Wiener Filtering for Passive Linear Quantum Systems

This paper considers a version of the Wiener filtering problem for equalization of passive quantum linear quantum systems. We demonstrate that taking into consideration the quantum nature of the signals involved leads to features typically not encoun…

Authors: V. Ugrinovskii, M.R. James

Wiener Filtering f or Passiv e Lin ear Quantum Systems V . Ugrinovskii M. R. James Abstract — This paper considers a versio n of the Wiener filtering problem fo r equalization of passiv e quan t um linear quantum systems. W e demonstrate that taking into c onsidera- tion the quantum nature of th e signals inv olved leads t o features typically not encoun tered i n classical equalization problems. Most significantly , findi n g a mean-square optimal quan t u m equalizing filter amounts to solv ing a nonconv ex constrained optimization problem. W e discuss two approaches to solving this problem, both i nvo lving a relaxation of the constraint. In both cases, unlike classical equalization, there is a t hreshold o n the variance of the noise below which an improv ement of the mean-square err or cannot be guaranteed. I . I N T R O D U C T I O N The task o f transferrin g quantu m inform ation differs sig- nificantly from its classical ( n on-q uantum) coun terpart, since the laws o f q uantum mech anics limit the accu racy of in- formation transfer th roug h qu antum cha nnels. Sp e cifically , the signal-to-noise ratio of possible qu antum measurements on th e tr ansmission lin e is lim ited [4], reflecting the well known fact that a q uantum state canno t be cloned at the remote locatio n. This motiv ates a great intere st in devel- oping systematic methodolog ies for the de sig n of optim a lly perfor ming quantum communication systems. In the classical communication th eory , op timization plays an instru mental role in balan cing various trade-offs in the design of classical communication systems. The most cele- brated example of u sing op timization in signal p rocessing are due to N. W iener [1 5] who developed a general method for reducing the effects of n o ise a nd chann el distor tion th rough minimization of the mean square error (M SE) between the signal an d its estimate over a class o f line ar filters. This paper highlights conceptual challenges that ar ise when the W iener o ptimization p a r adigm is applied in the deriv ation of coh erent quan tu m filters, i.e., filters which them selves are quantum systems. T o b e concr ete, we restrict attention to one type of the co herent filtering problem concer ned with equalizing distortions of quan tum sign als transmitted via a quan tum commun ication channel. Owing to the an alogy with classical chan nel equ a lization, we call this prob lem th e quantu m eq u alization pr oblem . The pap er shows that the requirem ent fo r the filter to be physically realizable translates This work was supp orted by the Australi an Researc h Council and the ARC Centre for Quant um Computation and Communication T echnology . V . Ugrino vskii is with the School of Enginee ring and Infor - mation T echnology , Unive rsity of N ew South W ales at the Aus- tralia n Defence Force Academy , Canberra, ACT 2600, Australia, v.ougrinovski @adfa.edu.au M. R. James are with the ARC Centre for Quantum Computa- tion and Communication T echnology , Research School of Engineer - ing, The Austra lian na tional Univ ersity , Canb erra, ACT 2601, Aust ralia, matthew.james @anu.edu.au. into add itional constraints wh ich rend er the pro blem of o pti- mizing the me a n square of the eq u alization error non conv ex. The pa per is centered aro und the so-called passive quan- tum equalizers. Mathematically , dynamics of a passi ve quan- tum system in the Heisenb erg pictur e ar e described by complex quantu m stochastic differential equation s expressed