Journal
PHYSICAL REVIEW LETTERS
Volume 117, Issue 18, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.117.182503
Keywords
-
Categories
Funding
- Major State Basic Research Development Program of China [2013CB834401]
- National Key Program for S&T Research and Development [2016YFA0400504]
- NSFC [U1232208, U1432125, 11205205, 11035007, 11235001, 11320101004, 11575007]
- Chinese Academy of Sciences
- Helmholtz-CAS Joint Research Group [HCJRG-108]
- CAS President's International Fellowship Initiative [2016VMA043]
- Nuclear Astrophysics Virtual Institute (NAVI) of the Helmholtz Association
- Ministry of Science and Technology of China
- China Postdoctoral Science Foundation [2014M562481]
- CAS
- Grants-in-Aid for Scientific Research [26287036, 16K13799] Funding Source: KAKEN
Ask authors/readers for more resources
Masses of Co-52g,Co-52m were measured for the first time with an accuracy of similar to 10 keV, an unprecedented precision reached for short-lived nuclei in the isochronous mass spectrometry. Combining our results with the previous beta-gamma measurements of Ni-52, the T = 2, J(pi) = 0(+) isobaric analog state ( IAS) in Co-52 was newly assigned, questioning the conventional identification of IASs from the beta-delayed proton emissions. Using our energy of the IAS in Co-52, the masses of the T = 2 multiplet fit well into the isobaric multiplet mass equation. We find that the IAS in Co-52 decays predominantly via gamma transitions while the proton emission is negligibly small. According to our large-scale shell model calculations, this phenomenon has been interpreted to be due to very low isospin mixing in the IAS.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available