs2 + 16α2 s)) 16 and 1 2 2isIm(α) − s2 h2 (s) = − γ e e 2 (s − 2α)3 (10α + α∗ (s − 2α)(s − α) + 2α2 s + s3 − 3αs2 − 9s) 16 respectively. Using the expression for Sos , the curves for this quan- tity are plotted, and the analytical results are shown in
5 Ordinary squeezing 0.4 0.6 φ π φ 5π (a) 9 9 φ 3π 9 φ 7π 9 15 (a) 0 0.4 -0.4 -0.8 ASS 10 0 0.5 1 0.2 0.0 5 =π φ= 5 π 9 9 φ= 3 π φ= 7 π -0.2 0 9 9 0 1 2 3 4 5 0 1 2 3 4 5 s s 0.8 1 Ordinary squeezing (b) φ π 9 (b) 0.6 φ 3π 0 9 0.4 φ 5π 9 φ 7π -1 φ π 9 9 0.2 φ 3π -2 9 5π 0.0 φ 9 -3 φ 7π 9 -0.2 0.0 0.5 1.0 1.5 2.0 2.5 3.0 -4 0.0 0.5 1.0 1.5 2.0 2.5 3.0 r r Figure 1. (Color online) The effects of postselected von Neu- mann measurement on ordinary squeezing of SPACS. Fig. Figure 2. (Color online) The effects of postselected von 1(a) shows the quantity Sos as a function of coupling strength Neumann measurement on ASS of SPACS. (a) the Sass as a for different weak values with fixed coherent state parameter function of coupling strength s for different weak values with (r = 1). Fig. 1(b) shows quantity Sos as a function of co- fixed coherent state parameter r (r = 1); (b) the Sass as herent state parameter r for different weak values with fixed a function of coherent state parameter r for different weak coupling strength (s = 0.5). Here, we take θ = π4 , δ = π6 . values with fixed weak coupling strength s (s = 0.5). Other parameters are the same as those used in Fig. (1). Fig. 1. In Fig. 1(a), we fixed the parameter r = 1 and plot the Sos as a function of coupling strength s action strength is too large, the system is strongly mea- for different weak values quantified by ϕ. As we ob- sured and the size of the weak value has little impact on served, when there is no interaction between system and the squeezing effect.This statement can also be observed poiner (s = 0), there is no ordinary squeezing effect of in Fig. 1(a) and (b). In the weak measurement regime initial SPACS at the r = 1 point. However, in moderate the SPACS showed a good ordinary squeezing effect after coupling strength regions such as 0 < s 1) no
6 matter how large the value is taken. In order to further 1.0 investigate the ASS of the radiation field in the weak s=0 measurement regime, we plot the Sass as a function of 0.8 s=0.5 the coherent state parameter r for different weak values with s = 0.5. the analytical results are shown in Fig. 2b. 0.6 s=2 F We can see that when r is relatively small, there is an ASS effect no matter how large the weak value becomes. 0.4 By increasing the system parameter r, Sass takes nega- tive values and its negativity is proportional to r. From 0.2 Fig. 2a we can also observe that in the weak measure- 0.0 ment regime, the weak values have positive effects on the ASS of SPACS, and it can also be considered a result of 0 1 2 3 4 5 the weak signal amplification feature of the postselected r weak measurement technique. Figure 3. (Color online) The state distance between |Φi and initial SPACS |φi as a function of coherent state parameter IV. STATE DISTANCE AND WIGNER r for various coupling strengths. Here, we set values θ = π4 , FUNCTION δ = π6 , ϕ = 7π . 9 The postselected measurement taken on polarization degree of freedom of the beam could spoil the inherent where CN (λ) is the normal ordered characteristic func- properties presented in its spatial part. Before we inves- tion,and is defined as tigate the phase-space distribution of SPACS after post- h † ∗ i selected von Neumanm measurement, we check the sim- CW (λ) = T r ρeλa −λ a . (25) ilarity between the initial SPACS |φi and the state |Φi after measurement. The state distance between those Using the notation λ0 ,λ00 for the real and imaginary parts two states can be