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• W3100694445 abstract "We study a classical bouncing scenario in beyond Horndeski theory. We give an example of spatially flat bouncing solution that is non-singular and stable throughout the whole evolution. The model is arranged in such a way that the scalar field driving the cosmological evolution initially behaves like full-fledged beyond Horndeski, whereas at late times it becomes a massless scalar field minimally coupled to gravity." @default.
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• W3100694445 date "2017-08-31" @default.
• W3100694445 modified "2023-10-01" @default.
• W3100694445 title "Cosmological bounce and Genesis beyond Horndeski" @default.
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• W3100694445 doi "https://doi.org/10.1088/1475-7516/2017/08/038" @default.
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