| Autor: |
Politi Giuseppe, Acosta Luis, Andrés Maria Victoria, Auditore Lucrezia, Beck Christian, Cap Tomasz, Cardella Giuseppe, Catara Francesco, Colonna Maria, De Filippo Enrico, D'Onofrio Antonio, Geraci Elena, Gnoffo Brunilde, Kalandarov Shuhrat, La Commara Marco, Lanza Edoardo G., Lanzalone Gaetano, Maiolino Concettina, Martorana Nunzia Simona, Pagano Angelo, Pagano Emanuele Vincenzo, Papa Massimo, Piasecki Erik, Pirrone Sara, Quattrocchi Lucia, Rizzo Francesca, Russotto Paolo, Santonocito Domenico, Siwek-Wilczynska Krystyna, Trifirò Antonio, Trimarchi Marina, Vitturi Andrea |
| Jazyk: |
angličtina |
| Rok vydání: |
2018 |
| Předmět: |
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| Zdroj: |
EPJ Web of Conferences, Vol 194, p 07003 (2018) |
| Druh dokumentu: |
article |
| ISSN: |
2100-014X |
| DOI: |
10.1051/epjconf/201819407003 |
| Popis: |
The study of nuclei properties and of collision dynamics is a very active research field whose result have implications in different domains as for example astrophysics. The present and future facilities delivering radioactive ion beams with high intensity allow to extend these studies in the region far from the stability valley. New insight has thus been found on the effects of neutron richness on reaction mechanisms as well as on nuclear structure and nuclear matter properties, as for instance, the role of symmetry energy term of the nuclear Equation of State. The presence of diverse reaction products demands for highly performing and very specialized devices, also able to disentangle among different mechanisms, from fast dynamical processes to statistical emission from equilibrated sources. Numerous studies of the effects of N/Z ratio on fusion and associated processes can be found at different energies, together with many examples of the influence of neutron richness on the reaction time scale and the competition between equilibrated and prompt processes. A survey of very recent findings obtained with the CHIMERA and FARCOS devices is presented. |
| Databáze: |
Directory of Open Access Journals |
| Externí odkaz: |
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