1 / 35

Search for B s  μμ and B d  μμ with 2 fb -1 of data

Search for B s  μμ and B d  μμ with 2 fb -1 of data. CDF 8925. blessed on Aug 09. Slava Krutelyov UCSB with D.Glenzinski, H.Held (KIT), C.-J.Lin (FNAL) T.Kamon, M.Weinberger (TAMU) M.Herndon (UWisconsin) SUSY-Group Meeting 08/29/2007. Motivation and history

jens
Download Presentation

Search for B s  μμ and B d  μμ with 2 fb -1 of data

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. Search for Bsμμ and Bdμμ with 2 fb-1 of data CDF 8925 blessed on Aug 09 Slava Krutelyov UCSB with D.Glenzinski, H.Held (KIT), C.-J.Lin (FNAL) T.Kamon, M.Weinberger (TAMU) M.Herndon (UWisconsin) SUSY-Group Meeting 08/29/2007 • Motivation and history • Analysis • Setup • Event selection: signal discriminants • muon ID with LH • Neural Net • (optimized) Expectations and results • Effects on SUSY

  2. S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  3. b m ~ n l’i23 l i22 m s Motivations: Models • MSSM • With RPV: can proceed at tree level • couplings not constrained much otherwise • In general case has a diagram ~ tan6b/MH4 • tan4b/MH4 come from MSSM is a 2HDM • remaining tan2b is from SUSY (stop L-R mixing) • Just need large tanb, not too-high MH, some stop mixing • SO(10) with Yukawa unification tanb~50 ! • mSUGRA with large tanb • Other BSM: with no extra flavor structure the enhancement < ~ a factor of 2 • With improving limits start asking any theorist “Is it allowed by Bsμμ?” • More in the end of the talk EXCLUDED Bsmm appears to get into the “model exclusion hall of fame” • Near 200 citations (combined for CDF/DØ RunII) in the past ~3 years S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  4. Bits of history • Search for Bsmm is as old as hadron colliders • First looked at by UA1 • Recent limits are all from Tevatron • DØ is often close to CDF Prior S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  5. Bs(d)m+m- Ingredients • Normalize to B+J/y K+ decays • Construct discriminant to select Bs and suppress bgd • MC sim for signal • Data mass sidebands for bgd estimate • Minimize expected 90% C.L. upper limit Signal sample (baseline) Normalization mode Bd Bs N(UU+UX) ~ 3×104 S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  6. Improving sensitivity: muon ID • Dx c2 cut  use muon LH (LH>0.1) • Combined dX, dPhi, dZ, EM, HAD • add dE/dX cut • Z>-0.2 • Suppress combinatorics • ~x2 less events (after preselection) • Bring Bhh below the horizon • Bhh fakes are ~0.05 for Bs and ~0.5 for Bd windows • cf. ~ 0.3 (Bs) and ~2 (Bd) with Dx c2cut S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  7. Normalization mode • B+J/ψK+ + c.c. S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  8. l/s μ l pmm pTmm pTm R=1 μ a l pTm Bs a Discriminating variables • Used as inputs to Neural Net S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  9. Preselections: signal+sidebands • Vertex Requirements: • c2(vtx) < 15 • s(L3D) < 150 mm • L3D < 1 cm • 0 < l < 3 mm • (l = proper decay length) • l/s(l) > 2 • pT(B)>4 GeV && |y(B)|<1 • 4669 < M(mm) < 5969 MeV • In addition: • Isolation>0.5 • Pointing angle Da<0.7 Bsmm Search Sample: N(CMU-CMU) = 15594 N(CMU-CMX) = 15072 (completely Bgd dominated) Note: without muon LH & dE/dX ~x2 more backgrounds here S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  10. Signal MC • Use Pythia • BGen for systematics • Reweigh to follow pT distributionfrom data • Compare using B+ data and MC S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  11. NN: inputs • After applying pre-selections use sidebands (bgd) and signal MC to train NN • 6 inputs to NN training • λ – lifetime • λ/σ – lifetime significance • Δα – 3D poining (vtx vs momentum) • Iso • pT(B) • pT(μ) min – lower of the pair S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  12. NN inputs: x-check w data B+ plots • Input variables are well-modeled • including pT(μ) high used in the trial NN S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  13. NN: output • Compared to LH (used previously) get a better (~2 times) rejection at the same efficiency • LH had 3 vars: Iso, P(λ), Δα • 5 var NN: add λ/σ and pT(B) • 7 var NN includes both pT(μ) • introduces mass biasnot used S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  