A scalar field as a candidate for the cosmological non-baryonic dark matter

DOI10.1023/A:1026617700841zbMath0934.83062OpenAlexW1680748658MaRDI QIDQ1308427

Hernando Quevedo, Daniel Sudarsky, Marcelo Salgado

Publication date: 23 November 1999

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

Full work available at URL: https://doi.org/10.1023/a:1026617700841

zbMATH Keywords

cosmological dark mattermassive scalar field non-minimally coupled to gravity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items

Periodic distribution of galaxies in generalized scalar tensor theory

Cites Work

• Inflationary universe: A possible solution to the horizon and flatness problems
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