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Stabilizing Preparation of Quantum Gaussian States via Continuous Measurement

Liying Bao [email protected]    Bo Qi [email protected]    Daoyi Dong [email protected] Key Laboratory of Systems and Control, Academy of Mathematics and Systems Science,
Chinese Academy of Sciences, Beijing 100190, China
University of Chinese Academy of Sciences, Beijing 100049, China School of Engineering and Information Technology, University of New South Wales, Canberra ACT 2600, Australia
Abstract

This paper provides a stabilizing preparation method for quantum Gaussian states by utilizing continuous measurement. The stochastic evolution of the open quantum system is described in terms of the quantum stochastic master equation. We present necessary and sufficient conditions for the system to have a unique stabilizing steady Gaussian state. The conditions are much weaker than those existing results presented in the approach of preparing Gaussian states through environment engineering. Parametric conditions of how to prepare an arbitrary pure Gaussian state are provided. This approach provides more degrees of freedom to choose the system Hamiltonian and the system-environment coupling operators, as compared with the case where dissipation-induced approach is employed. The stabilizing conditions for the case of imperfect measurement efficiency are also presented. These results may benefit practical experimental implementation in preparing quantum Gaussian states.

keywords:
Quantum Gaussian state; Continuous measurement; Riccati equation; Linear quadratic Gaussian system.
thanks: The material in this paper was not presented at any conference.

, , \corauth[cor1]Corresponding author.

1 Introduction

Continuous variable systems, which are quantum systems with infinite dimensional Hilbert spaces, have been an important platform for quantum cryptography, quantum information and quantum computation [Edwards & Belavkin, 2005, van Handel, Stockton, & Mabuchi, 2005, James, Nurdin, & Petersen, 2008, Wiseman & Milburn, 2010, Nurdin, Petersen, & James, 2012, Pan, Zhang, & James, 2016, Ma, Woolley, Petersen, & Yamamoto, 2018, Gao, Zhang, & Petersen, 2020, Gao, Dong, Petersen, & Ding, 2020, Ghalaii, Ottaviani, Kumar, Pirandola, & Razavi, 2021, Zhang & Pan, 2020, Zhang & Petersen, 2020, Gao, Dong, Petersen, & Ding, 2021, Guo, Peng, Liao, & Wang, 2021]. Gaussian states, which include a wide and important class of quantum states such as vacuum states, squeezed vacuum, squeezed coherent states, quasi-free states and ground states of some free Hamiltonians, are the basis for various continuous variable quantum information processing [De Palma, Trevisan, & Giovannetti, 2017, Holevo, 2020, Srikara, Thapliyal, & Pathak, 2020]. Since Gaussian states can be completely characterized by their first and second moments and the Gaussian character can be preserved under typical quantum operations, they are relatively easy to be studied analytically and are often used as theoretical testing ground [Bondurant, Kumar, Shapiro, & Maeda, 1984, Erkmen & Shapiro, 2008, Yokoyama et al., 2013, Chabaud, 2021]. Besides, protocols based on Gaussian states and Gaussian measurements (e.g., homodyne detection) are relatively experimentally friendly as compared to operations of general quantum states [Pinel, Jian, Treps, Fabre, & Braun, 2013, Banchi, Braunstein, & Pirandola, 2015, McDonald & Clerk, 2020, Bao, Qi, Dong, & Nori, 2021]. Thus Gaussian states are of great importance in both theoretical studies and experimental implementations.

The preparation of a desired Gaussian state is clearly a pivotal task in continuous variable quantum information processing [Diehl et al., 2008, Verstraete, Wolf, & Ignacio, 2009, Krauter et al., 2011, Koga & Yamamoto, 2012, Yamamoto, 2012, Ma, Woolley, Petersen, & Yamamoto, 2014, Ma, Woolley, Jia, & Zhang, 2019, Häffner, Zanin, Gomes, Céleri, & Souto Ribeiro, 2020, Giovanni, Brunelli, & Genoni, 2021]. There have been some results proposed on the basis of the dissipation-induced approach or the environment engineering approach [Diehl et al., 2008, Verstraete, Wolf, & Ignacio, 2009, Krauter et al., 2011, Koga & Yamamoto, 2012, Yamamoto, 2012, Ma, Woolley, Petersen, & Yamamoto, 2014]. The basic idea behind those results is that one can utilize the dissipative environment by engineering a proper Hamiltonian and appropriately designed dissipative channels such that the corresponding stable state is a desired useful Gaussian state. In [Koga & Yamamoto, 2012], necessary and sufficient conditions for a Gaussian master equation to have a unique steady pure state were provided and then based on those conditions a systematic procedure to prepare a desired state via dissipation was proposed. Based on the quantum stochastic differential equation, [Yamamoto, 2012] further investigated the pure Gaussian state generation and clarified a physical meaning that the nullifier dynamics of any Gaussian system generating a unique steady pure state is passive. An alternative method of preparing pure Gaussian state was presented in [Ma, Woolley, Petersen, & Yamamoto, 2014], where it was shown that a desired pure Gaussian state can be prepared by a cascade of one-dimensional open quantum harmonic oscillators, without any direct interaction Hamiltonians between these oscillators.

As mentioned, Gaussian states can be completely characterized by their first and second moments. In practice, most of the useful properties of Gaussian states such as the purity [Paris, Illuminati, Serafini, & De Siena, 2003], entanglement [Marian & Marian, 2008] and squeezing [Petersen, Madsen, & Mølmer, 2005] are only related with the second moment. In previous results, the covariance matrix which depicts the second moment of the Gaussian states is described in terms of the quantum master equation (QME) in essence [Koga & Yamamoto, 2012, Yamamoto, 2012, Ma, Woolley, Petersen, & Yamamoto, 2014]. In this paper, we provide an alternative way in preparing quantum Gaussian states by utilizing continuous measurement. To account for the randomness of quantum measurement, the evolution of the open quantum system is described in terms of the quantum stochastic master equation (QSME). The basic idea is that the covariance matrix determined by the QSME is smaller (in the sense of matrix partial order) than that determined by the QME if all the parameterizations are the same. Thus, by utilizing continuous measurement, the useful properties of Gaussian states can be improved. We first present necessary and sufficient conditions for the system to have a unique stabilizing steady pure Gaussian state. The conditions are much weaker than those presented in the dissipation-induced approach. Then general parametric conditions of generating an arbitrarily desired pure Gaussian state are provided. They provide more degrees of freedom to choose the system Hamiltonian and coupling channels as compared with previous results. For completeness and practical applications, we also consider the case where the detection is imperfect.

The paper is organized as follows. In Section II, we first give some preliminaries on Gaussian states and the QSME, and then set up the linear quadratic Gaussian system model to be utilized. The main results focusing on pure Gaussian states are presented in Section III. Section IV discusses the case where the detection efficiency is less than 1. Section V concludes the paper.

2 Gaussian states, QSME & linear quadratic Gaussian system

This section briefly introduces the Wigner representation of Gaussian states, the framework of continuous measurement and the setting of linear quadratic Gaussian system. After an appropriate setting is given, the preparation problem of Gaussian states is restated as a stabilizing steady state problem of a Riccati equation.

2.1 Wigner representation of Gaussian states

We start from reviewing the Wigner phase-space representation [Paris, Illuminati, Serafini, & De Siena, 2003, Wiseman & Milburn, 2010], which is one of the most commonly used representations for quantum Gaussian states.

Denote a^k\hat{a}_{k} and a^k\hat{a}^{\dagger}_{k}, k=1,,mk=1,...,m, as the canonical bosonic annihilation and creation operators of the kk-th mode, respectively. The corresponding canonical quadrature operators q^k\hat{q}_{k} and p^k\hat{p}_{k} are defined via

q^k=a^k+a^k2andp^k=ia^ka^k2,\hat{q}_{k}=\frac{\hat{a}_{k}+\hat{a}_{k}^{\dagger}}{2}~{}~{}\text{and}~{}~{}\hat{p}_{k}=i\frac{\hat{a}_{k}^{\dagger}-\hat{a}_{k}}{2},

which satisfy the canonical commutation relation

[q^k,p^j]=iδkj,[\hat{q}_{k},\hat{p}_{j}]=i\delta_{kj},

where i=1i=\sqrt{-1} and δkj\delta_{kj} is the Kronecker delta function. Denote the vector of quadrature operators for the mm mode system as

X^=(q^1,,q^m,p^1,,p^m),\hat{\textbf{X}}=(\hat{q}_{1},\cdots,\hat{q}_{m},\hat{p}_{1},\cdots,\hat{p}_{m})^{\top},

where \top is the matrix transpose. The operator vector X^\hat{\textbf{X}} satisfies the canonical commutation relations [Koga & Yamamoto, 2012, Yamamoto, 2012, Ma, Woolley, Petersen, & Yamamoto, 2014]

[X^,X^]=X^X^(X^X^)=iJ,\left[\hat{\textbf{X}},\hat{\textbf{X}}^{\top}\right]=\hat{\textbf{X}}\hat{\textbf{X}}^{\top}-(\hat{\textbf{X}}\hat{\textbf{X}}^{\top})^{\top}=iJ,

where J=(0ImIm0)J=\begin{pmatrix}0&I_{m}\\ -I_{m}&0\end{pmatrix}, and ImI_{m} is the m×mm\times m identity matrix.

The joint displacement operator can be described in terms of X^\hat{\textbf{X}} and JJ as

D^(𝜶)=exp(iX^J𝜶),\hat{D}(\bm{\alpha})=\textrm{exp}(i~{}\hat{\textbf{X}}^{\top}J\bm{\alpha}),

where 𝜶2m\bm{\alpha}\in\mathbb{R}^{2m} [Paris, Illuminati, Serafini, & De Siena, 2003, Wiseman & Milburn, 2010]. On the basis of D^(𝜶)\hat{D}(\bm{\alpha}), for an arbitrary quantum state operator ρ^\hat{\rho}, its Wigner characteristic function is defined as

χρ^(𝜶)=Tr[ρ^D^(𝜶)].\chi_{\hat{\rho}}(\bm{\alpha})=\textrm{Tr}[\hat{\rho}\hat{D}(\bm{\alpha})].

Now the Wigner function Wρ^(X)W_{\hat{\rho}}(X) of the state ρ^\hat{\rho} can be described as

Wρ^(X)=2md𝜶(2π)2mexp(iXJ𝜶)χρ^(𝜶),W_{\hat{\rho}}(X)=\int_{\mathbb{R}^{2m}}\frac{d\bm{\alpha}}{(2\pi)^{2m}}\textrm{exp}(-iX^{\top}J\bm{\alpha})\chi_{\hat{\rho}}(\bm{\alpha}),

where X=(q1,,qm,p1,,pm)X=(q_{1},...,q_{m},p_{1},\cdots,p_{m})^{\top} with qiq_{i} and pjp_{j} being real numbers [Paris, Illuminati, Serafini, & De Siena, 2003, Wiseman & Milburn, 2010].

