dc.contributor.author | Konieczka, M. | |
dc.contributor.author | Kortelainen, Markus | |
dc.contributor.author | Satuła, W. | |
dc.date.accessioned | 2018-03-26T09:18:00Z | |
dc.date.available | 2018-03-26T09:18:00Z | |
dc.date.issued | 2018 | |
dc.identifier.citation | Konieczka, M., Kortelainen, M., & Satuła, W. (2018). Gamow-Teller response in the configuration space of a density-functional-theory–rooted no-core configuration-interaction model. <i>Physical Review C</i>, <i>97</i>(3), Article 034310. <a href="https://doi.org/10.1103/physrevc.97.034310" target="_blank">https://doi.org/10.1103/physrevc.97.034310</a> | |
dc.identifier.other | CONVID_27938117 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/57420 | |
dc.description.abstract | Background: The atomic nucleus is a unique laboratory in which to study fundamental aspects of the electroweak interaction. This includes a question concerning in medium renormalization of the axial-vector current, which still lacks satisfactory explanation. Study of spin-isospin or Gamow-Teller (GT) response may provide valuable information on both the quenching of the axial-vector coupling constant as well as on nuclear structure and nuclear astrophysics.
Purpose: We have performed a seminal calculation of the GT response by using the no-core configuration-interaction approach rooted in multireference density functional theory (DFT-NCCI). The model treats properly isospin and rotational symmetries and can be applied to calculate both the nuclear spectra and transition rates in atomic nuclei, irrespectively of their mass and particle-number parity.
Methods: The DFT-NCCI calculation proceeds as follows: First, one builds a configuration space by computing relevant, for a given physical problem, (multi)particle-(multi)hole Slater determinants. Next, one applies the isospin and angular-momentum projections and performs the isospin and
K
mixing in order to construct a model space composed of linearly dependent states of good angular momentum. Eventually, one mixes the projected states by solving the Hill-Wheeler-Griffin equation.
Results: The method is applied to compute the GT strength distribution in selected
N
≈
Z
nuclei including the
p
-shell
8
Li
and
8
Be
nuclei and the
s
d
-shell well-deformed nucleus
24
Mg
. In order to demonstrate a flexibility of the approach we present also a calculation of the superallowed GT
β
decay in doubly-magic spherical
100
Sn
and the low-spin spectrum in
100
In
.
Conclusions: It is demonstrated that the DFT-NCCI model is capable of capturing the GT response satisfactorily well by using a relatively small configuration space, exhausting simultaneously the GT sum rule. The model, due to its flexibility and broad range of applicability, may either serve as a complement or even as an alternative to other theoretical approaches, including the conventional nuclear shell model. | |
dc.language.iso | eng | |
dc.publisher | American Physical Society | |
dc.relation.ispartofseries | Physical Review C | |
dc.subject.other | beta decay | |
dc.subject.other | electroweak interactions in nuclear physics | |
dc.subject.other | nuclear density functional theory | |
dc.title | Gamow-Teller response in the configuration space of a density-functional-theory–rooted no-core configuration-interaction model | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-201803191764 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.date.updated | 2018-03-19T13:15:16Z | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2469-9985 | |
dc.relation.numberinseries | 3 | |
dc.relation.volume | 97 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2018 American Physical Society. Published in this repository with the kind permission of the publisher. | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.relation.doi | 10.1103/physrevc.97.034310 | |
dc.type.okm | A1 | |