PHYSICAL REVIEW A 80, 013610 共2009兲 Generalized purity and quantum phase transition for Bose-Einstein condensates in a symmetric double well T. F. Viscondi, K. Furuya, and M. C. de Oliveira Instituto de Física “Gleb Wataghin,” Universidade Estadual de Campinas, 13083-970 Campinas, SP, Brazil 共Received 20 December 2008; published 16 July 2009兲 The generalized purity is employed for investigating the process of coherence loss and delocalization of the Q function in the Bloch sphere of a two-mode Bose-Einstein condensate in a symmetrical double well with cross collision. Quantum phase transition of the model is signaled by the generalized purity as a function of an appropriate parameter of the Hamiltonian and the number of particles 共N兲. A power-law dependence of the critical parameter with N is derived. DOI: 10.1103/PhysRevA.80.013610 PACS number共s兲: 03.75.Lm, 03.67.Mn, 03.75.Gg, 64.70.Tg II. GENERALIZED PURITY AND THE BECSDW MODEL I. INTRODUCTION Recently it has been pointed out that any bipartite and multipartite entanglement measure can signal the presence of a quantum phase transition 共QPT兲 关1–3兴 in many-particle systems. Related to that, a subsystem-independent generalization of entanglement has been introduced based on coherent states and convex sets characterizing the unentangled pure states as coherent states of a chosen Lie algebra 关4兴. Such a notion of entanglement defined relative to a distinguished subspace of observables is pointed as particularly useful for classifying multipartite entanglement and thus for QPT characterization. The generalized purity of the state relative to a certain distinguished subset of observables forming a local Lie algebra is directly related to the MeyerWallach measure 关5兴, and whenever a specific subsystem can be associated to the subset of observables the usual entanglement notion is recovered. On the other hand it has been demonstrated that the model describing a two-mode BoseEinstein condensate in a symmetric double well 共BECSDW兲 关6兴, with cross-collisional terms 关7,8兴, presents interesting dynamical regimes: The macroscopic self-trapping 共MST兲 and Josephson oscillations 共JO兲 of population 关6,8,9兴, both experimentally observed 关10兴. Recently a discussion of the transition from one regime to the other has been presented from the point of view of critical phenomena, as a continuous QPT problem in terms of the usual subsystem entropy 关11–13兴. It is thus certainly important to investigate which features of this transition are signaled by a subsystemindependent entanglement measure. In this paper we apply the concept of generalized purity in a BECSDW for a twofold purpose: 共i兲 To quantify the quality of the semiclassical approach commonly employed in the literature for the BECSDW; 共ii兲 To characterize the quantum critical phenomena occurring in this model with a subsystem-independent measure of quantum correlations 关4兴. In Sec. II we introduce the model, define the generalized purity of the su共2兲 algebra and analyze the quality of the semiclassical results. Section III is devoted to the connection between the classical bifurcation and the quantum phase transition from JO to MST regime, and to the characterization of this critical phenomenon using the purity of the su共2兲 algebra. Conclusions are drawn in Sec. IV. 1050-2947/2009/80共1兲/013610共5兲 The two-mode approximated BECSDW has been well studied in the literature 共see, e.g., 关6,9兴兲 as a model presenting a nonlinear self-trapping phenomenon. More recently, the importance of the cross-collisional terms for large number of particles in the condensate 共N Ⰷ 1兲 has been noticed 关7兴 and explored semiclassically with a time-dependent variational principle based on coherent states 关8兴. For a fixed number of condensed particles N, in order to explore the natural group