Investigating Shell Structure: Mass Measurements of Sc, Ti, and V Isotopes at new magic N = 32 and N = 34
ORAL
Abstract
*This work was supported by the Japan Society for the Promotion of Science KAKENHI (Grants No. 2200823, No. 24224008, No. 24740142, No. 15H02096, No. 15K05116, No. 17H01081, No. 17H06090, No. 18K13573, No. 18H05462, No. 19H00679, No. 19K14750, No. 20H05648, No. 21K13951, No. 22H01257, and No. 22H04946), RIKEN Junior Research Associate Program, the RIKEN programme for Evolution of Matter in the Universe (r-EMU), the UK STFC award ST/P003885/1, and the Royal Society. The MCSM and conventional shell-model calculations were performed on the supercomputer Fugaku at RIKEN AICS (hp210165, hp220174). This work was supported in part by MEXT as "Program for Promoting Researches on the Supercomputer Fugaku" (Simulation for basic science: from fundamental laws of particles to creation of nuclei) and by JICFuS.
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Publication: [1] "Study of the N = 32 and N = 34 Shell Gap for Ti and V by the First High-Precision Multireflection Time-of-Flight Mass Measurements at BigRIPS-SLOWRI" S. Iimura, M. Rosenbusch, A. Takamine et al., Physical Review Letters 130, 012501 (2023).
[2] "The new MRTOF mass spectrograph following the ZeroDegree spectrometer at RIKEN's RIBF facility" M. Rosenbusch et al., Nuclear Instruments and Methods in Physics Research Section A 1047 167824 (2022).
Presenters
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Shun Iimura
- Department of Physics, College of Science, Rikkyo University
- Rikkyo University
- RNC, RIKEN
- Department of Physics, Rikkyo University