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W2006106977 abstract "In this work the phenomenology of models possessing a non-minimal coupling between matter and geometry is discussed, with a particular focus on the possibility of describing the flattening of the galactic rotation curves as a dynamically generated effect derived from this modification to General Relativity. Two possibilities are discussed: firstly, that the observed discrepancy between the measured rotation velocity and the classical prediction is due to a deviation from geodesic motion, due to a non-(covariant) conservation of the energy-momentum tensor; secondly, that even if the principle of energy conservation holds, the dynamical effects arising due to the non-trivial terms in the Einstein equations of motion can give rise to an extra density contribution that may be interpreted as dark matter. In this work, The mechanism of the latter alternative is detailed; a numerical session ascertaining the order of magnitude of the relevant parameters is undertaken in another contribution to this volume, with possible cosmological implications discussed." @default.
W2006106977 created "2016-06-24" @default.
W2006106977 creator A5043227634 @default.
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W2006106977 date "2010-04-01" @default.
W2006106977 modified "2023-09-25" @default.
W2006106977 title "Dark matter as a dynamic effect due to a non-minimal gravitational coupling with matter (I): Analytical results" @default.
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W2006106977 doi "https://doi.org/10.1088/1742-6596/222/1/012010" @default.
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