High-spin structures in Xe 132 and Xe 133 and evidence for isomers along the N=79 isotones

A. Vogt; M. Siciliano; B. Birkenbach; P. Reiter; K. Hadyńska-Klȩk; C. Wheldon; J. J. Valiente-Dobón; E. Teruya; N. Yoshinaga; K. Arnswald; D. Bazzacco; A. Blazhev; A. Bracco; B. Bruyneel; R. S. Chakrawarthy; R. Chapman; D. Cline; L. Corradi; F. C.L. Crespi; M. Cromaz; G. De Angelis; J. Eberth; P. Fallon; E. Farnea; E. Fioretto; C. Fransen; S. J. Freeman; B. Fu; A. Gadea; W. Gelletly; A. Giaz; A. Görgen; A. Gottardo; A. B. Hayes; H. Hess; R. Hetzenegger; R. Hirsch; H. Hua; P. R. John; J. Jolie; A. Jungclaus; V. Karayonchev; L. Kaya; W. Korten; I. Y. Lee; S. Leoni; X. Liang; S. Lunardi; A. O. MacChiavelli; R. Menegazzo; D. Mengoni; C. Michelagnoli; T. Mijatović; G. Montagnoli; D. Montanari; C. Müller-Gatermann; D. Napoli; C. J. Pearson; Zs Podolyák; G. Pollarolo; A. Pullia; M. Queiser; F. Recchia; P. H. Regan; J. M. Régis; N. Saed-Samii; E. Şahin; F. Scarlassara; M. Seidlitz; B. Siebeck; G. Sletten; J. F. Smith; P. A. Söderström; A. M. Stefanini; O. Stezowski; S. Szilner; B. Szpak; R. Teng; C. Ur; D. D. Warner; K. Wolf; C. Y. Wu; K. O. Zell

doi:10.1103/PhysRevC.96.024321

High-spin structures in Xe 132 and Xe 133 and evidence for isomers along the N=79 isotones

A. Vogt^*, M. Siciliano, B. Birkenbach, P. Reiter, K. Hadyńska-Klȩk, C. Wheldon, J. J. Valiente-Dobón, E. Teruya, N. Yoshinaga, K. Arnswald, D. Bazzacco, A. Blazhev, A. Bracco, B. Bruyneel, R. S. Chakrawarthy, R. Chapman, D. Cline, L. Corradi, F. C.L. Crespi, M. CromazG. De Angelis, J. Eberth, P. Fallon, E. Farnea, E. Fioretto, C. Fransen, S. J. Freeman, B. Fu, A. Gadea, W. Gelletly, A. Giaz, A. Görgen, A. Gottardo, A. B. Hayes, H. Hess, R. Hetzenegger, R. Hirsch, H. Hua, P. R. John, J. Jolie, A. Jungclaus, V. Karayonchev, L. Kaya, W. Korten, I. Y. Lee, S. Leoni, X. Liang, S. Lunardi, A. O. MacChiavelli, R. Menegazzo, D. Mengoni, C. Michelagnoli, T. Mijatović, G. Montagnoli, D. Montanari, C. Müller-Gatermann, D. Napoli, C. J. Pearson, Zs Podolyák, G. Pollarolo, A. Pullia, M. Queiser, F. Recchia, P. H. Regan, J. M. Régis, N. Saed-Samii, E. Şahin, F. Scarlassara, M. Seidlitz, B. Siebeck, G. Sletten, J. F. Smith, P. A. Söderström, A. M. Stefanini, O. Stezowski, S. Szilner, B. Szpak, R. Teng, C. Ur, D. D. Warner, K. Wolf, C. Y. Wu, K. O. Zell

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Abstract

The transitional nuclei Xe132 and Xe133 are investigated after multinucleon-transfer (MNT) and fusion-evaporation reactions. Both nuclei are populated (i) in Xe136+Pb208 MNT reactions employing the high-resolution Advanced GAmma Tracking Array (AGATA) coupled to the magnetic spectrometer PRISMA, (ii) in the Xe136+Pt198 MNT reaction employing the GAMMASPHERE spectrometer in combination with the gas-detector array CHICO, and (iii) as an evaporation residue after a Te130(α,xn)Xe134-xn fusion-evaporation reaction employing the HORUS γ-ray array at the University of Cologne. The high-spin level schemes are considerably extended above the Jπ=(7-) and (10+) isomers in Xe132 and above the 11/2- isomer in Xe133. 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 (T1/2â‰1μs) isomer in Xe133 which closes a gap along the N=79 isotones. 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.

