Abstract
We develop a method to construct a microscopic optical potential from chiral interactions for nucleon-nucleus scattering. The optical potential is constructed by combining the Green's function approach with the coupled-cluster method. To deal with the poles of the Green's function along the real energy axis we employ a Berggren basis in the complex energy plane combined with the Lanczos method. Using this approach, we perform a proof-of-principle calculation of the optical potential for the elastic neutron scattering on O16. For the computation of the ground state of O16, we use the coupled-cluster method in the singles-and-doubles approximation, while for the A±1 nuclei we use particle-attached/removed equation-of-motion method truncated at two-particle-one-hole and one-particle-two-hole excitations, respectively. We verify the convergence of the optical potential and scattering phase shifts with respect to the model-space size and the number of discretized complex continuum states. We also investigate the absorptive component of the optical potential (which reflects the opening of inelastic channels) by computing its imaginary volume integral and find an almost negligible absorptive component at low energies. To shed light on this result, we computed excited states of O16 using the equation-of-motion coupled-cluster method with singles-and-doubles excitations and we found no low-lying excited states below 10 MeV. Furthermore, most excited states have a dominant two-particle-two-hole component, making higher-order particle-hole excitations necessary to achieve a precise description of these core-excited states. We conclude that the reduced absorption at low energies can be attributed to the lack of correlations coming from the low-order cluster truncation in the employed coupled-cluster method.
Original language | English |
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Article number | 024315 |
Journal | Physical Review C |
Volume | 95 |
Issue number | 2 |
DOIs | |
State | Published - Feb 15 2017 |
Funding
This work was supported by the Office of Nuclear Physics, U.S. Department of Energy under Contracts No. DE-FG02-96ER40963, No. DE-FG52-08NA28552 (RIBSS Center), and No. DE-SC0008499 (NUCLEI SciDAC collaboration), and by the Field Work Proposal ERKBP57 at Oak Ridge National Laboratory (ORNL). We also acknowledge the support of the National Science Foundation under Grants No. PHY-1520929 and No. PHY-1403906. Computer time was provided by the Institute for Cyber-Enabled Research at Michigan State University and the Innovative and Novel Computational Impact on Theory and Experiment (INCITE) program. This research used resources of the Oak Ridge Leadership Computing Facility located at ORNL, which is supported by the Office of Science of the Department of Energy under Contract No. DE-AC05-00OR22725.