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Anomalous Muon Magnetic Moment

Updated 30 January 2026
  • The anomalous magnetic moment of the muon is a high-precision observable that reveals quantum corrections to Dirac's g=2, integrating QED, electroweak, and hadronic effects.
  • Experimental techniques using muon spin precession combined with lattice QCD and dispersion methods enable precise measurement of a_mu at the sub-ppm level.
  • Recent improvements have reduced uncertainties to under 130 ppb, resolving earlier discrepancies and constraining new physics scenarios.

The anomalous magnetic moment of the muon, aμ(gμ2)/2a_\mu \equiv (g_\mu - 2)/2, is a precision observable at the interface of quantum field theory, flavor physics, and searches for physics beyond the Standard Model (SM). In the Dirac theory, g=2g=2 for pointlike spin-12\frac{1}{2} fermions; deviations arise from quantum corrections. The muon anomaly is uniquely sensitive to high-scale virtual effects since the SM contributions from QED, electroweak, and hadronic sectors enter at the tens of parts-per-billion level, while NNLO and beyond are accessible via modern experiment and theory. Persistent experimental–theoretical tensions have motivated extensive upgrades to both measurement campaigns and theoretical predictions. The status and future of aμa_\mu research reflect advances in both sub-ppm experimental control and the non-perturbative QCD sector.

1. Theoretical Structure and Calculation of aμa_\mu

The SM prediction for aμa_\mu is conventionally decomposed into QED, electroweak, and two dominant hadronic terms:

aμSM=aμQED+aμEW+aμHVP+aμHLbL.a_\mu^{\text{SM}} = a_\mu^{\text{QED}} + a_\mu^{\text{EW}} + a_\mu^{\text{HVP}} + a_\mu^{\text{HLbL}}.

  • QED: The dominant contribution, calculated up to five-loop order, yields aμQED=116584718.09(0.16)×1011a_\mu^{\text{QED}} = 116\,584\,718.09(0.16) \times 10^{-11}, with negligible residual uncertainty (0.001\lesssim 0.001 ppm) (Gray, 2010, Hertzog et al., 18 Dec 2025).
  • Electroweak: One- and two-loop corrections, dominated by W,ZW, Z, and HH exchange, add aμEW=154(2)×1011a_\mu^{\text{EW}}=154(2) \times 10^{-11} (Gray, 2010, Hertzog et al., 18 Dec 2025).
  • Hadronic Vacuum Polarization (HVP): Evaluated via a dispersion integral over e+ee^+ e^- \to hadrons data, the leading-order HVP is aμHVP=6857(41)×1011a_\mu^{\text{HVP}} = 6857(41) \times 10^{-11} (in 2010), with modern lattice QCD evaluations now playing a central role (Gray, 2010, Hertzog et al., 18 Dec 2025).
  • Hadronic Light-by-Light (HLbL): The HLbL contribution, the most model-dependent term, is estimated as aμHLbL=105(26)×1011a_\mu^{\text{HLbL}} = 105(26) \times 10^{-11} (Gray, 2010, Hertzog et al., 18 Dec 2025).

The sum yields a current theory value aμSM=(116591834±49)×1011a_\mu^{\text{SM}} = (116\,591\,834 \pm 49)\times 10^{-11} (2010 evaluation), recently updated to aμSM=116592022(63)×1011a_\mu^{\text{SM}} = 116\,592\,022(63)\times 10^{-11} (2025 White Paper with lattice HVP) (Hertzog et al., 18 Dec 2025).

2. Experimental Determination: Principle and Methodology

Measurement of aμa_\mu exploits the spin precession of relativistic polarized muons stored in a highly uniform magnetic field BB, with focusing provided by electric quadrupoles. The anomalous precession frequency

ωa=qm[aμB(aμ1γ21)β×E]\vec{\omega}_a = -\frac{q}{m}\left[a_\mu \vec{B} - \left(a_\mu - \frac{1}{\gamma^2-1}\right)\vec{\beta} \times \vec{E}\right]

is isolated by setting the muon momentum to the "magic" value (pmagic3.094p_{\text{magic}} \simeq 3.094 GeV/cc, γmagic29.3\gamma_{\text{magic}} \simeq 29.3), nullifying electric field corrections at leading order (Gray, 2015, Gray, 2010).

The anomaly is determined from the frequency ratio R=ωa/ωpR = \omega_a / \omega_p, with ωp\omega_p measured via nuclear magnetic resonance (NMR) of protons in water at well-calibrated temperatures. The final result is then

aμ=RλR,λ=μμ/μp.a_\mu = \frac{R}{\lambda - R}, \qquad \lambda = \mu_\mu/\mu_p.