in term s of annihilation op erators only [7]. Such systems are simple to implement exper imentally by cascading co n- ventional quantu m optics co mpon ents such as beam splitters and optical cavities [ 1 1]. Fu r thermor e, in a gen eral qu antum system, passi v ity ensures that the sy stem dissipates energy in the input. A strik ing o bservation that emerges from o ur analysis is that passivity appear s to be a r ather restrictive proper ty in the context of equalization , in that an optim al passiv e coher ent equ alizer is not always a b le to imp rove the MSE. It turns out that the achiev able improvement dep ends on the v ariance of the quantum noise in the filter input signal. W e give examples which r ev eal a thresho ld on this variance above w h ich th e op timal passive coheren t equ a lize r delivers an improved MSE. The p aper is organ ized as f ollows. In th e n ext section we present the basics of p assi ve linear quantu m systems. The quantum passiv e equ alization pro blem is posed in Section II I. A relaxation of the pro b lem is proposed in Section IV. Next, in Section V, the pr oblem is particularized to dem onstrate the dependency b etween th e power spectrum density of the equalization err or and the variance of the system noise. T wo examples of t he qua n tum coherent filter design are presented in that section, r eflecting two approac hes to optimizatio n of the equalizatio n erro r , the first one is via dir ect op timization of the power spectrum density , and th e second o ne is using the W iener-Hopf f actorizatio n techn ique [8]. Finally , conclud in g remar ks are gi ven in Section VI. Notation: For an operato r a in a Hilbert sp ace H , a ∗ denotes the Hermitian adjoint operator , and if a is a complex number, a ∗ is its comp lex con jugate. Let a = ( a 1 , . . . , a n ) be a column vector co m prised of n operators (i.e., a is an operato r H → H n ); th en a # = ( a ∗ 1 , . . . , a ∗ n ) , a T = ( a T 1 . . . a T n ) (i.e, the row of operators), and a † = ( a # ) T . The notation col( a, b ) de n otes the colum n vector obtained by co ncatenating vectors a and b . For a comp lex matrix A = ( A ij ) , A # , A T , A † denote, respec tively , the matr ix of co mplex conjug ates ( A ∗ ij ) , th e transp ose matrix and the Hermitian ad joint matrix. [ · , · ] denotes the comm u tator o f two operators in H . tr[ · ] deno tes the trace of a matrix. I is the iden tity ma trix. The quantu m exp ectation of a n op e rator V with respec t to a state ρ , is den oted h V i = tr[ ρV ] [12]. I I . O P E N L I N E A R PA S S I V E Q U A N T U M S Y S T E M S An op en q u antum annih ilatio n-only system represents a linear system ˙ a = A a + B u , a ( t 0 ) = a , y = C a + D u ; (1) where A , B , C , D are complex m × m , m × n , n × m , n × n matr ices, and u is a (column) vector of n qu a ntum input pro cesses. T h e input is assumed to b e of the fo rm u ( t ) = u 0 ( t ) + b ( t ) , (2) where b is a (co lumn) vector o f n quantum no ise pr ocesses, b = ( b 1 , . . . , b n ) , a n d u 0 ( t ) is an adapted process [5]. The noise p rocesses can be rep r esented as a n nihilation o perator s on an ap p ropria te F ock space [5], but fro m the system theory viewpoint they can be trea te d as quantum Gaussian white noise processes with z e r o mean, an d the covariance  b ( t ) b # ( t )   b † ( t ′ ) b T ( t ′ )  =  I + Σ T b Π b Π † b Σ b  δ ( t − t ′ ) , (3) where Σ b , Π b are complex matrices with the properties that Σ b = Σ † b , Π T b = Π b . Alon g with their adjoint (creation) oper a to rs b ∗ j ( t ) , the noise o perators satisfy can on- ical commutatio n relation s [ b j ( t ) , b ∗ k ( t ′ )] = δ j k δ ( t − t ′ ) , [ b j ( t ) , b k ( t ′ )] = 0 . Here, δ j k = 0 when j 6 = k , and is the identity ope rator when j = k ; δ ( t − t ′ ) is the δ -fun ction. The colu mn vector