Articles dans des revues avec comité de lecture (125)

  1. 69. Pastore, A., Martini, M., Davesne, D., Navarro, G., Goriely, S., & Chamel, N. (2014). Linear response theory and neutrino mean free path using Brussels-Montreal Skyrme functionals. Physical review. C, Nuclear physics, 90, 025804. doi:10.1103/PhysRevC.90.025804
  2. 70. Chamel, N., Molter, E., Fantina, A., & Pena Arteaga, D. (2014). Maximum strength of the magnetic field in the core of the most massive white dwarfs. Physical Review D - Particles, Fields, Gravitation and Cosmology, 90, 043002. doi:10.1103/PhysRevD.90.043002
  3. 71. Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2014). Constraints on the equation of state of cold dense matter from nuclear physics and astrophysics. EPJ web of conferences, 66, 07005. doi:10.1051/epjconf/20146607005
  4. 72. Pearson, M. J., Chamel, N., Fantina, A., & Goriely, S. (2014). Symmetry energy: nuclear masses and neutron stars. European Physical Journal A. Hadrons and Nuclei, 50, 43. doi:10.1140/epja/i2014-14043-8
  5. 73. Velchev, C., Pavlov, R., Mihailov, L., Chamel, N., Stoyanov, Z., Mutafchieva, Y. Y., & Ivanovich, M. M. (2014). Correlation effects of heliumoid electron-nuclear systems. Dokladi na B''lgarskata akademiâ na naukite, 67(11), 1513-1520.
  6. 74. Goriely, S., Chamel, N., & Pearson, M. J. (2013). Hartree-Fock-Bogoliubov nuclear mass model with 0.50 MeV accuracy based on standard forms of Skyrme and pairing functionals. Physical review. C, Nuclear physics, 88, 061302.
  7. 75. Potekhin, A., Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2013). Analytical representations of unified equations of state for neutron-star matter. Astronomy & astrophysics, 560, 48. doi:10.1051/0004-6361/201321697
  8. 76. Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2013). Neutron star properties with unified equations of state of dense matter. Astronomy & astrophysics, 559, 128. doi:10.1051/0004-6361/201321884
  9. 77. Chamel, N., Fantina, A., & Davis, P. (2013). Stability of super-Chandrasekhar magnetic white dwarfs. Physical review. D, Particles, fields, gravitation, and cosmology, 88(8), 081301. doi:10.1103/PhysRevD.88.081301
  10. 78. Pearson, M. J., Goriely, S., & Chamel, N. (2013). Microscopic mass models for astrophysics. International journal of mass spectrometry, 349(1), 57. doi:10.1016/j.ijms.2013.04.003
  11. 79. Goriely, S., Chamel, N., & Pearson, M. J. (2013). Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XIII. The 2012 atomic mass evaluation and the symmetry coefficient. Physical review. C, Nuclear physics, 88, 024308. doi:10.1103/PhysRevC.88.024308
  12. 80. Chamel, N., Haensel, P., Zdunik, J. L., & Fantina, A. (2013). On the maximum mass of neutron stars. International journal of modern physics E, 22, 1330018. doi:10.1142/S021830131330018X

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