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\section*{Books}

\subsection*{Chapters of Books}

\item[1] ``Comparison of equation of state models with different cluster dissolution mechanisms'', Helena Pais and Stefan Typel, Chapter 4 of Nuclear Particle Correlations and Cluster Physics, edited W. U. Schroder, World Scientific (2017) (eprint arXiv:1612.07022 [nucl-th]) (2017).

\section*{Papers}

\subsection*{International Journals}

\item[2] ``Isoscaling in dilute warm nuclear systems'', A Rebillard-Soulie, R Bougault, H Pais, B Borderie, A Chbihi, C Ciampi, Q Fable, J Frankland, E Galichet, T Genard, D Gruyer, N Le Neindre, I Lombardo, O Lopez, L Manduci, M Parlog, G Verde, J. Phys. G {\bf 51 (1)}, 015104 (2024).

\item[3] ``Influence of the tetraneutron on the EoS under core-collapse supernovae and heavy-ion collisions conditions'', Helena Pais, C. Albertus, MA Pérez-García, Constança Providência, Astron.Astrophys. {\bf 679}, A113 (2023).

\item[4] ``Strong magnetic fields and pasta phases reexamined'', Luigi Scurto, Helena Pais, Francesca Gulminelli, Phys. Rev. C {\bf 107}, 045806 (2023).

\item[5] ``Employing ternary fission of 242Pu as a probe of very neutron-rich matter'', JB Natowitz, H Pais, G Ropke, Phys. Rev. C {\bf 107(1)}, 014618 (2023).

\item[6] ``Landau parameters and entrainment matrix of cold stellar matter: effect of the symmetry energy and strong magnetic fields'', Helena Pais, Oleksii Ivanytskyi, Constança Providência, J. Cosmol. Astropart. Phys. {\bf 04, 024}, 024 (2022).

\item[7] ``Delta baryons in neutron stars'', Kauan D. Marquez, Débora P. Menezes, Helena Pais, Constança Providência, Phys. Rev. C {\bf 106}, 055801 (2022).

\item[8] ``Heavy baryons in hot stellar matter with light nuclei and hypernuclei'', Tiago Custódio, Helena Pais, Constança Providência, Phys. Rev. C {\bf 105}, 065803 (2022).

\item[9] ``Inner crust equations of state for CompOSE'', Tuhin Malik, Helena Pais, Eur. Phys. J. A {\bf 58}, 154 (2022).

\item[10] ``CompOSE reference manual'', S Typel, M Oertel, T Klahn, D Chatterjee, V Dexheimer, C Ishizuka, M Mancini, J Novak, H Pais, C Providencia, AR Raduta, M Servillat, L Tolos, Eur. Phys. J. A {\bf 58(11)}, 221 (2022).

\item[11] ``Pasta phases in neutron stars under strong magnetic fields'', Xiaopeng Wang, Jing Li, Jianjun Fang, Helena Pais, Constança Providência, Phys. Rev. D {\bf 105}, 063004 (2022).

\item[12] ``A Nonequilibrium Information Entropy Approach to Ternary Fission of Actinides'', G. Röpke, J. B. Natowitz, H. Pais, Phys. Rev. C {\bf 103}, L061601 (2021).

\item[13] ``Strong magnetic fields: neutron stars with an extended inner crust'', Helena Pais, Bruno Bertolino, Jianjun Fang, Xiaopeng Wang, Constança Providência, Eur. Phys. J. A {\bf 57}, 193-1-193-9 (2021).

\item[14] ``Critical properties of calibrated relativistic mean-field models for the transition to warm, nonhomogeneous nuclear and stellar matter'', Olfa Boukari, Helena Pais, Sofija Antić, Constança Providência, Phys. Rev. C {\bf 103}, 055804 (2021).

\item[15] ``Binding energy shifts from heavy-ion experiments in a nuclear statistical equilibrium model'', S. Mallik, H. Pais, F. Gulminelli, Eur. Phys. J. A {\bf 27}, 262 (2021).

\item[16] ``Light hyperclusters and hyperons in low-density hot stellar matter'', Tiago Custódio, Helena Pais, Constança Providência, Phys. Rev. C {\bf 104}, 035801 (2021).

