The Void Phenomenon
P. J. E. Peebles
TL;DR
The paper analyzes the void phenomenon—the pronounced emptiness of voids in the galaxy distribution—and argues that simple biased galaxy formation within CDM struggles to explain observed void emptiness without invoking suppressed galaxy formation or modifications to the mass distribution. It promotes the nearest-neighbor statistic as a robust, interpretable metric to quantify void populations, applying it to dwarfs, irregulars, and low surface brightness galaxies to derive quantitative limits on void populations. Theoretical discussion contrasts Einstein–de Sitter and low-density cosmologies, outlining potential resolutions including suppression mechanisms and warm dark matter, and emphasizes the need for more observational tests and simulations. Overall, the work positions voids as a stringent benchmark for structure formation theories and the scientific method in cosmology, highlighting a potential crisis that could drive paradigm shifts or theory refinement.
Abstract
Advances in theoretical ideas on how galaxies formed have not been strongly influenced by the advances in observations of what might be in the voids between the concentrations of ordinary optically selected galaxies. The theory and observations are maturing, and the search for a reconciliation offers a promising opportunity to improve our understanding of cosmic evolution. I comment on the development of this situation and present an update of a nearest neighbor measure of the void phenomenon that may be of use in evaluating theories of galaxy formation.
