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Nuclear spins, magnetic moments and quadrupole moments of Cu isotopes from N = 28 to N = 46: probes for core polarization effects

Measurements of the ground-state nuclear spins, magnetic and quadrupole moments of the copper isotopes from 61Cu up to 75Cu are reported. The experiments were performed at the ISOLDE facility, using the technique of collinear laser spectroscopy. The trend in the magnetic moments between the N=28 and...

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Autores principales: Vingerhoets, P., Flanagan, K.T., Avgoulea, M., Billowes, J., Bissell, M.L., Blaum, K., Brown, B.A., Cheal, B., De Rydt, M., Forest, D.H., Geppert, Ch., Honma, M., Kowalska, M., Kramer, J., Krieger, A., Mane, E., Neugart, R., Neyens, G., Nortershauser, W., Otsuka, T., Schug, M., Stroke, H.H., Tungate, G., Yordanov, D.T.
Lenguaje:eng
Publicado: 2010
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevC.82.064311
http://cds.cern.ch/record/1309766
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author Vingerhoets, P.
Flanagan, K.T.
Avgoulea, M.
Billowes, J.
Bissell, M.L.
Blaum, K.
Brown, B.A.
Cheal, B.
De Rydt, M.
Forest, D.H.
Geppert, Ch.
Honma, M.
Kowalska, M.
Kramer, J.
Krieger, A.
Mane, E.
Neugart, R.
Neyens, G.
Nortershauser, W.
Otsuka, T.
Schug, M.
Stroke, H.H.
Tungate, G.
Yordanov, D.T.
author_facet Vingerhoets, P.
Flanagan, K.T.
Avgoulea, M.
Billowes, J.
Bissell, M.L.
Blaum, K.
Brown, B.A.
Cheal, B.
De Rydt, M.
Forest, D.H.
Geppert, Ch.
Honma, M.
Kowalska, M.
Kramer, J.
Krieger, A.
Mane, E.
Neugart, R.
Neyens, G.
Nortershauser, W.
Otsuka, T.
Schug, M.
Stroke, H.H.
Tungate, G.
Yordanov, D.T.
author_sort Vingerhoets, P.
collection CERN
description Measurements of the ground-state nuclear spins, magnetic and quadrupole moments of the copper isotopes from 61Cu up to 75Cu are reported. The experiments were performed at the ISOLDE facility, using the technique of collinear laser spectroscopy. The trend in the magnetic moments between the N=28 and N=50 shell closures is reasonably reproduced by large-scale shell-model calculations starting from a 56Ni core. The quadrupole moments reveal a strong polarization of the underlying Ni core when the neutron shell is opened, which is however strongly reduced at N=40 due to the parity change between the $pf$ and $g$ orbits. No enhanced core polarization is seen beyond N=40. Deviations between measured and calculated moments are attributed to the softness of the 56Ni core and weakening of the Z=28 and N=28 shell gaps.
id cern-1309766
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2010
record_format invenio
spelling cern-13097662023-03-14T19:11:22Zdoi:10.1103/PhysRevC.82.064311http://cds.cern.ch/record/1309766engVingerhoets, P.Flanagan, K.T.Avgoulea, M.Billowes, J.Bissell, M.L.Blaum, K.Brown, B.A.Cheal, B.De Rydt, M.Forest, D.H.Geppert, Ch.Honma, M.Kowalska, M.Kramer, J.Krieger, A.Mane, E.Neugart, R.Neyens, G.Nortershauser, W.Otsuka, T.Schug, M.Stroke, H.H.Tungate, G.Yordanov, D.T.Nuclear spins, magnetic moments and quadrupole moments of Cu isotopes from N = 28 to N = 46: probes for core polarization effectsNuclear Physics - ExperimentMeasurements of the ground-state nuclear spins, magnetic and quadrupole moments of the copper isotopes from 61Cu up to 75Cu are reported. The experiments were performed at the ISOLDE facility, using the technique of collinear laser spectroscopy. The trend in the magnetic moments between the N=28 and N=50 shell closures is reasonably reproduced by large-scale shell-model calculations starting from a 56Ni core. The quadrupole moments reveal a strong polarization of the underlying Ni core when the neutron shell is opened, which is however strongly reduced at N=40 due to the parity change between the $pf$ and $g$ orbits. No enhanced core polarization is seen beyond N=40. Deviations between measured and calculated moments are attributed to the softness of the 56Ni core and weakening of the Z=28 and N=28 shell gaps.Measurements of the ground-state nuclear spins, magnetic and quadrupole moments of the copper isotopes from 61Cu up to 75Cu are reported. The experiments were performed at the ISOLDE facility, using the technique of collinear laser spectroscopy. The trend in the magnetic moments between the N=28 and N=50 shell closures is reasonably reproduced by large-scale shell-model calculations starting from a 56Ni core. The quadrupole moments reveal a strong polarization of the underlying Ni core when the neutron shell is opened, which is however strongly reduced at N=40 due to the parity change between the $pf$ and $g$ orbits. No enhanced core polarization is seen beyond N=40. Deviations between measured and calculated moments are attributed to the softness of the 56Ni core and weakening of the Z=28 and N=28 shell gaps.arXiv:1011.5420oai:cds.cern.ch:13097662010-11-25
spellingShingle Nuclear Physics - Experiment
Vingerhoets, P.
Flanagan, K.T.
Avgoulea, M.
Billowes, J.
Bissell, M.L.
Blaum, K.
Brown, B.A.
Cheal, B.
De Rydt, M.
Forest, D.H.
Geppert, Ch.
Honma, M.
Kowalska, M.
Kramer, J.
Krieger, A.
Mane, E.
Neugart, R.
Neyens, G.
Nortershauser, W.
Otsuka, T.
Schug, M.
Stroke, H.H.
Tungate, G.
Yordanov, D.T.
Nuclear spins, magnetic moments and quadrupole moments of Cu isotopes from N = 28 to N = 46: probes for core polarization effects
title Nuclear spins, magnetic moments and quadrupole moments of Cu isotopes from N = 28 to N = 46: probes for core polarization effects
title_full Nuclear spins, magnetic moments and quadrupole moments of Cu isotopes from N = 28 to N = 46: probes for core polarization effects
title_fullStr Nuclear spins, magnetic moments and quadrupole moments of Cu isotopes from N = 28 to N = 46: probes for core polarization effects
title_full_unstemmed Nuclear spins, magnetic moments and quadrupole moments of Cu isotopes from N = 28 to N = 46: probes for core polarization effects
title_short Nuclear spins, magnetic moments and quadrupole moments of Cu isotopes from N = 28 to N = 46: probes for core polarization effects
title_sort nuclear spins, magnetic moments and quadrupole moments of cu isotopes from n = 28 to n = 46: probes for core polarization effects
topic Nuclear Physics - Experiment
url https://dx.doi.org/10.1103/PhysRevC.82.064311
http://cds.cern.ch/record/1309766
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