Chinese Physics B, Volume. 29, Issue 9, (2020)

Effects of postselected von Neumann measurement on the properties of single-mode radiation fields

Yusuf Turek
Author Affiliations
  • School of Physics and Electronic Engineering, Xinjiang Normal University, Urumqi 830054, China
  • show less

    Postselected von Neumann measurement characterized by postselection and weak value has been found to possess potential applications in quantum metrology and solved plenty of fundamental problems in quantum theory. As an application of this new measurement technique in quantum optics and quantum information processing, its effects on the features of single-mode radiation fields such as coherent state, squeezed vacuum state and Schr?dinger cat sate are investigated by considering full-order effects of unitary evolution. The results show that the conditional probabilities of finding photons, second-order correlation functions, Qm-factors and squeezing effects of those states after the postselected measurement is significantly changed are comparable with the corresponding initial pointer states.

    Keywords

    1. Introduction

    Most researches in von Neumann type quantum measurement in recent years has focused on postseleceted weak measurement with sufficiently weak coupling between the measured system and pointer since it is useful to study the nature of the quantum world. This kind of postsselected weak measurement theory is originally proposed by Aharonov, Albert, and Vaidman in 1988,[1] and considered as a generalized version of standard von Neumann type measurement.[2] The result of weak coupling postselected weak measurement is called the “weak value”, and generally is a complex number. One of the special feature of the weak value is that it can take the values which lie beyond the normal eigenvalue range of corresponding observable, and this effect will be very clear if the pre- and post-selected states are almost orthogonal. This feature of the weak value is called the signal amplification property of postselected weak measurement and its first weak signal amplification property experimentally demonstrated in 1991.[3] After that, it has been widely used to elucidate tremendous fundamental problems in quantum mechanics. For details about the weak measurement and its applications in signal amplification processes, we refer the readers to the recent overview of the field.[4,5] As we mentioned earlier, in postselected weak measurement the interaction strength is weak, and it is enough to consider up to the first-order evolution of a unitary operator for the whole measurement processes. However, if we want to connect the weak and strong measurement, check to clear the measurement feedback of postselected weak measurement and analyze experimental results obtained in nonideal measurements, the full order evolution of a unitary operator will be needed.[68] We call this kind of measurement the postselected von Neumann measurement. We know that in some quantum metrology problems, the precision of the measurement depends on measuring devices and requires to optimize the pointer states. The merits of postselected von Neumann measurement can be seen in pointer optimization schemes.

    Recently, the state optimization problem in postselected von Neumann measurement has been presented widely, such as taking the Gaussian states,[4,9] Hermite–Gaussian or Laguerre–Gaussian states, and non-classical states.[10,11] The advantages of non-classical pointer states in increasing postselected measurement precision have been examined in recent studies.[10,12,13] Furthermore, in Ref. [14], the authors studied the effects of postselected measurement characterized by a modular value[15] to show the properties of semi-classical and non-classical pointer states considering the coherent, coherent squeezed, and Schrödinger cat state as a pointer. Since in their scheme the pointer operator is a projection operator onto one of the states of the basis of the pointer's Hilbert space and interaction strength only has taken one definite value, it cannot completely describe the effects of postselected measurement on the properties of the radiation field. However, to the knowledge of the author, the issue related to the study of the effects of postselected von Neumann measurement considering all interaction strengths to the inherent properties such as photon distribution, photon statistics, and squeezing effects of radiation field have not been handled and need to be investigated.

    Furthermore, the above-mentioned properties of quantum radiation fields have many useful technological applications in quantum optics and quantum information processing such as single photon generation and detection,[16] gravitational wave detection,[17,18] quantum teleportation,[1922] quantum computation,[23] generation and manipulation of atom–light entanglement,[2426] and precision measurements,[27] etc. We know that the realization of these processes depends on the optimization of the related input quantum states such as coherent state,[28] squeezed state[29,30] and Schrödinger cat state.[3133] As introduced in previous part, the postselected weak measurement technique has more advantages on signal optimization problem[34] and precision metrology[3543] than traditional measurement theory. Thus, the investigation of the effects of postselected von Neumann measurement on the statistical and squeezing properties of radiation fields is worth studying to optimize the related quantum states to provide more effective methods for the implementation of the above-mentioned technological processes.

    In this paper, motivated by the above-listed problems, we describe and examine the effects of postselected von Neumann measurement characterized by postselection and weak value on the properties of single-mode radiation fields. In order to achieve our goal, we choose the three typical states such as coherent state, squeezed vacuum state, and Schrödinger cat state as pointers and consider their polarization degree of freedom as a measured system, respectively. By taking full-order evolution of the unitary operator of our system, we separately study the photon distributions, statistical properties and squeezing effects of radiation fields and compare those with the initial state cases. To give more details about the effects of postselected von Neumann measurement on radiation fields, we plot more figures by considering all parameters that are related to the properties of those radiation fields, respectively. This study shows that the postselected measurement changes the properties of single-mode radiation fields dramatically for strong and weak measurement regimes with specific weak values. Especially the photon statistics and squeezing effect of coherent pointer state is too sensitive for the postselected von Neumann measurement processes.

    This paper is organized as follows: In Section 2, we describe the model of our theory by brief reviewing the postselected von Neumann measurement and outline the tasks we want to investigate. In Section 3, we separately calculate exact analytical expressions of photon distribution, second-order correlation function, Mandel factor and squeezing parameter of those three-pointers by taking into account the full-order evaluation of unitary operator under final states given after postselected measurement finished and present our main results. Finally, we summarize our findings of this study in Section 4.

    2. Model setup

    To build up our model, we begin to review some basic concepts of the von Neumann measurement theory. The standard measurement consists of three elements; measured system, pointer (measurement device or meter) and environment, which induce the interaction between the system and the pointer. The description of the measurement process can be written in terms of Hamiltonian, and the total Hamiltonian of a measurement composed of three parts:[44]

    $$ \begin{eqnarray}H={H}_{{\rm{s}}}+{H}_{{\rm{p}}({\rm{m}})}+{H}_{{\rm{int}}},\end{eqnarray}$$ (1)

    where Hs and Hp(m) represents the Hamiltonian of measured system and measuring device, respectively, and Hint is the interaction Hamiltonian between the measured system and the pointer. By considering the measurement efficiency and accuracy, in standard quantum measurement theory the interaction time between the system and the meter required to be too short so that the Hs and Hp(m) do not affect the final readout of the measurement result. Thus, in general, a measurement can only be described by the interaction part Hint of the total Hamiltonian, and it is taken to the standard von Neumann Hamiltonian as[2]

    $$ \begin{eqnarray}{H}_{{\rm{int}}}=g(t)\hat{A}\hat{P},\,\,\,\displaystyle {\int }_{{t}_{0}}^{t}g(t){\rm{d}}t=g\delta (t-{t}_{0}),\end{eqnarray}$$ (2)

    where A^ represents the Hermitian operator corresponding to the observable of the system that we want to measure with A^|ϕn=an|ϕn, and P^ is the conjugate momentum operator to the position operator X^ of the pointer, i.e., [X^,P^]=iI^. The coupling g(t) is a nonzero function in a finite interaction time interval tt0.

