Parties d'ouvrages collectifs (4)
  1. 1. Blaschke, D., & Chamel, N. (2018). Phases of Dense Matter in Compact Stars. In L. Rezzolla, P. M. Pizzochero, D. I. Jones, N. Rea, & I. Vidaña (Eds.), The Physics and Astrophysics of Neutron Stars, Vol. 457. Astrophysics and Space Science Library (1 ed., pp. 337-400). Springer. doi:10.1007/978-3-319-97616-7
  2. 2. Chamel, N., Mutafchieva, Y. D., Stoyanov, Z. K., Mihailov, L., & Pavlov, R. (2017). Landau Quantisation of Electron Motion in the Crust of Highly Magnetised Neutron Stars. In A. Tadjer, R. Pavlov, J. Maruani, E. J. Brändas, & G. Delgado-Barrio (Eds.), Quantum Systems in Physics, Chemistry, and Biology: Advances in Concepts and Applications (pp. 181-191). Springer. doi:10.1007/978-3-319-50255-7_11
  3. 3. Chamel, N., Pearson, M. J., & Goriely, S. (2013). Pairing: from atomic nuclei to neutron-star crusts. In R. Broglia & V. Zelevinsky (Eds.), 50 years of nuclear BCS: Pairing in Finite Systems (pp. 284-296). World Scientific. doi:10.1142/9789814412490_0021
  4. 4. Goriely, S., Chamel, N., & Pearson, M. J. (2012). Neutron-star crusts and finite nuclei. In C. Bertulani & J. Piekarewicz (Eds.), Neutron Star Crust (pp. 213-233). Hauppauge, New York: Nova Science Publishers.
    5.   Articles dans des revues avec comité de lecture (140)
  5. 1. Bauswein, A., Nikolaidis, A., Lioutas, G., Kochankovski, H., Char, P., Mondal, C., Oertel, M., Tolos, L., Chamel, N., & Goriely, S. (2026). Stellar properties indicating the presence of hyperons in neutron stars. Physical Review Research, 8(1). doi:10.1103/ygtr-ktqk
  6. 2. Shchechilin, N., Chamel, N., & Chugunov, A. I. (2025). Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions. European Physical Journal A. Hadrons and nuclei, 61(6), 132. doi:10.1140/epja/s10050-025-01594-6
  7. 3. Grams, G., Shchechilin, N., Diverrès, T., Fantina, A. F., Chamel, N., & Gulminelli, F. (2025). Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas–Fermi Approaches. Universe, 11(6), 172. doi:10.3390/universe11060172
  8. 4. Chamel, N. (2025). Superfluid fraction in the crystalline crust of a neutron star: Role of quantum zero-point motion of ions. Physical Review C, 111(5). doi:10.1103/PhysRevC.111.055803
  9. 5. Allard, V., & Chamel, N. (2025). Evidence of Gapless Superfluidity in MXB 1659-29 With and Without Late Time Cooling. Universe, 11(5), 140. doi:10.3390/universe11050140
  10. 6. Chamel, N. (2025). Superfluid fraction in the crystalline crust of a neutron star: Role of BCS pairing. Physical Review C, 111(4), 045803. doi:10.1103/PhysRevC.111.045803
  11. 7. Grams, G., Shchechilin, N., Sánchez Fernández, A., Ryssens, W., Chamel, N., & Goriely, S. (2025). Skyrme–Hartree–Fock–Bogoliubov mass models on a 3D mesh: IV. Improved description of the isospin dependence of pairing. European Physical Journal A. Hadrons and nuclei, 61, 35. doi:10.1140/epja/s10050-025-01503-x
  12. 8. Chamel, N., Shchechilin, N., & Chugunov, A. I. (2025). Pressure and chemical potentials in the inner crust of a cold neutron star within Hartree-Fock and extended Thomas-Fermi methods. Physical Review C, 111(1). doi:10.1103/PhysRevC.111.015805
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