a Part 1: Matter-Antimatter Asymmetry Part 2: CP Violation and the SM g b Part 3: Beyond the Standard Model New Results from the BaBar Experiment K. Honscheid Dept. of Physics Ohio State University K. Honscheid, WSU Apr. 15, 2005 Matter, Energy and the Big Bang • Einstein showed us that matter and energy are equivalent • When matter and antimatter meet, they annihilate into energy • Energy can also materialize as particleantiparticle pair Predict: Exp: nMatter/nPhoton~ 0 nb/ng~ (6.1 +/- 0.3) x 10-10 (WMAP) K. Honscheid, WSU Apr. 15, 2005 So how can this happen? In 1967, A. Sakharov showed that the generation of the net baryon number in the universe requires: 1. Baryon number violation (Proton Decay) 2. Thermal non-equilibrium 3. C and CP violation (Asymmetry between particle and anti-particle) Transition to broken electroweak symmetry provides these conditions K. Honscheid, WSU Apr. 15, 2005 Experimental Possibilities: • Get equal amounts of matter and anti-matter • Wait… • See what’s left (in anything) K. Honscheid, WSU Apr. 15, 2005 PEP-II Asymmetric B Factory Stanford Linear Accelerator Center, Stanford, California K. Honscheid, WSU Apr. 15, 2005 The BaBar Experiment K. Honscheid, WSU Apr. 15, 2005 Preparing the Matter – Antimatter Sample B mesons contain a b quark and a light anti-quark. BB Threshold mB = 5.28 GeV (~5x mProton) bb 0.28 hadr The Upsilon(4S) - a copious, clean source of B meson pairs 1 of every 4 hadronic events is a BB pair No other particles produced in Y(4S) decay Equal amounts of matter and anti-matter Collect a few 108 B0 B0 pairs K. Honscheid, WSU Apr. 15, 2005 Analysis techniques Threshold kinematics: we know the initial energy of the system *2 mES Ebeam pB*2 Signal * E EB* Ebeam Event topology Signal (spherical) Background Background (jet-structure) K. Honscheid, WSU Apr. 15, 2005 Searching for the Asymmetry 227 x 106 B0 Mesons 227 x 106 B0 Mesons Count B0K+ Decays Count B0K-+ Decays Is N(B0K+ ) equal to N(B0K-+ )? K. Honscheid, WSU Apr. 15, 2005 How to Tell a Pion from a Kaon Angle of Cherenkov light is related to particle velocity – Transmitted by internal reflection – Detected by~10,000 PMTs Quartz bar Particle c Cherenkov light K. Honscheid, WSU Apr. 15, 2005 Active Detector Surface Searching for the Asymmetry 227 x 106 B0 Mesons 227 x 106 B0 Mesons Count B0K+ Decays Count B0K-+ Decays Is N(B0K+ ) equal to N(B0K-+ )? B0K+ B0K+ BABAR BABAR background subtracted K. Honscheid, WSU Apr. 15, 2005 Direct CP Violation in B Decays nK 1606 51 Using n B 0 K 910 n B 0 K 696 AK 0.133 0.030 0.009 ACP We obtain Br B f Br B f Br B f Br B f nK 1606 51 AK 0.133 0.030 0.009 First confirmed observation of direct CP violation in B decays K. Honscheid, WSU Apr. 15, 2005 Part 2: CP Violation in the Standard Model CP Operator: CP( g q coupling q’ J ) = q’ g* q J Mirror To incorporate CP violation g ≠ g* (coupling has to be complex) K. Honscheid, WSU Apr. 15, 2005 The Kobayashi-Maskawa Matrix • The weak interaction can change the favor of quarks and lepton • Quarks couple across generation boundaries Vcb Vub • Mass eigenstates are not the weak eigenstates • The CKM Matrix rotates the quarks from one basis to the other d’ s’ b’ d u s b Vud Vlus Vub d l 3 = c Vcdl Vcs Vcbl 2 t l Vtd Vltd Vtb 3 2 l=cos(c)=0.22 K. Honscheid, WSU Apr. 15, 2005 s b The Unitarity