Geometric conditions on the type of matter determining the flat behavior of the rotational curves in galaxies

DOI10.1023/A:1015343528053zbMath0999.83074arXivastro-ph/0005528MaRDI QIDQ1604925

F. Siddhartha Guzmán, Tonatiuh Matos, Erandy Ramírez, Darío Núñez

Publication date: 9 July 2002

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

Full work available at URL: https://arxiv.org/abs/astro-ph/0005528

zbMATH Keywords

test particleaxisymmetric stationary spacetimedisk of matter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Observational and experimental questions in relativity and gravitational theory (83B05)

Related Items (3)

Straight spinning cosmic strings in Brans–Dicke gravity ⋮ Linearized modified gravity theories with a cosmological term: advance of perihelion and deflection of light ⋮ ON THE CONTRIBUTIONS FROM DILATONIC STRINGS TO THE FLAT BEHAVIOR OF THE ROTATIONAL CURVES IN GALAXIES

Cites Work

• Wormholes in spacetime and their use for interstellar travel: A tool for teaching general relativity
• Scalar fields as dark matter in spiral galaxies
• Cosmological Imprint of an Energy Component with General Equation of State
• General Relativity
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