2009

Absence of anti-correlations and of baryon acoustic oscillations in the galaxy correlation function from the Sloan Digital Sky Survey DR7

Labini, Francesco Sylos, Vasilyev, Nikolay L., Baryshev, Yurij V. et al.

Understand

One of the most striking features predicted by standard models of galaxy formation is the presence of anti-correlations in the matter distribution at large enough scales (r>r_c).

Simple arguments show that the location of the length-scale r_c, marking the transition from positive to negative correlations, is the same for any class of objects as for the full matter distribution, i.e.
it is invariant under biasing.
This scale is predicted by models to be at about the same distance of the scale signaling the baryonic acoustic oscillation scale r_{bao}.

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Gabrielli, A., Joyce, M., Sylos Labini, F., 2002, Phys.Rev., D65, 083523
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