    One can express the position X^ and momentum operator P^ of the pointer using the annihilation a^ and creation operator a^ (satisfying [a^,a^]=1) as[45]

    $$ \begin{eqnarray}\begin{array}{lll}\hat{X} & = & \sigma ({\hat{a}}^{\dagger }+\hat{a}),\end{array}\end{eqnarray}$$ (3)

    $$ \begin{eqnarray}\begin{array}{lll}\hat{P} & = & \frac{{\rm{i}}}{2\sigma }({\hat{a}}^{\dagger }-\hat{a}),\end{array}\end{eqnarray}$$ (4)

    where σ is the width of the beam. The Hamiltonian Hint can be rewritten in terms of a and a as Hint=ig(t)2σA^(aa). If the Hermitian operator A^ satisfies the property A^2=I^, then the unitary evolution operator eit0tHintdτ of our coupling system can be given by

    $$ \begin{eqnarray}{{\rm{e}}}^{-{\rm{i}}g\hat{A}\otimes \hat{P}}=\frac{1}{2}(\hat{I}+\hat{A})\otimes D\left(\frac{s}{2}\right)+\frac{1}{2}(\hat{I}-\hat{A})\otimes D\left(-\frac{s}{2}\right),\end{eqnarray}$$ (5)

    where s is defined by s: ≡ g/σ, and D(s2) is a displacement operator and its expression can be written as D(s2)=es2(a^a^). We must note that s characterizes the measurement strength, and s ≪ 1 (s > 1) corresponds to weak (strong) measurement regimes.

    Assume that the system initially prepared in the state |ψi〉 and the initial pointer state is |ϕ〉, then after interaction we project the state eit0tHintdτ|ψi|ϕ onto the postselected system state |ψf〉, we can obtain the final state of the pointer. Furthermore, the normalized final state of the pointer can be written as

    $$ \begin{eqnarray}\begin{array}{lll}|\varPhi \rangle & = & {\mathscr{N}}\left[\frac{1}{2}(\hat{I}+{\langle A\rangle }_{w})\otimes D\left(\frac{s}{2}\right)\right.\\ & & \left.+\frac{1}{2}(\hat{I}-{\langle A\rangle }_{w})\otimes D\left(-\frac{s}{2}\right)\right]|\phi \rangle.\end{array}\end{eqnarray}$$ (6)

    Here N is the normalization coefficient of |Φ〉, and

    $$ \begin{eqnarray}{\langle A\rangle }_{{\rm{w}}}=\frac{\langle {\psi }_{{\rm{f}}}|\hat{A}|{\psi }_{{\rm{i}}}\rangle }{\langle {\psi }_{{\rm{f}}}|{\psi }_{{\rm{i}}}\rangle }\end{eqnarray}$$ (7)

    is called the weak value of Hermitian operator A^. From Eq. (6), we know that when the preselected state |ψi〉 and the postselected state |ψf〉 of the system are almost orthogonal, the absolute value of the weak value can be arbitrarily large and can be beyond the eigenvalue region of observable A. This feature leads to weak value amplification of weak signals and solving a lot of important problems in physics.

    In this study, we take the transverse spatial degree of freedom of single-mode radiation field as pointer and its Hamiltonian Hm(p) is related to the generating processes of single mode radiation fields such as coherent state, squeezed vacuum state and Schrödinger cat state, etc. The polarization degree of freedom of single mode radiation field is taken to be the measured system, and its Hamiltonian Hs is related to the polarization of the beam. Based on the basic requirements of quantum measurement theory,[44] the Hs and Hm(p) do not affect our measurement results. Thus, in our current research, it is not necessary to give the explicit expressions of the system and meter in hereafter. We suppose that the operator to be observed is the spin x component of a spin-1/2 particle, i.e.,

    $$ \begin{eqnarray}A={\sigma }_{x}=|{\uparrow }_{z}\rangle \langle {\downarrow }_{z}|+|{\downarrow }_{z}\rangle \langle {\uparrow }_{z}|,\end{eqnarray}$$ (8)

    where |↑z〉 and 〈z| are eigenstates of the z-component of spin, σz, with the corresponding eigenvalues 1 and –1, respectively. We assume that the pre- and post-selected states of measured system are

    $$ \begin{eqnarray}|{\psi }_{{\rm{i}}}\rangle =\cos \frac{\theta }{2}|{\uparrow }_{z}\rangle +{{\rm{e}}}^{{\rm{i}}\phi }\sin \frac{\theta }{2}|{\downarrow }_{z}\rangle,\end{eqnarray}$$ (9)

    and

    $$ \begin{eqnarray}|{\psi }_{{\rm{f}}}\rangle =|{\uparrow }_{z}\rangle,\end{eqnarray}$$ (10)

    respectively, and the corresponding weak value, Eq. (6), reads

    $$ \begin{eqnarray}{\langle {\sigma }_{x}\rangle }_{{\rm{w}}}={{\rm{e}}}^{{\rm{i}}\phi }\tan \frac{\theta }{2},\end{eqnarray}$$ (11)

    where θ∈[0,ψ] and φ∈[0,2π). In our system, the post-selection probability is Ps=cos2θ2. Note that throughout the rest of this study we will use this weak value for our purposes.

    Furthermore, we take the initial pointer state |ϕ〉 as a coherent state, squeezed vacuum state and Schrödinger cat state to study the effects of postselected measurement on the properties of those pointers, respectively. To achieve our goal: We study the conditional probability of finding n photons after postselected measurement. For the state |Φ〉, the conditional probability of finding n photons can be calculated by Ppost(n)=|n|Φ|2, and we compare it with the probability P(n) = |〈 n|ϕ〉|2 of initial pointer state |ϕ〉.We investigate the second-order correlation function g(2)(0) and Mandel factor Qm for the |Φ〉 state. The second-order correlation function of a single-mode radiation field is defined as g(2)(0)=aaaaaa2, and the Mandel factor Qm of the radiation field can be expressed in terms of g(2)(0) as Qm=n[g(2)(0)1]. If 0 ≤ g(2)(0) < 1 and –1 ≤ Qm < 0 simultaneously, the corresponding radiation field has sub-Poissonian statistics and more nonclassical. We have mention that the quantity Qm can never be smaller than –1 for any radiation field, and negative Qm values, which are equivalent to sub-poissonian statistics, cannot be produced by any classical field.[46]We check the squeezing parameter of single-mode radiation field for the |Φ〉 state. The squeezing parameter of the single-mode radiation field reads[47]Sϕ=:Xϕ2:Xϕ2, where Xϕ=12(aeiϕ+aeiϕ),[Xϕ,Xϕ+π2]=i is the quadrature operator of the field, and :: stands for the normal ordering of the operator defined by :aa: = aa, whereas aa = aa + 1. We can see that Sθ is related to the variance of Xθ, i.e., Sϕ=(ΔXϕ)212, where ΔXϕ=Xϕ2Xϕ2. The minimum value of Sϕ is –1/2 and for a nonclassical state Sϕ∈[–1/2,0).

