Ab initio excited states from the in-medium similarity renormalization group

N. M. Parzuchowski, T. D. Morris, S. K. Bogner

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16 Scopus citations

Abstract

We present two new methods for performing ab initio calculations of excited states for closed-shell systems within the in-medium similarity renormalization group (IMSRG) framework. Both are based on combining the IMSRG with simple many-body methods commonly used to target excited states, such as the Tamm-Dancoff approximation (TDA) and equations-of-motion (EOM) techniques. In the first approach, a two-step sequential IMSRG transformation is used to drive the Hamiltonian to a form where a simple TDA calculation (i.e., diagonalization in the space of 1p1h excitations) becomes exact for a subset of eigenvalues. In the second approach, EOM techniques are applied to the IMSRG ground-state-decoupled Hamiltonian to access excited states. We perform proof-of-principle calculations for parabolic quantum dots in two dimensions and the closed-shell nuclei O16 and O22. We find that the TDA-IMSRG approach gives better accuracy than the EOM-IMSRG when calculations converge, but it is otherwise lacking the versatility and numerical stability of the latter. Our calculated spectra are in reasonable agreement with analogous EOM-coupled-cluster calculations. This work paves the way for more interesting applications of the EOM-IMSRG approach to calculations of consistently evolved observables such as electromagnetic strength functions and nuclear matrix elements, and extensions to nuclei within one or two nucleons of a closed shell by generalizing the EOM ladder operator to include particle-number nonconserving terms.

Original languageEnglish
Article number044304
JournalPhysical Review C
Volume95
Issue number4
DOIs
StatePublished - Apr 4 2017

Funding

We thank Gaute Hagen, Heiko Hergert, Morten Hjorth-Jensen, Gustav Jansen, and Ragnar Stroberg for useful discussions, and we thank Gaute Hagen for the use of his EOM-CCSD code. This work was supported in part by the National Science Foundation under Grant No. PHY-1404159, and by the NUCLEI SciDac Collaboration under DOE Grant No. DE-SC000851. This work was supported by the Office of Nuclear Physics, U.S. Department of Energy, under Grant No. DE-SC0008499 (NUCLEI SciDAC Collaboration). Oak Ridge National Laboratory is supported by the Office of Science of the Department of Energy under Contract No. DE-AC05-00OR22725.

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