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Domain walls and strings formation in the early Universe

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arxiv 2011.07041 v1 pith:BHJ4FDEP submitted 2020-11-09 hep-th

Alexander A. Kirillov , Boris S. Murygin This is my paper · ORCID
classification hep-th
keywords domainearlyfieldsformationscalarstringsuniversewalls
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Solitons formation through classical dynamics of two scalar fields with the potential having a saddle point and one minimum in (2+1)-space-time is discussed. We show that under certain conditions in the early Universe both domain walls and strings can be formed even if scalar fields are inflaton ones.

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  1. Soliton foam formation in the early Universe

    hep-th 2024-12 conditional novelty 6.0 of 10

    Post-inflationary quantum fluctuations of two scalar fields can form a three-dimensional soliton foam of closed domain walls, string-bounded walls, and scalar radiation, without a thermal phase transition.

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