    In the next section, we will study the above properties of three typical radiation fields by taking into the postselected measurement with arbitrary interaction strengths and weak values, respectively.

    3. Effects of postselected measurement to typical single-mode radiation fields

    In this section, we study the statistical properties and squeezing effects of typical single-mode radiation fields such as a coherent state, squeezed vacuum state and Schrödinger cat state, respectively, and compare the results with the corresponding initial state’s case.

    3.1. Coherent state

    The coherent state is typical semi-classical, quadrature minimum-uncertainty state for all mean photon numbers. The coherent state was originally introduced by Schrödinger in 1926 as a Gaussian beam to describe the evolution of a harmonic oscillator,[48] and the mathematical formulation of coherent state (also called Glauber state) has been introduced by Glauber in 1963.[28] Coherent states play an important role in representing quantum dynamics, especially when the quantum evolution is close to classical.[49,50] Here we take the coherent state as initial pointer state[51]

    $$ \begin{eqnarray}|\alpha \rangle =D(\alpha )|0\rangle,\end{eqnarray}$$ (18)

    where D(α) = eαa†α*a, and α = rei ϑ is an arbitrary complex number. After unitary evolution given in Eq. (4), the total system state is post-selected to |ψf〉, then we obtain the following normalized final state of coherent pointer state:

    $$ \begin{eqnarray}\begin{array}{lll}|\varPsi \rangle & = & \frac{\lambda }{\sqrt{2}}\left[\left(1+{\langle A\rangle }_{{\rm{w}}}\right){{\rm{e}}}^{-{\rm{i}}\frac{s}{2}{\rm{Im}}(\alpha )}|\alpha +\frac{s}{2}\rangle\right. \\ & & \left.+(1-{\langle A\rangle }_{{\rm{w}}}){{\rm{e}}}^{{\rm{i}}\frac{s}{2}{\rm{Im}}(\alpha )}|\alpha -\frac{s}{2}\rangle \right],\end{array}\end{eqnarray}$$ (19)

    where the normalization coefficient is given as

    $$ \begin{eqnarray}\begin{array}{lll}{\lambda }^{-2} & = & 1+|{\langle A\rangle }_{{\rm{w}}}{|}^{2}+{{\rm{e}}}^{-\frac{1}{2}{s}^{2}}(1+|{\langle A\rangle }_{{\rm{w}}}{|}^{2}\\ & & +2{\rm{Re}}{\langle A\rangle }_{{\rm{w}}})\cos (2s{\rm{Im}}(\alpha )),\end{array}\end{eqnarray}$$ (20)

    and Im (Re) represents the imaginary (real) part of a complex number.

    The conditional probability of finding n photons after taking a postselected measurement for state |Ψ〉 is obtained from Eq. (11) by changing |Φ〉 to a specific normalized state |Ψ〉. We plot the conditional probability of finding n photons under the normalized state |Ψ〉 and the analytical results are shown in Fig. 1. As indicated in Fig. 1, the black solid line represents the photon distribution probability for the initial state of coherent pointer state before postselected measurement, and it has a Poisson probability distribution. However, as shown in Fig. 1 the postselected measurement can change the photons Poisson distribution with increasing the weak value and changing the interaction strength s. Furthermore, from Fig. 1(a) we can know that Pcoh(n) is larger, in the postslected case for some small photon number regions rather than the no interaction case.

    Photon distribution Pcoh(n) of coherent state as a function of photon number n for ϑ = π/3, φ = π/4, r = 1. (a) Pcoh(n) plotted for s = 2, and for various weak values (〈σx〉w = eiπ/3 tanθ/2) in the no interaction case (black curve). (b) Pcoh(n) plotted for θ = 7π/9, and for various coupling strength s.

    Figure 1.Photon distribution Pcoh(n) of coherent state as a function of photon number n for ϑ = π/3, φ = π/4, r = 1. (a) Pcoh(n) plotted for s = 2, and for various weak values (〈σxw = eiπ/3 tanθ/2) in the no interaction case (black curve). (b) Pcoh(n) plotted for θ = 7π/9, and for various coupling strength s.

    For coherent state |α〉 (Eq. (17)) the second-order correlation function g(2)(0) is equal to one, i.e., g(2)(0) = 1 and the Mandel factor is equal to zero. Now we will calculate the gcoh(2)(0) and Qm,coh considering the final pointer state |Ψ〉 for the coherent pointer state. The expectation value of the photon number operator n^=aa under the state |Ψ〉 is

    $$ \begin{eqnarray}\begin{array}{lll}{\langle n\rangle }_{\varPsi } & = & \frac{|\lambda {|}^{2}}{4}\left\{{\left|1+{\langle A\rangle }_{{\rm{w}}}\right|}^{2}{\left|\alpha +\frac{s}{2}\right|}^{2}+{\left|1-{\langle A\rangle }_{{\rm{w}}}\right|}^{2}{\left|\alpha -\frac{s}{2}\right|}^{2}\right.\\ & & +2{{\rm{e}}}^{-\frac{{s}^{2}}{2}}{\rm{Re}}\left[{{\rm{e}}}^{2{\rm{i}}s{\rm{Im}}(\alpha )}(1-|{\langle A\rangle }_{{\rm{w}}}{|}^{2}-2{\rm{i}}\,{\rm{Im}}{\langle A\rangle }_{{\rm{w}}}))\right.\\ & & \left.\left.\times {\left(\alpha +\frac{s}{2}\right)}^{\ast }(\alpha -\frac{s}{2})\right]\right\}.\end{array}\end{eqnarray}$$ (21)

    If we take s = 0, then 〈 ns = 0 = |α|2. This is the photon number for the initial coherent state |α〉. We can also obtain the expectation value of a2a2 as

    $$ \begin{eqnarray}\begin{array}{lll}{\langle {a}^{\dagger 2}{a}^{2}\rangle }_{\varPsi } & = & \,\frac{|\lambda {|}^{2}}{4}\left\{|1+{\langle A\rangle }_{{\rm{w}}}{|}^{2}|\alpha +\frac{s}{2}{|}^{4}+|1-{\langle A\rangle }_{{\rm{w}}}{|}^{2}|\alpha -\frac{s}{2}{|}^{4}\right.\\ & & +2{{\rm{e}}}^{-\frac{{s}^{2}}{2}}{\rm{Re}}\left[{{\rm{e}}}^{2{\rm{i}}s|\alpha |\sin \phi }\left(1+{\langle A\rangle }_{{\rm{w}}}^{\ast }\right)(1-{\langle A\rangle }_{{\rm{w}}})\right.\\ & & \left.\left.\times {(\alpha +\frac{s}{2})}^{\ast 2}{(\alpha -\frac{s}{2})}^{2}\right]\right\}.\end{array}\end{eqnarray}$$ (22)

    If we take s = 0, it will give the value under the initial state |α〉, i.e., 〈 aaaas = 0 = |α|4. By substituting the above expressions to Eqs. (12) and (13), we obtain the concrete expressions of gcoh(2)(0) and Qm,coh. To investigate the effect of postselected measurement on the photon statistical properties of coherent state we plot the analytical figures of gcoh(2)(0) and Qm,coh, and the results are shown in Fig. 2.

