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

collaborators
Showing 2020Show all

6 papers · 1 filter

nucl-th2020

A Nonequilibrium Information Entropy Approach to Ternary Fission of Actinides

G. Röpke, J. B. Natowitz, H. Pais

Ternary fission of actinides probes the state of the nucleus at scission. Light clusters are produced in space and time very close to the scission point. Within the nonequilibrium…

nucl-ex2020★ 6 cited

Isotopic equilibrium constants for very low-density and low-temperature nuclear matter

J. B. Natowitz, H. Pais, G. Roepke +4

Yields of equatorially emitted light isotopes, , observed in ternary fission in the reaction Pu(,f) are employed to determine apparent chemical eq…

nucl-th2020★ 12 cited

Light clusters in warm stellar matter: calibrating the cluster couplings

Tiago Custódio, Alexandre Falcão, Helena Pais +3

The abundances of light clusters within a formalism that considers in-medium effects are calculated using several relativistic mean-field models, with both density-dependent and de…

nucl-th2020★ 6 cited

Critical properties of calibrated relativistic mean-field models for the transition to warm, non-homogeneous nuclear matter

Olfa Boukari, Helena Pais, Sofija Antić +1

The critical properties for the transition to warm, asymmetric, non-homogeneous nuclear matter are analysed within a thermodynamical spinodal approach for a set of well calibrated…

nucl-th2020★ 13 cited

Improved method for the experimental determination of in-medium effects from heavy-ion collisions

Helena Pais, Rémi Bougault, Francesca Gulminelli +13

The equation of state with light clusters for nuclear and stellar matter is determined using chemical equilibrium constants evaluated from the analysis of the recently published (X…

nucl-th2020★ 10 cited

Neutron star inner crust: effects of rotation and magnetic fields

Ivo Sengo, Helena Pais, Bruno Franzon +1

We study the role of the pasta phases on the properties of rotating and magnetized neutron stars. In order to investigate such systems, we make use of two different relativistic me…