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1 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) hadrons The Hadronic Contribution to (g – 2) Michel Davier Laboratoire de l’Accélérateur Linéaire, Orsay Tau Workshop 2004 September 14 - 17, 2004, Nara, Japan davier@lal.in2p3.fr
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2 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Magnetic Anomaly Schwinger 1948 QED Prediction: Computed up to 4 th order [Kinoshita et al.] (5 th order estimated) QEDQED QEDHadronicWeakSUSY...... or other new physics ?
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3 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Why Do We Need to Know it so Precisely? BNL (2004) Experimental progress on precision of (g –2) Outperforms theory pre- cision on hadronic contribution
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4 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) The Muonic (g –2) Contributions to the Standard Model (SM) Prediction: Source (a)(a) Reference QED ~ 0.3 10 –10 [Schwinger ’48 & others] Hadrons ~ (15 4) 10 –10 [Eidelman-Jegerlehner ’95 & others] Z, W exchange ~ 0.4 10 –10 [Czarnecki et al. ‘95 & others] The Situation 1995 ”Dispersion relation“ hadhad had ... Dominant uncertainty from lowest order hadronic piece. Cannot be calculated from QCD (“first principles”) – but: we can use experiment (!)
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5 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Hadronic Vacuum Polarization Define: photon vacuum polarization function (q 2 ) Ward identities: only vacuum polarization modifies electron charge with : Leptonic lep (s) calculable in QED. However, quark loops are modified by long-distance hadronic physics, cannot (yet) be calculated within QCD (!) Way out: Optical Theorem (unitarity)... Im[ ] | hadrons | 2... and the subtracted dispersion relation of (q 2 ) (analyticity)... and equivalently for a [had]
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6 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Improved Determination of the Hadronic Contribution to (g –2) and (M Z )2 Energy [GeV]Input 1995Input after 1998 2m - 1.8Data Data (e + e – & ) + QCD 1.8 – J/ DataQCD J/ - DataData + QCD - 40 DataQCD 40 - QCD Eidelman-Jegerlehner’95, Z.Phys. C67 (1995) 585 Improvement in 4 Steps: Inclusion of precise data using SU(2) (CVC) Extended use of (dominantly) perturbative QCD Theoretical constraints from QCD sum rules and use of Adler function Alemany-Davier-Höcker’97, Narison’01, Trocóniz-Ynduráin’01, + later works Martin-Zeppenfeld’95, Davier-Höcker’97, Kühn-Steinhauser’98, Erler’98, + others Groote-Körner-Schilcher-Nasrallah’98, Davier-Höcker’98, Martin-Outhwaite- Ryskin’00, Cvetič-Lee-Schmidt’01, Jegerlehner et al’00, Dorokhov’04 + others Since then: Improved determi- nation of the dispersion integral: better data extended use of QCD Better data for the e + e – + – cross section CMD-2’02, KLOE’04
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7 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) The Role of Data through CVC – SU(2) hadrons W e+e+ e –e – CVC: I =1 & V W: I =1 & V,A : I =0,1 & V Hadronic physics factorizes in Spectral Functions : Isospin symmetry connects I=1 e + e – cross section to vector spectral functions: branching fractions mass spectrum kinematic factor (PS) fundamental ingredient relating long distance (resonances) to short distance description (QCD)
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8 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) SU(2) Breaking Corrections for SU(2) breaking applied to data for dominant – + contrib.: Electroweak radiative corrections: dominant contribution from short distance correction S EW to effective 4-fermion coupling (1 + 3 (m )/4 )(1+2 Q )log(M Z /m ) subleading corrections calculated and small long distance radiative correction G EM (s) calculated [ add FSR to the bare cross section in order to obtain – + ( ) ] Charged/neutral mass splitting: m – m 0 leads to phase space (cross sec.) and width (FF) corrections - mixing (EM – + decay) corrected using FF model intrinsic m – m 0 and – 0 [not corrected !] Electromagnetic decays, like: , , , l + l – Quark mass difference m u m d generating “second class currents” (negligible) Electromagnetism does not respect isospin and hence we have to consider isospin breaking when dealing with an experimental precision of 0.5% Cirigliano-Ecker-Neufeld’ 02 Marciano-Sirlin’ 88 Braaten-Li’ 90 Alemany-Davier-Höcker’ 97, Czyż-Kühn’ 01
