検索対象:     
報告書番号:
※ 半角英数字
 年 ~ 
 年
検索結果: 1 件中 1件目~1件目を表示
  • 1

発表形式

Initialising ...

選択項目を絞り込む

掲載資料名

Initialising ...

発表会議名

Initialising ...

筆頭著者名

Initialising ...

キーワード

Initialising ...

使用言語

Initialising ...

発行年

Initialising ...

開催年

Initialising ...

選択した検索結果をダウンロード

論文

Fusion-fission study at JAEA for heavy-element synthesis

西尾 勝久

Physics Procedia, 47, p.172 - 177, 2013/00

 被引用回数:0 パーセンタイル:0.04(Physics, Nuclear)

Fission fragment mass and kinetic energy distributions were measured in the reactions of $$^{30}$$Si,$$^{31}$$P,$$^{34,36}$$S,$$^{40}$$Ar,$$^{40,48}$$Ca + $$^{238}$$U at energies around the Coulomb barrier. The mass distributions changed drastically with incident energy. The results are explained by a change of the ratio between fusion and qasifission with nuclear orientation. A calculation based on a fluctuation dissipation model reproduced the mass distributions and their energy dependence. Fusion probabilities are defined as the ratio of fusion-fission events to the total fission events. They were used to determine the cross section to produce super-heavy nucleus (SHN) in a statistical model calculation. The calculated cross sections agreed with the experimental data for $$^{263,264}$$Sg and $$^{267,268}$$Hs produced in the reactions of $$^{30}$$Si + $$^{238}$$U and $$^{34}$$S + $$^{238}$$U, respectively. It is shown that the reaction at sub-barrier energies can be used for heavy element synthesis. In the measurement and analysis for $$^{48}$$Ca+$$^{238}$$U, we also estimated that the copernicium isotopes (Z=112) can be produced at lower incident energies than those used so far, suggested that more neutron rich SHN can be produced with smaller number of neutron evaporation.

1 件中 1件目~1件目を表示
  • 1