Participations à des congrès et colloques internationaux (16)
  1. 7. Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2015). Unified equations of state for neutron stars within the energy-density functional theory and neutron-star structure. Paper session presented at Annual NewCompStar Conference 2015 (15-19 June 2015: Budapest, Hungary).
  2. 8. Pastore, A., Martini, M., Davesne, D., Navarro, G., Chamel, N., & Goriely, S. (2014). Neutrino mean free path in neutron matter with Brussels-Montreal Skyrme functionals. Poster présenté à la conférence Nuclear Physics in Astrophysics VI (19-24 May 2013: Lisbon (Portugal)).
  3. 9. Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2014). Nuclear-matter properties and neutron-star structure with unified equations of state. Paper session presented at Workshop MODE-SNR-PWN (19-21 May 2014: Lyon (France)).
  4. 10. Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2014). Unified equations of state of dense matter: nuclear-matter properties and neutronstar structure. Paper session presented at The Structure and Signal of Neutron Stars, from Birth to Death (24-28 March 2014: Florence (Italy)).
  5. 11. Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2014). Properties of neutron stars with unified equations of state. Paper session presented at Mons Meeting 2014 (26-29 August 2014: Mons, Belgium).
  6. 12. Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2013). Unified equations of state of dense matter: neutron-star structure and nuclear-matter properties. Paper session presented at CoCoNuT Meeting 2013 (04-06 December 2013: Meudon, France).
  7. 13. Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2012). Structure of neutron stars with unified equations of state. Paper session presented at Program "From nucleon structure to nuclear structure and compact astrophysical objects" (11-29 June 2012: Beijing, China).
  8. 14. Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2012). Unified equations of state for neutron stars (and supernova cores) and neutron star structure. Paper session presented at CoCoNuT Meeting 2012 (24-26 October 2012: Palma de Mallorca, Spain).
  9. 15. Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2011). Unified equation of state for neutron stars (and supernova cores) using the energy-density functional theory. Paper session presented at Workshop MODE-SNR-PWN 2011 (21-24 November 2011: Nançay, France).
  10. 16. Fantina, A., Chamel, N., Pearson, M. J., & Goriely, S. (2011). Unified equation of state for supernova cores and neutron stars using the nuclear energy-density functional theory. Paper session presented at Workshop CompStar 2011 “Gravitational waves and electromagnetic radiation from compact stars” (09-12 May 2011: Catania, Italy).
    11.   Divers (7)
  11. 1. Chamel, N. (2020). Introduction à la thermodynamique: PHYS-F-201.
  12. 2. Chamel, N., & Stoyanov, Z. (2020). Equilibrium structure of the outer crust of a magnetar. doi:10.5281/zenodo.3839787
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