Original language	English
Article number	024321
Journal	Physical Review C
Volume	96
Issue number	2
DOIs	https://doi.org/10.1103/PhysRevC.96.024321
Publication status	Published - 24 Aug 2017

ASJC Scopus subject areas

Nuclear and High Energy Physics

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prc_vogt_high_spin_structures_in_xe132_and_xe133_and_evidence_for_isomers_along_the_n_79_isotones_accepted_version_2017_08_07Accepted author manuscript, 783 KB

Birmingham Nuclear Physics Group Consolidated Grant
Jones, P., Evans, P., Freer, M. & Wheldon, C.
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/08/14 → 30/09/18
Project: Research Councils

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Vogt, A., Siciliano, M., Birkenbach, B., Reiter, P., Hadyńska-Klȩk, K., Wheldon, C., Valiente-Dobón, J. J., Teruya, E., Yoshinaga, N., Arnswald, K., Bazzacco, D., Blazhev, A., Bracco, A., Bruyneel, B., Chakrawarthy, R. S., Chapman, R., Cline, D., Corradi, L., Crespi, F. C. L., ... Zell, K. O. (2017). High-spin structures in Xe 132 and Xe 133 and evidence for isomers along the N=79 isotones. Physical Review C, 96(2), Article 024321. https://doi.org/10.1103/PhysRevC.96.024321

@article{6adfa18cc2d649a4ba9dade7f06ce34a,

title = "High-spin structures in Xe 132 and Xe 133 and evidence for isomers along the N=79 isotones",

abstract = "The transitional nuclei Xe132 and Xe133 are investigated after multinucleon-transfer (MNT) and fusion-evaporation reactions. Both nuclei are populated (i) in Xe136+Pb208 MNT reactions employing the high-resolution Advanced GAmma Tracking Array (AGATA) coupled to the magnetic spectrometer PRISMA, (ii) in the Xe136+Pt198 MNT reaction employing the GAMMASPHERE spectrometer in combination with the gas-detector array CHICO, and (iii) as an evaporation residue after a Te130(α,xn)Xe134-xn fusion-evaporation reaction employing the HORUS γ-ray array at the University of Cologne. The high-spin level schemes are considerably extended above the Jπ=(7-) and (10+) isomers in Xe132 and above the 11/2- isomer in Xe133. 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 (T1/2{\^a}‰1μs) isomer in Xe133 which closes a gap along the N=79 isotones. 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.",

author = "A. Vogt and M. Siciliano and B. Birkenbach and P. Reiter and K. Hady{\'n}ska-Klȩk and C. Wheldon and Valiente-Dob{\'o}n, {J. J.} and E. Teruya and N. Yoshinaga and K. Arnswald and D. Bazzacco and A. Blazhev and A. Bracco and B. Bruyneel and Chakrawarthy, {R. S.} and R. Chapman and D. Cline and L. Corradi and Crespi, {F. C.L.} and M. Cromaz and {De Angelis}, G. and J. Eberth and P. Fallon and E. Farnea and E. Fioretto and C. Fransen and Freeman, {S. J.} and B. Fu and A. Gadea and W. Gelletly and A. Giaz and A. G{\"o}rgen and A. Gottardo and Hayes, {A. B.} and H. Hess and R. Hetzenegger and R. Hirsch and H. Hua and John, {P. R.} and J. Jolie and A. Jungclaus and V. Karayonchev and L. Kaya and W. Korten and Lee, {I. Y.} and S. Leoni and X. Liang and S. Lunardi and MacChiavelli, {A. O.} and R. Menegazzo and D. Mengoni and C. Michelagnoli and T. Mijatovi{\'c} and G. Montagnoli and D. Montanari and C. M{\"u}ller-Gatermann and D. Napoli and Pearson, {C. J.} and Zs Podoly{\'a}k and G. Pollarolo and A. Pullia and M. Queiser and F. Recchia and Regan, {P. H.} and R{\'e}gis, {J. M.} and N. Saed-Samii and E. {\c S}ahin and F. Scarlassara and M. Seidlitz and B. Siebeck and G. Sletten and Smith, {J. F.} and S{\"o}derstr{\"o}m, {P. A.} and Stefanini, {A. M.} and O. Stezowski and S. Szilner and B. Szpak and R. Teng and C. Ur and Warner, {D. D.} and K. Wolf and Wu, {C. Y.} and Zell, {K. O.}",

