g Factor of the 7− isomer in 126Sn and first observation of spin-alignment in relativistic fission
We report on the g factor measurement of the isomeric 7− state (E*=2219 keV, T1/2=5.9(8) μs) in the neutron-rich 126Sn nucleus. The nucleus was produced by the fission of a relativistic 238U beam and reaction products were selected by the FRS fragment separator at GSI. For the first time, spin-align...
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| creator | Ilie, G. Neyens, G. Simpson, G.S. Jolie, J. Blazhev, A. Grawe, H. Lozeva, R.L. Vermeulen, N. Atanasova, L. Balabanski, D.L. Becker, F. Bednarczyk, P. Brandau, C. Caceres, L. Chamoli, S.K. Daugas, J.M. Doornenbal, P. Gerl, J. Górska, M. Grȩbosz, J. Hass, M. Ionescu-Bujor, M. Jungclaus, A. Kmiecik, M. Kojouharov, I. Kurz, N. Maj, A. Mallion, S. Perru, O. Pfützner, M. Podolyák, Zs Prokopowicz, W. De Rydt, M. Saito, T.R. Schaffner, H. Turzó, K. Walker, J. Werner-Malento, E. Wollersheim, H.J. |
| description | We report on the g factor measurement of the isomeric 7− state (E*=2219 keV, T1/2=5.9(8) μs) in the neutron-rich 126Sn nucleus. The nucleus was produced by the fission of a relativistic 238U beam and reaction products were selected by the FRS fragment separator at GSI. For the first time, spin-alignment was observed after relativistic fission. It was used to deduce the g factor of the 7− isomeric state, g(7−)=−0.098(9), from the measured perturbed angular distribution of its γ decay using the RISING Cluster detectors. The observed value confirms the suggested ν(h11/2−1d3/2−1) dominant configuration, which has been proposed for the 7− isomers in neutron-rich Sn isotopes. The failure of the g factor additivity rule and the importance of core polarization evolution with increasing distance from the doubly-magic 132Sn is discussed. The first observation of 18(8)% of spin-alignment produced by the relativistic fission of a 238U beam paves the way to study moments of neutron-rich (sub-)microsecond isomers, which are difficult to align by other means. |
| doi_str_mv | 10.1016/j.physletb.2010.03.033 |
| format | Article |
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The nucleus was produced by the fission of a relativistic 238U beam and reaction products were selected by the FRS fragment separator at GSI. For the first time, spin-alignment was observed after relativistic fission. It was used to deduce the g factor of the 7− isomeric state, g(7−)=−0.098(9), from the measured perturbed angular distribution of its γ decay using the RISING Cluster detectors. The observed value confirms the suggested ν(h11/2−1d3/2−1) dominant configuration, which has been proposed for the 7− isomers in neutron-rich Sn isotopes. The failure of the g factor additivity rule and the importance of core polarization evolution with increasing distance from the doubly-magic 132Sn is discussed. The first observation of 18(8)% of spin-alignment produced by the relativistic fission of a 238U beam paves the way to study moments of neutron-rich (sub-)microsecond isomers, which are difficult to align by other means.</description><identifier>ISSN: 0370-2693</identifier><identifier>EISSN: 1873-2445</identifier><identifier>DOI: 10.1016/j.physletb.2010.03.033</identifier><identifier>CODEN: PYLBAJ</identifier><language>eng</language><publisher>Kidlington: Elsevier B.V</publisher><subject>Exact sciences and technology ; Lifetimes ; Nuclear moments ; Nuclear physics ; Nuclear Theory ; Physics ; Projectile fission reactions ; Shell model calculations ; The physics of elementary particles and fields</subject><ispartof>Physics letters. 