Articles dans des revues avec comité de lecture (125)
  1. 105. Chamel, N., Goriely, S., & Pearson, M. J. (2009). Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XI: Stabilizing neutron stars against a ferromagnetic collapse. Physical review. C, Nuclear physics, 80, 065804. doi:10.1103/PhysRevC.80.065804
  2. 106. Goriely, S., Chamel, N., & Pearson, M. J. (2009). Recent breakthroughs in Skyrme-Hartree-Fock-Bogoliubov mass formulas. European Physical Journal A. Hadrons and nuclei, 42, 547-552. doi:10.1140/epja/i2009-10784-7
  3. 107. Goriely, S., Chamel, N., & Pearson, M. J. (2009). Skyrme-Hartree-Fock-Bogoliubov nuclear mass formulas: Crossing the 0.6 MeV threshold with microscopically deduced pairing. Physical Review Letters, 102(15), 152503. doi:10.1103/PhysRevLett.102.152503
  4. 108. Chamel, N., Margueron, J., & Khan, E. (2009). Neutron specific heat in the crust of neutron stars from the nuclear band theory. Physical Review C (Nuclear Physics), 79(1), 012801. doi:10.1103/PhysRevC.79.012801
  5. 109. Minaya Rainirez, E., Audi, G., Lunney, D., Naimi, S., Beck, D., Herfurth, F., Blaum, K., Borgmann, C., George, S., Kellerbauer, A., Bohm, C., Neidherr, D., Breitenfeldt, M., Rosenbusch, M., Schweikhard, L., Chamel, N., Goriely, S., Herlert, A., Kowalska, M., Pearson, J., & Schwarz, S. (2009). Neutron drip-line topography. AIP Conference Proceedings, 1165, 94-97. doi:10.1063/1.3232162
  6. 110. Chamel, N., Goriely, S., & Pearson, M. J. (2008). Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. IX: Constraint of pairing force to 1S0 neutron-matter gap. Nuclear physics. A, 812(1-4), 72-98. doi:10.1016/j.nuclphysa.2008.08.015
  7. 111. Chamel, N., & Haensel, P. (2008). Physics of neutron star crusts. Living Review on Relativity, 11.
  8. 112. Onsi, M., Dutta, A., Chatri, H., Goriely, S., Chamel, N., & Pearson, M. J. (2008). Semi-classical equation of state and specific-heat expressions with proton shell corrections for the inner crust of a neutron star. Physical review. C. Nuclear physics, 77(6), 065805. doi:10.1103/PhysRevC.77.065805
  9. 113. Chamel, N. (2008). Two-fluid models of superfluid neutron star cores. Monthly notices of the Royal Astronomical Society, 388(2), 737-752. doi:10.1111/j.1365-2966.2008.13426.x
  10. 114. Chamel, N., Naimi, S., Khan, E., & Margueron, J. (2007). Validity of the Wigner-Seitz approximation in neutron star crust. Physical Review C (Nuclear Physics), 75(5), 055806. doi:10.1103/PhysRevC.75.055806
  11. 115. Chamel, N. (2006). Effective mass of free neutrons in neutron star crust. Nuclear physics. A, 773(3-4), 263-278. doi:10.1016/j.nuclphysa.2006.04.010
  12. 116. Chamel, N., & Carter, B. D. (2006). Effect of entrainment on stress and pulsar glitches in stratified neutron star crust. Monthly notices of the Royal Astronomical Society, 368(2), 796-808. doi:10.1111/j.1365-2966.2006.10170.x
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