\item[17] ``Light element (Z=1,2) production from spontaneous ternary fission of $^{252}$Cf'', G. R\"opke, J.\,B. Natowitz, H. Pais, Eur. Phys. J. A {\bf 56}, 238 (2020).

\item[18] ``Improved method for the experimental determination of in-medium effects from heavy-ion collisions'', Helena Pais, Rémi Bougault, Francesca Gulminelli, Constança Providência et al, J. Phys. G: Nucl. Part. Phys. {\bf 47}, 105204 (2020).

\item[19] ``Low-density in-medium effects on light clusters from heavy-ion data'', Helena Pais, Rémi Bougault, Francesca Gulminelli, Constança Providência, et al, Phys. Rev. Lett. {\bf 125}, 012701 (2020).

\item[20] ``Neutron star inner crust: Effects of rotation and magnetic fields'', Ivo Sengo, Helena Pais, Bruno Franzon, Constança Providência, Phys. Rev. D {\bf 102}, 063013 (2020).

\item[21] ``Isotopic equilibrium constants for very low-density and low-temperature nuclear matter'', J. B. Natowitz, H. Pais, G. Roepke, J. Gauthier, K. Hagel, M. Barbui, R. Wada, Phys. Rev. C {\bf 102}, 064621 (2020).

\item[22] ``Light clusters in warm stellar matter: calibrating the cluster couplings'', Tiago Custódio, Alexandre Falcão, Helena Pais, Constança Providência, Francesca Gulminelli, Gerd Roepke, European Physical Journal A {\bf 56}, 295 (2020).

\item[23] ``Hyperonic Stars and the Nuclear Symmetry Energy'', Constança Providência, Morgane Fortin, Helena Pais, Aziz Rabhi, Front. Astron. Space Sci {\bf 6} (2019).

\item[24] ``Full distribution of clusters with universal couplings and in-medium effects'', Helena Pais, Francesca Gulminelli, Constança Providência, Gerd Röpke, Phys. Rev. C {\bf 99}, 055806 (2019).

\item[25] ``Limiting magnetic field for minimal deformation of a magnetised neutron star'', R. O. Gomes, H. Pais, V. Dexheimer, C. Providência, S. Schramm, Astronomy \& Astrophysics Journal {\bf 627}, A61 (2019).

\item[26] ``What do we learn about vector interactions from GW170817?'', Veronica Dexheimer, Rosana de Oliveira Gomes, Stefan Schramm, Helena Pais, J. Phys. G: Nucl. Part. Phys. {\bf 46}, 034002 (2019).

\item[27] ``Light clusters in warm stellar matter: explicit mass shifts and universal cluster-meson couplings'', Helena Pais, Francesca Gulminelli, Constança Providência, Gerd Röpke, Phys. Rev. C {\bf 97}, 045805 (2018).

\item[28] ``Stability of the neutron-proton-electron matter under strong magnetic fields: The covariant Vlasov approach'', Sidney Avancini, B. P. Bertolino, Aziz Rabhi, Jianjun Fang, Helena Pais, and Constança Providência, Phys. Rev. C {\bf 98}, 025805 (2018).

\item[29] ``Crust-core transition of a neutron star: effects of the symmetry energy and temperature under strong magnetic fields'', Jianjun Fang, Helena Pais, Sagar Pratapsi, Constança Providência, Phys. Rev. C 95 (Rapid Communication) {\bf 95}, 062801 (2017).

\item[30] ``Effect of strong magnetic fields on the crust-core transition and inner crust of neutron stars'', Jianjun Fang, Helena Pais, Sagar Pratapsi, Sidney Avancini, Jing Li, Constança Providência, Phys. Rev. C {\bf 95}, 045802 (2017).

\item[31] ``Warm unstable asymmetric nuclear matter: critical properties and the density dependence of the symmetry energy'', N. Alam, H. Pais, C. Providência, B. K. Agrawal, Phys. Rev. C {\bf 95}, 055808 (2017).

\item[32] ``Light Clusters and Pasta Phases in Warm and Dense Nuclear Matter'', Sidney S. Avancini, Márcio Ferreira, Helena Pais, Constança Providência, Gerd Röpke., Phys. Rev. C {\bf 95}, 045804 (2017).

