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\section*{Books}

\subsection*{Chapters of Books}

\item[1] ``The Inner Crust and its Structure'', Débora P. Menezes, Sidney S. Avancini, Constança Providência, Marcelo D. Alloy, "Neutron Star Crust", edited by C.\,A. Bertulani and J. Piekarewicz
Nova Publishers {\bf chap 10} (2012).

\section*{Papers}

\subsection*{International Journals}

\item[2] ``Thermal evolution of relativistic hyperonic compact stars with calibrated equations of state'', Morgane Fortin, Adriana R. Raduta, Sidney Avancini, Constança Providência, Phys. Rev. D {\bf 103}, 083004 (2021).

\item[3] ``Relativistic hypernuclear compact stars with calibrated equations of state'', Morgane Fortin, Adriana R. Raduta, Sidney Avancini, and Constança Providência, Phys. Rev. D {\bf 101}, 034017 (2020).

\item[4] ``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[5] ``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[6] ``Hypernuclei and massive neutron stars'', M. Fortin, S.\,S. Avancini, C. Providência, I. Vidaña, Phys. Rev. C {\bf 95}, 065803 (2017).

\item[7] ``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[8] ``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[9] ``Neutrino diffusion in the pasta phase matter within the Thomas-Fermi approach'', U.\,J. Furtado, S.\,S. Avancini, J. R. Marinelli, W. Martarello, C. Providência, Eur. Phys. J. A {\bf 52}, 290 (2016).

\item[10] ``Imprint of the symmetry energy on the inner crust and strangeness content of neutron stars'', Constança Providência, Sidney S. Avancini, Rafael Cavagnoli, Silvia Chiacchiera, Camille Ducoin, Fabrizio Grill, Jérôme Margueron, Débora P. Menezes, Aziz Rabhi, Isaac Vidaña, EPJA {\bf 50-2}, 44-1-44-18 (2014).

\item[11] ``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[12] ``Relativistic Mean-Field Hadronic Models under Nuclear Matter Constraints'', M. Dutra, O. Lourenço, S. S. Avancini, B. V. Carlson, A. Delfino, D. P. Menezes, C. Providência, S. Typel, J. R. Stone, Phys. Rev. C {\bf 90}, 055203-1-055203-35 (2014).

\item[13] ``Effect of strong magnetic fields on the nuclear “pasta” phase structure'', R. C. R. de Lima, S. S. Avancini, and C. Providência, Phys. Rev. C {\bf 88}, 035804 (2013).

\item[14] ``Neutron star inner crust and symmetry energy'', Fabrizio Grill, Constança Providência, Sidney S. Avancini, Phys. Rev. C {\bf 85}, 055808 (2012).

\item[15] ``Light clusters in nuclear matter and the “pasta” phase'', S. S. Avancini, C. C. Barros, Jr., L. Brito, S. Chiacchiera, D. P. Menezes, C. Providência, Phys Rev C {\bf 85}, 035806 (2012).

\item[16] ``QCD critical end point under strong magnetic fields'', Sidney S. Avancini, Débora P. Menezes, Marcus B. Pinto,  Constança Providência, Phys. Rev. D (Rapid Communication) {\bf 85}, 091901 (2012).

\item[17] ``Erratum: Warm “pasta” phase in the Thomas-Fermi approximation [Phys. Rev. C 82, 055807 (2010)]'', Sidney S. Avancini, Silvia Chiacchiera, Débora P. Menezes,  Constança Providência, Phys. Rev. C {\bf 85}, 059904 (2012).

\item[18] ``Finite temperature quark matter under strong magnetic fields'', S. S. Avancini, D. P. Menezes, and C. Providência, Phys. Rev. C {\bf 83}, 065805 (2011).

\item[19] ``\α particles and the “pasta” phase in nuclear matter'', S. S. Avancini, C. C. Barros, Jr., D. P. Menezes, and C. Providência, Physical Review C {\bf 82}, 025808 (2010).

\item[20] ``Warm “pasta” phase in the Thomas-Fermi approximation'', Sidney S. Avancini, Silvia Chiacchiera, Débora P. Menezes, and Constança Providência, Physical Review C {\bf 82}, 055807 (2010).

\item[21] ``Quark matter under strong magnetic fields in the Nambu–Jona-Lasinio model'', D. P. Menezes, M. Benghi Pinto, S. S. Avancini, A. Pérez Martínez, e C. Providência, Phys. Rev. C {\bf 79}, 035807-13 (2009).

\item[22] ``Quark matter under strong magnetic fields in the su(3) Nambu-Jona-Lasinio Model'', D.\,P. Menezes, M. Benghi Pinto, S.\,S. Avancini, C. Providência, Physical Review C {\bf 80}, 065805 (2009).

\item[23] ``Nuclear “pasta” phase within density dependent hadronic models'', S. S. Avancini, L. Brito, J. R. Marinelli, D. P. Menezes, M. M. W. de Moraes, C. Providência, and A. M. Santos, Phys. Rev. C {\bf 79}, 035804-14 (2009).

\item[24] ``Skyrme forces versus relativistic models: Reexamining instabilities'', M. Dutra, O. Lourenço, A. Delfino, J. S. Sá Martins, C. Providência, S. S. Avancini, and D. P. Menezes, Phys. Rev. C {\bf 77}, 035201-1-035201-13 (2008).

\item[25] ``Warm and cold pasta phase in relativistic mean field theory'', S.\,S. Avancini, D.\,P. Menezes, M.\,D. Alloy, J.\,R. Marinelli, M.\,M.\,W. Moraes, C. Providência, Phys. Rev. C {\bf 78}, 015802-1-015802-12 (2008).

