Designing the Four Rod Crab Cavity for the High-Luminosity LHC
WP 4: Crab Cavity
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Transcript of WP 4: Crab Cavity
WP 4: Crab CavityEd Ciapala, Erk Jensen
BE-RF, CERN
HL-LHC Meeting, CERN, 20 July 2010
Crab cavities: ContextMany bunches require non-
zero crossing angle to avoid parasitic collisions and to reduce beam-beam effects;
With non-zero crossing angle, luminosity gain by squeezing beams further is small (red curve below).
Crab cavities can compensate for this geometric effect and thus allow for a luminosity increase of about 50 % at β* of 25 cm.
In addition, crab cavities provide an ideal knob for luminosity levelling;
This allows optimizing for integratedrather than peak luminosity!20 July
2010 2HL-LHC Meeting WP4: Crab Cavity
Local and Global Scheme Local Scheme: Global Scheme:
20 July 2010 HL-LHC Meeting WP4: Crab Cavity 3
Advantages:• Only one cavity per beam;• Larger beam separation near IP4;• Elliptical cavity of known
technology.Disadvantages:• Constraining betatron phase
advance;• Requires larger collimator settings;• Works only for H or V crossing;• Only 800 MHz or higher fits.
Advantages:• Individual luminosity control at each
IP;• Adapted to H or V crossing;• Orbit perturbed only locally;• Could work lower f – better
performance.Disadvantages:• Requires novel Compact Cavities (194
mm separation), which are not validated;
• Requires 4 cavities per IP;• What if a cavity trips?
CERN StrategyAim ultimately at a significant luminosity
increase using the local scheme with compact crab cavities around the IPs.◦ This requires a substantial R&D program, but first
results are encouraging (see below).To mitigate the risk, and in parallel to the above,
design and implement a elliptical cavity in IR4 to obtain measurable luminosity increase in a global scheme.◦ Conceptual design exists (US-LARP), including coupler,
cryostat, wrong-order-mode dampers, ...◦ Space is available in IR4 (was foreseen for ACN200
system).◦ What could a test of the KEK crab cavity in SPS tell us?20 July
2010 HL-LHC Meeting WP4: Crab Cavity 4
Collaboration In order to encourage collaboration and to assure its
consistency and continuity, CERN has to take the lead in the world wide Crab Cavity development program. This is also a necessary strong sign to assure partners!
In the past, CERN was merely observer; results obtained by collaborators so far: ◦ US-LARP: design of elliptical cavity system, some 3 compact
designs, ◦ EuCARD WP 10.3: specifications, compact cavity design (Lancaster),◦ KEK-B positive results, compact cavity design (“Kota” cavity).
CERN is in the process of defining the strategy and a work plan (in parallel to ongoing efforts), which it will then adhere to.
Expected in September 2010: “Statement of Need”, Initial Cost & Schedule, work plan!
This will allow identification of work packages for partners. HL-LHC is one important element of the overall strategy
(focussing on “design” questions); other elements – coordinated with it – are: ◦ US-LARP and maybe APUL, EuCARD, the French “Grand Emprunt” in
Rhône-Alpes region, DoE SBIR & MTTR programs, ...)
20 July 2010 HL-LHC Meeting WP4: Crab Cavity 5
Elliptical cavity design
20 July 2010 HL-LHC Meeting WP4: Crab Cavity 6
Taken from Rama Calaga’s Talk at Chamonix 2010, http://indico.cern.ch/conferenceDisplay.py?confId=67839
Compact cavity designs
20 July 2010 HL-LHC Meeting WP4: Crab Cavity 7
EUCARD 4-rod cavity (Lancaster)
ODU Parallel Bar Cavity
SLAC Half-wave Spoke Resonator
KEK Kota Cavity
Taken from Graeme Burt’s Highlight Talk at EuCARD Annual Meeting, http://indico.cern.ch/conferenceDisplay.py?confId=73614
The possible issuesWill it work?Machine protection!
◦Major concern: single turn failure! Requires study!Collimation efficiency and hierarchy
◦ Initial calculations indicate that this might be OK – still, it requires more study!
Crab cavity induced noise◦Phase noise leads to beam offset – requires study!
Impedance, both longitudinal and transverse!Operational: how to make “invisible”, how to
commission? What happens during the ramp?20 July 2010 HL-LHC Meeting WP4: Crab Cavity 8
WP4: Possible design subjects (1/2)
20 July 2010 HL-LHC Meeting WP4: Crab Cavity 9
Tasks Collaborator
1Design optimization for novel schemes (minimum # of peripherals)
CI, LARP, CERN,KEK
2 Cavity and cryomodule specifications (LHC report) CERN, KEK, CNRS
3 Local IR layout and spatial integration CERN, KEK
4 Multipacting simulations of cavity & couplers CI, LARP
5 FEM simulations: mechanical & thermal aspects CI, LARP
6Fabrication and measurements on copper models: field profile, impedance, error sensitivity)
CI, LARP
7Demonstration of field gradients in compact cavities (4 structures)
LARP, CERN, CI
8 Q-slope, onset of field emission and quench LARP, CERN
9 Performance difference between 2 K & 4 K LARP, CERN
10 Coupler development and testing CERN, CEA
11 Tuner concepts and mock up on copper models CERN, CEA
12 Study of mech. resonances, microphonics CERN, CEA
13 Performance with couplers and horizontal cryostat CERN, CEA
14Performance with beam (e.g. SPS – impedance, collimation, …)
CERN, LARP
15 Interlocks and fast Feedback (other measures like Qext) CERN,
16 Common power and cryogenic systems across the IPs (?) CERN, CEA?
17 LLRF and controls – (phase control!) CERN, CI
Technology Issues
20 July 2010 HL-LHC Meeting WP4: Crab Cavity 10
WP4: Possible design subjects (2/2)
Tasks Collaborator
1RF behavior for cavity quench or turbulent behavior *
CERN, LARP, KEK
2Tracking simulations for loss maps for fast failure modes
CERN, LARP, KEK
3Beam-beam simulations to investigate instabilities, noise issues and DA
CI, LARP, CERN
4Impedance and growth rate estimates for specific HOMs to specify exact damping and feedback measures*
CERN, LARP
5Effect of non-zero dispersion and stable working points
CERN, LARP
6 Crab consistent optics CERN, LARP, KEK
Beam Issues
* Cavity design dependent
WP4: Possible Participants
CERNCockcroft Institute (U Lancaster)US-LARPKEKCEACNRS...
20 July 2010 HL-LHC Meeting WP4: Crab Cavity 11