Skip to search formSkip to main contentSkip to account menu

Science case for the Einstein telescope

The Einstein Telescope (ET), a proposed European ground-based gravitational-wave detector of third-generation, is an evolution of second-generation detectors such as Advanced LIGO, Advanced Virgo,…
View on IOP Publishing (opens in a new tab)

Testing modified gravity at cosmological distances with LISA standard sirens

Modifications of General Relativity leave their imprint both on the cosmic expansion history through a non-trivial dark energy equation of state, and on the evolution of cosmological perturbations in…
View on IOP Publishing (opens in a new tab)

Prospects for fundamental physics with LISA

In this paper, which is of programmatic rather than quantitative nature, we aim to further delineate and sharpen the future potential of the LISA mission in the area of fundamental physics. Given the…
View on Springer (opens in a new tab)

Missing link: A nonlinear post-Friedmann framework for small and large scales

We present a nonlinear post-Friedmann framework for structure formation, generalizing to cosmology the weak-field (post-Minkowskian) approximation, unifying the treatment of small and large scales.…
View PDF on arXiv (opens in a new tab)

Cosmology with Phase 1 of the Square Kilometre Array Red Book 2018: Technical specifications and performance forecasts

Abstract We present a detailed overview of the cosmological surveys that we aim to carry out with Phase 1 of the Square Kilometre Array (SKA1) and the science that they will enable. We highlight…
View on Cambridge Press (opens in a new tab)

Anisotropies and non-Gaussianity of the cosmological gravitational wave background

The Stochastic Gravitational Wave Background (SGWB) is expected to be a key observable for Gravitational Wave (GW) interferometry. Its detection will open a new window on early universe cosmology and…
View PDF on arXiv (opens in a new tab)

Probing the imprint of interacting dark energy on very large scales

The observed galaxy power spectrum acquires relativistic corrections from light-cone effects, and these corrections grow on very large scales. Future galaxy surveys in optical, infrared and radio…
View PDF on arXiv (opens in a new tab)

How the scalar field of unified dark matter models can cluster

In this framework, a technique for reconstructing models where the effective speed of sound is small enough that the scalar field can cluster is proposed, which avoids the strong time evolution of the gravitational potential and the large integrated Sachs–Wolfe effect.
View on IOP Publishing (opens in a new tab)

Characterizing the cosmological gravitational wave background: Anisotropies and non-Gaussianity

A future detection of the Stochastic Gravitational Wave Background (SGWB) with GW experiments is expected to open a new window on early universe cosmology and on the astrophysics of compact objects.…
View PDF on arXiv (opens in a new tab)

Unified Dark Matter models with fast transition

We investigate the general properties of Unified Dark Matter (UDM) fluid models where the pressure and the energy density are linked by a barotropic equation of state (EoS) p = p(ρ) and the…
View PDF on arXiv (opens in a new tab)
...
By clicking accept or continuing to use the site, you agree to the terms outlined in our Privacy Policy (opens in a new tab), Terms of Service (opens in a new tab), and Dataset License (opens in a new tab)