Chameleon fields may modify gravity on cluster scales while recovering general relativity
locally. This article reviews signatures of chameleon modifications in the nonlinear …

The current standard cosmological model is constructed within the framework of general
relativity with a cosmological constant Λ, which is often associated with dark energy, and …

Since the discovery of the accelerated expansion of the present universe, significant
theoretical developments have been made in the area of modified gravity. In the meantime …

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 analyse modelling techniques for the large-scale structure formed in scalar-tensor
theories of constant Brans-Dicke parameter which match the concordance model …

In the context of upcoming large-scale structure surveys such as Euclid, it is of prime
importance to quantify the effect of peculiar velocities on geometric probes. Hence, the …

Mapping the large-scale structure through cosmic time has numerous applications in studies
of cosmology and galaxy evolution. At z≳ 2, the structure can be traced by the neutral …

We constrain f (R) and chameleon-type modified gravity in the framework of the Berstchinger-
Zukin parametrization using the recently released Planck data, including both the cosmic …

The morphological properties of the large scale structure of the Universe can be fully
described by four Minkowski functionals (MFs), which provide important complementary …

We present new and accurate measurements of the cosmic distance–redshift relation,
spanning 0.2< z< 1, using the topology of large-scale structure as a cosmological standard …