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- W2003143012 abstract "We introduce a simple model for the formation of voids. In this model the underdensity of galaxies in voids is the product of two factors. The first arises from a gravitational expansion of the negative density perturbation. The second is due to biasing: galaxies are less likely to form in an underdense region. One feature of the model is an upper cutoff in void sizes. We calculate the volume-filling factor of characteristic voids for different cold dark matter (CDM) models and find that our formation model points to ΛCDM models as preferred models of the power spectrum. A natural consequence of our model is that the underdensity of the dark matter inside voids is smaller than the galaxy underdensity." @default.
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- W2003143012 date "2001-02-10" @default.
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- W2003143012 title "A Model of Void Formation" @default.
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- W2003143012 doi "https://doi.org/10.1086/318652" @default.
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