1 / 9

Vacuum at F11 and the Interaction Points

Vacuum at F11 and the Interaction Points. Ron Moore FNAL. F11 vacuum and CDF proton halo losses – store 1289. before ferrite replacement @ F11 pressure and losses rise and fall. p intensity. F11 pressure. CDF PHSM. CDF LOSTP. F11 vacuum and CDF proton halo losses– store 1486.

doli
Download Presentation

Vacuum at F11 and the Interaction Points

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. Vacuum at F11 and the Interaction Points Ron Moore FNAL TeV Halo Meeting – 3 July 02

  2. F11 vacuum and CDF proton halo losses – store 1289 before ferrite replacement @ F11 pressure and losses rise and fall p intensity F11 pressure CDF PHSM CDF LOSTP

  3. F11 vacuum and CDF proton halo losses– store 1486 after ferrite replacement @ F11 pressure reduced, no dramatic rise losses do not rise F11 temperature F11 pressure CDF LOSTP

  4. D0 Pressure Profile FromMike McGee’s Simulation One half of IR D0IG01 pressure 2.4*10-9 torr Average pressure = 1.26*10-8 torr

  5. CDF Pressure Profile FromMike McGee’s Simulation One half of IR B0IG01 pressure 2.5*10-10 torr Average pressure = 1.22*10-8 torr

  6. D0 outgassing rate measured = 7.3*10-9 torr*liter/sec expected = 29*10-9 torr*liter/sec CDF outgassing rate measured = 7.1*10-9 torr*liter/sec expected = 29*10-9 torr*liter/sec Both outgassing rates 1/4 the expected rates

  7. Summary • Replacing ferrite rods improved vacuum @ F11 and eliminated CDF proton loss bump • Expected average pressure @ IPs  1.2*10-8 torr • But, measured outgassing rates are 1/4 expected • Models are being reexamined • Vacuum at IPs likely better than initially believed • IPs are not “hot spots” of poor vacuum R. Moore - FNAL

  8. Proton halo over past 4 months Proton loss rates from experiments divided by narrow-gate intensity D0 CDF

More Related