    Second-order correlation function gcoh(2)(0) and Mandel factor Qm,coh for the coherent state after postselected measurement. Here φ = 4π/5, ϑ = π/3. gcoh(2)(0) vs. coherent state parameter r for different interaction strength s (black sold line represents the initial coherent state |α〉) and for (a) θ = π/3, or (b) θ = 7π/9. The Mandel factor Qm,coh plotted as a function of the weak value for different r of coherent state and for (c) s = 0.2, or (d) s = 2.

    Figure 2.Second-order correlation function gcoh(2)(0) and Mandel factor Qm,coh for the coherent state after postselected measurement. Here φ = 4π/5, ϑ = π/3. gcoh(2)(0) vs. coherent state parameter r for different interaction strength s (black sold line represents the initial coherent state |α〉) and for (a) θ = π/3, or (b) θ = 7π/9. The Mandel factor Qm,coh plotted as a function of the weak value for different r of coherent state and for (c) s = 0.2, or (d) s = 2.

    From Fig. 2 we can deduce that in postselected weak measurement region with large weak values (see the curves in Figs. 2(b) and 2(c)), the final state of the pointer state possesses sub-Poisson statistics (0 < g(2)(0) < 1 and –1 < Qm < 0). From Fig. 2(d), we can see that in strong postselected measurement, the system has super Poisson statistics (g(2)(0) > 1 and Qm > 0). Thus, the results summarized in Fig. 2 confirm that the postselected measurement can change the statistical properties of the coherent state significantly.

    Since the coherent state is a minimum uncertainty state, there is no squeezing effect for coherent state |α〉, i.e., Sϕ = 0. Next, we investigate the squeezing parameter Sϕcoh for |Ψ〉 of the coherent pointer state. The expectation value of Xϕ, coh under the state |Ψ〉 is given by

    $$ \begin{eqnarray}\begin{array}{lll}{\langle {X}_{\phi,{\rm{coh}}}\rangle }_{\varPsi } & = & \frac{|\lambda {|}^{2}}{\sqrt{2}}\left\{(1+|{\langle A\rangle }_{{\rm{w}}}{|}^{2})|\alpha |\cos (\phi -\theta )+s\cos \phi \,{\rm{Re}}[{\langle A\rangle }_{{\rm{w}}}]+\frac{1}{2}{{\rm{e}}}^{-\frac{1}{2}{s}^{2}}{\rm{Re}}[{{\rm{e}}}^{2{\rm{i}}s{\rm{Im}}(\alpha )}(1-{\langle A\rangle }_{{\rm{w}}})(1+{\langle A\rangle }_{{\rm{w}}}^{\ast })\right.\\ & & \times (2r\cos (\theta -\phi )+{\rm{i}}s\sin \phi )].\end{array}\end{eqnarray}$$ (23)

    If s = 0, then the above expression will reduce to the expectation value of Xϕ under the initial coherent pointer state |α〉, i.e., 〈 Xϕ, ohs = 0 = Re [α e−i ϕ]. The expectation value of Xϕ,coh2 with |Ψ〉 is given by

    $$ \begin{eqnarray}\begin{array}{lll}{\langle {X}_{\phi,{\rm{coh}}}^{2}\rangle }_{\varPsi } & = & \frac{1}{2}\left\langle (a{{\rm{e}}}^{-{\rm{i}}\phi }+{a}^{\dagger }{{\rm{e}}}^{{\rm{i}}\phi })(a{{\rm{e}}}^{-{\rm{i}}\phi }+{a}^{\dagger }{{\rm{e}}}^{{\rm{i}}\phi })\right\rangle \\ & = & \frac{1}{2}\left[\langle {a}^{2}\rangle {{\rm{e}}}^{-2{\rm{i}}\phi }+\langle {a}^{\dagger 2}\rangle {{\rm{e}}}^{2{\rm{i}}\phi }+2\langle {a}^{\dagger }a\rangle +1\right]\\ & = & \frac{1}{2}\left[2{\rm{Re}}[\langle {a}^{2}\rangle {{\rm{e}}}^{-2{\rm{i}}\phi }]+2\langle n\rangle +1\right],\end{array}\end{eqnarray}$$ (24)

    where

    $$ \begin{eqnarray}\begin{array}{lll}\langle {a}^{2}\rangle & = & \frac{|\lambda {|}^{2}}{4}\left\{|1+{\langle A\rangle }_{{\rm{w}}}{|}^{2}{\left(\alpha +\frac{s}{2}\right)}^{2}\right.\\ & & +{\left|1-{\langle A\rangle }_{{\rm{w}}}\right|}^{2}{\left(\alpha -\frac{s}{2}\right)}^{2}\\ & & +{{\rm{e}}}^{2{\rm{i}}s{\rm{Im}}(\alpha )}{{\rm{e}}}^{-\frac{{s}^{2}}{2}}(1-{\langle A\rangle }_{{\rm{w}}})(1+{\langle A\rangle }_{{\rm{w}}}^{\ast }){(\alpha -\frac{s}{2})}^{2}\\ & & +\left.{{\rm{e}}}^{-2{\rm{i}}s{\rm{Im}}(\alpha )}{{\rm{e}}}^{-\frac{{s}^{2}}{2}}(1+{\langle A\rangle }_{{\rm{w}}})(1-{\langle A\rangle }_{{\rm{w}}}^{\ast }){\left(\alpha +\frac{s}{2}\right)}^{2}\right\}.\end{array}\end{eqnarray}$$ (25)

    The squeezing parameter Sϕ, coh of state |Ψ〉 can be obtained by substituting Eqs. (23) and (24) into Eq. (17), and its analytical results are given in Fig. 3.

    The squeezing parameter Sϕ,coh for the coherent state after postselected measurement. Here φ = 4π/5, ϑ = π/3. Sϕ, coh vs. interaction strength s for various r and P quadrature of the coherent state (ϕ = π/2), but with different weak values: (a) θ = π/9, (b) θ = 7π/9. (c) Sϕ, coh plotted as a function of interaction strength s for various r and for θ = π/9, ϕ = 0 (represents the X quadrature of coherent state). (d) Sϕ, coh vs. coherent state parameter r for different weak values and for ϕ = π/2, s = 2.

    Figure 3.The squeezing parameter Sϕ,coh for the coherent state after postselected measurement. Here φ = 4π/5, ϑ = π/3. Sϕ, coh vs. interaction strength s for various r and P quadrature of the coherent state (ϕ = π/2), but with different weak values: (a) θ = π/9, (b) θ = 7π/9. (c) Sϕ, coh plotted as a function of interaction strength s for various r and for θ = π/9, ϕ = 0 (represents the X quadrature of coherent state). (d) Sϕ, coh vs. coherent state parameter r for different weak values and for ϕ = π/2, s = 2.

