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• W2051504644 abstract "Through a detailed numerical investigation in three spatial dimensions, we demonstrate that long-lived time-dependent field configurations emerge dynamically during symmetry breaking in an expanding de Sitter spacetime. We investigate two situations: a single scalar field with a double-well potential and an SU(2) non-Abelian Higgs model. For the single scalar, we show that large-amplitude oscillon configurations emerge spontaneously and persist to contribute about 1.2% of the energy density of the Universe. We also show that for a range of parameters, oscillon lifetimes are enhanced by the expansion and that this effect is a result of parametric resonance. For the SU(2) case, we see about 4% of the final energy density in oscillons." @default.
• W2051504644 created "2016-06-24" @default.
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• W2051504644 date "2010-08-16" @default.
• W2051504644 modified "2023-10-02" @default.
• W2051504644 title "Long-lived time-dependent remnants during cosmological symmetry breaking: From inflation to the electroweak scale" @default.
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• W2051504644 doi "https://doi.org/10.1103/physrevd.82.043517" @default.
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