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- W2785924179 abstract "A few years ago Baker cite{baker} proposed a Lema$hat{i}$tre-Tolman metric to interpolate smoothly between the Schwarzschild metric at small scales and the Friedmann-Robertson-Walker (FRW) metric at large scales. As it stands, by implementing the Bona-Stela construction cite{bona} its predictions are incompatible with solar system data. We find a different metric within the same class which avoids this problem while introducing a variable modified gravitational potential which dominates Newtonian gravity for low central baryoinc densities at early time, that can go some way to explain the growth rate of the baryonic matter density perturbation and the enhancement of the higher CMB acoustic peak anisotropies." @default.
- W2785924179 created "2018-02-23" @default.
- W2785924179 creator A5076879275 @default.
- W2785924179 date "2016-01-04" @default.
- W2785924179 modified "2023-10-01" @default.
- W2785924179 title "Modified Newtonian Mechanics from an interpolating metric" @default.
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