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Theoretical Status of the Muon G 2 − Andreas Nyffeler Theoretical status of the muon g 2 − Andreas Nyffeler PRISMA Cluster of Excellence, Institut f¨urKernphysik, Helmholtz-Institut Mainz Johannes Gutenberg Universit¨atMainz, Germany [email protected] Helmholtz Programme Matter and the Universe (MU) HIM, Mainz, 12-13 December 2016 Outline • Basics of the anomalous magnetic moment • Muon g 2: QED, weak interactions, hadronic contributions − • Hadronic vacuum polarization (HVP) • Hadronic light-by-light scattering (HLbL) • New Physics contributions to the muon g 2 − • Conclusions and Outlook Basics of the anomalous magnetic moment Electrostatic properties of charged particles: Charge Q, Magnetic moment ~µ, Electric dipole moment ~d For a spin 1/2 particle: e 1 ~µ = g ~s; g = 2(1 + a); a = (g 2) : anomalous magnetic moment 2m | {z } 2 − Dirac Long interplay between experiment and theory: structure of fundamental forces In Quantum Field Theory (with C,P invariance): γ(k) 2 3 µν 0 µ 2 iσ kν 2 =( ie)¯u(p ) 6γ F (k ) + F (k )7 u(p) 1 2 4 5 − 2m | {z } | {z } p p’ Dirac Pauli F1(0) = 1 and F2(0) = a 2 ae : Test of QED. Most precise determination of α = e =4π. aµ: Less precisely measured than ae , but all sectors of Standard Model (SM), i.e. QED, Weak and QCD (hadronic), contribute significantly. Sensitive to possible contributions from New Physics. Often (but not always !): 2 2 m` mµ a` 43000 more sensitive than ae [exp. precision ! factor 19] ∼ mNP ) me ∼ Some theoretical comments • Anomalous magnetic moment is finite and calculable Corresponds to effective interaction Lagrangian of mass dimension 5: AMM e`a` ¯ µν eff = (x)σ (x)Fµν (x) L − 4m` (mass dimension 6 in SM with SU(2)L U(1)Y invariant operator) × a` = F2(0) can be calculated unambiguously in renormalizable QFT, since there is no counterterm to absorb potential ultraviolet divergence. • Anomalous magnetic moments are dimensionless To lowest order in perturbation theory in quantum electrodynamics (QED): α = a = a = [Schwinger '48] e µ 2π • Loops with different masses ae = aµ - Internal large masses decouple) (not6 always !): " !# 1 m 2 m4 m α 2 = e + O e ln µ 4 45 mµ mµ me π - Internal small masses give rise to large log's of mass ratios: 1 m 25 m α 2 = ln µ − + O e 3 me 36 mµ π Milestones in measurements of the muon g 2 − Authors Lab Muon Anomaly Garwin et al. '60 CERN 0.001 13(14) Charpak et al. '61 CERN 0.001 145(22) Charpak et al. '62 CERN 0.001 162(5) Farley et al. '66 CERN 0.001 165(3) Bailey et al. '68 CERN 0.001 166 16(31) Bailey et al. '79 CERN 0.001 165 923 0(84) Brown et al. '00 BNL 0.001 165 919 1(59) (µ+) Brown et al. '01 BNL 0.001 165 920 2(14)(6) (µ+) Bennett et al. '02 BNL 0.001 165 920 4(7)(5) (µ+) Bennett et al. '04 BNL 0.001 165 921 4(8)(3) (µ−) World average experimental value (dominated by g 2 Collaboration at BNL, − Bennett et al. '06 + CODATA 2008 value for λ = µµ/µp): aexp = (116 592 089 63) 10−11 [0:5ppm] µ ± × −11 Goal of new planned g 2 experiments: δaµ = 16 10 Fermilab E989: partly recycled− from BNL: moved ring× magnet ! (http://muon-g-2.fnal.gov/bigmove/ ) First beam in 2017, should reach this precision by 2020. J-PARC E34: completely new concept with low-energy −11 muons, not magic γ. Aims in Phase 1 for about δaµ = 45 10 . × Theory needs to match this precision ! Muon g 2: Theory − In Standard Model: SM QED weak had aµ = aµ + aµ + aµ In contrast to ae , here the contributions from weak and strong interactions 2 (hadrons) are relevant, since aµ (mµ=M) . ∼ QED contributions • Diagrams with internal electron loops are enhanced. • At 2-loops: vacuum polarization from electron loops enhanced by QED short-distance logarithm • At 3-loops: light-by-light scattering from electron loops enhanced by QED infrared logarithm [Aldins et al. '69, '70; Laporta, Remiddi '93] e 3 3 (3) 2 2 mµ α α aµ = π ln + ::: = 20:947 ::: + ... lbyl 3 me π π µ • Loops with tau's suppressed (decoupling) QED result up to 5 loops Include contributions from all leptons (Schwinger '48; . ; Aoyama et al. '12): 2 QED α α aµ =0 :5 + 0:765 857 425 (17) × π |{z} × π mµ=me,τ α 3 α 4 + 24:050 509 96 (32) + 130:8796 (63) |{z} × π |{z} × π mµ=me,τ num. int. α 5 + 753:29 (1:04) | {z } × π num. int. = 116 584 718:853 (9) (19) (7) (29) [36] 10−11 |{z} |{z} |{z} |{z} × mµ=me,τ c4 c5 α(ae ) • Up to 3-loop analytically known (Laporta, Remiddi '93). • 4-loop: analytical results for electron and tau-loops (asymptotic expansions) by Steinhauser et al. '15 + '16. • Earlier evaluation of 5-loop contribution yielded c5 = 662(20) (Kinoshita, Nio '06, numerical evaluation of 2958 diagrams, known or likely to be enhanced). New value is 4.5σ from this leading log estimate and 20 times more precise. • Aoyama et al. '12: What about the 6-loop term ? Leading contribution from light-by-light scattering with electron loop and insertions of vacuum-polarization QED −11 loops of electrons into each photon line ) aµ (6-loops) ∼ 0:1 × 10 Contributions from weak interaction Numbers from recent reanalysis by Gnendiger et al. '13. 