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Challenges for Polarimetry at the ILC Spin Tracking Studies Moritz - - PowerPoint PPT Presentation

Challenges for Polarimetry at the ILC Spin Tracking Studies Moritz Beckmann, Jenny List DESY - FLC LCWS 2012, Arlington, TX, USA October 25, 2012 Introduction: Polarimetry at the ILC Two laser Compton polarimeters per beam in the beam


slide-1
SLIDE 1

Challenges for Polarimetry at the ILC

Spin Tracking Studies Moritz Beckmann, Jenny List

DESY - FLC

LCWS 2012, Arlington, TX, USA October 25, 2012

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SLIDE 2

Introduction: Polarimetry at the ILC

  • Two laser Compton polarimeters per beam in the beam

delivery system (BDS)

150 m ~1 650 m upstream polarimeter IP downstream polarimeter

  • Polarimeters measure with 0.25 % systematic uncertainty

(goal)

  • What happens between polarimeter and IP?

Moritz Beckmann (DESY) LCWS Oct 25, 2012 2/ 17

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SLIDE 3

Introduction: Polarimetry at the ILC

  • Two laser Compton polarimeters per beam in the beam

delivery system (BDS)

150 m ~1 650 m upstream polarimeter IP downstream polarimeter

  • Polarimeters measure with 0.25 % systematic uncertainty

(goal)

  • What happens between polarimeter and IP?
  • In addition: calibration with average polarization from

collision data (up to 0.1 %)

  • Must understand spin diffusion/depolarization to 0.1 %

Moritz Beckmann (DESY) LCWS Oct 25, 2012 2/ 17

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SLIDE 4

Introduction: Simulation Framework

UP IP DP Particle / spin tracking along the BDS Bmad Beam-beam collision GP++/CAIN Data analysis ROOT Polarimeter simulation LCPolMC Polarimeter simulation LCPolMC

UP/DP: up-/downstream polarimeter

Framework could be used with different input also for other machines, e. g. CLIC

Moritz Beckmann (DESY) LCWS Oct 25, 2012 3/ 17

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SLIDE 5

Introduction: Principles of Spin Propagation

  • Spin propagation in electromagnetic fields

is described by T-BMT equation (semi- classical)

  • Approximation (

B⊥ only) for illustration: spin precession θspin =

  • g−2

2

· E

m + 1

  • ≈568

·θorbit

B

Moritz Beckmann (DESY) LCWS Oct 25, 2012 4/ 17

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SLIDE 6

Introduction: Principles of Spin Propagation

  • Spin propagation in electromagnetic fields

is described by T-BMT equation (semi- classical)

  • Approximation (

B⊥ only) for illustration: spin precession θspin =

  • g−2

2

· E

m + 1

  • ≈568

·θorbit

B

  • Polarization vector

P =   Px Py Pz   with polarization

  • P
  • Moritz Beckmann (DESY)

LCWS Oct 25, 2012 4/ 17

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SLIDE 7

Introduction: ILC Beam Delivery System

Latest available beamline design (SB2009 Nov10 lattice)

Moritz Beckmann (DESY) LCWS Oct 25, 2012 5/ 17

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SLIDE 8

Spin Propagation through BDS (Idealized Lattice)

distance s along BDS [m]

500 1000 1500 2000 2500 3000 3500

polarization

  • 0.8
  • 0.6
  • 0.4
  • 0.2

0.2 0.4 0.6 0.8

UP IP DP

  • e

z

P | P |

UP/DP: up-/downstream polarimeter

  • 1000 runs with random bunches, 10 000 sim. particles each
  • Drawn: median ± 1σ
  • Perfect magnet alignment, no collision effects

Moritz Beckmann (DESY) LCWS Oct 25, 2012 6/ 17

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SLIDE 9

Spin Fan-Out

distance s along BDS [m]

3400 3450 3500 3550

polarization

0.7992 0.7994 0.7996 0.7998 0.8

]

  • 3

relative change [10

  • 1
  • 0.5

IP DP

  • e

z

P | P |

Only minor spin fan-out in quadrupoles

Moritz Beckmann (DESY) LCWS Oct 25, 2012 7/ 17

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SLIDE 10

Spin Fan-Out

distance s along BDS [m]