    We can observe from Fig. 3 that after postselected measurement the squeezing parameter of the initial coherent state changes dramatically, and we can see the phase-dependent squeezing effect. The X quadrature (ϕ = 0) of the final state is not squeezed (see Fig. 3(c)), but P quadrature (ϕ=π2) of the final state has a squeezing effect for moderate interaction strengths (see Figs. 3(a), 3(b), and 3(d)) with any weak values.

    3.2. Squeezed vacuum state

    Our second pointer state is the squeezed vacuum state. Squeezed states of the radiation field are generated by degenerate parametric down-conversion in an optical cavity.[52] The squeezed state have important applications in many quantum information processing tasks, including gravitational wave detection,[18,17] quantum teleportation.[19,20] Suppose that a measuring device can be initially prepared in the squeezed vacuum state[51] defined by

    $$ \begin{eqnarray}|\xi \rangle =S(\xi )|0\rangle,\end{eqnarray}$$ (26)

    where S(ξ)=exp(12ξa212ξa2), and ξ = η ei δ is an arbitrary complex number with modulus η and argument δ ∈ [0,2π]. As indicated in Eq. (26), the squeezed vacuum state is generated by the action on the vacuum state |0〉 of the squeezing operator S(ξ). After the postselected measurement processes as outlined in Section 2, the normalized final pointer state can be written as

    $$ \begin{eqnarray}|\phi \rangle =\frac{\kappa }{2}\left[\left(1+{\langle A\rangle }_{{\rm{w}}}\right)|\xi,\frac{s}{2}\rangle +(1-{\langle A\rangle }_{{\rm{w}}})|\xi,-\frac{s}{2}\rangle \right],\end{eqnarray}$$ (27)

    where the normalization coefficient κ is given by

    $$ \begin{eqnarray}\begin{array}{lll}\kappa & = & \sqrt{2}\left[1+|{\langle A\rangle }_{{\rm{w}}}{|}^{2}+(1-|{\langle A\rangle }_{{\rm{w}}}{|}^{2})\right.\\ & & {\left.\times \exp \left(-\frac{1}{2}{s}^{2}{\left|\cosh \eta +{{\rm{e}}}^{{\rm{i}}\delta }\sinh \eta \right|}^{2}\right)\right]}^{-\frac{1}{2}}\end{array}\end{eqnarray}$$ (28)

    and we note that |ξ,±s2=D(±s2)S(ξ)|0 is a squeezed coherent state.

    The probability amplitude of finding n photons in a squeezed coherent state is given by

    $$ \begin{eqnarray}\begin{array}{l}&\langle n|\pm \frac{s}{2},\xi \rangle \\ =&\frac{1}{\sqrt{\cosh \eta }}\exp \left[-\frac{1}{2}{\left|\pm \frac{s}{2}\right|}^{2}-\frac{1}{2}{\left(\pm \frac{s}{2}\right)}^{\ast 2}{{\rm{e}}}^{{\rm{i}}\delta }\tanh \eta \right]\\ &\times \frac{{\left(\frac{1}{2}{{\rm{e}}}^{{\rm{i}}\delta }\tanh \eta \right)}^{\frac{n}{2}}}{\sqrt{n!}}{H}_{n}\left[\chi {({{\rm{e}}}^{{\rm{i}}\delta }\sinh (2r))}^{-\frac{1}{2}}\right]\end{array}\end{eqnarray}$$ (29)

    with χ=±s2coshη+(±s2)eiδsinhη. To find the conditional probability of n photons under the state |φ〉, we can use Eq. (12) by changing |Φ〉 to |φ〉, and use Eq. (29). The effects of postselected measurement to the probability of finding n photons for state |φ〉 is displayed in Fig. 4. The black thick curve in Fig. 4(a) corresponds to the conditional photon probability for the initial pointer state |ξ〉. As illustrated in Fig. 4, the postselected measurement can change the photon distribution of the field, and in fewer photon number region the Psq(n) with the state |φ〉 is larger than the no interaction case (see Fig. 4(a)). For definite squeeze parameter η and weak measurement region (s < 1) with large weak values, Pqs is larger than strong measurement region (s > 1), but its occurrence probability is small.

    Photon distribution Psq(n) of squeezed vacuum state after postselected measurement as a function of n. Here δ = π/3, φ = π/3, η = 0.5. (a) Psq(n) is plotted for s = 1, and for the no interaction case (black curve) and various weak values. (b) Psq(n) is plotted for θ = 7π/9, and for various interaction strength s.

    Figure 4.Photon distribution Psq(n) of squeezed vacuum state after postselected measurement as a function of n. Here δ = π/3, φ = π/3, η = 0.5. (a) Psq(n) is plotted for s = 1, and for the no interaction case (black curve) and various weak values. (b) Psq(n) is plotted for θ = 7π/9, and for various interaction strength s.

    The second-order correlation function g(2)(0) and the Mandel factor Qm of the initial squeezed vacuum pointer state |ξ〉 is given by

    $$ \begin{eqnarray}{g}^{(2)}(0)=3+\frac{1}{{\sinh }^{2}\eta }\end{eqnarray}$$ (30)

    and

    $$ \begin{eqnarray}{Q}_{{\rm{m}}}=1+2{\sinh }^{2}\eta,\end{eqnarray}$$ (31)

    respectively. It is clear that the number fluctuations of the squeezed vacuum pointer state initially are super-Poissonian, and for all values of η both g(2)(0) and Qm cannot take the values to possess the sub-Poissonian statistics, which is a nonclassical property of the field. Now, we study the effect of postselected measurement to g(2)(0) and Qm of the squeezed vacuum pointer state under the normalized final pointer state |φ〉. The expectation value of the photon number operator aa and the (aa)2 under the final state |φ〉 can be calculated, and their explicit expressions are given in Appendix A (since the expressions are too cumbersome to write here, we display them in the Appendix).

    The analytical results for gsq(2)(0) and Qm,sq under the state |φ〉 are presented in Fig. 5. It can be observed from Figs. 5(a) and 5(c) that both gsq(2)(0) and Qm,sq can take the values, in which only sub-Poisson radiation field can possess the region s ≳ 0.5 for large weak values. For definite measurement strength s and larger weak value, the value gsq(2)(0) is lower than one and the value of Qm,sq is less than zero when the squeezed state parameter η is less than one (see Figs. 5(b) and 5(d)). Thus, it is apparent that the postselected measurement dramatically changes the photon statistical properties of the initial squeezed pointer state |ξ〉.

    Second-order correlation function gsq(2)(0) and the Mandel factor Qm,sq of the squeezed vacuum state after postselected measurement. Here φ = π/3, δ = π/3: (a) gsq(2)(0) vs. interaction strength s for different weak values and for η = 0.2; (b) gsq(2)(0) plotted as a function of squeezed vacuum state parameter η for various interaction strengths and for θ = 7π/9; (c) Qm,sq vs. interaction strength s for different weak values and for η = 0.2; (d) Qm,sq plotted as a function of squeezed vacuum state parameter η for various interaction strengths and for θ = 7π/9. Inset: the enlarged curves in the interval η∈[0,0.5].

