ROTATIONAL BANDS IN DOUBLY ODD 116Sb
- D. P. SUN,
- S. Y. WANG,
- B. QI,
- C. LIU,
- C. J. XU,
- M. Z. GUO,
- Y. Y. CAI,
- L. W. DUAN,
- G. WANG,
- X. B. HU,
- Y. Q. LI,
- L. LIU,
- H. HUA,
- Z. Y. LI,
- L. H. ZHU,
- X. G. WU,
- G. S. LI,
- C. Y. HE,
- Y. LIU,
- X. Q. LI,
- Y. ZHENG,
- L. L. WANG, and
- L. WANG
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, People's Republic of China
School of Physics, and SK Lab. of Nucl. Phys. & Tech., Peking University, Beijing 100871, People's Republic of China
School of Physics, and SK Lab. of Nucl. Phys. & Tech., Peking University, Beijing 100871, People's Republic of China
China Institute of Atomic Energy, Beijing 102413, People's Republic of China
China Institute of Atomic Energy, Beijing 102413, People's Republic of China
China Institute of Atomic Energy, Beijing 102413, People's Republic of China
China Institute of Atomic Energy, Beijing 102413, People's Republic of China
China Institute of Atomic Energy, Beijing 102413, People's Republic of China
China Institute of Atomic Energy, Beijing 102413, People's Republic of China
China Institute of Atomic Energy, Beijing 102413, People's Republic of China
China Institute of Atomic Energy, Beijing 102413, People's Republic of China
China Institute of Atomic Energy, Beijing 102413, People's Republic of China
High spin states of 116Sb were populated using the 114Cd(7Li, 5n) fusion evaporation reaction at a beam energy of 48 MeV. The previously reported rotational bands, built on πg9/2 ⊗ νh11/2 and πg9/2 ⊗ νd5/2 configurations, have been extended and a new ΔI = 1 band has been identified.