1 / 34

Unveiling New Physics with Super-B Factory: Highlights from Toru Iijima’s Talk at Nagoya University

Discover the cutting-edge physics breakthroughs discussed at the 2nd Super-B Factory Workshop in Hawaii by Toru Iijima on April 20, 2005. Explore topics such as CP violation, NP scenarios, CKM corrections, and the paradigm shift towards New Physics.

karib
Télécharger la présentation

Unveiling New Physics with Super-B Factory: Highlights from Toru Iijima’s Talk at Nagoya University

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Highlights of Super-KEB Physics LoI Toru Iijima Nagoya University April 20, 2005 2nd Super B Factory Workshop in Hawaii

  2. In This Talk, … Physics case with 5ab-1 50 ab-1 data at Super-B based on • Letter of Intent for KEK Super B Factory ( KEK Report 2004-4 ) • Physics at Super B Factory ( hep-ex/0406071 ) Contents; • Super-B Motivation • Super-B Physics Reach • Studies of NP Scenario • Summary cf) SLAC-R-709 The Discovery Potential of a Super B Factory Proceedings of the 2003 SLAC Workshops

  3. Success of B Factories First precise test of KM picture for CPV. • sin2f1= +0.726±0.037 is now a precise measurement (~5%). • The other angles are being measured more seriously. • f2 from Srr and rp Dalitz • 2f1+f3 from BD(*)p • f3 from BDK (w/ D Dalitz) + side measurements too. |Vcb|, |Vub|. Dmd A bit old… sorry. ! Paradigm change: look for Alternatives to CKM Corrections by NP ? ~300fb-1(KEKB) ~250fb-1(PEP-II) Far Precise Test to Look for Correction by NP !

  4. New Physics in bs loop ? b⇔s (3rd ⇔ 2nd) should be explored. • Present constraint mainly with transitions between • 3⇔1 generation • 2⇔1 generation • CPV (bsqq) Anomaly? <charmonium> = 0.726±0.037 <bs penguin> = 0.43±0.07 (’05 winter) 0.39  0.11 (Belle) 0.45  0.10 (BABAR) 3.7s deviation !! -hf x Sf Search for New Origin of Flavor Mixing & CP Violation !

  5. Off-diagonal terms Flavor Physics Luminosity frontier Diagonal terms: LHC/ILC Energy frontier cf) Top quark: Mass/width by Tevatron Mixing/phase by B factories B and t are in the 3rd generation (“hub” quark & lepton) probe for both 32, 31 transitions. B Physics in LHC Era • Once NP found in B/LHC, the next question would be What is the NP scenario ? • Orthogonality of B physics to LHC • The squark/slepton mass matrix • Sensitive to SUSY breaking mechanism.

  6. Cont’d B & t decays would be ideal probes for flavor structure of NP. • Super-B key measurements • CPV in bs • FCNC (Kll, Kvv etc.) • LFV (t decays) • Higgs mediation (BDtn etc.) • CKM • + their correlation + Synergy to LHC and other flavor physics exp’s. LHC LC EDM LFV B physics K physics Muon g-2 Charm physics Elucidation of New Physics Scenario

  7. Super Belle Aerogel Cherenkov counter + TOF counter g “TOP” + RICH CsI(Tl) 16X0 g pure CsI (endcap) Si vtx. det. 4 lyr. DSSD SC solenoid 1.5T g 2 pixel/striplet lyrs. + 4 lyr. DSSD Tracking + dE/dx small cell + He/C2H5 • remove inner lyrs. Use fast gas m / KL detection 14/15 lyr. RPC+Fe g tile scintillator New readout and computing systems

  8. Vub Charged Higgs direct CPV f2(a) isospin analysis p+ p- Ks trajectory B vertex IP profile g g Feature of Super-Belle Exp. Belle SuperBelle • Cleaner than hadron machines even after the upgrade • Many off-timing hits, but typical track eff. 91%  89% • B decays with neutrinos BDtn, tn, u ln etc. • B decays with g, p0B Xsg, p0p0 etc. • B vertex reconstruction with Ks only ! BKsp0, Ksp0g etc. B meson beam ! Dtn etc. B e- (8GeV) e+(3.5GeV) full (0.1~0.3%) reconstruction BgDp etc. Υ(4S) p B

  9. CPV (b  s) FCNC w/ n CKM and rich t physics Physics Reach at Super-KEKB SuperKEKB 5ab-1 50ab-1 LHCb 2fb-1 Physics at Super B Factory (hep-ex/0406071)

