Algebraic and group treatments to nonlinear displaced number states and their nonclassicality features: A new approach
Asili Firouzabadi Na), Tavassoly M Ka),b), Faghihi M Jc)†
Atomic and Molecular Group, Faculty of Physics, Yazd University, Yazd, Iran
The Laboratory of Quantum Information Processing, Yazd University, Yazd, Iran
Physics and Photonics Department, Graduate University of Advanced Technology, Mahan, Kerman, Iran

Corresponding author. E-mail: mj.faghihi@kgut.ac.ir

Abstract

Recently, nonlinear displaced number states (NDNSs) have been manually introduced, in which the deformation function f( n) has been artificially added to the previously well-known displaced number states (DNSs). Indeed, just a simple comparison has been performed between the standard coherent state and nonlinear coherent state for the formation of NDNSs. In the present paper, after expressing enough physical motivation of our procedure, four distinct classes of NDNSs are presented by applying algebraic and group treatments. To achieve this purpose, by considering the DNSs and recalling the nonlinear coherent states formalism, the NDNSs are logically defined through an algebraic consideration. In addition, by using a particular class of Gilmore–Perelomov-type of SU(1, 1) and a class of SU(2) coherent states, the NDNSs are introduced via group-theoretical approach. Then, in order to examine the nonclassical behavior of these states, sub-Poissonian statistics by evaluating Mandel parameter and Wigner quasi-probability distribution function associated with the obtained NDNSs are discussed, in detail.

Keyword: 42.50.Ct; 42.50.Dv; 42.50.–p; 03.65.–w; displaced number state; nonlinear coherent state; Wigner function; nonclassical state
1. Introduction

Nowadays, nonclassical states of the radiation field have obtained a great deal of attention in various fields of research, such as quantum optics, quantum cryptography, and quantum communication.[17] These states may be generated through the conditional measurement techniques or the atom– field interactions in cavity QED, [810] and also may be revealed, for instance, in the Jaynes– Cummings model[1118] and in the field of nonlinear coherent states[1926] which naturally arise from the canonical (standard) coherent states.

The standard coherent state defined by

is a quantum state which describes the radiation field, i.e., known as displaced vacuum states, | α 〉 = (α )| 0〉 , where (α ) = exp (α â α * â ) is the well-known displacement operator in which â and â are the bosonic annihilation and creation operators, respectively. Considering this idea, regarding the construction of coherent state, the displaced number states (DNSs) have been introduced by the displacement operator acting on the number state | n〉 which are defined by | n, α 〉 = (α )| n〉 :[27]

It has been shown that DNSs indicate several interesting nonclassicality features such as unusual oscillations in the photon number distribution interpreting as the interference in the phase space.[28]

On the other hand, nonlinear coherent states, which are known as a natural generalization of canonical coherent states (corresponding to simple harmonic oscillator) to f-deformed ones (associated with nonlinear oscillators), [19, 20] can be considered as suitable candidates from which nonclassical light comes out.[2933] It is worthwhile to mention that there are many generalized coherent states categorized in this special class of quantum states, which exhibit the nonclassicality features of light, i.e., ‘ nonclassical’ light.[3437]

Based on the above explanations, regarding the DNSs as well as the nonlinear coherent states, one may motivate to establishing a direct connection between DNSs and nonlinear coherent states, which leads to the concept of ‘ nonlinear displaced number states’ (NDNSs). This idea has recently been introduced by de Oliveira et al.[38] In detail, in this attempt, the authors have paid attention to the forms of the standard coherent state

and the nonlinear coherent state

(the latter has been defined by Man’ ko et al.[20]). Then, in a simple and unsatisfactory comparison between the coefficients of coherent state, DNS and nonlinear coherent state, the authors have manually inserted the nonlinearity function f(n) into their DNSs in a special form, by which they proposed the states

being called NDNSs by them. It seems that the above construction of NDNS in Ref.  [38] is so artificial such that there may not be found any clear physical or even reliable mathematical reason for its basis. Hence, one may naturally seek a satisfactory method containing logical mathematical backgrounds and, if possible, enough physical motivations for the construction of the NDNSs. In this regard, in this paper via modifying the definition of NDNSs in Ref.  [38] we intend to outline a logical formalism from which NDNSs can be reasonably constructed. For this purpose, by recalling the nonlinear coherent states approach together with the displacement operator, an algebraic method through which the NDNSs are introduced, is presented. In addition, with the help of a particular class of Gilmore– Perelomov-type of SU(1, 1) and a class of SU(2) coherent states, the NDNSs are defined via group-theoretical approach. Then, in each case, some of the well-known nonclassicality features are numerically evaluated.

