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New Physics in $b \to s \mu \mu$: FCC-hh or a Muon Collider?

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arxiv 2205.13552 v2 pith:LFACSXEZ submitted 2022-05-26 hep-ph hep-ex

classification hep-phhep-ex
keywords fcc-hhphysicscollidercollidersanomaliesdiscoveryenergyfuture
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Rare flavour-changing neutral-current transitions $b \to s \mu^+ \mu^-$ probe higher energy scales than what is directly accessible at the LHC. Therefore, the presence of new physics in such transitions, as suggested by the present-day LHCb anomalies, would have a major impact on the motivation and planning of future high-energy colliders. The two most prominent options currently debated are a proton-proton collider at 100 TeV (FCC-hh) and a multi-TeV muon collider (MuC). In this work, we compare the discovery prospects at these colliders on benchmark new physics models indirectly detectable in $b \to s \mu^+ \mu^-$ decays but beyond the reach of the high-$p_T$ searches at the HL-LHC. We consider a comprehensive set of scenarios: semileptonic contact interactions, $Z^\prime$ from a gauged $U(1)_{B_3 - L_\mu}$ and $U(1)_{L_\mu - L_\tau}$, the scalar leptoquark $S_3$, and the vector leptoquark $U_1$. We find that a 3 TeV MuC has a sensitivity reach comparable to the one of the FCC-hh. However, for a heavy enough mediator, the new physics effects at a 3 TeV MuC are only observed indirectly via deviations in the highest energy bin, while the FCC-hh has a greater potential for the discovery of a resonance. Finally, to completely cover the parameter space suggested by the $bs\mu\mu$ anomalies, among the proposed future colliders, only a MuC of 10 TeV (or higher) can meet the challenge.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Probing maximal flavor changing $Z'$ in $U(1)_{L_\mu-L_\tau}$ at $\mu$TRISTAN

    hep-ph 2025-07 conditional novelty 5.0 of 10

    MuTRISTAN's mu+mu+ mode could discover a mu-tau flavor-changing Z' with gauge coupling near 0.024 for masses around 500 GeV.

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