A state is called Gaussian if its Wigner function is in the form of

W(X)=exp[12(XX¯)V1(XX¯)](2π)mdet[V],W(X)=\frac{\textrm{exp}[-\frac{1}{2}(X-\bar{X})^{\top}V^{-1}(X-\bar{X})]}{(2\pi)^{m}\sqrt{\textrm{det}[V]}}, (1)

where X¯=X^=Tr(X^ρ^)\bar{X}=\langle\hat{\textbf{X}}\rangle=\textrm{Tr}(\hat{\textbf{X}}\hat{\rho}) is the mean value vector whose element X¯i=X^i=Tr(X^iρ^)\bar{X}_{i}=\langle\hat{\textbf{X}}_{i}\rangle=\textrm{Tr}(\hat{\textbf{X}}_{i}\hat{\rho}), VV is the covariance matrix whose element Vij=12ΔX^iΔX^j+ΔX^jΔX^iV_{ij}=\frac{1}{2}\langle\Delta\hat{\textbf{X}}_{i}\Delta\hat{\textbf{X}}_{j}+\Delta\hat{\textbf{X}}_{j}\Delta\hat{\textbf{X}}_{i}\rangle with ΔX^i=X^iX^i\Delta\hat{\textbf{X}}_{i}=\hat{\textbf{X}}_{i}-\langle\hat{\textbf{X}}_{i}\rangle, and det[V]\textrm{det}[V] denotes the determinant of matrix VV [Edwards & Belavkin, 2005, Wiseman & Milburn, 2010]. In addition to the positive semidefinite condition V0V\geq 0, VV should satisfy the Heisenberg uncertainty principle [Koga & Yamamoto, 2012, Yamamoto, 2012, Ma, Woolley, Petersen, & Yamamoto, 2014]

V±i2J.V\geq\pm\frac{i}{2}J.

It is straightforward to see that a Gaussian state is determined by the mean vector X¯\bar{X} and the covariance matrix VV.

In this paper, we only focus on the covariance matrix VV. This is because, on the one hand, that one can always adjust the mean of a Gaussian state to any target mean by a suitable Weyl operator [Parthasarathy, 2010]. On the other hand it is noted that most of the useful properties of Gaussian states such as the purity, entanglement and squeezing are only related with the covariance matrix in practice. To be specific, the purity of a mm mode Gaussian state depends only on the covariance matrix as Tr[ρ^2]=12mdet[V]\textrm{Tr}[\hat{\rho}^{2}]=\frac{1}{2^{m}\sqrt{\textrm{det}[V]}} [Paris, Illuminati, Serafini, & De Siena, 2003]. Moreover, for a two-mode pure Gaussian state, its 4×44\times 4 covariance matrix contains all the necessary information to determine its entanglement properties for both entanglement criteria and entanglement measures [Rendell & Rajagopal, 2005, Marian & Marian, 2008]. In addition, squeezed coherent states have been extensively studied in quantum information, such as quantum teleportation and ghost imaging. The squeezing properties are also determined by the covariance matrix [Petersen, Madsen, & Mølmer, 2005].

2.2 Quantum stochastic master equation

In previous results, the commonly used model in preparing a target Gaussian state is to engineer a dissipative system described by the quantum master equation [Edwards & Belavkin, 2005, Wiseman & Milburn, 2010, Koga & Yamamoto, 2012, Yamamoto, 2012]

dρ^tdt=i[H^,ρ^t]+i=1m(L^iρ^tL^i12L^iL^iρ^t12ρ^tL^iL^i),\frac{d\hat{\rho}_{t}}{dt}=-i[\hat{H},\hat{\rho}_{t}]+\sum_{i=1}^{m}(\hat{L}_{i}\hat{\rho}_{t}\hat{L}_{i}^{\dagger}-\frac{1}{2}\hat{L}_{i}^{\dagger}\hat{L}_{i}\hat{\rho}_{t}-\frac{1}{2}\hat{\rho}_{t}\hat{L}_{i}^{\dagger}\hat{L}_{i}), (2)

where ρ^t\hat{\rho}_{t} is the density operator, H^\hat{H} is the effective Hamiltonian of the system and L^i,i=1,,m\hat{L}_{i},~{}i=1,\ldots,m, are the dissipative channels which describe the interaction between the system and the environment. The dissipative QME (2) can be viewed as an average (unconditional) evolution of the quantum state under the assumption that all the measurement results are discarded. Intuitively if one can utilize the measurement information, the corresponding conditional covariance matrix may be reduced, and thus the useful properties of the Gaussian states can be improved. In this paper, we present how to prepare a desired quantum Gaussian state by utilizing continuous measurement. To account for the randomness of quantum measurement, the evolution of the open quantum system is described in terms of the quantum stochastic master equation.

To proceed, we specify the following notation for clarity. For a matrix Q=(qij)Q=(q_{ij}), let QQ^{\dagger}, QQ^{\top} and QQ^{*} represent the conjugate transpose, transpose and conjugate for all the elements of QQ, respectively. For example, Q=(qji),Q=(qji),Q^{\dagger}=(q^{*}_{ji}),~{}Q^{\top}=(q_{ji}), and Q=(qij)=(Q)Q^{*}=(q^{*}_{ij})=(Q^{\dagger})^{\top}.

The dynamics of the open system coupled with mm independent measurement channels {L^i}i=1m\{\hat{L}_{i}\}^{m}_{i=1} can be described by a family of unitary operators {U^t}t+\{\hat{U}_{t}\}_{t\in\mathbb{R_{+}}}, which satisfy

d\displaystyle d U^t=K^U^tdt+i=1m(L^idA^i,tL^idA^i,t)U^t,\displaystyle\hat{U}_{t}=-\hat{K}\hat{U}_{t}dt+\sum^{m}_{i=1}(\hat{L}_{i}d\hat{A}^{\dagger}_{i,t}-\hat{L}_{i}^{\dagger}d\hat{A}_{i,t})\hat{U}_{t}, (3)
U^0=I,\displaystyle\hat{U}_{0}=I,

where K^=iH^+12i=1mL^iL^i\hat{K}=i\hat{H}+\frac{1}{2}\sum^{m}_{i=1}\hat{L}^{\dagger}_{i}\hat{L}_{i} [Edwards & Belavkin, 2005]. Here we have assumed =1\hbar=1. The differential of the annihilation operators of the bath dA^i,td\hat{A}_{i,t} obeys the quantum Ito^\hat{\textrm{o}} rules:

dA^i,tdA^j,t=δi,jdt,dA^i,tdA^j,t=0,d\hat{A}_{i,t}d\hat{A}_{j,t}^{\dagger}=\delta_{i,j}dt,~{}d\hat{A}_{i,t}d\hat{A}_{j,t}=0,
dA^i,tdA^j,t=0,dA^i,tdA^j,t=0.d\hat{A}^{\dagger}_{i,t}d\hat{A}^{\dagger}_{j,t}=0,~{}d\hat{A}^{\dagger}_{i,t}d\hat{A}_{j,t}=0.

For any system operator X^\hat{X}, its time evolution in the Heisenberg picture is represented by

jt(X^)=U^t(X^I)U^t.j_{t}(\hat{X})=\hat{U}_{t}^{\dagger}(\hat{X}\otimes I)\hat{U}_{t}.

From (3) and the quantum Ito^\hat{\textrm{o}} rules, we have

djt(X^)=jt([X^])dt+\displaystyle dj_{t}(\hat{X})=j_{t}(\mathcal{L}[\hat{X}])dt+ i=1m(jt([L^i,X^])dAi,t\displaystyle\sum^{m}_{i=1}\Big{(}j_{t}([\hat{L}^{\dagger}_{i},\hat{X}])dA_{i,t} (4)
+jt([X^,Li^])dAi,t),\displaystyle+j_{t}([\hat{X},\hat{L_{i}}])dA^{\dagger}_{i,t}\Big{)},

where

[X^]=i[H^,X^]+i=1m(L^iX^L^i12L^iL^iX^12X^L^iL^i).\mathcal{{L}}[\hat{X}]=i[\hat{H},\hat{X}]+\sum_{i=1}^{m}(\hat{L}_{i}^{\dagger}\hat{X}\hat{L}_{i}-\frac{1}{2}\hat{L}_{i}^{\dagger}\hat{L}_{i}\hat{X}-\frac{1}{2}\hat{X}\hat{L}_{i}^{\dagger}\hat{L}_{i}).

Consider mm family of measurement operators {Yi,t}t+\{Y_{i,t}\}_{t\in\mathbb{R_{+}}}, where

Y^i,t=U^t(A^i,t+A^i,t)U^t\hat{Y}_{i,t}=\hat{U}^{\dagger}_{t}(\hat{A}_{i,t}+\hat{A}^{\dagger}_{i,t})\hat{U}_{t}

for i=1,,mi=1,\cdots,m. From (3) and the quantum Ito^\hat{\textrm{o}} rules, we have

dY^i,t=jt(L^i+L^i)dt+dA^i,t+dA^i,t.d\hat{Y}_{i,t}=j_{t}(\hat{L}_{i}+\hat{L}_{i}^{\dagger})dt+d\hat{A}_{i,t}+d\hat{A}^{\dagger}_{i,t}. (5)

Once Y^i,t=U^t(A^i,t+A^i,t)U^t\hat{Y}_{i,t}=\hat{U}^{\dagger}_{t}(\hat{A}_{i,t}+\hat{A}^{\dagger}_{i,t})\hat{U}_{t}, i=1,,mi=1,\cdots,m, are observed, one can associate a conditional expectation to each observable X^\hat{X} of the system. The conditional expectation gives the least squares estimator of jt(X^)j_{t}(\hat{X}) as [jt(X^)|Y^0t]\mathcal{E}[j_{t}(\hat{X})|\hat{Y}^{t}_{0}], where Y^0t\hat{Y}^{t}_{0} is the algebra generated by Y^i,st\hat{Y}_{i,s\leq t}, i=1,,mi=1,\cdots,m. Since Y^0t\hat{Y}^{t}_{0} is nondemolition, the observation process is in essence equivalent to mm classical stochastic processes

{yi,st,i=1,,m}.\{y_{i,s\leq t},i=1,\cdots,m\}.

Thus [jt(X^)|Y^0t]\mathcal{E}[j_{t}(\hat{X})|\hat{Y}^{t}_{0}] actually represents the expectation of X^\hat{X} conditioned on the classical stochastic observations {yi,st\{y_{i,s\leq t}, i=1,,m}i=1,\cdots,m\}. This conditional expectation can be conveniently written in the Schrödinger picture as

[jt(X^)|Y^0t]=Tr(ρ^tcX^)\mathcal{E}[j_{t}(\hat{X})|\hat{Y}^{t}_{0}]=\text{Tr}(\hat{\rho}^{c}_{t}\hat{X})

with ρ^tc\hat{\rho}^{c}_{t} denoting the conditional system state at time tt. The stochastic master equation of ρtc\rho^{c}_{t} is described as [van Handel, Stockton, & Mabuchi, 2005, Edwards & Belavkin, 2005, Wiseman & Milburn, 2010]

dρ^tc=[ρ^tc]dt+\displaystyle d\hat{\rho}_{t}^{c}=\mathcal{L}^{\dagger}[\hat{\rho}^{c}_{t}]dt+ i=1m(L^iρ^tc+ρ^tcL^i\displaystyle\sum_{i=1}^{m}\Big{(}\hat{L}_{i}\hat{\rho}^{c}_{t}+\hat{\rho}^{c}_{t}\hat{L}^{\dagger}_{i} (6)
Tr[ρ^tc(L^i+L^i)]ρ^tc)dwi,t,\displaystyle-\text{Tr}[\hat{\rho}^{c}_{t}(\hat{L}_{i}+\hat{L}_{i}^{\dagger})]\hat{\rho}^{c}_{t}\Big{)}dw_{i,t},

where the innovations

dwi,t=dyi,tρ^tc,L^i+L^idtdw_{i,t}=d{y}_{i,t}-\langle\hat{\rho}^{c}_{t},\hat{L}_{i}+\hat{L}_{i}^{\dagger}\rangle dt

are Gaussian, and

[ρ^tc]=i[H^,ρ^tc]+i=1m(L^iρ^tcL^i12L^iL^iρ^tc12ρ^tcL^iL^i).\mathcal{{L}}^{\dagger}[\hat{\rho}_{t}^{c}]=-i[\hat{H},\hat{\rho}_{t}^{c}]+\sum_{i=1}^{m}(\hat{L}_{i}\hat{\rho}_{t}^{c}\hat{L}_{i}^{\dagger}-\frac{1}{2}\hat{L}_{i}^{\dagger}\hat{L}_{i}\hat{\rho}_{t}^{c}-\frac{1}{2}\hat{\rho}_{t}^{c}\hat{L}_{i}^{\dagger}\hat{L}_{i}).

