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Title: High-spin structure of Xe 134

Abstract

Detailed spectroscopic information on the N~82 nuclei is necessary to benchmark shell-model calculations in the region. The nuclear structure above long-lived isomers in 134Xe is investigated after multinucleon transfer (MNT) and actinide fission. Xenon-134 was populated as (i) a transfer product in 136Xe+238U and 136Xe+208Pb MNT reactions and (ii) as a fission product in the 136Xe+238U reaction employing the high-resolution Advanced Gamma Tracking Array (AGATA). Trajectory reconstruction has been applied for the complete identification of beamlike transfer products with the magnetic spectrometer PRISMA. The 136Xe+198Pt MNT reaction was studied with the γ-ray spectrometer GAMMASPHERE in combination with the gas detector array Compact Heavy Ion Counter (CHICO). Several high-spin states in 134Xe on top of the two long-lived isomers are discovered based on γγ-coincidence relationships and information on the γ-ray angular distributions as well as excitation energies from the total kinetic energy loss and fission fragments. The revised level scheme of 134Xe is extended up to an excitation energy of 5.832 MeV with tentative spin-parity assignments up to 16+. Previous assignments of states above the 7- isomer are revised. Latest shell-model calculations employing two different effective interactions reproduce the experimental findings and support the new spin and parity assignments.

Authors:
 [1];  [1];  [1];  [1];  [2];  [3];  [4];  [5];  [6];  [7];  [8];  [9];  [10];  [11];  [3];  [7];  [12];  [3];  [1];  [12] more »;  [5];  [3];  [9];  [13];  [1];  [6];  [14];  [7];  [15];  [3];  [11];  [1];  [11];  [16];  [1];  [17];  [18];  [12];  [7];  [10];  [16];  [12];  [5];  [19];  [20];  [21];  [20];  [20];  [3];  [6];  [7];  [6];  [22];  [7];  [1];  [20];  [23];  [3];  [20];  [24];  [10];  [14];  [3];  [1];  [25];  [21];  [11];  [11];  [5];  [7];  [12];  [26];  [1];  [11] « less
+ Show Author Affiliations
  1. Univ. zu Koln (Germany)
  2. Univ. di Padova (Italy); National Inst. of Nuclear Physics (INFN), Legnaro (Italy). National Lab. of Legnaro (INFN-LNL)
  3. National Inst. of Nuclear Physics (INFN), Legnaro (Italy). National Lab. of Legnaro (INFN-LNL)
  4. Univ. of Birmingham (United Kingdom)
  5. National Inst. of Nuclear Physics (INFN), Padova (Italy)
  6. Univ. of Surrey, Guildford (United Kingdom)
  7. Univ. di Milano (Italy)
  8. Commissariat a l'Energie Atomique et aux Energies Alternatives (CEA-Saclay), Gif-sur-Yvette (France)
  9. Univ. of Manchester (United Kingdom). Schuster Lab.
  10. Univ. of the West of Scotland, Paisley (United Kingdom)
  11. Univ. of Rochester, NY (United States)
  12. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  13. Spanish National Research Council (CSIC), Valencia (Spain). Univ. of Valencia (UV), Inst. de Fisica Corpuscular
  14. Uppsala Univ. (Sweden)
  15. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of Oslo (Norway); Inst. de Recherche sur les lois Fondamentales de l'Univers (IRFU), Gif-sur-Yvette (France)
  16. Univ. di Padova (Italy); Istituto Nazionale di Fisica Nucleare (INFN), Padova (Italy)
  17. Consejo Superior de Investigaciones Cientificas (CSIC), Madrid (Spain)
  18. Institut de Recherche sur les lois Fondamentales de l'Univers (IRFU), Gif-sur-Yvette (France)
  19. National Inst. of Nuclear Physics (INFN), Padova (Italy); Univ. di Padova (Italy); Univ. of the West of Scotland (United Kingdom)
