Technological Challenges for the LHC Upgrade Ingrid-Maria Gregor, - - PowerPoint PPT Presentation

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Technological Challenges for the LHC Upgrade Ingrid-Maria Gregor, - - PowerPoint PPT Presentation

Technological Challenges for the LHC Upgrade Ingrid-Maria Gregor, DESY a detector physicists view . LISHEP2011 Interna0onalSchoolofHEP RiodeJaneiro,Brazil July9,2011 100 Outline The LHC (current status)


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Technological Challenges for the LHC Upgrade

Ingrid-Maria Gregor, DESY

LISHEP
2011

Interna0onal
School
of
HEP

Rio
de
Janeiro,
Brazil July
9,
2011 … a detector physicists view ….

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

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Outline

Lately inside the LHC 2 protons 0.000000000000000000001 sec before collision

Apologies for the many interesting topics I didn’t cover!

The LHC (current status) Future Plans Overview Beam parameters and what they mean Beam Intensity Higher Field Magnets Luminosity Leveling Crab Cavities Conclusions

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Ingrid-Maria Gregor, DESY: The EUDET Telescope - at DESY and CERN

The LHC (current status)

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

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The CERN accelerator complex

LEP e+e- (1989-2000) 104 GeV/c per beam LHC pp and ions 7 TeV/c per beam 26.8 km length 8.3 Tesla superconducting magnets

Switzerland Lake Geneva France LHC accelerator

(100m below surface) SPS accelerator

CMS ALICE LHCb ATLAS CERN

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

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LHC Accelerator

Last magnet: April 26th 2007

27 km circumference 8500 of 8.4T dipole magnets Cooled to 1.9K with 140 tons of liquid helium Energy of one beam = 362 MJ Kinetic energy of a 747 at take off

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

LHC challenges

The LHC surpasses existing accelerators/colliders in many aspects : The energy of the beam of 7 TeV that is achieved within the size constraints of the existing 26.7 km LEP tunnel. LHC dipole field 8.3 T HERA/Tevatron ~ 4 T The luminosity of the collider that will reach unprecedented values for a hadron machine:

LHC pp ~ 1034 cm-2 s-1 Tevatron pp 3x1032 cm-2 s-1 SppS pp 6x1030 cm-2 s-1

Very high field magnets and very high beam intensities: Operating the LHC is a great challenge. There is a significant risk to the equipment and experiments. A factor 2 in field A factor 4 in size A factor 30 in luminosity

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

7 based on graph from R.Assmann

Livingston type plot: Energy stored magnets and beam Potential equipment damage in case of failures during operation.

Beam Power

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

CERN Accelerator Complex

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Year Top energy [GeV] Length [m] Linac PSB PS SPS LHC 1979 0.05 30 1972 1.4 157 1959 26.0 628 1976 450.0 6911 2008 7000.0 26657

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

LHC Start Up

2008

Accelerator complete Ring cold and under vacuum 10.09: First beams around 19.09: Accident

2008 –2009

14 months of major repairs and consolidation NewQuench Protection System for online monitoring and protection of all inter-magnet joints But: uncertainties about the splice quality (copper stabilizer) Risk of thermal runaway scenarios => decision to limit beam energy to 3.5 TeV for first operation 20.11. Restart LHC at 1.18TeV 29.11: Both beams accelerated to 1.18 TeV simultaneously -> LHC Highest Energy Accelerator

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  • O. Brüning et al.

2010

19.03 Ramp to 3.5 TeV Collisions at 3.5+3.5 TeV LHC Reaches target energy for 2010/2011

2011

22.04: LHC sets world record beam intensity record broken almost on daily basis more Tops recorded than Tevatron …..

