We consider the effect of a canonically normalised scalar field degree of freedom on the dynamics of gravity from small to large scales. We show that the effects of modified gravity can be completely captured by the time variations of the scalar field mass and its coupling to matter. This leads to a parameterisation of modified gravity where local constraints are easy to analyse and large scale structure effects apparent
We consider the scalar mode of gravity as expressed by a conformal factor of the metric and present ...
We study how the filamentary pattern of the cosmic web changes if the true gravity deviates from gen...
In theories of modified gravity with the chameleon screening mechanism, the strength of the fifth fo...
We consider modified gravity models driven by a scalar field whose effects are screened in high dens...
Extending general relativity by adding extra degrees of freedom is a popular approach for explaining...
Reconstruction of the local velocity field from the overdensity field and a gravitational accelerati...
We study the linear and nonlinear structure formation in the dilaton and symmetron models of modifie...
The velocity field of dark matter and galaxies reflects the continued action of gravity throughout c...
The morphological properties of the large scale structure of the Universe can be fully described by ...
We consider a class of phenomenological modified gravity models where the terms added to the standar...
Extremely large surveys with future experiments like Euclid and the SKA will soon allow us to access...
In this work we study the cosmology of the general f(T) gravity theory. We express the modified Eins...
The turn-around radii of the galaxy groups show the imprint of a long battle between their self-grav...
In this work we systematically study the linear and nonlinear structure formation in chameleon theor...
We perform high-resolution N-body simulations for f(R) gravity based on a self-adaptive particle-mes...
We consider the scalar mode of gravity as expressed by a conformal factor of the metric and present ...
We study how the filamentary pattern of the cosmic web changes if the true gravity deviates from gen...
In theories of modified gravity with the chameleon screening mechanism, the strength of the fifth fo...
We consider modified gravity models driven by a scalar field whose effects are screened in high dens...
Extending general relativity by adding extra degrees of freedom is a popular approach for explaining...
Reconstruction of the local velocity field from the overdensity field and a gravitational accelerati...
We study the linear and nonlinear structure formation in the dilaton and symmetron models of modifie...
The velocity field of dark matter and galaxies reflects the continued action of gravity throughout c...
The morphological properties of the large scale structure of the Universe can be fully described by ...
We consider a class of phenomenological modified gravity models where the terms added to the standar...
Extremely large surveys with future experiments like Euclid and the SKA will soon allow us to access...
In this work we study the cosmology of the general f(T) gravity theory. We express the modified Eins...
The turn-around radii of the galaxy groups show the imprint of a long battle between their self-grav...
In this work we systematically study the linear and nonlinear structure formation in chameleon theor...
We perform high-resolution N-body simulations for f(R) gravity based on a self-adaptive particle-mes...
We consider the scalar mode of gravity as expressed by a conformal factor of the metric and present ...
We study how the filamentary pattern of the cosmic web changes if the true gravity deviates from gen...
In theories of modified gravity with the chameleon screening mechanism, the strength of the fifth fo...