It is clear that by taking the expectation of (6), we can obtain the quantum master equation (2).

2.3 Quantum linear quadratic Gaussian system

We are interested in systems of mm degrees of freedom with the phase space operator vector

X^=(q^1,,q^m,p^1,,p^m)\hat{\textbf{X}}=(\hat{q}_{1},\cdots,\hat{q}_{m},\hat{p}_{1},\cdots,\hat{p}_{m})^{\top}

as defined in subsection 2.1. Recall that the operator vector X^\hat{\textbf{X}} satisfies the canonical commutation relation

[X^,X^]\displaystyle\left[\hat{\textbf{X}},\hat{\textbf{X}}^{\top}\right] =X^X^(X^X^)=iJ.\displaystyle=\hat{\textbf{X}}\hat{\textbf{X}}^{\top}-(\hat{\textbf{X}}\hat{\textbf{X}}^{\top})^{\top}=iJ.

The system is coupled to mm measurement channels via the operator vector L^=ΛX^\hat{\textbf{L}}=\Lambda\hat{\textbf{X}}, where Λm×2m\Lambda\in\mathbb{C}^{m\times 2m}. The Hamiltonian which is quadratic in X^\hat{\textbf{X}} is represented as

H^(ut)=12X^GX^+X^Kut+utKX^,\hat{H}(u_{t})=\frac{1}{2}\hat{\textbf{X}}^{\top}G~{}{\hat{\textbf{X}}}+\hat{\textbf{X}}^{\top}Ku_{t}+u_{t}^{\top}K^{\dagger}\hat{\textbf{X}},

where G=G2m×2mG=G^{\top}\in\mathbb{R}^{2m\times 2m}, K2m×mK\in\mathbb{C}^{2m\times m} and utmu_{t}\in\mathbb{R}^{m} is the control. For such a system, from (3)-(5), we have the quantum linear equations in the Heisenberg picture as

dX^t=(AX^t+But)dt+dV^t,\displaystyle d\hat{\textbf{X}}_{t}=(A\hat{\textbf{X}}_{t}+Bu_{t})dt+d\hat{\textbf{V}}_{t},
dY^t=CX^tdt+dW^t,\displaystyle d\hat{\textbf{Y}}_{t}=C\hat{\textbf{X}}_{t}dt+d\hat{\textbf{W}}_{t},

where

A\displaystyle A =J(G+12i(ΛΛΛΛ))2m×2m,\displaystyle=J\Big{(}G+\frac{1}{2i}(\Lambda^{\dagger}\Lambda-\Lambda^{\top}\Lambda^{*})\Big{)}\in\mathbb{R}^{2m\times 2m},
B\displaystyle B =J(K+K)2m×m,\displaystyle=J(K+K^{*})\in\mathbb{R}^{2m\times m},
C\displaystyle C =Λ+Λm×2m,\displaystyle=\Lambda+\Lambda^{*}\in\mathbb{R}^{m\times 2m},

and the quantum noise increments are given by

dV^t=iJ(ΛdA^tΛdA^t),\displaystyle d\hat{\textbf{V}}_{t}=iJ(\Lambda^{\top}d\hat{\textbf{A}}_{t}^{\dagger}-\Lambda^{\dagger}d\hat{\textbf{A}}_{t}),
dW^t=dA^t+dA^t.\displaystyle d\hat{\textbf{W}}_{t}=d\hat{\textbf{A}}_{t}+d\hat{\textbf{A}}_{t}^{\dagger}.

For the quantum linear quadratic system, if the initial state ρ^\hat{\rho} of the system is Gaussian, then under the nondemolition measurement of the output operators Y^t\hat{\textbf{Y}}_{t}, the conditional dynamics (6) is also Gaussian. Thus for the linear quadratic Gaussian system, its dynamics can be sufficiently described by the time flow of the conditional mean vector X¯t=Tr(X^ρ^tc)\bar{X}_{t}=\textrm{Tr}(\hat{\textbf{X}}\hat{\rho}^{c}_{t}) and the covariance matrix VtV_{t}, whose element

Vt=,ij12ΔcX^iΔcX^j+ΔcX^jΔcX^icV_{t}{{}_{,ij}}=\frac{1}{2}\langle\Delta_{c}\hat{\textbf{X}}_{i}\Delta_{c}\hat{\textbf{X}}_{j}+\Delta_{c}\hat{\textbf{X}}_{j}\Delta_{c}\hat{\textbf{X}}_{i}\rangle_{c}

with ΔcX^i=X^iX^ic\Delta_{c}\hat{\textbf{X}}_{i}=\hat{\textbf{X}}_{i}-\langle\hat{\textbf{X}}_{i}\rangle_{c} and X^ic=Tr(X^iρtc)\langle\hat{\textbf{X}}_{i}\rangle_{c}=\text{Tr}(\hat{\textbf{X}}_{i}\rho^{c}_{t}). Using (6), we have the conditional expectation X¯t\bar{X}_{t} of X^\hat{\textbf{X}} under the measurement of Y^t\hat{\textbf{Y}}_{t} as

dX¯t\displaystyle d\bar{X}_{t} =(AX¯t+But)dt+(VtC+M)dy~t,\displaystyle=(A\bar{X}_{t}+Bu_{t})dt+(V_{t}C^{\top}+M)d\tilde{y}_{t}, (7)
X¯0\displaystyle\bar{X}_{0} =X¯,\displaystyle=\bar{X},

where

M=i2J(ΛΛ)2m×m,M=\frac{i}{2}J(\Lambda^{\top}-\Lambda^{\dagger})\in\mathbb{R}^{2m\times m},

and

dy~t=dytCX¯tdtd\tilde{y}_{t}=dy_{t}-C\bar{X}_{t}dt

is the Gaussian innovation which describes the information gain from the the measurement. The conditional covariance matrix satisfies the matrix Riccati equation

ddtVt\displaystyle\frac{d}{dt}V_{t} =AVt+VtA+N(VtC+M)(VtC+M),\displaystyle=AV_{t}+V_{t}A^{\top}+N-(V_{t}C^{\top}+M)(V_{t}C^{\top}+M)^{\top}, (8)
V0\displaystyle V_{0} =V,\displaystyle=V,

where

N=12J(ΛΛ+ΛΛ)J2m×2m.N=\frac{1}{2}J(\Lambda^{\dagger}\Lambda+\Lambda^{\top}\Lambda^{*})J^{\top}\in\mathbb{R}^{2m\times 2m}.

It is worth noting that the equation for VtV_{t} is deterministic and does not depend on the stochastic measurement results.

Taking expectation values of (7) and (8), we have the moment equations for the unconditional approach as

dX¯t=(AX¯t+But)dt,\displaystyle d\bar{X}_{t}=(A\bar{X}_{t}+Bu_{t})dt, (9)
ddtVt=AVt+VtA+N,\displaystyle\frac{d}{dt}V_{t}=AV_{t}+V_{t}A^{\top}+N,

which correspond to the quantum master equation (2). To prepare a desired Gaussian state, most of the previous results are on the basis of the moment equations (9). Note that the final term in (8) causes a reduction in the conditional covariance matrix as compared with that in (9). Recall that most of the useful properties of the Gaussian states are determined by the covariance matrix. Thus intuitively by utilizing the conditional covariance matrix equation (8), one may provide weaker conditions in preparing a desired Gaussian state.

Let us first look at the equation of the conditional expectation (7). We can choose BB such that its column space is the same as that of VC+MVC^{\top}+M, where VV is the steady solution of (8). Then we choose FF such that it satisfies

BF=VCM.BF=-VC^{\top}-M.

Thus, for the Markovian feedback (or direct feedback) utdt=Fdytu_{t}dt=Fdy_{t} [Wiseman & Milburn, 2010], the equation (7) of the first moment becomes deterministic in the limit tt\rightarrow\infty as

ddtX¯t=(AMCVCC)X¯t.\frac{d}{dt}\bar{X}_{t}=(A-MC-VC^{\top}C)\bar{X}_{t}. (10)

Therefore, if AMCVCCA-MC-VC^{\top}C is stable, then the solution of (10) will approach to 0 approximately. In the following we will give necessary and sufficient conditions for the conditional covariance matrix equation (8) to have a steady solution and meanwhile AMCVCCA-MC-VC^{\top}C is stable. From now on we focus on the conditional covariance matrix equation (8).

3 Main results

In subsection 3.1, we first present necessary and sufficient condition for the Riccati equation (8) to have a unique stabilizing steady solution, which corresponds to a conditional covariance matrix of some Gaussian state. In subsection 3.2, we further prove that the corresponding Gassian state is pure. Then in subsection 3.3, we provide algebraic characterization of how to prepare a pure Gaussian state with the desired covariance matrix.

3.1 Stabilizing steady solution of the Riccati equation

Above all, we present the following lemma (Theorem 3.4 in [Zhou, Doyle, & Glover, 1995]) concerning the properties of detectability, which is to be utilized in the main results.

Lemma 1.

The following are equivalent:
(i) [C,A][C,~{}A] is detectable;
(ii) The matrix [AλIC]\begin{bmatrix}A-\lambda I\\ C\end{bmatrix} has full column rank for all Re(λ)0\textrm{Re}(\lambda)\geq 0;
(iii) For all λ\lambda and x0x\neq 0 such that Ax=λxAx=\lambda x and Re(λ)0\textrm{Re}(\lambda)\geq 0, Cx0Cx\neq 0;
(iv) There exists a matrix FF such that A+FCA+FC is stable, i.e., all the eigenvalues of A+FCA+FC have negative real parts;
(v) (A,C)(A^{\top},~{}C^{\top}) is stabilizable.

The definition of stabilizing steady solution is defined as the following.

Definition 1.

A matrix VV is called a stabilizing steady solution of (8), if

(i) it satisfies the algebraic Riccati equation

AV+VA+N(VC+M)(VC+M)=0,AV+VA^{\top}+N-(VC^{\top}+M)(VC^{\top}+M)^{\top}=0,

or, equivalently,

(AMC)V+V(AMC)VCCV+14JCCJ=0,(A-MC)V+V(A-MC)^{\top}-VC^{\top}CV+\frac{1}{4}JC^{\top}CJ^{\top}=0, (11)

where

AMC=J(G+12i(ΛΛΛΛ))2m×2m.A-MC=J\Big{(}G+\frac{1}{2i}(\Lambda^{\top}\Lambda-\Lambda^{\dagger}\Lambda^{*})\Big{)}\in\mathbb{R}^{2m\times 2m}.

(ii) AMCVCCA-MC-VC^{\top}C is stable, i.e., all the eigenvalues of AMCVCCA-MC-VC^{\top}C sit in the left half plane.

Now we provide necessary and sufficient conditions for the Riccati equation (8) to have a unique stabilizing steady solution, which corresponds to a quantum Gaussian state.

Theorem 1.

The Riccati equation (8) has a unique stabilizing steady solution VV which is positive semidefinite if and only if [C,A][C,~{}A] is detectable.

Proof: Sufficiency: Firstly, according to Theorem 13.7 in [Zhou, Doyle, & Glover, 1995], if

  1. 1.

    [C,AMC][C,~{}A-MC] is detectable, and

  2. 2.