structure of the model, we conveniently adopt the Schwinger’s pseudospin operators defined in terms of the creation † , d⫾ on the approximated and annihilation boson operators d⫾ localized states 兩u⫾典 关6,8兴: Jx ⬅ 共d−†d− − d+†d+兲 / 2, Jy ⬅ i共d−†d+ − d+†d−兲 / 2, and Jz ⬅ 共d+†d− + d−†d+兲 / 2, where J = N / 2. In that form the two-mode BEC Hamiltonian writes as 冋 Ĥ = 2 2⌳共N − 1兲 + 册 ⍀ Jz + 2共 − 兲J2x + 4Jz2 , 2 共1兲 where ⍀ is the tunneling parameter and is the self-collision parameter of the condensate which is much larger than the so-called cross-collision terms = ⑀2 , ⌳ = ⑀3/2, with ⑀ = 具u+ 兩 u−典. ⍀⬘ ⬅ 2关2⌳共N − 1兲 + ⍀ / 2兴 is an effective tunneling parameter dependent on N. The natural associated algebra of the model is su共2兲. In this form Hamiltonian 共1兲 is a realization of the Lipkin-Meshkov-Glick model 关14兴, whose ground-state entanglement has been investigated recently 关4,13兴. We should remark that this model with the crosscollision terms included describes more appropriately the experimental observation of an atom-number-dependent tunneling rate in an optical lattice realization 关7,8,10兴. Thus in principle any conclusions derived here can be implemented in the same experimental setup. By means of a semiclassical method exploring SU共2兲 coherent states we demonstrated that for a sufficiently large N, even a small amount of cross-collisional rate can change the dynamical regime of oscillations of the condensate from MST to JO 关8兴. The quantum and semiclassical dynamics of the BECSDW are known to be qualitatively very similar 关6,8兴 for large number of particles 共N Ⰷ 1兲, except for the presence of collapses and revivals in the quantum time evolutions for the mean values of 具Jx典共t兲. This breaking of quantum-classical correspondence is due to quantum fluctuations, which drive the system state away from being coherent 013610-1 ©2009 The American Physical Society PHYSICAL REVIEW A 80, 013610 共2009兲 VISCONDI, FURUYA, AND DE OLIVEIRA 关15兴. When we treat the semiclassical dynamics employing a time-dependent variational principle 关16兴, we restrict the evolution of the state to a nonlinear subspace constituted only by the coherent states of SU共2兲 关8兴. Such an evolution is exact for an initially coherent state only in the classicalmacroscopic limit of N → ⬁ 关17兴. Also, in the time-dependent variational principle approach we force the system quantum representations to be always localized in the phase space. From this point of view, the coherent states are the closest to the classical ones, which are points in the classical phase space, and converges to them in the limit N → ⬁. The delocalization of the quantum state is responsible for the quantitative disagreement between the two dynamics 关8兴. As a consequence, collapses and revivals of expectation values of relevant observables occurring in the quantum description are never recovered with the semiclassical approach. For a more complete analysis of the quality of the semiclassical approximation, it becomes fundamental to have a good quantitative measure of the “distance” of a given state to the subspace of the coherent states. When the complete dynamics of the system is restricted to a space that carries an irreducible representation of SU共2兲 共here this condition is satisfied due to the particle number conservation兲, there is a simple measure 共obtained from the total uncertainty of the algebra 关18兴兲 called generalized purity of the algebra Psu共2兲 关4,19兴, and defined as Psu共2兲共兩典兲 = 1 兺 具兩Jk兩典2 . J2 k=x,y,z 共2兲 It should be noticed that in this last form it is easy to relate the generalized purity with the concept of spin squeezing recently employed for experimental verification of entanglement for BEC trapped in a double or six-well potential of an optical lattice 关20兴 共see references therein for a general coverage