Computation of spectroscopic factors with the coupled-cluster method
arXiv:1004.2611 · doi:10.1103/PhysRevC.82.014310
Abstract
We present a calculation of spectroscopic factors within coupled-cluster theory. Our derivation of algebraic equations for the one-body overlap functions are based on coupled-cluster equation-of-motion solutions for the ground and excited states of the doubly magic nucleus with mass number and the odd-mass neighbor with mass . As a proof-of-principle calculation, we consider O and the odd neighbors O and N, and compute the spectroscopic factor for nucleon removal from O. We employ a renormalized low-momentum interaction of the type derived from a chiral interaction at next-to-next-to-next-to-leading order. We study the sensitivity of our results by variation of the momentum cutoff, and then discuss the treatment of the center of mass.
8 pages, 6 figures, 3 tables
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Cited by in corpus (15)
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- Elastic proton scattering of medium mass nuclei from coupled-cluster theory
- Ab-initio approach to effective single-particle energies in doubly closed shell nuclei
- Efimov Physics around the neutron rich Calcium-60 isotope
- Coupled-cluster studies of infinite nuclear matter
- Radiative capture reactions in lattice effective field theory
- Adiabatic projection method for scattering and reactions on the lattice
- Astrophysical factor for the reaction from -matrix analysis and asymptotic normalization coefficient for . Is any fit acceptable?
- Microscopic description of translationally-invariant core+N+N overlap functions
- Closed-shell properties of O with {\em ab initio} coupled-cluster theory
- Spectroscopic factor strengths using approaches
- Nuclear Physics without High-Momentum Potentials: Constructing the Nuclear Effective Interaction Directly from Scattering Observables