    [CJ,(AMC)][CJ^{\top},~{}(A-MC)^{\top}] has no unobservable modes on the imaginary axis,

then the Riccati equation (11) has a unique stabilizing solution VV, i.e., AMCVCCA-MC-VC^{\top}C is stable. Moreover, VV is positive semidefinite.

Secondly, let us prove that [CJ,(AMC)][CJ^{\top},~{}(A-MC)^{\top}] has no unobservable modes on the imaginary axis if [C,AMC][C,~{}A-MC] is detectable. Suppose, on the contrary, that [CJ,(AMC)][CJ^{\top},~{}(A-MC)^{\top}] has an unobservable mode on the imaginary axis. From Lemma 1, there exists ww\in\mathbb{R} and a corresponding x0x\neq 0, such that

(AMC)x\displaystyle(A-MC)^{\top}x =iwx,\displaystyle=iwx,
CJx\displaystyle CJ^{\top}x =0.\displaystyle=0.

Thus, we have

(AMC)Jx\displaystyle(A-MC)J^{\top}x =J(G+12i(ΛΛΛΛ))Jx\displaystyle=J(G+\frac{1}{2i}(\Lambda^{\top}\Lambda-\Lambda^{\dagger}\Lambda^{*}))J^{\top}x
=J(AMC)x\displaystyle=J(A-MC)^{\top}x
=Jiwx\displaystyle=Jiwx
=iwJx\displaystyle=-iwJ^{\top}x

Combining this conclusion with CJx=0CJ^{\top}x=0 contradicts with the condition that [C,AMC][C,~{}A-MC] is detectable. Thus, [CJ,(AMC)][CJ^{\top},~{}(A-MC)^{\top}] has no unobservable modes on the imaginary axis if [C,AMC][C,A-MC] is detectable. Moreover, it is straightforward to verify that [C,AMC][C,~{}A-MC] being detectable is equivalent to [C,A][C,~{}A] being detectable.

Necessity: Since the unique stabilizing solution of the Riccati equation (11) can be represented as [Zhou, Doyle, & Glover, 1995]

V=\displaystyle V= 0e((AMC)CCV)t(VCCV\displaystyle\int_{0}^{\infty}\textrm{e}^{\big{(}(A-MC)^{\top}-C^{\top}CV\big{)}^{\top}t}~{}\big{(}VC^{\top}CV
+14JCCJ)e((AMC)CCV)tdt,\displaystyle+\frac{1}{4}JC^{\top}CJ^{\top}\big{)}~{}\textrm{e}^{\big{(}(A-MC)^{\top}-C^{\top}CV\big{)}t}dt,

the matrix (AMC)CCV(A-MC)^{\top}-C^{\top}CV should be stable. This implies that [(AMC),C][(A-MC)^{\top},~{}C^{\top}] is stabilizable, and [C,A][C,~{}A] is detectable accordingly.   \blacksquare

Remark 3.1.

A similar result was also given in [Wiseman & Milburn, 2010], while our proof is different from that there. In existing results, to ensure the system described by (9) to have a unique steady state, the system matrix AA is usually supposed to be stable. However, under the continuous measurement and quantum filtering framework, Theorem 1 provides a much weaker condition for the Riccati equation concerning the conditional covariance matrix to have a unique stabilizing steady solution.

It can be seen that if [C,A][C,~{}A] is detectable, AMCVCCA-MC-VC^{\top}C is stable, and the solution of (10) will approximately approach to 0.

From Theorem 1, if [C,A][C,~{}A] is detectable, then there is a unique stabilizing solution of the Riccati equation (11) satisfying V0V\geq 0. But as a covariance matrix depicting quantum Gaussian state, VV must satisfy the Heisenberg uncertainty principle,

V±i2J.V\geq\pm\frac{i}{2}J.

In fact, V±i2JV\geq\pm\frac{i}{2}J essentially implies V>0V>0 as proved in [Pirandola, Serafini, & Lloyd, 2009].

A necessary and sufficient condition for the solution VV of the Riccati equation (11) to satisfy the Heisenberg uncertainty principle is given in Theorem 2.

Theorem 2.

The Riccati equation (8) has a unique stabilizing steady solution VV satisfying V±i2JV\geq\pm\frac{i}{2}J if and only if [C,A][C,~{}A] is detectable.

Since the proof of Theorem 2 involves a Riccati equation in the complex field. We introduce two lemmas for Riccati equations in the complex field.

Lemma 3.2.

Suppose Fn×n,On×m,F\in\mathbb{C}^{n\times n},~{}O\in\mathbb{C}^{n\times m}, and Zk×nZ\in\mathbb{C}^{k\times n}. If [O,F][O^{\dagger},~{}F^{\dagger}] is detectable and [Z,F][Z,F] has no unobservable modes on the imaginary axis, then the Riccati equation for XX

FX+XFXOOX+ZZ=0F^{\dagger}X+XF-XOO^{\dagger}X+Z^{\dagger}Z=0

has a unique stabilizing solution which is positive semidefinite.

The proof of Lemma 3.2 is presented in Appendix B by analyzing the Riccati equation in the complex domain (see Appendix A).

Lemma 3.3.

[CJ,(AMC)][CJ^{\top},~{}(A-MC)^{\top}] has no unobservable modes on the imaginary axis if and only if AMCi2JCTCA-MC-\frac{i}{2}JC^{T}C has no eigenvalues on the imaginary axis.

Proof: Sufficiency: Suppose, on the contrary, that [CJ,(AMC)][CJ^{\top},~{}(A-MC)^{\top}] has an unobservable mode on the imaginary axis. Then there exists λ\lambda\in\mathbb{R} and a corresponding vector x0x\neq 0, such that

(AMC)x\displaystyle(A-MC)^{\top}x =iλx,\displaystyle=i\lambda x,
CJx\displaystyle CJ^{\top}x =0.\displaystyle=0.

Thus, we have

(AMCi2JCC)x\displaystyle(A-MC-\frac{i}{2}JC^{\top}C)^{\top}x
=\displaystyle= (AMC)xi2CCJx\displaystyle(A-MC)^{\top}x-\frac{i}{2}C^{\top}CJ^{\top}x
=\displaystyle= iλx,\displaystyle i\lambda x,

which contradicts with the condition that AMCi2JCCA-MC-\frac{i}{2}JC^{\top}C has no eigenvalues on the imaginary axis.

Necessity: Suppose AMCi2JCCA-MC-\frac{i}{2}JC^{\top}C has an eigenvalue on the imaginary axis. Then there exists λ\lambda\in\mathbb{R} and a corresponding vector x0x\neq 0, such that

(AMCi2JCC)x=iλx.(A-MC-\frac{i}{2}JC^{\top}C)x=i\lambda x. (12)

Multiplying the above equation from left by xJx^{\dagger}J^{\top} yields

xJ(AMCi2JCC)x\displaystyle x^{\dagger}J^{\top}(A-MC-\frac{i}{2}JC^{\top}C)x
=\displaystyle= x(G+12i(ΛΛΛΛ))xi2xCCx,\displaystyle x^{\dagger}\big{(}G+\frac{1}{2i}(\Lambda^{\top}\Lambda-\Lambda^{\dagger}\Lambda^{*})\big{)}x-\frac{i}{2}x^{\dagger}C^{\top}Cx,
=\displaystyle= iλxJx.\displaystyle i\lambda x^{\dagger}J^{\top}x.

Since (xJx)=xJx(x^{\dagger}Jx)^{\dagger}=-x^{\dagger}Jx is a pure imaginary number and G+12i(ΛΛΛΛ)G+\frac{1}{2i}(\Lambda^{\top}\Lambda-\Lambda^{\dagger}\Lambda^{*}) as well as CCC^{\top}C are real symmetric matrices, we have Cx=0Cx=0, and (AMC)x=iλx(A-MC)x=i\lambda x from (12), accordingly. Then, since (AMC)J=J(AMC)(A-MC)J^{\top}=J(A-MC)^{\top}, we have

(AMC)Jx\displaystyle(A-MC)^{\top}Jx =J(AMC)JJx\displaystyle=J^{\top}(A-MC)J^{\top}Jx
=Jiλx\displaystyle=J^{\top}i\lambda x
=iλJx,\displaystyle=-i\lambda Jx,
CJJx\displaystyle CJ^{\top}Jx =0,\displaystyle=0,

which contradicts with the condition that [CJ,(AMC)][CJ^{\top},~{}(A-MC)^{\top}] has no unobservable modes on the imaginary axis.

Thus, [CJT,(AMC)T][CJ^{T},~{}(A-MC)^{T}] has no unobservable modes on the imaginary axis if and only if AMCi2JCTCA-MC-\frac{i}{2}JC^{T}C has no eigenvalues on the imaginary axis.   \blacksquare

Now we give the proof of Theorem 2.

Proof: Sufficiency: From Theorem 1, if [C,A][C,~{}A] is detectable, then the Riccati equation (8)(\ref{conditioncovariance}) has a unique stabilizing steady solution VV which is positive semidefinite. Since VV is real and symmetric, and JJ is antisymmetric, we just need to prove Vi2JV\geq\frac{i}{2}J.

Suppose Y=Vi2JY=V-\frac{i}{2}J. From (11)(\ref{riccati}) we have the Riccati equation for YY as

(AMC\displaystyle(A-MC- i2JCC)Y+Y(AMCi2JCC)\displaystyle\frac{i}{2}JC^{\top}C)Y+Y(A-MC-\frac{i}{2}JC^{\top}C)^{\dagger} (13)
YCCY=0.\displaystyle-YC^{\top}CY=0.

From the proof of Theorem 1, if [C,AMC][C,~{}A-MC] is detectable, then [CJ,(AMC)][CJ^{\top},~{}(A-MC)^{\top}] has no unobservable modes on the imaginary axis. This conclusion combined with Lemma 3.3 implies that AMCi2JCCA-MC-\frac{i}{2}JC^{\top}C has no eigenvalues on the imaginary axis. Thus, [0,(AMCi2JCC)][0,(A-MC-\frac{i}{2}JC^{\top}C)^{\dagger}] has no unobservable modes on the imaginary axis. Moreover, [C,AMCi2JCC][C,~{}A-MC-\frac{i}{2}JC^{\top}C] is detectable if [C,A][C,~{}A] is detectable. According to Lemma 3.2, the Riccati equation (13) for YY has a unique stabilizing solution which is positive semidefinite, i.e., Vi2JV\geq\frac{i}{2}J, if [C,A][C,~{}A] is detectable.

Necessity: It can be obtained from the necessity part of Theorem 1.   \blacksquare

3.2 Stabilizing steady pure Gaussian state

From Theorem 2 we can see that if [C,A][C,~{}A] is detectable, then the stabilizing steady state solution of (8) corresponds to a conditional covariance matrix of some Gaussian state. Since pure Gaussian states of continuous variable systems are the key ingredients of secure optical communications and Heisenberg limited interferometry, the characterization of pure Gaussian states has attracted much attention.

Note that the purity of a mm mode Gaussian state is simply

Tr[ρ^2]=12mdet[V].\textrm{Tr}[\hat{\rho}^{2}]=\frac{1}{2^{m}\sqrt{\textrm{det}[V]}}.

In [Koga & Yamamoto, 2012], by utilizing a dissipation-induced approach on the basis of the model (9), an explicit algebraic characterization of the purity of Gaussian state was given. For the model (9), to have a unique stabilizing steady pure state with covariance matrix VsV_{s}, besides AA being stable, VsV_{s} must satisfy the following matrix equations:

(Vs+i2J)Λ=0,JGVs+VsGJ=0.(V_{s}+\frac{i}{2}J)\Lambda^{\top}=0,~{}JGV_{s}+V_{s}GJ^{\top}=0. (14)

However, these matrix equations are not easy to verify without knowing the solution VsV_{s}.

