We study the O(N ) linear sigma model with spontaneous symmetry breaking at finite temperature in the framework of the two-particle point-irreducible (2PPI) effective action. We go beyond the Hartree approximation by including the twoloop contribution, i.e., the sunset diagram. A phase transition of second order is found, whereas it is of first order in the one-loop Hartree approximation. Furthermore, we show the temperature-dependence of the variational mass parameters and comment on their relation to the physical sigma and pion masses. * talk given by S. Michalski.
We consider the out-of-equilibrium evolution of a classical condensate field and its quantum fluctuations for a scalar O(N) model with spontaneously broken symmetry. In contrast to previous studies we do not consider the large N limit, but the case of finite N , including N = 1, i.e., plain λφ 4 theory. The instabilities encountered in the one-loop approximation are prevented, as in the large-N limit, by back reaction of the fluctuations on themselves, or, equivalently, by including a resummation of bubble diagrams. For this resummation and its renormalization we use formulations developed recently based on the effective action formalism of Cornwall, Jackiw and Tomboulis. The formulation of renormalized equations for finite N derived here represents a useful tool for simulations with realistic models. Here we concentrate on the phase structure of such models. We observe the transition between the spontaneously broken and the symmetric phase at low and high energy densities, respectively. This shows that the typical structures expected in thermal equilibrium are encountered in nonequilibrium dynamics even at early times, i.e., before an efficient rescattering can lead to thermalization.
We study the O(N ) linear sigma model in 1+1 dimensions by using the 2PI formalism of Cornwall, Jackiw and Tomboulis in order to evaluate the effective potential at finite temperature. At next-to-leading order in a 1/N expansion one has to include the sums over "necklace"' and generalized "sunset" diagrams. We find that -in contrast to the Hartree approximation -there is no spontaneous symmetry breaking in this approximation, as to be expected for the exact theory. The effective potential becomes convex throughout for all parameter sets which include N = 4, 10, 100, couplings λ = 0.1, 0.5 and temperatures between 0.3 and 1 (in arbitrary units). The Green's functions obtained by solving the Schwinger-Dyson equations are enhanced in the infrared region. We also compare the effective potential as a function of the external field φ with those obtained in the 1PI and 2PPI expansions.
We calculate the two-particle irreducible (2PI) effective potential of the O(N ) linear sigma model in 1+1 dimensions. The approximations we use are the nextto-leading order of a 1/N expansion (for arbitrary N ) and a kind of "resummed loop approximation" for N = 1. We show that the effective potential of the 1/N expansion is convex for N = 4 and N = 10 whereas it is not for the "loop" expansion and the case N = 1 of the 1/N expansion.
We investigate the out-of-equilibrium evolution of a classical background field and its quantum fluctuations in the scalar O(N ) model with spontaneous symmetry breaking 1 . We consider the 2-loop 2PI effective action in the Hartree approximation, i.e. including bubble resummation but without non-local contributions to the Dyson-Schwinger equation. We concentrate on the (nonequilibrium) phase structure of the model and observe a first-order transition between a spontaneously broken and a symmetric phase at low and high energy densities, respectively. So typical structures expected in thermal equilibrium are encountered in nonequilibrium dynamics even at early times before thermalization.
The model
ApplicationsScalar models have a wide range of applications in quantum field theory. Normally they are parts of more complex models like e.g. the Standard Model or Grand Unified Theories but they often serve as toy models for a simplified description of complex phenomena such as inflationary cosmology or meson interactions in relativistic heavy ion collisions.
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