This study aims to construct a theoretical formulation of a nonequilibrium process for a system of Bose--Einstein condensate associated with a spontaneous symmetry breakdown. For this, Thermo Field Dynamics is used. We then describe the most general forms of a 4x4 transformation and an unperturbed Hamiltonian. After calculating the $4\times 4$ self-energy and identifying its on-shell, we impose the renormalization condition in which the entire on-shell self-energy should vanish. This condition provides a sufficient number of independent equations to determine all of the parameters in an unperturbed Hamiltonian, among which the quantum transport equations for normal and anomalous number distributions are included.
This study aims to construct a theoretical formulation of a nonequilibrium process for a system of Bose--Einstein condensate associated with a spontaneous symmetry breakdown. For this, Thermo Field Dynamics is used. We then describe the most general forms of a 4x4 transformation and an unperturbed Hamiltonian. After calculating the 4×4 self-energy and identifying its on-shell, we impose the renormalization condition in which the entire on-shell self-energy should vanish. This condition provides a sufficient number of independent equations to determine all of the parameters in an unperturbed Hamiltonian, among which the quantum transport equations for normal and anomalous number distributions are included.
This study aims to construct a theoretical formulation of a nonequilibrium process for a system of Bose–Einstein condensate associated with a spontaneous symmetry breakdown. For this, Thermo Field Dynamics is used. We then describe the most general forms of a 4 × 4-matrix transformation and an unperturbed Hamiltonian. After calculating the 4 × 4-matrix self-energy and identifying its on-shell, we impose the renormalization condition in which the entire on-shell self-energy should vanish. This condition provides a sufficient number of independent equations to determine all of the parameters in an unperturbed Hamiltonian, among which the quantum transport equations for normal and anomalous number distributions are included.
In recent experiments of Bose-Einstein condensation of a magnetically trapped dilute alkaline atomic gas, the nonequilibrium process of thermalization into the condensed state has been observed in a reasonably long time scale. This presents a new challenge to develop a theory to treat strongly space-time dependent nonequilibrium processes. In this paper, we present a nonequilibrium formulation of Bose-Einstein condensed states in the field theoretical framework of thermo-field dynamics. By use of an effective Hamiltonian method, a quasi-particle field equation is derived. This equation contains information regarding the renormalized energy, decay width and time-variation of particle distributions. It is shown that, in the present formulation, the strong space-time dependence can be treated, even including quantum corrections, as the use of the quasi-particle field equation enables us to factorize double-time functions of the self-energy.
We study the thermal processes for the system of cold neutral atomic gas in the framework of nonequilibrium Thermo Field Dynamics (TFD) which is a real-time canonical formalism of quantum field theory for thermal situations [1]. The system is suitable for testing quantum many-body theories in nonequilibrium situations because temporal changes in thermal processes are so slow that various nonequilibrium phenomena can be observed experimentally. In nonequilibrium TFD, the quantum transport equation, which is the equation for a time-dependent number distribution introduced as an unknown parameter, is derived from the self-consistent renormalization condition on the self-energy [2]. The correction on the excitation energy is important both physically and in the renormalization of quantum field theory. Recently we have proposed the new self-consistent renormalization method in nonequilibrium TFD, in which the on-shell self-energy in time-dependent case is introduced as a generalization of the ordinary on-shell self-energy in stationary case and the renormalization conditions on it yields the quantum transport equation and the diagonal correction of the quasiparticle energy in a unified manner [2]. In this work, the renormalization condition is extended to the imaginary and off-diagonal parts of the self-energy. In our previous work [3], we applied nonequilibrium TFD to the one dimensional system of confined cold neutral atomic Bose gas. There the nonequilibrium situation was set up by a sudden displacement of the confining potential and a sudden switch-on of the interparticle interaction. We investigated the thermal process for the system by solving the quantum transport equation, but neglecting the correction of the quasiparticle energy. Then it was found that in some particular parameter region it gives rise to an unphysical result, namely the negative number distribution. Here we take account of the correction of the quasiparticle energy and solve the quantum transport equation again. The correction affects drastically the thermal relaxation process and resolves the difficulty in some parameter region, as will be shown.
The non-Markoffian transport equations for the systems of cold Bose atoms confined by a external potential both without and with a Bose-Einstein condensate are derived in the framework of nonequilibrium thermal filed theory (Thermo Field Dynamics). Our key elements are an explicit particle representation and a self-consistent renormalization condition which are essential in thermal field theory. The non-Markoffian transport equation for the non-condensed system, derived at the two-loop level, is reduced in the Markoffian limit to the ordinary quantum Boltzmann equation derived in the other methods. For the condensed system, we derive a new transport equation with an additional collision term which becomes important in the Landau instability.