A natural question is whether the unique stabilizing steady solution VV of the Riccati equation (8) satisfying V±i2JV\geq\pm\frac{i}{2}J corresponds to some pure Gaussian state. The following Theorem 3 gives an affirmative answer.

Theorem 3.

If [C,A][C,~{}A] is detectable, then the Riccati equation (8) has a unique stabilizing steady solution VV, which can be considered as a conditional covariance matrix of some pure Gaussian state.

Proof: To prove the steady state being pure, we resort to the correspondence of Gaussian states between the Schro¨\ddot{\textrm{o}}dinger picture and the Heisenberg picture.

Consider the following stochastic master equation of ρ^t\hat{\rho}_{t} starting from an initial pure Gaussian state ρ^0\hat{\rho}_{0},

dρ^t=[ρ^t]dt+i=1m(L^iρ^t+ρ^tL^iTr[ρ^t(L^i+L^i)]ρ^t)dwi,t,d\hat{\rho}_{t}=\mathcal{L}^{\dagger}[\hat{\rho}_{t}]dt+\sum_{i=1}^{m}\Big{(}\hat{L}_{i}\hat{\rho}_{t}+\hat{\rho}_{t}\hat{L}^{\dagger}_{i}-\text{Tr}[\hat{\rho}_{t}(\hat{L}_{i}+\hat{L}_{i}^{\dagger})]\hat{\rho}_{t}\Big{)}dw_{i,t}, (15)

where the innovations

dwi,t=dyi,tρ^t,L^i+L^idtdw_{i,t}=d{y}_{i,t}-\langle\hat{\rho}_{t},\hat{L}_{i}+\hat{L}_{i}^{\dagger}\rangle dt

are Gaussian, and

[ρ^t]=i[H^,ρ^t]+i=1m(L^iρ^tL^i12L^iL^iρ^t12ρ^tL^iL^i).\mathcal{{L}}^{\dagger}[\hat{\rho}_{t}]=-i[\hat{H},\hat{\rho}_{t}]+\sum_{i=1}^{m}(\hat{L}_{i}\hat{\rho}_{t}\hat{L}_{i}^{\dagger}-\frac{1}{2}\hat{L}_{i}^{\dagger}\hat{L}_{i}\hat{\rho}_{t}-\frac{1}{2}\hat{\rho}_{t}\hat{L}_{i}^{\dagger}\hat{L}_{i}).

It is straightforward to verify that

dTr(ρ^t2)=0.d~{}\text{Tr}(\hat{\rho}^{2}_{t})=0.

This combined with the initial state ρ^0\hat{\rho}_{0} being pure implies that the state ρ^t\hat{\rho}_{t} is pure for all time tt. Physically this means that if the initial state is pure and there is no information loss during the measurement process, then the state will always be pure.

Moreover, the evolution (15) preserves the Gaussian property. Thus (15) can be fully depicted by the equations of the first- and second-moment in the Heisenberg picture whose dynamics are the same as (7) and (8), while the initial values should correspond to the pure state ρ^0\hat{\rho}_{0}, respectively. Recall that the purity of the Gaussian state only depends on the second moment. Hence, from the correspondence between the Schro¨\ddot{\textrm{o}}dinger picture and the Heisenberg picture for Gaussian states, if (8) has a unique stabilizing steady solution, it must correspond to a pure Gaussian state. Thus, from Theorem 2, if [C,A][C,~{}A] is detectable, then the Riccati equation (8) has a unique stabilizing steady solution VV, which can be considered as a conditional covariance matrix of some pure Gaussian state.    \blacksquare

To prepare a Gaussian state, the approach via continuous measurement has the following advantages:

(i) From Theorem 3, to prepare a pure Gaussian state, the conditions that need to be satisfied via the continuous measurement are much weaker as compared with conditions given by the dissipation-induced approach.

(ii) For the unconditional approach, if VsV_{s} is a unique steady pure state of (9), then it must also be a unique steady pure state of the conditional covariance matrix equation (8). This is because that VsV_{s} being a unique steady pure state of (9) is equivalent to that (14) holds. This further yields

VsC+M=0.V_{s}C^{\top}+M=0.

Thus, (8) and (9) have the same steady pure state.

(iii) Under the same system Hamiltonian and coupling operators, the conditional covariance matrix VcV_{\text{c}} obtained via continuous measurement approach evolving under (8) takes the form [Giovanni, Brunelli, & Genoni, 2021]

Vunc=Vc+Σ,V_{\text{unc}}=V_{c}+\Sigma,

where VuncV_{\text{unc}} obeys (9), and

Σ=E[X¯cX¯c+X¯cX¯c](E[X¯c]E[X¯c]+E[X¯c]E[X¯c]),\Sigma=\textrm{E}[\bar{X}_{c}\bar{X}_{c}^{\top}+\bar{X}_{c}^{\top}\bar{X}_{c}]-\Big{(}\textrm{E}[\bar{X}_{c}]\textrm{E}[\bar{X}_{c}^{\top}]+\textrm{E}[\bar{X}_{c}^{\top}]\textrm{E}[\bar{X}_{c}]\Big{)},

with X¯c\bar{X}_{c} obeying (7). Note that the Gaussian state which corresponds to VuncV_{\text{unc}} may be mixed. Since most of the useful properties of a Gaussian state are determined by the covariance matrix, generally the smaller the covariance matrix (in the matrix partial order) is, the more useful the Gaussian state is. Thus, continuous measurement approach can prepare more useful Gaussian states under the same system parameters.

To better illustrate the advantage of the conditional method in preparing pure Gaussian states, we give a single mode example.

Example 1. Consider the Hamiltonian as

H^=κa^2+a^2+a^a^+a^a^2=κq^2,\hat{H}=\kappa\frac{\hat{a}^{2}+\hat{a}^{\dagger 2}+\hat{a}^{\dagger}\hat{a}+\hat{a}\hat{a}^{\dagger}}{2}=\kappa\hat{q}^{2},

with κ\kappa the damping rate of the cavity. The corresponding GG matrix is G=(2κ000)G=\begin{pmatrix}2\kappa&0\\ 0&0\end{pmatrix}. It can be verified that there does not exist a positive definite matrix VV such that it satisfies the second equation of (14). In other words, if the system Hamiltonian is H^=κq^2\hat{H}=\kappa\hat{q}^{2}, no matter how to choose the coupling operator L^\hat{L}, no pure Gaussian states can be prepared by utilizing the dissipation-induced (unconditional) approach.

Now we employ the conditional approach, and verify that pure Gaussian states can be prepared via continuous measurement. We take V=12(1001)V=\frac{1}{2}\begin{pmatrix}1&0\\ 0&1\end{pmatrix} as an example. It is clear that VV corresponds to a pure Gaussian state. To prepare it, select the measurement operator as

L^=κ((222i)a^22ia^)=κ((1i)q^+ip^).\hat{L}=\sqrt{\kappa}\Big{(}(\sqrt{2}-\frac{\sqrt{2}}{2}i)\hat{a}-\frac{\sqrt{2}}{2}i\hat{a}^{\dagger}\Big{)}=\sqrt{\kappa}\Big{(}(1-i)\hat{q}+i\hat{p}\Big{)}.

The corresponding parameters are

Λ=κ(1i,i),C=κ(2,0),AMC=(κ00κ).\Lambda=\sqrt{\kappa}(1-i,~{}i),~{}C=\sqrt{\kappa}(2,0),~{}A-MC=\begin{pmatrix}\kappa&0\\ 0&-\kappa\end{pmatrix}.

It can be verified that [C,AMC][C,~{}A-MC] is detectable, and V=12(1001)V=\frac{1}{2}\begin{pmatrix}1&0\\ 0&1\end{pmatrix} is a solution of (11).

3.3 Prepare a Gaussian state with desired covariance matrix

In this subsection, we give an algebraic characterization of how to prepare a Gaussian state with the desired covariance matrix. Let the complex matrix Λ\Lambda be decomposed into

Λ=R+iIm\Lambda=\textrm{R}+i\textrm{Im}

with its real part Rm×2m\textrm{R}\in\mathbb{R}^{m\times 2m} and imaginary part Imm×2m\textrm{Im}\in\mathbb{R}^{m\times 2m}, respectively.

Theorem 4.

Let VsV_{s} be a covariance matrix corresponding to a pure Gaussian state. Then, this is a unique stabilizing steady solution of (8) if the following two conditions hold:
(i) Rank(RVsJ R)=2m\text{Rank}\begin{pmatrix}\textrm{R}V_{s}J\\ \textrm{ R}\end{pmatrix}=2m;
(ii) G=RIm ImR+2JVsRR+2RRVsJG=-\textrm{R}^{\top}\textrm{Im }-\textrm{Im}^{\top}\textrm{R}+2J^{\top}V_{s}\textrm{R}^{\top}\textrm{R}+2\textrm{R}^{\top}\textrm{R}V_{s}J.

Proof: We first prove that VsV_{s} is a solution of (11) if condition (ii) is satisfied. By substituting Λ=R+iIm\Lambda=\textrm{R}+i\textrm{Im} into (11), this is equivalent to prove that VsV_{s} satisfies

J(G+RIm+ImR)Vs+Vs(G+RIm+ImR)J\displaystyle J(G+\textrm{R}^{\top}\textrm{Im}+\textrm{Im}^{\top}\textrm{R})V_{s}+V_{s}(G+\textrm{R}^{\top}\textrm{Im}+\textrm{Im}^{\top}\textrm{R})J^{\top}
4VsRRVs+JRRJ=0.\displaystyle-4V_{s}\textrm{R}^{\top}\textrm{R}V_{s}+J\textrm{R}^{\top}\textrm{R}J^{\top}=0.

Multiplying the above equation by JJ^{\top} from left and by JJ from right, we have the following equivalent equation

(G+R Im+ImR)VsJ+JVs(G+RIm+ImR)\displaystyle(G+\textrm{R}^{\top}\textrm{ Im}+\textrm{Im}^{\top}\textrm{R})V_{s}J+J^{\top}V_{s}(G+\textrm{R}^{\top}\textrm{Im}+\textrm{Im}^{\top}\textrm{R}) (16)
4JVsRRVsJ+RR=0.\displaystyle-4J^{\top}V_{s}\textrm{R}^{\top}\textrm{R}V_{s}J+\textrm{R}^{\top}\textrm{R}=0.

Since VsV_{s} corresponds to a pure Gaussian state, we have [Wolf, Giedke, Kru¨\ddot{\textrm{u}}ger, Werner, & Cirac, 2004]

JVsJVs=I4.JV_{s}JV_{s}=-\frac{I}{4}.

Then RR\textrm{R}^{\top}\textrm{R} can be expressed as

RR=2RRVsJVsJ2JVsJVsRR.\textrm{R}^{\top}\textrm{R}=-2\textrm{R}^{\top}\textrm{R}V_{s}JV_{s}J-2J^{\top}V_{s}J^{\top}V_{s}\textrm{R}^{\top}\textrm{R}.

Substituting this expression of RR\textrm{R}^{\top}\textrm{R} into the left hand side of (16), we have

(G+R Im+ImR2JVsRR2RRVsJ)VsJ\displaystyle~{}~{}~{}(G+\textrm{R}^{\top}\textrm{ Im}+\textrm{Im}^{\top}\textrm{R}-2J^{\top}V_{s}\textrm{R}^{\top}\textrm{R}-2\textrm{R}^{\top}\textrm{R}V_{s}J)V_{s}J
+JVs(G+RIm +ImR2JVsRR2RRVsJ)\displaystyle+J^{\top}V_{s}(G+\textrm{R}^{\top}\textrm{Im }+\textrm{Im}^{\top}\textrm{R}-2J^{\top}V_{s}\textrm{R}^{\top}\textrm{R}-2\textrm{R}^{\top}\textrm{R}V_{s}J)
=0,\displaystyle=0,

if condition (ii) is met. Thus VsV_{s} is a solution of (11).

