heat load due to e-cloud in the hl-lhc triplets

68
Heat load due to e-cloud in the HL-LHC triplets G. Iadarola, G. Rumolo 19th HiLumi WP2 Task Leader Meeting - 18 October 2013 Many thanks to: H.Bartosik, R. De Maria, R. Tomas, L. Tavian

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Heat load due to e-cloud in the HL-LHC triplets. G. Iadarola , G. Rumolo. Many thanks to: H.Bartosik , R. De Maria, R. Tomas, L. Tavian. 19th HiLumi WP2 Task Leader Meeting - 18 October 2013. Outline. Present inner triplets Layout and optics PyECLOUD simulations - PowerPoint PPT Presentation

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Page 1: Heat load due  to e-cloud in the HL-LHC triplets

Heat load due to e-cloud in the HL-LHC tripletsG. Iadarola, G. Rumolo

19th HiLumi WP2 Task Leader Meeting - 18 October 2013

Many thanks to: H.Bartosik, R. De Maria, R. Tomas, L. Tavian

Page 2: Heat load due  to e-cloud in the HL-LHC triplets

Outline

• Present inner triplets

o Layout and optics

o PyECLOUD simulations

o Heat load measurements and estimate of the SEY

• Inner triplets for the HL-LHC upgrade

o Layout and optics

o Heat load estimates from PyECLOUD simulations

Page 3: Heat load due  to e-cloud in the HL-LHC triplets

Outline

• Present inner triplets

o Layout and optics

o PyECLOUD simulations

o Heat load measurements and estimate of the SEY

• Inner triplets for the HL-LHC upgrade

o Layout and optics

o Heat load estimates from PyECLOUD simulations

Page 4: Heat load due  to e-cloud in the HL-LHC triplets

B2L1 A2L1

3L1 1L1

Machine layout and optics near IP1

IP1, 4 TeV, β* = 0.6 m

IP1

1R1

A2R1 B2R1

3R1

Page 5: Heat load due  to e-cloud in the HL-LHC triplets

Machine layout and optics near IP1

IP1, 4 TeV, β* = 0.6 m

IP1 1R1

A2R1 B2R1

3R1

Page 6: Heat load due  to e-cloud in the HL-LHC triplets

Machine layout and optics near IP1

IP1, 4 TeV, β* = 0.6 m

IP1 1R1

A2R1 B2R1

3R1

Page 7: Heat load due  to e-cloud in the HL-LHC triplets

Machine layout and optics near IP1

IP1, 4 TeV, β* = 0.6 m

IP1 1R1

A2R1 B2R1

3R1

Page 8: Heat load due  to e-cloud in the HL-LHC triplets

Machine layout and optics near IP1

IP1, 4 TeV, β* = 0.6 m

IP1 1R1

A2R1 B2R1

3R1

Page 9: Heat load due  to e-cloud in the HL-LHC triplets

The longitudinal direction

The delay between two following bunch passages changes along the machine elements

• Locations of long range encounters spaced by half the bunch spacing

7.5 m

Beam 2

Beam 1 IP1

25 ns spac.

Page 10: Heat load due  to e-cloud in the HL-LHC triplets

The longitudinal direction

The delay between two following bunch passages changes along the machine elements

• Locations of long range encounters spaced by half the bunch spacing

7.5 m

Bea

m 1

25 ns 3R1 sey = 1.40

10 20 30 40 500

5

10x 10

9

e- per

uni

t len

gth

[m-1

]

Time [ns]

10 20 30 40 50

Bea

m 2

Time [ns]

Beam 2

Beam 1 IP1

25 ns spac.

Page 11: Heat load due  to e-cloud in the HL-LHC triplets

Outline

• Present inner triplets

o Layout and optics

o PyECLOUD simulations

o Heat load measurements and estimate of the SEY

• Inner triplets for the HL-LHC upgrade

o Layout and optics

o Heat load estimates from PyECLOUD simulations

Page 12: Heat load due  to e-cloud in the HL-LHC triplets

PyECLOUD simulations for the inner triplets

Quite a challenging simulation scenario:

• Two beams with:

o Different transverse position (off center)

o Different transverse shape

o Arbitrarily delayed with respect to each other (no real bunch spacing)

Page 13: Heat load due  to e-cloud in the HL-LHC triplets

PyECLOUD simulations for the inner triplets

Quite a challenging simulation scenario:

