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How Robust is the N=34 Subshell Closure? First Spectroscopy of ^{52}Ar.

Authors :
Liu HN
Obertelli A
Doornenbal P
Bertulani CA
Hagen G
Holt JD
Jansen GR
Morris TD
Schwenk A
Stroberg R
Achouri N
Baba H
Browne F
Calvet D
Château F
Chen S
Chiga N
Corsi A
Cortés ML
Delbart A
Gheller JM
Giganon A
Gillibert A
Hilaire C
Isobe T
Kobayashi T
Kubota Y
Lapoux V
Motobayashi T
Murray I
Otsu H
Panin V
Paul N
Rodriguez W
Sakurai H
Sasano M
Steppenbeck D
Stuhl L
Sun YL
Togano Y
Uesaka T
Wimmer K
Yoneda K
Aktas O
Aumann T
Chung LX
Flavigny F
Franchoo S
Gašparić I
Gerst RB
Gibelin J
Hahn KI
Kim D
Koiwai T
Kondo Y
Koseoglou P
Lee J
Lehr C
Linh BD
Lokotko T
MacCormick M
Moschner K
Nakamura T
Park SY
Rossi D
Sahin E
Sohler D
Söderström PA
Takeuchi S
Törnqvist H
Vaquero V
Wagner V
Wang S
Werner V
Xu X
Yamada H
Yan D
Yang Z
Yasuda M
Zanetti L
Source :
Physical review letters [Phys Rev Lett] 2019 Feb 22; Vol. 122 (7), pp. 072502.
Publication Year :
2019

Abstract

The first γ-ray spectroscopy of ^{52}Ar, with the neutron number N=34, was measured using the ^{53}K(p,2p) one-proton removal reaction at ∼210  MeV/u at the RIBF facility. The 2_{1}^{+} excitation energy is found at 1656(18) keV, the highest among the Ar isotopes with N>20. This result is the first experimental signature of the persistence of the N=34 subshell closure beyond ^{54}Ca, i.e., below the magic proton number Z=20. Shell-model calculations with phenomenological and chiral-effective-field-theory interactions both reproduce the measured 2_{1}^{+} systematics of neutron-rich Ar isotopes, and support a N=34 subshell closure in ^{52}Ar.

Details

Language :
English
ISSN :
1079-7114
Volume :
122
Issue :
7
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
30848641
Full Text :
https://doi.org/10.1103/PhysRevLett.122.072502