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Elastic Scattering of Halo Nuclei
Author(s) -
R. C. Johnson,
Jim Al-Khalili,
J. A. Tostevin
Publication year - 1997
Publication title -
physical review letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.688
H-Index - 673
eISSN - 1079-7114
pISSN - 0031-9007
DOI - 10.1103/physrevlett.79.2771
Subject(s) - halo , elastic scattering , scattering , physics , projectile , core (optical fiber) , inelastic scattering , halo nucleus , coupling (piping) , excitation , atomic physics , nuclear physics , materials science , optics , astrophysics , quantum mechanics , composite material , galaxy
The existence of a class of light nuclei with a localized central core surrounded by a dilute “halo” of neutron matter is now well established. Evidence for these novel structures has been gained mainly from measurements of total neutron removal [1] and breakup reaction cross sections [2‐ 4], particularly at high energy. We investigate to what extent complementary information can be gained from high quality elastic scattering measurements at lower energies. In this Letter we show that, in certain circumstances, the elastic scattering of a halo nucleus from a stable target can give simple direct evidence for the structure of the halo. The theory makes explicit use of the characteristics of halo nuclei, namely their very small neutron separation energy and the large spatial extension of the halo, which in turn result in strong coupling between the halo ground state and low energy excitations. This coupling of the elastic and projectile excitation channels plays a crucial role in the analysis, the results of which cannot be readily understood in terms of optical or folding model approaches. In elastic scattering, the analysis is expected to be particularly useful in systems where the ratio of the halo particle mass to the core mass is small.

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