G. Rumolo, G. Iadarola, H. Bartosik, G. Arduini for CMAC#6, 16 August 2012 Many thanks to: V. Baglin, G. Bregliozzi, S. Claudet, O. Dominguez, J. Esteban-

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Presentation transcript:

G. Rumolo, G. Iadarola, H. Bartosik, G. Arduini for CMAC#6, 16 August 2012 Many thanks to: V. Baglin, G. Bregliozzi, S. Claudet, O. Dominguez, J. Esteban- Müller, B. Goddard, W. Höfle, V. Kain, F. Roncarolo, E. Shaposhnikova, L. Tavian, F. Zimmermann Experience with 25ns beams in the LHC and future perspectives

Focus of the talk  Review our present knowledge on electron cloud in the LHC with 25ns beam & anticipate future operation  25ns tests in the LHC in 2012  SEY evolution  Scrubbing runs and operation after LS1  Required yearly scrubbing time 2

Commissioning with beam 03/04 14/03 Physics run 50ns 11/ /08 3 Commissioning with beam 13/03 05/04 75ns physics run (nominal) 12/04 21/02 Scrubbing run 50ns Physics run 50ns 30/10 29/06 26/ /10 25ns MDs (nominal) Milestones of 25ns beam in the LHC /07 25ns MDs (nominal) Scrubbing run 25ns /10 25/0927/ /12

25ns TESTS in 2012 and SEY EVOLUTION

Beam 1 Beam injection tests (10 July 2012) Bunch-by-bunch intensity Beam 1 Bunch-by-bunch intensity Beam 2

6 Some electron cloud observables during the injection tests on 10 July 2012 ⇒ Dynamic pressure rise ⇒ Bad lifetime and degrading transverse emittances towards the tail(s) of the batches ⇒ Heat load in the arcs

7 Some electron cloud observables during the injection tests on 10 July 2012 ⇒ Dynamic pressure rise Mainly in common areas and never above the interlock value of 4e-7 mbar ⇒ Bad lifetime and degrading transverse emittances towards the tail(s) of the batches ⇒ Heat load in the arcs

8 Some electron cloud observables during the injection tests on 10 July 2012 ⇒ Dynamic pressure rise ⇒ Bad lifetime and degrading transverse emittances towards the tail(s) of the batches ⇒ Heat load in the arcs

10/07/12 12h55 Beam 1 Beam 2 Beam 1 Beam 2 Beam evolution and emittances BSRT Snapshots → Up to 4x emittance growth for both beams → Affecting last bunches of batches → Affecting especially the vertical plane

10 Some electron cloud observables during the injection tests on 10 July 2012 ⇒ Dynamic pressure rise ⇒ Bad lifetime and degrading transverse emittances towards the tail(s) of the batches ⇒ Heat load in the arcs

Simulation points 10/07/12 12h00-12h15 10/07/12 12h45-13:00 →A clear increase in the heat load was measured in the arcs →This is due to Electron Cloud + Synchrotron Radiation + Image Currents Heat load

12 29/0607/ /1014/10 Six snapshots from the 25ns MDs to reproduce the measured heat load by PyECLOUD simulations! Flashback on 2011 (see Chamonix 2012) Beam 1 Beam 2 Energy Heat load averaged sector by sector [x 10 mW/m/beam]

→  max decreased from the initial 2.1 to 1.52 in the arcs after approximately 50h machine time with 25ns beams in 2011 (injected nominal and degraded) →It was found to be slightly higher (1.65) in 2012, but it has already decreased to 1.55 at the end the injection tests (4h beam time, 1h between measurements) Scrubbing history of LHC arcs 25ns GeV 25ns TeV 29/06 07/ /1014/10 50ns 10/07/2012 3w p operation (50ns) ions + Winter shut-down + 3m operation (50ns) hours  max

Beam 1 Beam 2 ⇒ Deterioration in SEY confirmed by worse beam lifetime July 10, 2012 Beam 2 - October 24, 2011 Beam observations

SCRUBBING RUNS in 2012 and AFTER LS1

Scrubbing run in MDs 16 ⇒ Need to further lower the SEY in the arcs from the presently estimated value of 1.55 – Effect of the filling pattern on scrubbing efficiency – Effect of bunch intensity →Scrubbing dose →Beam stability – MDs: Ramping a stable beam configuration to high energy →Photoelectrons →Lower SEY thresholds for (significant) e-cloud build up 25 Sep 26 Sep 27 Sep ⇒ The 2012 scrubbing run is scheduled on 25–27 September 2012 −Continue scrubbing of the machine for 25ns beams and enable MDs using these beams before LS1 −Validate the scrubbing procedure and establish a strategy for operation with 25ns beams after LS1 ~1.45 ~1.55

Effect of filling scheme Trains of 72 Trains of 144 Trains of 216 Trains of 288

Ideal bunches Effect of filling scheme → Scan in SEY at nominal bunch intensity Degraded bunches (as from last fill)

Effect of bunch intensity → Scan in bunch intensity at SEY max =1.55 Max scrubbing 8 x ppb (however, only 10% larger than at 1.3 x ppb) Threshold value for electron cloud build up Heat load 20% lower than at 1.3 x ppb

Effect of bunch intensity → Scan in bunch intensity at SEY max =1.55 Electron distribution in the dipole chamber: – The central density is higher for lower intensities – The two stripes move further out with higher intensities Lower intensity beams also tend to be more unstable due to larger central densities they generate All in all, it seems better to use higher intensities and move the beam radially to better scrub the central part Electron distribution

