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- W4240208092 abstract "It is assumed that the dark energy observed today is frozen as a result of a phase transition involving the source of that energy. Postulating that the dark energy de-coherence which results from this phase transition drives statistical variations in the energy density specifies a class of cosmological models in which the cosmic microwave background (CMB) fluctuation amplitude at last scattering is approximately 10{sup -5}." @default.
- W4240208092 created "2022-05-12" @default.
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- W4240208092 date "2004-12-17" @default.
- W4240208092 modified "2023-10-14" @default.
- W4240208092 title "CMB Fluctuation Amplitude from Dark Energy Partitions" @default.
- W4240208092 doi "https://doi.org/10.2172/839718" @default.
- W4240208092 hasPublicationYear "2004" @default.
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