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Inclusive semileptonic B decays: experimental Elisabetta Barberio University of Melbourne FPCP: Vancouver April 2006
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April 2006 E. Barberio 2 Standard Model Consistency Tests V ub and V cb provide a test of CP violation in the Standard Model comparing the measurements on the ( , ) plane The width of the green ring need to be reduced to match sin2 and other measurements The error on the ring width is dominated by V ub Goal: Accurate determination of |V ub |
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April 2006 E. Barberio 3 Semileptonic B decays tree level, short distance: decay properties depend directly on |V cb |, |V ub |,m b perturbative regime ( s n ) V cb, V ub u + long distance:,u But quarks are bound by soft gluons: non-perturbative ( QCD ) long distance interactions of b quark with light quark
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April 2006 E. Barberio 4 Inclusive semileptonic decays Short distance is calculable Long distance leading order and short distance contribution are cleanly separated and probability to hadronnize is 1 To compare Operator Product Expansion predictions with experiments: integration over neutrino and lepton phase space provides smearing over the invariant hadronic mass of the final state Many theorists love inclusive semileptonic decays
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April 2006 E. Barberio 5 Inclusive semileptonic decays V ub : 7.5% precision shared between experimental and theoretical errors small rate and large b cl background space cuts to remove b cl background which introduce O(1) dependence on non-preturbative b-quark distribution function V cb vs V ub V cb : most accurate determination from the inclusive decays 2% precision limited by theory error precise Heavy Quarks parameters, tests of OPE
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April 2006 E. Barberio 6 V cb from inclusive semileptonic decays sl described by Heavy Quark Expansion in (1/m b ) n and s k The expansion depend on m b definition: non-perturbative terms are expansion dependent exp. |V cb |<1% non perturbative parameters need to be measured Theory error was dominated by 1/m b 3 terms and above
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April 2006 E. Barberio 7 X n are relate to non-perturbative parameters Bc moments in semileptonic decays higher moments are sensitive to 1/m b 3 terms reduce theory error on V cb and HQ parameters moments evaluated on the full lepton spectrum or part of it: p > p min in the B rest frame
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April 2006 E. Barberio 8 Difficulty to go from measured shape to true shape: e.g. QED corrections, accessible phase space, resolution, background rate shape |V cb | m c, 2 G, m b, 2 rate |V cb | shape Inclusive SL decays
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April 2006 E. Barberio 9 Most recent measurements from Belle moments in semileptonic decays P l min =0.7 GeV P l min =0.4 GeV E : lepton energy spectrum in B X c ( BaBar Belle CLEO Delphi ) M X 2 : hadronic mass spectrum in B X c ( BaBar CDF CLEO Delphi ) P * l (GeV) m x (GeV) P * l (GeV) from the moments of these distributions we get V cb and HQ parameters
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April 2006 E. Barberio 10 Parameters Extraction BABAR: up to 1/m b 3 : fit ~90 measurement to extract HQ parameter and V cb at the same time M X moments o= used, = unused in the nominal fit B A B AR 2 /ndf =20/15 M1xM1x M2xM2x M3xM3x M4xM4x M0lM0l M1lM1l M2lM2l M3lM3l Red line: HQE fit Yellow band: theory errors P.Gambino, N.Uraltsev hep-ph/0401063 hep-ph/0403166
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April 2006 E. Barberio 11 Vcb and HQ parameters Exp HQ sl Global fit Kinetic scheme expansion (hep-ph/0507253) V cb @ 2% m b < 1%, m c @ 5% (1S) expansion scheme has similar results used measurements:
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April 2006 E. Barberio 12 V ub inclusive determination B X u l rate tree level from OPE corrected for perturbative s and non-perturbative 1/m b terms BUT….. Br B X u l )/Br B X c l ) =1/50 In principle main uncertainty from m b 5
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April 2006 E. Barberio 13 Shape Function Shape Function need to be determined from experimental data Limited phase space to reduce the B X c l background: OPE doesn ’ t work everywhere in the phase space non- perturbative Shape Function F(K + ) to extrapolate to the full phase space 0 F(K + ) = M B -m b K+K+ Detailed shape not constrained, in particular the low tail Mean and r.m.s. are known
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April 2006 E. Barberio 14 Inclusive B X u l B l XuXu Signal events have smaller M X and P + Larger E l and q 2 m u << m c exploits different kinematics q 2 = lepton-neutrino mass squared m X = hadron system mass E l = lepton energy P + = E X -|P X | bubu bcbc bubu bcbc bubu bcbc bubu bcbc Not to scale!
