The dynamical scaling for the one-particle Green function up to O(1/m) is discussed on the basis of the same model and formulation as in I. A characteristic frequency ωq is studied, and the result is shown to be consistent with that obtained in I. The dynamic critical exponents ^z and λ are calculated up to O(1/m).
The classical 1/n expansion for critical phenomena is extended to a quantum system by introducing the Bose field with m(=n/2) independent components. The case just at the critical point is considered. It is shown that there is no quantum effect on r; up to 0(1/m). The energy spectrum E. of one-particle excitation is expressed as E.ocq•-c and t; is calcu-lated exactly up to 0 (1/m). The result turns out to be in accordance with the one ob-tained recently by Kondor and Szepfalusy. The dynamic scaling for the present model will be discussed in a subsequent paper.
We study the dynamic critical exponent from effective and microscopic theories. We employ a simple TDGL model, or model A in the classification of Hohenberg and Halperin, as an effective theory and the imaginary time formalism of the finite-temperature filed theory as a microscopic theory. Taking an O(N) scalar model as an example and carrying out the 1/N expansion up to the NLO in the 1PI and 2PI effective actions, we compare the low-energy and low-momentum behavior of the response function in the effective theory and of the retarded Green's function in the microscopic theory. At the NLO of the 1PI 1/N expansion the low-energy and low-momentum behavior of the two-point function is very much different in the microscopic and effective theories: in the field theory it is dominated by the propagating mode while in model A it is dominated by the diffusive mode. Also, in the microscopic theory the dynamic critical exponent, z, depends on whether the kinematics is relativistic or nonrelativistic. In contrast, at the NLO of the 2PI 1/N expansion the microscopic and effective theories are equivalent. They satisfy exactly the same Kadanoff-Baym equation. Also, whether the kinematics is relativistic or nonrelativistic in the microscopic theory becomes irrelevant. This implies that the diffusive mode with z = 2 + O(1/N) is dominant at low energies and momenta even in the microscopic theory at the NLO of the 2PI 1/N expansion, though we do not explicitly solve the Kadanoff-Baym equation. We also try to improve the calculation of the dynamic critical exponent of model A by incorporating the static 2PI NLO correlations. The obtained critical exponent is slightly smaller than the previous result and its N dependence is also milder than the previous one.
Progress of Theoretical Physics Vol. 52 No. 4 (1974) pp. 1135-1145 Quantum Effect, Critical Dynamics and One-Particle Excitation in 1/n Expansion. I Ryuzo Abe Progress of Theoretical Physics Vol. 52 No. 5 (1974) pp. 1463-1472 Quantum Effect, Critical Dynamics and One-Particle Excitation in 1/n Expansion. II Ryuzo Abe and Shinobu Hikami Progress of Theoretical Physics Vol. 53 No. 1 (1975) pp. 97-110 On the Critical Dynamics in Bose Systems and the Time-Dependent Ginzburg-Landau Model Masuo Suzuki Progress of Theoretical Physics Vol. 53 No. 2 (1975) pp. 591-593 Dynamic Critical Behavior of Bose Systems at Tλ Giko Igarashi Progress of Theoretical Physics Vol. 54 No. 1 (1975) pp. 289-290 Coherent Representation of Dynamical Renormalization Group in Bose Systems Fumihiko Tanaka Progress of Theoretical Physics Vol. 54 No. 6 (1975) pp. 1679-1692 Coherent Representation of Dynamical Renormalization Group in Bose Systems Fumihiko Tanaka
Critical exponents in the ${\mathit{CP}}^{\mathit{N}\mathrm{\ensuremath{-}}1}$ model, which describes localized-moment ferromagnets and antiferromagnets (N=2 in the Heisenberg model), are calculated from two-particle Green's functions to first order in 1/N. For d=2+\ensuremath{\varepsilon} the results agree with earlier renormalization group calculations. For d=3 the leading 1/N corrections turn out to be very large at N=2. For d=4-\ensuremath{\varepsilon} the 1/N corrections are small at any N and insufficient to describe correctly the magnetic phase transition. \textcopyright{} 1996 The American Physical Society.
An extended expression of the dynamic self-energy of one-particle Green function is obtained up to order 1/m in m-component Bose systems, by means of a complex unperturbed propagator. As applications of it, dynamic critical exponents of the TDGL model as well as of a Bose system are evaluated to order 1/m, for both short-range and long-range interactions. These confirm the previous results of the TDGL model and of the Bose system for short-range interactions. An effective interaction Veff(p, iωn) is obtained to order 1/m, which is useful for discussion on anomalies of transport coefficients near the λ-transition.
It is useful to compare the results obtained so far with other approaches to the critical exponents. One is a similar field-theoretic approach based on perturbation expansions of φ 4-theories. But instead of working in D = 4−ε dimensions and continuing the results to ε = 1 to obtain critical exponents in the physical dimension D = 3, perturbation expansions can be derived directly in three dimensions, and studied in the regime of small masses. Fundamentally, this approach is less satisfactory than the previous one since there is no small parameter analogous to ε which permits us to prove the existence of a scaling limit at least for small ε. Another disadvantage is that it is impossible to calculate the expansion coefficients analytically, except for one- and two loop-diagrams. In one respect the three-dimensional approach has, however, an advantage: the power series have long been available up to six loops for ω, η, and ν, and there exist recent results up to seven loops for the critical exponents η and ν. Although numerical expansions are not as esthetic as the exact expansions derived in this book, their increased order leads to a higher accuracy in the critical exponents, as we shall see below in Section 20.4. Another approach is based on high-temperature expansions for lattice models of the O(N)symmetric classical Heisenberg model with the energy of Eq. (1.52). The critical exponents will be derived from such expansions in Section 20.8. Finally we take advantage of the fact that the O(N)-symmetric classical Heisenberg model is exactly solvable in the limit of large N, where it reduces to the spherical model [recall the remark after Eq. (1.69)]. It is therefore possible to expand the φ 4-theory around this limit in powers of 1/N. The results will be compared with those from the perturbation expansions in