1 / 24

Concluding Remarks

Concluding Remarks. L. Littenberg - BNL K-Rare Decays Frascati - 27 May 05. Isidori Arguments. Motivation, c’d. K  & MSSM. Contribution of K  after LHC. E949. E787/949 Events. E949 Event. Products of E787/949. SPI measurements. Analysis methods. J-PARC K +  +  LOI.

dawson
Download Presentation

Concluding Remarks

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. Concluding Remarks L. Littenberg - BNL K-Rare Decays Frascati - 27 May 05

  2. Isidori Arguments

  3. Motivation, c’d

  4. K & MSSM

  5. Contribution of K after LHC

  6. E949

  7. E787/949 Events E949 Event

  8. Products of E787/949 SPI measurements Analysis methods

  9. J-PARC K++ LOI • Stopped K+ experiment • Builds on E787/949 experience • Lower energy separated beam • Higher B spectrometer • More compact apparatus • Better resolution • Finer segmentation • Improved  veto (crystal barrel) • Aims for 50 events • Not an early experiment for J-PARC • Needs beamline • place on the floor • $ for detector

  10. K decay at rest • Decades of experience • Bckgnd <1.5 x 10-11 • Almost everything well-understood • Can confidently scale in most parameters • Biggest questions are money and will • Need appropriate beamline • Need better duty cycle • Need funding for detector • Need collaboration • Couldbe sure of ~50 SM events, maybe 100 if pnn2 region can be used

  11. NA48/3

  12. NA48/3 • Ambitious in-flight attempt to get ~65 SM events with good S:B • Benefits from several years of thought (CKM, etc.) • Brute force approach to beam • Needs some development of techniques • Has reasonable toolset • Equiv p* resolution 1.3 MeV/c (c.f. 2.3 for E949) • Redundant background rejection methods • Benefit of decay in vacuum, high energy • Concerns • There’s always a beam pion • Unanticipated background

  13. E391a KL0

  14. po produced at CC02 po produced at CV (?) KL popopo KL p+p-po KL  popo KL gg Confronting the Enemy Run 1 expected s.e.s ~ 10-8, expected BG ~310-9

  15. Responding to experience Run I  Run 2  Run 3 • Neutron background much reduced, now confronting KL decay contribution • Confident they can reduce the background to < 10-9

  16. Products of E381a Beam design & MC proofing Photonuclear SPI measurements Charged particle inefficency measurements

  17. E391a to J-PARC 50 more KL Thicker photon vetoes Deeper, more granular crystals Faster electronics Goal: 40 evts in 3 years, starting in 2009?, S:B ~ 1

  18. J-PARC KL - Part II Evts 3 options: 180 60 290

  19. KLOD IHEP 60 GeV proton beam - take off at 35 mr KL’s peak at ~6 GeV/c Aim to get 28 events/9 background in 3 years Could be ready to run in 2008?

  20. KOPIO

  21. Kinematic Separation of Signal and Backgrounds Signal Backgrounds

  22. Charged particle ineff. measurements KOPIO Products 3rd generation shashliyk Accelerator R&D Bomb detection

  23. Future History K+ SM KL

  24. K & Ke+e- • Could enhanced endpoint of K show up in Ke+e-? • With UC, predicted BR at endpoint predicted as ~10-8 • That part of Ke+e- maybe 3 larger. •  gives K  Ke+e- maybe 400 times smaller. • In amplitude 20 times smaller • Could be 10% effect in interference?

More Related