The main objective of naXys is the study of complex systems (i.e. systems composed of a large number of simple elements in interaction and exhibiting emerging phenomena), by means of the analysis of real-world data, their modelling through mathematics and numerical simulations, and their control and optimisation.
Within the research groups several research lines are in place:
- Dynamical astronomy, cosmology and astrobiology
- Mathematical biology
- Bio-inspired Evolution Strategies & Quantum Optics
- Socio-economic complexity
- Stability and robustness
The marine aspect of the research focuses on oceanic systems on planets and their satellites.
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Engelse naam: Namur Institute for Complex Systems - naXys
Overkoepelend instituut: Département de mathématique (Unamur), meer
Adres:
Rempart de la Vierge 8
5000 - Namur
België
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Type: Wetenschappelijk
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1 Directeur: Hoofd van de onderzoeksgroep/afdeling 2 Mariene onderzoeker: Is werkzaam in deze groep en treedt op als (co)auteur in minstens één mariene publicatie in de laatste 5 jaar. 3 Gespecialiseerd personeel: Levert administratieve of technische ondersteuning aan het zeewetenschappelijk onderzoek.
( 9 peer reviewed ) opsplitsen filter
 Spaak, J.W.; De Laender, F. (2021). Effects of pigment richness and size variation on coexistence, richness and function in light-limited phytoplankton. J. Ecol. 109(6): 2385-2394. https://hdl.handle.net/10.1111/1365-2745.13645, meer- Noyelles, B. (2018). Corrigendum to “Interpreting the librations of a synchronous satellite – How their phase assesses Mimas’ global ocean” [Icarus 282 (2017) 276–289]. Icarus 305: 80-83. https://dx.doi.org/10.1016/j.icarus.2018.01.005, meer
- Noyelles, B. (2018). Rotation of a synchronous viscoelastic shell. Monthly Notices of the Royal Astronomical Society 474(4): 5614-5644. https://dx.doi.org/10.1093/mnras/stx3122, meer
- Bolmont, E.; Selsis, F.; Owen, J.E.; Ribas, I.; Raymond, S.N.; Leconte, J.; Gillon, M. (2017). Water loss from terrestrial planets orbiting ultracool dwarfs: implications for the planets of TRAPPIST-1. Monthly Notices of the Royal Astronomical Society 464(3): 3728-3741. https://dx.doi.org/10.1093/mnras/stw2578, meer
- Noyelles, B. (2017). Interpreting the librations of a synchronous satellite - How their phase assesses Mimas' global ocean. Icarus 282: 276-289. https://dx.doi.org/10.1016/j.icarus.2016.10.001, meer
- Bolmont, E.; Libert, A.-S.; Leconte, J.; Selsis, F. (2016). Habitability of planets on eccentric orbits: limits of the mean flux approximation. Astron. Astrophys. 591: 17 pp. https://dx.doi.org/10.1051/0004-6361/201628073, meer
- Bolmont, E.; Mathis, S. (2016). Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets. Celestial Mechanics & Dynamical Astronomy 126(1): 275-296. https://dx.doi.org/10.1007/s10569-016-9690-3, meer
- Turbet, M.; Leconte, J.; Selsis, F.; Bolmont, E.; Forget, F.; Ribas, I.; Raymond, S.N.; Anglada-Escudé, G. (2016). The habitability of Proxima Centauri b. II. Possible climates and observability. Astron. Astrophys. 596: A112. https://hdl.handle.net/10.1051/0004-6361/201629577, meer
- Tajeddine, R.; Rambaux, N.; Lainey, V.; Charnoz, S.; Richard, A.; Rivoldini, A.; Noyelles, B. (2014). Constraints on Mimas' interior from Cassini ISS libration measurements. Science (Wash.) 346(6207): 322-324. https://dx.doi.org/10.1126/science.1255299, meer
- Noyelles, B.; Nimmo, F. (2014). New clues on the interior of Titan from its rotation state. Proceedings of the International Astronomical Union 9(310): 17-20. https://dx.doi.org/10.1017/S1743921314007728, meer
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