Triangle Visualizing CKM information from Bd decays • • The CKM matrix Vij is unitary with 4 independent fundamental parameters Unitarity constraint from 1st and 3rd columns: i V*i3Vi1=0 d s b u Vud Vus Vub c Vcd Vcs Vcb t Vtd Vts Vtb CKM phases (in Wolfenstein convention) 1 1 e-iγ 1 1 1 e-iβ 1 1 • Testing the Standard Model – Measure angles, sides in as many ways possible – SM predicts all angles are large K. Honscheid, WSU Apr. 15, 2005 Understanding CP Violation in B K Tree decay B0 K-+ A1 = a1 eifif11eid1 + A2 = a2 eif2 eid2 Vus* g B 0 b d Vub s u u d K A Vus*Vub B0 K+- A1 = a1 e-if-if11eid1 + A2 = a2 e-if2 eid2 Penguin decay B b 0 u,c,t g d s u u d K A Vts*Vtb • include the strong phase (doesn’t change sign) • more than one amplitude with different weak phase; (A = A1+A2) |A|2 – |A|2 G(B) – G(B) ~2 sin(f1 f2) sin(d1 d2) Asymmetry = = = 0 2 2 |A| + |A| G(B) + G(B) K. Honscheid, WSU Apr. 15, 2005 B0 B0 Mixing and CP Violation fb A neutral B Meson fb N(B0)-N(B0) N(B0)+N(B0) The SM allows B0 B0 oscillations CPV through interference between mixing and decay amplitudes B0 ACP e i f M 12 Mixing frequency md 0.5 ps-1 Interference between B0 fraction ~ sin(m t) d ‘B B fCP’ and ‘B fCP’ 2i M ie B 0 fCP ACP e i f K. Honscheid, WSU Apr. 15, 2005 Time-Dependent CP Asymmetries b W+ B0 c c s d d J / CP Eigenstate: hCP = -1 K 0 KS0 0 0 G(Bphys (t ) fCP ) G(Bphys (t ) fCP ) AfCP (t ) sin2 hfCP Im lbfCP sin md t 0 0 G(Bphys (t ) fCP ) G(Bphys (t ) fCP ) Amplitude of CP asymmetry Im lb ccs VcsVcb* VtbVtd* VcsVcd* Vtd* sin2b Im * * * Im Vtd VcsVcb VtbVtd VcsVcd Quark subprocess B0 mixing K0 mixing K. Honscheid, WSU Apr. 15, 2005 Time-dependent analysis requires B0 flavor tagging t =0 We need to know the flavour of the B at a reference t=0. z = t gbc 0 At t=0 we B0 know this meson is B0 B rec K s (4S) bg =0.56 B0 The two mesons oscillate coherently : at any given time, if one is a B0 the other is necessarily a B0 tag W l (e-, m -) In this example, the tagside meson decays first. It decays semi-leptonically and the charge of the lepton gives the flavour of the tag-side meson : l = B0 l = B 0. Kaon tags also used. B0 b d t picoseconds later, the B 0 (or perhaps its now a B 0) decays. K. Honscheid, WSU Apr. 15, 2005 l l Step by Step Approach to CP Violation B tagged 1. B tagged 2. 3. t (ps) 4. ACP(t) 5. sin 2b 6. Start with a few x 108 B0 B0 pairs (more is better) Reconstruct one B0 in a CP eigenstate decay mode Tag the other B to make the matter/antimatter distinction Determine the time between the two B0 decays, t Plot t distribution separately for B and B tagged events Extract ACP and sin2b sinmt t (ps) K. Honscheid, WSU Apr. 15, 2005 Results: sin 2b and the observation of CP 227 million BB pairs J/Ks and other b cc s final states CP = -1 7730 events (12w) sin(2b) w = mis-tag fraction •B •B •B •B •B J/ Ks0, Ks0 +-, 00 (2S) Ks0 c1 Ks0 J/ K*0, K*0 Ks0 hc Ks0 CP = +1 •B J/ KL0 BaBar result: sin2b = 0.722 0.040 0.023 K. Honscheid, WSU Apr. 15, 2005 The Unitarity Triangle (r,h) Vub* Vud Vcd Vcb* (0,0) a g Vtd Vtb* Vcd Vcb* o (0,1) [23.3 ± 1.5] K. Honscheid, WSU Apr. 15, 2005 Ks is not the only CP Eigenstate Access to a from the interference of a b→u decay (g) with B0B0 mixing (b) Tree decay B0B0 mixing b B 0 d Vtb* Vtd* t t Vud* g d B 0 B b Vtb Vtd q / p Vtb*Vtd / VtbVtd* 0 b d Vub d u u d A