The Void Phenomenon
By P. Peebles, Joseph Henry. 2001
273 citations recorded by the source corpus.
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.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/c5a8477bb3930c5d4cc1210de6d6ce913578bd00
How researchers see this paper
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In Astronomy and Astrophysics
- Simon D. M. White
- Volker Springel
- F. V. D. Bosch
- L. Hernquist
- C. Baugh
- P. Hopkins
- Carlos S. Frenk
- Andrey V. Kravtsov
In Atomic and Molecular Physics, and Optics
- Michael S. E. Vogeley
- F. Hoyle
- J. Brinkmann
- Randall R. Rojas
- Risa Wechsler
- Mark Neyrinck
- Andrey V. Kravtsov
- Rien van de Weygaert
In Instrumentation
- Simon D. M. White
- Volker Springel
- F. V. D. Bosch
- Carlos S. Frenk
- C. Baugh
- A. Benson
- L. Hernquist
- P. Hopkins
Citations in the corpus
- Voids in the Point Source Catalogue Survey and the Updated Zwicky Catalog (2001, background): “Peebles (2001) discusses an apparent discrepancy between the cold dark matter (CDM) model and observations.”
- zobov: a parameter-free void-finding algorithm (2007, background): “For example, Peebles (2001) has pointed out that there seem to be fewer galaxies in voids than cosmological simulations predict.”
- Is there a "too big to fail" problem in the field? (2014, background): “…discrepancies have been discovered in the field in various contexts, e.g. related to the paucity of low-mass galaxies in voids (“void phenomenon”; Peebles 2001), the sizes of mini-voids in the Local Volume (Tikhonov & Klypin 2009), or the slowly rising galaxy velocity function (Zwaan et al.…”
- Equivalence Principle Implications of Modified Gravity Models (2009, result): “[41] G. Farrar and P. J. E. Peebles, “Interacting Dark Matter and Dark Energy,” Astrophys.”
- The Aspen-Amsterdam void finder comparison project (2008, background): “But while the general picture appears to be well supported by the standard Λ Cold Dark Matter (ΛCDM) cosmology, Peebles (2001) pointed out some potentially critical issues.”
- Galaxy Groups Within 3500 km s−1 (2017, background): “The lack of dwarf galaxies in underdense regions (Peebles 2001; Kreckel et al. 2011; Rizzi et al. 2017) is an extension to Figure 9.”
- Cosmic Voids in Sloan Digital Sky Survey Data Release 7 (2011, background): “Peebles (2001) describes the “void phenomenon”: galaxies of all types appear to respect the same voids, in contrast to the prediction of CDM that low density regions should contain many low mass objects.”
- The Dependence of Halo Clustering on Halo Formation History, Concentration, and Occupation (2005, background): “The currently favored CDM model predicts substantial mass in voids, so the absence of galaxies in these regions has been suggested to be a potentially serious problem for the prevailing paradigm (Peebles 2001).”
- A hierarchy of voids: much ado about nothing (2003, background): “In recent years, the possibility that void galaxies are a systematically different population has received considerable attention (see e.g. Szomoru et al. 1996; El-Ad & Piran 2000; Peebles 2001; Mathis & White 2002, Rojas et al. 2003; Benson et al. 2003).”
- Dwarf galaxies in voids: suppressing star formation with photoheating (2005, background): “Peebles (2001) pointed out that the dwarf galaxies in the Optical Redshift Survey (ORS) follow the distribution of bright galaxies remarkably closely.”
- Non-linear evolution of cosmological structures in warm dark matter models (2011, background): “Thirdly, the observed number of dwarf galaxies in the voids appears to be far smaller than expected from CDM (Peebles 2001; Tikhonov et al. 2009; Peebles & Nusser 2010).”
- Photometric Properties of Void Galaxies in the Sloan Digital Sky Survey (2003, background): “Peebles (2001) pointed out the apparent discrepancy between Cold Dark Matter Models (CDM) and observations.”
- Unusually Large Fluctuations in the Statistics of Galaxy Formation at High Redshift (2003, background): “However, voids are observed to be rather deficient in dwarf galaxies as well as in larger galaxies on the scale of the Milky Way (e.g., Kirshner et al. 1981; Eder et al. 1989; Grogin & Geller 1999, 2000; El-Ad & Piran 2000; Peebles 2001).”
- Modified Gravity and Cosmology (2011, unknown): “Cosmological voids seem to be more empty of galaxies than expected, as has been championed by Peebles [1030].”
- A cosmic watershed: the WVF void detection technique (2007, background): “Voids provide a unique and still largely pristine environment for studying the evolution of galaxies (Hoffman, Silk & Wyse 1992; Little & Weinberg 1994; Peebles 2001).”