    Figure 5.Second-order correlation function gsq(2)(0) and the Mandel factor Qm,sq of the squeezed vacuum state after postselected measurement. Here φ = π/3, δ = π/3: (a) gsq(2)(0) vs. interaction strength s for different weak values and for η = 0.2; (b) gsq(2)(0) plotted as a function of squeezed vacuum state parameter η for various interaction strengths and for θ = 7π/9; (c) Qm,sq vs. interaction strength s for different weak values and for η = 0.2; (d) Qm,sq plotted as a function of squeezed vacuum state parameter η for various interaction strengths and for θ = 7π/9. Inset: the enlarged curves in the interval η∈[0,0.5].

    The squeezing parameter Sϕ of the initial squeezed vacuum state |ξ〉 can be calculated using Eqs. (14)–(16) and (33), and written as

    $$ \begin{eqnarray}{S}_{\phi }=\frac{1}{2}\left[{\cosh }^{2}\eta -\sinh (2\eta )\cos (2\phi -\delta )+{\sinh }^{2}\eta \right]{\rm{}}-\frac{1}{2}.\end{eqnarray}$$ (32)

    It is evident from Eq. (32) that the squeezing effect of the squeezed vacuum state is phase-dependent: (i) If ϕ=δ2, then Sϕ=12(1e2η), it has squeezing effect for η > 0. (ii) If ϕ=δ2+π2, then Sϕ=12(e2η1), there is no squeezing effect. This reveals that it spreads out the quadrature Xϕ=δ2 and at the same time squeezes the quadrature Xϕ=δ2+π2.

    The squeezing parameter Sϕ,sq of the final normalized state |φ〉 after postselected von-Nuemann measurement can be calculated as the same processes of the initial state |ξ〉, and the analytical results are shown in Fig. 6. According to Figs. 6(a) and 6(b), the postselected measurement would have a negative effect on the squeezing effect of the squeezed vacuum state since Sϕ,sq gradually becomes larger with increasing the measurement strength s. However, as indicated in Fig. 6(c), in weak measurement regime where 0 < s < 1, the postselected measurement still has the effects on squeezing of the squeezed vacuum pointer state. As mentioned above the squeezing effect of the squeezed vacuum state is phase-dependent, and the postselected measurement has no positive effect on the squeezing of Xϕ=π2 quadrature (see Fig. 6(d)).

    Squeezing parameter Sϕ,sq of the squeezed vacuum state after postselected measurement. Here φ = π/3. (a) Sϕ vs. η of the squeezed vacuum state for different interaction strength s and for δ = ϕ = 0, θ = π/9. (b) Sϕ,sq plotted as a function of ϕ for various interaction strength s and for η = 0.5,δ = π/3, and θ = π/9. Sϕ,sq vs. interaction strength s for different weak values and for δ = 0 and η = 0.5, but with different ϕ: (c) ϕ = 0, (d) ϕ=π2. Inset: the enlarged curves in the interval s ∈ (0,1].

    Figure 6.Squeezing parameter Sϕ,sq of the squeezed vacuum state after postselected measurement. Here φ = π/3. (a) Sϕ vs. η of the squeezed vacuum state for different interaction strength s and for δ = ϕ = 0, θ = π/9. (b) Sϕ,sq plotted as a function of ϕ for various interaction strength s and for η = 0.5,δ = π/3, and θ = π/9. Sϕ,sq vs. interaction strength s for different weak values and for δ = 0 and η = 0.5, but with different ϕ: (c) ϕ = 0, (d) ϕ=π2. Inset: the enlarged curves in the interval s ∈ (0,1].

    3.3. Schrödinger cat state

    In the above two subsections, we have already confirmed that postselected measurement characterized by a weak value can really change the statistical and squeezing effect of single-mode radiation fields. To further increase the reliability of our conclusions, in this subsection, we check the same phenomena by taking the Schrödinger cat state as a pointer. Schrödinger’s cat is a gedanken experiment in quantum physics, proposed by Schrödinger in 1935,[53] and its corresponding state is called the Schrödinger cat state. The Schrödinger cat state plays significant roles not only in fundamental tests of quantum theory,[5457] but also in many quantum information processing such as quantum computation,[23] quantum teleportation,[21,22] and precision measurements.[27] The Schrödinger cat state is composed by the superposition of two coherent correlated states moving in the opposite directions, and defined as[47]

    $$ \begin{eqnarray}|\varTheta \rangle =K\left(|\alpha \rangle +{{\rm{e}}}^{{\rm{i}}\omega }|-\alpha \rangle \right),\end{eqnarray}$$ (33)

    where

    $$ \begin{eqnarray}K={\left[2+2{{\rm{e}}}^{-2|\alpha {|}^{2}}\cos \omega \right]}^{-\frac{1}{2}}\end{eqnarray}$$ (34)

    is the normalization constant and α = r ei δ is a coherent state parameter with modulus r and argument δ. The normalized final state of the Schrödinger cat state after the postselected weak measurement is given by taking |ϕ〉 = |Θ〉 in Eq. (6), i.e.,

    $$ \begin{eqnarray}\begin{array}{lll}|\chi \rangle & = & \frac{\kappa }{2}\left[(1+{\langle A\rangle }_{{\rm{w}}})D(\frac{s}{2})\right.\\ & & \left.+(1-{\langle A\rangle }_{{\rm{w}}})D(-\frac{s}{2})\right]|\varTheta \rangle \end{array}\end{eqnarray}$$ (35)

    with the normalization coefficient

    $$ \begin{eqnarray}\begin{array}{lll}{\kappa }^{-2} & = & \frac{1}{2}(1+|{\langle A\rangle }_{{\rm{w}}}{|}^{2})+{K}^{2}(1-|{\langle A\rangle }_{{\rm{w}}}{|}^{2})\cos (2s{\rm{Im}}[\alpha ]){{\rm{e}}}^{-\frac{{s}^{2}}{2}}\\ & & +\frac{{K}^{2}}{2}{\rm{Re}}[(1-{\langle A\rangle }_{{\rm{w}}})(1+{\langle A\rangle }_{{\rm{w}}}^{\ast })\\ & & \times ({{\rm{e}}}^{{\rm{i}}\omega }{{\rm{e}}}^{-\frac{1}{2}|2\alpha +s{|}^{2}}+{{\rm{e}}}^{-{\rm{i}}\omega }{{\rm{e}}}^{-\frac{1}{2}|2\alpha -s{|}^{2}})].\end{array}\end{eqnarray}$$ (36)

    Here we must mention that ω ∈ [0,2π], and when ω = 0 (ω = π) it is called the even (odd) Schrödinger cat state. Similar to the previous two cases, the conditional probability Psh(n) of the Schrödinger cat state can be obtained by replacing the |ϕ〉 in Eq. (5) to |χ〉, and the analytical results of the even Schrödinger cat state is presented in Fig. 7. As shown in Fig. 7, the postselected measurement can change photon distribution of the field, and in fewer photon regions with large weak values, Psh(n) is larger than the initial photon distribution of the Schrödinger even cat state. By comparing Fig. 7 and Fig. 4 we can also obtain the same common sense that the even Schrödinger cat state has similar properties as a squeezed state.

