Probing uncertainties of nuclear structure corrections in light muonic atoms

PHYSICAL REVIEW C(2019)

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摘要
Recent calculations of nuclear structure corrections to the Lamb shift in light muonic atoms are based on an expansion in a parameter eta, where only terms up to second order are retained. The parameter eta can be shown to be proportional to root M-r/m(p), where m(r) is the reduced mass of the muon-nucleus system and m(p) is the proton mass, so that it is small and the expansion is expected to converge. However, practical implementations show that the eta convergence may be slower than expected. In this work, we probe the uncertainties due to this expansion using a different formalism, which is based on a multipole expansion of the longitudinal and transverse response functions. We refer to this alternative expansion as the eta-less formalism. We generalize this formalism to account for the cancellation of elastic terms such as the third Zemach moment (or Friar moment) and embed it in a computationally efficient framework. We implement and test this approach in the case of muonic deuterium. The comparison of results in the point nucleon limit for both methods achieve subpercent agreement. When nucleon form factors are introduced, we find 4% and 2% differences in the third Zemach moment and nuclear polarizability, respectively, compared to the eta-less expansion, indicating that the nucleon form factor approximations by Ji et al. [J. Phys. G 45, 093002 (2018)] should be improved. However, we find that the sum of these terms removes this dependence and the uncertainty due to the eta expansion and the related second-order approximation in the nucleon form factors amounts only to 0.2% and thus is fully justified in muonic deuterium. This computationally efficient framework paves the way for further studies in light muonic systems with more than two nucleons, where controlling and reducing uncertainties in nuclear structure corrections is key to the experimental efforts of the CREMA Collaboration.
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Nuclear Structure
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