We study the late-time integrated Sachs–Wolfe (ISW) effect in f (R) gravity using N-body
simulations. In the f (R) model under study, the linear growth rate is larger than that in …

We use large-volume N-body simulations to predict the clustering of dark matter in redshift
space in f (R) modified gravity cosmologies. This is the first time that the non-linear matter …

In order to explain cosmic acceleration without invoking``dark''physics, we consider f (R)
modified gravity models, which replace the standard Einstein-Hilbert action in General …

We investigate the impact on cosmological observables of f (Q)-gravity, a specific class of
modified gravity models in which gravity is described by the nonmetricity scalar, Q. In …

We study the matter and velocity divergence power spectra in af (R) gravity theory and their
time evolution measured from several large-volume N-body simulations with varying box …

In this work, we analyse the Lyman α forest in cosmological hydrodynamical simulations of
Chameleon-type f (R)-gravity with the goal to assess whether the impact of such models is …

In this paper, a specific family of f (R) models that can produce the Λ CDM background
expansion history is constrained by using the currently available geometric and dynamic …

This study investigates the cosmic bulk flow through an analysis of luminosity distance
variations in a perturbed Friedmann universe governed by f (R) gravity. The Hubble …

We present an analysis of galaxy–galaxy weak gravitational lensing (GGL) in chameleon f
(R) gravity–a leading candidate of non-standard gravity models. For the analysis, we have …

We study the growth of matter density perturbations δ m for a number of viable f (R) gravity
models that satisfy both cosmological and local gravity constraints, where the Lagrangian …