402 citations · 4.2k across the 129 of their papers we have counts for
131 papers
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…
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…
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…
Light clusters in the liquid proto-neutron star inner crust
H. Dinh Thi, A. F. Fantina, F. Gulminelli
Being born hot from core-collapse supernova, the crust of the proto-neutron star is expected to be made of a Coulomb liquid and composed of an ensemble of different nuclear species…
The proto-neutron star inner crust in a multi-component plasma approach
H. Dinh Thi, A. F. Fantina, F. Gulminelli
Proto-neutron stars (PNS) are born hot, with temperatures exceeding a few times K. In these conditions, the PNS crust is expected to be made of a Coulomb liquid composed…
Nuclear physics constraints from binary neutron star mergers in the Einstein Telescope era
Francesco Iacovelli, Michele Mancarella, Chiranjib Mondal +5
The next generation of ground-based gravitational-wave detectors, Einstein Telescope (ET) and Cosmic Explorer (CE), present a unique opportunity to put constraints on dense matter,…