Density-dependent nuclear interactions and the beta decay of 14C: chiral three-nucleon forces and Brown-Rho scaling
J. W. Holt, N. Kaiser, and W. Weise

TL;DR
This paper investigates how density-dependent nuclear interactions, derived from chiral effective field theory and Brown-Rho scaling, explain the unusually long beta decay lifetime of 14C by incorporating medium modifications into shell model calculations.
Contribution
It demonstrates that medium modifications of nuclear forces are crucial for accurately reproducing the long lifetime of 14C within a shell model framework.
Findings
Both three-nucleon forces and Brown-Rho scaling yield similar qualitative results.
Medium modifications significantly increase the 14C lifetime to archaeological timescales.
Effective interactions at low-momentum scales are essential for accurate decay predictions.
Abstract
We study the role of density-dependent low-momentum nucleon-nucleon interactions in describing the anomalously long beta decay lifetime of 14C. We approach this problem both from the perspective of chiral effective field theory, in which genuine three-body forces generate an effective density-dependent two-body interaction, as well as from the perspective of Brown-Rho scaling, in which the masses and form factor cutoffs in one-boson-exchange interactions are modified in a dense nuclear medium due to the partial restoration of chiral symmetry. The beta decay transition of 14C to the ground state of 14N is calculated within the shell model using a model space consisting of two 0p-shell holes within a closed 16O core. The effective 0p-shell interaction is calculated up to second order in perturbation theory with single-particle energies extracted from experiment. We find that both…
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Taxonomy
TopicsNuclear physics research studies · Scientific Research and Discoveries · Quantum, superfluid, helium dynamics