\item[33] ``Correlation of the neutron star crust-core properties with the slope
of the symmetry energy and the lead skin thickness'', H. Pais, A. Sulaksono, B. K. Agrawal, C. Providência, Phys. Rev. C {\bf 93}, 045802 (2016).

\item[34] ``Neutron stars: From the inner crust to the core with the (extended) Nambu–Jona-Lasinio model'', Helena Pais, Débora P.  Menezes, Constança Providência, Phys. Rev. C {\bf 93}, 065805 (2016).

\item[35] ``The Vlasov formalism for extended relativistic mean field models: the crust-core transition and the stellar matter equation of state'', Helena Pais, Constança Providência, Phys. Rev. C {\bf 94}, 015808 (2016).

\item[36] ``Larger and more heterogeneous neutron star crusts: A result of strong magnetic fields'', Jianjun Fang, Helena Pais, Sidney Avancini, and Constança Providência, Phys. Rev. C {\bf 94}, 062801(R) (2016).

\item[37] ``Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation'', N. Alam, B. K. Agrawal, M. Fortin, H. Pais, C. Providência, Ad. R. Raduta, A. Sulaksono, Phys. Rev. C {\bf 94}, 052801(R) (2016).

\item[38] ``Light clusters, pasta phases and phase transitions in core-collapse supernova matter'', Helena Pais, Silvia Chiacchiera, Constança Providência, Phys. Rev. C 91, 055801 (2015).

\item[39] ``Equation of state and thickness of the inner crust of neutron stars'', Fabrizio Grill, Helena Pais, Constança Providência, Isaac Vidaña, Sidney S. Avancini, Phys. Rev. C {\bf 90}, 045803 (2014).

\item[40] ``Phase transitions in core-collapse supernova matter at sub-saturation densities'', Helena Pais, William G. Newton, and Jirina R. Stone, Phys. Rev. C {\bf 90}, 065802 (2014).

\item[41] ``Exploring the Nuclear Pasta Phase in Core-Collapse Supernova Matter'', Helena Pais and Jirina R. Stone, Physical Review Letters {\bf 109}, 151101 (2012).

\item[42] ``Dynamical properties of nuclear and stellar matter and the symmetry energy'', Helena Pais, Alexandre Santos, L. Brito and C. Providência, Physical Review C {\bf 82}, 025801 (2010).

\item[43] ``Quark-hadron phase transition in a neutron star under strong magnetic fields'', A. Rabhi, H. Pais, P. K. Panda, C. Providência, J. Phys. G {\bf 36}, 115204 (2009).

\item[44] ``Dynamical instabilities of warm npe matter: \δ meson effects'', Helena Pais, Alexandre Santos, and Constança Providência, Physical Review C {\bf 80}, 045808 (2009).

\section*{Proceedings}

\subsection*{International Conferences}

\item[45] ``Física Nuclear nas Estrelas'', Ivo Sengo, Helena Pais, Constança Providência, Contribution in M. Abreu \& . N. Garcia (Eds.), Física para o desenvolvimento equilibrado – um contributo [Physics for sustainable development – a contribution] (pp. 393–400). União dos Físicos de Países de Língua Portuguesa. ISBN: 978-85-89064-34-7. (2020).

\item[46] ``Light and heavy clusters in warm stellar matter'', Helena Pais, Francesca Gulminelli, Constança Providência, Gerd Röpke, Nucl. Sci. Tech. {\bf 29}, 181 (2018).

\item[47] ``Comparison of EoS models with different cluster suppression mechanisms'', Stefan Typel, Helena Pais, Nuovo Cim. C {\bf 39}, 393 (2017).

\item[48] ``Pasta phases in core-collapse supernova matter'', Helena Pais, Silvia Chiacchiera, and Constança Providência, Journal of Physics: Conference Series {\bf 706}, 042007 (2016).

\item[49] ``Emergence of new correlations between neutron star radii and nuclear matter properties'', N. Alam, B. K. Agrawal, H. Pais, C. Providência, A. Sulaksono, DAE Symp. Nucl. Phys. 61, 900 (2016) {\bf 61}, 900 (2016).