1-loop contributions [Jackiw, Weinberg '72; . ]: a) b) c) γ W W µ νµ p Z H 2 2Gµm 10 aweak, (1)(W ) = µ + O(m2 =M2 ) = 388:70 × 10−11 µ 16π2 3 µ W p 2 2 2 2Gµm (−1 + 4s ) − 5 aweak, (1)(Z) = µ W + O(m2 =M2 ) = −193:89 × 10−11 µ 16π2 3 µ Z weak, (1) −14 Contribution from Higgs negligible: aµ (H) ≤ 5 × 10 for mH = 126 GeV. aweak, (1) = (194:80 0:01) 10−11 µ ± × 2-loop contributions (1678 diagrams) [Czarnecki et al. '95, '96; . ]: weak, (2) −11 2 α MZ aµ = ( 41:2 1:0) 10 ; large since GF mµ ln − ± × ∼ π mµ Total weak contribution: aweak = (153:6 1:0) 10−11 µ ± × Under control ! With knowledge of MH = 125:6 ± 1:5 GeV, uncertainty now mostly hadronic ±1:0 × 10−11 (Peris et al. '95; Knecht et al. '02; Czarnecki et al. '03, '06). 3-loop effects via RG: ±0:20 × 10−11 (Degrassi, Giudice '98; Czarnecki et al. '03). Hadronic contributions to the muon g 2 − Largest source of uncertainty in theoretical prediction of aµ ! Different types of contributions: Z γ (a) (b) (c) Light quark loop not well defined Hadronic \blob" ! (a) Hadronic vacuum polarization (HVP) (α2); (α3); (α4) O O O (b) Hadronic light-by-light scattering (HLbL) (α3); (α4) O O 2 (c) 2-loop electroweak contributions (αGF m ) O µ 2-Loop EW e u,d Small hadronic uncertainty from triangle diagrams. Anomaly cancellation within each generation ! γ Z γ Z µ µ Cannot separate leptons and quarks ! Hadronic vacuum polarization HVP aµ = µ µ Optical theorem (from unitarity; conservation of probability) for hadronic contribution ! dispersion relation: 2 Im σ(e+e γ hadrons) ∼ ∼ − → ∗ → 1 α 2 Z 1 ds σ(e+e− γ∗ hadrons) aHVP = K(s) R(s); R(s)= ! ! µ 3 π s σ(e+e− γ∗ µ+µ−) 0 ! ! [Bouchiat, Michel '61; Durand '62; Brodsky, de Rafael '68; Gourdin, de Rafael '69] K(s) slowly varying, positive function ) aHVP positive. Data for hadronic cross section p µ σ at low center-of-mass energies s important due to factor1 =s: ∼ 70% from ππ [ρ(770)] channel, ∼ 90% from energy region below 1.8 GeV. Other method instead of energy scan: Radiative return e− γ (initial state radiation) at colliders with fixed center-of- Hadrons mass energy (DAΦNE, B-Factories, BEPC) [Binner et al. γ '99; Czy_zet al. '00-'03] e+ Measured hadronic cross-section 2 Pion form factor Fπ(E) (ππ-channel) j j 3 2 2 1 4mπ 2 R(s) = 1 − jFπ(s)j 4 s 2 2 (4mπ < s < 9mπ) R-ratio: Jegerlehner, AN '09 New results on e+e− π+π− from BESIII ! Ablikim et al. (BESIII Collaboration) '16 (Analysis by group at Mainz (Denig et al.)) 45 BESIII fit 40 BESIII 35 30 Fit of BESIII data with parametrization of 2 | π |F 25 pion form factor by Gounaris-Sakurai. Only 20 statistical errors shown. 15 10 0.6 0.65 0.7 0.75 0.8 0.85 0.9 s' [GeV] 0.15 0.15 BESIII fit BESIII fit 0.1 BaBar 0.1 KLOE 08 BESIII KLOE 10 KLOE 12 0.05 0.05 0 0 / BESIII fit - 1 / BESIII fit - 1 2 2 | | -0.05π -0.05π |F |F -0.1 -0.1 -0.15 -0.15 0.6 0.65 0.7 0.75 0.8 0.85 0.9 0.6 0.65 0.7 0.75 0.8 0.85 0.9 s' [GeV] s' [GeV] BaBar data higher than BESIII below Good agreement with KLOE 08 and ρ-mass, better agreement above. KLOE 12 up to mass range of ρ − ! Statistical and systematic errors included in interference, but disagreement with all data points. Width of BESIII fit band shows three data sets at higher energy. systematic uncertainty only. New results on e+e− π+π− from BESIII (continued) ! HVP Comparison of value for aµ (600 900 MeV) from the three experiments using radiative return method (initial− state radiation): KLOE 08 368.1 ± 0.4 ± 2.3 ± 2.2 BaBar 09 376.7 ± 2.0 ± 1.9 KLOE 10 365.3 ± 0.9 ± 2.3 ± 2.2 KLOE 12 366.7 ± 1.2 ± 2.4 ± 0.8 BESIII 368.2 ± 2.5 ± 3.3 360 365 370 375 380 385 390 395 ππ,LO -10 aµ (600 - 900 MeV) [10 ] Results from BESIII confirm KLOE, disagree with BaBar at level of 1 2 σ (at HVP − least after integration in dispersion integral to get aµ ).
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