a ( t ) = ( a 1 ( t ) , . . . , a m ( t )) repr esents the system modes an d consists of annihilation o perator s on a certain Hilb ert space H . A discussion abou t open linear quantum systems can be found in [7], [2], [6]. From now on, it will b e assumed th a t th e pair ( A, B ) is controllab le . For a system o f the form (1) to correspond to quantum physical d y namics, it mu st pre serve the c anonical commuta- tion relations d uring its ev olutio n [ 13], [6]. A c cording to [9], for th e system (1) this is guar anteed if an d on ly if th ere exists a Hermitian co mplex matrix Θ such th a t A Θ + Θ A † + B B † = 0 , B = − Θ C † , D = I . (4) W ithout lo ss of gener a lity we will assume f r om now on that the c ondition s (4) are satisfied for th e systems under consideratio n with Θ = I ; this can always be achie ved by an app ropria te choic e of c oordin ates [9]. Furth e rmore, we will assume th a t th e matrix A is Hurwitz. From (1), th e output of th e system can be represented as y ( t ) = C e A ( t − t 0 ) a + Z t t 0 g ( t − τ ) u 0 ( τ ) dτ + Z t t 0 g ( t − τ ) b ( τ ) dτ . (5) Here we intr oduced the no tation f or the impulse respo nse, associated with the system [16], g ( t ) = ( C e At B + δ ( t ) I , t ≥ 0 , 0 , t < 0 . (6) Let us in troduce the transfer fun ction of the system (1), G ( s ) = C ( sI − A ) − 1 B + I . Since B = − C † , the transfer function G ( s ) is square. This o b servation h olds for all passi ve systems consider ed hencefo rth. Furthermo re, if f ollows from the prop erties of the p hysical realizability [13] that for the passive system (1), G ( s )[ G ( − s ∗ )] † = I . (7) In the sequ el we will b e interested in stationar y behaviours of the systems und er consideration . Since the m atrix A is assumed to be stable and assuming that u 0 ( t ) is stationary , the stationary compon ent of the system outpu t is ob tained from (5) by letting t 0 → −∞ : y ( t ) = Z + ∞ −∞ g ( t − τ ) u 0 ( τ ) dτ + Z + ∞ −∞ g ( t − τ ) b ( τ ) dτ . (8) Also, f or conv enien ce the upp er limit of integration has been changed to + ∞ since g ( t ) is cau sal. Consider the correlation function o f stationary quantum operator pro cesses x j ( t ) , x k ( t ) associated with th e system, R x j , x k ( t ) = h ( x j (0) − h x j (0) i )( x k ∗ ( t ) − h x k ∗ ( t ) i ) i . The corresp onding power spectrum density is th en P x j , x k ( iω ) = Z + ∞ −∞ e − iωt R x j , x k ( t ) dt. (9) The Fourier tran sform is understo od in the sense of temp ered distributions when R x j , x k is not integrab le. Als o, consider the e xtension o f P x j , x k ( iω ) to the complex pla n e, given b y the bilater a l Lap lace tra n sform of R x j , x k , P x j , x k ( s ) = Z + ∞ −∞ e − st R x j , x k ( t ) dt. (10) Often, P x j , x k ( s ) is also referred to as the po wer sp ectrum density fun c tion [8], althou gh in general it may no t be real. Since th e matrix A is Hurwitz, P x j , x k ( s ) is well defined on s = iω and P x j , x k ( s ) | s = iω = P x j , x k ( iω ) , where the expression on th e left-han d side refers to the power-spectrum density d efined in (10), an d the expression on righ t-hand side is defined in (9). I t is easy to o b tain that the power spectr um density m atrix of the outpu t y ( t ) , P y , y ( s ) = ( P y j , y k ( s )) is related to the power spectrum de n sity m a tr ix o f th e noise b , P b , b ( s ) = ( P b j , b k ( s )) , in the standard ma n ner: P y , y ( s ) = G ( s ) P b , b ( iω )[ G ( − s ∗ )] † . (11) I I I . E Q UA L I Z A T I O N P R O B L E M F O R A N N I H I L AT I O N - O N LY C O M M U N I C AT I O N S Y S T E M S In this sectio n , a gener al eq ualization scheme fo r a passive commun ication system is outlined. Consider a system in Fig. 1 consisting of a quantum channel and an equa lize r . The inp ut si gn a l u plays the role of a me ssage