Now we prove that VsV_{s} is a unique stabilizing steady solution of (8). According to Theorem 2, we just need to prove that conditions (i) and (ii) imply that [C,AMC][C,~{}A-MC] is detectable. On the contrary, there exists λ\lambda with Re(λ)0\textrm{Re}(\lambda)\geq 0, and a corresponding eigenvector xx, such that

(AMC)x\displaystyle(A-MC)x =λx,\displaystyle=\lambda x,
Rx\displaystyle\textrm{R}~{}x =0.\displaystyle=0.

By utilizing condition (ii) and after some calculations, we have

2RRVsJx=λJx.\displaystyle 2\textrm{R}^{\top}\textrm{R}V_{s}Jx=-\lambda Jx.

Multiplying this equation by xJVsx^{\dagger}J^{\top}V_{s} from left yields

2xJVsRVsJx=λxJVsJx.\displaystyle 2x^{\dagger}J^{\top}V_{s}\textrm{R}^{\top}\textrm{R }V_{s}Jx=-\lambda x^{\dagger}J^{\top}V_{s}Jx. (17)

Note that condition (i) Rank(RVsJR)=2m\text{Rank}\begin{pmatrix}\textrm{R}V_{s}J\\ \textrm{R}\end{pmatrix}=2m and Rx=0\textrm{R}x=0 imply that RVsJx0\textrm{R}V_{s}Jx\neq 0. Thus, xJVsRRVsJx>0x^{\dagger}J^{\top}V_{s}\textrm{R}^{\top}\textrm{R}V_{s}Jx>0. In addition, since VsV_{s} corresponds to a Gaussian state, this yields Vs>0V_{s}>0, and xJVsJx>0x^{\dagger}J^{\top}V_{s}Jx>0 accordingly. Then from (17), λ<0\lambda<0. But this contradicts with Re(λ)0\textrm{Re}(\lambda)\geq 0. Therefore, [C,AMC][C,~{}A-MC] is detectable. Hence, VsV_{s} is a unique stabilizing steady solution of (8) under conditions (i) and (ii).   \blacksquare

Remark 3.4.

Under condition (ii) in Theorem 4, condition (i) holds if and only if [C,AMC][C,~{}A-MC] is detectable. The necessity part has been proven in the proof of Theorem 4. To prove the sufficiency, we first note that under condition (ii), [C,AMC][C,~{}A-MC] being detectable is equivalent to [R,JRRVsJ][\textrm{R},~{}J\textrm{R}^{\top}\textrm{R}V_{s}J] being detectable. Further, if condition (i) does not hold, then there exists x0x\neq 0, such that RVsJx=0\textrm{R}V_{s}Jx=0 and Rx=0\textrm{R}x=0. This clearly contradicts with [R,JRRVsJ][\textrm{R},~{}J\textrm{R}^{\top}\textrm{R}V_{s}J] being detectable.

Remark 3.5.

To make condition (i) of Theorem 4 hold, there are a lot of degrees of freedom to choose R. Here we give a simple choice such that R=(I0)\textrm{R}=\begin{pmatrix}I&0\end{pmatrix}, where II is the m×mm\times m identity matrix and 0 is the m×mm\times m null matrix. Now let us check conditon (i). Given a target covariance matrix VsV_{s} described by

Vs=(V11V12V12V22),V_{s}=\begin{pmatrix}V_{11}&V_{12}\\ V_{12}^{\top}&V_{22}\end{pmatrix},

since it corresponds to a pure Gaussian state,

V11=V11>0andV22=V22>0.V_{11}=V_{11}^{\top}>0~{}and~{}V_{22}=V_{22}^{\top}>0.

Then we have RVsJ=(V12V11).\textrm{R}V_{s}J=\begin{pmatrix}-V_{12}&V_{11}\end{pmatrix}. It is clear that

Rank(RVsJ R)=Rank(V12V11I0)=2m.\text{Rank}\begin{pmatrix}\textrm{R}V_{s}J\\ \textrm{ R}\end{pmatrix}=\textrm{Rank}\begin{pmatrix}-V_{12}&V_{11}\\ I&0\end{pmatrix}=2m.
Remark 3.6.

Note that in Theorem 4, to prepare a desired pure Gaussian state with covariance matrix VsV_{s}, there is no restriction on the imaginary part of the coupling matrix Λ\Lambda, which is helpful to relax the restrictions of experimental realizations.

4 Imperfect detection efficiency

In practical applications, we may not be able to achieve perfect detection efficiency and the imperfect efficiency η<1\eta<1 may have significant impact on the performance in preparing Gaussian states. In this section we consider the case where the detection efficiency η<1\eta<1. Here we assume that all the detection efficiencies are the same for simplicity. In this case the dynamics of the conditional state ρ^tc\hat{\rho}^{c}_{t} is described by

dρ^tc=\displaystyle d\hat{\rho}_{t}^{c}= [ρ^tc]dt\displaystyle\mathcal{L}^{\dagger}[\hat{\rho}^{c}_{t}]dt (18)
+\displaystyle+ ηi=1m(L^iρ^tc+ρ^tcL^iTr[ρ^tc(L^i+L^i)]ρ^tc)dwi,t,\displaystyle\sqrt{\eta}\sum_{i=1}^{m}\Big{(}\hat{L}_{i}\hat{\rho}^{c}_{t}+\hat{\rho}^{c}_{t}\hat{L}^{\dagger}_{i}-\text{Tr}[\hat{\rho}^{c}_{t}(\hat{L}_{i}+\hat{L}_{i}^{\dagger})]\hat{\rho}^{c}_{t}\Big{)}dw_{i,t},

where the innovations

dwi,t=dyi,tηρ^tc,L^i+L^idtdw_{i,t}=d{y}_{i,t}-\sqrt{\eta}\langle\hat{\rho}^{c}_{t},\hat{L}_{i}+\hat{L}_{i}^{\dagger}\rangle dt

are Gaussian, and

[ρ^tc]=i[H^,ρ^tc]+i=1m(L^iρ^tcL^i12L^iL^iρ^tc12ρ^tcL^iL^i).\mathcal{{L}}^{\dagger}[\hat{\rho}_{t}^{c}]=-i[\hat{H},\hat{\rho}_{t}^{c}]+\sum_{i=1}^{m}(\hat{L}_{i}\hat{\rho}_{t}^{c}\hat{L}_{i}^{\dagger}-\frac{1}{2}\hat{L}_{i}^{\dagger}\hat{L}_{i}\hat{\rho}_{t}^{c}-\frac{1}{2}\hat{\rho}_{t}^{c}\hat{L}_{i}^{\dagger}\hat{L}_{i}).

If the initial state is pure Gaussian, (18) still preserves the Gaussian nature. However, due to the imperfect detection, there is information loss during the measurement. This leads to that the Gaussian state may become mixed as the state evolving.

For the mm mode system considered in subsection 2.3, the first- and second-moment equations corresponding to (7) and (8) become

dX¯t\displaystyle d\bar{X}_{t} =(AX¯t+But)dt+η(VtC+M)dy~t,\displaystyle=(A\bar{X}_{t}+Bu_{t})dt+\sqrt{\eta}(V_{t}C^{\top}+M)d\tilde{y}_{t}, (19)
ddtVt\displaystyle\frac{d}{dt}V_{t} =AVt+VtA+Nη(VtC+M)(VtC+M).\displaystyle=AV_{t}+V_{t}A^{\top}+N-\eta(V_{t}C^{\top}+M)(V_{t}C^{\top}+M)^{\top}.

If VV is a stabilizing steady solution of (19), then VV needs to satisfy the following Riccati equation

AV+VA+Nη(VC+M)(VC+M)=0,AV+VA^{\top}+N-\eta(VC^{\top}+M)(VC^{\top}+M)^{\top}=0,

which is equivalent to

(AηMC)V\displaystyle(A-\eta MC)V +V(AηMC)\displaystyle+V(A-\eta MC)^{\top} (20)
ηVCCV+NηMM=0.\displaystyle-\eta VC^{\top}CV+N-\eta MM^{\top}=0.

Similar to Theorem 2 where the detection efficiency η=1\eta=1, we have the following conclusion.

Theorem 5.

The Riccati equation (19) has a unique stabilizing steady solution satisfying V±i2JV\geq\pm\frac{i}{2}J if and only if [C,AMC][C,~{}A-MC] is detectable.

To prove Theorem 5, we first rearrange (19) into the following form

(AηMC)V+V(AηMC)ηVCCV+QVQV=0,(A-\eta MC)V+V(A-\eta MC)^{\top}-\eta VC^{\top}CV+Q_{V}^{\top}Q_{V}=0,

where QV=[R1ηIm]JQ_{V}=\begin{bmatrix}\textrm{R}\\ \sqrt{1-\eta}~{}\textrm{Im}\end{bmatrix}J^{\top}. We have the following lemma.

Lemma 4.7.

[QV,(AηMC)][Q_{V},~{}(A-\eta MC)^{\top}] has no unobservable modes on the imaginary axis if [C,AMC][C,~{}A-MC] is detectable.

Proof: Suppose, on the contrary, that there exists λ\lambda\in\mathbb{R} and a corresponding vector x0x\neq 0, such that

(AηMC)x=iλx,\displaystyle(A-\eta MC)^{\top}x=i\lambda x,
QVx=[R1ηIm]Jx=0.\displaystyle Q_{V}x=\begin{bmatrix}\textrm{R}\\ \sqrt{1-\eta}\textrm{Im}\end{bmatrix}J^{\top}x=0.

We have CJx=2RJx=0CJ^{\top}x=2RJ^{\top}x=0. Moreover, since

(AηMC)J=J(AηMC),(A-\eta MC)J^{\top}=J(A-\eta MC)^{\top},

we have

(AηMC)Jx=J(AηMC)x=iλJx,(A-\eta MC)J^{\top}x=J(A-\eta MC)^{\top}x=i\lambda Jx,

which yields

(AηMC)Jx=iλJx.(A-\eta MC)J^{\top}x=-i\lambda J^{\top}x.

Combining this conclusion with CJx=0CJ^{\top}x=0 contradicts with the condition that [C,AMC][C,~{}A-MC] is detectable. Thus, [QV,(AηMC)][Q_{V},~{}(A-\eta MC)^{\top}] has no unobservable modes on the imaginary axis if [C,AMC][C,~{}A-MC] is detectable.   \blacksquare

Secondly, similar to (13), denoting Y=Vi2JY=V-\frac{i}{2}J, we have the Riccati equation about YY as

(AηMCi2ηJCC)Y+Y(AηMCi2ηJCC)\displaystyle(A-\eta MC-\frac{i}{2}\eta JC^{\top}C)Y+Y(A-\eta MC-\frac{i}{2}\eta JC^{\top}C)^{\top}
ηYCCY+QYQY=0,\displaystyle-\eta YC^{\top}CY+Q_{Y}^{\top}Q_{Y}=0,

where QY=1η[RIm]JQ_{Y}=\sqrt{1-\eta}\begin{bmatrix}\textrm{R}\\ \textrm{Im}\end{bmatrix}J^{\top}. Then we have the following lemma.

Lemma 4.8.

[QV,(AηMC)][Q_{V},~{}(A-\eta MC)^{\top}] has no unobservable modes on the imaginary axis if and only if [QY,(AηMCi2ηJCC)][Q_{Y},~{}(A-\eta MC-\frac{i}{2}\eta JC^{\top}C)^{\top}] has no unobservable modes on the imaginary axis.

