Deutsch
 
Hilfe Datenschutzhinweis Impressum
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT
  Masses of neutron-rich 52–54Sc and 54,56Ti nuclides: The N=32 subshell closure in scandium

Xu, X., Wang, M., Blaum, K., Holt, J. D., Litvinov, Y. A., Schwenk, A., et al. (2019). Masses of neutron-rich 52–54Sc and 54,56Ti nuclides: The N=32 subshell closure in scandium. Physical Review C, 99(6): 064303. doi:10.1103/PhysRevC.99.064303.

Item is

Basisdaten

einblenden: ausblenden:
Genre: Zeitschriftenartikel

Dateien

einblenden: Dateien
ausblenden: Dateien
:
1905.12577.pdf (Preprint), 238KB
Name:
1905.12577.pdf
Beschreibung:
-
OA-Status:
Sichtbarkeit:
Öffentlich
MIME-Typ / Prüfsumme:
application/pdf / [MD5]
Technische Metadaten:
Copyright Datum:
-
Copyright Info:
-
Lizenz:
-

Externe Referenzen

einblenden:

Urheber

einblenden:
ausblenden:
 Urheber:
Xu, X.1, Autor
Wang, M.1, Autor
Blaum, Klaus2, Autor           
Holt, J. D.1, Autor
Litvinov, Yu. A.1, Autor
Schwenk, Achim2, Autor           
Simonis, J.1, Autor
Stroberg, S. R.1, Autor
Zhang, Y. H.1, Autor
Xu, H. S.1, Autor
Shuai, P.1, Autor
Tu, X. L.1, Autor
Zhou, X. H.1, Autor
Xu, F. R.1, Autor
Audi, G.1, Autor
Chen, R. J.1, Autor
Chen, X. C.1, Autor
Fu, C. Y.1, Autor
Ge, Z.1, Autor
Huang, Wenjia2, Autor           
Litvinov, S.1, AutorLiu, D. W.1, AutorLam, Y. H.1, AutorMa, X. W.1, AutorMao, R. S.1, AutorOzawa, A.1, AutorSun, B. H.1, AutorSun, Y.1, AutorUesaka, T.1, AutorXiao, G. Q.1, AutorXing, Y. M.1, AutorYamaguchi, T.1, AutorYamaguchi, Y.1, AutorYan, X. L.1, AutorZeng, Q.1, AutorZhao, H. W.1, AutorZhao, T. C.1, AutorZhang, W.1, AutorZhan, W. L.1, Autor mehr..
Affiliations:
1Key Laboratory of High Precision Nuclear Spectroscopy and Center for Nuclear Matter Science, Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, People's Republic of China School of Science, Xi′an Jiaotong University, Xi′an 710049, China TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada GSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, Germany Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany Institut für Kernphysik and PRISMA Cluster of Excellence, Johannes Gutenberg-Universität, 55099 Mainz, Germany Reed College, Portland, 97202 Oregon, USA State Key Laboratory of Nuclear Physics and Technology, School of Physics, Peking University, Beijing 100871, People's Republic of China CSNSM-IN2P3-CNRS, Université de Paris Sud, 91405 Orsay, France Insititute of Physics, University of Tsukuba, Ibaraki 305-8571, Japan School of Physics and Nuclear Energy Engineering, Beihang University, Beijing 100191, People's Republic of China Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, People's Republic of China RIKEN Nishina Center, RIKEN, Saitama 351-0198, Japan Department of Physics, Saitama University, Saitama 338-8570, Japan, ou_persistent22              
2Division Prof. Dr. Klaus Blaum, MPI for Nuclear Physics, Max Planck Society, ou_904548              

Inhalt

einblenden:
ausblenden:
Schlagwörter: -
 MPINP: Präzisionsexperimente - Abteilung Blaum
 Zusammenfassung: Isochronous mass spectrometry has been applied in the storage ring CSRe to measure the masses of the neutron-rich 52–54Sc and 54,56Ti nuclei. The new mass excess values ME(52Sc)=−40525(65) keV, ME(53Sc)=−38910(80) keV, and ME(54Sc)=−34485(360) keV, deviate from the Atomic Mass Evaluation 2012 by 2.3σ, 2.8σ, and 1.7σ, respectively. These large deviations significantly change the systematics of the two-neutron separation energies of scandium isotopes. The empirical shell gap extracted from our new experimental results shows a significant subshell closure at N=32 in scandium, with a similar magnitude as in calcium. Moreover, we present ab initio calculations using the valence-space in-medium similarity renormalization group based on two- and three-nucleon interactions from chiral effective field theory. The theoretical results confirm the existence of a substantial N=32 shell gap in Sc and Ca with a decreasing trend towards lighter isotones, thus providing a consistent picture of the evolution of the N=32 magic number from the pf into the sd shell.

Details

einblenden:
ausblenden:
Sprache(n):
 Datum: 2019-06-03
 Publikationsstatus: Online veröffentlicht
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: Expertenbegutachtung
 Identifikatoren: DOI: 10.1103/PhysRevC.99.064303
 Art des Abschluß: -

Veranstaltung

einblenden:

Entscheidung

einblenden:

Projektinformation

einblenden:

Quelle 1

einblenden:
ausblenden:
Titel: Physical Review C
  Andere : Phys. Rev. C
Genre der Quelle: Zeitschrift
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: New York, NY : American Physical Society
Seiten: - Band / Heft: 99 (6) Artikelnummer: 064303 Start- / Endseite: - Identifikator: ISSN: 0556-2813
CoNE: https://pure.mpg.de/cone/journals/resource/954925225009