Comprehensive corrections for beam dynamics (electric field, pitch, phase-acceptance, differential decay, and muon loss) and systematic effects (magnetic field mapping, calibration, transients) are applied to reach ppb-level accuracy (Aguillard et al., 2024, Collaboration et al., 3 Jun 2025).

3. Hadronic Contributions: Dispersion and Lattice Approaches

3.1. Dispersion Relations

The leading-order HVP is given by a dispersion integral:

aμHVP,LO=(α23π2)sthrdsK(s)sRhad(s),a_\mu^{\text{HVP},\mathrm{LO}} = \left( \frac{\alpha^2}{3 \pi^2}\right) \int_{s_{\rm thr}}^\infty ds \, \frac{K(s)}{s} R_{\mathrm{had}}(s),

where K(s)K(s) is a known QED kernel and Rhad(s)=σ(e+ehadrons)/σ(e+eμ+μ)R_{\mathrm{had}}(s) = \sigma(e^+ e^- \to \mathrm{hadrons}) / \sigma(e^+ e^- \to \mu^+ \mu^-) (Hoecker, 2010). The π+π\pi^+\pi^- channel below 1 GeV dominates (\sim70%), with systematic cross-validation using τ\tau decay data and energy scans (Hertzog et al., 18 Dec 2025).

3.2. Lattice QCD

Lattice QCD measures the hadronic two-point function with physical-mass ensembles, using improved Wilson, domain-wall, or staggered fermions, and systematic control of volume, discretization, and isospin-breaking effects (Morte et al., 2011, Aubin et al., 2013, Marinkovic, 2017). The lattice result for the leading HVP is now aμHVP,LO=7132(61)×1011a_\mu^{\text{HVP,LO}} = 7132(61) \times 10^{-11}, in line with data-driven evaluations but with slightly higher uncertainty. Progress in noise reduction, continuum and infinite-volume extrapolations, and disconnected diagrams has narrowed the theory error to 0.5%\sim 0.5\%. The hadronic light-by-light piece is now also directly computed with lattice and dispersive approaches, converging to aμHLbL=115.5(9.9)×1011a_\mu^{\mathrm{HLbL}} = 115.5(9.9)\times 10^{-11} (Hertzog et al., 18 Dec 2025, Pauk et al., 2014).

4. Precision Measurements and the Evolution of the aμa_\mu Puzzle

A succession of experiments has refined aμexpa_\mu^{\rm exp}:

  • BNL E821: aμexp=(116592089±63)×1011a_\mu^{\rm exp} = (116\,592\,089 \pm 63)\times 10^{-11} (0.54 ppm), revealing a persistent 3.2σ\sigma excess over the SM (Gray, 2010).
  • Fermilab Muon g–2 (E989 Runs 1–6): Recent measurements yield aμFNAL=116592061(127)×1011a_\mu^{\rm FNAL} = 116\,592\,061(127)\times 10^{-11} (127 ppb), producing an experimental world average aμexp=116592061(124)×1011a_\mu^{\rm exp} = 116\,592\,061(124)\times 10^{-11} (124 ppb) (Collaboration et al., 3 Jun 2025).
  • The 2025 SM theory value, using lattice HVP, is aμSM=116591997(42)×1011a_\mu^{\rm SM} = 116\,591\,997(42)\times 10^{-11}, so Δaμ=aμexpaμSM=(64±131)×1011\Delta a_\mu = a_\mu^{\rm exp} - a_\mu^{\rm SM} = (64 \pm 131)\times 10^{-11}, a 0.5σ0.5\,\sigma effect—no significant deviation currently remains (Collaboration et al., 3 Jun 2025, Hertzog et al., 18 Dec 2025).

This reverses earlier claims of 3σ3\sigma4σ4\sigma deviations, arising from earlier, lower SM predictions (with data-driven HVP) (Aguillard et al., 2024, Tewsley-Booth, 2022).

5. New Physics Interpretations and Model Constraints

Explanatory scenarios for any deviation Δaμ\Delta a_\mu include:

