818 research outputs found
Out of Equilibrium Dynamics of Supersymmetry at High Energy Density
We investigate the out of equilibrium dynamics of global chiral supersymmetry
at finite energy density. We concentrate on two specific models. The first is
the massive Wess-Zumino model which we study in a selfconsistent one-loop
approximation. We find that for energy densities above a certain threshold, the
fields are driven dynamically to a point in field space at which the fermionic
component of the superfield is massless. The state, however is found to be
unstable, indicating a breakdown of the one-loop approximation. To investigate
further, we consider an O(N) massive chiral model which is solved exactly in
the large limit. For sufficiently high energy densities, we find that for
late times the fields reach a nonperturbative minimum of the effective
potential degenerate with the perturbative minimum. This minimum is a true
attractor for O(N) invariant states at high energy densities, and this provides
a mechanism for determining which of the otherwise degenerate vacua is chosen
by the dynamics. The final state for large energy density is a cloud of
massless particles (both bosons and fermions) around this new nonperturbative
supersymmetric minimum. By introducing boson masses which softly break the
supersymmetry, we demonstrate a see-saw mechanism for generating small fermion
masses. We discuss some of the cosmological implications of our results.Comment: 31 pages, 15 figure
Nonequilibrium dynamics in scalar hybrid models
We study by numerical simulations the transition from the metastable "false
vacuum" to the broken symmetry phase in the preheating stage after cosmic
inflation in a scalar hybrid model. We take quantum fluctuations and their back
reaction into account by applying a one-loop bubble-resummation.Comment: 5 pages, 4 figures, contribution to the conference Strong and
Electroweak Matter (SEWM2004), Helsinki, Finland, 16-19 June 200
Nonequilibrium evolution and symmetry structure of the large-N model at finite temperature
We consider the large-N theory with spontaneously broken symmetry at
finite temperature. We study, in the large-N limit, quantum states which are
characterized by a time dependent, spatially homogenous expectation value of
one of the field components, , and by quantum fluctuations of the
other components, that evolve in the background of the classical field.
Investigating such systems out of equilibrium has recently been shown to
display several interesting features. We extend here this type of
investigations to finite temperature systems. Essentially the novel features
observed at T=0 carry over to finite temperature. This is not unexpected, as
the main mechanisms that determine the late-time behavior remain the same. We
extend two empirical - presumably exact - relations for the late-time behavior
to finite temperature and use them to define the boundaries between the region
of different asymptotic regimes. This results in a phase diagram with the
temperature and the initial value of the classical field as parameters, the
phases being characterized by spontaneous symmetry breaking resp. symmetry
restoration. The time evolution is computed numerically and agrees very well
with the expectations.Comment: 21 pages, 13 Figures, LaTeX, some typos correcte
Scalar O(N) Model at Finite Temperature -- 2PI Effective Potential in Different Approximations
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
next-to-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.Comment: LaTeX, 5 pages. Contribution to the Proceedings of 6th Conference on
Strong and Electroweak Matter 2004 (SEWM04), Helsinki, Finland, 16-19 Jun
200
One-loop corrections to the Nielsen-Olesen vortex: collective oscillations
We connect the translation modes of the instanton in the two-dimensional
Abelian Higgs model with local translations of the vortex of the related model
in (3+1) dimensions, the Nielsen-Olesen vortex. In this context these modes
describe collective oscillations of the string. We construct the wave function
of this mode and we derive, via a virial theorem, an effective action for these
oscillations, which is consistent with the action constructed by Nielsen and
Olesen using general arguments. We discuss some aspects of renormalization,
based on a recent computation of one loop corrections to string tension of the
vortex.Comment: 18 pages, 1 figur
One-loop corrections to the metastable vacuum decay
We evaluate the one-loop prefactor in the false vacuum decay rate in a theory
of a self interacting scalar field in 3+1 dimensions. We use a numerical
method, established some time ago, which is based on a well-known theorem on
functional determinants. The proper handling of zero modes and of
renormalization is discussed. The numerical results in particular show that
quantum corrections become smaller away from the thin-wall case. In the
thin-wall limit the numerical results are found to join into those obtained by
a gradient expansion.Comment: 31 pages, 7 figure
Self-consistent bounces in two dimensions
We compute bounce solutions describing false vacuum decay in a Phi**4 model
in two dimensions in the Hartree approximation, thus going beyond the usual
one-loop corrections to the decay rate. We use zero energy mode functions of
the fluctuation operator for the numerical computation of the functional
determinant and the Green's function. We thus avoid the necessity of
discretizing the spectrum, as it is necessary when one uses numerical
techniques based on eigenfunctions. Regularization is performed in analogy of
standard perturbation theory; the renormalization of the Hartree approximation
is based on the two-particle point-irreducible (2PPI) scheme. The iteration
towards the self-consistent solution is found to converge for some range of the
parameters. Within this range we find the corrections to the leading one-loop
approximation to be relatively small, not exceeding one order of magnitude in
the total transition rate.Comment: 30 pages, 12 figure
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Translation of the German original
Nonequilibrium dynamics: a renormalized computation scheme
We present a regularized and renormalized version of the one-loop nonlinear
relaxation equations that determine the non-equilibrium time evolution of a
classical (constant) field coupled to its quantum fluctuations. We obtain a
computational method in which the evaluation of divergent fluctuation integrals
and the evaluation of the exact finite parts are cleanly separated so as to
allow for a wide freedom in the choice of regularization and renormalization
schemes. We use dimensional regularization here. Within the same formalism we
analyze also the regularization and renormalization of the energy-momentum
tensor. The energy density serves to monitor the reliability of our numerical
computation. The method is applied to the simple case of a scalar phi^4 theory;
the results are similar to the ones found previously by other groups.Comment: 15 pages, 9 postscript figures, revtex; version published in Phys.
Rev, with minor corrections; improves the first version of 1996 by including
the discussion of energy momentum tenso
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