6,047 research outputs found
Quantum parametric resonance
The quantum mechanical equivalent of parametric resonance is studied. A simple model of a periodically kicked harmonic oscillator is introduced which can be solved exactly. Classically stable and unstable regions in parameter space are shown to correspond to Floquet operators with qualitatively different properties. Their eigenfunctions, which are calculated exactly, exhibit a transition: for parameter values with classically stable solutions the eigenstates are normalizable while they cannot be normalized for parameter values with classically unstable solutions. Similarly, the spectrum of quasi energies undergoes a specific transition. These observations remain valid qualitatively for arbitrary linear systems exhibiting classically parametric resonance such as the paradigm example of a frequency modulated pendulum described by Mathieu's equation
How parametric resonance mechanism follows quench mechanism in disoriented chiral condensate
We show how parametric resonance mechanism follows quench mechanism in the
classical linear sigma model. The parametric resonance amplifies long
wavelength modes of the pion for more than . The shifting from the
quench mechanism to the parametric resonance mechanism is described by a time
dependent quantity. After the quench mechanism is over, that quantity has an
oscillating part, which causes the parametric resonance. Since its frequency is
: pion mass), very long wavelength modes such as k = 40 MeV
of the pion are amplified by the parametric resonance.Comment: LaTeX, 10 page
Excitation of a Kaluza-Klein mode by parametric resonance
In this paper we investigate a parametric resonance phenomenon of a
Kaluza-Klein mode in a -dimensional generalized Kaluza-Klein theory. As the
origin of the parametric resonance we consider a small oscillation of a scale
of the compactification around a today's value of it. To make our arguments
definite and for simplicity we consider two classes of models of the
compactification: those by () and those by (, ). For these models we show that
parametric resonance can occur for the Kaluza-Klein mode. After that, we give
formulas of a creation rate and a number of created quanta of the Kaluza-Klein
mode due to the parametric resonance, taking into account the first and the
second resonance band. By using the formulas we calculate those quantities for
each model of the compactification. Finally we give conditions for the
parametric resonance to be efficient and discuss cosmological implications.Comment: 36 pages, Latex file, Accepted for publication in Physical Review
Parametric Resonance For Complex Fields
Recently, there have been studies of parametric resonance decay of
oscillating real homogeneous cosmological scalar fields, in both the
narrow-band and broad-band case, primarily within the context of inflaton decay
and (p)reheating. However, many realistic models of particle cosmology, such as
supersymmetric ones, inherently involve complex scalar fields. In the
oscillations of complex scalars, a relative phase between the oscillations in
the real and imaginary components may prevent the violations of adiabaticity
that have been argued to underly broad-band parametric resonance. In this
paper, we give a treatment of parametric resonance for the decay of homogeneous
complex scalar fields, analyzing properties of the resonance in the presence of
out of phase oscillations of the real and imaginary components. For
phase-invariant coupling of the driving parameter field to the decay field, and
Mathieu type resonance, we give an explicit mapping from the complex resonance
case to an equivalent real case with shifted resonance parameters. In addition,
we consider the consequences of the complex field case as they apply to
``instant preheating,'' the explosive decay of non-convex potentials, and
resonance in an expanding FRW universe. Applications of our considerations to
supersymmetric cosmological models will be presented elsewhere.Comment: 20 pages, 2 figure
- …