Muon capture on 6Li, 12C, and 16O from ab initio nuclear theory
Jokiniemi, L., Navrátil, P., Kotila, J., & Kravvaris, K. (2024). Muon capture on 6Li, 12C, and 16O from ab initio nuclear theory. Physical Review C, 109(6), Article 065501. https://doi.org/10.1103/physrevc.109.065501
Julkaistu sarjassa
Physical Review CPäivämäärä
2024Tekijänoikeudet
© 2024 American Physical Society
Muon capture on nuclei is one of the most promising probes of the nuclear electroweak current driving the yet-hypothetical neutrinoless double-beta (0νββ) decay. Both processes involve vector and axial-vector currents at finite momentum transfer, q∼100 MeV, as well as the induced pseudoscalar and weak-magnetism currents. Comparing measured muon-capture rates with reliable ab initio nuclear-theory predictions could help us validate these currents. To this end, we compute partial muon-capture rates for 6Li, 12C and 16O, feeding the ground and excited states in 6He, 12B and 16N, using ab initio no-core shell model with two- and three-nucleon chiral interactions. We remove the spurious center-of-mass motion by introducing translationally invariant operators and approximate the effect of hadronic two-body currents by Fermi-gas model. We solve the bound-muon wave function from the Dirac wave equations in the Coulomb field created by a finite nucleus. We find that the computed rates to the low-lying states in the final nuclei are in good agreement with the measured counterparts. We highlight sensitivity of some of the transitions to the sub-leading three-nucleon interaction terms. We also compare summed rates to several tens of final states with the measured total capture rates and note that we slightly underestimate the total rate with this simple approach due to limited range of excitation energies.
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American Physical SocietyISSN Hae Julkaisufoorumista
2469-9985Asiasanat
Julkaisu tutkimustietojärjestelmässä
https://converis.jyu.fi/converis/portal/detail/Publication/220445391
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Suomen AkatemiaRahoitusohjelmat(t)
Akatemiatutkija, SA; Akatemiatutkijan tutkimuskulut, SALisätietoja rahoituksesta
This work was supported by Arthur B. McDonald Canadian Astroparticle Physics Research Institute, by the NSERC Grant No. SAPIN-2022-00019, by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Work Proposals No. SCW0498, and by the Academy of Finland, Grant Nos. 314733 and 345869. K.K. receives partial support through the Scientific Discovery through Advanced Computing (SciDAC) program funded by U.S. Department of Energy, Office of Science, Advanced Scientific Computing Research and Nuclear Physics. TRIUMF receives federal funding via a contribution agreement with the National Research Council of Canada. This work was prepared in part by LLNL under Contract No. DE-AC52-07NA27344. ...Lisenssi
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