collaborators

5 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

Cosmology with HI Intensity Mapping

Laura Wolz, Gabriele Autieri, José Luis Bernal +18

The redshifted spectral emission from neutral hydrogen (HI) at rest wavelength 21 cm can be used as a tracer of large-scale structure and its evolution. Within the HI intensity map…

astro-ph.CO2026

The impact of evolving dark energy on the Weyl potential measured from the Dark Energy Survey Year 3 data

Benedetta Rosatello, Gen Ye, Maria Berti +3

Measurements from the Dark Energy Survey (DES) Year 3 data have shown that the Weyl potential -- the sum of the spatial and temporal distortions of the geometry -- evolves more slo…

astro-ph.CO2025

Weighing neutrinos with 21cm Intensity Mapping at the SKAO

Gabriele Autieri, Maria Berti, Marta Spinelli +2

We explore the constraining power of future 21cm intensity mapping (IM) observations at the SKAO, focusing primarily on the sum of neutrino masses, . We forecast observatio…

astro-ph.CO2025

Reconstructing the dark energy density in light of DESI BAO observations

Maria Berti, Emilio Bellini, Camille Bonvin +3

In light of the evidence for dynamical dark energy (DE) found from the most recent Dark Energy Spectroscopic Instrument (DESI) baryon acoustic oscillation (BAO) measurements, we pe…