Instability of coherent states of a real scalar field
arXiv:hep-th/0510097 · doi:10.1063/1.2167918
Abstract
We investigate stability of both localized time-periodic coherent states (pulsons) and uniformly distributed coherent states (oscillating condensate) of a real scalar field satisfying the Klein-Gordon equation with a logarithmic nonlinearity. The linear analysis of time-dependent parts of perturbations leads to the Hill equation with a singular coefficient. To evaluate the characteristic exponent we extend the Lindemann-Stieltjes method, usually applied to the Mathieu and Lame equations, to the case that the periodic coefficient in the general Hill equation is an unbounded function of time. As a result, we derive the formula for the characteristic exponent and calculate the stability-instability chart. Then we analyze the spatial structure of the perturbations. Using these results we show that the pulsons of any amplitudes, remaining well-localized objects, lose their coherence with time. This means that, strictly speaking, all pulsons of the model considered are unstable. Nevertheless, for the nodeless pulsons the rate of the coherence breaking in narrow ranges of amplitudes is found to be very small, so that such pulsons can be long-lived. Further, we use the obtaned stability-instability chart to examine the Affleck-Dine type condensate. We conclude the oscillating condensate can decay into an ensemble of the nodeless pulsons.
11 pages, 8 figures, submitted to Physical Review E
References in corpus (18)
- Q-Balls and Baryogenesis in the MSSM
- Structure of Resonance in Preheating after Inflation
- Oscillons: Resonant Configurations During Bubble Collapse
- Pseudo-Stable Bubbles
- Inflationary Models with Logarithmic Potentials
- Q-ball formation in the gravity-mediated SUSY breaking scenario
- Boson Stars: Alternatives to primordial black holes?
- Analytical and numerical properties of Q-balls
- Inflatonic Solitons In Running Mass Inflation
- Resonance Structure for Preheating with Massless Fields
- Numerical simulations of fragmentation of the Affleck-Dine condensate
- Strings, Textures, Inflation and Spectrum Bending
- Resonant nucleation of spatio-temporal order via parametric modal amplification
- The Dynamics of Affleck-Dine Condensate Collapse
- Resonant Nucleation
- Q-ball collisions in the MSSM: gravity-mediated supersymmetry breaking
- The Lame equation in parametric resonance after inflation
- Q-ball Formation in Affleck-Dine Baryogenesis with Gravity-mediated SUSY Breaking
Cited by in corpus (13)
- Analytical Characterization of Oscillon Energy and Lifetime
- Some stationary properties of a -ball in arbitrary space dimensions
- Numerical simulation of oscillatons: extracting the radiating tail
- Gravitational geons in asymptotically anti-de Sitter spacetimes
- Efficient self-resonance instability from axions
- Oscillons in dilaton-scalar theories
- Gravipulsons
- Analytical study of the parametric instability of an oscillating scalar field in an expanding universe
- Deflection of light in time-periodic spherically symmetric gravitational fields
- Passage of test particles through oscillating spherically-symmetric dark matter configurations
- Gravitational frequency shift of light signals in a pulsating dark matter halo
- On the oscillation-driven cosmological expansion at the post-inflation stage
- Resonant phenomena in finite motions of test particles in oscillating dark matter configurations