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Muon Magnetic Anomaly

Updated 4 December 2025
  • Muon Magnetic Anomaly is the deviation of the muon’s gyromagnetic ratio from 2, serving as a precise test of quantum electrodynamics and the Standard Model.
  • Experimental techniques measure this anomaly via muon spin precession in uniform magnetic fields using high-precision NMR and calorimetry to achieve sub-ppm accuracy.
  • The observed tension between experimental results and theoretical predictions drives investigations into new physics models, such as supersymmetry and dark sector candidates.

The muon magnetic anomaly, denoted aμ=(gμ2)/2a_\mu = (g_\mu-2)/2, is a fundamental experimental and theoretical quantity in particle physics that quantifies the deviation of the muon's gyromagnetic ratio, gμg_\mu, from the Dirac value of 2. Precise measurement and calculation of aμa_\mu provide stringent tests of the Standard Model (SM), constrain radiative corrections, and serve as sensitive probes of physics beyond the SM. In recent years, measurements at Fermilab (E989) and Brookhaven (E821) have demonstrated a persistent tension between the experimental value of aμa_\mu and its SM prediction, reaching a significance of over 4σ4\sigma with current global averages. This anomaly is dominated by uncertainties in QCD-driven hadronic vacuum polarization, with new experimental approaches and theoretical developments aiming to resolve the discrepancy.

1. Formal Definition and Theoretical Decomposition

The anomalous magnetic moment is defined as: aμ=gμ22a_\mu = \frac{g_\mu - 2}{2} for a spin-½ particle of mass mμm_\mu and charge qq: μμ=gμq2mμS\vec{\mu}_\mu = g_\mu \frac{q}{2m_\mu} \vec{S}

Within the Standard Model, the anomaly is decomposed as: aμSM=aμQED+aμEW+aμHVP+aμHLbLa_\mu^{\rm SM} = a_\mu^{\rm QED} + a_\mu^{\rm EW} + a_\mu^{\rm HVP} + a_\mu^{\rm HLbL} where:

  • aμQEDa_\mu^{\rm QED}: Quantum electrodynamics contributions, computed up to 5 loops, providing the dominant term (>99%>99\%), e.g. aμQED=116584718.931(0.104)×1011a_\mu^{\rm QED} = 116584718.931(0.104) \times 10^{-11} (Malaescu, 2022).
  • aμEWa_\mu^{\rm EW}: Electroweak loops (W, Z, Higgs), small but precisely determined (153.6(1.0)×1011\simeq 153.6(1.0) \times 10^{-11}) (Malaescu, 2022).
  • aμHVPa_\mu^{\rm HVP}: Hadronic vacuum polarization, a leading source of theory uncertainty (6845(40)×1011\simeq 6845(40) \times 10^{-11}).
  • aμHLbLa_\mu^{\rm HLbL}: Hadronic light-by-light scattering, a subleading but non-negligible contribution (92(18)×1011\simeq 92(18) \times 10^{-11}).

Total SM value (Theory Initiative, 2020): aμSM=116591810(43)×1011a_\mu^{\rm SM} = 116\,591\,810\,(43)\times10^{-11} with error dominated by the hadronic contributions (Pocanic, 1 Dec 2025, Malaescu, 2022).

2. Experimental Techniques and Key Observables

The leading method for measuring aμa_\mu exploits its imprint on the spin precession of muons stored in a uniform magnetic field BB. The anomalous precession frequency: ωa=ωsωc=aμqBmμ\omega_a = \omega_s - \omega_c = a_\mu \frac{qB}{m_\mu} is extracted from the time- and energy-dependent distribution of decay positrons via: N(t)=N0et/τμ[1+Acos(ωat+ϕ)]N(t) = N_0 e^{-t/\tau_\mu} [1 + A \cos(\omega_a t + \phi)] where higher-energy positrons, preferentially emitted along the muon-spin direction, are detected by an array of segmented electromagnetic calorimeters.

The magnetic field is measured by nuclear magnetic resonance (NMR) probes: a precision in-vacuum trolley carrying 17 probes performs spatial mapping every few days, while 378 fixed probes monitor field drift. The average field seen by muons is expressed via the equivalent proton Larmor frequency ωp\omega_p, calibrated by a water-based reference probe (Tewsley-Booth, 2022, Albahri et al., 2021).

The final determination utilizes the ratio: aμ=ωaωpμμpμμ1a_\mu = \frac{\omega_a}{\langle \omega_p \rangle_\mu} \cdot \frac{\mu_p}{\mu_\mu} - 1 with all quantities referenced to fundamental constants and controlled for systematics at the sub-ppm level.

3. Systematics, Corrections, and Error Control

Achieving high precision in aμa_\mu requires rigorous control of systematic uncertainties:

Source Typical magnitude (Run-1/2/3) Key controls
Magnetic field calibration 56–70 ppb Trolley/fixed NMR cross-calibrate
Transient fields (ESQ, kickers) 37–92 ppb Dedicated probes, mapping models
Muon distribution weighting 11–40 ppb Straw trackers, profile modeling
Electric field & pitch effects 40 ppb Momentum selection, quad scans
Calorimeter gain/timing 25–30 ppb Laser calibration, segmentation
Pileup correction 25 ppb Pulse-fit algorithms
Lost muon effects 15 ppb Collimator scans, fit models

Total systematics from all sources are controlled to 100\simeq100 ppb in current data, with further hardware upgrades and analysis refinements targeting 140 ppb for the experiment’s final precision (Sorbara, 12 Mar 2025, Albahri et al., 2021).

