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Cited by 278

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Dark matter as a geometric effect in f(R) gravity

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Böhmer, Christian G., Harko, Tiberiu, Lobo, Francisco S.N.·2008·Astroparticle Physics

Abstract

Abstract We consider the behavior of the tangential velocity of test particles moving in stable circular orbits in f ( R ) modified theories of gravity. A large number of observations at the galactic scale have shown that the rotational velocities of massive test particles (hydrogen clouds) tend towards constant values at large distances from the galactic center. We analyze the vacuum gravitational field equations in f ( R ) models in the constant velocity region, and the general form of the metric tensor is derived in a closed form. The resulting modification of the Einstein–Hilbert Lagrangian is of the form R 1 + n , with the parameter n expressed in terms of the tangential velocity. Therefore we find that to explain the motion of test particles around galaxies requires only very mild deviations from classical general relativity, and that modified gravity can explain the galactic dynamics without the need of introducing dark matter.

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Crossref · 10.1016/j.astropartphys.2008.04.003

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Metadata

Authors
Böhmer, C. G., Harko, T., & Lobo, F. S. N.
Venue
Astroparticle Physics
Publisher
Elsevier BV
Published
2008-07
Volume
29
Issue
6
Pages
386-392
ISSN
0927-6505 (ISSN-L)
OpenAlex
W1995482552
Cited by
278
References
2
FWCI
8.65
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Dark matter as a geometric effect in f(R) gravity. https://app.cochat.ai/papers/10.1016/j.astropartphys.2008.04.003
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Böhmer, C. G., Harko, T., & Lobo, F. S. N. (2008). Dark matter as a geometric effect in f(R) gravity. Astroparticle Physics. https://doi.org/10.1016/j.astropartphys.2008.04.003

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.