A solution for galactic disks with Yukawian gravitational potential

DOI10.1007/s10714-007-0420-8zbMath1129.83344arXivgr-qc/0702092OpenAlexW3100970538MaRDI QIDQ995899

O. D. Miranda, José Carlos N. de Araujo

Publication date: 10 September 2007

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0702092

Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15)

Related Items (4)

Gravitons in fractional action cosmology ⋮ The conservation of energy-momentum and the mass for the graviton ⋮ Probing Yukawian gravitational potential by numerical simulations. I: Changing \(N\)-body codes ⋮ Probing Yukawian gravitational potential by numerical simulations. II: Elliptical galaxies

Cites Work

• Potential-density pairs for axisymmetric galaxies: the influence of scalar fields
• On the Distribution of Matter Within Highly Flattened Galaxies.
• Cosmological Physics

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