  20. National Inst. of Nuclear Physics (INFN), Padova (Italy); Univ. di Padova (Italy)
  21. Ruder Boskovic Inst., Zagreb (Croatia)
  22. Univ. of Torino (Italy)
  23. Univ. of Surrey, Guildford (United Kingdom); National Physical Lab, Middlesex (United Kingdom)
  24. Univ. of Copenhagen (Denmark). The Niels Bohr Inst.
  25. Univ. of Lyon (France)
  26. Daresbury Lab. (United Kingdom). Council for the Central Lab. of the Research Councils (CCLRC)
Publication Date:
Research Org.:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1423600
Grant/Contract Number:  
AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review C
Additional Journal Information:
Journal Volume: 93; Journal Issue: 5; Journal ID: ISSN 2469-9985
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS

Citation Formats

Vogt, A., Birkenbach, B., Reiter, P., Blazhev, A., Siciliano, M., Valiente-Dobón, J. J., Wheldon, C., Bazzacco, D., Bowry, M., Bracco, A., Bruyneel, B., Chakrawarthy, R. S., Chapman, R., Cline, D., Corradi, L., Crespi, F. C. L., Cromaz, M., de Angelis, G., Eberth, J., Fallon, P., Farnea, E., Fioretto, E., Freeman, S. J., Gadea, A., Geibel, K., Gelletly, W., Gengelbach, A., Giaz, A., Görgen, A., Gottardo, A., Hayes, A. B., Hess, H., Hua, H., John, P. R., Jolie, J., Jungclaus, A., Korten, W., Lee, I. Y., Leoni, S., Liang, X., Lunardi, S., Macchiavelli, A. O., Menegazzo, R., Mengoni, D., Michelagnoli, C., Mijatović, T., Montagnoli, G., Montanari, D., Napoli, D., Pearson, C. J., Pellegri, L., Podolyák, Zs., Pollarolo, G., Pullia, A., Radeck, F., Recchia, F., Regan, P. H., Şahin, E., Scarlassara, F., Sletten, G., Smith, J. F., Söderström, P. -A., Stefanini, A. M., Steinbach, T., Stezowski, O., Szilner, S., Szpak, B., Teng, R., Ur, C., Vandone, V., Ward, D., Warner, D. D., Wiens, A., and Wu, C. Y. High-spin structure of Xe134. United States: N. p., 2016. Web. doi:10.1103/PhysRevC.93.054325.
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Vogt, A., Birkenbach, B., Reiter, P., Blazhev, A., Siciliano, M., Valiente-Dobón, J. J., Wheldon, C., Bazzacco, D., Bowry, M., Bracco, A., Bruyneel, B., Chakrawarthy, R. S., Chapman, R., Cline, D., Corradi, L., Crespi, F. C. L., Cromaz, M., de Angelis, G., Eberth, J., Fallon, P., Farnea, E., Fioretto, E., Freeman, S. J., Gadea, A., Geibel, K., Gelletly, W., Gengelbach, A., Giaz, A., Görgen, A., Gottardo, A., Hayes, A. B., Hess, H., Hua, H., John, P. R., Jolie, J., Jungclaus, A., Korten, W., Lee, I. Y., Leoni, S., Liang, X., Lunardi, S., Macchiavelli, A. O., Menegazzo, R., Mengoni, D., Michelagnoli, C., Mijatović, T., Montagnoli, G., Montanari, D., Napoli, D., Pearson, C. J., Pellegri, L., Podolyák, Zs., Pollarolo, G., Pullia, A., Radeck, F., Recchia, F., Regan, P. H., Şahin, E., Scarlassara, F., Sletten, G., Smith, J. F., Söderström, P. -A., Stefanini, A. M., Steinbach, T., Stezowski, O., Szilner, S., Szpak, B., Teng, R., Ur, C., Vandone, V., Ward, D., Warner, D. D., Wiens, A., & Wu, C. Y. High-spin structure of Xe134. United States. https://doi.org/10.1103/PhysRevC.93.054325
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Vogt, A., Birkenbach, B., Reiter, P., Blazhev, A., Siciliano, M., Valiente-Dobón, J. J., Wheldon, C., Bazzacco, D., Bowry, M., Bracco, A., Bruyneel, B., Chakrawarthy, R. S., Chapman, R., Cline, D., Corradi, L., Crespi, F. C. L., Cromaz, M., de Angelis, G., Eberth, J., Fallon, P., Farnea, E., Fioretto, E., Freeman, S. J., Gadea, A., Geibel, K., Gelletly, W., Gengelbach, A., Giaz, A., Görgen, A., Gottardo, A., Hayes, A. B., Hess, H., Hua, H., John, P. R., Jolie, J., Jungclaus, A., Korten, W., Lee, I. Y., Leoni, S., Liang, X., Lunardi, S., Macchiavelli, A. O., Menegazzo, R., Mengoni, D., Michelagnoli, C., Mijatović, T., Montagnoli, G., Montanari, D., Napoli, D., Pearson, C. J., Pellegri, L., Podolyák, Zs., Pollarolo, G., Pullia, A., Radeck, F., Recchia, F., Regan, P. H., Şahin, E., Scarlassara, F., Sletten, G., Smith, J. F., Söderström, P. -A., Stefanini, A. M., Steinbach, T., Stezowski, O., Szilner, S., Szpak, B., Teng, R., Ur, C., Vandone, V., Ward, D., Warner, D. D., Wiens, A., and Wu, C. Y. Wed . "High-spin structure of Xe134". United States. https://doi.org/10.1103/PhysRevC.93.054325. https://www.osti.gov/servlets/purl/1423600.