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B</title><description>We report on the g factor measurement of the isomeric 7− state (E*=2219 keV, T1/2=5.9(8) μs) in the neutron-rich 126Sn nucleus. The nucleus was produced by the fission of a relativistic 238U beam and reaction products were selected by the FRS fragment separator at GSI. For the first time, spin-alignment was observed after relativistic fission. It was used to deduce the g factor of the 7− isomeric state, g(7−)=−0.098(9), from the measured perturbed angular distribution of its γ decay using the RISING Cluster detectors. The observed value confirms the suggested ν(h11/2−1d3/2−1) dominant configuration, which has been proposed for the 7− isomers in neutron-rich Sn isotopes. The failure of the g factor additivity rule and the importance of core polarization evolution with increasing distance from the doubly-magic 132Sn is discussed. The first observation of 18(8)% of spin-alignment produced by the relativistic fission of a 238U beam paves the way to study moments of neutron-rich (sub-)microsecond isomers, which are difficult to align by other means.</description><subject>Exact sciences and technology</subject><subject>Lifetimes</subject><subject>Nuclear moments</subject><subject>Nuclear physics</subject><subject>Nuclear Theory</subject><subject>Physics</subject><subject>Projectile fission reactions</subject><subject>Shell model calculations</subject><subject>The physics of elementary particles and fields</subject><issn>0370-2693</issn><issn>1873-2445</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNqFkM1qGzEQx0VJoM7HKwRdcgrrjKS15L0lhLoJGHpochZaaWTLrLWLtCzkDXLuI_ZJqsVtroWBgZn_bz7-hNwwWDJg8v6wHPbvucOxXXIoRRAlxBeyYGslKl7XqzOyAKGg4rIRX8lFzgcAYCuQC-J2dGPs2CfaezrukarfH79oyP0REw2RMi5_Rmqioz6kPNK-zZgmM4Y-zkQeQqxMF3bxiHGcgYRd6U4hj8EWJueivCLn3nQZr__mS_K2-fb69Fxtf3x_eXrcVpZzoap1rbyRrpGmlYjO1gYZB8FsW4NT2FjusV2ja1vpW66Usw7FmoG3vmnAKHFJ7k5z96bTQwpHk951b4J-ftzqEPkgNECtQNRyYkUtT2qb-pwT-k-EgZ6d1Qf9z1k9O6uh8EIU8PYEDiZb0_lkog35k-ZcilXN5nMeTjosP08Bk842YLToQkI7ateH_636A8HjlAM</recordid><startdate>20100419</startdate><enddate>20100419</enddate><creator>Ilie, G.</creator><creator>Neyens, G.</creator><creator>Simpson, G.S.</creator><creator>Jolie, J.</creator><creator>Blazhev, A.</creator><creator>Grawe, H.</creator><creator>Lozeva, R.L.</creator><creator>Vermeulen, N.</creator><creator>Atanasova, L.</creator><creator>Balabanski, D.L.</creator><creator>Becker, F.</creator><creator>Bednarczyk, P.</creator><creator>Brandau, C.</creator><creator>Caceres, L.</creator><creator>Chamoli, S.K.</creator><creator>Daugas, J.M.</creator><creator>Doornenbal, P.</creator><creator>Gerl, J.</creator><creator>Górska, M.</creator><creator>Grȩbosz, J.</creator><creator>Hass, M.</creator><creator>Ionescu-Bujor, M.</creator><creator>Jungclaus, A.</creator><creator>Kmiecik, M.</creator><creator>Kojouharov, I.</creator><creator>Kurz, N.</creator><creator>Maj, A.</creator><creator>Mallion, S.</creator><creator>Perru, O.</creator><creator>Pfützner, M.</creator><creator>Podolyák, Zs</creator><creator>Prokopowicz, W.</creator><creator>De Rydt, M.</creator><creator>Saito, T.R.</creator><creator>Schaffner, H.</creator><creator>Turzó, K.</creator><creator>Walker, J.</creator><creator>Werner-Malento, E.</creator><creator>Wollersheim, H.J.</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>6I.</scope><scope>AAFTH</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0002-1142-8067</orcidid><orcidid>https://orcid.org/0000-0003-0495-2028</orcidid></search><sort><creationdate>20100419</creationdate><title>g Factor of the 7− isomer in 126Sn and first observation of spin-alignment in relativistic fission</title><author>Ilie, G. ; Neyens, G. ; Simpson, G.S. ; Jolie, J. ; Blazhev, A. ; Grawe, H. ; Lozeva, R.L. ; Vermeulen, N. ; Atanasova, L. ; Balabanski, D.L. ; Becker, F. ; Bednarczyk, P. ; Brandau, C. ; Caceres, L. ; Chamoli, S.K. ; Daugas, J.M. ; Doornenbal, P. ; Gerl, J. ; Górska, M. ; Grȩbosz, J. ; Hass, M. ; Ionescu-Bujor, M. ; Jungclaus, A. ; Kmiecik, M. ; Kojouharov, I. ; Kurz, N. ; Maj, A. ; Mallion, S. ; Perru, O. ; Pfützner, M. ; Podolyák, Zs ; Prokopowicz, W. ; De Rydt, M. ; Saito, T.R. ; Schaffner, H. ; Turzó, K. ; Walker, J. ; Werner-Malento, E. ; Wollersheim, H.J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c2237-847fa6d96ab6eedc4ae12031cb40d7e9c2feb8edbb6fb277dcde3810fcf990a73</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Exact sciences and technology</topic><topic>Lifetimes</topic><topic>Nuclear moments</topic><topic>Nuclear physics</topic><topic>Nuclear Theory</topic><topic>Physics</topic><topic>Projectile fission reactions</topic><topic>Shell model calculations</topic><topic>The physics of elementary particles and fields</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Ilie, G.