R. Ostojic CERN, AT Department. R. Ostojic, LTC, 10 May 2006 2 LHC Insertion Magnets Dispersion...

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R. Ostojic CERN, AT Department

Transcript of R. Ostojic CERN, AT Department. R. Ostojic, LTC, 10 May 2006 2 LHC Insertion Magnets Dispersion...

R. Ostojic

CERN, AT Department

R. Ostojic, LTC, 10 May 2006 2

LHC Insertion Magnets

Dispersion suppressor Matching section Separation dipoles Final focus

154 superconducting magnets:• 102 quadrupoles cooled at 1.9 K,

with gradients of 200 T/m• 52 dipoles and quadrupoles

cooled at 4.5 K, with fields of 4 T and gradients of 160 T/m

R. Ostojic, LTC, 10 May 2006 3

LHC Magnet Classes

1. MB – class (MB, MQ, MQM)(8.5 T, Nb-Ti cable at 1.9 K; -channel polyimide insulation)

1b. MQX- class (MQXA, MQXB)(8.5 T; Nb-Ti cable at 1.9 K; closed-channel polyimide insulation)

2. MQY- class (MQM, MQY)(5 T; Nb-Ti cable at 4.5 K; -channel polyimide insulation)

3. RHIC – class (D1, D2, D3, D4) (4 T; Nb-Ti cable at 4.5 K; closed-channel polyimide insulation)

4. MQTL – class (MQTL, MCBX and all correctors)(3 T; Nb-Ti wire at 4.5 K; impregnated coil)

5. Normal conducting magnets (MBW, MBWX, MQW)(1.4 T; normal conducting; impregnated coil)

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Upgrade of the Matching Sections and Separation Dipoles

• The present matching quadrupoles are state-of-the-art Nb-Ti quadrupoles which operate at 4.5 K. – The upgrade of the matching sections should in the first

place focus on modifying the cooling scheme and operating the magnets at 1.9 K.

– In case larger apertures are required, new magnets could be built as extensions of existing designs.

• The 4 T-class separation dipoles should be replaced with higher field magnets cooled at 1.9 K.

• The MQTL-class should be replaced by magnets more resistant to high radiation environment.

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The LHC low- triplet

MQXA MQXB MQXAMQXB

6.372.985

5.5 5.52.715

6.37

MCBXAMCBXH/V

b3b6

MCBXMCBXH/V

MQSX

1.0

TASB

MCBXMCBXH/V

Q3 Q2 Q1

MCSOXa3a4b4

DFBX

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LHC low- triplets

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Limits of the present LHC triplets

• Aperture70 mm coil63 mm beam tube 60 mm beam screen * = 0.55 m

• Gradient– 215 T/m operational 205 T/m

• Field quality– Excellent, no need for correctors down to * ~ 0.6 m

• Peak power density– 12 mW/cm3 L = 3 1034

• Total cooling power– 420 W at 1.9 K L = 3 1034

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Aperture issue

• The coil aperture was the most revisited magnet parameter of the low-quadrupoles.– Aperture of 70 mm defined in the “Yellow Book” (1995,

nominal *= 0.50 m, ultimate 0.25 m).– Subsequent studies showed a need for increasing the

crossing angle by a factor of two.– e-cloud instability introduction of beam screens.

• Upgrade target remains a * of 0.25 m (irrespective of magnet technology).– Luminosity increase by a factor ~1.5.

• Higher luminosity implies substantially greater load on the cryogenic system.– feedback to the choice of aperture and magnet design.

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Enabling operation of the LHCwith minimal disruption

• Maintenance and repair of insertion magnets:– Large number of magnets of different type means

limited number of spare magnets ready for exchange.

– A facility is planned at CERN for repair/rebuild of matching section quadrupoles.

• Particular problem: low-beta quadrupoles and separation dipoles

• Only one spare of each type (best magnets already in the LHC).

• As of 2006, there will be no operating facility for repair and testing of these magnets.

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Quadrupole-first layouts

Use of aperture:• Increase the aperture to

reduce heat loads (peak and total)

• Profit from better field quality to reduce the number of correctors and introduce stronger orbit correctors

• Decrease * to complement other ways of increasing luminosity.

0.00

20.00

40.00

60.00

80.00

100.00

120.00

140.00

0.00 0.10 0.20 0.30 0.40 0.50 0.60

*[m]

Dm

in [

mm

]

0.00

0.10

0.20

0.30

0.40

0.50

0.60

0.70

0.80

0.90

Fp

Q2/Q3

Q1

L < 10 m

L ~ Fp/*

Optimize the aperture and length of the quadrupoles according to their position in the triplet.

Q3 Q2B Q2A Q1

LHC Low- Triplet

1.0

Symmetric Triplet

2.0 2.0 2.0 L* = 23 m

Triplet with "long" Q3

2.0 2.0 2.0

Triplet with "short" Q1

2.0 2.0 2.0

10.0 8.0 8.08.0

8.0 8.0 8.0 4.0

8.0 8.0 8.0 8.0

6.3 5.5 6.32.73.0 5.5

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Large aperture quadrupoles using existing LHC cables

Cable parameters MQY MQ MB Width [mm] 8.3 15.10 15.10 Mid-thickness [mm] 0.84/

1.28 1.48 1.90

Critical current, Ic [A] @ 9 T, 1.9K

5070/ 9110

12960 13750

dIc/dB [A/T] 1350/ 2550

3650 4800

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Large aperture quadrupoles

100

120

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160

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200

220

240

50 60 70 80 90 100 110 120

Coil aperture [mm]

Gra

die

nt

[T/m

]

MQY cable

MB/MQ cable

MQ cable

Operating current at 80% of conductor limit As the quadrupole aperture

increases, the operating gradient decreases by 20 T/m for every 10mm of coil aperture.

To get a GL similar to the present triplet, quadrupole lengths need to be increased by 20-30%.

The Nb-Ti technology proven for quadrupoles up to 12 m long.

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• Technology and manufacturing issues are well mastered.

• Relatively easy extension of main magnet parameters (aperture and length) without extensive R&D.

• Focus R&D on magnet “transparency”:

– Cable and coil insulation

– Thermal design of the collaring and yoking structures

– Coupling to the heat exchanger

C. Meuris et al, 1999

LHC dipoles

R&D directions for Nb-Ti quads

FRESCA, 10 T, 88 mmD. Leroy et al., 1999

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Summary

• LHC contains several generations of Nb-Ti magnets. Extensive experience exists in building magnets of different aperture and length. Upgrading the magnets to a higher class should be considered as a first option.

• Nb-Ti (1.9K) technology is a clear choice for upgrading the large number of magnets in the LHC insertions (dipoles and quadrupoles) of the 4 T class.

• The availability of spare low- triplets and separation dipoles is a serious concern. Any proposal for the upgrade must take this issue into account and provide an appropriate solution.

– The shortest route for providing new magnets in a time frame compatible with LHC luminosity runs is to use Nb-Ti technology.

• Nb-Ti (1.9K) technology has reached its limits for large series production with the LHC main dipoles; improvements for small series are still possible.

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Comment

• It is generally accepted that a new generation of magnets (Nb3Sn, HTS,…) will be required for the next hadron collider. CERN should take part in a wider effort to develop and demonstrate the feasibility of the new technology.

– In the interest of LHC operation, we must have an alternative; Nb-Ti technology can offer an appropriate intermediate solution.

• The pitfalls in building Nb-Ti magnets should not be underestimated. There is a need to start design studies and development before LHC construction teams move on to other projects.

• Initial experience from operating the LHC with beam is crucial for refining magnet parameters and making sure there are no “unknown unknowns”.