Little perturbations grow up\(\dots \)without dark matter

DOI10.1007/s10773-011-0948-yzbMath1241.83077OpenAlexW2065184994WikidataQ62045352 ScholiaQ62045352MaRDI QIDQ427340

Elmo Benedetto, Antonio Feoli

Publication date: 13 June 2012

Published in: International Journal of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10773-011-0948-y

zbMATH Keywords

dark mattercosmological perturbationsstructure formation

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Radiative transfer in astronomy and astrophysics (85A25) Astrophysical cosmology (85A40)

Related Items (2)

A determination of the Ω0mh2 cosmological parameter without tension ⋮ Vorticity of matter or vorticity of space?

Cites Work

• Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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