year = "2017",

month = aug,

day = "24",

doi = "10.1103/PhysRevC.96.024321",

language = "English",

volume = "96",

journal = "Physical Review C",

issn = "2469-9985",

publisher = "American Physical Society (APS)",

number = "2",

}

Vogt, A, Siciliano, M, Birkenbach, B, Reiter, P, Hadyńska-Klȩk, K, Wheldon, C, Valiente-Dobón, JJ, Teruya, E, Yoshinaga, N, Arnswald, K, Bazzacco, D, Blazhev, A, Bracco, A, Bruyneel, B, Chakrawarthy, RS, Chapman, R, Cline, D, Corradi, L, Crespi, FCL, Cromaz, M, De Angelis, G, Eberth, J, Fallon, P, Farnea, E, Fioretto, E, Fransen, C, Freeman, SJ, Fu, B, Gadea, A, Gelletly, W, Giaz, A, Görgen, A, Gottardo, A, Hayes, AB, Hess, H, Hetzenegger, R, Hirsch, R, Hua, H, John, PR, Jolie, J, Jungclaus, A, Karayonchev, V, Kaya, L, Korten, W, Lee, IY, Leoni, S, Liang, X, Lunardi, S, MacChiavelli, AO, Menegazzo, R, Mengoni, D, Michelagnoli, C, Mijatović, T, Montagnoli, G, Montanari, D, Müller-Gatermann, C, Napoli, D, Pearson, CJ, Podolyák, Z, Pollarolo, G, Pullia, A, Queiser, M, Recchia, F, Regan, PH, Régis, JM, Saed-Samii, N, Şahin, E, Scarlassara, F, Seidlitz, M, Siebeck, B, Sletten, G, Smith, JF, Söderström, PA, Stefanini, AM, Stezowski, O, Szilner, S, Szpak, B, Teng, R, Ur, C, Warner, DD, Wolf, K, Wu, CY & Zell, KO 2017, 'High-spin structures in Xe 132 and Xe 133 and evidence for isomers along the N=79 isotones', Physical Review C, vol. 96, no. 2, 024321. https://doi.org/10.1103/PhysRevC.96.024321

TY - JOUR

T1 - High-spin structures in Xe 132 and Xe 133 and evidence for isomers along the N=79 isotones

AU - Vogt, A.

AU - Siciliano, M.

AU - Birkenbach, B.

AU - Reiter, P.

AU - Hadyńska-Klȩk, K.

AU - Wheldon, C.

AU - Valiente-Dobón, J. J.

AU - Teruya, E.

AU - Yoshinaga, N.

AU - Arnswald, K.

AU - Bazzacco, D.

AU - Blazhev, A.

AU - Bracco, A.

AU - Bruyneel, B.

AU - Chakrawarthy, R. S.

AU - Chapman, R.

AU - Cline, D.

AU - Corradi, L.

AU - Crespi, F. C.L.

AU - Cromaz, M.

AU - De Angelis, G.

AU - Eberth, J.

AU - Fallon, P.

AU - Farnea, E.

AU - Fioretto, E.

AU - Fransen, C.

AU - Freeman, S. J.

