2017
DOI: 10.1088/1402-4896/aa842a
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Medium and high spin structure in the94Y isotope produced in fission induced by cold neutrons

Abstract: The level scheme of the neutron-rich 94Y isotope has been extended up to the 5324 keV excitation energy. During the analysis, a structure above the previously known (5+) isomer, at 1202 keV, was extended by employing multifold gamma-ray coincidence relationships measured with the EXILL array. For some of the new states, the spin-parity assignment has been proposed on the basis of gamma angular correlations and shell-model considerations. The newly identified structure is characteristic of spherical or nearly s… Show more

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Cited by 2 publications
(8 citation statements)
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“…One clearly sees three strong γ lines which were uniquely attributed to 94 Y: 305.5(1)keV, 583.8(2) keV and 718.7(3) keV. The same γ rays were reported very recently in [27].…”
Section: Resultssupporting
confidence: 80%
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“…One clearly sees three strong γ lines which were uniquely attributed to 94 Y: 305.5(1)keV, 583.8(2) keV and 718.7(3) keV. The same γ rays were reported very recently in [27].…”
Section: Resultssupporting
confidence: 80%
“…Most of the observed (yrast) levels of 90 Y and 92 Y were so far measured in fusion-evaporation reactions 74 Ge( 18 O, γnp) and 76 Ge( 18 O, γ3np) for 90 Y [44]) or in multinucleon transfer reactions 238 U( 82 Se, Xγ) and 208 Pb( 90 Zr, Xγ) for 92 Y [45]. For 94 Y, very recently several transitions were reported in [27] where the level scheme has been extended up to the 5.3 MeV excitation energy.…”
Section: Resultsmentioning
confidence: 99%
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“…Inspired by the new results in the 96 Y isotope, our collaboration made an effort to develop the level scheme of the 94 Y nucleus, located 5 neutrons away from the N = 60 boundary. Using data from EXILL (and crosschecked with partially sorted data from FIPPS), the level scheme was extended up to 5 MeV excitation energy [19], however, no evidence of deformed structure in this isotope was found. This is not surprising, taking into account the significant decrease in population of the rotational bands, in comparison with the spherical pattern when further away from N = 60.…”
Section: Data Analysis and Discussionmentioning
confidence: 99%