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Current Status

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https://twiki.cern.ch/twiki/bin/view/AtlasPublic/ LuminosityPublicResults#2011_pp_Collisions LHC Design July 2011

Momentum at collision [TeV/c] 7 3.5 Luminosity [cm-2s-1] 1.00E+34 1.26E+33 Number of bunches per beam 2808 1380 Bunch intensity 1.15E+11 1.25E+11

The performance of LHC is excellent Within a few months the goal for the year 2011 was reached: 1fb-1 ! Hopes are up to reach 5 fb-1 in 2011...

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Ingrid-Maria Gregor, DESY: The EUDET Telescope - at DESY and CERN

Future Plans Overview

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Physics reason for an upgrade

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  • L. Rossi

Operation at even higher luminosity has three main purposes:

Perform more accurate measurement on the new particles discovered in the LHC Observe rare processes (predicted or newly discovered) with rates below the current sensitivity Extend the exploration of the energy frontier, extending the discovery reach by probing rare events. Besides the with to increase the luminosity there are some more technical reason: Radiation damage limit of IR quadrupoles ~400/fb ->~2020 this limit will be reached Hardware and shielding has not really been optimized for very high radiation Necessity to increase the heat removal capacity Restoring cooling capacity in IR5 left and decouple RF from magnets

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

How the luminosity might evolve

  • Int. Lumi by end of 2020:

220 fb-1 Or (positive assumption to reach L= 2·1034) 300 fb-1

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  • E. Todesco
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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC 14

  • E. Todesco

How the luminosity might evolve

Error halving time (years)

Even with a terrific machine, at some point the time to accumulate enough statistics to reduce the error bands is getting very high -> an upgrade is needed!

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Future plans for LHC (“Chamonix 2011”)

Run until end of 2012 constantly improvements of the beam parameters (i.e. bunch spacing) Shut down for ~15 month to fully repair all ~10000 joints (non superconducting between SC magnets)

Resolder, install clamps …. Tie in LINAC4 (high intensity)

Shut down in 2018

collimation upgrade (dispersion suppressors) preparation for crab cavities & RF cryosystem detector upgrades

Shut down in ~2021

Full luminosity: 5x1034 leveled New inner triplets based on Nb3Sn Crab cavities

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Ingrid-Maria Gregor, DESY: The EUDET Telescope - at DESY and CERN

Understanding the Beam Parameters

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“So to achieve high luminosity, all one has to do is make high population bunches of low emittance to collide at high frequency at locations where the beam optics provides as low values of the amplitude functions as possible.” PDG 2010, chapter 25

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Beam Parameter Overview

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Parameter Unit nominal upgrade Energy [TeV] 7 Protons/Bunch [1011] 1.15 1.7 Bunch Spacing [ns] 50…25 50…25 εn (x, y) [μm] 3.75 3.75 σz (rms) [cm] 7.55 7.55 Bunch Length (4 σ) [ns] 1.0 1.0 Longitudinal Emittance [eVs] 2.5 2.5 β* at IP1, IP5 [m] 0.55 0.25…0.14 Betatron Tunes {64.31, 59.32} {64.31, 59.32} Piwinski parameter: 0.65 1.4…2.5 BB Parameter, ξ , per IP 0.003 0.005…0.008 Crossing‐angle: θc [μrad] 285 315…509 Main RF [MHz] 400 400 Crab RF [MHz] 400 Peak luminosity w/o crab cavity 1034 cm‐2s‐1 1 3.3…3.8 Peak luminosity with crab cavity 1034 cm‐2s‐1 1.2 5.8…10.3 Pile up events per crossing 19 44…280

?