of the spin squeezing concept and utilization兲. We postpone entanglement analysis to the next section. We want first to remark that the generalized purity is a good measure of distance from a coherent state, among other reasons, because it is invariant under a transformation of the group SU共2兲 on the state 兩典: Psu共2兲共兩典兲 = Psu共2兲共U兩典兲 , ∀ U 苸 SU共2兲. Thus, all states connected by a SU共2兲 transformation possess the same purity. However, the most interesting property of Psu共2兲 共concerning the purpose of quantitatively compare the correspondence between the semiclassical and the exact quantum dynamics兲 is the fact that this measure attains its maximum value at one, if and only if, 兩典 is the coherent state closest to a classical one: 兩 , 典 = R共 , 兲兩J , −J典 = e−i共Jx sin −Jy cos 兲兩J , −J典. As soon as the dynamics takes the state away from the space consisting only of the states 兩 , 典, making the system more delocalized in the phase space, Psu共2兲 decreases monotonically to zero. We remark that Psu共2兲 only has such properties clearly defined for pure states and only then it is a measure of existing quantum correlations of the state in the classical phase space. We choose as initial state 兩J , J典x ⬅ 兩 = 2 , = 0典, where N = 100 particles are in the same well, with ⍀ = 1 and = 2N⍀ . For this set of parameters it is known that by setting = 100 the state is in the self-trapping region of the phase space, FIG. 1. 共Color online兲 Time evolution of Psu共2兲 for MST and JO dynamical regimes of the two-mode BEC model. The dashed curve 2⍀ represents the MST regime with = N and = 100 , whereas the 2⍀ solid curve represents the regime of JO with = N and = 10 . For both cases the initial state of the system is the coherent state 兩J , J典x ⬅ 兩 = 2 , = 0典, where N = 100 particles are initially in the same well. whereas for = 10 it is outside the self-trapping region and thus in the JO regime 关8兴. In Fig. 1 we plot Psu共2兲, where the MST regime is in dashed line, and solid one for JO regime. In the MST regime Psu共2兲 quickly drops down from 1 stabilizing close to 0.9 for ⍀t ⬇ 10, indicating that the dynamics takes the state away from the subspace of the coherent states. The region of almost constant purity coincides with the collapse region of population dynamics 关8兴. Note that close to ⍀t = 30 the purity shows small oscillations, and in the region close to ⍀t = 60 the purity increases again until it practically recovers the value 1. At this instant the quantum state gets closer to a coherent one, being this responsible for the revival of the oscillations of the population dynamics 关8兴. In the MST regime the large value of Psu共2兲 indicates a relative good agreement between the quantum and semiclassical results. This agreement is due to the oscillation of the mean value of the generator Jx in the MST since the purity depends on the normalized square of such a mean value. The oscillations of 具Jx典 around a value close to J keeps also Psu共2兲 close to its maximum possible value. In the JO regime the purity also decays rapidly with the time as the system is driven away from a coherent one, but the purity reaches much lower values compared to the MST, never returning close to 1. Hence, this regime presents lower quantitative agreement between the quantum and classical evolutions, when compared to the MST regime. Close to ⍀t = 250 关inset of Fig. 1兴 the state gets the closest possible to a coherent one, but Psu共2兲 is still lower than 0.4. This result is expected because the classical orbit delocalizes much more on the Bloch sphere for this regime, and this entails a correspondingly large delocalization of the semiclassical Q function on the sphere, Q共 , 兲 = 具 , 兩兩 , 典, with = 兩典具兩, during its evolution 关8,21兴. The larger the region traveled by the classical trajectory in the phase space, the