1 / 20

LUMI06 preliminary conclusions

Explore the evaluation of novel technologies for optimizing particle accelerator upgrades like high-field quadrupoles and beam-beam compensators. Discover the risks, returns, and recommendations for R&D efforts based on rankings and guidelines for optics design.

acord
Download Presentation

LUMI06 preliminary conclusions

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. LUMI06preliminary conclusions Walter Scandale, Frank Zimmermann 3rd CARE-HHH-APD Workshop LUMI’06, Valencia, October 2006

  2. IR-ranking criteria • luminosity reach • energy deposition • beam lifetime & integrated luminosity • chromatic aberrations • technological difficulty: • hardware development, • experimental validation, • operational implementation

  3. Difficult to rank the IR from their performance:on-going studies not yes made with homogeneous parameters for an easy comparisonEasier to rank the technological objects

  4. (1) state-of-the-art NbTi quadrupole magnet • better heat transfer than present LHC triplets and/or low- gradient optics • can sustain (factor ~3-4?) higher interaction rate • (2) Nb3Sn high-field quadrupoles • gain in aperture or gradient >30% • under investigation by US-LARP • several talks (Tanaji, Ezio, Peter L., Rogelio,…) • main risk: no long prototype yet available (expected by 2009 – impossible to predict before this date) • could be available by 2015 • (3) Nb3Sn high-field dipoles, possibly open plane • simulation studies by Ramesh Gupta, Tanaji Sen and Nikolai Mokhov • under investigation by NED • main risk: no funding yet available to continue NED • prototyping cannot start before 2009 • could be available by ~2017

  5. (4) slim NbTi quadrupole doublet • standard technology • main risk: integration in the experiment • available by 2015 • (5) detector-integrated dipole • standard technology • main risk: integration in the experiment • available by 2015 • (6) wire compensation of long-range beam-beam effects • dc wire exists and already beneficial • requires experimental check with colliding beams • under investigation at CERN & RHIC • main risk: jitter control for ac wire • (7) crab cavities • investigated by R. Calaga, J. Tuckmantel, R. Tomas, F. Caspers • main risks: phase noise & synchronization at each IR, space

  6. (8) electron lens • investigated at Tevatron • main risks: jitter, p&e-orbit control, e- profile control, coherent or incoherent e-p interaction • head-on compensation and benefit could be demonstrated at RHIC • available by 2012 the above are the technological blocks from which all the proposed insertions can be constructed

  7. guidelines for optics design • quadrupole vs dipole first: quadrupole 1st needs less technological items and hence has to be preferred • compensation of crossing: wires are promising and should be considered for main variants of future optics layouts; crab cavities only for global small-angle option • dipoles & quadrupoles embedded in experiment: they can boost any future optics layout and should be investigated together with experimenters • electron lens: might be considered if head-on compensation proven to be efficient at Tevatron (or RHIC)

  8. ranking the schemes Low-gradient large-aperture NbTimagnets with large l* Risk 0, Return + Quad 1st“pushed” NbTi: tailored aperture & length, 2x better cooling, ~20% higher field NbTi-Nb3Sn hybrid scheme Quad 1st Nb3Sn Quad 1st withdetector-integrated dipole Detector-integrated quadrupole Quad 1stflat beam Separate-channel quad 1st Nb3Sn or NbTipluscrab cavities Dipole firstoptions withNb3Sn Pulsed or dc beam-beam compensator Risk 0, Return ++ Electron lens Risk 0, Return + Risk +, Return ++ Risk ++, Return +++ Risk ++, Return +++ Risk +, Return +++ Risk 0, Return ++ Risk +++, Return + retain options with perceived lowest risk or highest return (in red) Risk +++, Return + Risk +++, Return ++

  9. recommendations for further R&D • concentrate on (pushed) NbTi and Nb3Snquadrupole 1st options • extend study of detector-integrated dipoles & quadrupoles • optimize long-range beam-beam compensators & demonstrate their feasibility

  10. combination of tools • new low-b quadrupoles need to be complemented by wire compensator, by D0, or by small-angle crab cavityin order to realize a significant gain in luminosity! • D0 is efficient for much smaller b* and for higher beam current • wire compensator is efficient mainly for higher beam current • crab cavity allows for larger separation at 1st parasitic encounters if D0 is used

  11. IR upgrade: recommendations • quadrupole 1st is preferred: less demanding development; optimal layout under investigation • NbTi & Nb3Sn & hybrid solutions • incentive to develop high-gradient large-aperture quadrupoles • investigations to minimize chromaticity and impact on field quality • pursue D0 and Q0 • wire compensation & small angle crab cavities

  12. “forward-looking baseline scenario” we propose choosing a hybrid scheme as suggested by Tom Taylor where one (or two) quadrupole(s) per triplet is (are) made from Nb3Sn, and the others from NbTi

  13. beam parameter sets • old Lumi’05 upgrade parameters raised concern about electron cloud or pile up • recently we constructed several additional upgrade parameter sets, inspired by Jim Virdee, Jean-Pierre Koutchouk, and Roland Garoby • for the new sets both electron cloud and pile up appear acceptable, and the strain is put elsewhere

  14. LUMI’05

  15. +LUMI’06

  16. Beam parameters • new parameter sets with acceptable electron cloud & increased pile-up events • 25 ns spacing ultimate beam with low b* - may need D0 and small-angle crab cavities • 50 ns spacing long bunches – may need wire compensation • ( 25-ns large emittance & 12.5 ns short bunches imply unacceptable heat load -> revisit them only if there will be bunch current limitations)

  17. Conclusion on injector upgrade • Intensity limitations in the PSB and in the SPS • The LINAC4 will mitigate the space-charge in the PSB • PS2/PS2+ should be successor of PS: reliability & availability, well advanced technology • optimum extraction energy, layout, & other parameters to be determined (to mitigate the SPS intensity limitations, ion acceleration, nu-physics) • PS2/PS2+ is insufficient (other measures in SPS) • Comparison PS2/PS2+ needed (eventually launch s.c. magnet R&D: superferric and 3.5-4.5 T, 2 T/s rate) • superferric LER in SPS to be investigated (mitigate intensity limitations in the SPS by RF stacking in LER) • studies on space-charge compensation (e-lens) ?

More Related