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論文

Evidence of nonstatistical neutron emission following $$beta$$ decay near doubly magic $$^{132}$$Sn

Heideman, J.*; Grzywacz, R.*; Xu, Z. Y.*; Madurga, M.*; Escher, J. E.*; 河野 俊彦*; Algora, A.*; Andreyev, A. N.; 他41名*

Physical Review C, 108(2), p.024311_1 - 024311_9, 2023/08

$$beta$$-delayed neutron emission was observed in the study of the $$beta$$ decay of $$^{134}$$In at ISOLDE CERN. Neutron emission probabilities from the unbound states in $$^{134}$$Sn to known low-lying, single-particle states in $$^{133}$$Sn were measured. The neutron energies were determined using the time-of-flight technique and the decay from excited states in $$^{133}$$Sn was studied by detecting its $$gamma$$ rays. Individual $$beta$$-delayed neutron emission probabilities were determined by correlating the relative intensities and energies of neutrons and $$gamma$$ rays. The new results suggest the violation of the assumption that neutrons are emitted statistically via the intermediate compound nucleus. This impacts the neutron-emission probabilities and other properties of nuclei participating in the r-process. A model of neutron emission, which links the observed neutron emission probabilities to nuclear shell effects, is proposed.

論文

Charge radii, moments, and masses of mercury isotopes across the $$N$$=126 shell closure

Day Goodacre, T.*; Afanasjev, A. V.*; Barzakh, A. E.*; Nies, L.*; Marsh, B. A.*; Sels, S.*; Perera, U. C.*; Ring, P.*; Wienholz, F.*; Andreyev, A. N.; et al.

Physical Review C, 104(5), p.054322_1 - 054322_18, 2021/11

 被引用回数:8 パーセンタイル:80.56(Physics, Nuclear)

Combining laser spectroscopy with Penning-trap mass spectroscopy at the Isolde facility at CERN, the charge radii of neutron-rich mercury isotopes $$^{202,203,206,207,208}$$Hg were successfully measured. Furthermore, more precise values for the masses of $$^{206,207,208}$$Hg was obtained, as well as the magnetic moment of $$^{207}$$Hg. These results were used to understand the systematics of Hg isotopes across the $$N$$=126 shell closure. Comparison with covariant density functional theory calculations revealed that in particular the 1$$i_{11/2}$$ and 2$$g_{9/2}$$ neutron orbitals affect the evolution of charge radii.

論文

Characterization of the shape-staggering effect in mercury nuclei

Marsh, B. A.*; Day Goodacre, T.*; 角田 佑介*; Andreyev, A. N.; 他41名*

Nature Physics, 14(12), p.1163 - 1167, 2018/12

 被引用回数:82 パーセンタイル:96.77(Physics, Multidisciplinary)

In rare cases, the removal of a single proton (Z) or neutron (N) from an atomic nucleus leads to a dramatic shape change. These instances are crucial for understanding the components of the nuclear interactions that drive deformation. The mercuryisotopes (Z = 80) are a striking example: their close neighbours, the lead isotopes (Z = 82), are spherical and steadily shrink with decreasing N. The even-mass (A = N + Z) mercury isotopes follow this trend. The odd-mass mercury isotopes $$^{181,183,185}$$Hg, however, exhibit noticeably larger charge radii. Due to the experimental difficulties of probing extremely neutron-deficient systems, and the computational complexity of modelling such heavy nuclides, the microscopic origin of this unique shape staggering has remained unclear. Here, by applying resonance ionization spectroscopy, mass spectrometry and nuclear spectroscopy as far as $$^{177}$$Hg, we determine $$^{181}$$Hg as the shape-staggering endpoint. By combining our experimental measurements with Monte Carlo shell model calculations, we conclude that this phenomenon results from the interplay between monopole and quadrupole interactions driving a quantum phase transition, for which we identify the participating orbitals. Although shape staggering in the mercury isotopes is a unique and localized feature in the nuclear chart, it nicely illustrates the concurrence of single-particle and collective degrees of freedom at play in atomic nuclei.

