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Asia Pacific Physics Conference (APPC)

Description of Photon Field in Dynamics Simulation of Bound States Based on Quantum Field Theory

Masato Senami, Soujiro Takada, Akitomo Tachibana

Published Mar 19, 2014• 0 citations
Publisher

Abstract

Quantum field theory (QFT) is considered to be most correct for the description of quantum systems. For the reason, we study local physical quantities defined in QFT, such as local polarizability, local conductivity, local spin torque [1–4]. In these works, for quantum states, we used wave packets derived by first principles calculation based on quantum mechanics. To treat states and physical quantities consistently, quantum systems should be treated in QFT. Hence, we are developing a first principles calculation program package based on quantum electrodynamics (QED). We name this program package QEDynamics [5]. The purpose of this program package is to study time evolution of quantum systems consisting of molecules or condensed matter. This challenge has two points of difficulties. One is the non-perturbativity, and the other is the time evolution of quantum systems. The formulation of QFT has been developed in a perturbative method. Hence perturbative calculations are widely used. For non-perturbative systems i.e. bound states, many methods are explored, lattice quantum chromodynamics, NRQED [6], Bethe-Salpeter method, and so on. All methods have various advantages and disadvantages, and hence we should be careful with the treatment of non-perturbative systems. Moreover, in most perturbative calculations, the existence of asymptotic states is assumed and the time integration from −∞ to∞ is performed for calculations, such as cross section. Thus the time evolution i.e. the study of nonequilibrium systems is restricted in specific cases. In literature, nonequilibrium systems are studied by Boltzmann equation, closed time path formalism [7], thermo field dynamics [8] and so on. We solve directly Heisenberg equations of field operators in QED in the present version of QEDynamics for the study of time evolution. In computational simulations, operators are difficult to handle. In our program, the evolution of the operators is calculated as the transition between modes prepared by the method of first principles computations of quantum structures. This mode expansion is based on the method used in Furry picture. This choice of the expansion functions of field operator has an advantage representing bound states. In this article, we show the present status of our program. In particular, the computation method of the evolution of photon fields are explained. Hence most other detail information cannot be mentioned in this article. For the information, please see Ref. [5].