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@article{osti_1423600,
title = {High-spin structure of Xe134},
author = {Vogt, A. and Birkenbach, B. and Reiter, P. and Blazhev, A. and Siciliano, M. and Valiente-Dobón, J. J. and Wheldon, C. and Bazzacco, D. and Bowry, M. and Bracco, A. and Bruyneel, B. and Chakrawarthy, R. S. and Chapman, R. and Cline, D. and Corradi, L. and Crespi, F. C. L. and Cromaz, M. and de Angelis, G. and Eberth, J. and Fallon, P. and Farnea, E. and Fioretto, E. and Freeman, S. J. and Gadea, A. and Geibel, K. and Gelletly, W. and Gengelbach, A. and Giaz, A. and Görgen, A. and Gottardo, A. and Hayes, A. B. and Hess, H. and Hua, H. and John, P. R. and Jolie, J. and Jungclaus, A. and Korten, W. and Lee, I. Y. and Leoni, S. and Liang, X. and Lunardi, S. and Macchiavelli, A. O. and Menegazzo, R. and Mengoni, D. and Michelagnoli, C. and Mijatović, T. and Montagnoli, G. and Montanari, D. and Napoli, D. and Pearson, C. J. and Pellegri, L. and Podolyák, Zs. and Pollarolo, G. and Pullia, A. and Radeck, F. and Recchia, F. and Regan, P. H. and Şahin, E. and Scarlassara, F. and Sletten, G. and Smith, J. F. and Söderström, P. -A. and Stefanini, A. M. and Steinbach, T. and Stezowski, O. and Szilner, S. and Szpak, B. and Teng, R. and Ur, C. and Vandone, V. and Ward, D. and Warner, D. D. and Wiens, A. and Wu, C. Y.},
abstractNote = {Detailed spectroscopic information on the N~82 nuclei is necessary to benchmark shell-model calculations in the region. The nuclear structure above long-lived isomers in 134Xe is investigated after multinucleon transfer (MNT) and actinide fission. Xenon-134 was populated as (i) a transfer product in 136Xe+238U and 136Xe+208Pb MNT reactions and (ii) as a fission product in the 136Xe+238U reaction employing the high-resolution Advanced Gamma Tracking Array (AGATA). Trajectory reconstruction has been applied for the complete identification of beamlike transfer products with the magnetic spectrometer PRISMA. The 136Xe+198Pt MNT reaction was studied with the γ-ray spectrometer GAMMASPHERE in combination with the gas detector array Compact Heavy Ion Counter (CHICO). Several high-spin states in 134Xe on top of the two long-lived isomers are discovered based on γγ-coincidence relationships and information on the γ-ray angular distributions as well as excitation energies from the total kinetic energy loss and fission fragments. The revised level scheme of 134Xe is extended up to an excitation energy of 5.832 MeV with tentative spin-parity assignments up to 16+. Previous assignments of states above the 7- isomer are revised. Latest shell-model calculations employing two different effective interactions reproduce the experimental findings and support the new spin and parity assignments.},
doi = {10.1103/PhysRevC.93.054325},
journal = {Physical Review C},
number = 5,
volume = 93,
place = {United States},
year = {Wed May 25 00:00:00 EDT 2016},
month = {Wed May 25 00:00:00 EDT 2016}
}
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https://doi.org/10.1103/PhysRevC.93.054325
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<mml:math altimg="si8.gif" overflow="scroll" xmlns:xocs="http://www.elsevier.com/xml/xocs/dtd" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ja="http://www.elsevier.com/xml/ja/dtd" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:cals="http://www.elsevier.com/xml/common/cals/dtd"><mml:mi>γ</mml:mi></mml:math>-ray tracking algorithms: a comparison
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AGATA—Advanced GAmma Tracking Array
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<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="2011-01-01">January 2011</span></small> </h2> <ul class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#5C7B2D;"> Kempley, R. 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D.; Erten, H. N.; Hopke, P. K.</span> </li> <li> Nuclear Physics A, Vol. 179, Issue 3</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1016/0375-9474(72)90612-4" class="text-muted" target="_blank" rel="noopener noreferrer">10.1016/0375-9474(72)90612-4<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div> <div> <h2 class="title" style="margin-bottom:0;" data-apporder=""> <a href="https://doi.org/10.1016/s0168-9002(04)01477-9" target="_blank" rel="noopener noreferrer" class="name">γγ-ray tracking algorithms: a comparison<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="2004-11-11">November 2004</span></small> </h2> <ul class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#5C7B2D;"> Lopezmartens, A.; Hauschild, K.; Korichi, A.</span> </li> <li> Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Vol. 533, Issue 3</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1016/s0168-9002(04)01477-9" class="text-muted" target="_blank" rel="noopener noreferrer">10.1016/s0168-9002(04)01477-9<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div> <div> <h2 class="title" style="margin-bottom:0;" data-apporder=""> <a href="https://doi.org/10.1006/ndsh.1993.1025" target="_blank" rel="noopener noreferrer" class="name">Nuclear Data Sheets for A = 138<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="1993-05-01">May 1993</span></small> </h2> <ul class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#5C7B2D;"> Tuli, J. K.