LHC Beam Operations Past, Present and Future Maria Kuhn on behalf of the LHC team 03-14-2013 Moriond QCD 2013 August 2008 First injection test August, 2011 November 29, 2009 2.3 x 1033, 2.6 fb-1 1380 bunches Beam back 4 July, 2012 September 10, 2008 Higgs like discovery June 28 2011 First beams around October 14 2010 April 2010 1 x 1032 248 bunches 1380 bunches 1380 6 June, 2012 6.8 x 1033 Squeeze to 3.5 m 2008 2009 2010 03-14-2013 Disaster Accidental release of 600 MJ stored in one sector of LHC dipole magnets 2012 November 2010 Ions March 30, 2010 September 19, 2008 2011 First collisions at 3.5 TeV 18 June, 2012 6.6 fb-1 to ATLAS & CMS Moriond QCD 2013 LHC Timeline 2 Integrated luminosity 2010-2012 03-14-2013 Moriond QCD 2013 3 Peak luminosity 2010-2012 2011: average 12 collisions/xing, with tails up to ~20 Record peak luminosity: 7.73 x 1033cm-2s-1 2012: ~30 collisions/xing at beginning of fill with tails up to ~ 40. ALICE and LHCb (and TOTEM and ALFA) LHCb 2012: 1.9 fb-1 delivered! Peak luminosities achieved in ALICE around 5 x 10 30cm-2s-1 03-14-2013 Moriond QCD 2013 5 Luminosity N kb f N kb f g L= F = F * * * 4ps xs y 4pen b 2 2 N Number of particles per bunch Kb Number of bunches f Revolution frequency s = be * σ* Beam size at interaction point F Reduction factor due to crossing angle ε Emittance εn Normalized emittance β* Beta function at IP 03-14-2013 Moriond QCD 2013 * In 2012: εn = 2.5 mm e = 5.9 x 10-4 mm s* = 18.8 mm (p = 4 TeV, b* = 0.6m) 6 Performance from injectors 2012 Design report injected into LHC tested Bunch spacing [ns] Protons per bunch [ppb] Norm. emittance H&V [mm] Exit SPS 25 1.15 x 1011 3.5 50 1.7 x 1011 1.8 25 1.2 x 1011 2.7 N.B. the importance of 50 ns in the performance so far. This at the expense of high pile-up. 03-14-2013 Moriond QCD 2013 7 LHC Peak Performance in 2012 Design Report 2012 Energy [TeV] 7.0 4.0 4/7 design energy b* (IP1&IP5) [m] 0.55 0.6 exploiting available aperture, tight collimator settings, stability 25 50 2808 1374 Bunch spacing [ns] Number of bunches Comments Half nominal number of bunches, given by 50 ns Bunch intensity [ppb] 1.15 x 1011 Normalized emittance [mm] 3.75 at collision ~2.5 at collision again remarkable injector performance (but emittance preservation challenges in LHC) Peak luminosity [cm-2s-1] 1.0 x 1034 7.73 x 1033 77 % of design luminosity 03-14-2013 1.6 – 1.7 x 1011 150 % of nominal Moriond QCD 2013 8 WHAT WE HAVE LEARNT SO FAR… 03-14-2013 Moriond QCD 2013 9 In general – beam & optics • Excellent single beam lifetime – vacuum • Excellent magnetic field quality • Beam-Beam – Head-on is not a limitation • Collective effects! – Single and coupled bunch instabilities • Better than expected aperture • b* reach established and exploited – Not trivial: small beams at the IP means large beams at the triplets! 03-14-2013 Moriond QCD 2013 10 Operational robustness - LHC cycle Pre-cycle Injection 450 GeV Ramp Squeeze Collide • Altogether good lifetime throughout the whole LHC cycle • Machine remarkably reproducible – optics, orbit, collimator set-up, tune… 03-14-2013 Moriond QCD 2013 11 2012 Machine protection – the challenge met Beam 140 MJ 11 magnet quenches at 450 GeV – injection kicker flash-over Not a single beaminduced quench at 4 TeV Can’t over stress the importance of this to the success of the LHC (so far). From commissioning to real confidence in under two years. 