3400 3450 3500 3550

polarization

0.7992 0.7994 0.7996 0.7998 0.8

]

  • 3

relative change [10

  • 1
  • 0.5

IP DP

  • e

z

P | P |

Only minor spin fan-out in quadrupoles

P P' P

Moritz Beckmann (DESY) LCWS Oct 25, 2012 7/ 17

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SLIDE 11

Collision Effects

Simulation of Collision Effects (GP++):

  • T-BMT precession: deflection from colliding bunch

(∼ 10−4 rad)

  • Sokolov-Ternov: spin flip by emission of beamstrahlung

Moritz Beckmann (DESY) LCWS Oct 25, 2012 8/ 17

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SLIDE 12

Collision Effects: Energy Loss

  • Energy loss by beamstrahlung:
  • 0.6
  • 0.4
  • 0.2

# of entries

1 10

2

10

3

10

4

10

5

10

6

10

7

10

particle energy [GeV]

100 150 200 250

before collision after collision

  • Spin precession ∝ E

⇒ Spin fan-out due to energy spread

Moritz Beckmann (DESY) LCWS Oct 25, 2012 9/ 17

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SLIDE 13

Collision Effects: Energy Loss vs. Laser-Spot

  • Laser-spot size at Compton IP only ∼ 0.1 − 1 mm
  • chicane ⇒ dispersion (black: reference particle)
  • Without collision: 0.124 % beam energy spread

Entire beam within laser-spot

  • 0.005

0.005

  • 0.15
  • 0.1
  • 0.05

0.05 0.1 0.15

  • 3

10 ×

1 10

2

10

3

10

4

10

5

10

no collision

particle energy [GeV]

249 250 251

vertical particle position y [mm]

  • 0.1

0.1 Moritz Beckmann (DESY) LCWS Oct 25, 2012 10/ 17

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SLIDE 14

Collision Effects: Energy Loss vs. Laser-Spot

  • Laser-spot size at Compton IP only ∼ 0.1 − 1 mm
  • chicane ⇒ dispersion (black: reference particle)
  • After collision: Off-energy particles evade laser-spot
  • Downstream polarimeter needs detailed investigation

(energy and polarization correlated!)

  • 0.4
  • 0.3
  • 0.2
  • 0.1
  • 0.02
  • 0.015
  • 0.01
  • 0.005

0.005 0.01 0.015 0.02

1 10

2

10

3

10

4

10

5

10

6

10

after collision

particle energy [GeV]

150 200 250

vertical particle position y [mm]

  • 20
  • 10

10 20 Moritz Beckmann (DESY) LCWS Oct 25, 2012 11/ 17

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SLIDE 15

Collision Effects: Spin Propagation

  • Collisions, but still perfect alignment
  • Crossing angle 14 mrad, bunches crabbed

distance s along BDS [m]

3400 3450 3500 3550

z

  • long. polarization P

0.77 0.78 0.79 0.8

]

  • 3

relative change [10

  • 40
  • 30
  • 20
  • 10

IP DP

  • e

no collision lumi-weighted after collision measurable

  • Much stronger spin fan-out
  • Polarization within 0.1 mm laser-spot different: “measureable”

Moritz Beckmann (DESY) LCWS Oct 25, 2012 12/ 17

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SLIDE 16

Collision Effects: Spin Propagation

10 20 30

z

longitudinal polarization P

0.77 0.78 0.79 0.8

]

  • 3

relative change [10

  • 40
  • 30
  • 20
  • 10

no coll. full lumi

UP IP before collision IP lumi-weighted IP after collision DP DP measurable (r=0.1, 0.2, 0.5, 1 mm)

Moritz Beckmann (DESY) LCWS Oct 25, 2012 13/ 17

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SLIDE 17

Collision Effects: Spin Propagation

10 20 30

z

longitudinal polarization P

0.77 0.78 0.79 0.8

]

  • 3

relative change [10

  • 40
  • 30
  • 20
  • 10

no coll. full lumi

UP IP before collision IP lumi-weighted IP after collision DP DP measurable (r=0.1, 0.2, 0.5, 1 mm)

2.5% ≈ 0.3% ≈

  • What does the measurement tell us about the

polarization at the IP?? ∆Pz ∼ 2.5 %

  • Can we trust the simulation to calculate back?

