## Abstract

Recent calculations of nuclear structure corrections to the Lamb shift in light muonic atoms are based on an expansion in a parameter η, where only terms up to second order are retained. The parameter η can be shown to be proportional to mr/mp, where mr is the reduced mass of the muon-nucleus system and mp is the proton mass, so that it is small and the expansion is expected to converge. However, practical implementations show that the η 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 η-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 η-less expansion, indicating that the nucleon form factor approximations by Ji et al. [J. Phys. G 45, 093002 (2018)10.1088/1361-6471/aad3eb] should be improved. However, we find that the sum of these terms removes this dependence and the uncertainty due to the η 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.

Original language | American English |
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Article number | 064315 |

Journal | Physical Review C |

Volume | 100 |

Issue number | 6 |

DOIs | |

State | Published - 20 Dec 2019 |

### Bibliographical note

Funding Information:The authors would like to thank Nir Nevo Dinur for insightful discussions. This work has been supported by the Cluster of Excellence “Precision Physics, Fundamental Interactions, and Structure of Matter” ( PRISMA + EXC 2118/1) funded by the German Research Foundation (DFG) within the German Excellence Strategy (Project No. 39083149), and by the National Natural Science Foundation of China (Grant No. 11805078). APPENDIX A:

Publisher Copyright:

© 2019 American Physical Society.