Vud* Vub q A l e i 2 b e i 2g ei 2a p A abg sin2a ACP(t)=sin(2a)sin(mdt). K. Honscheid, WSU Apr. 15, 2005 Time-dependent ACP of B→ Blue : Fit projection Red : qq background + B0→K cross-feed B0 B0 N ( B ) 467 33 (227M BB ) B( B ) (4.7 0.6 0.2) 10 0 6 "sin( 2a ) " 0.30 0.17 0.03 BR result in fact obtained from 97MBB K. Honscheid, WSU Apr. 15, 2005 Houston, we have a problem B0 +K K K B0 K+- q q B0+ 157 19 (4.7 0.6 0.2) x 10-6 B0K+ 589 30 (17.90.9 0.7) x 10-6 Penguin/Tree ~ 30% K. Honscheid, WSU Apr. 15, 2005 The route to sin2a: Penguin Pollution Access to a from the interference of a b→u decay (g) with B0B0 mixing (b) • Tree decay B0B0 mixing b B 0 d Vtb* Vtd* t t Vud* g d B 0 B b Vtb Vtd q / p Vtb*Vtd / VtbVtd* Penguin decay Vub 0 b d d u u d B b 0 u,c,t d q A e i 2 b e i 2g ei 2a p A lCP e i 2a Inc. penguin contribution S sin( 2a ) C 0 Time-dep. asymmetry : NB : T P e ig eid T P e ig eid S 1 C 2 sin( 2a eff ) C sin d A (t ) S sin( md t ) C cos(md t ) T = "tree" amplitude A Vtd*Vtb A Vud* Vub lCP g d u u d How can we obtain α from αeff ? P = "penguin" amplitude K. Honscheid, WSU Apr. 15, 2005 How to estimate |aaeff| : Isospin analysis • Use SU(2) to relate decay rates of different hh final states (h {,r}) • Need to measure several related B.F.s Α A( B 0 ) ~ Α A( B 0 ) Α A( B ) 0 0 Α 00 A( B 0 0 0 ) ~ 00 Α A( B 0 0 0 ) Difficult to reconstruct. Limiting factor in analysis Gronau, London : PRL65, 3381 (1990) K. Honscheid, WSU Apr. 15, 2005 Now we need B→ • 61±17 events in signal peak (227MBB) – Signal significance = 5.0 – Detection efficiency 25% Using isospin relations and • 3 B.F.s – B0 – B – B0 2 asymmetries – – C C |aaeff |< 35° B±→r±0 • • Time-integrated result gives : B( B ) (1.17 0.32 0.10) 10 0 0 0 C 0 0 0.12 0.56 0.06 6 • Large penguin pollution ( P/T ) – Isospin analysis not currently viable in the B→ system K. Honscheid, WSU Apr. 15, 2005 B → rr: Sometimes you have to be lucky P → VV decay three possible ang mom states: S wave (L=0, CP even) P wave (L=1, CP odd) D wave (L=2, CP even) d 2N f L cos 2 1 cos 2 2 14 (1 f L ) sin 2 1 sin 2 2 d cos1d cos 2 r helicity angle We are lucky: ~100% longitudinally polarized! Transverse component taken as zero in analysis PRL 93 (2004) 231801 K. Honscheid, WSU Apr. 15, 2005 Time dependent analysis of B→rr • Maximum likelihood fit in 8-D variable space very clean tags B0 32133 events in fit sample (122M BB ) N ( B r r ) 617 52 S r r ( long) 0.33 0.24 00..08 14 Cr r (long) 0.03 0.18 0.09 B0 ACP (t ) f L Glong G 0.99 0.0300..04 03 (97M BB ) B( B 0 r r ) (30 4 5) 106 c. f . B( B 0 ) 4.7 106 K. Honscheid, WSU Apr. 15, 2005 Searching for B→rr • Similar analysis used to search for rr – Dominant systematic stems from the potential interference from B→a1±± (~22%) N ( B 0 r 0 r 0 ) 3322 20 12 (227 M BB ) Rec. Eff. 27% c.f. B→ B.F.= 4.7 x 106 and B→ B.F.