More details to come: detector magnets, misalignments

  • Uncertainty in DP laser-spot size/position

⇒ ∆Pz = O(0.1 %)

Moritz Beckmann (DESY) LCWS Oct 25, 2012 14/ 17

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SLIDE 18

Collision Effects: Spin Propagation

10 20 30

z

longitudinal polarization P

0.77 0.78 0.79 0.8

]

  • 3

relative change [10

  • 40
  • 30
  • 20
  • 10

no coll. low lumi full lumi

UP IP before collision IP lumi-weighted IP after collision DP DP measurable (r=0.1, 0.2, 0.5, 1 mm)

Low luminosity sample (switched off bunch crabbing):

  • Collision effects and also their consequences reduced
  • Downstream measurement less affected by collision effects

and less dependent on laser-spot size/position

Moritz Beckmann (DESY) LCWS Oct 25, 2012 15/ 17

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SLIDE 19

Conclusion

  • A spin tracking framework for high energy linear colliders

including collision effects has been set up

  • ILC: understanding of polarization to permille-level required
  • Precision goals for upstream measurement seem achievable

Moritz Beckmann (DESY) LCWS Oct 25, 2012 16/ 17

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SLIDE 20

Conclusion

  • A spin tracking framework for high energy linear colliders

including collision effects has been set up

  • ILC: understanding of polarization to permille-level required
  • Precision goals for upstream measurement seem achievable
  • Downstream polarimeter struggles fiercely with collision

effects:

  • High-precision simulation including all effects required at

high luminosities to obtain polarization at IP from data

  • Measurement highly sensitive to size/position of laser-spot
  • Idea: determine lumi-weighted polarization rather/also from

upstream polarimeter and luminosity measurement?

Moritz Beckmann (DESY) LCWS Oct 25, 2012 16/ 17

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SLIDE 21

Conclusion

  • A spin tracking framework for high energy linear colliders

including collision effects has been set up

  • ILC: understanding of polarization to permille-level required
  • Precision goals for upstream measurement seem achievable
  • Downstream polarimeter struggles fiercely with collision

effects:

  • High-precision simulation including all effects required at

high luminosities to obtain polarization at IP from data

  • Measurement highly sensitive to size/position of laser-spot
  • Idea: determine lumi-weighted polarization rather/also from

upstream polarimeter and luminosity measurement?

  • Downstream polarimeter needed nevertheless:
  • Measure depolarization without collision effects / calibrate UP
  • Measure additional depolarization at low luminosities to test

simulations

Moritz Beckmann (DESY) LCWS Oct 25, 2012 16/ 17

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SLIDE 22

Thanks for your attention!

Thanks for support and useful discussions to:

  • David Sagan (Cornell U.)
  • Deepa Angal-Kalinin (Daresbury Lab.)
  • Anthony Hartin, Mathias Vogt, Nick Walker (DESY)
  • Andrei Seryi (JAI)
  • Kenneth Moffeit, Yuri Nosochkov, Michael Woods (SLAC)
  • Jeff Smith (formerly SLAC)
  • und many others...

Moritz Beckmann (DESY) LCWS Oct 25, 2012 17/ 17

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SLIDE 23

Backup slides

Moritz Beckmann (DESY) LCWS Oct 25, 2012 18/ 17

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SLIDE 24

Compton Polarimeters: Principles

  • Compton scattering with polarized laser:

∼ 1500 electrons per bunch

  • Measure energy spectrum of scattered electrons
  • Energy distribution → spatial distribution
  • Cherenkov gas detector counts electrons per channel

Moritz Beckmann (DESY) LCWS Oct 25, 2012 19/ 17

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SLIDE 25

Compton Polarimeters: Principles

50 100 150 200 250 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0

σ Compton [mbarn / GeV]

Compton−scattered Electron Energy [GeV] λ Pe = +1

(same)

λ Pe = −1

(opposite)

  • σCompton depends on polarization (laser × beam)
  • Measure asymmetry and compare to analyzing power

(predicted asymmetry for 100 % polarization)

Moritz Beckmann (DESY) LCWS Oct 25, 2012 20/ 17

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SLIDE 26

Compton Polarimeters: Systematic Errors

Goal: relative systematic error on measurement < 0.25 % (SLC polarimeter: 0.5 %)

  • Detector linearity: contribution of ∼ 0.1 − 0.2 % (goal)

Prototype tests ongoing . . .