  10. Measurement of f2 and f3 • f2 measurement • Bpp (isospin analysis) Df2 = 3.9/1.2 deg. (5/50ab-1) • Brp (Dalitz plot analysis) Df2 = 2.9/0.9 deg. (5/50ab-1) • f3 measurement by BDK • Dalitz analysis Df3 = 4/1.2 deg. (5/50ab-1) Model error ? • ADS method Df3 = 16/ 5 deg. (5/50ab-1) Limited by stat. Belle @ present (model)

  11. Measurement of |Vub| • Inclusive bu l n withfully reconstructed tag. Mx, q2, P+ • Good determination of mb by bc l n / bsg is essential. • Exclusive Bp l n withfull recon or D* l n tagging. • High quality data in high q2 • Form factor by unquenched lattice Dp l n @ CLEO-c Extrapolation from present (Mx,q2) measurement. dmb ~ 70 MeV presently ~5% determination is possible.

  12. Vub & f3 sin2f1 & Dmd CKM at Super-B 50 ab-1 CKM is only one part of Super-B physics programs, but still provides model indep. approach to constrain NP. M12=M12SM+M12NP

  13. J/y KS0 fK0 (input S=+0.24) Expectation at 5ab-1 New CPV Phases in bsqq • bs loop is the ideal place to look for new CPV phases. The region for 5s discovery w/ present <bs Penguin> DS theory error fK0: ~0.05 h’K0: ~0.10

  14. <0.37<0.60 <0.3<0.55 <0.5<0.60 A A A h’Ks K+K-Ks fKs -hf x Sf -hf x Sf -hf x Sf Cont’d • 5s confidence region for A and S (5ab-1/50ab-1) Sanda @ CKM2005. The reason why present B is so successful. “Luminosity requirement was set so that we can find CPV even if sin2f1 ~0.10, but it is turned out to be large (~0.72)” Theoretical limitation The region to cover Luminosity goal

  15. C7 Present result +0.63 -0.50 S= -0.79±0.09 (Belle) S= +0.25±0.63±0.14 (BaBar) BXsg CP Asymmetry • Sensitive NP. • Theoretically clean. • Standard Model “~Zero”. • Helicity flip of g suppressed by ~ms/mb Belle Present Belle (stat./syst.) 5ab-1 50ab-1 Acpmix(BK*g, K*Ksp0) 0.56 / 0.09 0.14 0.04 Acpdir(BXsg) 0.051 / 0.038 0.011 0.005

  16. Update from a recent study @ 5ab-1 dC9 ~ 11% dC10 ~14% d q0 ~11% BXsll FB Asymmetry • Good electroweak probe for bs loop. • q2 distribution has different pattern depending on sign(C7). Belle at 250fb-1 q0(the point w/ AFB=0) is sensitive for New Physics SM; q02=(4.2±0.6)GeV2 ※ shown w/ reversed sign definition.

  17. tlg w/ improvement Extrapolation Present CLEO tlp/h/h’ t3l tl Ks tB g/p Lepton Flavor Violation LFV in neutrino sector ⇒LFV in charged leptons ? Search for “SM Zero” tlg t3l, lh B-factory = “Tau-factory” 1010t pairs at 10ab-1 Search region enters into O(10-810-9)

  18. Super-B Present Belle • t3l,lh • Neutral Higgs mediated decay. • Important when MSUSY >> EW scale. Gaugino mass = 200GeV tlg/3l,lh tlg • SUSY + Seasaw • Large LFV Br(tmg)=O(10-7~9)

  19. c b H+/W+ t+ nt Search for Charged Higgs • BDtn (semileptonic decay) Band width from form-factor uncertainty • Full reconstruction tag • Signal  large missing mass • Expected at 5ab-1

  20. Sensitivity for Charged Higgs Constraint from BXsg BDtn D(Form-factor) ~5% D(Form-factor) ~15% Btn (present) LHC 100fb-1 D(form-factor) can be reduced with the present BDmn data.

  21. Elucidation of NP Scenario • T. Goto, Y.Okada, Y.Shimizu,T.Shindou, M.Tanaka, hep-ph/0306093, also in SuperKEKB LoI 1 Hard to distingusih only with mass 2 3 4 Can we distinguish these 4 senarios at Super-KEKB?

  22. 280fb-1 5ab-1 50ab-1 Acp(BfKs) vs SUSY Models U(2) tanb=30 mSUGURA tanb=30 Acpmix SU(5)+nR tanb=30 degenerate SU(5)+nR tanb=30 non-degenerate If confirmed with the central value unchanged. Large impact on LHC physics and cosmology if new CPV in bs: Eg. mSUGRA, Gauge mediated SUSY breaking

  23. Acp(BXsg) vs SUSY models 5ab-1 50ab-1 Mixing CPV Direct CPV U(2) tanb=30 mSUGURA tanb=30 U(2) tanb=30 mSUGURA tanb=30 Acpdir Acpmix SU(5)+nR tanb=30 non-degenerate SU(5)+nR tanb=30 degenerate SU(5)+nR tanb=30 non-degenerate SU(5)+nR tanb=30 degenerate up to 2TeV can be explored.