</span> </li> <li> Nuclear Data Sheets, Vol. 69, Issue 1</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1006/ndsh.1993.1025" class="text-muted" target="_blank" rel="noopener noreferrer">10.1006/ndsh.1993.1025<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div> <div> <h2 class="title" style="margin-bottom:0;" data-apporder=""> <a href="https://doi.org/10.1016/0375-9474(81)90407-3" target="_blank" rel="noopener noreferrer" class="name">Energy levels and transition probabilities in 130Sn.<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="1981-08-01">August 1981</span></small> </h2> <ul class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#5C7B2D;"> Fogelberg, B.; Heyde, K.; Sau, J.</span> </li> <li> Nuclear Physics A, Vol. 365, Issue 3, p. 530</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1016/0375-9474(81)90407-3" class="text-muted" target="_blank" rel="noopener noreferrer">10.1016/0375-9474(81)90407-3<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div> </div> <div class="pagination-container small"> <a class="pure-button prev page" href="#" rel="prev"><span class="sr-only">Previous Page</span><span class="fa fa-angle-left"></span></a> <ul class="pagination d-inline-block" style="padding-left:.2em;"></ul> <a class="pure-button next page" href="#" rel="next"><span class="sr-only">Next Page</span><span class="fa fa-angle-right"></span></a> </div> </div> </div> <div class="col-sm-3 order-sm-3"> <ul class="nav nav-stacked"> <li class="active"><a href="" class="reference-type-filter tab-nav" data-tab="biblio-references" data-filter="type" data-pattern="*"><span class="fa fa-angle-right"></span> All References</a></li> <li class="small" style="margin-left:.75em; text-transform:capitalize;"><a href="" class="reference-type-filter tab-nav" data-tab="biblio-references" data-filter="type" data-pattern="journal"><span class="fa fa-angle-right"></span> journal<small class="text-muted"> (48)</small></a></li> </ul> <div style="margin-top:2em;"> <form class="pure-form small text-muted reference-search"> <label for="reference-search-text" class="sr-only">Search</label> <input class="search form-control pure-input-1" id="reference-search-text" placeholder="Search" style="margin-bottom:10px;" /> <fieldset aria-label="Sort By"> <legend class="legend-filters sr-only">Sort by:</legend> <div style="margin-left:1em; font-weight:normal; line-height: 1.6em;"><input type="radio" class="sort" name="references-sort" data-sort="name" style="position:relative;top:2px;" id="reference-search-sort-name"><label for="reference-search-sort-name" style="margin-left: .3em;">Sort by title</label></div> <div style="margin-left:1em; font-weight:normal; line-height: 1.6em;"><input type="radio" class="sort" name="references-sort" data-sort="date" data-order="desc" style="position:relative;top:2px;" id="reference-search-sort-date"><label for="reference-search-sort-date" style="margin-left: .3em;">Sort by date</label></div> </fieldset> <div class="text-left" style="margin-left:1em;"> <a href="" class="filter-clear clearfix" title="Clear filter / sort" style="font-weight:normal; float:none;">[ × clear filter / sort ]</a> </div> <input type="submit" id="sort_submit_references" name="submit" aria-label="submit" style="display: none;"/> </form> </div> </div> </div> </section> <section id="biblio-citations" class="tab-content tab-content-sec osti-curated" data-tab="biblio"> <div class="row"> <div class="col-sm-9 order-sm-9"> <div class="padding"> <p class="lead text-muted" style="font-size: 18px; margin-top:0px;">Works referencing / citing this record:</p> <div class="list"> <div> <h2 class="title" style="margin-bottom:0;" data-apporder=""> <a href="https://doi.org/10.1103/physrevc.99.064321" target="_blank" rel="noopener noreferrer" class="name">Emerging collectivity from the nuclear structure of <math> <mmultiscripts> <mi>Xe</mi> <mprescripts/> <none/> <mn>132</mn> </mmultiscripts> </math> : Inelastic neutron scattering studies and shell-model calculations<span class="fa fa-external-link" aria-hidden="true"></span></a> <small class="text-muted" style="text-transform:uppercase; font-size:0.75rem;"><br/> <span class="type">journal</span>, <span class="date" data-date="2019-06-01">June 2019</span></small> </h2> <ul class="small references-list" style="list-style-type:none; margin-top: 0.5em; padding-left: 0; line-height:1.8em;"> <li> <span style="color:#5C7B2D;"> Peters, E. E.; Stuchbery, A. E.; Chakraborty, A.</span> </li> <li> Physical Review C, Vol. 99, Issue 6</li> <li> <span class="text-muted related-url">DOI: <a href="https://doi.org/10.1103/physrevc.99.064321" class="text-muted" target="_blank" rel="noopener noreferrer">10.1103/physrevc.99.064321<span class="fa fa-external-link" aria-hidden="true"></span></a></span> </li> </ul> <hr/> </div> </div> <div class="pagination-container small"> <a class="pure-button prev page" href="#" rel="prev"><span class="sr-only">Previous Page</span><span class="fa fa-angle-left"></span></a> <ul class="pagination d-inline-block" style="padding-left:.2em;"></ul> <a class="pure-button next page" href="#" rel="next"><span class="sr-only">Next Page</span><span class="fa fa-angle-right"></span></a> </div> </div> </div> <div class="col-sm-3 order-sm-3"> <ul class="nav nav-stacked"> <li class="active"><a href="" class="reference-type-filter tab-nav" data-filter="type" data-pattern="*"><span class="fa fa-angle-right"></span> All Cited By</a></li> <li class="small" style="margin-left:.75em; text-transform:capitalize;"><a href="" class="reference-type-filter tab-nav" data-filter="type" data-pattern="journal"><span