619 citations
- Centre National de la Recherche ScientifiqueFR423 papers
- École Nationale Supérieure d'Ingénieurs de CaenFR351 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR331 papers
- Université de Caen NormandieFR210 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR184 papers
- Grand Accélérateur National d'Ions LourdsFR182 papers
- Université Paris-SudFR92 papers
- Horia Hulubei National Institute for R and D in Physics and Nuclear EngineeringRO74 papers
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- Institut Pluridisciplinaire Hubert CurienFR60 papers
101 papers · 1 filter
Probing the density dependence of nuclear symmetry energy through isospin transport in heavy-ion reactions
S. Mallik, F. Gulminelli, C. Ciampi +1
The density dependence of the nuclear symmetry energy remains one of the key uncertainties in contemporary nuclear physics, with significant implications for the structure of exoti…
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…
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…
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…
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…
Role of the Meson in the Equation of State an Direct Urca Cooling of Neutron Stars
Luigi Scurto, Helena Pais, Marco Antonelli +1
The direct Urca (dUrca) process is a key mechanism driving rapid neutrino cooling in neutron stars, with its baryon density activation threshold determined by the microscopic model…