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        First-Order Quantum Phase Transition for Dicke Model Induced by Atom-Atom Interaction?

        2018-01-24 06:22:59XiuQinZhao趙秀琴NiLiu劉妮andJiuQingLiang梁九卿InstituteofTheoreticalPhysicsShanxiUniversityTaiyuan030006China
        Communications in Theoretical Physics 2017年5期

        Xiu-Qin Zhao(趙秀琴),Ni Liu(劉妮), and Jiu-Qing Liang(梁九卿)Institute of Theoretical Physics,Shanxi University,Taiyuan 030006,China

        2Department of Physics,Taiyuan Normal University,Taiyuan 030001,China

        1 Introduction

        In contrast to classical phase transition,quantum phase transition(QPT),[1]which occurs at absolute zero temperature,can only be accessed by changing the physical parameters,for instance,the magnetic field strength.QPT takes place in many-body system and such QPT is a second-order phase transition.

        Dicke model(DM)[2]is mainly used to describe the interaction between an ensemble ofNidentical two-level atoms and a quantized single-mode bosonic field. Although the form of DM is simple,it contains a rich physical meaning.Moreover,the Dicke Hamiltonian,which contains a phase transition from the normal phase to the super-radiant phase,[3?6]is extensively used in theoretical research.In the atomic physics and solid state physics,the Dicke model has a wide range of research.In the processing of quantum information and quantum computing,QPT has a certain relationship between quantum entanglement and quantum chaos.[3?4,7?9]

        The Dicke-type QPT,[10?11]which is useful to understand quantum many body systems,has been observed in recent experimental setup in 2010.[12]At the same time,a series of theoretical analysis are presented,[10,13?20]especially controlling the atom-atom interactions by the Feshbach resonances.[21]It is highlighted that the effective atomic interaction strength can be manipulated by Feshbach resonance,and in Feshbach resonance point,that is near its size and even up to the magnitude of MHz.Noting that the effective dipole-dipole interactions between the atoms are ignored in the above mentioned DM.In fact,the dipole-dipole interactions,which are spatially dependent on the leading term varying asfor small samples,whererijis the distance betweeni-th andj-th atoms,have a significant contribution to dephasing.[22]Meanwhile,the fluorescent spectrum and the second-order intensity correlation function are strongly dependent on the interatom interactions.[22?24]The hamiltonian of DM shows the great importance of the spin-spin interactions.[24]

        In this paper,we discuss the extended Dicke model including the atom-atom interaction.Based on the spin coherent-state(SCS)variational method,[25?26]we reveal the exact solutions of the ground state about the extended Dicke Hamiltonian.According to the analytic solutions,the mean photon numbers,the scaled atomic population and the average energy have been plotted.We also plot the critical curves and ground state phase figure.For theitem,the SCS variational method can not deal with the square item of the atom-atom interaction.In order to solve theitem,the self-consistent- field method[27?36]are introduced.Finally,a first-order phase transition[37]for the extended DM,which is different from the previous conclusion,[24]are revealed.It is demonstrated thatthe critical phase transition point from the normal phase to the superradiant phase is shifted by the dipole-dipole interaction and the self-consistent method applies to the case of small change.

        2 The Extended Hamiltonian

        The proposed DM Hamiltonian describing the interaction of an ensemble ofNidentical two-level atoms coupled to a single mode high- finesse optical cavity is given.For the atom-atom interaction,we only consider a simple two-body interactional potential and obtain the following Hamiltonian,which is expressed as the following three parts

        where the Hamiltonian of the photon is

        and the Hamiltonian of the atomic part and the part of the atom-photon interaction are respectively

        whereg0is the coeffcient of the atom-photon coupling strength.

        In order to properly represent the elastic collision between the atoms,we only consider the two-body interaction with theδpotential and introduce the wave functions of the macroscopic condensate states Ψl(r,t).According to the second quantization of Gross–Pitaevskii equation,the Hamiltonian of the atomic part in Eq.(3)could be obtained that

        wherel=1,2 refer to the different atomic components;mRis the atomic mass,Vl(r)is the coulomb potential of the atoms;Ψl(r)satisfy the commutation relation of the boson field operatorandq1?2=4πρ1?2/mRdescribe the interaction between the intraspecies and interspeciess-wave scattering lengths of the atoms,and thes-wave scattering lengths could be tuned via the Feshbach resonance technique in the experiments.

