Articles dans des revues avec comité de lecture (125)
  1. 117. Carter, B. D., Chamel, N., & Haensel, P. (2006). Entrainment coefficient and effective mass for conduction neutrons in neutron star crust: Macroscopic treatment. International Journal of Modern Physics D: Gravitation, Astrophysics and Cosmology, 15(5), 777-803.
  2. 118. Chamel, N., & Haensel, P. (2006). Entrainment parameters in a cold superfluid neutron star core. Physical Review C (Nuclear Physics), 73(4), 045802. doi:10.1103/PhysRevC.73.045802
  3. 119. Carter, B. D., Chachoua, E., & Chamel, N. (2006). Covariant Newtonian and relativistic dynamics of (magneto)-elastic solid model for neutron star crust. General Relativity and Gravitation, 38(1), 83-119. doi:10.1007/s10714-005-0210-0
  4. 120. Carter, B. D., Chamel, N., & Haensel, P. (2005). Effect of BCS pairing on entrainment in neutron superfluid current in neutron star crust. Nuclear physics. A, 759(3-4), 441-464. doi:10.1016/j.nuclphysa.2005.05.151
  5. 121. Carter, B. D., & Chamel, N. (2005). Covariant analysis of Newtonian multi-fluid models for neutron stars: II Stress - energy tensors and virial theorems. International Journal of Modern Physics D: Gravitation, Astrophysics and Cosmology, 14(5), 717-748.
  6. 122. Carter, B. D., & Chamel, N. (2005). Covariant analysis of Newtonian multi-fluid models for neutron stars: III.Transvective, viscous and superfluid drag dissipation. International Journal of Modern Physics D: Gravitation, Astrophysics and Cosmology, 14(5), 749-774.
  7. 123. Chamel, N. (2005). Band structure effects for dripped neutrons in neutron star crust. Nuclear Physics A, 747(1), 109-128. doi:10.1016/j.nuclphysa.2004.09.011
  8. 124. Carter, B. D., Chamel, N., & Haensel, P. (2004). Entrainment coefficient and effective mass for conduction neutrons in neutron star crust: simple microscopic models. Nuclear physics. A, 748(3-4), 675-697. doi:10.1016/j.nuclphysa.2004.11.006
  9. 125. Carter, B. D., & Chamel, N. (2004). Covariant analysis of Newtonian multi-fluid models for neutron stars: I Milne-Cartan structure and variational formulation. International Journal of Modern Physics D: Gravitation, Astrophysics and Cosmology, 13(2), 291-325.
    10.   Communications publiées lors de congrès ou colloques nationaux et internationaux (29)
  10. 1. Grams, G., Ryssens, W., Scamps, G., Goriely, S., & Chamel, N. (2023). Progress on Brussels-Skyrme atomic mass models on a grid: stiff neutron matter equation of state. Journal of physics. Conference series (Online),(2586), 012040. doi:10.1088/1742-6596/2586/1/012040
  11. 2. Chamel, N., Perot, L., Fantina, A., Chatterjee, D., Ghosh, S., Novak, J., & Oertel, M. (2023). Electron captures and stability of white dwarfs. In R. Ruffini & G. Vereshchagin (Eds.), Proceedings of The Sixteenth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories (pp. 4488-4507) World Scientific Publishing. doi:10.1142/9789811269776_0379
  12. 3. Shchechilin, N., Chamel, N., & Pearson, J. M. (2023). Nuclear Pasta in Cold Non-Accreting Neutron Stars: Symmetry Energy Effects. Physical sciences forum,(7(1)), 10. doi:10.3390/ECU2023-14017
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