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Heterogeneous cosmological phase transitions: seeded by domain walls and junctions

Abstract:
Heterogeneous nucleation is central to many familiar first-order phase transitions such as the freezing of water and the solidification of metals, and it can also play a crucial role in cosmology. We examine nucleation seeded by preexisting domain walls and demonstrate its strong impact on the dynamics of cosmological phase transitions. The bubble solutions take the form of spherical caps, and the contact angle is fixed by the ratio of the domain-wall tension to the bubble-wall tension. A larger domain-wall tension, or equivalently a smaller contact angle, reduces the wall-seeded bubble volume and lowers the critical nucleation action. For theories with ℤ n≥3 symmetry, domain-wall junctions naturally appear and we find that they seed nucleation even more efficiently than the walls themselves. Using a two-scalar-field model as an illustration, we compute nucleation temperatures for both homogeneous and heterogeneous channels and show that junction-seeded nucleation occurs at a higher temperature and is the dominant mechanism that completes the first-order cosmological phase transition.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1088/1475-7516/2026/05/036

Authors

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Role:
Author
ORCID:
0000-0002-2957-7319
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Physics - Central
Role:
Author
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Role:
Author
ORCID:
0000-0002-7441-7648


Publisher:
IOP Publishing
Journal:
Journal of Cosmology and Astroparticle Physics More from this journal
Volume:
2026
Issue:
05
Pages:
036
Article number:
036
Publication date:
2026-05-14
Acceptance date:
2026-03-06
DOI:
EISSN:
1475-7516
ISSN:
1475-7516


Language:
English
Keywords:
Source identifiers:
4048044
Deposit date:
2026-05-14
ARK identifier:
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