• Two beams with:

o Different transverse position (off center)

o Different transverse shape

o Arbitrarily delayed with respect to each other (no real bunch spacing)

• Quadrupolar magnetic field

• Non elliptical chamber

Page 14: Heat load due  to e-cloud in the HL-LHC triplets

PyECLOUD simulations for the inner triplets

Quite a challenging simulation scenario:

• Two beams with:

o Different transverse position (off center)

o Different transverse shape

o Arbitrarily delayed with respect to each other (no real bunch spacing)

• Quadrupolar magnetic field

• Non elliptical chamber

Required the introduction of new

features in PyECLOUD

Page 15: Heat load due  to e-cloud in the HL-LHC triplets

PyECLOUD simulations for the inner triplets

Quite a challenging simulation scenario:

• Two beams with:

o Different transverse position (off center)

o Different transverse shape

o Arbitrarily delayed with respect to each other (no real bunch spacing)

• Quadrupolar magnetic field

• Non elliptical chamber

Required the introduction of new

features in PyECLOUD

Beam properties (delay, position, size) changing along the structure:

• Simulated 10 slices per magnet

• SEY = 1.0, 1.1, … , 2.0

• 50 ns and 25 ns

Page 16: Heat load due  to e-cloud in the HL-LHC triplets

PyECLOUD simulations for the inner triplets

Quite a challenging simulation scenario:

• Two beams with:

o Different transverse position (off center)

o Different transverse shape

o Arbitrarily delayed with respect to each other (no real bunch spacing)

• Quadrupolar magnetic field

• Non elliptical chamber

Required the introduction of new

features in PyECLOUD

Beam properties (delay, position, size) changing along the structure:

• Simulated 10 slices per magnet

• SEY = 1.0, 1.1, … , 2.0

• 50 ns and 25 ns

~1000 simulations,~48 h for two bunch trains,

~120 GB of sim. data

Page 17: Heat load due  to e-cloud in the HL-LHC triplets

Simulated scenarios

8 72 8 7272 8 72

25 ns beam – 1.15 x 1011 ppb38 8 72 8 7272 8 72 38

4 36 4 3636 4 36

50 ns beam – 1.65 x 1011 ppb19 4 36 4 3636 4 36 19

Other beam parameters:

• Beam energy: 4 TeV

• Transverse emittance: 2.4 μm

• Bunch length: 1.3 ns

• Optics with β* = 0.6 m

Page 18: Heat load due  to e-cloud in the HL-LHC triplets

Few snapshots of the electron distribution (50 ns spacing)

Beam 1

A look to the EC buildup

Page 19: Heat load due  to e-cloud in the HL-LHC triplets

The presence of two beams enhances the multipacting efficiency, especially far enough from the locations of the long range encounters

A look to the EC buildupB

eam

1

25 ns 3R1 sey = 1.40

0.5 1 1.5 2 2.5 30

5

10x 10

9

e- per

uni

t len

gth

[m-1

]

Time [us]

0.5 1 1.5 2 2.5 3

Bea

m 2

Time [us]

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Scr

ubbi

ng d

ose

(50e

V) [

mA

/m]

25 ns 3R1

s = 47.90 ms = 48.54 ms = 49.19 ms = 49.83 ms = 50.47 ms = 51.12 ms = 51.76 ms = 52.40 ms = 53.05 m

Bea

m 1

25 ns 3R1 sey = 1.40

0.2 0.4 0.6 0.8 1 1.2 1.40

5

10x 10

9

e- per

uni

t len

gth

[m-1

]

Time [us]

0.2 0.4 0.6 0.8 1 1.2 1.4

Bea

m 2

Time [us]

Page 20: Heat load due  to e-cloud in the HL-LHC triplets

The presence of two beams enhances the multipacting efficiency, especially far enough from the locations of the long range encounters

A look to the EC buildupB

eam

1

25 ns 3R1 sey = 1.40

0.5 1 1.5 2 2.5 30

5

10x 10

9

e- per

uni

t len

gth

[m-1

]

Time [us]

0.5 1 1.5 2 2.5 3

Bea

m 2

Time [us]

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Scr

ubbi

ng d

ose

(50e

V) [

mA

/m]

25 ns 3R1

s = 47.90 ms = 48.54 ms = 49.19 ms = 49.83 ms = 50.47 ms = 51.12 ms = 51.76 ms = 52.40 ms = 53.05 m

