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Nuclear masses in astrophysics

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 29 Jul 2009Embargo end date: 01 Jan 2008Publisher:Sissa MedialabJournal:Proceedings of 10th Symposium on Nuclei in the Cosmos — PoS(NIC X)Funded by:NSF | Operation of the National...

Authors: Klaus Blaum; Christine Weber; Hendrik Schatz;

doi: 10.22323/1.053.0028 , 10.48550/arxiv.0812.1675

arXiv: http://arxiv.org/abs/0812.1675

Nuclear masses in astrophysics

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Abstract

Among all nuclear ground-state properties, atomic masses are highly specific for each particular combination of N and Z and the data obtained apply to a variety of physics topics. One of the most crucial questions to be addressed in mass spectrometry of unstable radionuclides is the one of understanding the processes of element formation in the Universe. To this end, accurate atomic mass values of a large number of exotic nuclei participating in nucleosynthesis are among the key input data in large-scale reaction network calculations. In this paper, a review on the latest achievements in mass spectrometry for nuclear astrophysics is given.

Proceedings of the 10th Symposium on Nuclei in the Cosmos, NIC X - Mackinac Island, Michigan, USA (10 pages, 4 figures)

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Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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