Abstract
Background: In this new era of radioactive beam facilities, the discovery of novel modes of excitation in nuclei far away from stability represents an area of intense research activity. In addition, some of these modes of excitation, particularly the isoscalar monopole and isovector dipole resonances, appear to be sensitive to the uncertain density dependence of the symmetry energy.
Purpose: It is the main goal of this paper to examine the emergence, evolution, and nature of both the soft and giant isoscalar monopole modes as a function of neutron excess in three unstable nickel isotopes: , and .
Methods: The distribution of isoscalar monopole strength is computed in a relativistic random-phase approximation by using several accurately calibrated effective interactions. In particular, a nonspectral Green's function approach is adopted that allows for an exact treatment of the continuum without any reliance on discretization. The discretization of the continuum is neither required nor admitted.
Results: In the case of , the lack of low-energy strength results in a direct correlation between the centroid energy of the giant monopole resonance and the incompressibility coefficient of symmetric nuclear matter. In contrast, the large neutron excess in both and generates a significant, yet relatively featureless, amount of low-energy strength that is driven by transitions into the continuum. Moreover, the evolution of monopole strength with neutron excess displays sensitivity to the density dependence of the symmetry energy.
Conclusions: It is suggested that future measurements of the distribution of isoscalar monopole strength at radioactive beam facilities using a very long chain of both stable and unstable isotopes could place important constraints on the equation of state of neutron-rich matter and ultimately on the properties of neutron stars. However, given the nature of the low-energy monopole excitations, a proper treatment of the continuum is absolutely essential.
- Received 14 October 2014
DOI:https://doi.org/10.1103/PhysRevC.91.014303
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