activity
20242026
collaborators

5 papers

gr-qc2026

Looking for non-gaussianity in Pulsar Timing Arrays through the four point correlator

Adrien Kuntz, Clemente Smarra, Massimo Vaglio

Pulsar Timing Arrays have recently reported strong evidence for a stochastic gravitational wave background. In standard analyses, it is modeled through pulsar-dependent Fourier coe…

gr-qc2025

Searching for Gravitational Waves with Gaia and its Cross-Correlation with PTA: Absolute vs Relative Astrometry

Massimo Vaglio, Mikel Falxa, Giorgio Mentasti +5

Astrometric missions like Gaia provide exceptionally precise measurements of stellar positions and proper motions. Gravitational waves traveling between the observer and distant st…

gr-qc2025

Systematic bias in LISA ringdown analysis due to waveform inaccuracy

Lodovico Capuano, Massimo Vaglio, Rohit S. Chandramouli +3

Inaccurate modeling of gravitational-wave signals can introduce systematic biases in the inferred source parameters. As detector sensitivities improve and signals become louder, mi…

gr-qc2025

Probing supermassive black hole scalarization with Pulsar Timing Arrays

Clemente Smarra, Lodovico Capuano, Adrien Kuntz

Scalar-tensor theories with a scalar field coupled to the Gauss-Bonnet invariant can evade no-hair theorems and allow for non-trivial scalar profiles around black holes. This coupl…

gr-qc2024

Scalar emission from neutron star-black hole binaries in scalar-tensor theories with kinetic screening

Ramiro Cayuso, Adrien Kuntz, Miguel Bezares +1

We explore scalar radiation from neutron star-black hole binaries in scalar-tensor theories with kinetic screening (-essence). Using 3+1 numerical relativity simulations in the…