Bea

m 1

25 ns 3R1 sey = 1.40

0.2 0.4 0.6 0.8 1 1.2 1.40

5

10x 10

9

e- per

uni

t len

gth

[m-1

]

Time [us]

0.2 0.4 0.6 0.8 1 1.2 1.4

Bea

m 2

Time [us]

Page 21: Heat load due  to e-cloud in the HL-LHC triplets

Heat load density along the triplet - 50 ns

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

Locations of long range encounters

Remarks:

• EC much weaker close to long range encounters

• Modules with the same beam screen behave very similarly

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

1R1 A2R1 B2R1 3R1

Page 22: Heat load due  to e-cloud in the HL-LHC triplets

Heat load density along the triplet - 50 ns

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

1R1 A2R1 B2R1 3R1

Remarks:

• EC much weaker close to long range encounters

• Modules with the same beam screen behave very similarly

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Hea

t loa

d [W

/m]

50 ns 1R1

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Scr

ubbi

ng d

ose

(50e

V) [

mA

/m]

25 ns 1R1

s = 23.90 ms = 24.54 ms = 25.18 ms = 25.83 ms = 26.47 ms = 27.11 ms = 27.76 ms = 28.40 ms = 29.05 m

The presence of the two beams leads to an important lowering of the multipacting threshold w.r.t. the single beam case (dashed)

Page 23: Heat load due  to e-cloud in the HL-LHC triplets

Heat load density along the triplet - 50 ns

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

1R1 A2R1 B2R1 3R1

Remarks:

• EC much weaker close to long range encounters

• Modules with the same beam screen behave very similarly

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

The presence of the two beams leads to an important lowering of the multipacting threshold w.r.t. the single beam case (dashed)

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Hea

t loa

d [W

/m]

50 ns A2R1

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Scr

ubbi

ng d

ose

(50e

V) [

mA

/m]

50 ns A2R1

s = 32.86 ms = 33.41 ms = 33.97 ms = 34.52 ms = 35.08 ms = 35.63 ms = 36.19 ms = 36.74 ms = 37.30 m

Page 24: Heat load due  to e-cloud in the HL-LHC triplets

Heat load density along the triplet - 50 ns

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

1R1 A2R1 B2R1 3R1

Remarks:

• EC much weaker close to long range encounters

• Modules with the same beam screen behave very similarly

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

The presence of the two beams leads to an important lowering of the multipacting threshold w.r.t. the single beam case (dashed)

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Hea

t loa

d [W

/m]

50 ns B2R1

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Scr

ubbi

ng d

ose

(50e

V) [

mA

/m]

50 ns B2R1

s = 39.36 ms = 39.91 ms = 40.47 ms = 41.02 ms = 41.58 ms = 42.13 ms = 42.69 ms = 43.24 ms = 43.80 m

Page 25: Heat load due  to e-cloud in the HL-LHC triplets

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

Heat load density along the triplet - 50 ns

1R1 A2R1 B2R1 3R1

Remarks:

• EC much weaker close to long range encounters

• Modules with the same beam screen behave very similarly

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

The presence of the two beams leads to an important lowering of the multipacting threshold w.r.t. the single beam case (dashed)

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Hea

t loa

d [W

/m]

50 ns 3R1

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Scr

ubbi

ng d

ose

(50e

V) [

mA

/m]

50 ns 3R1

s = 47.90 ms = 48.54 ms = 49.19 ms = 49.83 ms = 50.47 ms = 51.12 ms = 51.76 ms = 52.40 ms = 53.05 m

Page 26: Heat load due  to e-cloud in the HL-LHC triplets

20 25 30 35 40 45 50 550

1

2

3

4

5

6

7

s [m]

Ave

rage

hea

t loa

d [W

/m]

25 ns - 576 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

Heat load density along the triplet - 25 ns

Locations of long range encounters

Remarks:

• EC much weaker close to long range encounters

• Modules with the same beam screen behave very similarly

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

1R1

A2R1 B2R1 3R1

Page 27: Heat load due  to e-cloud in the HL-LHC triplets

20 25 30 35 40 45 50 550

1

2

3

4

5

6

7

s [m]

Ave

rage

hea

t loa

d [W

/m]

25 ns - 576 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

Heat load density along the triplet - 25 ns

Remarks:

