Is the Structure of ^{42}Si Understood?


Journal

Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141

Informations de publication

Date de publication:
07 Jun 2019
Historique:
revised: 23 04 2019
received: 12 03 2019
entrez: 9 7 2019
pubmed: 10 7 2019
medline: 10 7 2019
Statut: ppublish

Résumé

A more detailed test of the implementation of nuclear forces that drive shell evolution in the pivotal nucleus ^{42}Si-going beyond earlier comparisons of excited-state energies-is important. The two leading shell-model effective interactions, SDPF-MU and SDPF-U-Si, both of which reproduce the low-lying ^{42}Si(2_{1}^{+}) energy, but whose predictions for other observables differ significantly, are interrogated by the population of states in neutron-rich ^{42}Si with a one-proton removal reaction from ^{43}P projectiles at 81  MeV/nucleon. The measured cross sections to the individual ^{42}Si final states are compared to calculations that combine eikonal reaction dynamics with these shell-model nuclear structure overlaps. The differences in the two shell-model descriptions are examined and linked to predicted low-lying excited 0^{+} states and shape coexistence. Based on the present data, which are in better agreement with the SDPF-MU calculations, the state observed at 2150(13) keV in ^{42}Si is proposed to be the (0_{2}^{+}) level.

Identifiants

pubmed: 31283300
doi: 10.1103/PhysRevLett.122.222501
doi:

Types de publication

Journal Article

Langues

eng

Pagination

222501

Auteurs

A Gade (A)

National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.

B A Brown (BA)

National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.

J A Tostevin (JA)

Department of Physics, University of Surrey, Guildford, Surrey GU2 7XH, United Kingdom.

D Bazin (D)

National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.

P C Bender (PC)

National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.

C M Campbell (CM)

Nuclear Science Division, Lawrence Berkeley National Laboratory, California 94720, USA.

H L Crawford (HL)

Nuclear Science Division, Lawrence Berkeley National Laboratory, California 94720, USA.

B Elman (B)

National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.

K W Kemper (KW)

Department of Physics, Florida State University, Tallahassee, Florida 32306, USA.

B Longfellow (B)

National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.

E Lunderberg (E)

National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.

D Rhodes (D)

National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.

D Weisshaar (D)

National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.

Classifications MeSH