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Periodic Cosmic String Formation and Dynamics

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arxiv 2503.03116 v2 pith:VU26BTKB submitted 2025-03-05 hep-ph astro-ph.COgr-qc

classification hep-phastro-ph.COgr-qc
keywords fieldperiodicdynamicsformationlargescalarstringbursts
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abstract

We study string formation and dynamics in a scalar field theory with a global $U(1)$ symmetry. If a scalar field $\Phi$ is initially displaced from the minimum of a wine-bottle potential, even if uniformly over large spatial patches, small spatial perturbations to $\Phi$ grow via parametric resonance as $\Phi$ oscillates; this occurs for a wide range of initial $U(1)$ charge densities. The growth of perturbations leads to the formation of spatially coherent, temporally stable "counter-rotating regions" (CRR): spatially connected regions exhibiting $\Phi$ evolution with large, opposite-sign rotation speeds in field space which persist over long durations. These CRR are separated by domain boundaries that have a large field gradient and zero rotational speed in field space. String or vortex topological defects form, are confined to, and then annihilate periodically on these boundaries. We demonstrate these periodic dynamics with numerical simulations in both 2+1 and 3+1 dimensions, in both Minkowski spacetime and in a radiation-dominated FLRW universe, and we explain some features of the evolution (semi-)analytically. At late times in an expanding universe, when $\Phi$ approaches the potential minimum, the CRR and vortices dissipate into scalar radiation. Phenomenologically, periodic bursts of string formation and annihilation can lead to periodic bursts of gravitational-wave production. For small initial $U(1)$ charge density, these gravitational-wave bursts can be synchronized across the whole Universe. Owing to their periodic nature, they could give rise to a gravitational-wave frequency spectrum consisting of a forest of peaks. These periodic scalar field dynamics also occur with large, untuned initial $U(1)$ charge density; they may thus have implications for models that depend on a coherent field rotation, such as kination and the axion kinetic-misalignment mechanism. [abridged]

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Anisotropic Gravitational Waves from Anisotropic Axion Rotation

    hep-ph 2025-08 conditional novelty 6.0 of 10

    A transiently dominant rotating axion sources an induced gravitational wave background whose amplitude and large-scale anisotropy trace the axion's isocurvature fluctuations, with detection prospects for BBO and DECIGO.

  2. Searching Stochastic Gravitational Wave Background Landscape Across Frequency Bands

    gr-qc 2025-11 conditional novelty 5.0 of 10

    A hybrid cosmic string–domain wall model can fit the NANOGrav 15-year signal, and its high-frequency tail lies within LISA's projected reach, making the interpretation testable.

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