= 1.2 x 106 6 B( B 0 r 0 r 0 ) (0.5400..36 32 0.19) 10 B (B→rr = 33 x 106 1.1106 90% C.L. K. Honscheid, WSU Apr. 15, 2005 Isospin analysis using B→rr 0 0 0 • The small rate of B r r – |aaeff | is small[er] means – P/T is small in the B→rr system (…Relative to B→ system) – No isospin violation (~1%) – No EW Penguins (~2%) A A 2 2da A00 2 peng A00 A0 A0 |aaeff |< 11° a 100 8(stat.) 4(syst.) 11( penguin) K. Honscheid, WSU Apr. 15, 2005 The Unitarity Triangle [103 (r,h) ± 11]o Vub* Vud Vcd Vcb* (0,0) g Vtd Vtb* Vcd Vcb* b [23.3 ±(0,1) 1.5]o K. Honscheid, WSU Apr. 15, 2005 The 3rd Angle: g Basic Idea Use interference between B D 0K and B D 0K decays where the D 0 (D 0 ) decay to a common final state f Vus* A VubVcs* l 3 r 2 h 2 eig Vub Vcb V * cs A VcbVus* l 3 Color suppressed Size of CP asymmetry depends on (*)0 | A ( B D K )| rB(*) ~ 0.1 0.3 (*)0 | A(B D K ) | K. Honscheid, WSU Apr. 15, 2005 First Look at the Data 214M pairs CP K K 75 13 18 7 CP Only a loose bound on rB with current statistics: (rB)2 = 0.19±0.23 KS 0 76 13 BABAR-CONF-04/039 Several other methods are being investigated More data would help a lot… K. Honscheid, WSU Apr. 15, 2005 Combined Experimental Constraint on g BABAR & Belle combined From combined GLW and ADS fit: 20 g 51 34 o CKM indirect constraint o 8 fit: g 58 7 K. Honscheid, WSU Apr. 15, 2005 The Unitarity Triangle [103 ± 11]o Vub* Vud Vcd Vcb* a Vtd Vtb* Vcd Vcb* b (0,0)+20 ]o [51 -34 [23.3 ± 1.5]o K. Honscheid, WSU Apr. 15, 2005 Putting it all together • The complex phase in the CKM matrix correctly describes CPV in the B meson system. • Based on SM CPV the baryon to photon ratio in the universe should be nb/ng~ 10-20 h • Experimentally we find nb/ng~ (6.1±0.3) x 10-10 (WMAP) r K. Honscheid, WSU Apr. 15, 2005 Part 3: Beyond Consistency the Standard Checks Model • FCNC transitions bsg and bdg are sensitive probes of new physics h a 2 g (3 ) VtdVtb VcdVcb b (1 ) • Precise Standard Model predictions. 0, 0 1, 0 r Ali et al hep-ph/0405075 • Experimental challenges for bdg (Brg Bwg) – Continuum background – Background from bsg (BK*g) (50-100x bigger) K. Honscheid, WSU Apr. 15, 2005 Combined B0r0g,B0wg,B-r-g results • No signals observed @90% CL K. Honscheid, WSU Apr. 15, 2005 CKM constraints from Br(w)g BABAR BF ratio upper limit < 0.029 → |Vtd/Vts| < 0.19 (90% CL) Ali et al. hep-ph/0405075 (z2,R) = (0.85,0.10) no theory error (z2,R) = (0.75,0.00) with theory error Penguins are starting to provide meaningful CKM constraint rg 95% CL BABAR allowed region (inside the blue arc) K. Honscheid, WSU Apr. 15, 2005 New CP Violating Phases in Penguin Decays? c b cb V W c J / Vcs d s K 0 + mixing lCP = -e-2b + mixing lCP = -e-2b + mixing lCP = -e-2b d W b t Vts* Vtb d d W b d t Vtb s s s Vts* s d d d f ,h,... K 0 K 0 w, 0 ,... K. Honscheid, WSU Apr. 15, 2005 Update on BfKo W b d u , c ,t B0g B 0 fKS0 s s f s d KS0 0.07 0.04 0.00 0.23 0.05 hCP SfK 0 0.50 0.25 C fK 0 hep-ex/0502019 114 ± 12 events SM Belle B 0 [BELLE-CONF-0435] fKL0 98 ± 18 events K. Honscheid, WSU Apr. 15, 2005 Reaching for more statistics – B 0 f K 0 revisited • Analysis does not require that ss decays through f resonance, it works with non-resonant K+K- as well – 85% of KK is non-resonant – can select clean and high statistics sample – But not ‘golden’ due to possible additional SM contribution with ss popping W B 0 b t s s s d g d b B t g 0 d OK s u u s s d K0 K0 b K K Nsig = 452 ± 28 (excl. f res.) VubVus ~ l 4Ru e i g VtbVts ~ l 2 W K+K- B 0 W d u s s u s d K K K0 Not OK • But need to understand CP eigenvalue of K+K-KS: • Perform partial wave analysis f has well defined CP eigenvalue of +1, - CP of non-resonant KK depends angular momentum L of KK pair – Estimate fraction of S wave (CP even) and P wave (CP odd) and calculate average CP eigenvalue from fitted composition