signal to be transmitted thr ough the chan nel, of the fo rm u ( t ) = u 0 ( t ) + b ( t ) , (12) and w denotes the vector comprised of additional quantum noises. It include s the n oise in puts that are n ecessarily present in the p h ysically realizable system G ( s ) [6], [14], as well as noises introduc e d by measurem ent devices. In P S f r a g r e p l a c e m e n t s G ( s ) H ( s ) u w y w z ˆ u ˆ z y u Fig. 1. A general quantum communica tion system. T he transfer function G ( s ) represents the channel, and H ( s ) represents an equali zing filter . terms of the notation adopted in the previous sectio n, we have u 0 = col( u 0 , 0) , an d b = col( b, w ) . The comb ined input u = col( u, w ) drives an annihilation - only (passiv e) quantum system G ( s ) , as described in the previous section , to p roduce the outp ut y = co l( y u , y w ) , altho ugh f or filtering purpo ses, we are on ly interested in the o utput comp onent y u which corr e sp onds to the inpu t channel u . The objective: In the classical fil tering theo ry [8], the equalizer is to com pensate for signal distortions in the output y u ( t ) , by min imizing the eq ualization error e ( t ) = ˆ u ( t ) − u ( t ) between classical signals ˆ u ( t ) , u ( t ) in the mea n - square sense. The classical power sp e ctrum density P e,e ( iω ) is usually L 2 -integrable an d is related to the c o rrelation function of the er r or e ( t ) via the inverse Fourie r tr ansform , R e,e ( t ) = 1 2 π Z + ∞ −∞ P e,e ( iω ) e iωt dω . In this case, minim izing the mean -square error covariance measure tr R e,e (0) is equiv alent to minimizing tr P e,e ( iω ) pointwise in ω . Alternativ ely , the optimal causal filter can be sought to satisfy the W iener-Hopf equation [8], R u,y u ( t ) = Z + ∞ 0 h ( t − τ ) R y u ,y u ( τ ) dτ , t > 0; (13) here h ( t ) is the un ilateral in verse Laplace transf o rm o f a causal transfe r fun c tion H ( s ) . The equation (13) reflects the p rojection pro perty of classical least-square estimates, E ( e ( t ) y u ( τ ) † ) = 0 f or − ∞ < τ < t . Th e so lu tion to equation (13) is obtained usin g spectral factorization. Analogou s to the classical mean-squ are equalization, we wish to obtain a quantum system H ( s ) whose outpu t ˆ u matches th e inpu t u op timally , in th e sense that the equal- ization err or e ( t ) = ˆ u ( t ) − u ( t ) mu st ha ve a minimu m covariance. Owing to the physical realizability requirem ent reflected in the identity (7), quantu m channels ar e n ot gu ar- anteed to generate L 2 -integrable power spectrum densities. For this reaso n, we will pose the prob le m dire c tly as opti- mization o f the p ower spectrum density , to either m inimize tr P e,e ( iω ) p ointwise for every ω , or obtain a causal H ( s ) by solving the corre sp onding spe c tr al factorization prob lem. Both app roaches will b e discussed in Section V. Admissible equ alizing fi lters: The key distinction of the proble m und er conside ration fro m classical coun terparts is that the system H ( s ) must be ph ysically realizab le as a q uantum sy stem. This mand ates imposing additiona l r e - quiremen ts o n the filter . Firstly , to ensure tha t the L TI filter system obtain e d fro m th e optimizatio n pro blem ( 1 6) or fr om spectral factorization can be made physically realizable, it may need to be equipped with additional noise inputs z — it was observed in [ 6], [14] that any L TI system can b e made phy sically re alizable b y addin g no ise. W ith out loss of generality , we will assume that the ad ded noise z is in a Gaussian v acuum state, i.e. , the corresp o nding mean and covariance o f z are h z ( t ) i = 0 ,  z ( t ) z # ( t )   z † ( t ′ ) z T ( t ′ )  =  I 0 0 0  δ ( t − t ′ ) . (14) Secondly , to facilitate implem entation of the resu ltin g quantum filter [ 11], we restrict attention to