Effect of beam energy → Ramping to 4 TeV during MDs A few concurrent effects at top energy: – More production of photoelectrons causes higher electron densities (lower SEY threshold, ~1.37) and larger heat loads +Due to the shorter bunches, the central peak in the electron distribution is less pronounced +The beam is more rigid and generally more stable against coherent mechanisms (even with low chromaticity) Scrubbing the LHC at injection energy with filling patterns based on long bunch trains should give enough margin to ramp up a non-degraded beam with shorter trains Then the scrubbing process will continue thanks to photoelectrons

Scrubbing runs after LS1 22 ⇒ Rough time estimate for first scrubbing run after LS1 (2014) − ~50h = 2 days machine time, as was needed in 2011, to lower  max from 2.1 to 1.55 (including set up of all injection steps, bunches) −An additional 20h net beam time with 2100 bunches to get to 1.45 (scrubbing limit at flat bottom), estimated with a simple model (Chamonix 2012) = 6 days machine time (applying scrubbing factor from 2011 = 0.14) −At least 4 days machine time for operation & further scrubbing at 7 TeV with increasing number of bunches (perhaps gradually including ramps at intermediate energies?) −Total of 12 days with very good machine availability and no contingency ⇒ Scrubbing scenarios could also foresee a staged approach – First, “light” scrubbing with 25ns beams (few to allow a period of electron cloud free operation with 50ns and intensity ramp up. Then, full scrubbing for 25ns operation ⇒ In subsequent years, scrubbing should go much faster because, in absence of venting, de-conditioning is weak and re-conditioning much faster Much to be yet validated with the 2012 scrubbing run + MDs with ramp to 4TeV 2 days 6 days 4 days

Effect of beam energy → Ramping to 7 TeV after LS1 with different filling patterns Due to photoelectrons: – Threshold behaviour much less sharp than at injection – Effect of filling pattern only visible due to the different number of bunches (memory between batches is irrelevant) The absolute value of the scrubbing efficiency and heat load strongly depend on the reliability of our photoemission model Still relatively high scrubbing efficiency and heat load well below 200 W/hcell Scrubbing efficiency

Effect of beam energy → Ramping to 7 TeV after LS1 Differences with injection energy: – Strong peak where the SR hits directly – Lower SEY threshold value for stripe formation – Much less pronounced central spike (effect of bunch length) Stripes in the same position  benefits from + more scrubbing possible Beam is more stable (low central density, higher energy) Electron GeV

Summary and conclusions 25 ⇒ The electron cloud still affects 25ns beams in the LHC −SEY has come down to 1.55 and needs further lowering −There is a slight effect of de-conditioning between runs, but re-conditioning appears to be faster ⇒ Scrubbing runs are needed to be able to run LHC with 25ns beams for possible future operation (after LS1) – 2012 →Scrubbing run (3d) important to continue acquiring experience on operation with 25ns and scrubbing procedures →MDs with ramps to 4 TeV important to learn experimentally how the electron cloud effects behave with energy (and validate our models for extrapolation to 7 TeV) – After LS1 →First scrubbing run might have to be long to recover acceptable SEY conditions (~12d) →Future scrubbing runs should be shorter in absence of venting

SPARE SLIDES

25ns experience in 2011 DATESHORT DESCRIPTION 29 JuneInjections of 9 x 24b trains per beam with different spacings between them 26 AugustTwo attempts to inject a 48b train with damper on and off: fast instability dumps the beam within 500 turns in both cases (SBI and CBI) 7 OctoberHigh chromaticity (Q’ x,y ≈15): Injection tests with trains of bunches from the SPS + ramp to 3.5 TeV & 5h store with 60b ( ) per beam 14 OctoberHigh chromaticity: injection of up to 1020 bunches per beam in 72b trains (decreasing spacings between trains at each fill: 6.3–3.2–1  s) October Injection of up to 2100 bunches in Beam 1 and 1020 in Beam 2 (1  s train spacing) Scrubbing 29/0607/ /1014/10 Beam 1 Beam 2 Energy

28 Measured heat load Total simulated heat load fastBCT + bunch-by- bunch b-length (B1) fastBCT + bunch-by- bunch b-length (B2) Simulator PyECLOUD  max in the arcs: estimation technique R 0 =0.7, scan in  max E max =330 eV

Commissioning with beam 03/04 14/03 Physics run 50ns 30/ /08 29 Commissioning with beam 13/03 05/04 75ns physics run (nominal) 12/04 21/02 Scrubbing run 50ns Physics run 50ns 30/10 Nominal: 1.1 x ppb 2.5  m 29/06 26/ /10 25ns MDs (nominal) Milestones of 25ns beam in the LHC /07 25ns MDs (nominal) Scrubbing run 25ns /10 ?? 25/0927/09

10/07/12 11h49-12h00 Beam 1 Beam 2

Scrubbing run in ⇒ The 2012 scrubbing run is scheduled on 27–29 September 2012 −Continue scrubbing of the machine for 25ns beams and enable MDs using these beams before LS1 −Validate the scrubbing procedure and establish a strategy for operation with 25ns beams after LS1 ⇒ Need to further lower the SEY in the arcs from the presently estimated value of 1.55 – Effect of the filling pattern on scrubbing efficiency – Effect of bunch intensity →Scrubbing dose →Beam stability – Ramping to high energy (probably to be done in MDs after the scrubbing run) →Photoelectrons →Lower SEY thresholds for e-cloud build up ⇒ After 2012 scrubbing + 25ns studies in MDs, we will have collected enough data to predict the evolution of the LHC performance with 25ns beams.