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Normal ordering of three-nucleon interactions for ab initio calculations of heavy nuclei

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arxiv 2211.16262 v3 pith:7M5NJTAI submitted 2022-11-29 nucl-th

classification nucl-th
keywords interactionscalculationsnormalnucleiorderingallowsbasisframework
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Three-nucleon (3N) interactions are key for an accurate solution of the nuclear many-body problem. However, fully taking into account 3N forces constitutes a computational challenge and hence approximate treatments are commonly employed. The method of normal ordering has proven to be a powerful tool that allows to systematically include 3N interactions in an efficient way, but traditional normal-ordering frameworks require the representation of 3N interactions in a large single-particle basis, typically necessitating a truncation of 3N matrix elements. While this truncation has only a minor impact for light and medium-mass nuclei, its effects become sizable for heavier systems and hence limit the scope of \textit{ab initio} calculations. In this work, we present a novel normal-ordering framework that allows to circumvent this limitation by performing the normal ordering directly in a Jacobi basis. We discuss in detail the new framework, benchmark it against established results, and present calculations for ground-state energies and charge radii of heavy nuclei, such as $^{132}$Sn and $^{208}$Pb.

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Cited by 2 Pith papers

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  1. Constraining Hamiltonians from chiral effective field theory with neutron-star data

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    Neutron-star data, run through fast emulators, directly constrain the six two-nucleon low-energy constants of an N2LO chiral Hamiltonian, with future detectors able to strongly pin down the 3P1 channel.

  2. Improved structure of calcium isotopes from ab initio calculations

    nucl-th 2024-11 conditional novelty 6.0 of 10

    IMSRG(3)-N7 calculations for calcium-44, -48, and -52 show that three-body flow corrections substantially lower the 48Ca 2+ energy, improving the description of the N=28 shell closure, while leaving the 52Ca charge-ra...

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