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- W2768657341 abstract "A previous work found that a nonminimally coupled theory of gravity can, under appropriate conditions, give rise to an additional contribution to the field equations interpreted as dark matter [1]: in particular, the density of this dark matter component was found to scale as a power of the density of visible matter. However, no explicit solution for the modified field equations was provided, so that a direct computation of the specific density profile followed by visible matter is missing. This question is now addressed: analytical solutions to the modified field equations are derived in the appropriate perturbative regime and characterised, with an emphasis on directly obtaining the visible matter profile in a self-consistent way. We compare with known profiles for visible and dark matter and obtain constraints on the parameters of the model." @default.
- W2768657341 created "2017-12-04" @default.
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- W2768657341 date "2017-12-14" @default.
- W2768657341 modified "2023-09-26" @default.
- W2768657341 title "Visible and dark matter profiles in a non-minimally coupled model" @default.
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- W2768657341 doi "https://doi.org/10.1088/1361-6382/aa9a11" @default.
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