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The structure of the Universe on 100 Mpc Scales

Jaan Einasto
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Abstract

Observational evidence for the presence of a preferred scale around 100 Mpc in the distribution of high-density regions in the Universe is summarised. Toy models with various degrees of regularity are analysed to understand better the observational data. Predictions of models which produce a feature on the initial power spectrum of matter are analysed and compared with new observational data on the CMB angular spectrum, cluster mass function, and galaxy and cluster power spectrum.

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Jaan Einasto. 2000-11-17. The structure of the Universe on 100 Mpc Scales. https://arxiv.org/abs/astro-ph/0011334

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