14. NN output: x-check for biases • The correlation is negligible • No evidence of a bias here or in other x-checks • checked w/ control samples, trained on part of sidebands, bootstrap • use of sidebands is justifiable S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  15. NN outputs: x-check w data B+ • Good agreement S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  16. Control Samples • Independent bkg control samples to cross check bkg estimate procedure • OS - : Opposite-sign dimuon sample with ct<0 • SS+ : Same-sign dimuon sample with ct>0 • SS- : Same-sign dimuon sample with ct<0 • FM : Fake muon sample ct>0 • (require at least one muon leg to fail our muon likelihood and dE/dX requirement) S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  17. Control Samples: NN x-checks • NN performance: observation is consistent with expectations • Using a wider ± 150 MeV signal window for cross-check • For obsv<pred, prob= probability for making an observation ≤ obsv S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  18. Applying NN: getting expected bgd CMU-CMX CMU-CMU • Shape in sidebands give contribution of combinatorial bgd to signal bins • Separate fit in each NN bin: pol1 in bins 1, 2; pol0 in bin 3 S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  19. Inputs to the (exp./obs.) limit • Inputs to be used in the “main” formula • The biggest uncertainty is from fu/fs (after bgd stat) S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  20. Optimization: choice of NN bins • Relative (unnormalized) numbers are shown • The choice (of 3 bins) is • [0.8, 0.95]U(0.95, 0.995]U(0.995, 1] S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  21. Bhh contributions Contribution to Bdμμ • The contribution to Bs is small, considerable for Bd Contribution to Bsμμ S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  22. Expectations and observations: Bs S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  23. Expectations and observations: Bd S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  24. Results: limits • New world-best result S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  25. Results: 2D plots • P-value with bgd-only hypothesis, 10K pseudoexperiments CMU-CMU CMU-CMX Bsmm16% 67% Bdmm7% 58% • Observed events are consistent with expectation S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  26. Results: 2D plot combined S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  27. Results: 1D plots • Bs • 2 events in CMU-CMU channel • 1 event in CMU-CMX channel S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  28. Limits history • Getting better and better • faster than 1/sqrt(Lumi), slower than 1/Lumi • Unofficial Tevatron combination: Br(Bsμμ) < 4.5x10-8 @ 95% S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  29. S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  30. [easy model to exclude] SO(10) R. Dermisek et al., hep-ph/0507233 (2005) SUSY contemplations (1) • The importance of Bsμμ grows with tanβ • SUSY with large tanβ becomes more popular • driven by a more significant aμ now at ~3.4 σ away from SM • The SO(10) scenario by Raby et al. is practically excluded now S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  31. SUSY contemplations (2) • Light MSSM Higgs scenario is next in line for significant exclusion. Belyaev et al. SUSY07 S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  32. CDF Limit 5.8x10-8 2 fb-1 SUSY contemplations (3) • The limit eats further into the mSUGRA space now • not as significant with bsγ constraint considered S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  33. SUSY contemplations (4) • Start getting beyond bsγ at high tanβ • Still a way to go  2x10-8 will be way more noticeable S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  34. Summary • We have updated the Bmm analysis with 2 fb-1 • The limits improved significantly: • Br(Bsmm)<5.8×10-8 @ 95%CL • Br(Bdmm)<1.8×10-8 @ 95%CL • Both limits are the best in the world!!!! • Plan to prepare/publish in PRL • draft in progress ( to GPs this week?) S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

  35. backup S. Krutelyov Search for Bs,d-->mumu with 2 fb-1

More Related