The plan of this paper is as follows: In the next section, the NDNS is algebraically introduced. In Section  3, by considering two particular classes of coherent states, the NDNS is defined via group-theoretical approach. Section  4 deals with studying the nonclassicality signs of the obtained NDNSs through the Mandel parameter as well as the Wigner quasi-distribution function. Finally, Section  5 contains a summary and concluding remarks.

2. Nonlinear displaced number states: Algebraic approach

This section is devoted to the construction of the NDNSs via algebraic method. To reach this goal, it is necessary to introduce the generalized displacement operators f (α ) by joining the nonlinear coherent state method and the standard displacement operator. So, the generalized displacement operator reads as f (α ) = exp (α  α *  ), in which  = â f() and  = f()â represent the nonlinear (f-deformed) annihilation and creation operators, respectively.[19, 20] Now, the following communication relations are obviously satisfied

where f () is generally a Hermitian operator-valued function which depends on the number operator. The relation  (3) clearly shows that the f-deformed displacement operator f (α ) cannot be generally separated by the well-known Baker– Campbell– Hausdorff (BCH) formula (noticing that the BCH lemma is satisfied under specific conditions). This is due to the fact that, the commutation relation of  and  is a complicated operator. In order to dispel this problem and to be able to use the generalized displacement operator on the number state, Roy and Roy[39] gave a proposition and defined two new auxiliary operators as follows:

which has been also established in a general mathematical framework by Ali et al. in Ref.  [34]. In other words, it should be declared that, incorporating the concept of nonlinear coherent states with the displacement operator is achieved only by making use of the above-mentioned auxiliary operators (since only by these new operators the necessary condition for BCH is satisfied). As a consequence of the latter relation, it may be observed that, by considering a special composition of the operators  and , the generators { , ,  , Î } and also {,  ,  , Î } constitute the commutation relations of the Weyl– Heisenberg Lie algebra and the following relations clearly hold[35, 39]

As a result, two generalized displacement operators can be defined which are given by

in which we have used the BCH formula. Now, by the action of two distinct displacement-type or generalized displacement operators defined in Eqs.  (6) and (7) on the number state, the NDNSs are introduced in the following ways:

By substituting Eq.  (6) into relations  (8) and after some lengthy but straightforward manipulations, the explicit form of the NDNSs is given by

where [f(n)]! = f(n)f(n − 1) … f(1) with the conventional relation [f(0)]! = 1,

corresponds to the associated Laguerre polynomials and , i = 1, 2, refers to the normalization factors which are given by

Similarly, the exact form of the second type of the NDNSs reads as

with the following normalization constants

By looking deeply at the NDNSs obtained in Eqs.  (10) and (12) and comparing them with the introduced NDNSs in Eq.  (2), it is manifestly found that they are essentially different from each other by the term [f(n)]!. We would like to emphasize the fact that the nonlinear terms [f(n)]! and [f(m)]! are logically obtained in our introduced state while the term [f(n)]! which is seen in Ref.  [38] does not arise from a reasonable procedure, since the authors have manually entered this term in DNSs. It is also valuable to state that based on our formalism, many NDNSs can be easily constructed by using various nonlinearity functions associated with nonlinear oscillators as well as every solvable quantum systems (due to the simple relation en = n f2(n)), refer to Refs.  [35] and [36]. In the next section, by using the group-theoretical method, another class of NDNS with particular nonlinearity function f(n) is acquired.

3. Nonlinear displaced number states: Group-theoretical approach

It is illustrated that, by considering the group algebra[40] and paying attention to the fact that the construction of a unitary displacement operator with  and  is possible through the particular nonlinearity functions associated with the specific physical systems, a few classes of nonlinear coherent states may be produced. Based on this fact, in the following, two types of NDNSs are introduced by using the group representation.

