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Download Perspectives on Nuclear Data for the Next Decade: Workshop by OECD Publishing PDF

By OECD Publishing

With a declining variety of nuclear facts evaluators on the planet and an expanding call for for top of the range facts, there's a threat that evaluators will be aware of generating new nuclear information to the detriment of constructing new types and strategies for eva

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Extra resources for Perspectives on Nuclear Data for the Next Decade: Workshop Proceedings -- Bruyeres-le-Châtel, France, 26-28 September 2005

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Conf. on Exotic Nuclei and Atomic Masses (E NAM ’95), Arles, June 1995, p. ps [12] E. doc 24 Why we need nuclear mass data and how we obtain it David Lunney Centre de Spectrom´etrie Nucl´eaire et de Spectrom´etrie de Masse IN2P3-CNRS, Universit´e de Paris Sud, Orsay, France November 13, 2006 Abstract The nuclear binding energy is of fundamental importance for a diverse range of physics and its determination results from mass measurements, employing an equally diverse range of experimental techniques.

In spite of the numerous advantages of this new interaction over the earlier one, we have observed that D1S was still unable to reproduce the Neutron Matter (NM) Equation Of State (EOS). The NM EOS was predicted by different authors. Their results, obtained by variational calculations, are very similar. We have chosen the EOS proposed by Friedman-Pandharipande (FP) as our benchmark to improve the Gogny force parameterization. The aim of the present study is to investigate a new parameterization of the Gogny force which fits the EOS of FP.

9] and Mahaux et al. [10] respectively. It can be checked that the nuclear matter properties obtained with D1S and with the new parameterization are in close agreement with the empirical values. However, it is worth mentioning the differences between predictions based on the two parameterizations. The numbers in Table 1 show that the compression modulus, the surface energy, the effective mass and the symmetry energy are a bit different for the two parameterizations. 8 MeV) between the symmetry energy obtained with D1S and the new parameterization can roughly be explained by assuming the so-called parabolic approximation: E E (ρ, β) = (ρ, β = 0) + Esym (ρ)β 2 .

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