Back to Search Start Over

Proton Shell Gaps in N=28 Nuclei from the First Complete Spectroscopy Study with FRIB Decay Station Initiator.

Authors :
Cox I
Xu ZY
Grzywacz R
Ong WJ
Rasco BC
Kitamura N
Hoskins D
Neupane S
Ruland TJ
Allmond JM
King TT
Lubna RS
Rykaczewski KP
Schatz H
Sherrill BM
Tarasov OB
Ayangeakaa AD
Berg HC
Bleuel DL
Cerizza G
Christie J
Chester A
Davis J
Dembski C
Doetsch AA
Duarte JG
Estrade A
Fijałkowska A
Gray TJ
Good EC
Haak K
Hanai S
Harke JT
Harris C
Hermansen K
Hoff DEM
Jain R
Karny M
Kolos K
Laminack A
Liddick SN
Longfellow B
Lyons S
Madurga M
Mogannam MJ
Nowicki A
Ogunbeku TH
Owens-Fryar G
Rajabali MM
Richard AL
Ronning EK
Rose GE
Siegl K
Singh M
Spyrou A
Sweet A
Tsantiri A
Walters WB
Yokoyama R
Source :
Physical review letters [Phys Rev Lett] 2024 Apr 12; Vol. 132 (15), pp. 152503.
Publication Year :
2024

Abstract

The first complete measurement of the β-decay strength distribution of _{17}^{45}Cl_{28} was performed at the Facility for Rare Isotope Beams (FRIB) with the FRIB Decay Station Initiator during the second FRIB experiment. The measurement involved the detection of neutrons and γ rays in two focal planes of the FRIB Decay Station Initiator in a single experiment for the first time. This enabled an analytical consistency in extracting the β-decay strength distribution over the large range of excitation energies, including neutron unbound states. We observe a rapid increase in the β-decay strength distribution above the neutron separation energy in _{18}^{45}Ar_{27}. This was interpreted to be caused by the transitioning of neutrons into protons excited across the Z=20 shell gap. The SDPF-MU interaction with reduced shell gap best reproduced the data. The measurement demonstrates a new approach that is sensitive to the proton shell gap in neutron rich nuclei according to SDPF-MU calculations.

Details

Language :
English
ISSN :
1079-7114
Volume :
132
Issue :
15
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
38682970
Full Text :
https://doi.org/10.1103/PhysRevLett.132.152503