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Issue DateTitleAuthor(s)TypeAccess
117-Oct-2014Equation of state and thickness of the inner crust of neutron starsGrill, F. ; Pais, H. ; Providência, C. ; Vidaña, I. ; Avancini, S. S. articleopenAccess
22-Dec-2014Phase transitions in core-collapse supernova matter at sub-saturation densitiesPais, H. ; Newton, W. G. ; Stone, J. R. articleopenAccess
313-Jun-2017Crust-core transition of a neutron star: Effects of the symmetry energy and temperature under strong magnetic fieldsFang, J. ; Pais, H. ; Pratapsi, S. ; Providência, C. articleopenAccess
4Apr-2017Effect of strong magnetic fields on the crust-core transition and inner crust of neutron starsFang, J. ; Pais, H. ; Pratapsi, S. ; Avancini, S. ; Li, J. ; Providência, C. articleopenAccess
59-Nov-2016Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturationAlam, N. ; Agrawal, B. K. ; Fortin, M. ; Pais, H. ; Providência, C. ; Raduta, Ad. R. ; Sulaksono, A. articleopenAccess
623-May-2017Warm unstable asymmetric nuclear matter: Critical properties and the density dependence of the symmetry energyAlam, N. ; Pais, H. ; Providência, C. ; Agrawal, B. K. articleopenAccess
720-Apr-2017Light clusters and pasta phases in warm and dense nuclear matterAvancini, S. S. ; Ferreira, M. ; Pais, H. ; Providência, C. ; Röpke, G. articleopenAccess
87-May-2015Light clusters, pasta phases, and phase transitions in core-collapse supernova matterPais, H. ; Chiacchiera, S. ; Providência, C. articleopenAccess
923-Jun-2021Light hyperclusters and hyperons in low-density hot stellar matterCustódio, Tiago; Pais, Helena ; Providência, Constança preprintopenAccess
107-Dec-2016Larger and more heterogeneous neutron star crusts: A result of strong magnetic fieldsFang, J. ; Pais, H. ; Avancini, S. ; Providência, C. articleopenAccess
1129-Jul-2016Vlasov formalism for extended relativistic mean field models: The crust-core transition and the stellar matter equation of statePais, H. ; Providência, C. articleopenAccess
127-Apr-2016Correlation of the neutron star crust-core properties with the slope of the symmetry energy and the lead skin thicknessPais, H. ; Sulaksono, A. ; Agrawal, B. K. ; Providência, C. articleopenAccess
138-Jun-2016Neutron stars: From the inner crust to the core with the (extended) Nambu–Jona-Lasinio modelPais, H. ; Menezes, D. P. ; Providência, C. articleopenAccess
142-Nov-2018Hyperonic stars and the symmetry energyProvidência, Constança ; Fortin, Morgan; Pais, Helena ; Rabhi, Aziz articleopenAccess
154-Apr-2018Light clusters in warm stellar matter: explicit mass shifts and universal cluster-meson couplingsPais, Helena ; Gulminelli, Francesca ; Providência, Constança ; Ropke, Gerd articleopenAccess
1629-Aug-2018Stability of the neutron-proton-electron matter under strong magnetic fields: The covariant Vlasov approachAvancini, Sidney ; Bertolino, B. P. ; Rabhi, Aziz ; Fang, Jianjun ; Pais, Helena ; Providência, Constança articleopenAccess
1719-Dec-2022Strong magnetic fields and pasta phases revisitedScurto, Luigi ; Pais, Helena ; Gulminelli, FrancescaarticleopenAccess
1824-Nov-2022Employing ternary fission of Pu 242 as a probe of very neutron-rich matterNatowitz, J. B.; Pais, H. ; Röpke, G.articleopenAccess
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