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σ =

  • β⋆ǫ

β⋆

ǫ

L = frev n1n2 4πσxσy n1n2 = nBNB

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Understanding LHC Luminosity

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n1 n2 Interaction Region area A with is the beam envelope at the IP; determined by the magnet arrangement and powering beam emittance (the extent occupied by the

particles of the beam in space and momentum phase space as it travels)

area A for a bunched beam luminosity “head on collision”

Beta function

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L =

  • γfrev

  • nbNb

β⋆

  • Nb

ǫN Rφ

  • θc

σz σx

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Understanding LHC Luminosity

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Angle at IP to avoid that the bunches collide in other places that the IP Crossing angle reduces luminosity “Piwinski parameter” effective cross section Piwinski parameter describes the effect that the crossing angle is affecting the beam dynamics The shorter the bunches ( ) the smaller is the effect

  • B. Holzer

σz

Geometry factor 2 2

effective cross section

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Understanding Luminosity

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L =

  • γfrev

  • nbNb

β⋆

  • Nb

ǫN Rφ

  • Total beam current.

β* Brightness Geometry Factor Number of bunches Energy

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Ingrid-Maria Gregor, DESY: The EUDET Telescope - at DESY and CERN

Collimation

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LHC Collimation

Provide passive protection against irregular fast losses and failures. Provide cleaning for slow losses in the super-conducting environment. Manage radiation impact of beam loss. Minimize background in the experiments.

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LHC has almost 100 collimators and absorbers. Alignment tolerances < 0.1 mm to ensure that over 99.99% of the protons are intercepted. The presently installed LHC collimation system provides

  • ptimum robustness but its performance is limited to a

beam intensity of 40% with respect to nominal. beam 1.2

http://indico.cern.ch/conferenceDisplay.py?confId=139719

At higher energies collimation gets harder!

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Aperture and collimation

Primary 6 σ Secondary 8.8 σ Dump Protection 10.5 σ Tertiary 15 σ Triplet 18 σ

With collisions the aperture limit of the LHC is in the strong focusing quadrupoles (triplets) that are installed just next to the experiments.

Hierarchy of collimators must be preserved in all phases to avoid quenching super- conducting magnets and for damage protection. β* is presently limited to 3.5 m by aperture and tolerances.

Collimation hierarchy Exp.

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

LHC Collimation System

Limited in LHC by collimation system to ~ 20% at 3.5TeV Under certain assumptions on loss rates, imperfections Injectors can deliver nominal beams With experience assume that LHC can Move to tight collimator settings Improve loss rates Get the imperfection factor down

✦ Should allow to push to higher intensities (to ~40% nominal)

Then need to install something more Collimators in the cold regions of the machine in 2012 Using “missing magnet” space in the dispersion suppressors Requires moving magnets in LSS3 and LSS7 (24 magnets each) Should allow us to get to nominal intensity at 7TeV Phase II collimators installed in 2018

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H-LHC change in layout in the IR

Dispersion suppressor Matching section Separation dipoles Final focus

Today: 6x3 m x1.5 T; h=80 mm HL-LHC: 1x4 m x 7 T; Ø=150 mm Today: Two-in-One Ø =56 mm; 4.2K HL-LHC: Two-in-One Ø70 mm; 1.9 K Today: Q4 Two-inOne Ø=70 mm, 4.2 K; D2 ↑↑ 9 m x 3.5 T, 4.2 K HL-LHC: Q4 Two-in-One Ø=90 mm, 1.9 K; CRAB CAVITY; D2 ↑↑ 9 m x 5 T; 1.9 K Today MQX: 4 x 6 m, Ø=70 mm; HL-LHC MQX: 4 x 8 m x; Ø=150 mm

CMS

  • L. Rossi
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Ingrid-Maria Gregor, DESY: The EUDET Telescope - at DESY and CERN

Higher Field Magnets

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Critical technologies: Magnets

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  • L. Rossi

Super conducting magnets beyond 10 tesla of accelerator qualities.

