Structure and Contents of Cosmic Voids: Tests of Cosmology and Gastrophysics

Mathematics – Logic

Scientific paper

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Scientific paper

Using the Sloan Digital Sky Survey (SDSS) we find that voids fill over 60% of the Universe while containing only approximately 10% of the galaxies. The shapes, sizes, and internal structures of voids can be used to determine the cosmological parameters of the Universe, particularly omega-m, sigma-8, omega-L, and the Hubble constant. Additionally, the detailed properties of objects in voids are a strong test of structure formation models. Ly-alpha absorbers from Hubble-STIS quasar absorption line systems are detected in the proximity of galaxies. However, we find that they do not match the underlying galaxy distribution; 60% of Ly-alpha absorbers live in large (R > 10 Mpc/h) cosmic voids.

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