Volume 430, Number 3, February II 2005
|Page(s)||827 - 842|
|Section||Cosmology (including clusters of galaxies)|
|Published online||26 January 2005|
Time evolution of the stochastic linear bias of interacting galaxies on linear scales
Institut für Astrophysik und Extraterrestrische Forschung, Auf dem Hügel 71, 53121 Bonn, Germany e-mail: firstname.lastname@example.org
Accepted: 1 October 2004
We extend the time dependent bias model of Tegmark & Peebles ([CITE]) to predict the large-scale evolution of the stochastic linear bias of different galaxy populations with respect to both the dark matter and each other. The resulting model equations contain a general expression, coined the “interaction term”, accounting for the destruction or production of galaxies. This term may be used to model couplings between different populations that lead to an increase or decrease of the number of a galaxies belonging to a population, e.g. passive evolution or merging processes. This is explored in detail using a toy model. In particular, it is shown that the presence of such a coupling may change the evolution of the bias parameter compared to an interaction-free evolution. We argue that the observation of the evolution of the large-scale bias and galaxy number density with wide-field surveys may be used to infer fundamental interaction parameters between galaxy populations, possibly giving an insight in their formation and evolution.
Key words: galaxies: statistics / cosmology: theory / cosmology: dark matter / cosmology: large-scale structure of Universe / Galaxy: fundamental parameters
© ESO, 2005
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