• EC much weaker close to long range encounters

• Modules with the same beam screen behave very similarly

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

As in the other quardupoles in the LHC, the multipacting threshold is already quite low even for a single beam with 25 ns spacing

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Hea

t loa

d [W

/m]

25 ns 1R1

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Scr

ubbi

ng d

ose

(50e

V) [

mA

/m]

25 ns 1R1

s = 23.90 ms = 24.54 ms = 25.18 ms = 25.83 ms = 26.47 ms = 27.11 ms = 27.76 ms = 28.40 ms = 29.05 m

1R1

A2R1 B2R1 3R1

Page 28: Heat load due  to e-cloud in the HL-LHC triplets

20 25 30 35 40 45 50 550

1

2

3

4

5

6

7

s [m]

Ave

rage

hea

t loa

d [W

/m]

25 ns - 576 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

Heat load density along the triplet - 25 ns

Remarks:

• EC much weaker close to long range encounters

• Modules with the same beam screen behave very similarly

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

The presence of the two beams leads to an important lowering of the multipacting threshold w.r.t. the single beam case (dashed)

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Hea

t loa

d [W

/m]

25 ns A2R1

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Scr

ubbi

ng d

ose

(50e

V) [

mA

/m]

50 ns A2R1

s = 32.86 ms = 33.41 ms = 33.97 ms = 34.52 ms = 35.08 ms = 35.63 ms = 36.19 ms = 36.74 ms = 37.30 m

1R1

A2R1 B2R1 3R1

Page 29: Heat load due  to e-cloud in the HL-LHC triplets

20 25 30 35 40 45 50 550

1

2

3

4

5

6

7

s [m]

Ave

rage

hea

t loa

d [W

/m]

25 ns - 576 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

Heat load density along the triplet - 25 ns

Remarks:

• EC much weaker close to long range encounters

• Modules with the same beam screen behave very similarly

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

The presence of the two beams leads to an important lowering of the multipacting threshold w.r.t. the single beam case (dashed)

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Hea

t loa

d [W

/m]

25 ns B2R1

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Scr

ubbi

ng d

ose

(50e

V) [

mA

/m]

50 ns B2R1

s = 39.36 ms = 39.91 ms = 40.47 ms = 41.02 ms = 41.58 ms = 42.13 ms = 42.69 ms = 43.24 ms = 43.80 m

1R1

A2R1 B2R1 3R1

Page 30: Heat load due  to e-cloud in the HL-LHC triplets

20 25 30 35 40 45 50 550

1

2

3

4

5

6

7

s [m]

Ave

rage

hea

t loa

d [W

/m]

25 ns - 576 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

Heat load density along the triplet - 25 ns

Remarks:

• EC much weaker close to long range encounters

• Modules with the same beam screen behave very similarly

20 25 30 35 40 45 50 550

0.5

1

1.5

2

2.5

3

s [m]

Ave

rage

hea

t loa

d [W

/m]

50 ns - 288 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

The presence of the two beams leads to an important lowering of the multipacting threshold w.r.t. the single beam case (dashed)

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Hea

t loa

d [W

/m]

25 ns 3R1

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Scr

ubbi

ng d

ose

(50e

V) [

mA

/m]

50 ns 3R1

s = 47.90 ms = 48.54 ms = 49.19 ms = 49.83 ms = 50.47 ms = 51.12 ms = 51.76 ms = 52.40 ms = 53.05 m

1R1

A2R1 B2R1 3R1

Page 31: Heat load due  to e-cloud in the HL-LHC triplets

1 1.2 1.4 1.6 1.8 20

0.02

0.04

0.06

0.08

0.1

0.12

0.14

0.16

0.18

0.2

SEYH

eat l

oad

per b

unch

[W]

25 ns

1 1.2 1.4 1.6 1.8 20

0.02

0.04

0.06

0.08

0.1

0.12

0.14

0.16

0.18

SEY

Hea

t loa

d pe

r bun

ch [W

]

50 ns

Average heat load density – 50 ns vs. 25 ns

Remarks:

• Above threshold values are very similar enhancement from hybrid spacings

much stronger on the 50 ns than on 25 ns

For each triplet we get:

