Simulation of fusion and quasi-fission in nuclear reactions leading to production of superheavy elements using the Constrained Molecular Dynamics model
- NázevTitle
- Simulation of fusion and quasi-fission in nuclear reactions leading to production of superheavy elements using the Constrained Molecular Dynamics modelSimulation of fusion and quasi-fission in nuclear reactions leading to production of superheavy elements using the Constrained Molecular Dynamics model
- Druh výsledkuResult type
- Článek v časopiseJournal article
- AutořiAuthors
- J. Klimo, M. Veselský, G. A. Souliotis, A. Bonasera
- DOIDOI
- 10.1016/j.nuclphysa.2019.121640
- Časopis / citaceJournal / citation
- Nuclear Physics A. 2019, 992 1-13. ISSN 0375-9474.
- RokYear
- 2019
- JazykLanguage
- eng
- WoSWoS
- 000497602500013
- ScopusScopus
- 2-s2.0-85072802011
- RIVRIV
- RIV/68407700:21670/19:00337621!RIV20-MSM-21670___
- ProjektProject
- Institucionální podpora na rozvoj výzkumné org.Institucionální podpora na rozvoj výzkumné org.
AbstraktAbstract
Fusion dynamics and the onset of quasi-fission in reactions, leading to production of superheavy nuclei are investigated using the constrained molecular dynamics model. Constraints on the parameters of the nuclear equation of state are derived from experimental fusion probabilities. The obtained constraint on the modulus of incompressibility of nuclear matter K-0 = 240 - 260 MeV is consistent with the results of previous study using the Boltzmann-Uehling-Uhlenbeck equation and also with constraints derived using the recent neutron star binary collision event GW170817. Unlike the modulus of incompressibility of symmetric nuclear matter, the stiffness of the density-dependence of symmetry energy influences the fusion probability only weakly. (C) 2019 Elsevier B.V. All rights reserved.
Fusion dynamics and the onset of quasi-fission in reactions, leading to production of superheavy nuclei are investigated using the constrained molecular dynamics model. Constraints on the parameters of the nuclear equation of state are derived from experimental fusion probabilities. The obtained constraint on the modulus of incompressibility of nuclear matter K-0 = 240 - 260 MeV is consistent with the results of previous study using the Boltzmann-Uehling-Uhlenbeck equation and also with constraints derived using the recent neutron star binary collision event GW170817. Unlike the modulus of incompressibility of symmetric nuclear matter, the stiffness of the density-dependence of symmetry energy influences the fusion probability only weakly. (C) 2019 Elsevier B.V. All rights reserved.