Mike Lamont An attempt at synthesis Acknowledgements all round

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Presentation transcript:

Mike Lamont An attempt at synthesis Acknowledgements all round Plans for 2016 and Run 2 Mike Lamont An attempt at synthesis Acknowledgements all round After LS1 “It’s going to be like after a war” Serge Claudet Evian 2012

This not a bad place to start Where are we? 1/2 6.5 TeV, 2*80 cm, 2*levelled with optics well under control Nominal 25 ns beam, 2244 bunches High electron cloud Operating with high chromaticity, octupoles, ADT throughout the cycle to combat instabilities Good transmission through the cycle Good luminosity performance - beam-beam OK Acceptable emittance growth (and enjoying sync. light) UFO rates down This not a bad place to start

Where are we? 2/2 Availability is reasonable Mature system performance QPS, RF, Cryogenics, ADT, Power converters Collimation, BI, Controls, LBDS, injection, TDI… Operational efficiency is good injection, cycle, decay and snapback, feedbacks Proven machine protection Challenges High e-cloud, UFOs, ULO, instabilities, (beam induced heating), R2E

Product lifecycle 2008 2012, 2016(?) 2011, 2015 2008 2009 2010

LHC HL-LHC FCC

Where do we want to go? Production operation Stable, safe operations Short term - 2016 Stable, safe operations Electron cloud off 6.5 TeV, 40 to 50 cm Nominal 25 ns beam, 2748 bunches, 288 bpi Reasonable availability Excellent operational efficiency Production operation

How are we going to get there? Choose a not too challenging operating regime that will allow stable and reproducible production Keep avoidable interruptions to production to a minimum (while remaining flexible) Don’t compromise: Machine safety “Remarkable cleaning stability with 6.5 TeV beam thanks to excellent machine reproducibility”

How are we going to get there? Continued improvement: incoming for 2016 Availability Sustained effort from QDS, cryogenics, circuits, power converters, LBDS, Injection, RF, Collimation… System performance across the board ADT performance monitoring, OBSBOX, Is the damper working? Operational efficiency Injection, pre-cycle, combined ramp & squeeze (Turn off electron cloud) Premature dumps BLM threshold adjustment Illustrative not encyclopedic

How are we going to get there? Continued improvement: incoming for 2016 Set-up efficiency Collimation (full validation for squeeze and collide in 1 fill) and still pushing Machine protection BCCM, Collimator BPM interlock, continued vigilance Beam performance Emittance growth, instabilities, good control of key parameters, reduction of chromaticity and octupoles, Illustrative not encyclopedic

2016 Initial beam commissioning Re-establish e-cloud conditions of 2015 Continue gentle increase in number of bunches at the heat-load limit Exploit

Initial commissioning System commissioning Transverse damper RF Beam instrumentation Feedbacks Injection, beam dumps Beam based measurements Optics meas. & correction Magnet model meas. & correction Aperture measurements

Initial commissioning++ Detailed breakdown by Belen at Evian Shouldn’t hold too many mysteries – 4 weeks should be OK Squeeze to 40 cm – check local aperture etc. Combined ramp and squeeze Characterize shortened pre-cycle Check out the ULO Check impedance of TDIs Commission additional interlocks Set-up TOTEM’s Roman Pots Prep for special runs: VdM (19 m), 2.5 km

Scrubbing and intensity ramp-up Re-establish 2012 ~2000 bunches conditions during dedicated 4 day run (450 GeV) Intensity ramp-up (288b) phase 1: below the heat load limit remedial scrubbing as required 3-12-48/72-288-570-860-1200-1700 ~7 steps – let’s say 3 days per step – 3 weeks Phase 2: (maximal) scrubbing during Stable Beam ~2000 to 2748 Small increments in number of bunches (“mini-steps”) playing on batch gap High Q’, octupoles, ADT, longer bunches, WP etc. Giovanni Iadarola

2016 Q1/Q2 (v1.1)

2016 Q3/Q4 (v1.1) Timing of MD2, floating MD, special runs to be determined

2016 version 1.1 Phase Days Initial Commissioning 28 Scrubbing: 4 days initially and then as required during ramp-up 7 Proton physics 25 ns 152 Special physics runs (high beta*; VdM) 8 Machine development 22 Technical stops 15 Technical stop recovery 6 Ion setup/proton-lead run 4 + 24 Total 266 days (38 weeks)

