\documentclass{article} \usepackage[latin1]{inputenc} \usepackage{fullpage} \begin{document} \begin{itemize} \section*{Papers} \subsection*{International Journals} \item[1] ``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[2] ``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[3] ``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[4] ``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[5] ``Comparison of equation of state models with different cluster dissolution mechanisms'', Helena Pais and Stefan Typel, eprint arXiv:1612.07022 [nucl-th], contribution to the special-topics volume on nuclear correlations and cluster physics, edited by W. U. Schroder (2016). \item[6] ``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[7] ``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[8] ``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[9] ``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[10] ``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[11] ``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[12] ``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[13] ``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[14] ``Exploring the Nuclear Pasta Phase in Core-Collapse Supernova Matter'', Helena Pais and Jirina R. Stone, Physical Review Letters {\bf 109}, 151101 (2012). \item[15] ``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[16] ``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[17] ``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[18] ``Comparison of EoS models with different cluster suppression mechanisms'', Stefan Typel, Helena Pais, Nuovo Cim. C {\bf 39}, 393 (2017). \item[19] ``Pasta phases in core-collapse supernova matter'', Helena Pais, Silvia Chiacchiera, and Constança Providência, Journal of Physics: Conference Series {\bf 706}, 042007 (2016). \item[20] ``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[21] ``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*{Oral} \item[22] ``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[23] ``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[24] ``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[25] ``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[26] ``Pasta phases in core-collapse supernova matter'', Helena Pais, Talk given at the Annual NewCompStar Conference 2015, Budapest, Hungary, June 15-19 (2015). \item[27] ``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[28] ``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[29] ``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[30] ``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[31] ``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[32] ``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[33] ``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[34] ``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[35] ``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[36] ``Estrelas de quarks num campo magnético forte'', Helena Pais (supervisor Constança Providência), MSc thesis, University of Coimbra (2008). \end{itemize} \end{document}