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Motivation for Nb3Sn

Nb3Sn can be used to increase aperture/gradient and/or increase heat load margin, relative to NbTi Nb3Sn allows higher current at higher B-fields

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Technical challenges:Nb3Sn is difficult material

Requires high temperature coil reaction after winding Materials compatibility (coil parts, insulation) Thermal expansion differentials (more critical for long magnets) Need to prevent degradation under stress Progress in Nb3Sn current density rapidly translated in record field dipoles Since ~2003, the critical current density

  • f Nb3Sn wires has been stable
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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

11 T LHC dipole

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Here cryo-collimators could be accomodated For HL-LHC the collimation needs to be improved, but no space is available replace 8T magnets (rather long) by 11 T magnets will gain space for collimation 11T magnets are under development within HL- LHC (in collaboration with Fermilab)

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Ingrid-Maria Gregor, DESY: The EUDET Telescope - at DESY and CERN

Beta*

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

The need for new quadrupoles

The minimum β* is limited by the aperture of the triplets at the IP and also by the chromatic aberations introduced by the very tight squeeze Small β*⇒huge β at focusing quad Need bigger quads to go to smaller β*

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Existing quads

  • 70 mm aperture
  • 200 T/m gradient

Proposed for upgrade

  • At least 120 mm aperture
  • 200 T/m gradient
  • Field 70% higher at pole face

⇒ Also beyond the limit of NbTi -> Nb3Sn

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

High Field Quadrupole (LARP)

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US-LARP is engaged in the production of a model by 2013 (4...6 m length) for the decision on the technology to be used (Nb3Sn vs. Nb-Ti) 120 mm aperture and 200 T/m gradient Testing first 1m long prototype High Field Quadrupole HQ (120 mm aperture, 1 m long) Achieved >155 T/m gradient in first test, at 4.5K Already above NbTi intrinsic limit at 1.9K First quench >150 T/m in second test Several coil failures due to insulation & conductor damage Traced to high compression during coil fabrication New & more challenging design - requires

  • ptimization

The Nb3Sn development plan aims at demonstrating readiness for a technology decision and construction initiation in 2014

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SQ SM TQS LR LQS-4m HQ TQC

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  • L. Rossi

LARP (US LHC program) Magnets

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Ingrid-Maria Gregor, DESY: The EUDET Telescope - at DESY and CERN

Luminosity Leveling

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Luminosity leveling

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see e.g. J.P.Koutchouk, Cham. 2010)

L ∝ 1 β∗

  • 1 + θ2

cσ2 z

4β∗ǫ

Three possibilities in LHC, specific to crossing at an angle (no yet decided):

Leveling via dynamic beta* adjustments

no additional hardware necessary, but is probably complex to implement but is cheap.

Leveling via dynamic bunch length adjustments

no or minor side effect if the beam remains stable; needed: reduction of the voltage by 16 + bunch shortening

Leveling via dynamic crossing angle adjustments

Leveling via the Xing angle appears to have the best potential (performance, complexity) but requires unexplored solutions (Crab Crossing) or some interference with detectors (Early Separation). Integrated Lumi is the same

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Ingrid-Maria Gregor, DESY: The EUDET Telescope - at DESY and CERN

Crab Cavities

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Increase peak luminosity with increasing x- angle Increase intensities and smaller emittances beyond head-on beam-beam limit Level luminosity (reduce Pile-up, radiation damage)

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Crab Crossing Restores Bunch Overlap

RF crab cavity deflects head and tail in

  • pposite direction so that collision is

effectively “head on” for luminosity and tune shift The crab cavity creates two-loop magnetic field (blue) inside to kick bunches sideway. 1st proposed in 1988, in operation at KEKB since 2007

→ world record luminosity!*

http://www.kek.jp/intra-e/feature/2010/KEKBCrabCavity.html

Example of an crab cavity creating a two-loop magnetic field

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

The challenge: a normal RF cavity requires a transverse dimension > 0.609 λ ! For 400 MHz, this means > 460 mm. The LHC beams are separated 194 mm (0.26 λ)! Something very unconventional is needed!