3.1. Gilmore– Perelomov-type of SU(1, 1) coherent states

Keeping in mind the approach of Man’ ko et al. in Ref.  [20], it is shown that, the (modified) trigonometric potential V (x) = U0 tan2(bx), in which U0 is the strength of the potential and b is its range, [41] corresponds to the nonlinearity function fGP(n) which is given by[42]

In the latter relation, Ω is the frequency of the field, μ is the mass of the particle, λ is related to the potential strength and is sometimes the so-called Bargmann index, which can take any positive integers or half integers, i.e., λ = 1/2, 1, 3/2, 2, … . Also, the parameter b denotes the potential range and is obtained via the relation λ (λ + 1) = 2μ U0/ħ 2b2. By substituting the nonlinearity function  (14) into the f-deformed bosonic annihilation operator  GP = â fGP(), one may define the new operators

and 0 = λ + n satisfying the commutation relations [0, ± ] = ± ± and [, + ] = 20, which are the well-known su(1, 1) Lie algebra.[42] Based on the group-theoretical construction for the Gilmore– Perelomov approach corresponding to discrete series representation of SU(1, 1) group, the displacement operator reads as .[43] Now, by the action of on the number state, the NDNSs associated with SU(1, 1) group are given by

where we have used and ζ = (ξ /| ξ | ) tanhξ with | ξ | < 1. The condition | ζ | < 1 implies the fact that the phase space of the SU(1, 1) coherent states is confined to the interior of the unit disk of the complex plane.

3.2. SU(2) coherent states

Another case of a physical potential, which can be equivalent to a nonlinearity function, is known as the modified Pö schl– Teller potential by relation V(x) = U0 tanh2(ax) with U0 and a as the depth and the range of well, respectively.[41] This potential is related to a system that possesses a finite discrete spectrum. The corresponding nonlinearity function is of the form

where μ denotes the reduced mass of the molecule and s means the depth of well which is related to its range though the relation s(s + 1) = 2 μ U0/ħ 2a2. Considering the f-deformed bosonic annihilation operator , the new operators, , , and may be defined with the commutation relations and . Paying attention to the fact that the introduced operators clearly satisfy the SU(2) Lie algebra, [42] the displacement-type operator corresponding to this group reads as with . By the action of such a displacement operator on the number state, the new class of NDNSs associated with SU(2) group is obtained by the following relation

where γ = (η /| η | ) tanh η . It may be noted that the parameter s can get values 1/2, 1, 3/2, 2, … . Adding our obtained results in the two latter sections, it is seen that we have produced four different classes of NDNSs, all of which have been introduced by some reasonable procedures. Anyway, we are now in a position to examine the nonclassicality features of the obtained NDNSs in the continuation of the paper.

4. Nonclassical criteria

Since the nonclassical light is of special attention in the field of quantum optics and quantum information processing, in this section, we are going to study some of the well-known nonclassicality features of the introduced NDNSs. For this purpose, sub-Poissonian statistics as well as the negativity of Wigner distribution function are examined, numerically. Before proceeding, it ought to be mentioned that for evaluating any quantity for the NDNSs which have been produced by algebraic method (the relations  (10) and (12)), a nonlinearity function should be chosen. For this purpose, we use the nonlinearity function f(n) = (1 + kn)− 1, which has been considered in Ref.  [38].

4.1. Sub-Poissonian statistics: Mandel parameter

This subsection deals with studying the quantum statistics of the states through the Mandel Q-parameter, which characterizes the photon statistics of light. This parameter has been defined as[44]

Whenever − 1 ≤ Q < 0 (Q > 0) the statistics are sub-Poissonian (super-Poissonian) and Q = 0 indicates the Poissonian statistics. By the way, the state vector of the system shows the nonclassical behavior when the photons statistics of field are sub-Poissonian.

Figure  1 shows the Mandel parameter for some different classes of NDNSs corresponding to (a) | α , f, n〉 ′ , (b) | α , f, n〉 ″ , (c) | ζ , f, n〉 , and (d) | γ , f, n〉 corresponding to the relations  (10), (12), (15), and (17), respectively. It is seen from Fig.  1(a) that, nonclassical behavior (sub-Poissonian statistics) is obviously observed in some intervals of α . In addition, by increasing the value of n, this behavior is strengthened. Unlike Fig.  1(a), figure  1(b) indicates that the maximum nonclassicality sign occurs when n = 0 (nonlinear displaced vacuum state). In these two latter figures, it is seen that, by increasing α , the Mandel parameter gets negative values everywhere, i.e., the photon statistics of the field becomes full sub-Poissonian. Figures  1(c) and 1(d) exhibit locally (around α = 0) sub-Poissonian statistics, in which by an increase of λ or s, the space for which the photon statistics is sub-Poissonian, is gradually decreased.