</creatorcontrib><creatorcontrib>Neyens, G.</creatorcontrib><creatorcontrib>Simpson, G.S.</creatorcontrib><creatorcontrib>Jolie, J.</creatorcontrib><creatorcontrib>Blazhev, A.</creatorcontrib><creatorcontrib>Grawe, H.</creatorcontrib><creatorcontrib>Lozeva, R.L.</creatorcontrib><creatorcontrib>Vermeulen, N.</creatorcontrib><creatorcontrib>Atanasova, L.</creatorcontrib><creatorcontrib>Balabanski, D.L.</creatorcontrib><creatorcontrib>Becker, F.</creatorcontrib><creatorcontrib>Bednarczyk, P.</creatorcontrib><creatorcontrib>Brandau, C.</creatorcontrib><creatorcontrib>Caceres, L.</creatorcontrib><creatorcontrib>Chamoli, S.K.</creatorcontrib><creatorcontrib>Daugas, J.M.</creatorcontrib><creatorcontrib>Doornenbal, P.</creatorcontrib><creatorcontrib>Gerl, J.</creatorcontrib><creatorcontrib>Górska, M.</creatorcontrib><creatorcontrib>Grȩbosz, J.</creatorcontrib><creatorcontrib>Hass, M.</creatorcontrib><creatorcontrib>Ionescu-Bujor, M.</creatorcontrib><creatorcontrib>Jungclaus, A.</creatorcontrib><creatorcontrib>Kmiecik, M.</creatorcontrib><creatorcontrib>Kojouharov, I.</creatorcontrib><creatorcontrib>Kurz, N.</creatorcontrib><creatorcontrib>Maj, A.</creatorcontrib><creatorcontrib>Mallion, S.</creatorcontrib><creatorcontrib>Perru, O.</creatorcontrib><creatorcontrib>Pfützner, M.</creatorcontrib><creatorcontrib>Podolyák, Zs</creatorcontrib><creatorcontrib>Prokopowicz, W.</creatorcontrib><creatorcontrib>De Rydt, M.</creatorcontrib><creatorcontrib>Saito, T.R.</creatorcontrib><creatorcontrib>Schaffner, H.</creatorcontrib><creatorcontrib>Turzó, K.</creatorcontrib><creatorcontrib>Walker, J.</creatorcontrib><creatorcontrib>Werner-Malento, E.</creatorcontrib><creatorcontrib>Wollersheim, H.J.</creatorcontrib><collection>ScienceDirect Open Access Titles</collection><collection>Elsevier:ScienceDirect:Open Access</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Physics letters. 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B</jtitle><date>2010-04-19</date><risdate>2010</risdate><volume>687</volume><issue>4-5</issue><spage>305</spage><epage>309</epage><pages>305-309</pages><issn>0370-2693</issn><eissn>1873-2445</eissn><coden>PYLBAJ</coden><abstract>We report on the g factor measurement of the isomeric 7− state (E*=2219 keV, T1/2=5.9(8) μs) in the neutron-rich 126Sn nucleus. The nucleus was produced by the fission of a relativistic 238U beam and reaction products were selected by the FRS fragment separator at GSI. For the first time, spin-alignment was observed after relativistic fission. It was used to deduce the g factor of the 7− isomeric state, g(7−)=−0.098(9), from the measured perturbed angular distribution of its γ decay using the RISING Cluster detectors. The observed value confirms the suggested ν(h11/2−1d3/2−1) dominant configuration, which has been proposed for the 7− isomers in neutron-rich Sn isotopes. The failure of the g factor additivity rule and the importance of core polarization evolution with increasing distance from the doubly-magic 132Sn is discussed. The first observation of 18(8)% of spin-alignment produced by the relativistic fission of a 238U beam paves the way to study moments of neutron-rich (sub-)microsecond isomers, which are difficult to align by other means.</abstract><cop>Kidlington</cop><pub>Elsevier B.V</pub><doi>10.1016/j.physletb.2010.03.033</doi><tpages>5</tpages><orcidid>https://orcid.org/0000-0002-1142-8067</orcidid><orcidid>https://orcid.org/0000-0003-0495-2028</orcidid><oa>free_for_read</oa></addata></record> |
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| subjects | Exact sciences and technology Lifetimes Nuclear moments Nuclear physics Nuclear Theory Physics Projectile fission reactions Shell model calculations The physics of elementary particles and fields |
| title | g Factor of the 7− isomer in 126Sn and first observation of spin-alignment in relativistic fission |
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