46 citations · 135 across the 22 of their papers we have counts for
22 papers
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…
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…
Emulator-Assisted Nuclear DFT Inference and Its Consequences for the Structure of Neutron Stars
Pietro Klausner, Marco Antonelli, Gianluca Colò +3
Nuclear density functional theory provides a unified description of finite nuclei and bulk nuclear matter, and is widely used to model the neutron star equation of state. However,…
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…
Advanced Virgo Plus for O5 -- Design Report Overview
F. Acernese, A. Agapito, D. Agarwal +578
This document presents an overview of the design, implementation, and expected performance of the Advanced Virgo Plus (AdV+) upgrades in view of the O5 observing run. Following the…
Medium effects on light clusters from heavy-ion collisions within a relativistic mean-field description
Tiago Custódio, Francesca Gulminelli, Alex Rebillard-Soulié +5
Central XeSn collisions from INDRA data are analysed using a Bayesian inference on light nuclei multiplicities to estimate the thermodynamical parameters a…
ESO Expanding Horizon White Paper: Revealing the properties of matter at supranuclear densities with gravitational waves
Tim Dietrich, Tanja Hinderer, Micaela Oertel +40
Understanding dense matter under extreme conditions is one of the most fundamental puzzles in modern physics. Complex interactions give rise to emergent, collective phenomena. Whil…
Nuclear parameter inference with semi-agnostic priors
Lami Suleiman, Anthea F. Fantina, Francesca Gulminelli +1
Radio pulsar timing, X-ray pulse profile modeling, and gravitational-wave detections of binary mergers involving at least one neutron star probe the properties of dense, neutron-ri…
Properties of neutron stars with hyperons within a generalized relativistic approach
Prasanta Char, Chiranjib Mondal, Timothé Alezraa +2
In this work, we study the effects of -hyperons on neutron star properties employing a generalized relativistic framework for the equation of state (EOS). Different choices for…
Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2
P. J. Davis, H. Dinh Thi, A. F. Fantina +3
The equation of state (EoS) is a needed input to determine the neutron-star global properties and to relate them. It is thus important to provide consistent and unified EoSs to avo…
Dense Matter in Neutron Stars with eXTP
Ang Li, Anna L. Watts, Guobao Zhang +82
In this White Paper, we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission to constrain the equation of state of dense matter in neutron stars, explo…
Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model
S. Burrello, F. Gulminelli, M. Antonelli +2
Accurate modeling of the neutron star crust is essential for interpreting multimessenger observations and constraining the nuclear equation of state (EoS). However, standard phenom…
Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches
Guilherme Grams, Nikolai N. Shchechilin, Théau Diverrès +3
We investigate the effects of temperature on the properties of the inner crust of a non-accreting neutron star. To this aim, we employ two different treatments: the compressible li…
Properties of the neutron star crust informed by nuclear structure data
Pietro Klausner, Marco Antonelli, Francesca Gulminelli
We perform a Bayesian analysis of the neutron star (NS) equation of state (EoS) based on a wide set of Skyrme functionals, derived from previous nuclear physics inferences. The nov…
Light clusters as a possible source of crustal impurities: a quasi-particle approach
Helena Pais, Hoa Dinh-Thi, Anthea F. Fantina +2
The presence of impurities in the neutron star crust is known to affect in an important way the thermal and electrical conductivity of the star. In this work, we explore the possib…
Strongly interacting matter in extreme magnetic fields
Prabal Adhikari, Martin Ammon, Sidney S. Avancini +58
Magnetic fields are ubiquitous across different physical systems of current interest; from the early Universe, compact astrophysical objects and heavy-ion collisions to condensed m…
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…
Calibrating the medium effects of light clusters in heavy-ion collisions
Tiago Custódio, Alex Rebillard-Soulié, Rémi Bougault +5
We propose a Bayesian inference estimation of in-medium modification of the cluster self-energies from light nuclei multiplicities measured in selected samples of central $^{136,12…
Inference of neutron-star properties with unified crust-core equations of state for parameter estimation
P. J. Davis, H. Dinh Thi, A. F. Fantina +3
Relating different global neutron-star (NS) properties, such as tidal deformability and radius, or mass and radius, requires an equation of state (EoS). Determining the NS EoS is t…
General predictions of neutron star properties using unified relativistic mean-field equations of state
Luigi Scurto, Helena Pais, Francesca Gulminelli
In this work we present general predictions for the static observables of neutron stars (NSs) under the hypothesis of a purely nucleonic composition of the ultra-dense baryonic mat…
Nuclear physics inputs for dense-matter modelling in neutron stars. The nuclear equation of state
A. F. Fantina, F. Gulminelli
In this contribution, we briefly present the equation-of-state modelling for application to neutron stars and discuss current constraints coming from nuclear physics theory and exp…
Crystallization of the inner crust of a neutron star and the influence of shell effects
T. Carreau, F. Gulminelli, N. Chamel +2
Context. In the cooling process of a non-accreting neutron star, the composition and properties of the crust are thought to be fixed at the finite temperature where nuclear reactio…