Fig.  1. Variation of the Mandel parameter for different classes of NDNSs: (a) | α , f, n〉 , fk(n) = (1 + kn)− 1, and k = 0.07; (b) | α , f, n〉 ″ , fk(n) = (1 + kn)− 1, and k = 0.07; (c) | ζ , f, n〉 , and n = 3; and (d) | γ , f, n〉 and n = 1.

4.2. Wigner distribution function

The Wigner function, known as the earliest quasi-probability distribution function, [45] is a useful criterion which specifies the nonclassicality of the field. It is now valuable to declare that although the Wigner function, in the sense that it is a distribution function, will have to be commonly positive, there may exist some finite regions in the phase space of the Wigner function of a quantum state, in which this function gets negative values; a fact that is called `nonclassicality feature’ . The Wigner function associated with any quantum state can be expressed as[4648]

where | n, α 〉 = (α )| n〉 is the displaced number state introduced in Ref.  [27] and denotes the density matrix operator of a quantum state. Considering the obtained NDNSs via algebraic method in Eqs.  (10) and (12), the corresponding Wigner functions may be evaluated in the form

Similarly, the Wigner function associated with NDNSs of SU(1, 1) and SU(2) groups are respectively evaluated as follows:

In Figs.  2, we have plotted the Wigner distribution function of the NDNSs obtained in relations  (10), (12), (15), and (17) for the same chosen parameters as mentioned in Fig.  1. Figures  2(a)– 2(d) indicate clearly the negativity of Wigner function in some finite regions of phase space, which implies the fact that the introduced NDNSs are ‘ nonclassical’ . It is also valuable to state that, by comparing quantitatively Fig.  2(a) with Figs.  2(b)– 2(d), it is seen that the amount of the negativity of the Wigner function (the depth of this nonclassicality feature) in Fig.  2(a) is nearly 10 times greater than the others. In other words, the strength of nonclassicality of the state in Eq.  (10) is more visible than the other states in Eqs.  (12), (15), and (17).

Fig.  2. Variation of the Wigner distribution function for the NDNSs similar to Fig.  1.

5. Summary and conclusion

In this paper, by modifying the formalism of NDNSs presented in Ref.  [38], we have introduced four distinct classes of NDNSs through algebraic and group treatments. For this purpose, by considering the DNSs together with nonlinear coherent states approach, two distinct classes of NDNSs were reasonably obtained via an algebraic treatment. In addition, by using a special class of Gilmore– Perelomov-type of SU(1, 1) and a class of SU(2) coherent states (group approach), two other NDNSs were also introduced. Then, in order to study the nonclassicality features of the introduced states, sub-Poissonian statistics by evaluating Mandel parameter and the variation of Wigner quasi-probability distribution function associated with the obtained NDNSs were numerically examined. The presented results showed that the NDNSs exhibit sub-Poissonian statics (nonclassical behavior) in a finite region. Also, as another appearance of the nonclassicality signs of the NDNSs, it was observed that the Wigner function is also negative in some areas of phase space. This means that the NDNSs can be considered as a good candidate for nonclassical light.

Acknowledgments

The authors would like to thank the referees for their helpful comments which clarified the content of the paper.

