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- W2024199154 abstract "We study non-linear structure formation in an interacting model of the dark sector of the Universe in which the dark energy density decays linearly with the Hubble parameter, $rho_{Lambda} propto H$, leading to a constant-rate creation of cold dark matter. We derive all relevant expressions to calculate the mass function and the cluster number density using the Sheth-Torman formalism and show that the effect of the interaction process is to increase the number of bound structures of large masses ($M gtrsim 10^{14} M_{odot}h^{-1}$) when compared to the standard $Lambda$CDM model. Since these models are not reducible to each other, this number counts signature can in principle be tested in future surveys." @default.
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- W2024199154 date "2015-02-02" @default.
- W2024199154 modified "2023-10-18" @default.
- W2024199154 title "Number counts and dynamical vacuum cosmologies" @default.
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- W2024199154 doi "https://doi.org/10.1093/mnras/stu2662" @default.
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