Half-lives of neutron-rich 128-130Cd

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Half-lives of neutron-rich 128-130Cd. / Dunlop, R.; Bildstein, V.; Dillmann, I. et al.
In: Physical Review C, Vol. 93, No. 6, 16.06.2016.

Research output: Contribution to journalArticlepeer-review

HarvardHarvard

Dunlop, R, Bildstein, V, Dillmann, I, Jungclaus, A, Svensson, CE, Andreoiu, C, Ball, GC, Bernier, N, Bidaman, H, Boubel, P, Burbadge, C, Caballero-Folch, R, Dunlop, MR, Evitts, LJ, Garcia, F, Garnsworthy, AB, Garrett, PE, Hackman, G, Hallam, S, Henderson, J, Ilyushkin, S, Kisliuk, D, Krucken, R, Lassen, J, Li, R, MacConnachie, E, MacLean, AD, McGee, E, Moukaddam, M, Olaizola, B, Padilla-Rodal, E, Park, J, Paetkau, O, Petrache, CM, Pore, JL, Radich, AJ, Ruotsalainen, P, Smallcombe, J, Smith, JK, Tabor, SL, Teigelhofer, A, Turko, J & Zidar, T 2016, 'Half-lives of neutron-rich 128-130Cd', Physical Review C, vol. 93, no. 6. https://doi.org/10.1103/PhysRevC.93.062801

APA

Dunlop, R., Bildstein, V., Dillmann, I., Jungclaus, A., Svensson, C. E., Andreoiu, C., Ball, G. C., Bernier, N., Bidaman, H., Boubel, P., Burbadge, C., Caballero-Folch, R., Dunlop, M. R., Evitts, L. J., Garcia, F., Garnsworthy, A. B., Garrett, P. E., Hackman, G., Hallam, S., ... Zidar, T. (2016). Half-lives of neutron-rich 128-130Cd. Physical Review C, 93(6). https://doi.org/10.1103/PhysRevC.93.062801

CBE

Dunlop R, Bildstein V, Dillmann I, Jungclaus A, Svensson CE, Andreoiu C, Ball GC, Bernier N, Bidaman H, Boubel P, et al. 2016. Half-lives of neutron-rich 128-130Cd. Physical Review C. 93(6). https://doi.org/10.1103/PhysRevC.93.062801

MLA

VancouverVancouver

Dunlop R, Bildstein V, Dillmann I, Jungclaus A, Svensson CE, Andreoiu C et al. Half-lives of neutron-rich 128-130Cd. Physical Review C. 2016 Jun 16;93(6). doi: 10.1103/PhysRevC.93.062801

Author

Dunlop, R. ; Bildstein, V. ; Dillmann, I. et al. / Half-lives of neutron-rich 128-130Cd. In: Physical Review C. 2016 ; Vol. 93, No. 6.

RIS

TY - JOUR

T1 - Half-lives of neutron-rich 128-130Cd

AU - Dunlop, R.

AU - Bildstein, V.

AU - Dillmann, I.

AU - Jungclaus, A.

AU - Svensson, C. E.

AU - Andreoiu, C.

AU - Ball, G. C.

AU - Bernier, N.

AU - Bidaman, H.

AU - Boubel, P.

AU - Burbadge, C.

AU - Caballero-Folch, R.

AU - Dunlop, M. R.

AU - Evitts, L. J.

AU - Garcia, F.

AU - Garnsworthy, A. B.

AU - Garrett, P. E.

AU - Hackman, G.

AU - Hallam, S.

AU - Henderson, J.

AU - Ilyushkin, S.

AU - Kisliuk, D.

AU - Krucken, R.

AU - Lassen, J.

AU - Li, R.

AU - MacConnachie, E.

AU - MacLean, A. D.

AU - McGee, E.

AU - Moukaddam, M.

AU - Olaizola, B.

AU - Padilla-Rodal, E.

AU - Park, J.

AU - Paetkau, O.

AU - Petrache, C. M.

AU - Pore, J. L.

AU - Radich, A. J.

AU - Ruotsalainen, P.

AU - Smallcombe, J.

AU - Smith, J. K.

AU - Tabor, S. L.

AU - Teigelhofer, A.

AU - Turko, J.

AU - Zidar, T.

PY - 2016/6/16

Y1 - 2016/6/16

N2 - The β-decay half-lives of 128–130Cd have been measured with the newly commissioned GRIFFIN γ-ray spectrometer at the TRIUMF-ISAC facility. The time structures of the most intense γ rays emitted following the β decay were used to determine the half-lives of 128Cd and 130Cd to be T1/2=246.2(21)ms and T1/2=126(4) ms, respectively. The half-lives of the 3/2+ and 11/2− states of 129Cd were measured to be T1/2(3/2+)=157(8) ms and T1/2(11/2−)=147(3) ms. The half-lives of the Cd isotopes around the N=82 shell closure are an important ingredient in astrophysical simulations to derive the magnitude of the second r-process abundance peak in the A∼130 region. Our new results are compared with recent literature values and theoretical calculations.

AB - The β-decay half-lives of 128–130Cd have been measured with the newly commissioned GRIFFIN γ-ray spectrometer at the TRIUMF-ISAC facility. The time structures of the most intense γ rays emitted following the β decay were used to determine the half-lives of 128Cd and 130Cd to be T1/2=246.2(21)ms and T1/2=126(4) ms, respectively. The half-lives of the 3/2+ and 11/2− states of 129Cd were measured to be T1/2(3/2+)=157(8) ms and T1/2(11/2−)=147(3) ms. The half-lives of the Cd isotopes around the N=82 shell closure are an important ingredient in astrophysical simulations to derive the magnitude of the second r-process abundance peak in the A∼130 region. Our new results are compared with recent literature values and theoretical calculations.

U2 - 10.1103/PhysRevC.93.062801

DO - 10.1103/PhysRevC.93.062801

M3 - Article

VL - 93

JO - Physical Review C

JF - Physical Review C

SN - 2469-9985

IS - 6

ER -