\item[50] ``Core-collapse supernova matter: light clusters, pasta phase and phase transitions'', Helena Pais, Constança Providência, William G. Newton, and Jirina R. Stone, eprint arXiv:1503.08753 (2015).

\item[51] ``Dynamical instabilities of warm npe matter: the delta meson effects'', H. Pais, A. Santos, C. Providência, AIP Conference Proceedings {\bf 1231}, 231-232 (2010).

\section*{Communications}

\subsection*{Invited}

\item[52] ``Strong magnetic fields and the inner crust of neutron stars'', Helena Pais, Invited speaker of the workshop Strongly interacting matter in ex- treme magnetic fields held at ECT*, Trento, Italy, September 2023. (2023).

\item[53] ``Constraining the low-density neutron star equation of state from heavy-ion collisions'', Helena Pais, Invited speaker of the workshop Neutron Rich Matter on Heaven and Earth to be held at the Institute of Nuclear Theory (INT), University of Washington, Seattle, USA, June 2023. (2023).

\item[54] ``Clusters, heavy baryons and strong magnetic fields: how complex is the neutron star non-homogeneous matter?'', Helena Pais, Invited as a review speaker of the final International PHAROS Conference 2022 held at La Sapienza University in Rome, Italy. (2022).

\item[55] ``Constraining the low-density neutron star equation of state from heavy-ion collisions'', Helena Pais, Invited speaker of the NuSym22, X International Symposium on Nuclear Symmetry Energy, held in Catania, Italy, September 2022. (2022).

\item[56] ``The equation of state for warm stellar matter: light and heavy clusters'', Helena Pais, Invited lecturer at the Carpathian Summer School of Physics 2020 in 2021, held in Sinaia, Romania, August 2021. (2021).

\item[57] ``Constraining the low-density neutron star equation of state from heavy-ion collisions'', Helena Pais, Invited for a review talk on the “Nuclear dynamics and thermodynamics” session of the GANIL Colloque 2021, held in Autrans-M ́eaudre en Vercors, France. (2021).

\item[58] ``Light clusters and pasta phases in warm stellar matter'', Helena Pais, Invited talk at the "Light clusters and nuclei and nuclear matter: Nuclear structure and decay, heavy ion collisions, and astrophysics" ECT* Workshop, Trento, Italy, September 4 (2019).

\item[59] ``Neutron Star Crust: open questions'', Helena Pais, Invited as a discussion moderator on the neutron star crust re-
search topic at the Investigating Crust of Neutron Stars (ICONS 2019) Workshop, Amsterdam, The Netherlands, April 17. (2019).

\item[60] ``Light clusters and pasta phases in warm stellar matter'', Helena Pais, Invited talk at the Department of Physics, Kent State University, Kent, OH, USA, December 4 (2019).

\item[61] ``The crust-core transition and the stellar matter equation of state'', Helena Pais, Invited talk given at the Department of Physics and Astronomy, University of Tennessee, Knoxville, TN, USA, January 24th (2018).

\item[62] ``Light and heavy clusters in warm stellar matter'', Helena Pais, Invited talk given at the International workshop on nuclear dynamics in heavy-ion reactions (IWND 2018), Huzhou, Zhejiang, China, June 12th (2018).

\item[63] ``Light and heavy clusters in warm stellar matter'', Helena Pais, Invited talk given at the Women in Nuclear and Hadron Theoretical Physics: the last frontier (WTPLF 2018), Genova, Italy, December 11. (2018).

\item[64] ``The crust-core transition and the stellar matter equation of state'', Helena Pais, Invited talk given at GANIL, Caen, France, April 20th (2018).

\item[65] ``The crust-core transition and the stellar matter equation of state'', Helena Pais, Invited talk given at the Department of Physics, Faculty of Science, University of Zagreb, Zagreb, Croatia, December 21st (2017).

\item[66] ``The crust-core transition and the stellar matter equation of state'', Helena Pais, Invited talk given at the Physics Department, Qufu Normal University, Shandong, China, June 21st. (2017).

\subsection*{Oral}

\item[67] ``Light and heavy clusters in warm stellar matter'', Helena Pais, Talk given at the ICONS: Investigating Crusts of Neutron Stars, Amsterdam, The
Netherlands, April 15-17 (2019).