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April 2006 E. Barberio 15 BaBar Lepton Endpoint B (10 -4 ) BABAR 80fb -1 5.72 ± 0.41 stat ± 0.65 sys Belle 27fb -1 8.47 ± 0.37 stat ± 1.53 sys CLEO 9fb -1 2.30 ± 0.15 stat ± 0.35 sys BABAR PRD 73:12006 Belle PLB 621:28 CLEO PRL 88:231803 BaBar E l >2.0 GeV Belle E l > 1.9 GeV Crucial accurate subtraction of background is crucial! S/B ~1/10 eff~ 40% First measurement from CLEO E l >2.3 GeV
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April 2006 E. Barberio 16 Measuring m X q 2 P + BABAR hep-ex/0507017 Belle PRL 95:241801 fully-reconstructed B meson flavor and momentum known lepton in the recoil-B m miss consistent with a neutrino lepton charge consistent with B flavor left-over particles belong to X equal m B on both sides; m miss = 0 Reconstruct all decay products to measure M X,q 2 or P + S/B ~ 2 Eff~ 0.1%
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April 2006 E. Barberio 17 P + BLNP PRL93:221802 Measuring Partial Branching Fraction B (10 -4 ) BABAR 211fb -1 m X 88.7 ± 0.9 stat ± 0.9 sys Belle 253fb -1 first measurement of P + spectrum m X < 1.712.4 ± 1.1 stat ± 1.0 sys m X 88.4 ± 0.8 stat ± 1.0 sys P + < 0.6611.0 ± 1.0 stat ± 1.6 sys
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Turning B into |V ub | HFAG main results: HQ parameters form b X c l and b X s hep-ph/0507253 Inclusive b → ulv q2q2 b → s Shape Function EE mbmb Inclusive b → clv mXmX ElEl HQE Fit mXmX ElEl WA duality |V ub | SSFs
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April 2006 E. Barberio 19 Belle E >1.8 GeV Dealing with Shape Function Solution use directly the spectrum: easy to fit shape function Better resolution K* peak (more difficult for SF) theory E* (GeV) E (GeV)
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April 2006 E. Barberio 20 Inclusive |V ub |: BLNP framework Inputs: m b (SF) = 4.60 0.04 GeV 2 (SF) = 0.20 0.04 GeV 2 Statistical 2.2% Expt. syst. 2.7% B X c l model 1.9% B X u l model 2.1% Subleading SF 3.8% other theory error 4.5% |V ub | = 7.3% |V ub | world average as of Winter 06 |V ub | BLNP =(4.45 0.20 0.26) 10 -3
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April 2006 E. Barberio 21 Theory Errors Quark-hadron duality is not considered (cut dependent) b cl and b s data fit well HQ predictions Weak annihilation 1.9% error l Expected to be <2% of the total rate l w.a. / (b u) < 7.4 % from CLEO HQ parameters 4.1% mainly m b ; kinematics cuts depend on m b, ! Sub-leading shape function 3.8% dominated by the lepton endpoint measurements B u b l q q
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April 2006 E. Barberio 22 Inclusive |V ub |: DGE framework DGE theory 2.9% matching scheme method and scale m b (MS) 1.3% on event fraction m b (MS)=4.20 0.04 GeV s 1.0% on event fraction total SL 3.0 % Dressed Gluon Exponentiation (DGE) on-shell b-quark calculation converted into hadronic variables used as approximation to the meson decay spectrum |V ub | DGE = (4.41 0.20 0.20) 10 -3 Still digesting the method
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April 2006 E. Barberio 23 Weight function LLR m x <1.67 GeV OPE m x <2.50 GeV V ub without Shape Function Based on Leibovich, Low, Rothstein, PLB 486:86 First proposal by Neubert m x cut Babar
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April 2006 E. Barberio 24 |V ub |: inclusive vs exclusive |V ub | inclusive W.A. Winter 06 |V ub | exclusive W.A. Winter 06
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April 2006 E. Barberio 25 |V ub |: CKM consistency Most probable value of V ub from measurements of other CKM parameters Standard Model predictions with ms measurement (thank to Pierini) V ub from exclusive measurements V ub from inclusive measurements
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April 2006 E. Barberio 26 Conclusions b cl V cb 2% error dominated by theory, m b @1% (kinetic and (1S) schemes), m c @5% (kinetic scheme) but how well do we know the B X c l spectrum? b ul V ub ~7.4% error shared between theoretical and experimental inclusive vs exclusive less than 1.4 difference, depending on the inclusive extracting method We have now different methods to extract V ub |V ub | @ 5% possible? Improve knowledge of B X c l, B X u l and more work on the theoretical error
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April 2006 E. Barberio 27 Inclusive |V ub |: comparisons HQ parameters from cl and sg HQ parameters from sg only
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April 2006 E. Barberio 28 M x unfolded spectrum for B X c l D* D** D Belle
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April 2006 E. Barberio 29 photon energy spectrum photon energy spectrum in B X not sensitive to new physics and give information on B structure E >2 GeV Belle E >1.8 GeV u, c, t CLEO E : photon energy spectrum in B s ( BaBar Belle CLEO Delphi )
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