Papers › Nonlinear evolution of initially biased tracers in modified gravity

Nonlinear evolution of initially biased tracers in modified gravity

20 Sep 2018arXiv:1809.07713links table onlyarchive 2025-07-28

Alejandro Aviles, Mario Alberto Rodriguez-Meza, Josue De-Santiago, Jorge L. Cervantes-Cota

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In this work we extend the perturbation theory for modified gravity (MG) in two main aspects. First, the construction of matter overdensities from Lagrangian displacement fields is shown to hold in a general framework, allowing us to find Standard Perturbation Theory (SPT) kernels from known Lagrangian Perturbation Theory (LPT) kernels. We then develop a theory of biased tracers for generalized cosmologies, extending already existing formalisms for ΛCDM. We present the correlation function in Convolution-LPT and the power spectrum in SPT for ΛCDM, f(R) Hu-Sawicky, and DGP braneworld models. Our formalism can be applied to many generalized cosmologies and to facilitate it, we are making public a code to compute these statistics. We further study the relaxation of bias with the use of a simple model and of excursion set theory, showing that in general the bias parameters have smaller values in MG than in General Relativity.

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