On the origin of cosmic structure

Details On the origin of cosmic structure On the origin of cosmic structure

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...392l...5l&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 392, no. 1, June 10, 1992, p. L5-L8.

Astronomy and Astrophysics

Astrophysics

3

Astronomical Models, Galactic Evolution, Gravitation Theory, Background Radiation, Cosmic Rays, Galactic Clusters, Galactic Structure

Scientific paper

A parameter-free theory of the origin and evolution of structure in an initially cold Friedmann universe predicts that self-gravitating systems, from stars and planetary systems to galaxy clusters, are formed from the bottom up by repeated clustering, while a qualitatively different kind of structure, characterized by convex, connected, underdense regions and connected sheetlike or filamentary overdense regions, evolves from quantum fluctuations at the Planck era.

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