activity
20242026
collaborators

6 papers

gr-qc2026

Beyond ΛCDM with the SKA Observatory -- I: Probing Gravity on Cosmological Scales

S. Camera, C. Addis, S. L. Guedezounme +26

General relativity (GR) is currently the best description of the gravitational interaction at our disposal and is one of the foundations of the concordance cosmological model. For…

astro-ph.CO2026

Testing the equivalence principle across the Universe: a model-independent approach with galaxy multi-tracing

Sveva Castello, Ziyang Zheng, Camille Bonvin +1

We present a test of the equivalence principle on cosmological scales. This cornerstone of general relativity has been tested with high precision for standard matter, but its valid…

astro-ph.CO2026

Testing the Equivalence Principle in Galaxy Clusters

Enea Di Dio, Sveva Castello, Camille Bonvin

Clusters of galaxies have been used to measure a subtle effect predicted by Einstein: gravitational redshift. This signal encodes pristine information about our Universe, since it…

astro-ph.CO2025

Gravitational Redshift from Galaxy Clusters -- a Relativistic Approach

Enea Di Dio, Sveva Castello, Camille Bonvin

The light that we receive from clusters of galaxies is redshifted by the presence of the clusters' gravitational potential. This effect, known as gravitational redshift, was first…

astro-ph.CO2025

The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Eleonora Di Valentino, Jackson Levi Said, Adam Riess +533

The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades.…

astro-ph.CO2024

Disentangling modified gravity from a dark force with gravitational redshift

Sveva Castello, Zhuangfei Wang, Lawrence Dam +2

The standard approach to test for deviations from general relativity on cosmological scales is to combine measurements of the growth rate of structure with gravitational lensing. I…