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9 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Mass Dependence of SU(2) Breaking Multiplicative SU(2) corrections applied to – – 0 spectral function: Only 3 and EW short-distance corrections applied to 4 spectral functions
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10 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) e + e – Radiative Corrections Multiple radiative corrections are applied on measured e + e – cross sections Situation often unclear: whether or not and if - which corrections were applied Vacuum polarization (VP) in the photon propagator: leptonic VP in general corrected for hadronic VP correction not applied, but for CMD-2 (in principle: iterative proc.) Final state radiation (FSR) [we need e + e – hadrons ( ) in disper-sion integral] usually, experiments obtain bare cross section so that FSR has to be added “by hand”; done for CMD-2, (supposedly) not done for others Initial state radiation (ISR) corrected by experiments
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11 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) 2002/2003 Analyses of a had Motivation for new work: New high precision e + e – results (0.6% sys. error) around from CMD-2 (Novosibirsk) New results from ALEPH using full LEP1 statistics New R results from BES between 2 and 5 GeV New theoretical analysis of SU(2) breaking Cirigliano-Ecker-Neufeld JHEP 0208 (2002) 002 ALEPH CONF 2002-19 CMD-2 PL B527, 161 (2002) Outline of the 2002/2003 analyses: Include all new Novisibirsk (CMD-2, SND) and ALEPH data Apply (revisited) SU(2)-breaking corrections to data Identify application/non-application of radiative corrections Recompute all exclusive, inclusive and QCD contributions to dispersion integral; revisit threshold contribution and resonances Results, comparisons, discussions... Davier-Eidelman-Höcker-Zhang Eur.Phys.J. C27 (2003) 497; C31 (2003) 503 BES PRL 84 594 (2000); PRL 88, 101802 (2002) Hagiwara-Martin-Nomura-Teubner, Phys.Rev. D69 (2004) 093003 (no data) Jegerlehner, hep-ph/0312372 (no data)
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12 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Comparing e + e – + – and – 0 Remarkable agreement But: not good enough...... Correct data for missing - mixing (taken from BW fit) and all other SU(2)-breaking sources
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13 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) The Problem zoom Relative difference between and e + e – data:
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14 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) – – 0 : Comparing ALEPH, CLEO, OPAL Good agreement observed between ALEPH and CLEO ALEPH more precise at low s CLEO better at high s Shape comparison only. SFs normalized to WA branching fraction (dominated by ALEPH).
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15 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Testing CVC Infer branching fractions from e + e – data: Difference: BR[ ] – BR[e + e – (CVC) ]: Mode ( – e + e – ) „Sigma“ – – 0 + 0.94 ± 0.322.9 – – 3 0 – 0.08 ± 0.110.7 – 2 – + 0 + 0.91 ± 0.253.6 leaving out CMD-2 : B 0 = (23.69 0.68) % (7.4 2.9) % relative discrepancy!
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16 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) New Precise e + e – + – Data from KLOE Using the „Radiative Return“... Overall: agreement with CMD-2 Some discrepancy on peak and above...