Based on Bogoliubov's truncated Hamiltonian H B for a weakly interacting Bose system, and adding a U(1) symmetry breaking term V 1/2 (λ a 0 +λ * a 0 + ) to H B , we show by using the coherent state theory and the mean-field approximation rather than the c-number approximations, that the Bose–Einstein condensation(BEC) occurs if and only if the U(1) symmetry of the system is spontaneously broken. The real ground state energy and the justification of the Bogoliubov c-number substitution are given by solving the Schrödinger eigenvalue equation and using the self-consistent condition.
Bose-Einstein condensates are bosonic many-body systems in which the quantum mechanical ground state is macroscopically occupied. If the interparticle interaction between the single bosons is attractive, this ground state is metastable and separated from the collapse by a barrier. A sufficient thermal excitation of the condensate can enable the crossing of this barrier and induce its collapse. In this thesis, the corresponding decay mechanism of the thermally induced coherent collapse of Bose-Einstein condensates with additional long-range interaction is investigated for the first time. For the description of the condensate’s dynamics a variational approach to the quantum wave function is used, which allows for the precise determination of the system’s transition state that governs the reaction dynamics. In order to quantitatively calculate the decay rate and lifetime of the condensate, respectively, a novel transition state theory for quantum wave packets is developed. This is based on a variational approach as well as normal form expansions of the dynamical equations and the energy functional in the vicinity of the transition state. The dynamical equations obtained from the variational approach induce a symplectic structure onto the space of variational parameters. Furthermore, the normal form expansions serve as a tool to locally construct canonical coordinates on this symplectic manifold. For this purpose, the dynamical equations as well as the energy functional are expanded and diagonalized. The eigenvectors of the linearized equations of motion thereby define a symplectic basis of the system. Afterwards, the transformations of the higher-order terms are carried out in two steps via nonlinear near-identity transformations: In the first step, the nonresonant terms of the expansions are eliminated and in the second step the remaining resonant terms are transformed in such a way that they fulfill canonical equations. The combination of these methods finally allows for the application of the well-established classical transition state theory. The procedure is valid for a wide variety of trial wave functions, for arbitrary dimensions of the variational space, in arbitrary order of the expansions, and it is independent of the precise form of the Hamilton operator. In addition, a procedure to handle bifurcations in the transition state is developed using a uniform rate formula in connection with an appropriate normal form of the potential energy surface. In contrast to the usual treatment which breaks down at the point of the bifurcation, the new method allows to cross the bifurcation smoothly, because it is valid on both sides of the bifurcation as well as arbitrarily close to it. At the same time, one can calculate the flux over the whole configuration of saddles which emerge in the bifurcation. The applicability of the newly developed transition state theory for wave packets is demonstrated for a cubic potential well. The thermal decay rates of a point particle and a frozen Gaussian wave packet, respectively, are calculated within the classical and quantum normal form approaches as well as the variational one. It is shown that the variational approach is capable to perfectly reproduce both the classical and quantum normal form results of the point particle in different limits. In the limit of a narrow trial wave function it agrees perfectly with the results using the classical normal form. The results with a broader trial wave function go even beyond the classical approach, i.e. they coincide with those of the quantum normal form. In the field of Bose-Einstein condensates with long-range interaction the application of transition state theory for quantum wave packets is extended to the field of nonlinear Schrödinger systems. For condensates with attractive 1/r-interaction, the thermal decay rates are calculated for different numbers of coupled Gaussian wave functions as well as different normal form orders. Significant corrections of the decay rate are obtained with increasing order of the normal forms. In the low-temperature regime convergence is observed in eighth order of the expansions. Finally, the thermally induced coherent collapse of dipolar condensates is investigated. These exhibit the feature of a biconcave ground state density distribution for certain values of the physical parameters. It is shown that such condensates reveal the astonishing effect of a symmetry-breaking collapse dynamics. This effect is directly related to the occurrence of the structured ground state, and it depends on the geometry of the external trapping potential. In case of a “conventional” density distribution, the collapse possesses an s-wave symmetry, while it has a d-wave symmetry in case of a blood-cell shaped ground state. The thermally induced coherent collapse plays a major role close to the stability threshold where the energy barrier is small and the decay rates are high. In case of Cr atoms, dipolar condensate have been first realized with, the region of interest is on the order of a Bohr radius above the critical scattering length. There, the lifetime of the condensate can be reduced to a millisecond. For the elements Dy and Er which have also been condensed in the laboratory, the effects become even stronger, i.e. the parameter region of importance becomes larger, the energy barriers become smaller, and the decay rates are higher.