  • Laser polarization: ∼ 0.1 %

Moritz Beckmann (DESY) LCWS Oct 25, 2012 21/ 17

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SLIDE 27

Compton Polarimeters: Systematic Errors

Goal: relative systematic error on measurement < 0.25 % (SLC polarimeter: 0.5 %)

  • Detector linearity: contribution of ∼ 0.1 − 0.2 % (goal)

Prototype tests ongoing . . .

  • Laser polarization: ∼ 0.1 %
  • Analyzing power: ∼ 0.1 % (UP: , DP: ?)
  • Detector alignment: can be determined from data ()

0.5 mm precision sufficient

  • Alignment of magnets negligible compared to detector

Field inhomogeneities? to be investigated

  • Disrupted electron beam at downstream polarimeter:
  • Dependence on laser-spot size and position: ??
  • Beam energy spread no concern for small laser-spot sizes

thanks to dispersion

Moritz Beckmann (DESY) LCWS Oct 25, 2012 21/ 17

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SLIDE 28

Misalignments

  • Every element is shifted/rotated randomly in/about all

directions/axes

  • Gaussian-distributed random numbers, σ = 10 µm/µrad
  • Static and time-dependent misalignments

Moritz Beckmann (DESY) LCWS Oct 25, 2012 22/ 17

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SLIDE 29

Misalignments

  • Every element is shifted/rotated randomly in/about all

directions/axes

  • Gaussian-distributed random numbers, σ = 10 µm/µrad
  • Static and time-dependent misalignments
  • Simplified orbit correction with kicker magnets and fast

feedback at IP

Moritz Beckmann (DESY) LCWS Oct 25, 2012 22/ 17

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SLIDE 30

Misalignments: Correction with Kicker Magnets BPM kicker magnet beam design orbit

  • ∼ 40 kicker magnets and many more Beam Position Monitors

spread over BDS

  • Calculate required kicks from measurements (SVD)
  • Automatic correction of spin alignment as well?

Moritz Beckmann (DESY) LCWS Oct 25, 2012 23/ 17

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SLIDE 31

Misalignments: Orbit Correction Strategy

Strategy here:

  • Interested in effects of kicks on polarization,

not in sophisticated correction algorithm

  • Get orbit corrected somehow with kickers such that
  • beam does no go lost
  • approximations (small coordinates) still hold

Moritz Beckmann (DESY) LCWS Oct 25, 2012 24/ 17

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SLIDE 32

Misalignments: Orbit Correction Strategy

Strategy here:

  • Interested in effects of kicks on polarization,

not in sophisticated correction algorithm

  • Get orbit corrected somehow with kickers such that
  • beam does no go lost
  • approximations (small coordinates) still hold
  • Fake correction at IP: shift and rotate bunch coordinates to

0.1 σ precision (goal), adjust beam size

Moritz Beckmann (DESY) LCWS Oct 25, 2012 24/ 17

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SLIDE 33

Misalignments: Spin Propagation

  • Misalignments reduce luminosity ⇒ less collision effects
  • Measured polarization depends on laser-spot size and position

10 20 30 40

z

longitudinal polarization P

0.77 0.78 0.79 0.8

]

  • 3

relative change [10

  • 40
  • 30
  • 20
  • 10

ideal FFB µ 5 µ 10

  • e

UP IP before collision IP lumi-weighted IP after collision DP DP measurable (r=0.1, 0.5, 1 mm)

Moritz Beckmann (DESY) LCWS Oct 25, 2012 25/ 17

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SLIDE 34

Collision Effects: Energy Loss vs. Laser-Spot

  • Laser-spot size at Compton IP only ∼ 100 µm − 1 mm
  • chicane ⇒ dispersion (black: reference particle)
  • After collision, bunch crabbing switched off
  • 0.4
  • 0.3
  • 0.2
  • 0.1
  • 0.02
  • 0.015
  • 0.01
  • 0.005

0.005 0.01 0.015 0.02

1 10

2

10

3

10

4

10

5

10

6

10

after collision

particle energy [GeV]

150 200 250

vertical particle position y [mm]