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Crab Cavities

  • E. Jenssen
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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Parallel bar cavity (ODU) Half wave resonator (SLAC) Four bar cavity (U Lancaster) Kota cavity (KEK)

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Ideas for Compact CC’s

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Back-up strategy: Elliptical Crab Cavities

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Retain a conventional cavity option in the unlikely event of major unforeseen ’show stopper’ with all compacts… Requires significant civil engineering costs due to needed dogleg sections in the IRs Still acceptable, in view of the importance gaining back luminosity from the crossing angle. A straightforward conventional cavity installation in IR 4 as a global scheme would serve as an alternate option in the worst case. Decision point 2015 – stop if Compact CC’s are validated! Cryostat design exists (from LARP) compatible with P4 (800 MHz)

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Ingrid-Maria Gregor, DESY: The EUDET Telescope - at DESY and CERN

Brightness

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  • Nb

ǫN

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Brightness

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LHC imposed brightness must be present from the lowest energy because brightness is (at best) conserved in a cascade of proton accelerators (Liouville’s theorem). Brightness (emittance and beam intensity) is defined in the accelerator chain before injection into the LHC. The emittance can be improved by increasing the injection energy It was decided to build a new linear accelerator at the beginning of the chain

Increasing the beam intensity by a factor of 2 Increase injection energy in the PS from 1.4 to 2 GeV, increasing the field in the PSB magnets and replacing its power supply Higher energy out of the PS gives smaller transverse emittance and beam sizes => reducing the injections losses into the SPS

Building etc. already existing

https://indico.cern.ch/conferenceDisplay.py?confId=129870

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⇒ Increase injection energy in the PSB from 50 to 160 MeV, Linac4 (160 MeV H-) to replace Linac2 (50 MeV H+) ⇒ Increase injection energy in the PS from 1.4 to 2 GeV, increasing the field in the PSB magnets, replacing power supply and changing transfer equipment ⇒ Upgrade the PSB , PS and SPS to make them capable to accelerate and manipulate a higher brightness beam (feedbacks, cures against electron clouds, hardware modifications to reduce impedance…)

Brightness

To increase reliability and lifetime (until ~2030!) (tightly linked with consolidation) ⇒ Upgrade/replace ageing equipment (power supplies, magnets, RF…) ⇒ Procure spares ⇒ Improve radioprotection measures (shielding, ventilation…)

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Linac4 PS injector, PS and SPS Beam characteristics at LHC injection

2011 - 2012

Continuation of construction…

  • Beam studies § simulations
  • Investigation of RCS option
  • Hardware prototyping
  • Design § construction of some

equipment

  • TDR

25 ns, 1.15 1011p/b, >2.9 mm.mrad 50 ns, 1.7 1011p/b, >2.5 mm.mrad 75 ns, 1.2 1011 p/b, ≤ 2 mm.mrad

2013 – 2014

(Long Shutdown 1)

  • Linac4 beam

commissioning

  • Connection to PSB ?
  • PSB modification (H- injection) ?
  • PSB beam commissioning ?
  • Modifications and installation of

prototypes in PS and SPS

2015 - 2017

  • Progressive increase of

Linac4 beam current

  • If Linac4 connected: progressive

increase of PSB brightness

  • Some improvement of PS beam

(Injection still at 1.4 GeV)

  • Equipment design § construction for

PS injector, PS and SPS

  • Beam studies
  • Little gain at LHC injection (pending

PS and SPS hardware upgrades)

2018

(Long Shutdown 2)

  • Extensive installations in PS injector,

PS and SPS

  • Beam commissioning

2019 –2021

After ~1 year of operation: beam characteristics for HL-LHC…

Preliminary Planning

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Ingrid-Maria Gregor, DESY: The EUDET Telescope - at DESY and CERN

HL-LHC Luminosity

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L =

  • γfrev

  • nbNb

β⋆

  • Nb

ǫN Rφ

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Recap

Total beam current. Limited by:

  • Uncontrolled beam loss!!
  • E-cloud and other instabilities
  • Action: Linac4

Reduce β*, limited by

  • magnet technology -> Nb3Ti
  • chromatic effects

Brightness, limited by

  • Injector chain
  • Max tune-shift

Geometric factor, related to crossing angle and bunch length Maximize number of bunches

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Booster energy upgrade 1.4 → 2 GeV, ~2014

IR upgrades:

detectors, low‐β quad’s
crab
cavi0es
 etc.
~2022

Linac4 ~2014

SPS enhancements 2012-2022

  • F. Zimmermann
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What can HL-LHC reach ?