        Based on the two-mode approximation and Ψl(r)=blφl,where two boson annihilation operatorsb1andb2respectively represent two atomic modes and they satisfy the commutationof the atom-photon interaction and the atomic part reduce to the following

        ω12being the atomic transition frequency between the frequency of the ground stateω1and the frequency of the excited statebeing the total atom number;the intraspecies and interspecies potential energies are respectively

        and

        Substituting Eqs.(2)–(8)into the total Hamiltonian(1), finally the system’s Hamiltonian takes the form

        For simplicity,we introduce the Schwinger angular momentum operators

        From Eq.(10),we can obtain thatOn the basis ofandwe get

        Substituting Eq.(11)into Eq.(9)and using the boson commutation relation,the Hamiltonian(9)is rewritten as

        where de fining the atom-photon interaction strengthg=being the atomic average interaction strength,ωa=(ω2?ω1)+(1/2)(N?1)(V22?V11)being the effective atomic frequency.The prefactorand 1/Ngive a finite free energy per atom in the thermodynamical limit(N→∞).Meanwhile,the constant terms related to the particle numbers have been ignored in Hamiltonian(12).For the atomic interaction strengthqis very weak,it was often overlooked.In the absence of the atomic interaction,the system Hamiltonian(12)reduces to the standard single-mode Dicke Hamiltonian.Hamiltonian(12)is to be used to describe the atomphoton collective nonlinear interaction and the atom-atom interaction.In the present paper,we mainly discuss the influence of the atom-atom interaction on the ground state properties of the generalized DM.In whole paper,we give the examples of the atom-atom repulsive interaction,i.e.,q>0.

        3 Spin Coherent-State Variational Method and Ground State Energy

        The Dicke Hamiltonian forNidentical two-level atoms interacting with a single mode of the electromagnetic field is written by[12,38]

        with ? =1,whereωais the frequency of the two-level atoms,ωis the frequency of the cavity- field mode,andgis the atom- field coupling strength.The boson operatorsa,a?are the annihilation and creation operators for the cavity field,and the pseudospinJi(i=z,±)is the collective atomic operators,which satisfy the angular momentum commutation relations([J±,Jz]= ?J±,[J+,J?]=2Jz)with the spin lengthj=N/2.As a classic problem in quantum optics,DM continually provides a fascinating avenue of research in a variety of contexts and is seen as a striking example for the macroscopic many-particle quantum state,which can be solved rigorously.The QPT from the normal phase to the superradiant phase occurs at the critical coupling strengthand the system enters the superradiant phase[12]forg>gc.

        Under the optical coherent state|α〉,we make the average of the DM’s Hamiltonian(13)

        whereαis the complex eigenvalue of photon annihilation operatora,i.e.,α=γeiηand satisfiesa|α〉=α|α〉.

        The average HamiltonianHsp(γ)possesses two macroscopic eigenstate,i.e.,the SCS|±n〉of south and north pole gauge.The SCS,which correspond to the normal and inverted pseudospin states in the dynamics of the DM,can be generated from the extreme Dicke states|j,±j〉|(Jz|j,±j〉= ±j|j,±j〉)with the SCS transformation|±n〉=R(n)|j,±j〉.[25?26]And the unitary operator is explicitly given by

        In fact,the SCS of the north and south pole gauges are the eigenstates of the spin projection operator J ·n|±n〉=±j|± n〉,where n=(sinθcosφ,sinθsinφ,cosθ)is the unit vector with the directional anglesθandφ.And the spin operators satisfy the minimum uncertainty relation(ΔJ+ΔJ?= 〈Jz〉/2)and therefore the SCSs|± n〉are called the macroscopic quantum states,which are orthogonal.Using the unitary transformationsR(n)for the spin operatorsJz,J+,J?

        Through a series of complicated and tedious calculation,we finally get the following spin Hamiltonian

        where

        In order to obtain the diagonalized spin Hamiltonian,it needs to satisfy the conditionsB(α,θ,φ)=C(α,θ,φ)=0,i.e.,

        In principle,the angle parametersθ,φcan be determined based on the above conditions Eq.(17).Meanwhile,we get the following relations of the parametersθandA

        Finally,the ground state energy functional of one variable is obtained:

        By the usual extremum condition of the energy function for the first-order derivative equal to zero,the macroscopic many-particle quantum state solutions are found:

        From Eq.(18),we find it possesses two solutions.One solution is the parameterγ=0,corresponding to a zerophoton-number solution and giving rise to the normal phase(NP)only if the second-order derivative is positive,namely,?E?(γ=0)/?γ>0.The other solution satisfies the condition

        and we obtain the average photon number

        If the second-order derivative in the solutionγ/=0 is positive,we define the system into the superradiant phase(SP).In the critical phase transition pointthe Dicke system undergoes a QPT from the NP to the SP,which has a wide range of research.[2?4,6,11?14,18?19,24]

        The ground-state energy of the DM system is

        The atomic population difference is proportional to the atom- field interaction strength in the SP region and satisfies the following relation

        The mean photon number distribution meets the following nonlinear relationship wheng>gc

        Itisworth whileto emphasizethattheSCS method is completely consistent to the Holstein–Primakofftransformation[3]in deal with the ground state properties of the standard DM and is valid for arbitrary atom numberN,which is superior to the Holstein–Primakoff transformation under the condition of the thermodynamic limit.

