The MEG~II experiment at the Paul Scherrer Institut searches for the charged Lepton Flavor Violating decay $\mu^+ \to e^+\gamma$, a golden channel to test the validity of the Standard Model and to explore possible signatures of New Physics. In this thesis, we report the results of the MEG~II analysis of the dataset collected during the 2021–2022 physics runs, achieving the highest sensitivity to date on the $\mu^+ \to e^+\gamma$ branching ratio, $\mathcal{S} = 2.2 \times 10^{-13}$. No evidence for the $\mu^+ \to e^+\gamma$ decay was observed, and a new upper limit on the branching ratio was established: \[ \text{BR}(\mu^+\to e^+\gamma) \leq 1.5 \times 10^{-13} \ (90\% \ \text{C. L.}) \] which is twice as stringent as the previous limit. A central contribution to this achievement was the calibration of the experiment’s tracking detector—a single-volume cylindrical drift chamber—using 2022 data, along with the optimization of its performance through updates to the positron reconstruction algorithms, leading to a 10\% improvement in resolution. Systematic uncertainties related to tracker alignment were also significantly reduced thanks to a novel tracking algorithm for cosmic ray events. This thesis details the candidate’s work on these developments and their impact on the final analysis.
The MEG II Drift Chamber and the Search for Rare Muon Decays: Performance and Implications for Recent Experimental Results
VENTURINI, ANTOINE
2026
Abstract
The MEG~II experiment at the Paul Scherrer Institut searches for the charged Lepton Flavor Violating decay $\mu^+ \to e^+\gamma$, a golden channel to test the validity of the Standard Model and to explore possible signatures of New Physics. In this thesis, we report the results of the MEG~II analysis of the dataset collected during the 2021–2022 physics runs, achieving the highest sensitivity to date on the $\mu^+ \to e^+\gamma$ branching ratio, $\mathcal{S} = 2.2 \times 10^{-13}$. No evidence for the $\mu^+ \to e^+\gamma$ decay was observed, and a new upper limit on the branching ratio was established: \[ \text{BR}(\mu^+\to e^+\gamma) \leq 1.5 \times 10^{-13} \ (90\% \ \text{C. L.}) \] which is twice as stringent as the previous limit. A central contribution to this achievement was the calibration of the experiment’s tracking detector—a single-volume cylindrical drift chamber—using 2022 data, along with the optimization of its performance through updates to the positron reconstruction algorithms, leading to a 10\% improvement in resolution. Systematic uncertainties related to tracker alignment were also significantly reduced thanks to a novel tracking algorithm for cosmic ray events. This thesis details the candidate’s work on these developments and their impact on the final analysis.| File | Dimensione | Formato | |
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https://hdl.handle.net/20.500.14242/368412
URN:NBN:IT:UNIPI-368412