activity
20092026
most citedEquation of state and thickness of the inner crust of neutron stars

134 citations · 1.1k across the 54 of their papers we have counts for

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47 papers · 1 filter

nucl-th2026

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…

nucl-th2025

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…

nucl-th2025★ 9 cited

Inferring the Equation of State from Neutron Star Observables via Machine Learning

N. K. Patra, Tuhin Malik, Helena Pais +3

We have conducted an extensive study using a diverse set of equations of state (EoSs) to uncover strong relationships between neutron star (NS) observables and the underlying EoS p…

nucl-th2025★ 1 cited

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…

nucl-th2024★ 4 cited

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…

nucl-th2024★ 1 cited

Assessing the joint effect of temperature and magnetic field on the neutron star equation of state

Luigi Scurto, Valéria Carvalho, Helena Pais +1

In this work, we study the effect of strong magnetic fields on the equation of state (EoS) of warm, homogeneous, Neutron Star (NS) matter in beta equilibrium. NS matter is describe…