class="fa fa-angle-right"></span> journal<small class="text-muted"> (1)</small></a></li> </ul> <div style="margin-top:2em;"> <form class="pure-form small text-muted citation-search"> <label for="citation-search-text" class="sr-only">Search</label> <input class="search form-control pure-input-1" id="citation-search-text" placeholder="Search" style="margin-bottom:10px;" /> <fieldset aria-label="Sort By"> <legend class="legend-filters sr-only">Sort by:</legend> <div style="margin-left:1em; font-weight:normal; line-height: 1.6em;"><input type="radio" class="sort" name="references-sort" data-sort="name" style="position:relative;top:2px;" id="citation-search-sort-name"><label for="citation-search-sort-name" style="margin-left: .3em;">Sort by title</label></div> <div style="margin-left:1em; font-weight:normal; line-height: 1.6em;"><input type="radio" class="sort" name="references-sort" data-sort="date" data-order="desc" style="position:relative;top:2px;" id="citation-search-sort-date"><label for="citation-search-sort-date" style="margin-left: .3em;">Sort by date</label></div> </fieldset> <div class="text-left" style="margin-left:1em;"> <a href="" class="filter-clear clearfix" title="Clear filter / sort" style="font-weight:normal; float:none;">[ × clear filter / sort ]</a> </div> <input type="submit" id="sort_submit_citations" name="submit" aria-label="submit" style="display: none;"/> </form> </div> </div> </div> </section> <section id="biblio-related" class="tab-content tab-content-sec " data-tab="biblio"> <div class="row"> <div class="col-sm-9 order-sm-9"> <section id="biblio-similar" class="tab-content tab-content-sec active" data-tab="related"> <div class="padding"> <p class="lead text-muted" style="font-size: 18px; margin-top:0px;">Similar Records in DOE PAGES and OSTI.GOV collections:</p> <aside> <ul class="item-list" itemscope itemtype="http://schema.org/ItemList" style="padding-left:0; list-style-type: none;"> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="0" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/pages/biblio/1409951-high-spin-structures-xe132-xe133-evidence-isomers-along-isotones" itemprop="url">High-spin structures in <math> <mmultiscripts> <mi>Xe</mi><mprescripts/><none/> <mn>132</mn> </mmultiscripts> </math> and <math> <mmultiscripts> <mi>Xe</mi><mprescripts/><none/> <mn>133</mn> </mmultiscripts> </math> and evidence for isomers along the <math> <mrow> <mi>N</mi> <mo>=</mo> <mn>79</mn> </mrow> </math> isotones</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Vogt, A.</span> ; <span class="author">Siciliano, M.</span> ; <span class="author">Birkenbach, B.</span> ; <span class="author">...</span> <span class="text-muted pubdata"> - Physical Review C</span> </span> </div> <div class="abstract">In this study, the transitional nuclei <sup>132</sup>Xe and <sup>133</sup>Xe are investigated after multinucleon-transfer (MNT) and fusion-evaporation reactions. Both nuclei are populated (i) in <sup>136</sup>Xe + <sup>208</sup>Pb MNT reactions employing the high-resolution Advanced GAmma Tracking Array (AGATA) coupled to the magnetic spectrometer PRISMA, (ii) in the <sup>136</sup>Xe + <sup>198</sup>Pt MNT reaction employing the GAMMASPHERE spectrometer in combination with the gas-detector array CHICO, and (iii) as an evaporation residue after a <sup>130</sup>Te (α,xn) <sup>134-xn</sup>Xe fusion-evaporation reaction employing the HORUS γ -ray array at the University of Cologne. The high-spin level schemes are considerably extended above the J<sup>π</sup> = (7<sup>-</sup>) and (10<sup>+</sup>) isomers<a href='#' onclick='$(this).hide().next().show().next().show();return false;' style='margin-left:10px;'>more »</a><span style='display:none;'> in <sup>132</sup>Xe and above the 11/2<sup>-</sup> isomer in <sup>133</sup>Xe. The results are compared to the high-spin systematics of the Z = 54 as well as the N = 78 and N = 79 chains. Furthermore, evidence is found for a long-lived (T<sub>1/</sub>2 » 1 μs) isomer in <sup>133</sup>Xe which closes a gap along the N = 79 isotones. Finally, shell-model calculations employing the SN100PN and PQM130 effective interactions reproduce the experimental findings and provide guidance to the interpretation of the observed high-spin features.</span><a href='#' onclick='$(this).hide().prev().hide().prev().show();return false;' style='margin-left:10px;display:none;'>« less</a></div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <span class="fa fa-book text-muted" aria-hidden="true"></span> Cited by 14<div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc doi-link " href="https://doi.org/10.1103/PhysRevC.96.024321" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="1409951" data-product-type="Journal Article" data-product-subtype="AM" >https://doi.org/10.1103/PhysRevC.96.024321</a></span></li> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc fulltext-link " href="/pages/servlets/purl/1409951" title="Link to document media" target="_blank" rel="noopener" data-ostiid="1409951" data-product-type="Journal Article" data-product-subtype="AM" >Full Text Available</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="1" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/pages/biblio/1423613-isomers-high-spin-structures-isotones-xe135-ba137" itemprop="url">Isomers and high-spin structures in the <math> <mrow> <mi>N</mi> <mo>=</mo> <mn>81</mn> </mrow> </math> isotones <math> <mmultiscripts> <mi>Xe</mi><mprescripts/><none/> <mn>135</mn> </mmultiscripts> </math> and <math> <mmultiscripts> <mi>Ba</mi><mprescripts/><none/> <mn>137</mn> </mmultiscripts> </math></a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Vogt, A.