Beam-dynamics corrections (electric field, pitch angle, muon loss, phase acceptance) are explicitly quantified via dedicated simulation and data-driven studies, yielding additive corrections at the few-hundred-ppb level (Lucà, 2022).

4. Experimental Results and Statistical Tension

The global average of E821 (BNL) and E989 (Fermilab) data gives: aμexp=116592061(41)×1011(0.35 ppm)a_\mu^{\rm exp} = 116\,592\,061\,(41) \times 10^{-11} \quad (0.35~\text{ppm}) compared to the SM value aμSMa_\mu^{\rm SM} above, yielding: Δaμ=aμexpaμSM=(251±59)×1011\Delta a_\mu = a_\mu^{\rm exp} - a_\mu^{\rm SM} = (251 \pm 59) \times 10^{-11} corresponding to a 4.2σ4.2\sigma excess over the SM (Pocanic, 1 Dec 2025, Keshavarzi et al., 2021, Tewsley-Booth, 2022). Current uncertainties are balanced between statistical and systematic, with each at 29×1011\simeq 29 \times 10^{-11} (Pocanic, 1 Dec 2025).

Recent lattice QCD determinations (BMW 2024) of the HVP contribution are consistent with experiment within 1σ1\sigma, potentially reconciling the anomaly. Data-driven dispersive approaches (based on e+ee^+e^- \to hadrons cross-sections) maintain the 45σ4–5\sigma discrepancy (Pocanic, 1 Dec 2025).

5. Theoretical Interpretation and New Physics Scenarios

The observed tension in Δaμ\Delta a_\mu strongly motivates models of beyond-the-Standard-Model physics that generate loop-level corrections. Principal candidates include:

  • Supersymmetry (SUSY): Smuon–neutralino and sneutrino–chargino loops can naturally generate Δaμ\Delta a_\mu of the observed size for superpartner masses 100800\sim 100–800 GeV, and large tanβ\tan\beta ($40–60$) (Babu et al., 2021, Ahmed et al., 2021, Zhang et al., 2021). Collider searches at HL-LHC and HE-LHC can probe the relevant parameter space.
  • Dark photons and new gauge bosons: Sub-GeV U(1) bosons with millicharge couplings yield loop contributions of the correct order of magnitude (Malaescu, 2022).
  • Leptoquarks, two-Higgs-doublet models, flavor-violating sectors: These offer viable loop shifts but are increasingly constrained by LHC and flavor-observables (Keshavarzi et al., 2021).

Stringent bounds arise from global fits to LHC, flavor physics, and dark-matter relic density. Multi-loop extensions (e.g., Barr-Zee diagrams) and Higgs-sneutrino mixing further provide testable collider signatures (e.g., altered hμμh\to\mu\mu branching ratios) (Zhang et al., 2021).

6. Future Directions: MUonE and Complementary Experiments

With ongoing Run-4 to Run-6 analysis at Fermilab expected to push experimental precision below 0.2 ppm, definitive answers are anticipated in the near term. The CERN MUonE experiment aims to determine the leading-order HVP contribution via muonic Bhabha scattering, expected to reach <0.5%<0.5\% precision in the next several years and provide an independent check on dispersive/lattice inputs (Pocanic, 1 Dec 2025).

Parallel programs:

  • J-PARC E34 (Japan): alternative running-momentum muon ring (Keshavarzi et al., 2021)
  • Precision flavor, EDM, and dark-sector searches: MEG II, Mu3e, Mu2e, NA64μ, M³ (Keshavarzi et al., 2021)
  • High-statistics e+ee^+e^-\to hadrons data from CMD-3, BaBar, KLOE, BESIII, Belle II

The combination of experimental and theoretical advances places the muon anomaly at the crossroads of SM verification and the search for new physics.

7. Summary Table: Key Numbers and Uncertainties

Parameter Value (×1011\times 10^{-11}) Uncertainty (×1011\times 10^{-11})
aμexpa_\mu^{\rm exp} (BNL+FNAL) 116592061 41
aμSMa_\mu^{\rm SM} (Theory Initiative, 2020) 116591810 43
Δaμ\Delta a_\mu 251 59
QED (5-loop) 116584718.931 0.104
EW 153.6 1.0
HVP (data-driven, TIWP) 6845 40
HLbL 92 18
Experimental goal (Fermilab Run-6, projected) <20

Current status: With lattice-QCD-based HVP, the Δaμ\Delta a_\mu anomaly is potentially resolved, but data-driven approaches and low-energy e+ee^+e^-\to hadrons data still support an enduring tension. Continued improvements in both experimental measurement and theoretical calculation of hadronic contributions are critical for a decisive resolution of the muon magnetic anomaly.

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