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arXiv 0808.4065nucl-ex
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用JYFLTRAP和SHIPTRAP测量rp过程和nu p过程轨道附近的质量

Mass measurements in the vicinity of the rp-process and the nu p-process paths with JYFLTRAP and SHIPTRAP

C. Weber, V. -V. Elomaa, R. Ferrer, C. Fröhlich, D. Ackermann, J. Äystö, G. Audi, L. Batist, K. Blaum, M. Block, A. Chaudhuri, M. Dworschak, S. Eliseev, T. Eron… 展开作者

C. Weber, V. -V. Elomaa, R. Ferrer, C. Fröhlich, D. Ackermann, J. Äystö, G. Audi, L. Batist, K. Blaum, M. Block, A. Chaudhuri, M. Dworschak, S. Eliseev, T. Eronen, U. Hager, J. Hakala, F. Herfurth, F. P. Heßberger, S. Hofmann, A. Jokinen, A. Kankainen, H. -J. Kluge, K. Langanke, A. Martín, G. Martínez-Pinedo, M. Mazzocco, I. D. Moore, J. B. Neumayr, Yu. N. Novikov, H. Penttilä, W. R. Plaß, A. V. Popov, S. Rahaman, T. Rauscher, C. Rauth, J. Rissanen, D. Rodríguez, A. Saastamoinen, C. Scheidenberger, L. Schweikhard, D. M. Seliverstov, T. Sonoda, F. -K. Thielemann, P. G. Thirolf, G. K. Vorobjev

摘要:

位于JYFL/Jyväskylä的Penning阱装置JYFLTRAP和位于GSI/Darmstadt的SHIPTRAP已经确定了接近天体物理rp和nu p过程路径的非常缺中子核素的质量。从钇(Z = 39)到钯(Z = 46)的同位素都是在重离子熔融蒸发反应中产生的。总共研究了21种核素,其中近一半的质量值是首次通过实验确定的:88 Tc,90- 92 Ru,92- 94 Rh和94,95 Pd。对于95 Pdm,(21/2^+)高自旋态,进行了第一次直接质量测定。得到了典型$δm / m = 5 \times 10^{-8}$的相对质量不确定度。新的质量值的影响进行了研究,在nu p过程核合成计算。将得到的反应流和最终丰度与2003年原子质量评估的数据进行比较。

英文摘要:

The masses of very neutron-deficient nuclides close to the astrophysical rp- and nu p-process paths have been determined with the Penning trap facilities JYFLTRAP at JYFL/Jyväskylä and SHIPTRAP at GSI/Darmstadt. Isotopes from yttrium (Z = 39) to palladium (Z = 46) have been produced in heavy-ion fusion-evaporation reactions. In total 21 nuclides were studied and almost half of the mass values were experimentally determined for the first time: 88Tc, 90-92Ru, 92-94Rh, and 94,95Pd. For the 95Pdm, (21/2^+) high-spin state, a first direct mass determination was performed. Relative mass uncertainties of typically $δm / m = 5 \times 10^{-8}$ were obtained. The impact of the new mass values has been studied in nu p-process nucleosynthesis calculations. The resulting reaction flow and the final abundances are compared to those obtained with the data of the Atomic Mass Evaluation 2003.

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