Proof: Sufficiency: Suppose, on the contrary, that there exists λ\lambda\in\mathbb{R} and a corresponding vector x0x\neq 0, such that

(AηMC)x=iλx,\displaystyle(A-\eta MC)^{\top}x=i\lambda x,
QVx=[R1ηIm]Jx=0.\displaystyle Q_{V}x=\begin{bmatrix}\textrm{R}\\ \sqrt{1-\eta}\textrm{Im}\end{bmatrix}J^{\top}x=0.

Then we have CJx=2RJx=0CJ^{\top}x=2\textrm{R}J^{\top}x=0. Therefore,

(AηMCi2ηJCC)x\displaystyle(A-\eta MC-\frac{i}{2}\eta JC^{\top}C)^{\top}x =(AηMC)x=iλx,\displaystyle=(A-\eta MC)^{\top}x=i\lambda x,
QYx\displaystyle Q_{Y}x =0,\displaystyle=0,

which contradicts with the condition that [QY,(AηMCi2ηJCC)][Q_{Y},(A-\eta MC-\frac{i}{2}\eta JC^{\top}C)^{\top}] has no unobservable modes on the imaginary axis.

Necessity: Suppose there exists λ\lambda\in\mathbb{R} and a corresponding vector x0x\neq 0, such that

(AηMCi2ηJCC)x=iλx,\displaystyle(A-\eta MC-\frac{i}{2}\eta JC^{\top}C)^{\top}x=i\lambda x,
QYx=1η[R Im]Jx=0.\displaystyle Q_{Y}x=\sqrt{1-\eta}\begin{bmatrix}\textrm{R}\\ \textrm{ Im}\end{bmatrix}J^{\top}x=0.

Then we have CJx=0CJ^{\top}x=0. Therefore,

(AηMC)x\displaystyle(A-\eta MC)^{\top}x =(AηMCi2ηJCC)x=iλx,\displaystyle=(A-\eta MC-\frac{i}{2}\eta JC^{\top}C)^{\top}x=i\lambda x,
QVx\displaystyle Q_{V}x =0,\displaystyle=0,

which contradicts with the condition that [QV,(AηMC)][Q_{V},~{}(A-\eta MC)^{\top}] has no unobservable modes on the imaginary axis.

Thus, [QV,(AηMC)][Q_{V},~{}(A-\eta MC)^{\top}] has no unobservable modes on the imaginary axis if and only if [QY,(AηMCi2ηJCC)][Q_{Y},~{}(A-\eta MC-\frac{i}{2}\eta JC^{\top}C)^{\top}] has no unobservable modes on the imaginary axis.   \blacksquare

Now we give the proof of Theorem 5.

Proof: Sufficiency: If [C,AMC][C,~{}A-MC] is detectable, then from Lemma 4.7, [QV,(AηMC)][Q_{V},~{}(A-\eta MC)^{\top}] has no unobservable modes on the imaginary axis. Thus according to Theorem 13.7 in [Zhou, Doyle, & Glover, 1995], the Riccati equation (20) about VV has a unique stabilizing solution which is positive semidefinite.

To prove Vi2JV\geq\frac{i}{2}J, from Lemma 3.2, we just need to verify that [C,AMCi2ηJCC][C,~{}A-MC-\frac{i}{2}\eta JC^{\top}C] is detectable and [QY,(AηMCi2ηJCC)][Q_{Y},(A-\eta MC-\frac{i}{2}\eta JC^{\top}C)^{\top}] has no unobservable modes on the imaginary axis. In fact, as [C,AMC][C,~{}A-MC] is detectable, so is [C,AMCi2ηJCC][C,~{}A-MC-\frac{i}{2}\eta JC^{\top}C]. Moreover, from Lemmas 4.7 and 4.8, [QY,(AηMCi2ηJCC)][Q_{Y},(A-\eta MC-\frac{i}{2}\eta JC^{\top}C)^{\top}] has no unobservable modes on the imaginary axis. Thus, the Riccati equation (19) has a unique stabilizing steady solution satisfying V±i2JV\geq\pm\frac{i}{2}J if [C,AMC][C,~{}A-MC] is detectable.

Necessity: According to [Zhou, Doyle, & Glover, 1995], the solution of (20) has the following form

Y=0\displaystyle Y=\int_{0}^{\infty} e((AηMC)ηCCV)t(ηVCCV\displaystyle\textrm{e}^{\big{(}(A-\eta MC)^{\top}-\eta C^{\top}CV\big{)}^{\top}t}\big{(}\eta VC^{\top}CV
+NηMM)e((AηMC)ηCCV)t.\displaystyle+N-\eta MM^{\top}\big{)}\textrm{e}^{\big{(}(A-\eta MC)^{\top}-\eta C^{\top}CV\big{)}t}.

It is clear that (AηMC)ηCCV(A-\eta MC)^{\top}-\eta C^{\top}CV is stable. This yields [C,AMC][C,~{}A-MC] being detectable.   \blacksquare

Although the Gaussian state may be not pure if the detection is imperfect, the steady solution VcV_{\text{c}} of the conditional covariance matrix equation (19) is still smaller than the steady solution VuncV_{\text{unc}} obtained via the unconditional dissipation-induced approach (9).

5 Conclusion

In this paper we consider the problem of how to prepare Gaussian states via continuous measurement. We present some necessary and sufficient conditions for the conditional dynamics of the covariance matrix to have a unique stabilizing steady solution. This conditional method is much superior to the unconditional approaches in the following two aspects. On one hand, the conditions given by our method is much weaker than those given by the unconditional methods, which may be beneficial to experimental realizations. On the other hand, under the same system parameters, the Gaussian states prepared via the continuous measurement may be more useful in quantum information processing.

{ack}

This work was supported by the National Natural Science Foundation of China (Nos. 11688101, 61773370, 61833010 and 61621003) and the Australian Research Councils Discovery Projects funding scheme under Project DP190101566.

Appendix

Appendix A Riccati equation in the complex domain

In this Appendix, we present some results concerning a matrix Ricaati equation in the complex domain, which are similar to those in Section 13.2 of [Zhou, Doyle, & Glover, 1995], where the domain considered is real.

Let Fn×n,P=Pn×nF\in\mathbb{C}^{n\times n},~{}P=P^{\dagger}\in\mathbb{C}^{n\times n} and K=Kn×nK=K^{\dagger}\in\mathbb{C}^{n\times n}. The matrix Riccati equation to be considered is

FX+XF+XPX+K=0.F^{\dagger}X+XF+XPX+K=0. (21)

We associate a 2n×2n2n\times 2n matrix in the complex domain with the Riccati equation (21) as

H=[FPKF].H=\begin{bmatrix}F&P\\ -K&-F^{\dagger}\end{bmatrix}.

Noting that the 2n×2n2n\times 2n matrix

J=[0II0]J=\begin{bmatrix}0&I\\ -I&0\end{bmatrix}

has the property J2=IJ^{2}=-I. Then we have

J1HJ=JHJ=H.J^{-1}HJ=-JHJ=-H^{\dagger}.

Thus, HH and H-H^{\dagger} are similar. This further implies that λ\lambda is an eigenvalue of HH if and only if λ-{\lambda}^{*} is, where λ\lambda^{*} denotes the conjugate of λ\lambda.

Assume that HH has no eigenvalues on the imaginary axis. Then it must have nn eigenvalues in the left half plane and nn eigenvalues in the right half plane. Denote the corresponding two nn-dimensional spectral subspaces as 𝒳(H)\mathcal{X}_{-}(H) and 𝒳+(H)\mathcal{X}_{+}(H), respectively. To be specific, the former is the invariant subspace corresponding to eigenvalues in the left half plane and the latter corresponds to eigenvalues in the right half plane. By finding a basis of 𝒳(H)\mathcal{X}_{-}(H), stacking the basis vectors up to form a matrix, and partitioning the matrix, we have

𝒳(H)=Span[X1X2],\mathcal{X}_{-}(H)=\textit{Span}\begin{bmatrix}X_{1}\\ X_{2}\end{bmatrix},

where X1,X2n×nX_{1},~{}X_{2}\in\mathbb{C}^{n\times n}. If X1X_{1} is nonsingular, we can define

X=X2X11.X=X_{2}X_{1}^{-1}.

It can be verified that XX is independent of a specific choice of basis of 𝒳(H)\mathcal{X}_{-}(H), and is uniquely determined by HH, which can be described by the map

Ric:HX.\textit{Ric}:H\rightarrow X.

We will take the domain of Ric, denoted by dom(Ric)\textrm{dom}(\textit{Ric}), to consist of matrices HH with the following two properties:

  • Stability property: HH has no eigenvalues on the imaginary axis;

  • Complementarity: the two subspaces 𝒳(H)\mathcal{X}_{-}(H) and span[0I]\textit{span}\begin{bmatrix}0\\ I\end{bmatrix} are complementary, which is equivalent to X1X_{1} being nonsingular.

Now we have Theorem 6 concerning the properties of XX.

Theorem 6.

Suppose Hdom(Ric)H\in\textrm{dom}(\textit{Ric}) and X=Ric(H)X=\textit{Ric}(H). Then

(i) X=XX=X^{\dagger};

(ii) XX satisfies Riccati equation (21), i.e.,

FX+XF+XPX+K=0,F^{\dagger}X+XF+XPX+K=0,

(iii) F+PXF+PX is stable.

Proof: (i) Since Hdom(Ric)H\in\textrm{dom}(\textit{Ric}), there exists a stable matrix denoted by Hn×nH_{-}\in\mathbb{C}^{n\times n}, which is a matrix representation of H|𝒳(H)H|_{\mathcal{X}_{-}(H)}, such that

H[X1X2]=[X1X2]H.H\begin{bmatrix}X_{1}\\ X_{2}\end{bmatrix}=\begin{bmatrix}X_{1}\\ X_{2}\end{bmatrix}H_{-}. (22)

Multiplying this equation from left by [X1X2]J\begin{bmatrix}X_{1}\\ X_{2}\end{bmatrix}^{\dagger}J yields

[X1X2]JH[X1X2]=[X1X2]J[X1X2]H.\begin{bmatrix}X_{1}\\ X_{2}\end{bmatrix}^{\dagger}JH\begin{bmatrix}X_{1}\\ X_{2}\end{bmatrix}=\begin{bmatrix}X_{1}\\ X_{2}\end{bmatrix}^{\dagger}J\begin{bmatrix}X_{1}\\ X_{2}\end{bmatrix}H_{-}.

Noting that JH=(JH)JH=(JH)^{\dagger}, the left hand side of the above equation is Hermitian, and so is the right hand side. Thus, we have

(X1X2+X2X1)H\displaystyle(-X_{1}^{\dagger}X_{2}+X_{2}^{\dagger}X_{1})H_{-} =H(X1X2+X2X1)\displaystyle=H_{-}^{\dagger}(-X_{1}^{\dagger}X_{2}+X_{2}^{\dagger}X_{1})^{\dagger}
=H(X1X2+X2X1).\displaystyle=-H_{-}^{\dagger}(-X_{1}^{\dagger}X_{2}+X_{2}^{\dagger}X_{1}).

This is a Lyapunov equation. Since HH_{-} is stable, the unique solution is

X1X2+X2X1=0.-X_{1}^{\dagger}X_{2}+X_{2}^{\dagger}X_{1}=0.

Since X1X_{1} is nonsingular, XX can be represented as

X=(X1)1X1X2X11.X=(X_{1}^{\dagger})^{-1}X_{1}^{\dagger}X_{2}X_{1}^{-1}.

