Calculation of the evaporation residue cross sections for the synthesis of the superheavy element Z=119 via the 50Ti+249Bk hot fusion reaction
Creators
- 1. China Institute of Atomic Energy, Beijing 102413 (China)
- 2. Center of Theoretical Nuclear Physics, National Laboratory of Heavy Ion Accelerator, Lanzhou 730000 (China)
- 3. Department of Physics, Beijing Normal University, Beijing 100875 (China)
Description
The evaporation residue (ER) cross sections for 3n and 4n evaporation channels in the 50Ti + 249Bk reaction leading the formation of 296119 and 295119 isotopes are evaluated by means of a modified fusion-by-diffusion model. In the model, the dynamic evolution from dinucleus to mononucleus is taken into account with the two-dimensional coupled Langenvin equations. The calculated maximum ER cross sections in 3n and 4n evaporation channels of the 50Ti + 249Bk reaction are 0.17 and 0.57 pb, respectively. The cross section of 0.57 pb is close to the present experimental limit for the registration of the evaporation residual nuclei. Therefore, superheavy element 119 may be the most hopeful new element with Z>118 to be synthesized under somehow improved experimental conditions in the near future.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 84
- Journal Issue
- 3
- Journal Page Range
- p. 031602-031602.4
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43074382
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- BERKELIUM 249 TARGET; COMPUTERIZED SIMULATION; CROSS SECTIONS; DIFFUSION; ELEMENT 119; ELEMENT 119 ISOTOPES; EVOLUTION; SYNTHESIS; TITANIUM 50 REACTIONS; TWO-DIMENSIONAL CALCULATIONS
- Descriptors DEC
- ELEMENTS; HEAVY ION REACTIONS; ISOTOPES; NUCLEAR REACTIONS; SIMULATION; TARGETS; TRANSACTINIDE ELEMENTS; TRANSPLUTONIUM ELEMENTS; TRANSURANIUM ELEMENTS
Optional Information
- Notes
- (c) 2011 American Institute of Physics