402 citations · 4.2k across the 129 of their papers we have counts for
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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,…
Generalised description of Neutron Star matter with nucleonic Relativistic Density Functional
Prasanta Char, Chiranjib Mondal, Francesca Gulminelli +1
In this work, we propose a meta-modelling technique to nuclear matter on the basis of a relativistic density functional with density-dependent couplings. Identical density dependen…
Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers
C. Mondal, M. Antonelli, F. Gulminelli +3
Possible strong first-order hadron-quark phase transitions in neutron star interiors leave an imprint on gravitational waves, which could be detected with planned third-generation…
The proto-neutron star inner crust in the liquid phase
H. Dinh Thi, A. F. Fantina, F. Gulminelli
The crust of a neutron star is known to melt at a temperature that increases with increasing matter density, up to about K. At such high temperatures and beyond, the crus…