Page 32: Heat load due  to e-cloud in the HL-LHC triplets

Outline

• Present inner triplets

o Layout and optics

o PyECLOUD simulations

o Heat load measurements and estimate of the SEY

• Inner triplets for the HL-LHC upgrade

o Layout and optics

o Heat load estimates from PyECLOUD simulations

Page 33: Heat load due  to e-cloud in the HL-LHC triplets

Machine observations – 50 ns

No big change during ramp and squeeze

Data provided by L. Tavian

Page 34: Heat load due  to e-cloud in the HL-LHC triplets

Machine observations – 50 ns

No big change during ramp and squeeze

Page 35: Heat load due  to e-cloud in the HL-LHC triplets

Machine observations – 50 ns

Heat load much higher than in two-aperture quadrupoles

Data provided by L. Tavian

Page 36: Heat load due  to e-cloud in the HL-LHC triplets

Machine observations – 25 ns (4 TeV)

Data provided by L. Tavian

No big change during ramp and squeeze

Page 37: Heat load due  to e-cloud in the HL-LHC triplets

Machine observations – 25 ns (4 TeV)

No big change during ramp and squeeze

Page 38: Heat load due  to e-cloud in the HL-LHC triplets

Machine observations – 25 ns (4 TeV)

Data provided by L. Tavian

Heat load similar to two-aperture quadrupoles

Page 39: Heat load due  to e-cloud in the HL-LHC triplets

Comparison against simulations

1 1.2 1.4 1.6 1.8 20

50

100

150

SEY

Hea

t loa

d [W

]

25 ns - 800 bunches - short trains

Fill 3429

1 1.2 1.4 1.6 1.8 20

50

100

150

200

250

SEY

Hea

t loa

d [W

]

50 ns - 1374 bunches

Fill 3286

1 1.2 1.4 1.6 1.8 20

20

40

60

80

100

120

140

160

SEY

Hea

t loa

d [W

]

25 ns - 800 bunches

Fill 3405

50 ns, 4 TeV 25 ns, 450 GeV

25 ns, 4 TeV

1.2 < SEYmax < 1.3 is compatible with the observations

Page 40: Heat load due  to e-cloud in the HL-LHC triplets

Crosscheck with single beam MDs

For the estimated SEY value we do not expect nor observe EC in the triplets

with only one beam with 50 ns spacing circulating in the LHC

1 1.2 1.4 1.6 1.8 210

-3

10-2

10-1

100

101

102

SEY

Hea

t loa

d [W

/m]

50 ns B2R1

Page 41: Heat load due  to e-cloud in the HL-LHC triplets

Crosscheck with single beam MDs

For the estimated SEY value we do not expect nor observe EC in the triplets

with only one beam with 50 ns spacing circulating in the LHC

Page 42: Heat load due  to e-cloud in the HL-LHC triplets

Outline

• Present inner triplets

o Layout and optics

o PyECLOUD simulations

o Heat load measurements and estimate of the SEY

• Inner triplets for the HL-LHC upgrade

o Layout and optics

o Heat load estimates from PyECLOUD simulations

Page 43: Heat load due  to e-cloud in the HL-LHC triplets

Optics, layout and apertures

Q1 (A/B)

Q2 (A/B)

Q3 (A/B) D1

Q1

Q2 (A/B)

Q3 D1Present

HiLumi

IP1, 4 TeV, β* = 0.6 m

IP1, 7 TeV, β* = 0.15 m

Page 44: Heat load due  to e-cloud in the HL-LHC triplets

Optics, layout and apertures

Q1 (A/B)

Q2 (A/B)

Q3 (A/B) D1

Q1

Q2 (A/B)

Q3 D1

For the moment, only quadrupoles have been simulated

IP1, 7 TeV, β* = 0.15 m

Thanks to R. De Maria

Page 45: Heat load due  to e-cloud in the HL-LHC triplets

Optics, layout and apertures

Q1 (A/B)

Q2 (A/B)

Q3 (A/B) D1

Q1

Q2 (A/B)

Q3 D1Present

HiLumi

IP1, 4 TeV, β* = 0.6 m

IP1, 7 TeV, β* = 0.15 m

Page 46: Heat load due  to e-cloud in the HL-LHC triplets

Optics, layout and apertures

Q1 (A/B)

Q2 (A/B)

Q3 (A/B) D1

Q1

Q2 (A/B)

Q3 D1Present

HiLumi

IP1, 4 TeV, β* = 0.6 m

IP1, 7 TeV, β* = 0.15 m

Page 47: Heat load due  to e-cloud in the HL-LHC triplets

Optics, layout and apertures

Q1 (A/B)