    Photon distribution Psh(n) of the squeezed state as a function of photon number n. Here δ = π/3, φ = π/3, ω = 0, r = 0.5: (a) Psh(n) is plotted for s = 1, and for various weak values; (b) Psh(n) is plotted for θ = 7π/9, and for various interaction strength s.

    Figure 7.Photon distribution Psh(n) of the squeezed state as a function of photon number n. Here δ = π/3, φ = π/3, ω = 0, r = 0.5: (a) Psh(n) is plotted for s = 1, and for various weak values; (b) Psh(n) is plotted for θ = 7π/9, and for various interaction strength s.

    The Mandel factor and second-order correlation function for the Schrödinger cat state are given by

    $$ \begin{eqnarray}\begin{array}{ll}{Q}_{{\rm{m}}} & =\frac{4|\alpha {|}^{2}{{\rm{e}}}^{-2|\alpha {|}^{2}}\cos \omega }{1-{{\rm{e}}}^{-4|\alpha {|}^{2}}{\cos }^{2}\omega }\end{array}\end{eqnarray}$$ (37)

    and

    $$ \begin{eqnarray}{g}^{(2)}(0)=1+\frac{4{{\rm{e}}}^{-2|\alpha {|}^{2}}\cos \omega }{{(1-{{\rm{e}}}^{-2|\alpha {|}^{2}}\cos \omega )}^{2}},\end{eqnarray}$$ (38)

    respectively. It is apparent that both g(2)(0) and Qm have sub-Poisson statistics when cos ω < 0 (π2<ω<3π2).

    The gsh(2)(0) and Qm,sh of the Schrödinger cat state can be calculated using Eqs. (13) and (14) with the normalized final pointer state |χ〉. As indicated in Fig. 8, after postselected measurement, the statistical property of the Schrödinger cat state changes from sub-Poisson to super-Poisson gradually with increasing the interaction strength and weak value. However, as we can see from Figs. 8(b) and 8(d), in the postselected weak measurement regime, where 0 < s < 1, we can achieve the best performance for nonclassicality of the odd Schrödinger cat state with small coherent state modulus r.

    Second-order correlation function gsh(2)(0) and Mandel factor Qm,sh of the Schrödinger state after postselected measurement. Here φ = 0, δ = 0: (a) gsh(2)(0) plotted as a function ω of the Schrödinger cat state for various interaction strength s and for θ = π/9, r = 0.3; (b) gsh(2)(0) vs. parameter r of the Schrödinger cat state for different weak values and for s = 0.5, ω = ω; (c) Qm,sh plotted as a function ω of the Schrödinger cat state for various interaction strength s and for θ = π/9, r = 0.3; (d) Qm,sh vs. parameter r of the Schrödinger cat state for different weak values and for s = 0.5, ω = π.

    Figure 8.Second-order correlation function gsh(2)(0) and Mandel factor Qm,sh of the Schrödinger state after postselected measurement. Here φ = 0, δ = 0: (a) gsh(2)(0) plotted as a function ω of the Schrödinger cat state for various interaction strength s and for θ = π/9, r = 0.3; (b) gsh(2)(0) vs. parameter r of the Schrödinger cat state for different weak values and for s = 0.5, ω = ω; (c) Qm,sh plotted as a function ω of the Schrödinger cat state for various interaction strength s and for θ = π/9, r = 0.3; (d) Qm,sh vs. parameter r of the Schrödinger cat state for different weak values and for s = 0.5, ω = π.

    The squeezing parameter of the initial Schrödinger cat state |Θ〉 reads[47]

    $$ \begin{eqnarray}\begin{array}{lll}{S}_{\phi }^{{\rm{i}}n} & = & \frac{|\alpha {|}^{2}{{\rm{e}}}^{-4|\alpha {|}^{2}}}{{(1+{{\rm{e}}}^{-2|\alpha {|}^{2}}\cos \omega )}^{2}}\\ & & \times [1+(\cos 2\phi {({{\rm{e}}}^{2|\alpha {|}^{2}}+\cos \omega )}^{2}\\ & & +{\sin }^{2}\omega {\cos }^{2}\phi -1)].\end{array}\end{eqnarray}$$ (39)

    From this expression, we can deduce that the squeezing effect of the initial Schrödinger cat state is also phase-dependent, similar to the squeezed vacuum state. The quadrature of the field will be squeezed only when the inequality cos2ϕ<sin2ωcos2ϕ1(cosω+e2|α|2)2 is satisfied. The details of this squeezing effect are presented in Fig. 9(a) (see the black solid curve).

    Squeezing parameter Sϕ, sh of the Schrödinger cat state. Here φ = 0, δ = 0, r = 0.3. Sϕ, sh of the even Schrödinger cat state (ω = 0) vs. the squeezing parameter angle ϕ for different interaction strength and for θ = π/9 in (a); for different weak values and for s = 0.5 in (b). (c) Sϕ, sh plotted as a function of ω for various weak values and for s = 0.5, ϕ = π/2. (d) Sϕ, sh of the odd Schrödinger cat state (ω = π) vs. the squeezing parameter angle ϕ for different interaction strength and for θ = π/9.

    Figure 9.Squeezing parameter Sϕ, sh of the Schrödinger cat state. Here φ = 0, δ = 0, r = 0.3. Sϕ, sh of the even Schrödinger cat state (ω = 0) vs. the squeezing parameter angle ϕ for different interaction strength and for θ = π/9 in (a); for different weak values and for s = 0.5 in (b). (c) Sϕ, sh plotted as a function of ω for various weak values and for s = 0.5, ϕ = π/2. (d) Sϕ, sh of the odd Schrödinger cat state (ω = π) vs. the squeezing parameter angle ϕ for different interaction strength and for θ = π/9.

    The analytic expression of Sϕ,sch for the Schrödinger cat state after postselected measurement can be achieved using the final normalized state |χ〉, and the analytical results are summarized in Fig. 9. As indicated in Fig. 9, after postselected measurement, the squeezing effect of the Schrödinger cat state still depends on phase ϕ, and the squeezing effect of both the even and odd Schrödinger cat states are increased with increasing the interaction strength s and for small weak values (see Figs. 9(a), 9(b), and 9(d)). However, the odd Schrödinger cat pointer state has no squeezing effect (see Figs. 9(c) and 9(d)).

    4. Conclusion and remarks

    In summary, we have investigated the effects of postselected measurement characterized by postselection and weak value on the statistical properties and squeezing effects of single-mode radiation fields. To achieve our goal, we take the coherent state, squeezed vacuum state and Schrödinger cat state as a pointer, and their polarization degrees of freedom as the measurement system, respectively. We have derived analytical expressions of the pointer state’s normalized final state after postselected measurement considering all interaction strengths between the pointer and the measured system. We separately present the exact expressions of photon distributions, second-order correlation functions, Mandel factors and squeezing parameters of the above three typical single-mode radiation fields for the corresponding final pointer states, and plot the figures to analyze the results.