evaluated by of λ and setting z = x + ip to emphasize the analogy be- tween the radiation field quadratures and the normalized F = |hφ|Φi|2 , (23) dimensionless position and momentum observables of the and its value is bounded 0 ≤ F ≤ 1. If F = 1 (F = 0), beam in phase space. We can rewrite the definition of the then the two states are totally same (totally different). Wigner function in terms of x, p and λ0 , λ00 as The F in our case can be calculated after substituting Z +∞ equations Eq. (3)and Eq. (8) into the Eq. (23), and 1 0 00 W (x, p) = 2 e2i(pλ −xλ ) CW (λ)dλ0 dλ00 . (26) the analytical results are shown in Fig. 3. In Fig. 3 π −∞ we present the state distance F as a function of system parameter r for different coupling strengths with a fixed By substituting the final normalized pointer state |Φi large weak value. As shown in Fig. 3, in the weak cou- into Eq. (26), we can calculate the explicit expression of pling regime (s = 0.5), the state after the postselected its Wigner function and it reads as measurement maintains similarity with the the coherent 2|κ|2 2 state parameter r. However, with increasing the mea- W (z) = e−2|z−α| × surement strength, the initial state |φi is spoiled and the π(1 + |α|2 ) similarity between the pointer states before and after the {|1 + hσx iw |2 w(Γ) + |1 − hσx iw |2 w(−Γ) measurement is decreases. + 2 −1 + |2z − α|2 Re[(1 + hσx iw )∗ (1 − hσx iw )e2isIm[z] ]}. In order to further explain the squeezing effects of (27) SPACS after postselected von Neumann measurement, in the rest of this section we study the Wigner function with of |Φi. The Wigner distribution function is the closest 1 2 quantum analogue of the classical distribution function w(Γ) = e− 2 s e−2(Re[α]−Re[z])s × in phase space. According to the value of the Wigner s function we can intuitively determine the strength of its −1 + |2z − α|2 + 2s(Re[α] − 2Re[z] + ) (28) 2 quantum nature, and the negative value of the Wigner function proves the nonclassicality of the quantum state. This is a real Wigner function and its value is bounded The Wigner function exists for any state, and it is defined − π2 ≤ W (α) ≤ π2 in whole phase space. as the two-dimensional Fourier transform of the symmet- To depict the effects of the postselected von Neumann ric order characteristic function. Thus, the Wigner func- measurement on the non-classical feature of SPACS, in tion for the state ρ = |ΦihΦ| is written as [64] Fig. 4 we plot its curves for different parametric coherent Z +∞ state parameters r and coupling strengths s. Each col- 1 umn from left to right in-turn indicate the different coher- W (z) ≡ 2 exp(λ∗ z − λz ∗ )CW (λ)d2 λ, (24) π −∞ ent state parameters r for 0, 1 and 2, and each row from
7 Figure 4. (Color online) Wigner function of SPACS with changing parameters. Each column is defined for the different coherent state parameter α with r = 0, 1, 2, and are ordered accordingly from left to right. Figures (a) to (c) correspond to s = 0, (d) to (f) correspond to s = 0.5, and (g) to (k) correspond to s = 2. Other parameters are the same as those used in Fig. (3). up to down represent the different coupling strengths s SPACS and this kind of squeezing is pronounced with for 0, 0.5 and 2. It is observed that the positive peak of increasing coupling strength (see Figs. 4g-k ). Further- the Wigner function moves from the center to the edge more, in Figs. 4(g-k) we can see that in the strong mea- position in phase space and its shape gradually becomes surement regime significant interference structures man- irregular with changing coupling strength s. From the ifest and the negative regions become larger than the first row (see Figs. 4a-c ) we can see that the original initial