collaborators

10 papers

astro-ph.CO2026

CMB Constraints on Pre-Inflationary Axion Dark Matter Isocurvature

Catherine Petretti, Praniti Singh, Matteo Braglia +3

Although measurements of the Cosmic Microwave Background (CMB) are consistent with a nearly scale-invariant primordial spectrum of adiabatic perturbations, in which the energy dens…

astro-ph.HE2025

Search for continuous gravitational waves from known pulsars in the first part of the fourth LIGO-Virgo-KAGRA observing run

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1816

Continuous gravitational waves (CWs) emission from neutron stars carries information about their internal structure and equation of state, and it can provide tests of General Relat…

astro-ph.CO2025

Exotic Dark Matter and the DESI Anomaly

Matteo Braglia, Xingang Chen, Abraham Loeb

Exotic dark matter (EDM) refers to a dark matter species whose equation of state deviates from zero at late times. This behavior enables it to model a variety of non-standard late-…

astro-ph.CO2025

What it takes to solve the Hubble tension through scale-dependent modifications of the primordial power spectrum

Nanoom Lee, Matteo Braglia, Yacine Ali-Haïmoud

We investigate scale-dependent modifications to the primordial scalar power spectrum as potential solutions to the Hubble tension. We use the Fisher-bias formalism, recently adapte…

astro-ph.CO2025

Investigating the Origin of CMB Large-Scale Features Using LiteBIRD and CMB-S4

Catherine Petretti, Matteo Braglia, Xingang Chen +2

Several missions following Planck are currently under development, which will provide high-precision measurements of the Cosmic Microwave Background (CMB) anisotropies. Specificall…

astro-ph.CO2025

Reconstructing Primordial Curvature Perturbations via Scalar-Induced Gravitational Waves with LISA

Jonas El Gammal, Aya Ghaleb, Gabriele Franciolini +17

Many early universe scenarios predict an enhancement of scalar perturbations at scales currently unconstrained by cosmological probes. These perturbations source gravitational wave…