3-12-2012 LHC status - Kruger R. Assmann 12 Availiability 03-14-2013 Alick Macpherson Moriond QCD 2013 13 Machine performing well, huge amount of experience & understanding gained. Good system performance, excellent tools, reasonable availability following targeted consolidation. This is the legacy for post LS1 03-14-2013 Moriond QCD 2013 14 LS1 03-14-2013 Moriond QCD 2013 15 03-14-2013 Moriond QCD 2013 16 LHC MB circuit splice consolidation proposal Phase Phase III PhaseIII Insulation between Application bus of bar clamp and of to and ground, busshunts barLorentz insulation force clamping Installation new 03-14-2013 Moriond QCD 2013 27 POSSIBLE LIMITATIONS FOR POST LS1 03-14-2013 Moriond QCD 2013 18 25 ns & electron cloud • Photoelectrons from synchrotron radiation accelerated by the proton beam • Electrons bounce into chamber wall → secondary electrons are emitted • Due to short bunch spacing, high bunch intensity and low emittance: electron cloud build-up! 03-14-2013 Moriond QCD 2013 19 Electron cloud: possible consequences • • • • • • single-bunch instability multi-bunch instability emittance growth gas desorption from chamber walls heat load particle losses, interference with diagnostics,… Electron bombardment of a surface has been proven to reduce drastically the secondary electron yield (SEY) of a material. This technique, known as scrubbing, provides a mean to suppress electron cloud build-up and its undesired effects 03-14-2013 Moriond QCD 2013 20 Total intensity [p] 2.5 2 1.5 25 ns & electron cloud 1 0.5 The SEY evolution significantly slows down during the last scrubbing 0 10 20 30 40 50 60 70 80 Time [h] fills (more than expected from simulations and lab. experiments) 1.6 Reconstructed comparing heat load meas. and PyECLOUD sims. SEY max 1.55 1.5 1.45 1.4 1.35 End of 2012 tests Giovanni Iadarola and team - Evian 12 10 20 30 40 50 60 70 80 Time [h] • Downside: scrubbing takes time (several weeks!) • Electron cloud free environment after scrubbing at 450 GeV seem not be reachable in acceptable time. • Post LS1 operation with high heat load and electron cloud density seems to be unavoidable. 03-14-2013 Moriond QCD 2013 21 UFOs • UFOs: showstopper for 25 ns and 6.5 TeV? – 10x increase and harder UFOs – (but no increase in low intensity fills) • UFO “scrubbing”: does it work? • Deconditioning expected after LS1 • Post LS1 operation: start with lower energy and/or 50 ns Tobias Baer 03-14-2013 Moriond QCD 2013 22 OPERATIONAL SCENARIOS AFTER LS1 03-14-2013 Moriond QCD 2013 23 Beam from injectors LS1 to LS2 Number of bunches Bunch intensity [1011 ppb] Emittance at injection [mm] Emittance in collisions [mm] 25 ns ~nominal 2760 1.15 2.8 3.75 25 ns BCMS 50 ns 50 ns BCMS 2520 1380 1260 1.15 1.65 1.6 1.4 1.7 1.2 1.9 2.3 1.6 BCMS = Batch Compression and (bunch) Merging and (bunch) Splittings Rende Steerenberg, Gianluigi Arduini, Theodoros Argyropoulos, Hannes Bartosik, Thomas Bohl, Karel Cornelis, Heiko Damerau, Alan Findlay, Roland Garoby, Brennan Goddard, Simone Gilardoni, Steve Hancock, Klaus Hanke, Wolfgang Höfle, Giovanni Iadarola, Elias Metral, Bettina Mikulec, Yannis Papaphilippou, Giovanni Rumolo, Elena Shaposhnikova,… Batch compression & triple splitting in PS 24 50 ns versus 25 ns GOOD 50 ns 25 ns • Lower total