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Magnetic field generation from bubble collisions during first-order phase transition

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arxiv 2102.01398 v1 pith:LKUIA5NM submitted 2021-02-02 astro-ph.CO hep-phhep-th

classification astro-ph.COhep-phhep-th
keywords fieldmagneticbubblesphasecollisionsfirst-ordergenerationtransition
verification ladder T0 review T1 audit T2 compute T3 formal
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We study the magnetic fields generation from the cosmological first-order electroweak phase transition. We calculate the magnetic field induced by the variation of the Higgs phase for two bubbles and three bubbles collisions. Our study shows that electromagnetic currents in the collision direction produce the ring-like magnetic field in the intersect regions of colliding bubbles, which may seed the primordial magnetic field that are constrained by intergalatic field observations.

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Cited by 1 Pith paper

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

  1. Magnetogenesis from Sawtooth Coupling: Gravitational Wave Probe of Reheating

    astro-ph.CO 2025-06 conditional novelty 5.0 of 10

    A sawtooth coupling active during reheating can generate blue-tilted magnetic fields whose secondary gravitational waves peak at nanohertz to millihertz frequencies.

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