larger is the broadening of the distribution and smaller the coherence left on the state. Therefore, when the Hamiltonian has nonlinear terms in the dynamical group generators, the semiclassical approximation has better quantitative accordance with the exact quantum results 共for finite N兲 when the classical orbits sweep smaller 013610-2 PHYSICAL REVIEW A 80, 013610 共2009兲 GENERALIZED PURITY AND QUANTUM PHASE… “volume” in the phase space. Since the BECSDW model is integrable, we cannot analyze how chaotic trajectories would drive the system state away from a coherent one. However, our present results indicate that the validity of the semiclassical method rapidly decreases for this type of less localized trajectories. III. PHASE TRANSITION Now we can take advantage of the many qualities of Psu共2兲 to characterize the QPT 关3兴 in the BECSDW model. The QPT is connected to a nonanalyticity of the energy of the fundamental state of the system, when it is taken as a function of some real continuous parameter of the Hamiltonian 关1兴 at zero temperature, in the macroscopic limit N → ⬁. Generally speaking, the energy of the ground state in a finite system is an analytic function of any parameter of the Hamiltonian and only shows nonanalyticity when N → ⬁. Even though such a limit is not effectively taken here, we can still observe the scaling of the system properties for increasing N and infer about the QPT. The BECSDW suffers a sudden change in its dynamics ⍀ in the limit of no cross-collision terms and N when c = 2N Ⰷ 1. With ⍀ , ⬎ 0, such a transition 共JO to MST兲 does not occur due to a critical change in the ground state, but at the largest energy state for the parameter value corresponding to the bifurcation in the classical phase space, leading to the appearance of a separatrix of motion. However, it can be treated formally in the same way as a usual QPT since the maximum energy state is just the fundamental state through the transformation Ĥ → −Ĥ or, equivalently, ⍀ , → −⍀ , −. Moreover, there is evidence that energy levels up to the energy of the corresponding separatrix orbit sense the quantum phase transition 关22兴. In Fig. 2, we have the Q functions for the largest energy eigenstate of Ĥ for several values of and . Figure 2共a兲 shows the coherent state 兩 = , 典 = 兩J , J典z, which is the maximum energy state of the noninteracting case = = 0. Increasing , but still not considering the cross-collision terms, the Q function broadens along the x axis, and consequently we expect the decreasing in Psu共2兲. At = c 关Fig. 2共b兲兴 the distribution is greatly broadened but does not show a bifurcation, namely, the formation of two peaks. This behavior is expected since for finite N the quantum transition parameter qc 共N兲 is slightly different from the value of transition c of the classical limit. But for increased , such as in Fig. 2共c兲 for = ⍀N , two peaks emerge along the x axis as a signature of the bifurcation. The two peaks move away with increasing , while the increase in the cross collision causes the opposite effect. For = 2N⍀ and = 10 , the two peaks of the Q function become closer, as in Fig. 2共d兲. Our results for the phase-space distribution of the maximum energy state are confirmed as we analyze the behavior of Psu共2兲 as a function of the self-collision parameter and the number of particles, as in Fig. 3, neglecting the cross collisions. Psu共2兲 initially decreases slowly with ⍀N , independent of the value of N, corresponding to the region where the distributions broadens along the x axis. However, close FIG. 2. 