K. Honscheid, WSU Apr. 15, 2005 CP analysis of B K+K- KS • Result of angular analysis fCP -even As2 2 0.89 0.08 0.06 As Ap2 – Result consistent with cross check using iso-spin analysis (Belle) fCP -even 2G(B K KS0KS0 ) 0.75 0.11 G(B0 K K K 0 ) • Result of time dependent CP fit SK K K 0 0.42 0.17 0.04 S CK K K 0 0.10 0.14 0.06 S hfSK+K-KS/(2fCP-even-1)] = +0.55 ±0.22 ± 0.04 ±0.11 (stat) (syst) (fCP-even) K. Honscheid, WSU Apr. 15, 2005 hep-ex/0502013 More penguin exercises – B0 KS KS KS • Use beam line as constraint and accept only KS with sufficient number of SVX hits. • Decay B0 KS KS KS is ‘golden’ penguin – little SM pollution expected • Although 3-body decay, only L=even partial waves allowed: – CP(KSKSKS) = CP(KS) = even VtbVts ~ l 2 W b t g B0 d ss ud d us ss sd d K0 K K K 0 K0 K 0 • Result consistent with SM hfK0 S 0.71 00..38 32 0.04 C 0.34 00..28 25 0.05 K. Honscheid, WSU Apr. 15, 2005 IP-Constrained Vertexing + Same technique as Ks0 hep-ex/0503011 Constrain decay products to beam-spot in x-y: 0 KS 4mm B0 inflated beam beam 200mm Vertex precision depends on number of hits in SVT For 4 hits, t resolution as good as with charged-tracks (60% events) Crosscheck with J/KS: K. Honscheid, WSU Apr. 15, 2005 Combined “sin2b” Results sin2β ~ 2.9 sin2β ~ 2.9 + sin2βPenguin .43 ±.7 sin2β ~ 3.7 …but comparison ignores subleading diagrams ! sin 2 b penguin K. Honscheid, WSU Apr. 15, 2005 0.4 Corrections: b→s Decay Amplitude ~ VubVus* * ub us (u ) f V V A W 4 ig l e b • Decays involving Vub enter with decay phase g • Doubly-CKM suppressed w.r.t dominant diagram u W u g, Z,g d d Contributes to all b sss modes b u s d s s s color-allowed tree color-suppressed tree b penguin d Contribute to h’Ks, f0Ks, wKs, but not fKs [in KKKs (requires ss popup from soft g)] d W s s s u u d Contribute to non-resonant KKKs (requires ss popup from soft g) K. Honscheid, WSU Apr. 15, 2005 Adding Theoretical Uncertainties • size of possible discrepancies Δsin2β have been evaluated for some modes: – estimates of deviations based on QCD-motivated specific models; some have difficulties to reconcile with measured B.R. • • • • • Beneke at al, NPB675 Ciuchini at al, hep-ph/0407073 Cheng et al, hep-ph/0502235 Buras et al, NPB697 Charles et al, hep-ph/0406184 2xΔsin2β – model independent upper limits based on SU(3) flavor symmetry and measured b d,sqq B.R. • [Grossman et al, PRD58; Grossman et al, PRD68; Gronau, Rosner, PLB564; Gronau et al, PLB579; Gronau et al, PLB596; Chiang et al, PRD70] ‘naive’ upper limit based on final state quark content, CKM (λ2) and loop/tree (= 0.2-0.3) suppression factors [Kirkby,Nir, PLB592; Hoecker, hep-ex/0410069] K. Honscheid, WSU Apr. 15, 2005 Conclusion • Almost 40 years after the discovery of CP violation in the kaon system we are finally in a position to improve our understanding of CP violation in the Standard Model • Belle and BaBar give consistent results for sin2b. Both work extremely well • The SM prediction of a single phase in the CKM matrix as cause of CP violation appears to be correct. • We now know how to distinguish between matter and anti-matter aliens. • New Physics will be needed to explain the baryon asymmetry in the universe • Will we find hints in CP phases and/or rare decays? • Stay tuned as more data is coming in. K. Honscheid, WSU Apr. 15, 2005