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- W2161954501 abstract "We propose an alternative scenario for the dark matter gener ation from an evolving cosmological constant which interacts with the dominant background in certain intermediate phase of the universe, and relaxes to the observed small value at present . In this way, it is shown that the interaction of the cosmological constant with the radiation o r matter might generate the dark matter densities with a varied mass spectrum in the universe with their characteristic arc-like frozen signatures on the Cosmic Microwave Background Radiation (CMBR). This approach also suggests a possible solution to the long standing cosmological constant problem." @default.
- W2161954501 created "2016-06-24" @default.
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- W2161954501 date "2011-06-06" @default.
- W2161954501 modified "2023-09-24" @default.
- W2161954501 title "A new mechanism for dark matter generation from an interacting cosmological constant" @default.
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- W2161954501 doi "https://doi.org/10.22323/1.123.0218" @default.
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