pointer state. SPACS exhibit inherent features changing from single As mentioned above, the existence of and progressively photon state to coherent states with gradually increas- stronger negative regions of the Wigner function in phase ing coherent state parameter r. Figs. 4d-k indicate the space indicates the degree of nonclassicality of the associ- phase space density function W (z) after postselected von ated state. From the above analysis we can conclude that Neumann measurement. Fig. 4 d-f represent the Wigner after the postselected von Neumann measurement, the function for fixed weak interaction strength s = 0.5. It phase space distribution of SPACS is not only squeezed can be observed that the Wigner function distribution but the nonclassicality is also pronounced in the strong shows squeezing in phase space compared to the original measurement regime. V. CONCLUSION determined the final state of the pointer state along with the standard measurement process. We examined the or- In this paper we have studied the squeezing and dinary (first-order) and ASS effects after measurement, Wigner function of SPACS after postselected von Neu- and found that in the weak measurement region, the or- mann measurement. In order to achieve our goal, we first dinary squeezing and ASS of the light field increased sig-
8 nificantly as the weak value increased. in phase space. To further explain our work, we examined the similar- We anticipate that the theoretical scheme in this pa- ity between the initial SPACS and the state after mea- per may provide an effective method for solving practical surement. We observed that under weak coupling, the problems in quantum information processing associated state after the postselected measurement maintains sim- with SPACS. ilarity with the initial state. However, as the intensity of the measurement increases, the similarity between them gradually decreased and indicated that the measurement spoils the system state if the measurement is strong. We ACKNOWLEDGMENTS also investigate the Wigner function of the system after postselected measurement. It is observed that following This work was supported by the Natural Science Foun- the postselected von Neumann measurement, the phase dation of Xinjiang Uyghur Autonomous Region (Grant space distribution of SPACS is not only squeezed, but No. 2020D01A72), the National Natural Science Foun- also adevelops significant interference structures in the dation of China (Grant No. 11865017) and the Introduc- strongly measured regime. It also possess pronounced tion Program of High Level Talents of Xinjiang Ministry nonclassicality characterized with a large negative area of Science. [1] A. Mari and J. Eisert, Phys. Rev. Lett. 103, 213603 [23] S. L. Braunstein and H. J. Kimble, Phys. Rev. A 61, (2009). 042302 (2000). [2] Y. Yamamoto and H. A. Haus, Rev. Mod. Phys. 58, 1001 [24] V. Petersen, L. B. Madsen, and K. Mølmer, Phys. Rev. (1986). A 72, 053812 (2005). [3] H. Yuen and J. Shapiro, IEEE. T. Inform. Theory 26, 78 [25] J. Kempe, Phys. Rev. A 60, 910 (1999). (1980). [26] C. K. Hong and L. Mandel, Phys. Rev. A 32, 974 (1985). [4] S. L. Braunstein and H. J. Kimble, Phys. Rev. Lett. 80, [27] M. Hillery, Opt. Commun 62, 135 (1987). 869 (1998). [28] M. Hillery, Phys. Rev. A 36, 3796 (1987). [5] R. Lo Franco, G. Compagno, A. Messina, and A. Napoli, [29] C. Gerry and S. Rodrigues, Phys. Rev. A 35, 4440 (1987). Phys. Rev. A 76, 011804 (2007). [30] Xiaoping Yang and Xiping Zheng, Phys. Lett. A 138, 409 [6] R. L. Franco, G. Compagno, A. Messina, and A. Napoli, (1989). Int. J. Quantum. Inf 07, 155 (2009). [31] E. K. Bashkirov and A. S. Shumovsky, Int. J. Mod. Phys. [7] R. L. Franco, G. Compagno, A. Messina, and A. Napoli, B 4, 1579 (1990). Open. Syst. Inf. Dyn 13, 463 (2006). [32] M. H. Mahran, Phys. Rev. A 42, 4199 (1990). [8] R. Lo Franco, G. Compagno, A. Messina, and A. Napoli, [33] P. Marian, Phys. Rev. A 44, 3325 (1991). Phys. Rev. A 74, 045803 (2006). [34] M. A. Mir, Int. Journ. Mod. Phys. B 7, 4439 (1993). [9] R. Lo Franco, G. Compagno, A. Messina, and A. Napoli, [35] S.