| Equation of state and thickness of the inner crust of neutron stars F Grill, H Pais, C Providência, I Vidana, SS Avancini Physical Review C 90 (4), 045803, 2014 | 119 | 2014 |
| Quark–hadron phase transition in a neutron star under strong magnetic fields A Rabhi, H Pais, PK Panda, C Providencia Journal of Physics G: Nuclear and Particle Physics 36 (11), 115204, 2009 | 112 | 2009 |
| Exploring the nuclear pasta phase in core-collapse supernova matter H Pais, JR Stone Physical Review Letters 109 (15), 151101, 2012 | 97 | 2012 |
| Vlasov formalism for extended relativistic mean field models: The crust-core transition and the stellar matter equation of state H Pais, C Providência Physical Review C 94 (1), 015808, 2016 | 93 | 2016 |
| Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation N Alam, BK Agrawal, M Fortin, H Pais, C Providência, AR Raduta, ... Physical Review C 94 (5), 052801, 2016 | 90 | 2016 |
| What do we learn about vector interactions from GW170817? V Dexheimer, R de Oliveira Gomes, S Schramm, H Pais Journal of Physics G: Nuclear and Particle Physics 46 (3), 034002, 2019 | 69 | 2019 |
| Light clusters, pasta phases, and phase transitions in core-collapse supernova matter H Pais, S Chiacchiera, C Providência Physical Review C 91 (5), 055801, 2015 | 57 | 2015 |
| Hyperonic stars and the nuclear symmetry energy C Providência, M Fortin, H Pais, A Rabhi Frontiers in Astronomy and Space Sciences 6, 13, 2019 | 48 | 2019 |
| CompOSE reference manual: Version 3.01, CompStar Online Supernovæ Equations of State, “harmonising the concert of nuclear physics and astrophysics”, https … CompOSE Core Team, S Typel, M Oertel, T Klähn, D Chatterjee, ... The European Physical Journal A 58 (11), 221, 2022 | 42 | 2022 |
| Correlation of the neutron star crust-core properties with the slope of the symmetry energy and the lead skin thickness H Pais, A Sulaksono, BK Agrawal, C Providência Physical Review C 93 (4), 045802, 2016 | 38 | 2016 |
| Neutron stars: From the inner crust to the core with the (extended) Nambu–Jona-Lasinio model H Pais, DP Menezes, C Providência Physical Review C 93 (6), 065805, 2016 | 36 | 2016 |
| Light clusters in warm stellar matter: explicit mass shifts and universal cluster-meson couplings H Pais, F Gulminelli, C Providência, G Röpke Physical Review C 97 (4), 045805, 2018 | 35 | 2018 |
| Effect of strong magnetic fields on the crust-core transition and inner crust of neutron stars J Fang, H Pais, S Pratapsi, S Avancini, J Li, C Providência Physical Review C 95 (4), 045802, 2017 | 33 | 2017 |
| Low density in-medium effects on light clusters from heavy-ion data H Pais, R Bougault, F Gulminelli, C Providência, E Bonnet, B Borderie, ... Physical Review Letters 125 (1), 012701, 2020 | 32 | 2020 |
| Limiting magnetic field for minimal deformation of a magnetized neutron star RO Gomes, H Pais, V Dexheimer, C Providência, S Schramm Astronomy & Astrophysics 627, A61, 2019 | 31 | 2019 |
| Phase transitions in core-collapse supernova matter at sub-saturation densities H Pais, WG Newton, JR Stone Physical Review C 90 (6), 065802, 2014 | 29 | 2014 |
| Dynamical properties of nuclear and stellar matter and the symmetry energy H Pais, A Santos, L Brito, C Providencia Physical Review C 82 (2), 025801, 2010 | 28 | 2010 |
| Full distribution of clusters with universal couplings and in-medium effects H Pais, F Gulminelli, C Providência, G Röpke Physical Review C 99 (5), 055806, 2019 | 27 | 2019 |
| Light clusters and pasta phases in warm and dense nuclear matter SS Avancini, M Ferreira, H Pais, C Providência, G Röpke Physical Review C 95 (4), 045804, 2017 | 24 | 2017 |
| Warm unstable asymmetric nuclear matter: Critical properties and the density dependence of the symmetry energy N Alam, H Pais, C Providência, BK Agrawal Physical Review C 95 (5), 055808, 2017 | 22 | 2017 |
