Predictions for production of superheavy nuclei with Z = 105–112 in hot fusion reactions
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Title
Predictions for production of superheavy nuclei with Z = 105–112 in hot fusion reactions
Authors
Keywords
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Journal
Nuclear Science and Techniques
Volume 29, Issue 11, Pages -
Publisher
Springer Nature America, Inc
Online
2018-09-26
DOI
10.1007/s41365-018-0501-2
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Note: Only part of the references are listed.- Influence of proton shell closure on the evaporation residue cross sections of superheavy nuclei
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- Superheavy nuclei from 48 Ca-induced reactions
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- Production cross sections of superheavy elementsZ=119and 120 in hot fusion reactions
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- (2012) Kosuke Morita et al. JOURNAL OF THE PHYSICAL SOCIETY OF JAPAN
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- ISOSPIN DEPENDENCE OF REACTIONS 48Ca+243-251Bk
- (2009) CAIWAN SHEN et al. INTERNATIONAL JOURNAL OF MODERN PHYSICS E-NUCLEAR PHYSICS
- Production of new superheavyZ=108–114nuclei withU238,Pu244, andCm248,250targets
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- Possibilities of production of neutron-deficient isotopes of U, Np, Pu, Am, Cm, and Cf in complete fusion reactions
- (2008) G. G. Adamian et al. PHYSICAL REVIEW C
- Observation of the3nEvaporation Channel in the Complete Hot-Fusion ReactionMg26+Cm248Leading to the New Superheavy NuclideHs271
- (2008) J. Dvorak et al. PHYSICAL REVIEW LETTERS
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