beam current • Higher bunch intensity • Lower pile-up • Smaller emittance BAD • High pile-up • Need to level • Pile-up stays high • High bunch intensity – instabilities… • Larger crossing angle; higher b* • Larger emittance • Electron cloud: need for scrubbing; emittance blow-up; • Higher UFO rate • Higher injected bunch train intensity • Higher total beam current Expect to move to 25 ns because of pile up… 03-14-2013 Moriond QCD 2013 25 b* & crossing angle • b* reach depends on: – available aperture – collimator settings – required crossing angle which in turn depends on • emittance • bunch spacing 03-14-2013 Moriond QCD 2013 26 Potential performance Number of bunches Bunch intensity [1011 ppb] b*/ crossing angle Emittance LHC [mm] Peak Luminosity [cm-2s-1] ~Pile-up Int. Lumi per year [fb-1] 25 ns 2760 1.15 55/189 3.75 0.93 x 1034 25 ~24 25 ns BCMS 2520 1.15 45/149 1.9 1.7 x 1034 52 ~45 2.5 1.6 x 1034 level to 0.8 x 1034 87 level to 44 ~40* 1.6 2.3 x 1034 level to 0.8 x 1034 138 level to 44 ~40* 50 ns 50 ns BCMS • • • • • 1380 1260 1.6 1.6 42/136 38/115 All values at 6.5 TeV collision energy 1.1 ns bunch length 150 days proton physics 85 mb cross-section * different operational model – caveat - unproven All numbers approximate27 Potential performance – in words • Nominal 25 ns – gives more-or-less nominal luminosity (1.0 x 1034 cm-2s-1) • BCMS 25 ns – gives a healthy 1.7 x 1034 cm-2s-1 – peak <m> around 50 – 83% nominal intensity • Nominal 50 ns – gives a virtual luminosity of 1.6 x 1034 cm-2s-1 with a pile-up of 87 – levelling mandatory • BCMS 50 ns – gives a virtual luminosity of 2.3 x 1034 cm-2s-1 with a pile-up of 138 – levelling even more mandatory 03-14-2013 Moriond QCD 2013 28 2015 STRATEGY – FOR DISCUSSION 10-12-12 LHC Operation 29 30 Conclusions • Availability better than might have been expected. • Machine now magnetically, optically, operationally well understood • System performance – generally good to excellent – issues identified and being addressed • Limitations well studied, well understood and quantified – still some potential implications for post LS1 operation • Restart post LS1 with 50 ns – before moving to 25 ns – non electron cloud free environment to be accepted at least initially 03-14-2013 Moriond QCD 2013 31 BACKUP 10-12-12 LHC Operation 32 Post LS1 energy • Our best estimates to train the LHC (with large errors) – 30 quenches to reach 6.25 TeV – 100 quenches to reach 6.5 TeV • Two quenches/day 2 to 5 days of training per sector • The plan – Try to reach 6.5 TeV in four sectors in March 2014 – Based on that experience, we decide if to go at 6.5 TeV or step back to 6.25 TeV in March 2014 Ezio Todesco – Chamonix 12 03-14-2013 Moriond QCD 2013 33 2015 strategy – more detailed • • • • Low intensity commissioning of full cycle – 2 months First stable beams – low luminosity Intensity ramp-up – 1 to 2 months 50 ns operation (at pile-up limit) – Characterize vacuum, heat load, electron cloud, losses, instabilities, UFOs, impedance • Options thereafter: – 1 week scrubbing for 25 ns, say 1 week to get 25 ns operational (if b* and crossing angles are changed), intensity ramp up with 25 ns with further scrubbing required – Commission levelling of 50 ns and push bunch intensity up, emittance down… not at all favored by experiments! 03-14-2013 Moriond QCD 2013 34