-d. Du and C.-d. Gong, Phys. Rev. A 48, 2198 (1993). Eur. Phys. J-Spec. Top 160, 247 (2008). [36] A. V. Chizhov, J. W. Haus, and K. C. Yeong, Phys. Rev. [10] R. Lo Franco, G. Compagno, A. Messina, and A. Napoli, A 52, 1698 (1995). Phys. Lett. A 374, 2235 (2010). [37] R. Lynch and H. A. Mavromatis, Phys. Rev. A 52, 55 [11] B. R. Mollow and R. J. Glauber, Phys. Rev. 160, 1076 (1995). (1967). [38] M. A. Mir, Int. J. Mod. Phys. B 12, 2743 (1998). [12] R. Slusher and B. Yurke, J. Lightwave. Technol 8, 466 [39] R.-H. Xie and S. Yu, J. Opt. B-Quantum. S. O 4, 172 (1990). (2002). [13] H. Yuen and J. Shapiro, IEEE. T. Inform. Theory 24, [40] R.-H. Xie and Q. Rao, Physica. A 312, 421 (2002). 657 (1978). [41] Z. Wu, Z. Cheng, Y. Zhang, and Z. Cheng, Physica. B [14] C. M. Caves, Phys. Rev. D 23, 1693 (1981). 390, 250 (2007). [15] G. J. Milburn and S. L. Braunstein, Phys. Rev. A 60, [42] E. K. BASHKIROV, Int.J. Mod. Phys.B 21, 145 (2007). 937 (1999). [43] D. K. Mishra, Opt. Commun 283, 3284 (2010). [16] B. Schumacher, Phys. Rev. A 54, 2614 (1996). [44] D. K. Mishra and V. Singh, Opt. Quant. Electron 52, 68 [17] B. Schumacher and M. A. Nielsen, Phys. Rev. A 54, 2629 (2020). (1996). [45] S. Kumar and D. K. Giri, J. Optics-UK 49, 549 (2020). [18] F.-l. Li, H.-r. Li, J.-x. Zhang, and S.-y. Zhu, Phys. Rev. [46] P. V. P. Pinheiro and R. V. Ramos, Quant. Infor. Proc A 66, 024302 (2002). 12, 537 (2013). [19] T. C. Zhang, K. W. Goh, C. W. Chou, P. Lodahl, and [47] Y. Wang, W.-S. Bao, H.-Z. Bao, C. Zhou, M.-S. Jiang, H. J. Kimble, Phys. Rev. A 67, 033802 (2003). and H.-W. Li, Phys. Lett. A 381, 1393 (2017). [20] B. Kraus, K. Hammerer, G. Giedke, and J. I. Cirac, [48] M. Miranda and D. Mundarain, Quant. Infor. Proc 16, Phys. Rev. A 67, 042314 (2003). 298 (2017). [21] A. Kitagawa and K. Yamamoto, Phys. Rev. A 68, 042324 [49] S. Srikara, K. Thapliyal, and A. Pathak, Quant. Infor. (2003). Proc 19, 371 (2020). [22] A. Dolińska, B. C. Buchler, W. P. Bowen, T. C. Ralph, [50] J.-R. Zhu, C.-Y. Wang, K. Liu, C.-M. Zhang, and and P. K. Lam, Phys. Rev. A 68, 052308 (2003). Q. Wang, Quant. Infor. Proc 17, 294 (2018).
9 [51] J.-J. Chen, C.-H. Zhang, J.-M. Chen, C.-M. Zhang, and [59] Y. Turek, Eur. Phys. J. Plus 136, 221 (2021). Q. Wang, Quant. Infor. Proc 19, 198 (2020). [60] von Neumann J, Mathematical Foundations of Quantum [52] Y. Aharonov, D. Z. Albert, and L. Vaidman, Phys. Rev. Mechanics (Princeton University Press, Princeton, NJ, Lett. 60, 1351 (1988). 1955). [53] K. Nakamura, A. Nishizawa, and M.-K. Fujimoto, Phys. [61] Y. Aharonov and A. Botero, Phys. Rev. A 72, 052111 Rev. A 85, 012113 (2012). (2005). [54] B. de Lima Bernardo, S. Azevedo, and A. Rosas, Opt. [62] A. Di Lorenzo and J. C. Egues, Phys. Rev. A 77, 042108 Commun 331, 194 (2014). (2008). [55] Y. Turek, H. Kobayashi, T. Akutsu, C.-P. Sun, and [63] A. K. Pan and A. Matzkin, Phys. Rev. A 85, 022122 Y. Shikano, New. J. Phys 17, 083029 (2015). (2012). [56] Y. Turek, W. Maimaiti, Y. Shikano, C.-P. Sun, and [64] G. Agarwal, Quantum Optics (Cambridge University M. Al-Amri, Phys. Rev. A 92, 022109 (2015). Press, Cambridge, England, 2013). [57] Y. Turek and T. Yusufu, Eur. Phys. J. D 72, 202 (2018). [65] P. Shukla and R. Prakash, Mod. Phys. Lett. B 27, [58] Y. Turek, Chin. Phys. B 29, 090302 (2020). 1350086 (2013).
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