Ab initio calculation of the β -decay spectrum of He 6

G. B. King, A. Baroni, V. Cirigliano, S. Gandolfi, L. Hayen, E. Mereghetti, S. Pastore, M. Piarulli

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Abstract

We calculate the β spectrum in the decay of He6 using quantum Monte Carlo methods with nuclear interactions derived from chiral effective field theory and consistent weak vector and axial currents. We work at second order in the multipole expansion, retaining terms suppressed by O(q2/mπ2), where q denotes low-energy scales such as the reaction's Q value or the electron energy, and mπ is the pion mass. We go beyond the impulse approximation by including the effects of two-body vector and axial currents. We estimate the theoretical error on the spectrum by using four potential models in the Norfolk family of local two- and three-nucleon interactions, which have different cutoffs, fit two-nucleon data up to different energies, and use different observables to determine the couplings in the three-body force. We find the theoretical uncertainty on the β spectrum, normalized by the total rate, to be well below the permille level, and to receive contributions of comparable size from first- and second-order corrections in the multipole expansion. We consider corrections to the β decay spectrum induced by beyond-standard-model charged-current interactions in the standard model effective field theory, with and without sterile neutrinos, and discuss the sensitivity of the next generation of experiments to these interactions.

Original languageEnglish
Article number015503
JournalPhysical Review C
Volume107
Issue number1
DOIs
StatePublished - Jan 2023
Externally publishedYes

Funding

We acknowledge stimulating conversations with A. Garcia, D. Gazit, A. Glick-Magid, M. Hoferichter, J. Menéndez, and R. Schiavilla. A.B., S.G., and E.M. are supported by the US Department of Energy through the Office of Nuclear Physics under Contract No. DE-AC52-06NA25396, and the LDRD program at Los Alamos National Laboratory. Los Alamos National Laboratory is operated by Triad National Security, LLC, for the National Nuclear Security Administration of U.S. Department of Energy (Contract No. 89233218CNA000001). The work of S.G. was also supported by the DOE Early Career research Program. L.H. is supported through the U.S. Department of Energy, Low Energy Physics Grant No. DE-FG02-ER41042 and NSF Grant No. PHY-1914133. This work is also supported by the U.S. Department of Energy under Contract No. DE-SC0021027 (G.K. and S.P.), a 2021 Early Career Award No. DE-SC0022002 (M.P.), the FRIB Theory Alliance Award No. DE-SC0013617 (S.P. and M.P.), and the U.S. DOE NNSA Stewardship Science Graduate Fellowship under Cooperative Agreement No. DE-NA0003960 (G. K.). V.C. is supported by the U.S. Department of Energy under Contract No. DE-FG02-00ER4113. The many-body calculations were performed on the parallel computers of the Laboratory Computing Resource Center, Argonne National Laboratory, and the computers of the Argonne Leadership Computing Facility via the INCITE grant “Ab-initio nuclear structure and nuclear reactions,” the 2019/2020 ALCC grant “Low Energy Neutrino-Nucleus interactions” for the project NNInteractions, the 2020/2021 ALCC grant “Chiral Nuclear Interactions from Nuclei to Nucleonic Matter” for the project ChiralNuc, and by the 2021/2022 ALCC grant “Quantum Monte Carlo Calculations of Nuclei up to and Neutron Matter” for the project QMCNuc. This research also used resources provided by the Los Alamos National Laboratory Institutional Computing Program, which is supported by the U.S. Department of Energy National Nuclear Security Administration under Contract No. 89233218CNA000001.

FundersFunder number
Low Energy PhysicsDE-FG02-ER41042
National Science FoundationDE-SC0022002, DE-NA0003960, PHY-1914133, DE-SC0013617, DE-FG02-00ER4113, DE-SC0021027
U.S. Department of Energy89233218CNA000001
National Nuclear Security Administration
Nuclear PhysicsDE-AC52-06NA25396
Los Alamos National Laboratory

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