This combined with X1X2=X2X1X_{1}^{\dagger}X_{2}=X_{2}^{\dagger}X_{1} yields X=XX=X^{\dagger}.

(ii) Start with the equation

H[X1X2]=[X1X2]H.H\begin{bmatrix}X_{1}\\ X_{2}\end{bmatrix}=\begin{bmatrix}X_{1}\\ X_{2}\end{bmatrix}H_{-}.

Multiplying the above equation from right by X11X_{1}^{-1} yields

H[IX]=[IX]X1HX11.H\begin{bmatrix}I\\ X\end{bmatrix}=\begin{bmatrix}I\\ X\end{bmatrix}X_{1}H_{-}X_{1}^{-1}. (23)

Now multiplying from left by [XI]\begin{bmatrix}X&-I\end{bmatrix}, we have

[XI]H[IX]=0.\begin{bmatrix}X&-I\end{bmatrix}H\begin{bmatrix}I\\ X\end{bmatrix}=0.

This is precisely the Riccati equation (21).

(iii) Multiplying (23) from left by [I0]\begin{bmatrix}I&0\end{bmatrix}, we have

F+PX=X1HX11.F+PX=X_{1}H_{-}X_{1}^{-1}.

Thus F+PXF+PX is stable because HH_{-} is stable.   \blacksquare

A solution XX of (21) is called stabilizing if F+PXF+PX is stable. A necessary and sufficient condition for the existence of a unique stabilizing solution of (21) is stated in the following theorem.

Theorem 7.

Suppose HH has no imaginary eigenvalues and PP is either positive semi-definite or negative semi-definite. Then Hdom(Ric)H\in\textrm{dom}(\textit{Ric}) if and only if [P,F][P,~{}F^{\dagger}] is detectable.

Proof: Sufficiency: To prove that Hdom(Ric)H\in\textrm{dom}(\textit{Ric}), we just need to show that X1X_{1} is nonsingular, i.e., Ker(X1)=0\textrm{Ker}(X_{1})=0.

First, let us demonstrate that Ker(X1)\textrm{Ker}(X_{1}) is HH_{-}-invariant, where HH_{-} is given in (22). To prove this, let xKer(X1)x\in\textrm{Ker}(X_{1}). Multiplying (22) from left by [I0]\begin{bmatrix}I&0\end{bmatrix} yields

FX1+PX2=X1H.FX_{1}+PX_{2}=X_{1}H_{-}. (24)

Multiplying the above equation from left by xX2x^{\dagger}X_{2}^{\dagger}, and by xx from right, and recalling the fact that X2X1=(X2X1)X_{2}^{\dagger}X_{1}=(X_{2}^{\dagger}X_{1})^{\dagger}, we have

xX2PX2x=0.x^{\dagger}X_{2}^{\dagger}PX_{2}x=0.

Since PP is semi-definite, this implies that PX2x=0PX_{2}x=0. Then, from (24), we have X1Hx=0X_{1}H_{-}x=0, i.e., HxKer(X1)H_{-}x\in\textrm{Ker}(X_{1}), which proves that Ker(X1)\textrm{Ker}(X_{1}) is HH_{-}-invariant.

Now to prove that X1X_{1} is nonsingular, suppose, on the contrary, that Ker(X1)0\textrm{Ker}(X_{1})\neq 0. Then H|Ker(X1)H_{-}|_{\textrm{Ker}(X_{1})} has an eigenvalue λ\lambda with Re(λ)<0\textrm{Re}(\lambda)<0, and a corresponding eigenvector x0x\neq 0, i.e.,

Hx=λx,Re(λ)<0,\displaystyle H_{-}x=\lambda x,~{}\textrm{Re}(\lambda)<0,
xKer(X1),x0.\displaystyle x\in\textrm{Ker}(X_{1}),~{}x\neq 0.

Multiplying (22) from left by [0I]\begin{bmatrix}0&I\end{bmatrix} yields

KX1FX2=X2H.-KX_{1}-F^{\dagger}X_{2}=X_{2}H_{-}.

Multiplying the above equation by xx from right, we have

(F+λI)X2x=0.(F^{\dagger}+\lambda I)X_{2}x=0.

Since PX2x=0PX_{2}x=0, we have

[F+λIP]X2x=0.\begin{bmatrix}F^{\dagger}+\lambda I\\ P\end{bmatrix}X_{2}x=0.

Then the detectability of [P,F][P,~{}F^{\dagger}] implies X2x=0X_{2}x=0, which contradicts with the fact that [X1X2]\begin{bmatrix}X_{1}\\ X_{2}\end{bmatrix} has full column rank.

Necessity: From Theorem 6, Hdom(Ric)H\in\textrm{dom}(\textit{Ric}) implies that XX is a stabilizing solution such that F+PXF+PX is stable. From (v) of Lemma 1, this further implies that [P,F][P,~{}F^{\dagger}] is detectable.   \blacksquare

Theorem 8.

Suppose HH has the form

H=[FOOZZF].H=\begin{bmatrix}F&-OO^{\dagger}\\ -Z^{\dagger}Z&-F^{\dagger}\end{bmatrix}.

Then,

(i) Hdom(Ric)H\in\textrm{dom}(\textit{Ric}) if and only if [O,F][O^{\dagger},~{}F^{\dagger}] is detectable and [Z,F][Z,~{}F] has no unobservable modes on the imaginary axis;

(ii) X=Ric(H)0X=\textit{Ric}(H)\geq 0 if Hdom(Ric)H\in\textrm{dom}(\textit{Ric});

(iii) Hdom(Ric)H\in\textrm{dom}(\textit{Ric}), then Ker(X)=0\textrm{Ker}(X)=0 if and only if [Z,F][Z,~{}F] has no stable unobservable modes.

Proof: To prove (i), noting that from Theorem 7, the detectability of [O,F][O^{\dagger},~{}F^{\dagger}] is necessary. Hence, from Theorem 7, we only need to show that under the condition [O,F][O^{\dagger},~{}F^{\dagger}] being detectable, HH has no imaginary eigenvalues if and only if [Z,F][Z,~{}F] has no unobservable modes on the imaginary axis.

Suppose that there exists a real ω\omega such that iωi\omega is an eigenvalue of HH, and [xz]0\begin{bmatrix}x\\ z\end{bmatrix}\neq 0 is the corresponding eigenvector. Then, we have

FxOOz=iωx,\displaystyle Fx-OO^{\dagger}z=i\omega x,
ZZxFz=iωz.\displaystyle-Z^{\dagger}Zx-F^{\dagger}z=i\omega z.

Re-arranging the above equation yields

(FiωI)x=OOz,\displaystyle(F-i\omega I)x=OO^{\dagger}z, (25)
(FiωI)z=ZZx.\displaystyle-(F-i\omega I)^{\dagger}z=Z^{\dagger}Zx.

Thus

z(FiωI)x=zOOz=Oz2,\displaystyle z^{\dagger}(F-i\omega I)x=z^{\dagger}OO^{\dagger}z=||O^{\dagger}z||^{2},
x(FiωI)z=xZZx=Zx2.\displaystyle-x^{\dagger}(F-i\omega I)^{\dagger}z=x^{\dagger}Z^{\dagger}Zx=||Zx||^{2}.

Hence, x(FiωI)z\ x^{\dagger}(F-i\omega I)^{\dagger}z is real and

Zx2=x(FiωI)z=z(FiωI)x=Oz2.-||Zx||^{2}=x^{\dagger}(F-i\omega I)^{\dagger}z=z^{\dagger}(F-i\omega I)x=||O^{\dagger}z||^{2}.

Therefore, Zx=0Zx=0 and Oz=0O^{\dagger}z=0. From (25),

(FiωI)x=0,\displaystyle(F-i\omega I)x=0,
(FiωI)z=0.\displaystyle-(F-i\omega I)^{\dagger}z=0.

Combining this with Zx=0Zx=0 and Oz=0O^{\dagger}z=0, we have

[FiωIZ]x=0,\displaystyle\begin{bmatrix}F-i\omega I\\ Z\end{bmatrix}x=0,
[F+iωIO]z=0.\displaystyle\begin{bmatrix}F^{\dagger}+i\omega I\\ O^{\dagger}\end{bmatrix}z=0.

Under the condition that [O,F][O^{\dagger},~{}F^{\dagger}] is detectable, we have z=0z=0, and x0x\neq 0. Now it is straightforward to see that iωi\omega is an eigenvalue of HH if and only if iωi\omega is an unobservable mode of [Z,F][Z,~{}F].

To prove (ii), let X=Ric(H)X=\textit{Ric}(H). The Riccati equation is

FX+XFXOOX+ZZ=0,F^{\dagger}X+XF-XOO^{\dagger}X+Z^{\dagger}Z=0,

or equivalently,

(FOOX)X+X(FOOX)+XOOX+ZZ=0.(F-OO^{\dagger}X)^{\dagger}X+X(F-OO^{\dagger}X)+XOO^{\dagger}X+Z^{\dagger}Z=0. (26)

Noting that FOOXF-OO^{\dagger}X is stable by (iii) of Theorem 6, we have

X=\displaystyle X= 0e(FOOX)t(XOOX+ZZ)e(FOOX)t𝑑t.\displaystyle\int_{0}^{\infty}\textrm{e}^{(F-OO^{\dagger}X)^{\dagger}t}(XOO^{\dagger}X+Z^{\dagger}Z)\textrm{e}^{(F-OO^{\dagger}X)t}dt.

Since XOOX+ZZXOO^{\dagger}X+Z^{\dagger}Z is positive semi-definite, so is XX.

Finally, we prove (iii).

Sufficiency: Let us first show that Ker(X)\textrm{Ker}(X) is an FF-invariant subspace. Suppose xKer(X)x\in\textrm{Ker}(X), then Xx=0Xx=0. Multiplying (26) from left by xx^{\dagger} and right by xx yields

Zx=0.Zx=0.

Now multiply (26) from right by xx to get

XFx=0.XFx=0.

Thus, Ker(X)\textrm{Ker}(X) is FF-invariant.

Now if Ker(X)0\textrm{Ker}(X)\neq 0, then there exists a nonzero xKer(X)x\in\textrm{Ker}(X) and a corresponding λ\lambda such that

Fx\displaystyle Fx =(FOOX)x=λx,\displaystyle=(F-OO^{\dagger}X)x=\lambda x,
Zx\displaystyle Zx =0.\displaystyle=0.

From (iii) of Theorem 6, FOOXF-OO^{\dagger}X is stable, so Re(λ)<0\textrm{Re}(\lambda)<0. Thus, λ\lambda is a stable unobservable mode, which is a contradiction.

Necessity: Suppose, on the contrary, that [Z,F][Z,~{}F] has an unobservable stable mode λ\lambda, i.e., there is x0x\neq 0 such that Fx=λx,Re(λ)<0,Fx=\lambda x,~{}\textrm{Re}(\lambda)<0, and Zx=0Zx=0. By multiplying the Riccati equation (26) from left by xx^{\dagger} and right by xx, we have

2Re(λ)xXxxXOOXx=0.2\textrm{Re}(\lambda)x^{\dagger}Xx-x^{\dagger}XOO^{\dagger}Xx=0.

Since XX is positive semi-definite, i.e., xXx0x^{\dagger}Xx\geq 0, and xXOOXx0x^{\dagger}XOO^{\dagger}Xx\geq 0, we have xXx=0x^{\dagger}Xx=0, i.e., XX is singular, which is a contradiction.   \blacksquare

Appendix B Proof of Lemma 3.2

It is straightforward to see that Lemma 3.2 can be obtained from (i), (ii) of Theorem 8 and (iii) of Theorem 6.

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