Reference
1 Klauder J R and Skagerstam B S 1985 Coherent States: Applications in Physics and Mathematical Physics Singapore World Scientific [Cited within:1]
2 Schumacher B 1996 Phys. Rev. A 54 2614 DOI:10.1103/PhysRevA.54.2614 [Cited within:1] [JCR: 3.042]
3 Kempe J 1999 Phys. Rev. A 60 910 DOI:10.1103/PhysRevA.60.910 [Cited within:1] [JCR: 3.042]
4 Bennett C H, Shor P W, Smolin J A and Thapliyal A V 1999 Phys. Rev. Lett. 83 3081 DOI:10.1103/PhysRevLett.83.3081 [Cited within:1] [JCR: 7.943]
5 Ali S T, Antoine J P and Gazeau J P 2000 Coherent States, Wavelets and Their Generalizations New York Springer [Cited within:1]
6 Honarasa G R, Tavassoly M K and Hatami M 2012 Chin. Phys. B 21 054208 DOI:10.1088/1674-1056/21/5/054208 [Cited within:1] [JCR: 1.148] [CJCR: 1.2429]
7 Tavassoly M K and Jalali H R 2013 Chin. Phys. B 22 084202 DOI:10.1088/1674-1056/22/8/084202 [Cited within:1]
8 Meekhof D M, Monroe C, King B E, Itano W M and Wineland D J 1996 Phys. Rev. Lett. 76 1796 DOI:10.1103/PhysRevLett.76.1796 [Cited within:1] [JCR: 7.943]
9 Zou X, Pahlke K and Mathis W 2002 Phys. Rev. A 65 064303 DOI:10.1103/PhysRevA.65.064303 [Cited within:1] [JCR: 3.042]
10 Deleglise S, Dotsenko I, Sayrin C, Bernu J, Brune M, Raimond J M and Haroche S 2008 Nature 455 510 DOI:10.1038/nature07288 [Cited within:1] [JCR: 38.597]
11 Faghihi M J and Tavassoly M K 2013 J. Phys. B: At. Mol. Opt. Phys. 46 145506 DOI:10.1088/0953-4075/46/14/145506 [Cited within:1] [JCR: 2.031]
12 Faghihi M J and Tavassoly M K 2013 J. Opt. Soc. Am. B 30 2810 DOI:10.1364/JOSAB.30.002810 [Cited within:1] [JCR: 2.21]
13 Faghihi M J, Tavassoly M K and Bagheri Harouni M 2014 Laser Phys. 24 045202 DOI:10.1088/1054-660X/24/4/045202 [Cited within:1] [JCR: 2.545]
14 Faghihi M J, Tavassoly M K and Hatami M 2014 Physica A 407 100 DOI:10.1016/j.physa.2014.03.092 [Cited within:1]
15 Hekmatara H and Tavassoly M K 2014 Opt. Commun. 319 121 DOI:10.1016/j.optcom.2013.12.056 [Cited within:1] [JCR: 1.438]
16 Baghshahi H R and Tavassoly M K 2014 Phys. Scr. 89 075101 DOI:10.1088/0031-8949/89/7/075101 [Cited within:1]
17 Baghshahi H R, Tavassoly M K and Behjat A 2014 Chin. Phys. B 23 074203 DOI:10.1088/1674-1056/23/7/074203 [Cited within:1] [JCR: 1.148] [CJCR: 1.2429]
18 Baghshahi H R, Tavassoly M K and Behjat A 2014 Commun. Theor. Phys. 62 430 DOI:10.1088/0253-6102/62/3/22 [Cited within:1]
19 de Matos Filho R L and Vogel W 1996 Phys. Rev. A 54 4560 DOI:10.1103/PhysRevA.54.4560 [Cited within:3] [JCR: 3.042]
20 Man’ko V I, Marmo G, Sudarshan E C G and Zaccaria F 1997 Phys. Scr. 55 528 DOI:10.1088/0031-8949/55/5/004 [Cited within:4]
21 Tavassoly M K 2006 J. Phys. A: Math. Gen. 39 11583 DOI:10.1088/0305-4470/39/37/016 [Cited within:1] [JCR: 1.577]
22 Tavassoly M K and Parsaiean A 2007 J. Phys. A: Math. Theor. 40 9905 DOI:10.1088/1751-8113/40/32/014 [Cited within:1] [JCR: 1.766]
23 Tavassoly M K 2008 J. Phys. A: Math. Theor. 41 285305 DOI:10.1088/1751-8113/41/28/285305 [Cited within:1] [JCR: 1.766]