Q2 (A/B)

Q3 (A/B) D1

Q1

Q2 (A/B)

Q3 D1Present

HiLumi

IP1, 4 TeV, β* = 0.6 m

IP1, 7 TeV, β* = 0.15 m

Page 48: Heat load due  to e-cloud in the HL-LHC triplets

Optics, layout and apertures

Q1 (A/B)

Q2 (A/B)

Q3 (A/B) D1

Q1

Q2 (A/B)

Q3 D1Present

HiLumi

IP1, 4 TeV, β* = 0.6 m

IP1, 7 TeV, β* = 0.15 m

Page 49: Heat load due  to e-cloud in the HL-LHC triplets

Optics, layout and apertures

Q1 (A/B)

Q2 (A/B)

Q3 (A/B) D1

Q1

Q2 (A/B)

Q3 D1Present

HiLumi

IP1, 4 TeV, β* = 0.6 m

IP1, 7 TeV, β* = 0.15 m

Page 50: Heat load due  to e-cloud in the HL-LHC triplets

Optics, layout and apertures

Q1 (A/B)

Q2 (A/B)

Q3 (A/B) D1

Q1

Q2 (A/B)

Q3 D1Present

HiLumi

IP1, 4 TeV, β* = 0.6 m

IP1, 7 TeV, β* = 0.15 m

Page 51: Heat load due  to e-cloud in the HL-LHC triplets

Outline

• Present inner triplets

o Layout and optics

o PyECLOUD simulations

o Heat load measurements and estimate of the SEY

• Inner triplets for the HL-LHC upgrade

o Layout and optics

o Heat load estimates from PyECLOUD simulations

Page 52: Heat load due  to e-cloud in the HL-LHC triplets

Simulated scenario

8 72 8 7272 8 72

25 ns beam – 2.20 x 1011 ppb38 8 72 8 7272 8 72 38

Other beam parameters:

• Beam energy: 7 TeV

• Transverse emittance: 2.5 μm

• Bunch length: 1.0 ns

• Optics with β* = 0.15 m

Page 53: Heat load due  to e-cloud in the HL-LHC triplets

A look to the EC buildup – HiLumi triplets

Few snapshots of the electron distribution much wider stripes for HiLumi triplets

HiLumi

Present

Page 54: Heat load due  to e-cloud in the HL-LHC triplets

Heat load along the triplet

20 25 30 35 40 45 50 55 60 650

2

4

6

8

10

12

14

16

18

20

s [m]

Ave

rage

hea

t loa

d [W

/m]

25 ns - 576 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

20 25 30 35 40 45 50 55 60 650

1

2

3

4

5

6

7

s [m]

Ave

rage

hea

t loa

d [W

/m]

25 ns - 576 bunches

sey = 1.00sey = 1.20sey = 1.40sey = 1.60sey = 1.80sey = 2.00

Present triplets

HiLumi triplets

Locations of long range encounters

Page 55: Heat load due  to e-cloud in the HL-LHC triplets

1 1.2 1.4 1.6 1.8 20

100

200

300

400

500

600

SEY

Av.

e- e

nerg

y [e

V]

Only e- with En>50eV are considered

1R1A2R1B2R13R1

1 1.2 1.4 1.6 1.8 20

100

200

300

400

500

600

SEY

Av.

e- e

nerg

y [e

V]

Only e- with En>50eV are considered

A1R1B1R1A2R1B2R1A3R1B3R1

Bunch intensity is larger but also chamber is wider energy of multipacting electrons is quite similar

Present triplets HiLumi triplets

Heat loads

Page 56: Heat load due  to e-cloud in the HL-LHC triplets

1 1.2 1.4 1.6 1.8 20

0.5

1

1.5

2x 10

13

SEY

Impa

ctin

g e

- [m-1

]

25 ns - 576 bunchesOnly e- with En>50eV are considered

A1R1B1R1A2R1B2R1A3R1B3R1

1 1.2 1.4 1.6 1.8 20

0.5

1

1.5

2x 10

13

SEY

Impa

ctin

g e

- [m-1

]

25 ns - 576 bunchesOnly e- with En>50eV are considered

1R1A2R1B2R13R1

Bunch intensity is larger but also chamber is wider energy of multipacting electrons is quite similar number of impacting electrons about x2 larger

Heat loads

Present triplets HiLumi triplets

Page 57: Heat load due  to e-cloud in the HL-LHC triplets

1 1.2 1.4 1.6 1.8 20

200

400

600

800

1000

1200

SEY

Hea

t loa

d [W

]

25 ns - 2800 bunches

1 1.2 1.4 1.6 1.8 20

200

400

600

800

1000

1200

SEY

Hea

t loa

d [W

]

25 ns - 2800 bunches

Bunch intensity is larger but also chamber is wider energy of multipacting electrons is quite similar number of impacting electrons about x2 larger Total heat load about x2 larger

Heat loads

Present triplets HiLumi triplets

D1 and correctors not included!

