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- W4313184306 abstract "A classical field theory description (which can be obtained from an $$f(R,chi )$$ ) of dark energy–dark matter interaction is considered. Demanding that the interaction strength $$Q_{nu }$$ in the dark sector must have a field theory description and a fluid description, a unique form of interaction strength is obtained. It is shown that the one-to-one mapping between the classical field theory description and the phenomenological fluid description of dark energy–dark matter interaction exists only for this unique form of interaction. Then a novel autonomous system and its stability analysis for the general interacting dark sector is introduced, followed by the background analysis for a specific potential and interaction function." @default.
- W4313184306 created "2023-01-06" @default.
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- W4313184306 date "2022-01-01" @default.
- W4313184306 modified "2023-10-14" @default.
- W4313184306 title "Cosmological Perturbations in the Interacting Dark Sector: Mapping Fields and Fluids" @default.
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- W4313184306 doi "https://doi.org/10.1007/978-981-19-2354-8_121" @default.
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