        4 Self-Consistent Field Theory for Extended DM with Atomic Interaction

        In some physical theories,mean field theory also can be seen as the self-consistent field theory,[27]which can be used to research the behavior of the large and complex stochastic models in a simple manner.Both the stronginteraction[34]and the weak-interaction[29]are compatible with the self-consistent field theory.The self-consistent field theory has been applied in the atoms,[30]the condensed matter,[31]the Lorentz gas[32]and so on.A series of literature have studied the exact-energy self-consistent field,[28]the self-consistent- field perturbation theory for the Schr?dinger equation,[39]the self-consistent mean- field theory,[35]the self-consistent mean- field theory of asymmetric first-order structural phase transition,[33]the quantum quench in interacting field theory,[40]polariton condensation with nonlinear photons described by the generalized Dicke Hamiltonian on the mean- field level.[41]

        In this article,we begin the following discussion based on the mean field approximation and the self-consistent field theory to solve the extended DM containing the atom-atom interaction.

        For the atom-atom interaction(q/N)by the means of the self-consistent mean field theory,[27]we obtain

        and substitute Eq.(20)into this item

        Substituting Eq.(22)forg≤gcinto Hamiltonian(12),it turns into

        It is to be highlighted that Hamiltonian(23)only satisfies the case of the normal phase.And the corresponding scaled ground state energy

        Substituting Eq.(22)forg>gcagain into Hamiltonian(12),it turns into

        where

        which contained the atomic interaction part.

        For Hamiltonian(25),the atomic population difference has such form

        and the coresponding atom-atom interaction is

        Once again,we substitute Eq.(27)into Hamiltonian(12),it turns into

        where the effective atom frequency

        and at this time the coresponding atom-atom interaction is

        Hamiltonian(12)repeats the above steps(26),(27),and(29),(30)we obtain the third order case

        where Repeating the above iteration until thek-th grade and(k?1)-th grade approximation have almost no influence on to the system’s total energy and meet the permissible error of the self-consistent field theory.Finally we obtain then-th atomic effective frequency and the coresponding atom-atom interaction are respectively

        And the coresponding total Hamiltonian

        Whenn→∞,Hamiltonian(31)returns to

        When the atom-atom interaction is not considered,i.e.,q=0,Hamiltonian(32)returns to the standard Dicke hamiltonian(13). Ifnchanges into in finity,the selfconsistent method has quite high accuracy and there is almost no error.In fact,there is so little difference betweenω2andω1or betweenω3andω2.From Fig.1,we may more clearly see this small differences.In the whole paper,the unite vector isωaand we chooseωa=1 MHz.

        Fig.1 (Color online)The ratio of(a)ω2/ω1and(b)ω3/ω2as the function of the atom-atom interaction q.The plotted collective coupling strength g/ωaare respectively 1.2(the red solid line),1.5(the green solid line),1.8(the violet solid line).The frequency of the light field is ω = ωa.

        5 Ground State Properties for Extended DM

        Based on the above SCS method and Hamiltonian(32),the ground state energy functional

        We also obtain that the extended DM goes through a quantum phase transition with the phase transition point

        We also calculate the three corresponding physical quantity:the mean photon number,the atomic population imbalance,and the quasi-ground-state energy.

        The mean photon number

        The atomic population imbalance

        The quasi-ground-state energy

        Fig.2 (Color online)Variations of the average photon number npq(a)(the solid line),the atomic population imbalance Δnaq(b)(shte dashed line),and the average energy εq(c)(the dotted line)with respect to the atom- field coupling constant g/ωafor the given parameter q/ωa=0.00(the black line),0.05(the red line),0.10(the green line).

        Figure 2 shows the influence of the atom-atom interaction parameterq/ωaon the mean photon number(a),the atomic population imbalance(b),and the average groundstate energy(c).The average ground-state energy are continuous and slippy at the critical phase transition pointgcq,which shifts toward the lowergdirection with the increasing of the atom-atom interaction.In NP,the mean photon number and the atomic population imbalance have not been excited and the average energy is stable.On the opposite of NP,in the SP area,the excited photon or atom number are non-zero and increases as the collective coupling strength increases.At the same time,the average energy become low,but is continuous with the case of the NP zero.The three physical quantities are more and more close to the each other with the increasing of the collective coupling strength in the case of the atom-atom interactionq/ωa=0.00,0.05,0.10.The existence of the atom-atom interaction makes the phase transition point move left.Especially whenq/ωa=0.10,there is a big movement.