  24. CPV in bs and SUSY Scenario • Different SUSY breaking scenario can be distinguished in Acpmix(fKs) - Acpmix(K*0g) correlation. Expected precision at 5ab-1 Correlation of other ovservables are also useful. Acpdir(Xsg), AFB(Xsll), Br(tmg), CKM

  25. U(2) FS tanb=30 Mgluino=600GeV/c2 mSUGRA tanb=30 Mgluino=600GeV/c2 SU(5)+vR non-degenerate tanb=30 Mgluino=600GeV/c2 SU(5)+vR non-degenerate tanb=30 Mgluino=600GeV/c2 SU(5)+vR degenerate tanb=30 Mgluino=600GeV/c2 More Tests of SUSY Scenario Acpmix(fKs) Acpdir(Xsg) Br(tmg) Br(Xsg) AFB(Xsll) SUSY GUT relation Acpmix(Xsg) Acpmix(fKs) Correlation to bs Acpdir(Xsg) Br(Xsg) AFB(Xsll)

  26. Theoretical limitation ? Detector feasibility Synergy to LHC (need more studies) Summary Super-B is an unique facility to provide O(1010) B and t in clean environment (550ab-1) The Mission Far Precise Test to Look for Correction by NP. Search for New Origin of Flavor Mixing & CP Violation Elucidation of New Physics Scenario

  27. Cosmology Particle Physics at Higher Energy at TeV (Higgs, SUSY…), GUT 10-44 10-36 1032/1019 Accelerator frontier (Energy/Luminosity) 10-10 Physics at Super-KEKB/Belle New Origin of Flavor Mixing and CPV Elucidation of NP Scenario 10-5 1028/1015 時間(秒) Synergy with HE frontier and other flavor physics exp’s 1015/100 Hadron Physics New states Cosmology Baryogenesis 1012/0.1 温度/E (K/GeV) Particle Physics Super-B has Significant impact on particle physics in LHC era Links to other fields WMAP Dark Energy (73%) Big Bang ! GUT Dark Matter(23%) Inflation String Baryogenesis New Physics ~1 TeV CP Violation SUSY Standard Model Gauge Theory Higgs Quark/Lepton Neutrino Mass New hadrons? Nucleo- synsesis QGP We should convince community in and around HEP the importance of Super-B. Hadrons Nuclei

  28. Backup Slides

  29. KEKB Upgrade Scenario Lpeak = 1.41034cm-2s-1 Ltot = 330fb-1 (Nov.30, 2004) ~1010 BB/year !! & similar number oft+t- world records ! Major upgrade of KEKB & Belle detector (>1yr shutdown) SuperKEKB Crab cavities Lpeak (cm-2s-1) Lint 5x1034 ~1 ab-1 1.4x1034 330 fb-1 5x1035 ~10 ab-1

  30. Pattern of Deviation from SM Unitarity triangle Rare decay Y.Okada ++: Large, +: sizable, -: small

  31. 5ab-1 50ab-1 UT vs SUSY models Dm(Bs)/Dm(Bd) SU(5)+nR tanb=30 degenerate mSUGRA tanb=30 SU(5)+nR tanb=30 non-degenerate U(2) tanb=30 f3 (degree)

  32. CP Asymmetries in B ->f Ks and b-> sg CP asymmetry in B ->f Ks CP asymmetry in B -> K*g Direct asymmetry in b -> s g

  33. Agashe,Perez,Soni,hep-ph/0406101(PRL); hep-ph/0408134 SUSY vs. Warped Extra Dimensions at LHCb SuperKEKB B(B g Xsl+l-) = (4.51.0) x 10-6 (present WA) also constrains RR and LL mass insertions: i.e. related to S(fKs) “DNA Identification” of New Physics from Flavor Structure

  34. X(3872) Q(1540)pK- Pentaquark search in various methods (1520) pK- • e+e-  many K • Interaction with material Charmed partner pKS D-p Search for New Hadrons Observation of a New Narrow Charmonium State… PRL 91, 262001 (2003) Observation of double cc production in e+e- annihilation… PRL 89, 142001 (2002) hc (2S) cc0 hc DsJ(2317) DsJ(2457) Observation of DsJ(2317) and DsJ(2457) in B decays PRL 89, 142001 (2002) B factory is a gateway to new hadrons.

More Related