passiv e equalizer systems. In this case, the requ irement f or ph ysical realizab il- ity of the filter leads to a fo r mal constraint of the form (7) on the tr a nsfer f unction H ( s ) : H ( s )[ H ( − s ∗ )] † = I . (15) Let us deno te the set o f passiv e phy sically realizab le equal- izers s atisfying (15) as H r . T he pointwise optimizatio n of tr P e,e ( iω ) in th e class of phy sically realizab le filters is th us a constrain ed o ptimization prob lem, min H ∈ H r tr P e,e ( iω ) . (16) The con straint (15) precludes th e d irect app lication of standard filtering tech n iques to ob ta in an optimal q uantum W iener equalizer . In the next section we o utline a relaxation technique which h e lp s to overcome this prob lem. I V . C O N S T R A I N T R E L A X A T I O N Let us define th e par titions of the transf e r function s G ( s ) and H ( s ) c o mpatible with the par titio ns of u = col( u, w ) , y = c o l( y u , y w ) , and co l( y u , z ) , col( ˆ u, ˆ z ) , respectively: G ( s ) =  G 11 ( s ) G 12 ( s ) G 21 ( s ) G 22 ( s )  , H ( s ) =  H 11 ( s ) H 12 ( s ) H 21 ( s ) H 22 ( s )  . (17) W ith this no tation, we have that P e,e ( s ) = ( H 11 ( s ) G 11 ( s ) − I )( I + Σ T b )( G 11 ( − s ∗ ) † H 11 ( − s ∗ ) † − I ) + H 11 ( s ) G 12 ( s )( I + Σ T w ) G 12 ( − s ∗ ) † H 11 ( − s ∗ ) † + H 12 ( s ) H 12 ( − s ∗ ) † . (18) Also, the con straint (15) is equivalent to H 11 ( s ) H 11 ( − s ∗ ) † + H 12 ( s ) H 12 ( − s ∗ ) † = I , (19) H 11 ( s ) H 21 ( − s ∗ ) † + H 12 ( s ) H 22 ( − s ∗ ) † = 0 , (20) H 21 ( s ) H 21 ( − s ∗ ) † + H 22 ( s ) H 22 ( − s ∗ ) † = I . (21) From ( 18), we o bserve that the spectral d ensity fu nction P e,e ( s ) depends on th e v ariables H 11 , H 12 only . Therefo re one possible app roach to solving the equalizer design p rob- lem is to employ a two-step procedure whose first step is to optimize th e equ alization erro r with respect to H 11 ( s ) , H 12 ( s ) , sub ject to the constra int (19), followed by the seco nd step during which the remaining tran sfer functions H 21 ( s ) , H 22 ( s ) are computed to fulfill th e remain ing p hysical real- izability constrain ts (2 0), (21). Of co urse, there is no guaran tee th at with H 11 ( s ) , H 12 ( s ) found d uring th e first step, the remaining transf e r fun ctions H 21 ( s ) , H 22 ( s ) e xist and satisfy the conditions (20), (21). Nev ertheless, this appr o ach is attr a c ti ve in that it allows us to obtain tractable relaxation s of th e o r iginal quan tum equ alizer design p roblem . Indeed , using (19), H 12 ( s ) can b e elimina ted from the expression (18): P e,e ( s ) = ( H 11 ( s ) G 11 ( s ) − I )( I + Σ T b ) × ( G 11 ( − s ∗ ) † H 11 ( − s ∗ ) † − I ) + H 11 ( s ) G 12 ( s )( I + Σ T w ) G 12 ( − s ∗ ) † H 11 ( − s ∗ ) † − H 11 ( s ) H 11 ( − s ∗ ) † + I . (22) It also f ollows from (19) that H 11 ( iω ) H 11 ( iω ) † ≤ I ∀ ω ∈ R 1 . (23) This allows us to replace the o riginal prob lem of findin g an op tim al passi ve equ alizer H ( s ) with the p roblem of optimizing the equalization er ror in the class of causal transfer function s H 11 ( s ) subject to the quadra tic constraint (23). W e will give a precise me a ning to this statemen t in the next section, where we d iscuss two relaxed quan tum W iener filter pro b lem f ormulatio ns. V . T W O A P P RO AC H E S T O Q UA N T U M W I E N E R E Q UA L I Z AT I O N In this section w e apply the relax ation tec h nique discussed in the pr evious section to two problem s which demonstrate features of the qu antum Wiener filtering . Our aim is to highligh t ne w fea tu res of the problem of co h erent W iener equalization owing to the phy sical realizability co n straint (15), r a ther th a n ob tain a general solution to this problem. All signals in this section are a ssumed to b e scalar un less specified otherwise. A. Equalizatio n via