2020
DOI: 10.1088/1361-6471/abacda
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Exact sum rules with approximate ground states

Abstract: Electromagnetic and weak transitions tell us a great deal about the structure of atomic nuclei. Yet modeling transitions can be difficult: it is often easier to compute the ground state, if only as an approximation, than excited states. One alternative is through transition sum rules, in particular the non-energy-weighted and energy-weighted sum rules, which can be computed as expectation values of operators. We investigate by computing sum rules for a variety of nuclei, comparing the numerically exact full co… Show more

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Cited by 8 publications
(7 citation statements)
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References 55 publications
(96 reference statements)
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“…Note that the validity of the usual sum rule depends on the structure of the subspace (see Appendix A). This fact is known numerically [37], and it can be seen also with the DGCM and the GCM. table are the ratios of the left-hand side to the right-hand side of Eqs.…”
Section: B Resultsmentioning
confidence: 64%
“…Note that the validity of the usual sum rule depends on the structure of the subspace (see Appendix A). This fact is known numerically [37], and it can be seen also with the DGCM and the GCM. table are the ratios of the left-hand side to the right-hand side of Eqs.…”
Section: B Resultsmentioning
confidence: 64%
“…is more than 5 MeV. For example, 32 S is a rotational nucleus, while the Hartree-Fock minimum generates a spherical shape for it, therefore only a 0 + is projected out, as is also pointed out in [47]. PVPC is rather accurate for ground states of semi-magic nuclei, with ∆E PVPC g.s.…”
Section: A Even-even Nuclei In 1s0d Shellmentioning
confidence: 78%
“…Nuclear approaches to reactions and scattering face several challenges, especially since nuclear probes are often peripheral and, hence, require a correct asymptotic treatment. Major challenges include: the long-range Coulomb force, and in particular in the case of large projectile and/or target charges where the asymptotics may not be analytically known; the high sensitivity of reaction observables to the reaction thresholds (Q-values); the importance of the non-resonant continuum when nuclei break up into the continuum; and the difficulties in describing scattering states asymptotics with single-particle bound-state bases typically used in many-body methods (31).…”
Section: Rare Isotope Beam Facilities and Needs For Theorymentioning
confidence: 99%
“…Thus, for example, experiments can provide precise thresholds, whereas theory can pinpoint critical collective and clustering correlations in wave functions to achieve the best estimates for reaction rates for astrophysics. Indeed, to analyze and interpret experimental data, theory with uncertainties lower than 10% is needed (31).…”
Section: Rare Isotope Beam Facilities and Needs For Theorymentioning
confidence: 99%
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