2007

Galaxy clustering constraints on deviations from Newtonian gravity at cosmological scales II: Perturbative and numerical analyses of power spectrum and bispectrum

Shirata, Akihito, Suto, Yasushi, Hikage, Chiaki et al.

Understand

We explore observational constraints on possible deviations from Newtonian gravity by means of large-scale clustering of galaxies.

We measure the power spectrum and the bispectrum of Sloan Digital Sky Survey galaxies and compare the result with predictions in an empirical model of modified gravity.
Our model assumes an additional Yukawa-like term with two parameters that characterize the amplitude and the length scale of the modified gravity.
The model predictions are calculated using two methods; the second-order perturbation theory and direct N-body simulations.

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