Leveled peak luminosity: L = 5 1034 cm-2 sec-1 Virtual peak luminosity: L = 10 1034 cm-2 sec-1 Integrated luminosity: 200 fb-1 to 300 fb-1 per year Total integrated luminosity: ca. 3000 fb-1

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Goal:

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Conclusions

The LHC is running extremely good, the goal for 2011 to collect 1 fb-1 was already reached -> nex goal is 5 fb-1 An even more potent machine is envisaged for 2020+ to access rare decays R&D for this goal is in full swing, a good understanding of the current machine allows to plan for the future 5*1034 is a possible luminosity for HL-LHC

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2008 by Lars Ottesen Henriksen

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Acknowledgements and Further Reading

This talk represents the work of an almost countless number of people. I have incorporated significant material from:

The annual Chamonix meetings http://tinyurl.com/Chamonix2011 Frank Zimmermann’s many luminosity talks, Talks presented at LARP collaborations and DOE reviews See http://www.uslarp.org/

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Accelerator Physics in general:

Klaus Wille, “The Physics of Particle Accelerators”, Oxford University Press, 2000 CERN Accelerator School:http://cdsweb.cern.ch/record/603056/files/ CERN-2006-002.pdf Fundamentals of Accelerator Physics and Technology: http://uspas.fnal.gov/ materials/09UNM/UNMFund.html

HL-LHC Upgrade Details Breaching the Phase I Optics Limitations for the HL-LHC, S. Fartoukh

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  • F. Zimmermann
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LHC Layout

8 crossing interaction points (IP’s) Accelerator sectors labeled by which points they go between

ie, sector 3-4 goes from point 3 to point 4

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LHC Experiments

Compact Muon Solenoid (CMS) A Toroidal LHC ApparatuS (ATLAS) A Large Ion Collider Experiment (ALICE) B physics at the LHC (LHCb)

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Superconductivity and Accelerators

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Cryogenics is complicated and expensive, so what is the interest

  • f superconductivity?

High current density

➡ compact windings ➡ high magnetic fields and gradients

Larger ampere-turns in a small volume -> no need for iron (but iron is still useful for shielding) Reduced power consumption

➡ lower power bills (when cost of refrigeration power is offset)

Superconductivity opens up new technical possibilities

Higher magnetic fields -> increased bending power

➡ greater energy for a given radius

Higher electric fields -> higher accelerating gradients

➡ greater increase of energy per unit length

Higher quadrupole gradients ! more focusing power

➡ higher luminosity

  • A. Ballarino
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Summary of LHC Intensity Limits (7 TeV)

Ideal scenario: no imperfections included!

  • R. Assmann
  • R. Assman @ Chamonix 2010

Chamonix 2011

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eCloud Effect

Photoelectrons created in the vacuum pipe are accelerated by passing proton bunches. Slow or reflected secondary electrons survive until the next bunch arrives Depending on the pipe surface conditions and bunch spacing this may lead to an electron cloud build-up Effects on stability, emittance growth etc. are the consequence Currently the LHC is running at 50ns bunch spacing to reduce this effect

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Crab Cavities

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Main Technical question

Space constraints -> 800 MHz elliptical (simple) versus 400 MHz “exotic”

  • E. Jenssen

Simulations

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Jc(4.2 K, 6 Jc(1.9 K, 9

T(K) B(T) J(A/mm2) 49:(;( ;9<3&#=( ;9!3:(=(

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Operating temperature of superconductors (Niobium titanium)

