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  • 1
    Electronic Resource
    Electronic Resource
    Muon capture on neutron-rich nuclei (2001)
    Springer
    The European physical journal 11 (2001), S. 39-45 
    Details
    ISSN: 1434-601X
    Keywords: PACS. 24.30.Cz Giant resonances – 23.40.-s Beta decay; double beta decay; electron and muon capture – 23.40.Hc Relation with nuclear matrix elements and nuclear structure
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract: Future facilities will allow the exploration of extremely neutron-rich nuclei far from the valley of stability. It is discussed that the strong-neutron excess results in changes in the collective excitations of such nuclei compared to conventional stable nuclei. We propose muon capture as an experimental tool to explore such changes. We will quantify our discussion by the calculation of the total and differential muon capture rates on selected calcium isotopes between 40Ca and 60Ca. Our calculations are based on the random phase approximation and agree nicely with the measured rates for 40Ca and 44Ca.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/s100500170094
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    Paper (German National Licenses)
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  • 2
    Electronic Resource
    Electronic Resource
    Study of the 3He(4He,γ)7Be and 3H(4He,γ)7Li Reactions in an Extended Two-Cluster Model (2000)
    Springer
    Few body systems 29 (2000), S. 121-130 
    Details
    ISSN: 1432-5411
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract.  The 3He(4He, γ)7Be and 3H(4He, γ)7Li reactions are studied in an extended two-cluster model which contains α + h/t and 6Li + p/n clusterizations. We show that the inclusion of the 6Li + p/n channels can significantly change the zero-energy reaction cross sections, S(0), and other properties of the 7Be and 7Li nuclei, like the quadrupole moments Q. However, the results agree with the known correlation trend between S(0) and Q. Moreover, we demonstrate that the value of the zero-energy derivatives of the astrophysical S-factors are more uncertain than currently believed.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/s006010070012
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    Paper (German National Licenses)
    Fulltext
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