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17 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) The Problem (revisited) Relative difference between and e + e – data: zoom No correction for ± – 0 mass (~ 2.3 ± 0.8 MeV) and width (~ 3 MeV) splitting applied Jegerlehner, hep-ph/0312372 Davier, hep-ex/0312064
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18 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Evaluating the Dispersion Integral Better agreement between exclusive and inclusive ( 2) data than in 1997- 1998 analyses Agreement bet- ween Data (BES) and pQCD (within correlated systematic errors) use QCD use data use QCD
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19 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Results: the Compilation (including KLOE) Contributions to a had [in 10 –10 ] from the different energy domains: ModesEnergy [GeV] e+e –e+e – Low s expansion2m – 0.558.0 ± 1.7 ± 1.2 rad 56.0 ± 1.6 ± 0.3 SU(2) [ + – (DEHZ’03) ] 2m – 1.8[ 450.2 ± 4.9 ± 1.6 rad ]464.0 ± 3.0 ± 2.3 SU(2) + – (incl. KLOE) 2m – 1.8448.3 ± 4.1 ± 1.6 rad – + – 20 + – 20 2m – 1.816.8 ± 1.3 ± 0.2 rad 21.4 ± 1.3 ± 0.6 SU(2) 2 + 2 – 2m – 1.814.2 ± 0.9 ± 0.2 rad 12.3 ± 1.0 ± 0.4 SU(2) (782) 0.3 – 0.8138.0 ± 1.0 ± 0.3 rad – (1020) 1.0 – 1.05535.7 ± 0.8 ± 0.2 rad – Other exclusive2m – 1.824.0 ± 1.5 ± 0.3 rad – J / , (2S) 3.08 – 3.117.4 ± 0.4 ± 0.0 rad – R [QCD]1.8 – 3.733.9 ± 0.5 ± 0.0 rad – R [data]3.7 – 5.07.2 ± 0.3 ± 0.0 rad – R [QCD] 5.0 – 9.9 ± 0.2 theo – Sum (incl. KLOE) 2m – 693.4 ± 5.3 ± 3.5 rad 711.0 ± 5.0 ± 0.8 rad ± 2.8 SU(2)
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20 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Discussion The problem of the + – contribution : Experimental situation: new, precise KLOE results in approximate agreement with latest CMD-2 data data without m ( ) and ( ) corr. in strong disagreement with both data sets ALEPH, CLEO and OPAL spectral functions in good agreement within errors Concerning the remaining line shape discrepancy (0.7- 0.9 GeV 2 ): SU(2) corrections: basic contributions identified and stable since long; overall correction applied to is (– 2.2 ± 0.5) %, dominated by uncontroversial short distance piece; additional long-distance corrections found to be small lineshape corrections cannot account for the difference above 0.7 GeV 2 The fair agreement between KLOE and CMD-2 invalidates the use of data until a better understanding of the discrepancies is achieved
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21 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Preliminary Results a had [ee ]= (693.4 ± 5.3 ± 3.5) 10 –10 a [ee ]= (11 659 182.8 ± 6.3 had ± 3.5 LBL ± 0.3 QED+EW ) 10 –10 Hadronic contribution from higher order : a had [( / ) 3 ] = – (10.0 ± 0.6) 10 –10 Hadronic contribution from LBL scattering: a had [ LBL ] = + (12.0 ± 3.5) 10 –10 inclu- ding: a [exp ] – a [SM ]= (25.2 ± 9.2) 10 –10 2.7 „standard deviations“ Observed Difference with Experiment: BNL E821 (2004): a exp = (11 659 208.0 5.8) 10 10 Knecht-Nyffeler, Phys.Rev.Lett. 88 (2002) 071802 Melnikov-Vainshtein, hep-ph/0312226.0 not yet published preliminary Davier-Marciano, to appear Ann. Rev. Nucl. Part. Sc.
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22 Tau Workshop, Nara, Sept 14-17, 2004M. Davier – Hadronic Contribution to (g – 2) Conclusions and Perspectives Hadronic vacuum polarization is dominant systematics for SM prediction of the muon g – 2 New data from KLOE in fair agreement with CMD-2 with a (mostly) independent technique Discrepancy with data (ALEPH & CLEO & OPAL) confirmed Until / e + e – puzzle is solved, use only e + e – data in dispersion integral We find that the SM prediction differs by 2.7 [e + e – ] from experiment (BNL 2004) Future experimental input expected from: New CMD-2 results forthcoming, especially at low and large + – masses BABAR ISR: + – SF over full mass range, multihadron channels (2 + 2 – and + – 0 already available)
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