24 Honarasa G R, Tavassoly M K and Hatami M 2009 Phys. Lett. A 373 3931 DOI:10.1016/j.physleta.2009.08.055 [Cited within:1] [JCR: 1.11]
25 Honarasa G R, Tavassoly M K and Hatami M 2009 Opt. Commun. 282 2192 DOI:10.1016/j.optcom.2009.02.039 [Cited within:1] [JCR: 1.438]
26 Berrada K 2014 Chin. Phys. B 23 024208 DOI:10.1088/1674-1056/23/2/024208 [Cited within:1] [JCR: 1.148] [CJCR: 1.2429]
27 de Oliveira F A M, Kim M S, Knight P L and Buzek V 1990 Phys. Rev. A 41 2645 DOI:10.1103/PhysRevA.41.2645 [Cited within:2] [JCR: 3.042]
28 Schleich W and Wheeler J A 1987 J. Opt. Soc. Am. B 4 1715 DOI:10.1364/JOSAB.4.001715 [Cited within:1] [JCR: 2.21]
29 Tavassoly M K 2010 Opt. Commun. 283 5081 DOI:10.1016/j.optcom.2010.08.002 [Cited within:1] [JCR: 1.438]
30 Honarasa G R, Tavassoly M K, Hatami M and Roknizadeh R 2011 Physica A 390 1381 DOI:10.1016/j.physa.2010.10.049 [Cited within:1] [JCR: 1.676]
31 Safaeian O and Tavassoly M K 2011 J. Phys. A: Math. Theor. 44 225301 DOI:10.1088/1751-8113/44/22/225301 [Cited within:1] [JCR: 1.766]
32 Faghihi M J and Tavassoly M K 2011 Commun. Theor. Phys. 56 327 DOI:10.1088/0253-6102/56/2/24 [Cited within:1]
33 Piroozi E and Tavassoly M K 2012 J. Phys. A: Math. Theor. 45 135301 DOI:10.1088/1751-8113/45/13/135301 [Cited within:1] [JCR: 1.766]
34 Ali S T, Roknizadeh R and Tavassoly M K 2004 J. Phys. A: Math. Gen. 37 4407 DOI:10.1088/0305-4470/37/15/009 [Cited within:2] [JCR: 1.577]
35 Roknizadeh R and Tavassoly M K 2004 J. Phys. A: Math. Gen. 37 8111 DOI:10.1088/0305-4470/37/33/010 [Cited within:2] [JCR: 1.577]
36 Roknizadeh R and Tavassoly M K 2005 J. Math. Phys. 46 042110 DOI:10.1063/1.1861276 [Cited within:1] [JCR: 1.296]
37 Xu L J, Tan G B, Ma S J and Guo Q 2013 Chin. Phys. B 22 030311 DOI:10.1088/1674-1056/22/3/030311 [Cited within:1] [JCR: 1.148] [CJCR: 1.2429]
38 de Oliveira G C, de Almeida A R, Dantas C and Moraes A M 2005 Phys. Lett. A 339 275 DOI:10.1016/j.physleta.2005.03.033 [Cited within:6] [JCR: 1.11]
39 Roy B and Roy P 2000 J. Opt. B: Quantum Semiclas. Opt. 2 65 DOI:10.1088/1464-4266/2/1/311 [Cited within:2]
40 Gilmore R 1974 Lie Groups, Lie Algebras and Some of Their Applications New York John Wiley & Sons [Cited within:1]
41 Nieto M M 1978 Phys. Rev. A 17 1273 DOI:10.1103/PhysRevA.17.1273 [Cited within:2] [JCR: 3.042]
42 Miry S R and Tavassoly M K 2012 Phys. Scr. 85 035404 DOI:10.1088/0031-8949/85/03/035404 [Cited within:3]
43 Perelomov A M 1986 Generalized Coherent States and Their Applications: Modern Methods of Plant Analysis Berlin Springer-Verlag [Cited within:1]
44 Mand el L 1979 Opt. Lett. 4 205 DOI:10.1364/OL.4.000205 [Cited within:1] [JCR: 3.385]
45 Wigner E 1932 Phys. Rev. 40 749 DOI:10.1103/PhysRev.40.749 [Cited within:1] [JCR: 6.583]
46 Gerry C C and Knight P L 2005 Introductory Quantum Optics Cambridge Cambridge University Press [Cited within:1]
47 Vogel W and Welsch D G 2006 Quantum Optics New York John Wiley & Sons [Cited within:1]
48 Meng X G, Wang J S and Liang B L 2013 Chin. Phys. B 22 030307 DOI:10.1088/1674-1056/22/3/030307 [Cited within:1] [JCR: 1.148] [CJCR: 1.2429]