Record Details
Field | Value |
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Title | Predicting the production of neutron-rich heavy nuclei in multinucleon transfer reactions using a semi-classical model including evaporation and fission competition, GRAZING-F |
Names |
Yanez, R.
(creator) Loveland, W. (creator) |
Date Issued | 2015-04-09 (iso8601) |
Note | This is the publisher’s final pdf. The published article is copyrighted by the American Physical Society and can be found at: https://journals.aps.org/pra/. |
Abstract | Background: Multinucleon transfer reactions have recently attracted attention as a possible path to the synthesis of new neutron-rich heavy nuclei. Purpose: We study transfer reactions involving massive nuclei with the intention of understanding if the semi-classical model GRAZING coupled to an evaporation and fission competition model can satisfactorily reproduce experimental data on transfer reactions in which fission plays a role. Methods: We have taken the computer code GRAZING and have added fission competition to it (GRAZING-F) using our current understanding of Gamma(n)/Gamma(f), fission barriers, and level densities. Results: The code GRAZING-F seems to satisfactorily reproduce experimental data for +1p, +2p, and +3p transfers but has limitations in reproducing measurements of larger above-target and below-target transfers. Nonetheless, we use GRAZING-F to estimate production rates of neutron-rich N = 126 nuclei, actinides, and transactinides. Conclusions: The GRAZING code, with appropriate modifications to account for fission decay as well as neutron emission by excited primary fragments, does not predict large cross sections for multinucleon transfer reactions leading to neutron-rich transactinide nuclei but predicts opportunities to produce new neutron-rich actinide isotopes. |
Genre | Article |
Identifier | Yanez, R., & Loveland, W. (2015). Predicting the production of neutron-rich heavy nuclei in multinucleon transfer reactions using a semi-classical model including evaporation and fission competition, GRAZING-F. Physical Review C, 91(4), 044608. doi:10.1103/PhysRevC.91.044608 |