Year: 2025
Type: preprint
Abstract: In this Letter, we numerically present the possibility of the first-order phase transition occurring through the thermal fluctuation in the early universe. We find that when the temperature is slightly higher than the mass scale of the background field, the bubble-like field configurations appear proceeded by oscillons, which expand and collide to finish the phase transition. We provide the false vacuum decay rate and the accompanied gravitational waves. We also present the vacuum phase transition comparison of the quantum tunneling case and thermal fluctuation case.
Source: arXiv (Cornell University)
Authors: Bian, Ligong, Di, Yuefeng, Jia, Yongtao, Li, Yang, Zeng, Kehao
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
Awards: G1796291137, G4763861809, G6883445009
OpenAlex ID: W4415328810
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