SEYmax in the present triplets at the end of 2012

Page 58: Heat load due  to e-cloud in the HL-LHC triplets

Summary and conclusions

• Simulations show a strong enhancement of the EC due to the presence of the two

beams extremely low multipacting thresholds (SEYth<1.1 for 25 ns beams)

• Comparing measured heat load against simulation we infer SEYmax = ~1.3 for the

present triplets (crosschecked in different beam conditions )

• Simulations for the HiLumi scenario show x2 stronger heat load w.r.t. the present

scenario (SEYmax = ~1.3 HL = ~500 W – D1 and correctors to be added)

• Heat load could be strongly reduced by EC mitigation strategies:

o Low SEY coating (but we need SEYmax<1.1 to have full suppression)

o Clearing electrode (EC localized in a region where there should be enough

aperture to place a polarized plate/wire)

Page 59: Heat load due  to e-cloud in the HL-LHC triplets

Thanks for your attention!

Page 60: Heat load due  to e-cloud in the HL-LHC triplets

Machine layout and optics near IP1 - present

Common beam pipe Separated beam pipesSeparated beam pipes

IP1

IP1, 4 TeV, β* = 0.6 m

Page 61: Heat load due  to e-cloud in the HL-LHC triplets

Machine layout and optics near IP1 - HiLumi

Common beam pipe Separated beam pipesSeparated beam pipes

IP1

IP1, 4 TeV, β* = 0.6 m

Page 62: Heat load due  to e-cloud in the HL-LHC triplets

B2L1 A2L1

3L1 1L1

IP1, 4 TeV, β* = 0.6 m

IP1

1R1

A2R1 B2R1

3R1

Machine layout and optics near IP1 - present

Page 63: Heat load due  to e-cloud in the HL-LHC triplets

B2L1 A2L1

3L1 1L1

IP1, 4 TeV, β* = 0.6 m

IP1

1R1 (A/B)

2R1 (A/B)

3R1 (A/B)

Machine layout and optics near IP1 - HiLumi

Page 64: Heat load due  to e-cloud in the HL-LHC triplets

Bea

m 1

50 ns 3R1 sey = 1.40

20 40 60 800

2

4

x 109

e- per

uni

t len

gth

[m-1

]

Time [ns]

20 40 60 80

Bea

m 2

Time [ns]

The longitudinal direction

The delay between two following bunch passages changes along the machine elements

• Locations of long range encounters spaced by half the bunch spacing

15 m

Beam 2

Beam 1 IP1

50 ns spac.

Page 65: Heat load due  to e-cloud in the HL-LHC triplets

Average heat load density – 50 ns vs. 25 ns

1 1.2 1.4 1.6 1.8 20

1

2

3

4

5

6

7

8

9

10

SEY

Ave

rage

hea

t loa

d pe

r bun

ch [m

W/m

]

25 ns

1R1A2R1B2R13R1

1 1.2 1.4 1.6 1.8 20

1

2

3

4

5

6

7

8

9

10

SEY

Ave

rage

hea

t loa

d pe

r bun

ch [m

W/m

]

50 ns

1R1A2R1B2R13R1

Remarks:

• Above threshold values are very similar enhancement from hybrid spacings

much stronger on the 50 ns than on 25 ns

Page 66: Heat load due  to e-cloud in the HL-LHC triplets

A look to the EC buildup – HiLumi triplets

Few snapshots of the electron distribution much wider stripes

Page 67: Heat load due  to e-cloud in the HL-LHC triplets

Few snapshots of the electron distribution

Beam 1

A look to the EC buildup – present triplets

Page 68: Heat load due  to e-cloud in the HL-LHC triplets

A look to the EC buildup – HiLumi triplets

Few snapshots of the electron distribution much wider stripes