  • Supersymmetry (MSSM, μνμνSSM): One-loop diagrams with EW-scale charginos/sleptons yield δaμSUSY130×1011tanβ(100GeV/Λ)\delta a_\mu^{\rm SUSY} \sim 130 \times 10^{-11} \tan\beta (100\,\mathrm{GeV}/\Lambda), allowing natural explanations for Δaμ\Delta a_\mu at the 10910^{-9} level for light EW sparticles and large tanβ\tan\beta (Gray, 2010, Ahmed et al., 2021, Zhang et al., 2021). Current limits require any SUSY contributions to respect Δaμ109|\Delta a_\mu| \ll 10^{-9} given the new world average (Collaboration et al., 3 Jun 2025).
  • Extra Dimensions: Warped scenarios like the minimal RS model yield Δaμ8.8×1011(1TeV/T)2\Delta a_\mu \simeq 8.8 \times 10^{-11} (1\,\text{TeV}/T)^2, insufficient to account for the earlier discrepancies unless KK scales are already excluded by other observables (Beneke et al., 2012).
  • Lorentz Violation (SME): Constraints on SME parameters such as [cTT+0.35(cXX+cYY)+0.28cZZ]<8.5×1011[c_{TT} + 0.35(c_{XX} + c_{YY}) + 0.28c_{ZZ}] < 8.5 \times 10^{-11} emerge from absence of sidereal or energy-dependent signals (Aghababaei et al., 2017).
  • Noncommutative QED: Bounds on the noncommutativity scale θμν(43 TeV)2\theta^{\mu\nu} \sim (43~\text{TeV})^{-2} are set by requiring δaμNC\delta a_\mu^\text{NC} not to exceed the experimental limit (Rezaei et al., 2024).
  • Alternative UV-finite models: The BY theory and similar cannot resolve any previous aμa_\mu anomaly, indicating that only significant new low-scale dynamics or hadronic effects could have done so (Palle, 2016).

6. Experimental and Theoretical Innovations

6.1 Experimental Advances

Key technical upgrades at Fermilab E989 include:

  • Enhanced field uniformity by refined shimming and a dense NMR probe array.
  • Open-ended inflector design and elongated pion-decay channel to increase decay statistics by a factor of 20 (Gray, 2010, Gray, 2015).
  • Segmented tungsten/scintillating-fiber calorimeters and high-speed waveform digitizers for pileup control.
  • Active betatron-oscillation suppression and frequent in situ magnetic-field mapping.

6.2 Theoretical Developments

  • Refined e+ee^+ e^- \to hadrons datasets (BaBar ISR, CMD-3, KLOE) and improved isospin-breaking corrections have stabilized the HVP input, though lattice and dispersive results still show tension (Gray, 2010, Hertzog et al., 18 Dec 2025).
  • Dispersive methods for HLbL have fully connected the calculation to measurable amplitudes, reducing reliance on model extrapolation (Pauk et al., 2014).

The combined experimental and theory push has allowed precise closure of the earlier SM–experiment gap.

7. Outlook and Future Prospects

Surpassing the 124 ppb precision benchmark requires both experimental and theoretical innovation:

  • MUonE, J-PARC E34, and potential next-generation upgrades at FNAL may pursue sensitivity at the 40–50 ppb level (Hertzog et al., 18 Dec 2025).
  • Theory error budgets are dominated by the HVP (61 in 101110^{-11} units) and HLbL (10), motivating ongoing advances in precision lattice QCD calculations, scale setting, and data-driven radiative correction schemes.
  • Any future detection of a statistically significant deviation in aμa_\mu will demand reconciliation among e+ee^+e^-, τ\tau, lattice, and scattering-based methodologies, tightly constraining or discovering new TeV-scale particles or interactions.

Table: Evolution of aμa_\mu Measurements and Uncertainties

Measurement aμa_\mu [101110^{-11}] Uncertainty [ppb] Reference
BNL E821 (2004) 116592089(63)116\,592\,089(63) 540 (Gray, 2010)
FNAL E989 (2021) 116592040(54)116\,592\,040(54) 460 (Tewsley-Booth, 2022)
FNAL E989 (2024) 116592055(24)116\,592\,055(24) 200 (Aguillard et al., 2024)
FNAL E989 (2025) 116592061(127)116\,592\,061(127) 127 (Collaboration et al., 3 Jun 2025)
World Avg. (2025) 116592061(124)116\,592\,061(124) 124 (Collaboration et al., 3 Jun 2025)
SM Prediction (2025, lattice HVP) 116591997(42)116\,591\,997(42) 36 (Hertzog et al., 18 Dec 2025)

Current values reveal no significant tension: Δaμ=(64±131)×1011\Delta a_\mu = (64 \pm 131) \times 10^{-11} (0.5σ0.5\sigma).


The anomalous magnetic moment of the muon exemplifies the synergy between high-precision experiment and advanced quantum field-theoretic computation. With experimental uncertainty now below $130$ ppb and lattice-QCD-based SM predictions converging to comparable accuracy, aμa_\mu stands as a critical probe of virtual physics up to the multi-TeV scale, setting profound constraints on extensions to the Standard Model. The resolution of prior “g–2” anomalies now imposes stringent criteria on any candidate new physics models. Continued reductive progress in theory error and forthcoming measurements will further solidify aμa_\mu as a flagship observable of the precision frontier in particle physics.

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