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Linear Evolution of Small Scale Cosmological Density Perturbations
Published online by Cambridge University Press: 25 May 2016
Extract
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
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- Copyright © Kluwer 1999