</span> ; <span class="author">Birkenbach, B.</span> ; <span class="author">Reiter, P.</span> ; <span class="author">...</span> <span class="text-muted pubdata"> - Physical Review C</span> </span> </div> <div class="abstract">In this study, the high-spin structures and isomers of the N=81 isotones <sup>135</sup>Xe and <sup>137</sup>Ba are investigated after multinucleon-transfer (MNT) and fusion-evaporation reactions. Both nuclei are populated (i) in <sup>136</sup>Xe +<sup>238</sup>U and (ii) <sup>136</sup>Xe+<sup>208</sup>Pb MNT reactions employing the high-resolution Advanced Gamma Tracking Array (AGATA) coupled to the magnetic spectrometer PRISMA, (iii) in the <sup>136</sup>Xe+<sup>198</sup>Pt MNT reaction employing the γ-ray array GAMMASPHERE in combination with the gas-detector array CHICO, and (iv) via a <sup>11</sup>B+<sup>130</sup>Te fusion-evaporation reaction with the HORUS γ-ray array at the University of Cologne. The high-spin level schemesof <sup>135</sup>Xe and <sup>137</sup>Ba are considerably extended to higher energies. The 2058-keV<a href='#' onclick='$(this).hide().next().show().next().show();return false;' style='margin-left:10px;'>more »</a><span style='display:none;'> (19/2<sup>-</sup>) state in <sup>135</sup>Xe is identified as an isomer, closing a gap in the systematics along the N=81 isotones. Its half-life is measured to be 9.0(9) ns, corresponding to a reduced transition probability of B(E2,19/2<sup>-</sup>→15/2<sup>-</sup>)=0.52(6) W.u. The experimentally deduced reduced transition probabilities of the isomeric states are compared to shell-model predictions. Finally, latest shell-model calculations reproduce the experimental findings generally well and provide guidance to the interpretation of the new levels.</span><a href='#' onclick='$(this).hide().prev().hide().prev().show();return false;' style='margin-left:10px;display:none;'>« less</a></div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc doi-link " href="https://doi.org/10.1103/PhysRevC.95.024316" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="1423613" data-product-type="Journal Article" data-product-subtype="AM" >https://doi.org/10.1103/PhysRevC.95.024316</a></span></li> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc fulltext-link " href="/pages/servlets/purl/1423613" title="Link to document media" target="_blank" rel="noopener" data-ostiid="1423613" data-product-type="Journal Article" data-product-subtype="AM" >Full Text Available</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="2" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/pages/biblio/1979897-lifetime-measurements-states-s35-s36-s37-s38-using-agata-ray-tracking-spectrometer" itemprop="url">Lifetime measurements of states of <math> <mmultiscripts> <mi mathvariant="normal">S</mi><mprescripts/><none/> <mn>35</mn> </mmultiscripts> </math> , <math> <mmultiscripts> <mi mathvariant="normal">S</mi><mprescripts/><none/> <mn>36</mn> </mmultiscripts> </math> , <math> <mmultiscripts> <mi mathvariant="normal">S</mi><mprescripts/><none/> <mn>37</mn> </mmultiscripts> </math> , and <math> <mmultiscripts> <mi mathvariant="normal">S</mi><mprescripts/><none/> <mn>38</mn> </mmultiscripts> </math> using the AGATA <math> <mi>γ</mi> </math> -ray tracking spectrometer</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Grocutt, L.</span> ; <span class="author">Chapman, R.</span> ; <span class="author">Bouhelal, M.</span> ; <span class="author">...</span> <span class="text-muted pubdata"> - Physical Review. C</span> </span> </div> <div class="abstract">Lifetimes or lifetime limits of a small number of excited states of the sulfur isotopes with mass numbers A = 35 , 36, 37, and 38 have been measured using the differential recoil-distance method. The isotopes of sulfur were populated in binary grazing reactions initiated by a beam of <sup>36</sup>S ions of energy 225 MeV incident on a thin <sup>208</sup>Pb target which was mounted in the Cologne plunger apparatus. The combination of the PRISMA magnetic spectrometer and an early implementation of the AGATA γ-ray tracking array was used to detect γ rays in coincidence with projectile-like nuclear species. Lifetime measurements<a href='#' onclick='$(this).hide().next().show().next().show();return false;' style='margin-left:10px;'>more »</a><span style='display:none;'> of populated states were measured within the range from about 1 to 100 ps. The number of states for which lifetime measurements or lifetime limits were possible was limited by statistics. For <sup>35</sup>S, the lifetime was determined for the first 1/2<sup>+</sup> state at 1572 keV; the result is compared with a previous published lifetime value. The lifetime of the 3<sup>-</sup> state of <sup>36</sup>S at 4193 keV was determined and compared with earlier measurements. No previous lifetime information exists for the (6<sup>+</sup>) state at 6690 keV; a lifetime measurement with large associated error was made in the present work. For <sup>37</sup>S, the states for which lifetime limits were established were those at 646 keV with J<sup>π</sup> = 3/2<sup>-</sup> and at 2776 keV with J<sup>π</sup> = 11/2<sup>-</sup>; there are no previously published lifetime values for excited states of <sup>37</sup>S. Finally, a lifetime limit was established for the J<sup>π</sup> =(6<sup>+</sup>) state of <sup>38</sup>S at 3675 keV; no lifetime information exists for this state in the literature. Measured lifetime values were compared with the results of state-of-the-art shell-model calculations based on the PSDPF, SDPF-U, and FSU effective interactions. In addition, nuclear magnetic-dipole and electric-quadrupole moments, branching ratios, mixing ratios, and electromagnetic transition rates, where available, have been compared with shell-model values. The current work suffers from poor statistics; nevertheless, lifetime values and limits have been possible, allowing a useful discussion of the ability of state-of-the-art shell-model calculations to reproduce the experimental results.