dc.contributor.author | Kostensalo, Joel | |
dc.contributor.author | Suhonen, Jouni | |
dc.date.accessioned | 2017-09-04T10:53:29Z | |
dc.date.available | 2017-09-04T10:53:29Z | |
dc.date.issued | 2017 | |
dc.identifier.citation | Kostensalo, J., & Suhonen, J. (2017). gA-driven shapes of electron spectra of forbidden β decays in the nuclear shell model. <i>Physical Review C</i>, <i>96</i>(2), Article 024317. <a href="https://doi.org/10.1103/PhysRevC.96.024317" target="_blank">https://doi.org/10.1103/PhysRevC.96.024317</a> | |
dc.identifier.other | CONVID_27175511 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/55268 | |
dc.description.abstract | The evolution of the shape of the electron spectra of 16 forbidden β− decays as a function of gA was studied using the nuclear shell model in appropriate single-particle model spaces with established, well-tested nuclear Hamiltonians. The β spectra of 94Nb(6+)→94Mo(4+) and 98Tc(6+)→98Ru(4+) were found to depend strongly on gA, which makes them excellent candidates for the determination of the effective value of gA with the spectrum-shape method (SSM). A strong gA dependence is also seen in the spectrum of 96Zr(0+)→96Nb(6+). This decay could be used for determining the quenching of gA in sixth-forbidden decays in the future, when the measurement of the spectrum becomes experimentally feasible. The calculated shell-model electron spectra of the ground-state-to-ground-state decays of 87Rb, 99Tc, and 137Cs and the decay of 137Cs to the isomeric 11/2− state in 137Ba were found to be in excellent agreement with the spectra previously calculated using the microscopic quasiparticle-phonon model. This is further evidence of the robust nature of the SSM observed in the previous studies. | |
dc.language.iso | eng | |
dc.publisher | American Physical Society | |
dc.relation.ispartofseries | Physical Review C | |
dc.subject.other | nuclear shell model | |
dc.title | gA-driven shapes of electron spectra of forbidden β decays in the nuclear shell model | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-201709013643 | |
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 | 2017-09-01T12:15:18Z | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2469-9985 | |
dc.relation.numberinseries | 2 | |
dc.relation.volume | 96 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2017 American Physical Society. Published in this repository with the kind permission of the publisher. | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.subject.yso | elektronit | |
dc.subject.yso | ydinfysiikka | |
dc.subject.yso | spektrit | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p4030 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p6086 | |
dc.relation.doi | 10.1103/PhysRevC.96.024317 | |
dc.type.okm | A1 | |