DOI
10.7566/jpscp.1.016014

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Quantum field theory (QFT) is considered to be most correct for the description of quantum systems. For the reason, we study local physical quantities defined in QFT, such as local polarizability, local conductivity, local spin torque [1–4]. In these works, for quantum states, we used wave packets derived by first principles calculation based on quantum mechanics. To treat states and physical quantities consistently, quantum systems should be treated in QFT. Hence, we are developing a first principles calculation program package based on quantum electrodynamics (QED). We name this program package QEDynamics [5]. The purpose of this program package is to study time evolution of quantum systems consisting of molecules or condensed matter. This challenge has two points of difficulties. One is the non-perturbativity, and the other is the time evolution of quantum systems. The formulation of QFT has been developed in a perturbative method. Hence perturbative calculations are widely used. For non-perturbative systems i.e. bound states, many methods are explored, lattice quantum chromodynamics, NRQED [6], Bethe-Salpeter method, and so on. All methods have various advantages and disadvantages, and hence we should be careful with the treatment of non-perturbative systems. Moreover, in most perturbative calculations, the existence of asymptotic states is assumed and the time integration from −∞ to∞ is performed for calculations, such as cross section. Thus the time evolution i.e. the study of nonequilibrium systems is restricted in specific cases. In literature, nonequilibrium systems are studied by Boltzmann equation, closed time path formalism [7], thermo field dynamics [8] and so on. We solve directly Heisenberg equations of field operators in QED in the present version of QEDynamics for the study of time evolution. In computational simulations, operators are difficult to handle. In our program, the evolution of the operators is calculated as the transition between modes prepared by the method of first principles computations of quantum structures. This mode expansion is based on the method used in Furry picture. This choice of the expansion functions of field operator has an advantage representing bound states. In this article, we show the present status of our program. In particular, the computation method of the evolution of photon fields are explained. Hence most other detail information cannot be mentioned in this article. For the information, please see Ref. [5].
One of the major goals in the establishment of a quantum field theory for nonequilibrium systems is to study dynamical problems, following the evolution of the expectation value of a physical variable with respect to an in state. This is different from a scattering problem characterized by the transition amplitude between the in and out states, as is treated in every textbook on quantum field theory. This problem is usually coupled with how one could identify a relevant sector of the theory as the system (light fields vs. heavy fields, slow modes vs. fast modes, long wavelength modes vs. short ones, etc.) and determine the effect of its other sectors as the environment on this system, as we have discussed in the last chapter. Given a classical nonequilibrium system, described, for example, by a Langevin equation, there are essentially three possible strategies to follow. One may attempt to solve it, usually numerically. In the quantum field case, this gets difficult beyond the linear case. Second, one may try to transform it into an equation for the evolution of a probability distribution function in the system's configuration space. In the quantum field case the relevant object is the reduced density matrix, and the relevant equation is the Liouville-von Neumann equation. This is also infeasible beyond the linear case, unless under restrictive approximations (such as Gaussianity) which in fact reduce this approach to the third and coarsest.
Diagrammatical expansion of the quantum field theory with the finite time interval is discussed by evaluating the time evolution kernel. The coherent state representation is adopted which is the most convenient formalism for this purpose. It is applied to quantum electrodynamics (QED) to derive the Feynman rule for the kernel. The rule for the matrix element of any operator is also given. Our method can also be a systematic approach to the time dependent perturbation theory. As an example, a full order formula of the transition amplitude between the number states is given in terms of the connected Green's functions.
Diagrammatical expansion of the quantum field theory with the finite time interval is discussed by evaluating the time evolution kernel. The coherent state representation is adopted which is the most convenient formalism for this purpose. It is applied to quantum electrodynamics (QED) to derive the Feynman rule for the kernel. The rule for the matrix element of any operator is also given. Our method can also be a systematic approach to the time dependent perturbation theory. As an example, a full order formula of the transition amplitude between the number states is given in terms of the connected Green's functions.
Abstract We discuss how we formulate time evolution of physical quantities in the framework of the Rigged quantum electrodynamics (QED). The Rigged QED is a theory which has been proposed to treat dynamics of electrons, photons, and atomic nuclei in atomic and molecular systems in a quantum field theoretic way. To solve the dynamics in the Rigged QED, we need different techniques from those developed for the conventional QED. As a first step toward this issue, we propose a procedure to expand the Dirac field operator, which represents electrons, by the electron annihilation/creation operators and solutions of the Dirac equation for electrons in nuclear potential. Similarly, the Schrödinger field operators, which represent atomic nuclei, are expanded by nucleus annihilation/creation operators. Then, we derive time evolution equations for these annihilation and creation operators and discuss how time evolution of the operators for physical quantities can be calculated. In the end, we propose a method to approximate the evolution equations of the operators by the evolution equations for the density matrices of electrons and atomic nuclei. Under this approximation, we carry out numerical simulation of the time evolution of electron charge density of a hydrogen atom. © 2012 Wiley Periodicals, Inc.
In this work we shall study the interaction of matter and light. In so doing we shall rely heavily on the description of such processes provided by quantum mechanics. This appears on a number of levels: firstly, a quantum description of matter is indispensable if one wants to understand on the microscopic scale the different kinds of interaction processes that can occur. Secondly, a quantum description of light often turns out to be useful, sometimes necessary, to better understand these processes. We shall study phenomena such as spontaneous emission, which can only be properly treated by a theory taking into account the quantum nature of both light and matter. In the following chapters we shall address, amongst others, the following question: ‘given an atom prepared at a given time in a particular state and subjected from this time onwards to electromagnetic radiation, what is the state of the atom and radiation at any later moment in time?’ In order to be able to answer this question it will be necessary for us to know how to calculate the evolution of a quantum system in a small number of typical situations. These methods we shall demonstrate in the first chapter. The evolution of the coupled atom–light system depends on the temporal dependence of the applied light field, which could, for example, be applied from a given moment and thereafter remain unchanged in intensity, or, perhaps, be appreciable only for a finite period of time (pulsed excitation).
We develop a systematic method of operator perturbation theory in the Heisenberg picture, which is the formal analog of time-independent stationary-state perturbation theory in the Schr\"odinger picture. However, we use the eigenoperators and operator eigenfrequencies to calculate the time evolution of the dynamical variables of interest. The spectrum of the unperturbed Hamiltonian is assumed to be discrete. The method is especially well-suited for treating systems where the unperturbed Hamiltonian represents noninteracting fermions and/or bosons, and therefore, we illustrate the method using the exactly solvable model of Jaynes and Cummings: a single two-level atom interacting with a single quantized field mode. The time evolution of these operator solutions is shown to be unitary order by order in powers of the interaction strength. We find that the time evolution of exact operator solutions is well approximated for significantly longer times by the time evolution of this method's operator solutions than by the time evolution of the same operator solutions calculated using the Dyson expansion. We also demonstrate that time-dependent operator solutions are very convenient for computing quantities such as correlation functions.