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Accurate predictions for the scale-dependent galaxy bias from primordial non-Gaussianity
2011
Physical Review D
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The large-scale clustering of galaxies can serve as a probe of primordial non-Gaussianity in the Universe competitive with the anisotropies of the CMB. Here, we present improved theoretical predictions which include an important, previously overlooked correction to the bias. We demonstrate that the new predictions are able to reproduce the results of N-body simulations, explaining the significant departures seen from previous theoretical results. These refined predictions open the way to
doi:10.1103/physrevd.84.061301
fatcat:tirhlw7ifngp3elleuxjqdlnsu