  • 20
  • 10

10 20 Moritz Beckmann (DESY) LCWS Oct 25, 2012 26/ 17

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SLIDE 35

Collision Effects: Spin Propagation (Polarization)

  • Total polarization affected likewise
  • Polarization decrease in chicanes: fan-out due to energy

spread

distance s along BDS [m]

3400 3450 3500 3550

| P total polarization |

0.77 0.78 0.79 0.8

]

  • 3

relative change [10

  • 40
  • 30
  • 20
  • 10

IP DP

  • e

Moritz Beckmann (DESY) LCWS Oct 25, 2012 27/ 17

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SLIDE 36

Collision Effects: Spin Propagation (Positron Beam)

10 20 30

z

longitudinal polarization P

0.29 0.295 0.3

]

  • 3

relative change [10

  • 40
  • 30
  • 20
  • 10

no coll. low lumi full lumi

UP IP before collision IP lumi-weighted IP after collision DP DP measurable (r=0.1, 0.2, 0.5, 1 mm)

Moritz Beckmann (DESY) LCWS Oct 25, 2012 28/ 17

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SLIDE 37

Collision & Misalignments: Downstream Polarimeter Measurement

  • 0.4
  • 0.3
  • 0.2
  • 0.1
  • 0.02
  • 0.015
  • 0.01
  • 0.005

0.005 0.01 0.015 0.02

1 10

2

10

3

10

4

10

5

10

after collision

particle energy [GeV]

150 200 250

vertical particle position y [mm]

  • 20
  • 10

10 20

Moritz Beckmann (DESY) LCWS Oct 25, 2012 29/ 17

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SLIDE 38

Luminosity

  • Design values 1.8(1.5) · 1038 m−2s−1 (without waist shift)
  • Need to improve tuning of grid parameters in GP++
  • Does not change statement of this talk (effects might just

get stronger for higher luminosities)

2000 3000 4000 5000 ×

# of entries

20 40 60 80 100 120 140 160 180 200 0.1 0.2 0.3 (a) 0.008 ± : 0.165 σ ± µ 12 14 16 18

33

10 × 20 40 60 80 100 120 140 160 180 200

]

  • 1

s

  • 2

m ⋅

38

luminosity [10

  • e

+

e

0.8 0.9 1 1.1 1.2 (b) 0.010 ± : 0.862 σ ± µ 0.012 ± : 0.833 σ ± µ

CC on CC off CC on, no WS

Moritz Beckmann (DESY) LCWS Oct 25, 2012 30/ 17

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SLIDE 39

Polarization correction by angle measurement?

  • Detector solenoid and anti-DID
  • θr: angular spread within bunch
  • Solenoid field invalidates “B⊥ only” approximation
  • Still sharp value for b (ϑpol = b · ϑbunch) due to ideal

conditions (no misalignments)

3410 3412 3414 0.05 0.1 0.15 10 ×

rad] µ angle [

50 100 150

entrance solenoid IP

r

θ

bunch

ϑ b

3410 3412 3414

b [1]

200 400 600

distance to IP [m]

  • 4
  • 3
  • 2
  • 1

γ b=a

Moritz Beckmann (DESY) LCWS Oct 25, 2012 31/ 17

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SLIDE 40

Polarization correction by angle measurement?

  • This plot without detector magnets
  • Small misalignments (2µm / 2µrad) make correction for

incident angle impossible, since there is no more simple correlation between angles of bunch and polarization vector

  • “Steps” due to correction kickers with zero length

3410 3412 3414 0.02 0.04 0.06 10 ×

rad] µ angle [

20 40 60

entrance solenoid IP

r

θ

bunch

ϑ b

3410 3412 3414

b [1]

1000 2000 3000 4000 5000

distance to IP [m]

  • 4
  • 3
  • 2
  • 1

γ b=a

Moritz Beckmann (DESY) LCWS Oct 25, 2012 32/ 17

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SLIDE 41

Polarization

  • Here: longitudinal polarization Pz

(along beam axis)

  • Pz = pR − pL ∈ [−1, +1]
  • Beam with 90% R (and thus 10% L)

→ 80% longitudinal polarization

  • More general: polarization vector
  • P =

  Px Py Pz   with polarization

  • P
  • Moritz Beckmann (DESY)

LCWS Oct 25, 2012 33/ 17