Structure Formation in the Cosmological Voids

Mathematics – Logic

Scientific paper

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Scientific paper

While the dynamics of globular clusters are being explored, their counterparts, the cosmological voids, are still in the realm of the mysterious. To date, they are the largest known structures in the universe. Recently, there has been intense interest in the study of the void galaxies. These underdense regions of the universe are viewed as a cosmological phenomenon. Voids are interesting in fact that they are seemingly devoid of any matter while other regions of the universe are flourishing with star and formation growth. Goldberg and Vogeley (2002) have proposed an interesting technique for determining the cosmological void parameters. This theoretical standpoint utilizes Birchoff's theorem to treat voids as their own individually evolving universes. We have approached the question of voids from a numerical front. From the hierarchal data output, we are able to describe various structure formations, galaxy morphologies, power spectra, and the gases that constitute these regions of the universe.

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