most citedFrozen and -equilibrated and modes of cold neutron stars: nuclear metamodel predictions

11 citations · 11 across the 6 of their papers we have counts for

collaborators

6 papers

nucl-th2026

Ruling out nucleonic direct Urca cooling in low-mass neutron stars using nuclear data

Gabriele Montefusco, Pietro Klausner, Marco Antonelli +3

Connecting nuclear experiments to neutron star composition requires controlling the extrapolation of experimental information beyond the densities probed in the laboratory. We comb…

cond-mat.supr-con2026

Fluxtube Bouquets and Type-1.5 Clustering in Superfluid Neutron Star Cores

Adarsh Karekkat, Gabriele Montefusco, Marco Antonelli

We study mesoscopic configurations of a neutron superfluid coupled to a proton superconductor in the outer core of a neutron star. The condensates are described by a two-component…

gr-qc2026

Advanced Virgo during the LIGO-Virgo-KAGRA fourth observing run

Virgo Collaboration, F Acernese, A Agapito +546

From April 10, 2024 to November 18, 2025 Advanced Virgo participated in the fourth observing run of the network of gravitational-wave detectors, together with Advanced LIGO and KAG…

astro-ph.HE2026

Bayesian analysis of the shear modulus in the neutron-star crust

T. Diverrès, G. Montefusco, A. F. Fantina +1

The elastic properties of the neutron-star crust are important for the calculations of crustal modes. In particular, the ability of the crust to support shear stresses has been con…

nucl-th2026

An Asymptotically Causal Metamodel for Neutron Star Equations of State

Gabriele Montefusco, Marco Antonelli, Francesca Gulminelli

Nuclear metamodels - phenomenological parametrizations of the energy of nuclear matter - are convenient tools to explore the space of realistic neutron star configurations constrai…

nucl-th2024★ 11 cited

Frozen and -equilibrated and modes of cold neutron stars: nuclear metamodel predictions

Gabriele Montefusco, Marco Antonelli, Francesca Gulminelli

When the chemical re-equilibration timescale is sufficiently long, the normal and quasi-normal mode frequencies of neutron stars should be calculated in the idealized limit that th…