activity
20172020
most citedA comparison of Einstein-Boltzmann solvers for testing General Relativity

62 citations · 62 across the 1 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2020

Latest evidence for a late time vacuum -- geodesic CDM interaction

Natalie B. Hogg, Marco Bruni, Robert Crittenden +2

We perform a reconstruction of the coupling function between vacuum energy and geodesic cold dark matter using the latest observational data. We bin the interaction in seventeen re…

astro-ph.CO2019

Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds

Noemi Frusciante, Simone Peirone, Luis Atayde +1

We investigate the generalized cubic covariant Galileon model, a kinetically driven dark energy model within the Horndeski class of theories. The model extends the cubic covariant…

astro-ph.CO2019

Strong Lensing Time Delay Constraints on Dark Energy: a Forecast

Banafshe Shiralilou, Matteo Martinelli, Georgios Papadomanolakis +3

Measurements of time delays between multiple quasar images produced by strong lensing are reaching a sensitivity that makes them a promising cosmological probe. Future surveys will…

astro-ph.CO2019

Cosmological constraints and phenomenology of a beyond-Horndeski model

Simone Peirone, Giampaolo Benevento, Noemi Frusciante +1

We study observational constraints on a specific dark energy model in the framework of Gleyzes-Langlois-Piazza-Vernizzi theories, which extends the Galileon ghost condensate (GGC)…

astro-ph.CO2019

Cosmological data favor Galileon ghost condensate over CDM

Simone Peirone, Giampaolo Benevento, Noemi Frusciante +1

We place observational constraints on the Galileon ghost condensate model, a dark energy proposal in cubic-order Horndeski theories consistent with the gravitational-wave event GW1…

astro-ph.CO2019

Constraints on the interacting vacuum -- geodesic CDM scenario

Matteo Martinelli, Natalie B. Hogg, Simone Peirone +2

We investigate an interacting dark sector scenario in which the vacuum energy is free to interact with cold dark matter (CDM), which itself is assumed to cluster under the sole act…