Hostname: page-component-6bf8c574d5-b4m5d Total loading time: 0 Render date: 2025-02-22T01:11:09.760Z Has data issue: false hasContentIssue false
  • English
  • Français

Linear Evolution of Small Scale Cosmological Density Perturbations

Published online by Cambridge University Press:  25 May 2016

K. Yamamoto ,
N. Sugiyama  and
H. Sato
K. Yamamoto
Affiliation:
Department of Physics, Hiroshima University, Higashi-Hiroshima 739, Japan
N. Sugiyama
Affiliation:
Department of Physics, Kyoto University, Kyoto 606-01, Japan
H. Sato
Affiliation:
Department of Physics, Kyoto University, Kyoto 606-01, Japan

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We carefully re-examine the evolution of small scale cosmological perturbations, motivated from the studies of cosmic structure formation in the high-z universe. Under the assumption of the hierarchical clustering scenario, the evolution of density fluctuations on very small scales is especially important for the early formation of the bound objects such as population III stars or primordial sub-galaxies.

Type
IV. Structure Formation and Dark Matter
Information
Symposium - International Astronomical Union , Volume 183: Cosmological Parameters and the Evolution of the Universe , 1999 , pp. 273
Copyright
Copyright © Kluwer 1999 

References

1. Yamamoto, K., Sugiyama, N. and Sato, H. (1997) Physical Review D, in press, astro-ph/9709209.Google Scholar
2. Yamamoto, K., Sugiyama, N. and Sato, H. (1997) submitted to Astrophysical Journal, astro-ph/9709247.Google Scholar