AU - Fu, B.

AU - Gadea, A.

AU - Gelletly, W.

AU - Giaz, A.

AU - Görgen, A.

AU - Gottardo, A.

AU - Hayes, A. B.

AU - Hess, H.

AU - Hetzenegger, R.

AU - Hirsch, R.

AU - Hua, H.

AU - John, P. R.

AU - Jolie, J.

AU - Jungclaus, A.

AU - Karayonchev, V.

AU - Kaya, L.

AU - Korten, W.

AU - Lee, I. Y.

AU - Leoni, S.

AU - Liang, X.

AU - Lunardi, S.

AU - MacChiavelli, A. O.

AU - Menegazzo, R.

AU - Mengoni, D.

AU - Michelagnoli, C.

AU - Mijatović, T.

AU - Montagnoli, G.

AU - Montanari, D.

AU - Müller-Gatermann, C.

AU - Napoli, D.

AU - Pearson, C. J.

AU - Podolyák, Zs

AU - Pollarolo, G.

AU - Pullia, A.

AU - Queiser, M.

AU - Recchia, F.

AU - Regan, P. H.

AU - Régis, J. M.

AU - Saed-Samii, N.

AU - Şahin, E.

AU - Scarlassara, F.

AU - Seidlitz, M.

AU - Siebeck, B.

AU - Sletten, G.

AU - Smith, J. F.

AU - Söderström, P. A.

AU - Stefanini, A. M.

AU - Stezowski, O.

AU - Szilner, S.

AU - Szpak, B.

AU - Teng, R.

AU - Ur, C.

AU - Warner, D. D.

AU - Wolf, K.

AU - Wu, C. Y.

AU - Zell, K. O.

PY - 2017/8/24

Y1 - 2017/8/24

N2 - The transitional nuclei Xe132 and Xe133 are investigated after multinucleon-transfer (MNT) and fusion-evaporation reactions. Both nuclei are populated (i) in Xe136+Pb208 MNT reactions employing the high-resolution Advanced GAmma Tracking Array (AGATA) coupled to the magnetic spectrometer PRISMA, (ii) in the Xe136+Pt198 MNT reaction employing the GAMMASPHERE spectrometer in combination with the gas-detector array CHICO, and (iii) as an evaporation residue after a Te130(α,xn)Xe134-xn fusion-evaporation reaction employing the HORUS γ-ray array at the University of Cologne. The high-spin level schemes are considerably extended above the Jπ=(7-) and (10+) isomers in Xe132 and above the 11/2- isomer in Xe133. 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 (T1/2â‰1μs) isomer in Xe133 which closes a gap along the N=79 isotones. 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.

AB - The transitional nuclei Xe132 and Xe133 are investigated after multinucleon-transfer (MNT) and fusion-evaporation reactions. Both nuclei are populated (i) in Xe136+Pb208 MNT reactions employing the high-resolution Advanced GAmma Tracking Array (AGATA) coupled to the magnetic spectrometer PRISMA, (ii) in the Xe136+Pt198 MNT reaction employing the GAMMASPHERE spectrometer in combination with the gas-detector array CHICO, and (iii) as an evaporation residue after a Te130(α,xn)Xe134-xn fusion-evaporation reaction employing the HORUS γ-ray array at the University of Cologne. The high-spin level schemes are considerably extended above the Jπ=(7-) and (10+) isomers in Xe132 and above the 11/2- isomer in Xe133. 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 (T1/2â‰1μs) isomer in Xe133 which closes a gap along the N=79 isotones. 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.

UR - http://www.scopus.com/inward/record.url?scp=85028776828&partnerID=8YFLogxK

U2 - 10.1103/PhysRevC.96.024321

DO - 10.1103/PhysRevC.96.024321

M3 - Article

AN - SCOPUS:85028776828

SN - 2469-9985

VL - 96

JO - Physical Review C

JF - Physical Review C

IS - 2

M1 - 024321

ER -

High-spin structures in Xe 132 and Xe 133 and evidence for isomers along the N=79 isotones

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