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\section*{Papers}

\subsection*{International Journals}

\item[1] ``Constraining the high-density behavior of nuclear symmetry energy with direct Urca processes'', Olfa Boukari, Tuhin Malik, Aziz Rabhi, Constança Providência, Phy. Rev. C (PRC) {\bf (accepted)} (2024).

\item[2] ``Neutron stars within the Bogoliubov quark-meson coupling model'', Aziz Rabhi, Constança Providência, Steven A. Moszkowski, João da Providência, Henrik Bohr, Phys. Rev. C {\bf 103}, 035811 (2021).

\item[3] ``Crust-core transition of a neutron star: effect of the temperature under strong magnetic fields'', Márcio Ferreira, Aziz Rabhi, Constança Providência, Eur. Phys. J. A {\bf 57}, 263 (2021).

\item[4] ``Hyperonic Stars and the Nuclear Symmetry Energy'', Constança Providência, Morgane Fortin, Helena Pais, Aziz Rabhi, Front. Astron. Space Sci {\bf 6} (2019).

\item[5] ``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[6] ``Magnetic susceptibility and magnetization properties of asymmetric nuclear matter under a strong magnetic field'', A. Rabhi, M. A. Pérez-García, C. Providência, I. Vidaña, Phys. Rev. C {\bf 91}, 045803 (2015).

\item[7] ``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[8] ``The 1D Heisenberg antiferromagnet model by the variation after projection method'', A. Rabhi, M. Brajczewska, P. Schuck, J. da Providência, R. Bennaceur, International Journal of Modern Physics B {\bf 27}, 1350058 (2013).

\item[9] ``Interplay between the symmetry energy and the strangeness content of neutron stars'', Constança Providência and Aziz Rabhi, Phys. Rev. C {\bf 87}, 055801-055809 (2013).

\item[10] ``Warm and dense stellar matter under strong magnetic fields'', A. Rabhi, P. K. Panda, and C. Providência, Phys. Rev. C {\bf 84}, 035803 (2011).

\item[11] ``Quark matter under strong magnetic fields in chiral models'', Aziz Rabhi and Constança Providência, Phys. Rev. C {\bf 83}, 055801 (2011).

\item[12] ``Landau parameters for asymmetric nuclear matter with a strong magnetic field'', M. Ángeles Pérez-García, C. Providência, and A. Rabhi, Phys. Rev. C {\bf 84}, 045803 (2011).

\item[13] ``Dense stellar matter with trapped neutrinos under strong magnetic fields'', A. Rabhi,C. Providencia, JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS {\bf 37}, 075102 (2010).

\item[14] ``Spinodal instabilities and the distillation effect in nuclear
matter under strong magnetic fields'', A. Rabhi, C. Providência, and J. Da Providência, Phys. Rev. C {\bf 79}, 015804-1-015804-11 (2009).

\item[15] ``Effect of the \δ meson on the instabilities of nuclear matter under strong magnetic fields'', A. Rabhi, C. Providência, and J. Da Providência, Physical Review C {\bf 80}, 025806 (2009).

\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] ``Stellar matter with a strong magnetic field within density-dependent
relativistic models'', A. Rabhi, C. Providência and J. Da Providência, J. Phys. G: Nucl. Part. Phys. {\bf 35}, 125201-1-125201-17 (2008).

\item[18] ``Random phase approximation for the 1D anti-ferromagnetic Heisenberg model'', A. Rabhi, P. Schuck, J. Da Providencia, J. Phys.: Condens. Matter {\bf 18}, 10249-10258 (2006).

\item[19] ``Self-consistent random phase approximation in Schütte-Da-Providencia fermion-boson model'', A. RABHI, Phys. Rev. C {\bf 69}, 017306 (2004).

\item[20] ``Comment on " Energies of the ground state and first excited 0^{+) state in an exactly solvable pairing model".'', A. RABHI, Eur. Phys. J. A {\bf 20}, 277 (2004).

\item[21] ``Self-consistent quasiparticle RPA for the description of superfluid Fermi systems'', A. RABHI, R. BENNACEUR, G. CHANFRAY, P. SCHUCK, Phys. Rev. C {\bf 66}, 064315 (2002).

\section*{Communications}

\subsection*{Oral}

\item[22] ``Application of Self-consistent RPA to the description of dynamical properties of the linear antiferromagnetic chain.'', A. Rabhi, 1st Southern Mediterranean Summer Workshop on Subatomic Physics (Faculté des Sciences de Tunis), Tunis, Tunisia (2006).

\item[23] ``Self-consistent random phase approximation applied to a schematic field theoretical model (Schütte-Da Providencia model).'', A. RABHI, Rencontres Jeunes Chercheurs 2004, (young researchers meeting in nuclear physics 2004), Centre Paul Langevin, Aussois, France (2004).

\item[24] ``Application of standard RPA to the description of dynamical properties of the linear antiferromagnetic chain'', A. RABHI, 11th Workshop on Magnetism and Intermetallics, Departamento de Física, Coimbra, Portugal (2004).

\subsection*{Poster}

\item[25] ``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).

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