\item[68] ``Light and heavy clusters in warm stellar matter'', Helena Pais, Talk given at the PHAROS Working Group Meeting WWG1+WG2, Coimbra, Portugal, September 26-28 (2018).

\item[69] ``The crust-core transition and the stellar matter equation of state'', Helena Pais, Talk given at the Annual NewCompStar Conference 2017, Warsaw, Poland, March 27-31 (2017).

\item[70] ``The crust-core transition and the stellar matter equation of state'', Helena Pais, Talk given at the Nuclear Physics, Compact Stars, and Compact Stars Mergers (NPCSM 2016) long-term Workshop, Yukawa Institute for Theoretical physics, Kyoto, Japan (2016).

\item[71] ``Pasta phases in core-collapse supernova matter'', Helena Pais, Talk given at the XIII International Workshop on Hadron Physics (XIII Hadron Physics), Angra dos Reis, RJ, Brazil, March 22 - 27 (2015).

\item[72] ``The nuclear pasta phase'', Helena Pais, Talk given at Mini-workshop do Grupo Fisica Hadronica, Department of Physics, Federal University of Santa Catarina, Florianopolis, Brazil, April 22 (2015).

\item[73] ``Pasta phases in core-collapse supernova matter'', Helena Pais, Talk given at the Annual NewCompStar Conference 2015, Budapest, Hungary, June 15-19 (2015).

\item[74] ``Core-collapse supernova matter: light clusters, pasta phases and phase transitions'', Helena Pais, Talk given at the Nuclear Equation of State for Compact Stars and Supernovae (NEOS2014) Workshop, Frankfurt Institute for Advanced Studies (FIAS), Germany, December 3 - 5 (2014).

\item[75] ``Core-collapse supernova matter: light clusters, pasta phases and phase transitions'', Helena Pais, Talk given at the Compact Stars in the QCD Phase Diagram IV Workshop, Prerow, Germany, September 26 - 29 (2014).

\item[76] ``Nuclear pasta phase in core-collapse supernova matter'', Helena Pais, Talk given at the NewCompStar 2014 Conference, “The Structure and Signals of Neutron Stars, from Birth to Death”, Florence, Italy, March 24-28 (2014).

\item[77] ``3D EoS for supernovae and neutron stars simulations: the transition between uniform and non-uniform matter'', Helena Pais, Talk given at the CompStar2011 School and Workshop, “Gravitational Waves and Electromagnetic Radiation from Compact Stars”, Catania, Italy, 3-12 May (2011).

\subsection*{Poster}

\item[78] ``The Liquid-gas phase transition with the temperature-dependent DD-NLD model'', S. Antic, H. Pais, S. Typel, and C. Providência, Annual NewCompStar School 2016, Coimbra, Portugal (2016).

\item[79] ``3D EoS for SN and NS simulations: the phase transition between uniform and non-uniform matter'', Helena Pais, Jirina R. Stone, William G. Newton, International Workshop on Baryon and Lepton Number Violation, Gatlinburg, TN, USA, September 22-24 (2011).

\item[80] ``Dynamical instabilities of warm npe matter: the \δ meson effects'', Helena Pais, Alexandre Santos, Constança Providência, International Scientific Meeting on Nuclear Physics: “Basic concepts in Nuclear Physics: theory, experiments and applications”, La Rabida (Huelva), Spain, July 4-10 (2009).

\item[81] ``Quark stars in a strong magnetic field'', Helena Pais, Constança Providência, Aziz Rabhi, CompStar2009 Workshop, “The New Physics of Compact Stars”, Coimbra, Portugal, February 5-13 (2009).

\section*{Thesis}

\subsection*{PhD thesis}

\item[82] ``Three Dimensional Equation of State for Core-Collapse Supernova Matter'', Helena Pais  (supervisor Jirina R. Stone), PhD thesis, University of Tennessee - Knoxville (2013).

\subsection*{MSc thesis}

\item[83] ``Estrelas de quarks num campo magnético forte'', Helena Pais  (supervisor Constança Providência), MSc thesis, University of Coimbra (2008).

\end{itemize}
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