</span><a href='#' onclick='$(this).hide().prev().hide().prev().show();return false;' style='margin-left:10px;display:none;'>« less</a></div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc doi-link " href="https://doi.org/10.1103/physrevc.106.024314" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="1979897" data-product-type="Journal Article" data-product-subtype="AM" >https://doi.org/10.1103/physrevc.106.024314</a></span></li> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc fulltext-link " href="/pages/servlets/purl/1979897" title="Link to document media" target="_blank" rel="noopener" data-ostiid="1979897" data-product-type="Journal Article" data-product-subtype="AM" >Full Text Available</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="3" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/pages/biblio/1374540-doubly-magic-pb208-high-spin-states-isomers-e3-collectivity-yrast-decay" itemprop="url">Doubly magic <math> <mmultiscripts> <mi>Pb</mi><mprescripts/><none/> <mn>208</mn> </mmultiscripts> </math> : High-spin states, isomers, and <math> <mi>E</mi><mn>3</mn> </math> collectivity in the yrast decay</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Broda, R.</span> ; <span class="author">Janssens, R. V. F.</span> ; <span class="author">Iskra, Ł. W.</span> ; <span class="author">...</span> <span class="text-muted pubdata"> - Physical Review C</span> </span> </div> <div class="abstract">Yrast and near-yrast levels up to spin values in excess of I = 30h have been delineated in the doubly-magic <sup>208</sup>Pb nucleus following deep-inelastic reactions involving <sup>208</sup>Pb targets and, mostly, 430-MeV <sup>48</sup>Ca and 1440-MeV <sup>208</sup>Pb beams. The level scheme was established up to an excitation energy of 16.4 MeV, based on multi-fold γ-ray coincidence relationships measured with the Gammasphere array. Below the well-known, 0.5-μs 10<sup>+</sup> isomer, ten new transitions were added to earlier work. The delineation of the higher parts of the level sequence benefited from analyses involving a number of prompt- and delayed-coincidence conditions. Three new isomeric states were<a href='#' onclick='$(this).hide().next().show().next().show();return false;' style='margin-left:10px;'>more »</a><span style='display:none;'> established along the yrast line with I <sup>π</sup> = 20<sup>-</sup> (10342 keV), 23<sup>+</sup> (11361 keV), and 28<sup>-</sup> (13675 keV), and respective half-lives of 22(3), 12.7(2), and 60(6) ns. Gamma transitions were also identified preceding in time the 28<sup>-</sup> isomer, however, only a few could be placed in the level scheme and no firm spin-parity quantum numbers could be proposed. In contrast, for most states below this 28<sup>-</sup> isomer, firm spin-parity values were assigned, based on total electron-conversion coefficients, deduced for low-energy (<500 keV) transitions from γ-intensity balances, and on measured γ-ray angular distributions. The latter also enabled the quantitative determination of mixing ratios. The transition probabilities extracted for all isomeric transitions in <sup>208</sup>Pb have been reviewed and discussed in terms of the intrinsic structure of the initial and final levels involved. Particular emphasis was placed on the many observed E3 transitions as they often exhibit significant enhancements in strength (of the order of tens of W.u.) comparable to the one seen for the neutron j<sub>15/2</sub>→g<sub>9/2</sub> E3 transition in <sup>209</sup>Pb. In this context, the enhancement of the 725-keV E3 transition (56 W.u.) associated with the decay of the highest-lying 28<sup>-</sup> isomer observed in this work remains particularly challenging to explain. Large-scale shell-model calculations were performed with two approaches, a first one where the 1, 2, and 3 particle-hole excitations do not mix with one another, and another more complex one, in which such mixing takes place. We compared the calculated levels with the data and a general agreement is observed for most of the <sup>208</sup>Pb level scheme. At the highest spins and energies, however, the 2 correspondence between theory and experiment is less satisfactory and the experimental yrast line appears to be more regular than the calculated one. This regularity is notable when the level energies are plotted versus the I(I+1) product and the observed, nearly linear, behavior was considered within a simple “rotational” interpretation. Furthermore, within this approximate picture, the extracted moment of inertia suggests that only the 76 valence nucleons participate in the “rotation” and that the <sup>132</sup>Sn spherical core remains inert.