    We find that the photon distributions of those three pointer states change significantly after postelected measurement, especially the coherent pointer state. It is shown that postselected measurement changes the photon statistics and squeezing effect of coherent state dramatically, and it is noticed that the amplification effect of weak value plays a major role in this process. We also show that the postselected measurement changes the photon statistics of the squeezed vacuum state from super-Poisson to sub-Poisson for large weak values, and moderate interaction strengths. However, the photon statistics of the Schrödinger cat state changes from sub-Poisson to super-Poisson with increasing the interaction strength. In accordance with previous findings, the squeezing effects of squeezed vacuum and Schrödinger cat pointer states are still phase-dependent and the squeezing effect of squeezed vacuum pointer is decreased with increasing the interaction strength. On the contrary, the squeezing effect of the even Schrödinger cat state is increased with increasing the interaction strength for small weak values compared with the initial pointer state case.

    This work belongs to the state optimization using postselected von Neumann measurement. Those properties of radiation fields we investigated are directly effect on the implementations of the important quantum information processing mentioned in the introduction section. Thus, we anticipate that the results shown in this research can be useful to provide other effective methods for studying the related quantum information processing.

    In our current research, we only consider the three typical single-mode radiation fields to investigate the effects of postselected von Neuman measurement on their inherent properties, but real light beams are in fact the time-dependent and the representation of time dependence requires the use of two or more modes of the optical systems. Thus, it would be interesting to check the effects of postselected von Neumann measurement on other useful radiation fields in quantum optics and quantum information processing such as single photon-added[58,59] and photon-subtracted[60] states, pair-coherent state (two-mode field),[6164] and other multimode radiation fields.[65]

    Appendix A: The explicit expressions of some quantities

    (1) For squeezed vacuum pointer state The expectation value of photon number operator a?a under the state |χ? is given by ?a?a??=|κ|24{2(1+|?A?w|2)(s24+sinh2η)+2Re[(1??A?w)(1+?A?w)?I]} with I=exp[?s22|coshη+eiδsinhη|2]×(sinh2η+s24?s22(1+isinδsinh2η)). In calculating the squeezing parameter, we use ? X??φ and ?X?2?φ, and their expressions are given by ?X???=s|κ|242{cos?|1+?A?w|2?cos?|1+?A?w|2+2exp[?s22|coshη+eiδsinhη|2]×Re[e?iθ(1+?A?w)(1??A?w)?×(cosh2η+12eiδsinh2η?12)]?2exp[?s22|coshη+eiδsinhη|2]]×Re{eiθ(1+?A?w)?(1??A?w)×[cosh2η+eiδ12sinh2η?12]}?Xθ2?=12[2Re(I?Ie?2i?)+2?a?a?+1] with I?I=|κ|24{(s24?12sinh(2η)e?iδ)|1+?A?w|2+(s24?12sinh(2η)e?iδ)|1??A?w|2+(1?|?A?w|2)III}, where III=s24+s2(12e?iδsinh2η+sinh2η)+s2(coshη+eiδsinhη)2e?2iδsinh2η?e?iδ12sinh2η}exp[?s22|coshη+eiδsinhη|2].

    (2) For Schr?dinger cat pointer state The expectation value of photon number operator a?a and a?2a2 under the state |χ? is given by ?a?a?χ=|κ|2K24{|1+?A?w|2[|α+s2|2+|?α+s2|2+eiω(α+s2)?×(?α+s2)e?2|α|2+e?iω(?α+s2)?(α+s2)e?2|α|2]+|1??A?w|2[|α?s2|2+|α+s2|2?eiω(α?s2)?(α+s2)e?2|α|2?e?iω(α+s2)?(α?s2)e?2|α|2]?2Re[(eiω|α+s2|2e?2|α+s2|2+e?iωe?2|α?s2|2|α?s2|2?2e?s22×Re[e2isIm(α)(α+s2)?(α?s2)])(1??A?w)(1+?A?w)?]},?a?2a2?χ=|κ|2K24{|1+?A?w|2[|α+s2|4+|?α+s2|4+eiω(α?+s2)2(?α+s2)2e?2|α|2+e?iω(?α?+s2)2(α+s2)2e?2|α|2]+|1??A?w|2[|α?s2|4+|α+s2|4+eiωe?2|α|2(α??s2)2(α+s2)2+e?iωe?2|α|2(α?+s2)(α?s2)2]+2Re[(eiω|α+s2|4e?2|α+s2|2+e?iω|α?s2|4e?2|α?s2|2+2e?s22Re[e2isIm(α)(α?+s2)2(α?s2)2])(1??A?w)(1+?A?w)?]}. In calculation of the squeezing parameter, we use? X??χ and ?X?2?χ, and their expressions are given by ?X??χ=2Re[?a?χe?i?] with ?a?χ=|κ|2K24{|1+?A?w|2[s+ei?(?α+s2)e?2|α|2+e?i?(α+s2)e?2|α|2]+|1??A?w|2[?s?ei?(α+s2)e?2|α|2+e?i?(α?s2)e?2|α|2]+(1??A?w)(1+?A?w)?[(2iαsin(2sIm[α])?scos(2sIm[α]))e?12s2?ei?(α+s2)e?12|2α+s|2+e?i?(α?s2)e?12|2α?s|2]+(1??A?w)?(1+?A?w)[(?2iαsin(2sIm[α])+scos(2sIm[α]))e?12s2+ei?(?α+s2)e?12|2α?s|2+e?i?(α+s2)e?12|2α+s|2]},?X?2?χ=12[2?a?a?χ+2Re[?a2?χe?2i?]+1], with ?a2?χ=|κ|2K24{|1+?A?w|2[2(α2+s24)+eiωe?2|α|2(?α+s2)2+e?iωe?2|α|2(α+s2)2]+|1??A?w|2[2(α2+s24)+eiωe?2|α|2(α+s2)2+e?iωe?2|α|2(α?s2)2]+(1??A?w)(1+?A?w)?[2e?s24(cos(2sIm[α])(α2+s24)?isαsin(2sIm[α]))+e?iω(α?s2)2e?2|α?s2|2+eiω(α+s2)2e?2|α+s2|2]+(1+?A?w)(1??A?w)?[2e?s24(cos(2sIm[α])(α2+s24)?isαsin(2sIm[α]))+eiω(α?s2)2e?2|α?s2|2+e?iω(α+s2)2e?2|α+s2|2]}.

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    Yusuf Turek. Effects of postselected von Neumann measurement on the properties of single-mode radiation fields[J]. Chinese Physics B, 2020, 29(9):

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    Paper Information

    Received: Apr. 29, 2020

    Accepted: --

    Published Online: Apr. 29, 2021

    The Author Email: Yusuf Turek (yusufu1984@hotmail.com)

    DOI:10.1088/1674-1056/ab9f23

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