o ptimization of power spectru m density: An optical bea m splitter In th is section, we focus on the problem (1 6). The c o n- straint relax ation proposed in the pr evious section allows to r eplace this pro blem with the pr oblem inv olving the constraint (23). In the case of scalar signals u , y u and ˆ u , P ee ( s ) and Σ b are scalars, an d this pr o blems simp lifies significantly: min | H 11 ( iω ) | ≤ 1 P e,e ( iω ) , (24) P e,e ( iω ) = (1 + Σ b ) | H 11 ( iω ) G 11 ( iω ) − 1 | 2 + | H 11 ( iω ) | 2 G 12 ( iω )( I + Σ T w ) G 12 ( iω ) † −| H 11 ( iω ) | 2 + 1 . (25) In (24), th e m inimum is taken over the set of c a usal tran sfer function s H 11 ( s ) subje c t to the scalar version of the condi- tion (23). Obviously , we have in this ca se min | H 11 ( iω ) | ≤ 1 P e,e ( iω ) ≤ min H ∈ H r P e,e ( iω ); (26) i.e., the problem (2 4) delivers a lower bou nd o n the o ptimal power spectrum density . The requir e ment for H 11 ( s ) to b e causal is also no ntrivial — while the fre quency pointwise optimization is ea sy to perfo rm over complex H 11 , th e P S f r a g r e p l a c e m e n t s u w z ˆ u ˆ z y w H ( s ) y u Fig. 2. A beam splitter and a quantum equalizer system. pointwise optimal H 11 ,ω obtained this way mu st admit a causal extension into th e complex plane. I n general, th is issue can be addressed nu merically [1], using the standar d Matlab sof tware [10]. There f ore in the rema inder of th is section, we will be c o ncerne d with equalization of a static quantum system for which the cau sality co ndition is satisfied automatically . This simplified analysis aims to demonstrate that the p r oposed relaxation can lead to ph ysically realizab le equalizers which ar e optimal in the sense of ( 16). As an example of a static qu antum system consider a quantum -mechan ical bea m splitter, which is a two-input two- output quan tum system; see Fig. 2. In Fig. 2, the input u represents the signal we would like to split, and th e second input w is an a u xiliary no ise inpu t. The bea m splitter mixes the signals u and w , its outputs and inp uts are related via a unitary transfor mation:  y u y w  = G  u w  , G ( s ) =  √ η √ 1 − η − √ 1 − η √ η  ; (27 ) η ∈ (0 , 1) is a real par a meter k n own as transmittance. Th at is, G ( s ) is static in th is case, and y u = √ η u + p 1 − η w . The equalization problem is to estimate the sign al u from the outp ut y u of this d evice usin g a coherent equ alizer, i. e., a device which pre serves the cano n ical c o mmutation r elations. T o demo nstrate the applica tio n of a quantu m Wiener filter in this problem , suppose that the in put n oise b in (12) is in Gaussian vacuum state, and Σ b = 0 , Π b = 0 , wherea s the beamsplitter n oise w is in a Gaussian thermal state, so that Σ w = σ 2 w > 0 , Π w = 0 . With these assumptions, the expression f or the objective functio n in (25) bec omes P e,e ( iω ) = (1 − η ) σ 2 w | H 11 ( iω ) | 2 − 2 √ η Re H 11 ( iω ) + 2 . (28) The constrain t co ndition (23) red u ces in this case to | H 11 ( iω ) | 2 ≤ 1 . (29) Since all c o efficients in (28) ar e constants, th e optimal value and the op timal equalizer should also be constant. The prob lem (24) is thu s a regular con strained op tim ization problem , wh ich can be solved u sin g th e Lag range mu ltip lier technique . Pr op osition 1: 1. If σ 2 w ≤ √ η (1 − η ) , then the optimal equal- izer which attains m inimum in (1 6) is H ( s ) = I . 