\item[26] ``Center-of-Mass Correction in a Relativistic Hartree Approximation Including the Meson Degrees of Freedom'', P. Alberto, S.\,S. Avancini, M. Fiolhais, J.\,R. Marinelli, Physical Review C {\bf 75}, 054324 (2007).

\item[27] ``Density dependent hadronic models and the relation between neutron stars and neutron skin thickness.'', S. S. Avancini, J. R. Marinelli, D. P. Menezes, M. M. W. Moraes, and C. Providência, Phys. Rev. C {\bf 75}, 055805 (2007).

\item[28] ``Neutron Skin Thickness and Neutron Stars within a Density Dependent
Hadronic Model.'', S. S. Avancini, J. R. Marinelli, D. P. Menezes, M. M. W. de Moraes, C. Providência, Int. J. of Mod. Phys. E {\bf 16}, 2989-2992 (2007).

\item[29] ``Unstable modes in relativistic neutron-electron-proton (npe) matter at finite temperature'', Brito, L., C. Providência, Santos, A. M., Avancini, S. S., Menezes, D. P. and Chomaz, Ph., Phys.Rev. C {\bf 74}, 04580 (2006).

\item[30] ``Low-density instabilities in relativistic asymmetric matter of compact stars.'', C. Providência, L. Brito, S.\,S. Avancini, D.\,P. Menezes, Ph. Chomaz, Phys. Rev. C {\bf 73}, 025805 (2006).

\item[31] ``Coupling of nuclear and electron modes in relativistic stella matter.'', C. Providência, L. Brito, A.\,M.\,S. Santos, D.\,P. Menezes, S. S. Avancini, Phys. Rev. C {\bf 74}, 045802 (2006).

\item[32] ``Center-of-Mass Correction in a Relativistic Hartree Approximation'', P. Alberto, M. Fiolhais, S. S. Avancini, J. R. Marinelli, Brazilian Journal of Physics {\bf 36}, 1375-1378 (2006).

\item[33] ``Spinodal instabilities and the distillation effect in relativistic hadronic models.'', S. S. Avancini, L. Brito, Ph. Chomaz, D. P. Menezes, C. Providência, Phys. Rev. C {\bf 74}, 024317 (2006).

\item[34] ``Peierls-Yoccoz projection in $sigma-omega$ models'', P. Alberto, S. S. Avancini e M. Fiolhais, International Journal of Modern Physics E {\bf 14}, 1171-1196 (2005).

\item[35] ``Collective modes in relativistic asymmetric nuclear matter.'', S.\,S. Avancini, L. Brito, D. P. Menezes, C. Providência, Phys. Rev. C {\bf 71}, 044323 (2005).

\item[36] ``Asymmetric nuclear matter and its instabilities.'', S.\,S. Avancini, L. Brito, D.\,P. Menezes e C. Providencia, Braz. J. Phys. {\bf 35 B}, 832 (2005).

\item[37] ``Instabilities in asymmetric nuclear matter.'', S.\,S. Avancini, L. Brito, D.\,P. Menezes, C. Providênci, Phys. Rev. C {\bf 70}, 015203; nucl-th/0406022 (2004).

\item[38] ``Three-level Lipkin model in the context of the su_q(3) algebra.'', L. Brito, C. Providência, J. da Providência, S. S. Avancini,F. F. de Souza Cruz, D. P. Menezes, M. M. Watanabe Moraes, Phys. Rev. A {\bf 52}, 92 (1995).

\item[39] ``The q- Deformed Thouless Model for Superconductivity and the Study of Thermal Effects by Number Nonconserving Coherent States'', D. Bonatsos, S.\,S. Avancini, D.\,P. Menezes and C. Providência, Phys. Lett. A {\bf 192}, 192-200 (1994).

\item[40] ``Quantum algebraic description of the Moszkowski model'', D. P. Menezes, S. S. Avancini, C. Providência, J. Phys A {\bf 25}, 6317 (1992).

\section*{Proceedings}

\subsection*{International Conferences}

\item[41] ``Finite temperature matter subject to strong magnetic fields'', D.\,P. Menezes, S.\,S. Avancini and C. Providência, International Journal of Modern Physics E {\bf 20}, 93-99 (2011).

\item[42] ``EXOTIC PHASES IN HOT NEUTRON-PROTON-ELECTRON (NPE) MATTER'', S. S. Avancini, Marinelli JR,D. P. Menezes, Moraes MMW, C. Providência, Santos AM, INTERNATIONAL JOURNAL OF MODERN PHYSICS D {\bf 19}, 1587-1592 (2010).

\item[43] ``Centre-of-mass corrections in relativistic mean-field descriptions of light nuclei'', S.\,S. Avancini, P. Alberto, M. Fiolhais, Proceedings of Proceedings of the VIII International Workshop on Hadron Physics 2002, C. Vasconcellos et al. (Eds.), World Scientific, Singapore, 261-264 (2003).

\item[44] ``The suq(3) algebra: application to the three-level Lipkin model
Proceedings of The IV Wigner Symposium, Guadalajara, México, 7 – 11 August, 1995,'', Brito, L., Providência, C., da Providência, J., Avancini, S. S., de Souza Cruz, F. F., Menezes, D. P. and Watanabe Moraes, M. M., Eds. Natig M. Atakishiyev, Thomas H. Seligman and Kurt B. Wolf, World Scientific, Singapore, 54 (1996).

\item[45] ``The su_q(3) algebra: application to the 3-level Lipkin model.'', L. Brito, C. Providência, J. da Providência, S. S. Avancini, F. F. de Souza Cruz, D. P. Menezes e M. M. Watanabe Moraes, Proceedings of the IV Wigner Symposium, Natigb M. Atakishiyev, Thomas H. Seligman and Kurt Bernardo Wolf (Eds),World Scientific, Singapura, 54 (1996).

\end{itemize}
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