</span><a href='#' onclick='$(this).hide().prev().hide().prev().show();return false;' style='margin-left:10px;display:none;'>« less</a></div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <span class="fa fa-book text-muted" aria-hidden="true"></span> Cited by 15<div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc doi-link " href="https://doi.org/10.1103/PhysRevC.95.064308" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="1374540" data-product-type="Journal Article" data-product-subtype="AM" >https://doi.org/10.1103/PhysRevC.95.064308</a></span></li> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc fulltext-link " href="/pages/servlets/purl/1374540" title="Link to document media" target="_blank" rel="noopener" data-ostiid="1374540" data-product-type="Journal Article" data-product-subtype="AM" >Full Text Available</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> <li> <div class="article item document" itemprop="itemListElement" itemscope itemtype="http://schema.org/WebPage"><meta itemprop="position" content="5" /><div class="item-info"> <h2 class="title" itemprop="name headline"><a href="/pages/biblio/1489067-decay-study-mn-fe-co-ni-decay-chain" itemprop="url"><math> <msup> <mi>β</mi> <mo>−</mo> </msup> </math> decay study of the <math> <mrow> <mmultiscripts> <mi>Mn</mi> <mprescripts/> <none/> <mn>66</mn> </mmultiscripts> <mtext>−</mtext> <mmultiscripts> <mi>Fe</mi> <mprescripts/> <none/> <mn>66</mn> </mmultiscripts> <mtext>−</mtext> <mmultiscripts> <mi>Co</mi> <mprescripts/> <none/> <mn>66</mn> </mmultiscripts> <mtext>−</mtext> <mmultiscripts> <mi>Ni</mi> <mprescripts/> <none/> <mn>66</mn> </mmultiscripts> </mrow> </math> decay chain</a></h2> <div class="metadata"> <small class="text-muted" style="text-transform:uppercase;display:block;line-height:2.5em;">Journal Article</small><span class="authors"> <span class="author">Stryjczyk, M.</span> ; <span class="author">Tsunoda, Y.</span> ; <span class="author">Darby, I. G.</span> ; <span class="author">...</span> <span class="text-muted pubdata"> - Physical Review C</span> </span> </div> <div class="abstract">Here, shell evolution can impact the structure of the nuclei and lead to effects such as shape coexistence. The nuclei around <sup>68</sup>Ni represent an excellent study case, however, spectroscopic information of the neutron-rich, Z < 28 nuclei is limited. The goal is to measure γ-ray transitions in <sup>66</sup>Fe, <sup>66</sup>Co, and <sup>66</sup>Ni populated in the β– decay of <sup>66</sup>Mn to determine absolute β feedings and relative γ-decay probabilities and to compare the results with Monte Carlo shell model calculations in order to study the influence of the relevant single neutron and proton orbital occupancies around Z = 28 and N =<a href='#' onclick='$(this).hide().next().show().next().show();return false;' style='margin-left:10px;'>more »</a><span style='display:none;'> 40. The low-energy structures of <sup>65,66</sup>Fe, <sup>66</sup>Co, and <sup>66</sup>Ni were studied in the β– decay of 66Mn produced at ISOLDE, CERN. The beam was purified by means of laser resonance ionization and mass separation. The β and γ events detected by three plastic scintillators and two MiniBall cluster germanium detectors, respectively, were correlated in time to build the low-energy excitation schemes and to determine the β-decay half-lives of the nuclei. As a result, the relative small β-decay ground state feeding of <sup>66</sup>Fe obtained in this work is at variant to the earlier studies. Spin and parity 1+ was assigned to the <sup>66</sup>Co ground state based on the strong ground-state feeding in the decay of 66Fe as well as in the decay of <sup>66</sup>Co. Experimental log(ft) values, γ-ray de-excitation patterns, and energies of excited states were compared to Monte Carlo shell model calculations. Based on this comparison, spin and parity assignments for the selected number of low-lying states in the <sup>66</sup>Mn to <sup>66</sup>Ni chain were proposed. In conclusion, the β-decay chain starting <sup>66</sup>Mn toward <sup>66</sup>Ni, crossing N = 40, evolves from deformed nuclei to sphericity. The β-decay population of a selected number of 0+ and 2+ states in <sup>66</sup>Ni, which is understood within shape coexistence framework of Monte Carlo shell model calculations, reveals the crucial role of the neutron 0g<sub>9/2</sub> shell and proton excitations across the Z = 28 gap.</span><a href='#' onclick='$(this).hide().prev().hide().prev().show();return false;' style='margin-left:10px;display:none;'>« less</a></div><div class="metadata-links small clearfix text-muted" style="margin-top:15px;"> <span class="fa fa-book text-muted" aria-hidden="true"></span> Cited by 11<div class="pure-menu pure-menu-horizontal pull-right" style="width:unset;"> <ul class="pure-menu-list"> <li class="pure-menu-item"><span class="item-info-ftlink"><a class="misc doi-link " href="https://doi.org/10.1103/PhysRevC.98.064326" target="_blank" rel="noopener" title="Link to document DOI" data-ostiid="1489067" data-product-type="Journal Article" data-product-subtype="PA" >https://doi.org/10.1103/PhysRevC.98.064326</a></span></li> </ul> </div> </div> </div> <div class="clearfix"></div> </div> </li> </ul> </aside> </div> </section> </div> <div class="col-sm-3 order-sm-3"> <ul class="nav nav-stacked"> <li class="active"><a class="tab-nav disabled" data-tab="related" style="color: #636c72 !important; 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