論文

First accurate normalization of the $$beta$$-delayed $$alpha$$ decay of $$^{16}$$N and implications for the $$^{12}$$C($$alpha$$,$$gamma$$)$$^{16}$$O astrophysical reaction rate

Kirsebom, O. S.*; Tengblad, O.*; Andreyev, A. N.; 他41名*

Physical Review Letters, 121(14), p.142701_1 - 142701_6, 2018/10

 被引用回数:7 パーセンタイル:51.12(Physics, Multidisciplinary)

The $$^{12}$$C($$alpha$$,$$gamma$$)$$^{16}$$O reaction plays a central role in astrophysics, but its cross section at energies relevant for astrophysical applications is only poorly constrained by laboratory data. The reduced $$alpha$$ width, $$gamma_{rm 11}$$, of the bound 1$$^{-}$$ level in $$^{16}$$O is particularly important to determine the cross section. The magnitude of $$gamma_{11}$$ is determined via sub-Coulomb $$alpha$$-transfer reactions or the $$beta$$-delayed $$alpha$$ decay of $$^{16}$$N, but the latter approach is presently hampered by the lack of sufficiently precise data on the $$beta$$-decay branching ratios. Here we report improved branching ratios for the bound 1$$^{-}$$ level ($$b_{beta,11}$$) and for $$beta$$-delayed $$alpha$$ emission ($$b_{beta alpha}$$). Our value for $$b_{beta alpha}$$ is 33 $$%$$ larger than previously held, leading to a substantial increase in $$gamma_{11}$$. Our revised value for $$gamma_{11}$$ is in good agreement with the value obtained in $$alpha$$-transfer studies and the weighted average of the two gives a robust and precise determination of $$gamma_{11}$$, which provides significantly improved constraints on the $$^{12}$$C($$alpha$$,$$gamma$$)$$^{16}$$O cross section in the energy range relevant to hydro static He burning.

論文

Observation of spin-dependent charge symmetry breaking in $$Lambda N$$ interaction; $$gamma$$-ray spectroscopy of $$^4_{Lambda}$$He

山本 剛史*; 長谷川 勝一; 早川 修平; 細見 健二; Hwang, S.; 市川 裕大; 今井 憲一; 金原 慎二; 中田 祥之; 佐甲 博之; et al.

Physical Review Letters, 115(22), p.222501_1 - 222501_5, 2015/11

AA2015-0707.pdf:0.5MB

 被引用回数:65 パーセンタイル:92.69(Physics, Multidisciplinary)

The energy spacing between the spin-doublet bound state of $$^4_{Lambda}$$He$$(1^+,0^+)$$ was determined to be $$1406 pm 2 pm 2$$ keV, by measuring $$gamma$$ rays for the $$1^+ to 0^+$$ transition with a high efficiency germanium detector array in coincidence with the $$^4{rm He}(K^-,pi^-)^4_{Lambda}$$He reaction at J-PARC. In comparison to the corresponding energy spacing in the mirror hypernucleus $$^4_{Lambda}$$H, the present result clearly indicates the existence of charge symmetry breaking (CSB) in $$Lambda N$$ interaction. By combining the energy spacings with the known ground-state binding energies, it is also found that the CSB effect is large in the $$0^+$$ ground state but is vanishingly small in the $$1^+$$ excited state, demonstrating that the $$Lambda N$$ CSB interaction has spin dependence.

論文

Perspective of negative triangularity tokamak as fusion energy system

菊池 満; Medvedev, S.*; 滝塚 知典*; Fasoli, A.*; Wu, Y.*; Diamond, P. H.*; Duan, X.*; 岸本 泰明*; 花田 和明*; 他41名*

Europhysics Conference Abstracts (Internet), 39E, p.P4.179_1 - P4.179_4, 2015/06

核融合炉における熱粒子制御は挑戦的課題である。定常的な熱負荷とエルムによる過渡的熱負荷を緩和する新しい方策として負三角度トカマクを評価している。これまで、負三角度は磁気丘であるにもかかわらず、ダブルヌルでは炉に使えるレベルの規格化ベータ値3以上が安定であることを見いだしている。本論文では、シングルヌル平衡配位とその理想電磁流体安定性を報告する。

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