Modelling the rotational curves of spiral galaxies with a scalar field

DOI10.1051/0004-6361:20040192zbMath1060.85520arXivgr-qc/0411104OpenAlexW3105755135WikidataQ68848212 ScholiaQ68848212MaRDI QIDQ3156080

J. P. Mbelek

Publication date: 6 January 2005

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0411104

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Astrophysical cosmology (85A40)

Related Items (6)

Viability of nonminimally coupled \(f(R)\) gravity ⋮ Scalar-tensor theories and asymmetric resonant cavities ⋮ Revaluation of Mbelek and Lachièze-Rey scalar-tensor theory of gravitation to explain the measured forces in asymmetric resonant cavities ⋮ Characteristic size and mass of galaxies in the Bose-Einstein condensate dark matter model ⋮ Temporal variation of Earth-based gravitational constant measurements ⋮ IS DARK MATTER AN EXTRA-DIMENSIONAL EFFECT?

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