2016 beam parameters (nominal 25 ns) Energy 6.5 TeV Bunch spacing 25 ns Bunch population ~1.25e11 Max bunches/injection 288 Max. number bunches 2748 Nc GPDs 2736 Emittance exit SPS 2.7 mm.mrad Emittance into SB 3.4 mm.mrad Beta* GPDs 40 or 50 Crossing angle GPDs 185 or 165 Note the limit of around 1.3e11ppb from the SPS - see Verena’s talk

Integrated luminosity Fit 2015 post-TS2 greater than 459b Stable Beam distribution September 8th to 3rd November 52 days (90 m run taken out), 381 hours of Stable beam, ~31% physics efficiency * L(t) input initial luminosity, luminosity lifetime from burn Scale to 150 days (implies same availability, turnaround) Dump fill after 18 hours

40 versus 50 cm 40 cm 50 cm Beam size at IP (um) 14.2 15.9 Assume Nc = 2736, 3.5 micron, 1.2e11 ppb, 1.25 ns 40 cm 50 cm Beam size at IP (um) 14.2 15.9 Crossing angle (urad) 185*2 165*2 F (bunch length: 1.25 ns) 0.63 0.72 Peak luminosity (cm-2s-1) 1.1e34 1.0e34 Burn-off lifetime (hour) 25.8 28.5 Integrated per 150 days (fb-1) 33.2 30.7 Availability? Aperture? Interlocks? Phase advance?

Courtesy Steve Hancock from 2012

BCMS Is clearly interesting (see Run 2 below) 2015: one attempt – emittance blow-up to something similar to nominal Possible stability issues with low emittance Explore possibilities with “tuned” BCMS controlled emittance blow-up in injectors To be pursued when e-cloud settles down Bunch population < 1.3e11 Max bunches/injection 144 No colliding bunches GPDs 2448 Emittance exit SPS 1.9 um Emittance into SB 2.4 um Kevin Li et al

Run 2 EYETS – Extended Year End Technical Stop – 19 weeks – CMS pixel upgrade Assume machine stays cold during EYETS Assume for the moment: p-Pb end 2016, Pb-Pb end 2018 – see Jamie

Run 2 - objectives Deliver 100+ fb-1 to GPDs, keep ALICE, LHCb, TOTEM and ALFA happy Keep pushing performance and availability Now we’ve got the machine sorted out for Run 2 we can concentrate on the HL-LHC Look forward to HL-LHC without compromising present performance: ATS, beta* levelling, LRBB compensation, full de-tuning… Look forward to the post-LS2 LIU era and how to exploit the potential Prepare for (or go to) 7 TeV operation

2017

2017 version v0.1 Phase Days Initial Commissioning post EYETS 28 Scrubbing (assuming machine stays cold) 7 Proton physics 25 ns 163 Special physics runs 8 Machine development 15 Technical stops 10 Technical stop recovery 4 Total 235 days (34 weeks) Machine development scaled down Might debate: initial commissioning; start of YETS17-18

2018

2018 version 0.2 Phase Days Initial Commissioning 21 Scrubbing 4 Proton physics 25 ns 162 Special physics runs 8 Machine development 22 Technical stops 15 Technical stop recovery 6 Ion setup/ion run 4 + 24 Total 266 days (38 weeks)

Peak performance increase? Turn off electron cloud BCMS Injector optimization PSB to SPS Emittance conversation in LHC Novel optics… flat beams, squeezing further Reduced crossing angle (LRBB limits) Maximizing number of bunches 12b, SPS injection, PS – 80 bunches E-cloud should come as a matter of course, the others need to be actively pursued

Possible 2017/18 parameters Nominal BCMS Beta* (1/2/5/8) 0.4/10/0.4/3 Half crossing angle -185/200/185/-250 -155/200/155/-250 Nc 2736 2448 Proton per bunch 1.25e11 Emittance into SB 3.2 2.3 Bunch length 1.25 Peak luminosity ~1.3e34 ~1.6e34 Peak pile-up ~33 ~47 Luminosity lifetime ~23 ~17 150 days 38 fb-1 43 fb-1 Peak luminosity limited to ~1.7e34 by inner triplets (Laurent Tavian Evian 2012) Illustrative! All usual caveats apply

Conclusions Looking good for 2016 On the back of experience and a huge amount of effort across the board - should be entering the exploitation domain Clear priority to get e-cloud scrubbed Known unknowns: ULO, earth faults… Been operating the LHC for long enough not to worry about unknown unknowns Enthusiasm and commitment remains high – we could do some serious stuff in 2017 & 2018