共Color online兲 Q function for the largest energy state of the Ĥ spectrum for several value of parameters and . Considering the number of particles N = 100 and ⍀ = 1, we have the follow⍀ ing values for the collision rates: 共a兲 = = 0; 共b兲 = 2N , = 0; 共c兲 ⍀ 2⍀ = N , = 0, and 共d兲 = N , = 10 . to ⍀N = 21 , Psu共2兲 begins to decrease quickly and, although smoothly, the lowering of its value gets more steep as we increase N. This behavior of Psu共2兲 suggests us a strong dependence between the derivative of Psu共2兲 with respect to ⍀N and the number of particles. Since Psu共2兲 signals entanglement, it is clear that particle entanglement is considerably higher in the MST phase than in the JO phase. We can understand this feature since in the MST the atomic interaction is much stronger than in the JO regime, leading thus to a stronger entanglement. The peaking of the derivative of Psu共2兲 共or any other conceivable measure of entanglement兲 with ⍀N signals a QPT FIG. 3. 共Color online兲 Psu共2兲 for the largest energy eigenstate as a function of normalized self-collision parameter and the number of particles, with cross-collision rate = 0. 013610-3 PHYSICAL REVIEW A 80, 013610 共2009兲 VISCONDI, FURUYA, AND DE OLIVEIRA the overall behavior can be inferred from the discussion above 共see 关7,8兴 for a more complete discussion on the effect of the cross-collision terms兲. IV. CONCLUSION FIG. 4. 共Color online兲 Derivative of Psu共2兲 of the eigenstate N of largest energy eigenvalue with respect to ⍀ for various values of the total number of particles N. The dashed vertical line represents cN 1 the position at the value of the classical transition point ⍀ = 2 . All the curves for finite systems cross exactly at this critical value. 关1,2兴. In Fig. 4 we show dPsu共2兲 / d共N / ⍀兲 for several N. For increasing N we see the minimum derivative value shifting to the left 共closer to the classical critical value 0.5兲 as it becomes more pronounced. We define the value of at the minimum as the critical value of the quantum dynamical transition qc 共N兲. It is clear that the value of qc 共N兲 is brought ⍀ closer to the classical transition value c = 2N for increasing N, but we still need to characterize how this approximation N 共 q− 兲 happens. The values of ln关 ⍀c c 兴 from the curves in Fig. 4 suggest a power-law between 共qc − c兲 and N. A linear interpolation of the data points gives qc − c = ⍀e0,31⫾0,05N−1,657⫾0,009. It is clear that qc → c as N → ⬁, evidencing the signaling of the transition by Psu共2兲 in contrast to the findings of 关4兴 for the ground state. This is so because in the N → ⬁ limit, after the transition, the ground state is twofold degenerated. However, in our finite N inference, there is no degeneracy in the maximum energy level and Psu共2兲 is perfectly suited for indicating the QPT occurring at c, even though nothing can be said about its order 关2兴. The effect of the cross-collisional term is merely to shift the transition point c and, despite of not being considered here, 关1兴 L. A. Wu, M. S. Sarandy, and D. A. Lidar, Phys. Rev. Lett. 93, 250404 共2004兲; L.-A. Wu, M. S. Sarandy, D. A. Lidar, and L. J. Sham, Phys. Rev. A 74, 052335 共2006兲. 关2兴 T. R. de Oliveira, G. Rigolin, M. C. de Oliveira, and E. Miranda, Phys. Rev. Lett. 97, 170401 共2006兲. 关3兴 See L. Amico, R. Fazio, A. Osterloh, and V. Vedral, Rev. Mod. Phys. 80, 517 共2008兲, and references therein. 关4兴 H. Barnum, E. Knill, G. Ortiz, and L. Viola, Phys. Rev. A 68, 032308 共2003兲; H. Barnum, E. Knill, G. Ortiz, R. Somma, and L. Viola, Phys. Rev. Lett. 92, 107902 共2004兲; R. Somma, G. Ortiz, H. Barnum, E. Knill, and L. Viola, Phys. Rev. A 70, 042311 共2004兲. 