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arXiv 1310.2697nucl-thnucl-ex
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Sn同位素的低能电偶极响应

Low-energy electric dipole response of Sn isotopes

P. Papakonstantinou, H. Hergert, V. Yu. Ponomarev, R. Roth

摘要:

我们研究了低能偶极(LED)强度沿Sn同位素链在等势线(IS)和等矢量(IV,或E1)电通道的分布,提供可检验的预测和指导新的实验与稳定的目标和放射性核束。我们使用自洽准粒子随机相位近似(QRPA)与有限范围的相互作用,主要是Gogny D1 S力。我们还分析了一个现实的两体相互作用的表现,辅以现象学的三体接触项。我们发现,从N=50和高达N=82壳层封闭(132 Sn)的IS-LED光谱的最低能量的一部分是由一个集体跃迁,其性质随中子数变化平滑,不能被解释为中子皮肤振荡占主导地位。对于富中子的物种,这种状态有助于E1强度低于粒子阈值,但更多的E1强度是由其他,弱,但许多过渡附近或阈值以上。我们发现,在光谱中的强结构变化的效果超过N=82,即增加的LED强度和较低的激发能。我们的结果与Gogny相互作用与现有的数据是兼容的。在此基础上,我们预测:a)对于N=50-82,低于粒子阈值的总的IS强度应具有相同的数量级,b)对于N=50-82 MeV,高达约12 MeV的总的E1强度应是相似的,而c)对于N ~ 64 - 82,低于阈值的总的E1强度应具有相同的数量级,并且对于较轻者弱得多,更对称的同位素我们指出,我们的结果与其他非相对论性的研究,集体的IS模式在这些研究中的一些情况下,一个可能是激进的相对论性模型的分歧一般协议。

英文摘要:

We study the low-energy dipole (LED) strength distribution along the Sn isotopic chain in both the isoscalar (IS) and the isovector (IV, or E1) electric channels, to provide testable predictions and guidance for new experiments with stable targets and radioactive beams. We use the self-consistent Quasi-particle Random-Phase Approximation (QRPA) with finite-range interactions and mainly the Gogny D1S force. We analyze also the performance of a realistic two-body interaction supplemented by a phenomenological three-body contact term. We find that from N=50 and up to the N=82 shell closure (132Sn) the lowest-energy part of the IS-LED spectrum is dominated by a collective transition whose properties vary smoothly with neutron number and which cannot be interpreted as a neutron-skin oscillation. For the neutron-rich species this state contributes to the E1 strength below particle threshold, but much more E1 strength is carried by other, weak but numerous transitions around or above threshold. We find that strong structural changes in the spectrum take effect beyond N=82, namely increased LED strength and lower excitation energies. Our results with the Gogny interaction are compatible with existing data. On this basis we predict that a) the summed IS strength below particle threshold shall be of the same order of magnitude for N=50-82, b) the summed E1 strength up to approximately 12 MeV shall be similar for N=50-82 MeV, while c) the summed E1 strength below threshold shall be of the same order of magnitude for N ~ 64 - 82 and much weaker for the lighter, more-symmetric isotopes. We point out a general agreement of our results with other non-relativistic studies, the absence of a collective IS mode in some of those studies, and a possibly radical disagreement with relativistic models.

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