2. On the other h a nd, when σ 2 w > √ η (1 − η ) , an op timal equalizer is g iven by H 11 ( s ) = √ η σ 2 w (1 − η ) , H 12 ( s ) = r 1 − η σ 4 w (1 − η ) 2 , H 21 ( s ) = − H 12 ( s ) , H 22 ( s ) = H 11 ( s ) . (30) P S f r a g r e p l a c e m e n t s u v α β w z ˆ u y w v out u out ˆ z y u H ( s ) Fig. 3. A ca vity , beam splitters and an equaliz er system. Such an eq ualizer atten uates th e in put y u , an d must include an additio nal noise input z , to en sure that it is physical realizable. The co r respond ing expressions f or the optimal error power spectrum density are min H ∈ H r P ee = ( σ 2 w (1 − η ) − 2 √ η + 2 , if σ 2 w ≤ √ η (1 − η ) ; 2 − η σ 2 (1 − η ) , if σ 2 w > √ η (1 − η ) . (31) Comparing the power spe c tr um density of the err or at the input o f th e filter, P ( y u − u ) , ( y u − u ) ( iω ) , with P e,e ( iω ) in (31), we ob serve that P ( y u − u ) , ( y u − u ) ( iω ) = P e,e ( iω ) if σ 2 w ≤ √ η (1 − η ) , a nd P ( y u − u ) , ( y u − u ) ( iω ) > P e,e ( iω ) if σ 2 w > √ η (1 − η ) . Thus, Proposition 1 shows that the requirem e nt f o r p hysical realizability r estricts the capacity of an optimal coher e nt equalizer to respon d to noise in the input s ignal. It is still possible to red uce th e MSE by means of a co herent equalizer, howe ver this is on ly possible p rovided the covariance of the th ermal no ise in the inpu t signal is sufficiently large. This situation differs strikingly from the classical W iener equalization theor y . B. The W ien er -Hop f technique for q uantu m equa lization: A n equalizer for an o ptical cavity Let us modify the system in Fig. 2 to includ e an optical cavity and two ad ditional beam splitter s of tran smittance α and β ; see Fig. 3. W ith these mo dification the system becomes d ynamical. In Fig. 3, v denotes an ad ditional thermal Gaussian noise input into the system, with zer o mean and covariance  v ( t ) v ∗ ( t )   v ∗ ( t ′ ) v ( t ′ )  =  1 + σ 2 v 0 0 σ 2 v  δ ( t − t ′ ) . Correspon d ingly , the relation between the chan n el outpu t col( y u , y w ) and its in put col( u, v ) is fo und fro m th e r elations  y u y w  =  √ η √ 1 − η − √ 1 − η √ η   u out w  ,  u out v out  = ¯ G ( s )  u v  , ¯ G ( s ) =  ¯ G 11 ( s ) ¯ G 12 ( s ) ¯ G 21 ( s ) ¯ G 22 ( s )  = p αβ  G c − √ α ′ β ′ √ α ′ G c + √ β ′ − √ β ′ G c − √ α ′ − √ α ′ β ′ G c + 1  ; ( 32) G c ( s ) den otes the transfer fu nction of the o ptical cavity G c ( s ) = s − γ 2 + i Ω s + γ 2 + i Ω ; (33) γ , Ω a r e real co nstants, and α ′ = 1 − α α , β ′ = 1 − β β . Note th at G c ( s )[ G c ( − s ∗ )] ∗ = I . After these m o difications, the p ower sp ectrum density of the equ alization erro r in equation (22) is expressed as P e,e ( s ) = 2 + ( η σ 2 v ¯ G 12 ( s )[ ¯ G 12 ( − s ∗ )] ∗ + (1 − η ) σ 2 w ) × H 11 ( s )[ H 11 ( − s ∗ )] ∗ − √ η  H 11 ( s ) ¯ G 11 ( s ) + [ H 11 ( − s ∗ )] ∗ [ ¯ G 11 ( − s ∗ )] ∗  . (34) The au xiliary optimization problem considered in the p revi- ous sections is therefore to obtain a causal transfer function H 11 ( s ) which optimizes (3 4) su b ject to the constraint (29). Unlike the previous sectio n, the system con tains dynam- ics and the correspo nding optima l filter is expected to b e dynamica l. Therefo re, we cannot e xpect that the pointwise optimization in (24) will produce a causal tra n sfer fu nction H 11 ( s ) . In the classical case, th is issue is resolved using the W iener-Hopf spe ctral factorization method [8]. Therefo re, here we pro ceed as f ollows. First, we ap p ly the W iener-Hopf spectral factorization metho d [8] to obtain a cau sal op timal H 11 ( s ) that minimize s tr P e,e ( iω ) for P e,e ( s ) in (34); this step does not in volve th e physical realizability constraints. Next, we sho w that in fact the found H 11 ( s ) v alidates the required co nstraint (29), provided the variance of the system noise excee d s a cer ta in thr eshold. T h en we show that in this case a co mplete phy sically realizab le filter transfer f unction H ( s ) wh ich satisfies (19)–(21) can be constructed f rom th e found H 11 ( s ) . Since P e,e ( s ) in (34) de p ends o n H 11 ( s ) only , we c an minimize tr P e,e ( iω ) b y treating P e,e ( s ) as a power spectrum density of a class ical sy stem . Define ζ = 1 − η η σ 2 