        Fig.3 (Color online)Variations of the average photon number npq(a)(the solid line),the atomic population imbalance Δnaq(b)(the dashed line)and the average energy εq(c)(the dotted line)with respect to the atomatom interaction q/ωafor the given atom- filed coupling strength g/ωa=0.8(the black line),1.2(the red line),1.5(the green line).

        Figure 3 displays variations of the average photon numbernpq(a),the atomic population imbalance Δnaq(b),and the average energyεq(c)with respect toq/ωafor the giveng/ωa=0.8,1.2,1.5.The average photon number and the atomic population imbalance have not been excited,which are respectively a horizontal line,meanwhile the average energy increases obviously as the increase of the atom-atom interactionq/ωain the case ofg/ωa=0.8.With the increase ofg/ωa,there exists the excited photon or atom number and the average energy decreases.But the excited particle number almost has no change and the average energy is the lowest and almost keeps a straight line wheng/ωa=1.5.

        Fig.4 (Color online)Phase diagram in g-q space.The NP with γ=0 belongs to the normal phase.The SP with γ>0 is the right region of the boundary line gcq.The color index indicates the photon number γ2.

        In Fig.4 we plot the mean photon numberγ2as a function of the collective atom-photon coupling strengthgand the atom-atom interaction strengthq.The green region(γ=0)belongs to the NP and the color region(γ>0)is the SP.The critical line of the two regions aregcq,which shifts toward the lowergdirection whenq/=0 and the more moving to the left is seen when theqincreases from 0 to 0.10.

        In order to compared to the effect of the atom-atom interaction strengthqand the collective atom-photon coupling strengthgon the average ground state energy,in the following we introduce the difference in the SP between the average ground state energy and the case ofq=0,i.e.,Δε=εq?ε0.At the same time,the relative difference Δε/εhas been introduced.The conclusion has been plotted in Fig.5.For the given collective atom-photon coupling strengthg,the difference of Δεor Δε/εincreases or decreases with the increased atom-atom interaction.While the difference is more obvious wheng/ωa=1.2 than the case ofg/ωa=1.5 org/ωa=1.8.

        Fig.5 (Color online)(a)Δε and(b)Δε/ε0as the function of the atom-atom interaction strength q/ωafor the given collective atom- filed couping strength g/ωa=1.2(the red line),1.5(the green line),1.8(the violet line).

        We give the results of Δεand Δε/ε.

        6 The First-Order Superradiant Phase Transitions

        Based on the average ground-state energy Eq.(34),which is the function of the atom- field coupling constantgand the atom-atom interaction strengthq,the firstorder and second-order partial derivatives of the average ground-state energy are given

        Based on Eqs.(35),(36)Fig.6 and Fig.7 give the first-order and second-order derivatives in different system’s parameters.In the absence of the atom-atom interaction,i.e.,q=0,the first-order derivative is continuous in the phase boundary of the NP and the SP,but the second-order derivative is discontinuous.So we come to the conclusion that the standard DM exists a second-order QPT from the NP to the SP in the critical phase transition pointgc=1.While the atom-atom interaction is existent,the extented DM belongs to the first-order quantum phase transition,for the first-order and second-order derivative are both discontinuous in the critical phase transition pointgcq,which shifts to the left.

        Figure 7 displays the three-dimensional curves about the first-order derivative?εq/?gand the second-order derivative?2εq/?g2for the parametersg/ωaandq/ωa.They are discontinuous at the every critical phase transition point,which shifts to the left with the increasingq.They imply that the system undergoes a first-order QPT from the NP to the SP and the exclusive atom-atom interaction makes the phase transition point shift toward the lower atom-photon collective coupling strength.

        7 Conclusion

        In summary,an interesting prediction of the extended DM is that it undergoes a first-order QPT between the NP and the SP.In order to detect this first-order transition,we plotted the mean photon number,the scaled mean atom population and the average ground-state energy for different atom-atom interaction and discovered the QPT point shifts to left for the increasing atom-atom interaction.By the discontinuous first-order and second-order derivative,we come to the conclusion that the atom-atom interaction induces a first-order phase transition,which is different from the second-order QPT of the standard DM.We believe the atom-atom interaction can also have a deep influence on the physical properties such as the entanglement and the geometric phase in quantum information process.

        Fig.6 The first-order derivative of the average groundstate energy ?εq/?g(a)and the second-order derivative ?2εq/?g2(b)as the function of the collective coupling strength g/ωafor the given atom-atom interaction q/ωa=0.00(the black line),0.05(the red line),0.10(the green line)with ω/ωa=1.

        Fig.7 The first-order derivative of the average ground-state energy ?εq/?g(a)and the second-order derivative?2εq/?g2(b)as the function of the collective coupling strength g/ωaand the atom-atom interaction q/ωa(q/ωa ∈ [0.06,0.10])with ω/ωa=1.

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