  • R. Schmidt

The superconducting state only

  • ccurs in a limited domain of

temperature, magnetic field and transport current density Superconducting magnets produce high field with high current density Lowering the temperature enables better usage of the superconductor, by broadening its working range

Jc(4.2 K, 6 T)2300 A/mm2 Jc(1.9 K, 9 T)2300 A/mm2

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Hour Glass effect

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Hour glass effect

Relevant when β* is decreased

close to the bunch length σz. Define r = β* / σz . Luminosity gets reduced. For round beams the factor is

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Beam Beam Effects

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Two crossing beams see the field of each other Space charge cancellation not present anymore Important limitation for high luminosity Beam beam effects: considered to be a major challenge to reach LHC luminosity

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SLIDE 62

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Beam-beam interaction

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  • black

witness bunches (zero collisions);

  • red

bunches colliding in IP 1 5 and 2 (3 collisions);

  • blue

bunches colliding in IP 1 5 and 8 (3 collisions);

  • green

bunches colliding in IP 2 and 8 (2 collisions).

Effects of the beam-beam force are visible on the lifetime of the various bunches.

  • Also sensitive to tune working point.
  • This will become even more complicated with trains of bunches.

Beams in collision Beams in collision Beam1 Beam2

Intensity loss (%)

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SLIDE 63

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

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Total crossing angle of 300 µrad Beam size at IP 16 µm, in arcs about 1 m Beams in the arcs in two vacuum chambers

Crossing angle for multibunch operation

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SLIDE 64

1232 dipole magnets. B field 8.3 T (11.8 kA) @ 1.9 K (super-fluid Helium) 2 magnets-in-one design : two beam tubes with an

  • pening of 56 mm.

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

LHC dipole magnet

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Operating challenges:

  • Dynamic field changes at injection.
  • Very low quench levels (~ mJ/cm3)
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SLIDE 65

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1232 main dipoles + 3700 multipole corrector magnets 392 main quadrupoles + 2500 corrector magnets

Regular arc: Magnets

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SLIDE 66

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

Beam dump

Extraction kickers Dilution kickers Extraction septum magnets Dump block  Complex beam dumping system

commissioned. Beam swept over dump surface (power load)

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SLIDE 67

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Ingrid-Maria Gregor, DESY - Challenges at High Lumi LHC

CERN Accelerators

[fromWikipedia] “CERN operates a network of six accelerators and a decelerator. Each machine in the chain increases the energy of particle beams before delivering them to experiments or to the next more powerful accelerator…

All these accelerators are used to prepare the beam needed by the Large Hadron Collider

Two linear accelerators generate low energy particles. Linac2 accelerates protons to 50MeV for injection in to the Proton Synchrotron Booster (PSB), and Linac3 provides heavy ions at 4.2MeVu fori injection into the Low Energy Ion Ring (LEIR).

The Proton Synchrotron Booster increases the energy of particles generated by the proton linear accelerator

before they are transferred to the other accelerators. The Low Energy Ion Ring (LEIR) accelerates the ions from the ion linear accelerator, before transferring them to the Proton Synchrotron (PS). This accelerator was commissioned in 2005, after having been reconfigured from the previous Low Energy Antiproton Ring (LEAR). The 28GeV Proton Synchrotron (PS), built in 1959 and still operating as a feeder to the more powerful SPS. The Super Proton Synchrotron (SPS), a circular accelerator with a diameter of 2 kilometres built in a tunnel, which started operation in 1976. It was designed to deliver an energy of 300GeV and was gradually upgraded to 450GeV. As well as having its own beamlines for fixed-target experiments (currently COMPASS and NA62),it has been operated as a proton– antiproton collider (the SppS collider), and for accelerating high energy electrons and positrons which were injected into the Large Electron Positron Collider (LEP). Since2008, it has been used to inject protons and heavy ions into the Large Hadron Collider LHC). 67