w αβ , ρ = α ′ + β ′ + ζ σ 2 v 2 √ α ′ β ′ ≥ 1 . (35) Letting M ( s ) be the follo wing causal transfer f unction, M ( s ) = q 2 η σ 2 v p αβ (1 − α )(1 − β )( ρ + 1 ) × s + γ 2 q ρ − 1 ρ +1 + i Ω s + γ 2 + i Ω , (36) we obtain the identity M ( s )[ M ( − s ∗ )] ∗ = η σ 2 v ¯ G 12 ( s )[ ¯ G 12 ( − s ∗ )] ∗ + (1 − η ) σ 2 w . Therefo re, P e,e ( s ) = (( M ( s ) H 11 ( s ) − √ η Q ( s )) × (( M ( − s ) ∗ H 11 ( − s ) ∗ − √ η [ Q ( − s ∗ )] ∗ ) − η Q ( s )[ Q ( − s ∗ )] ∗ + 2 , (37) where Q ( s ) ,  ¯ G 11 ( − s ∗ ) M ( − s ∗ )  ∗ = 1 − √ α ′ β ′ p 2 η σ 2 v √ α ′ β ′ ( ρ + 1)   1 + γ 2 q ρ − 1 ρ +1 + 1+ √ α ′ β ′ 1 − √ α ′ β ′  s + i Ω − γ 2 q ρ − 1 ρ +1   . (38) Now co nsider a classical filtering problem of minimizing the M SE between the filter output ˆ u = H ( s ) y u , wh ere y u = M ( s ) u , and the sign al ¯ u = √ η Q ( s ) u . Let [ Q ( s )] + denote the causal pa rt of Q ( s ) . Acc o rding to the W iener- Hopf metho d [ 8], th e causal solution to th is problem is H 11 ( s ) = √ η M ( s ) [ Q ( s )] + . (39) This filter en sures that the erro r u − ¯ u and the filter input y u are ortho gonal. Since the expression for the power spe c tr um density of the error in th is pr oblem is exactly equa l to th e first term in (37), we con clude th at the filter (3 9) minimizes P e,e ( iω ) in the class o f ca u sal transfer fu n ctions. Th is yields the explicit expression for the op timal filter which is causal by way of co n struction: H 11 ( s ) = (1 − √ α ′ β ′ ) / √ η σ 2 v ( √ α ′ + √ β ′ ) 2 + ζ × s + γ 2 + i Ω s + γ 2 q ρ − 1 ρ +1 + i Ω . (40) Pr op osition 2: Under th e condition σ 2 v > − ζ ( α ′ + β ′ ) + q 4 ζ 2 α ′ β ′ + (1 − √ α ′ β ′ ) 2 ηαβ ( α ′ − β ′ ) 2 ( α ′ − β ′ ) 2 (41) the tran sfe r fu nction H 11 ( s ) in (4 0) satisfies (2 9). It can b e shown using Proposition 2 th at th e f ollowing constants are real under (4 1): α 11 = 1 − √ α ′ β ′ 2 √ η σ 2 v ( ρ + 1) p (1 − α )(1 − β ) , α 12 = q 1 − α 2 11 , β 12 = γ 2 r ρ − 1 ρ + 1 − α 2 11 . Pr op osition 3: Suppo se (41) hold s. Th en the op timal causal equalizer for the system un der consideration in this section is g iv en by the following tr ansfer fun ctions H 11 ( s ) = α 11 s + γ 2 + i Ω s + γ 2 q ρ − 1 ρ +1 + i Ω , (42) H 12 ( s ) = α 12 s + β 12 + iα 12 Ω s + γ 2 q ρ − 1 ρ +1 + i Ω , (43) H 21 ( s ) = − α 12 s − β 12 + iα 12 Ω s + γ 2 q ρ − 1 ρ +1 + i Ω , (44) H 22 ( s ) = α 11 s − γ 2 + i Ω s + γ 2 q ρ − 1 ρ +1 + i Ω . (45) As we see, the condition ( 41) plays a critical r ole in the above analysis. Th e expr ession on the rig ht-hand sid e of ( 41) depend s on σ 2 w . If ζ ( α ′ + β ′ ) > s 4 ζ 2 α ′ β ′ + (1 − √ α ′ β ′ ) 2 η αβ ( α ′ − β ′ ) 2 , (46) then th is expre ssion is n egative, and (41) h olds trivially . It can b e sh own that if σ 2 w > | 1 − √ α ′ β ′ | √ 1 − η then ( 46) holds, and hence (41) is trivially satisfied. T hus we h ave arri ved at a conclusion similar to that made in th e previous section: If the variance of the thermal n oise in th e system is sufficiently large, then there exists a filter which attenuates the therm a l noise compo nent of y u while injectin g a small amo unt of noise throu g h th e z channel. V I . C O N C L U S I O N S The paper h a s discussed a qu antum counter p art of th e clas- sical W iener filtering problem fo r equalization of quantum systems. The requirem e nt to ob tain a physically realizable passiv e causal equalizer imposes no nconve x constrain ts o n the filter transfer function. W e ha ve d iscussed one f orm of relax ation of th e se con straints, and h ave shown, via examples, th at the relaxation does not pre clude find ing a physically r ealizable coheren t filter able to re d uce the sig n al distortion caused by th e noisy quantum chan n el. R E F E R E N C E S [1] Z. Drmac, S. Gugercin, and C. Beat tie. 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