关5兴 D. A. Meyer and N. R. Wallach, J. Math. Phys. 43, 4273 共2002兲. In conclusion we considered the generalized purity, Psu共2兲, to analyze the dynamics of coherence loss of initially coherent state for the BECSDW model. In the MST regime Psu共2兲 remains high without significant departure from a coherentstate description. For the JO regime, on the other hand, we have seen that the decay of Psu共2兲 was in a similar time scale to the MST one, but the system state is strongly driven away from a coherent one and no considerable recurrence to any coherent state is observed. Since the coherent state represents the closest to the classical state, the value of the generalized purity enabled us to quantify the quality of the semiclassical approximation at each time in both regimes. Moreover, we have employed Psu共2兲 as a tool for characterizing a QPT in the same model. We have shown for finite number of particles the bifurcation of the Q function of the largest energy state as the self-collision parameter becomes larger than a critical value qc 共N兲. By increasing the number of particles N, Psu共2兲 has shown a more and more steep behavior near the critical value of ⍀N ; moreover, its value has approached the N known classical value ⍀c = 21 as N → ⬁. Finally we have shown that qc − c is consistent with a power law in N. Therefore, Psu共2兲 is an excellent measure of the dynamical loss of coherence, distinguishing the two types of population dynamics and indicating the QPT. When a state suffers fundamental changes resulting from the QPT, its generalized purity must follow its behavior because it has all the information about its coherence and the degree of localization over the phase space. ACKNOWLEDGMENTS We acknowledge J. Vidal for bringing several aspects of the LMG model to our knowledge and for his comments and L. Viola for a careful reading and suggestions. Our work is supported by FAPESP and CNPq. 关6兴 G. J. Milburn, J. Corney, E. M. Wright, and D. F. Walls, Phys. Rev. A 55, 4318 共1997兲. 关7兴 B. R. da Cunha and M. C. de Oliveira, Phys. Rev. A 75, 063615 共2007兲; B. da Cunha and M. de Oliveira, e-print arXiv:cond-mat/0507506. 关8兴 T. F. Viscondi, K. Furuya, and M. C. de Oliveira, e-print arXiv:0811.2139; Ann. Phys. 共in press兲. 关9兴 A. Smerzi, S. Fantoni, S. Giovanazzi, and S. R. Shenoy, Phys. Rev. Lett. 79, 4950 共1997兲; S. Raghavan, A. Smerzi, S. Fantoni, and S. R. Shenoy, Phys. Rev. A 59, 620 共1999兲. 关10兴 M. Albiez, R. Gati, J. Fölling, S. Hunsmann, M. Cristiani, and M. K. Oberthaler, Phys. Rev. Lett. 95, 010402 共2005兲. 关11兴 A. P. Hines, R. H. McKenzie, and G. J. Milburn, Phys. Rev. A 67, 013609 共2003兲. 013610-4 PHYSICAL REVIEW A 80, 013610 共2009兲 GENERALIZED PURITY AND QUANTUM PHASE… 关12兴 L. B. Fu and J. Liu, Phys. Rev. A 74, 063614 共2006兲. 关13兴 J. Vidal, G. Palacios, and C. Aslangul, Phys. Rev. A 70, 062304 共2004兲. 关14兴 H. J. Lipkin, N. Meshkov, and A. J. Glick, Nucl. Phys. 62, 188 共1965兲. 关15兴 The term “decoherence” is sometimes employed since the general purity can also be written as the trace of a squared density operator 关4兴 关reduced in the su共2兲 algebra兴. It should not be confused with the term common usage for describing classical emergence due to the system coupling to a reservoir. Instead here decoherence means a “departure from the most classical 共coherent兲 state.” 关16兴 M. Saraceno and P. Kramer, Geometry of the Time-Dependent Variational Principle in Quantum Mechanics, Lecture Notes in Physics Vol. 140 共Springer-Verlag, New York, 1981兲. 关17兴 This is also true when the Hamiltonian is linear in the generators of the dynamical group with = 0 = . 关18兴 R. Delbourgo, J. Phys. A 10, 1837 共1977兲; R. Delbourgo and J. R. Fox, ibid. 10, L233 共1977兲. 关19兴 A. A. Klyachko e-print arXiv:quant-ph/020601; A. A. Klyachko, B. Öztop, and A. S. Shumovsky, Phys. Rev. A 75, 032315 共2007兲. 关20兴 J. Estéve, C. Gross, A. Weller, S. Giovanazzi, and M. K. Oberthaler, Nature 共London兲 455, 1216 共2008兲. 关21兴 J. R. Anglin and A. Vardi, Phys. Rev. A 64, 013605 共2001兲; F. Trimborn, D. Witthaut, and H. J. Korsch, ibid. 79, 013608 共2009兲. 关22兴 T. Moreira, G. Q. Pellegrino, J. G. Peixoto de Faria, M. C. Nemes, F. Camargo, and A. F. R. de Toledo Piza, Phys. Rev. E 77, 051102 共2008兲. 013610-5
© Copyright 2026 Paperzz