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Q-ball Formation through Affleck-Dine Mechanism

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arxiv hep-ph/9909509 v3 pith:OK2LT4LK submitted 1999-09-25 hep-ph

Q-ball Formation through Affleck-Dine Mechanism

classification hep-ph
keywords q-ballaffleck-dinechargescondensateformationinitialmechanismq-balls
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We present the full nonlinear calculation of the formation of a Q-ball through the Affleck-Dine (AD) mechanism by numerical simulations. It is shown that large Q-balls are actually produced by the fragmentation of the condensate of a scalar field whose potential is very flat. We find that the typical size of a Q-ball is determined by the most developed mode of linearized fluctuations, and almost all the initial charges which the AD condensate carries are absorbed into the formed Q-balls, whose sizes and the charges depend only on the initial charge densities.

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Cited by 5 Pith papers

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  1. Reviving the Affleck-Dine Curvaton Scenario with Compensated Isocurvature Perturbations

    astro-ph.CO 2026-07 conditional novelty 6.0

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  2. Quantum-Corrected Q-balls in the Friedberg-Lee-Sirlin Model

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    hep-th 2025-10 conditional novelty 6.0

    Soliton formation in complex scalar field theory is framed as sound-mode-induced phase separation, and cylindrical Q-strings are shown to suffer a Rayleigh-Plateau membrane instability that breaks them into spheres.

  4. Fermion Condensate Inflation, Dynamical Waterfall Mechanism and Primordial Black Holes

    hep-th 2026-04 unverdicted novelty 5.0

    Torsion-induced fermion condensate produces hybrid inflation with axial-chemical-potential waterfall, Q-ball PBH seeds, and parity-violating signatures in Chern-Simons gravity.

  5. Dynamical Boson Stars

    gr-qc 2012-02 unverdicted novelty 2.0

    Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.