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Gd and
Gd using the (
) reactionRoss, T. J.*; Hughes, R. O.*; Allmond, J. M.*; Beausang, C. W.*; Angell, C.; Basunia, M. S.*; Bleuel, D. L.*; Hurke, J. T.*; Casperson, R. J.*; Escher, J. E.*; et al.
Physical Review C, 90(4), p.044323_1 - 044323_12, 2014/10
Times Cited Count:7 Percentile:44.33(Physics, Nuclear)
= 64 neutron subshell closure on the structure of
90 gadolinium nucleiRoss, T. J.*; Hughes, R. O.*; Beausang, C. W.*; Allmond, J. M.*; Angell, C.; Basunia, M. S.*; Bleuel, D. L.*; Burke, J. T.*; Casperson, R. J.*; Escher, J. E.*; et al.
Physical Review C, 88(3), p.031301_1 - 031301_4, 2013/09
Times Cited Count:7 Percentile:45.51(Physics, Nuclear)
Y by the (
) reactionRoss, T. J.*; Beausang, C. W.*; Hughes, R. O.*; Scielzo, N. D.*; Burke, J. T.*; Allmond, J. M.*; Angell, C.; Basunia, M. S.*; Bleuel, D. L.*; Casperson, R. J.*; et al.
Physical Review C, 86(6), p.067301_1 - 067301_5, 2012/12
Times Cited Count:3 Percentile:21.77(Physics, Nuclear)
,
) and (
,
) reactionsRoss, T. J.*; Beausang, C. W.*; Hughes, R. O.*; Allmond, J. M.*; Angell, C.; Basunia, M. S.*; Bleuel, D. L.*; Burke, J. T.*; Casperson, R. J.*; Escher, J. E.*; et al.
Physical Review C, 85(5), p.051304_1 - 051304_5, 2012/05
Times Cited Count:11 Percentile:51.40(Physics, Nuclear)The surrogate reaction technique has been employed to
cross sections in the actinide region to a precision of 20%, but in the rare earth region a factor of 2-3 discrepancy exists between the directly measured
and extracted surrogate cross sections. A possible origin of this discrepancy lies in differences between the initial spin/parity population distribution. To investigate this, the angular momentum transfer of the surrogate reaction in Gd nuclei has been measured.
PBender, P. C.*; Tabor, S. L.*; Tripathi, V.*; Hoffman, C. R.*; Hamilton, L.*; Volya, A.*; Clark, R. M.*; Fallon, P.*; Macchiavelli, A. O.*; Paschalis, S.*; et al.
Physical Review C, 85(4), p.044305_1 - 044305_10, 2012/04
Times Cited Count:12 Percentile:53.79(Physics, Nuclear)The available experimental information on
P has been greatly increased through the analysis of
decays in coincidence with protons from the interaction of an
O beam at 24 MeV with an
O target. Light charged particles from the reaction were detected with Microball, and multiple
ray coincidences with Gammasphere. Many newly observed
transitions have been identified and placed in the level scheme. Additionally, for most states, spins have been assigned based on measured
ray angular distributions while parities were inferred from lifetimes determined through Doppler-broadened line-shape analysis. Most of the states observed have been interpreted in terms of shell-model calculations using the WBP-a and SDPF-NR interactions having one particle in the 0
or 1
orbital. The two calculations agree almost equally well with the data resulting in root-mean-square differences of about 200 keV. However, two of a few high-lying states may be associated with stretched 



states, but the calculations over-predict their energies by 2-3 MeV. Furthermore, a newly observed long-lived 7919-keV state is established for which no explanation is available at present.