Polarized Positrons at a Linear Collider and FFTB (SLAC E-166) Achim W.
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Transcript Polarized Positrons at a Linear Collider and FFTB (SLAC E-166) Achim W.
Polarized Positrons at a Linear Collider
and FFTB (SLAC E-166)
Achim W. Weidemann
University of South Carolina, Columbia (@SLAC)
• Introduction (What, who)
• Motivation (Why)
• Experiment and Polarimetry (How)
• Outlook
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E-166 Experiment
E-166 is a demonstration of undulator-based
polarized positron production for linear colliders
• E-166 uses the 50 GeV SLAC beam in conjunction with 1 m-long, helical
undulator to make polarized photons in the FFTB.
• These photons are converted in a ~0.5 rad. len. thick target into polarized
positrons (and electrons).
• The polarization of the positrons and photons will be measured.
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E-166 Collaborators
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Physics Motivation for
Polarized Positrons
Polarized e+ in addition to polarized e- is recognized
as a highly desirable option by the WW LC
community (studies in Asia, Europe, and the US)
Having polarized e+ offers (next slides):
• Higher effective polarization -> enhancement of effective
luminosity for many SM and non-SM processes
• Ability to selectively enhance (reduce) contribution from
SM processes (better sensitivity to non-SM processes)
• Access to many non-SM couplings (larger reach for nonSM physics searches)
• Access to physics using transversely polarized beams
(only works if both beams are polarized)
• Improved accuracy in measuring polarization.
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Physics Motivation for
Polarized Positrons
– Electroweak processes e+e- -> WW, Z, ZH couple only to e-Le+R
or e-Re+L (and not e-Le+L or e-Re+R).
Can double or suppress rate using polarized positrons
(in addition to pol. e-).
– Effective polarization enhanced,
and error decreased, in electroweak
asymmetry measurements,
(NL – NR) / (NL + NR) = Peff ALR,
Peff = (P- - P+) / (1 – P-P+).
- Improved accuracy in polarization
measurement (Blondel scheme)
►Must have both e+ and epolarization for Giga-Z project
(sin2θW )
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(SUSY)Physics Motivation
for Polarized Positrons
Slepton and squark produced
dominantly via eR eL
(and not eReR or eLeL ).
Separation of the (LL, LR) selectron pair
eLeL
eLeR
with longitudinally polarized beams to test
association of chiral quantum numbers to
scalar fermions in SUSY :
With P(e-)= -80% and:
•P(e+)= 0% => no separation!
•P(e+)= -40% => 163fb vs 66 fb
Can’t do without positron polarization!
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Physics Motivation for
Polarized Positrons
• Transverse polarization of both beams
• ..allows separation of new physics, e.g.
extra dimensions
• More examples in JLC, TESLA TDRs,
Reviews, e.g. by G. Moortgat-Pick,
(POWER [Polarization at Work in
Energetic Reactions ] collaboration
http://www.ippp.dur.ac.uk/~gudrid/power/
)…
• Next question: How to make polarized
positrons?
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Polarized Positrons at LC
2 Target
assemblies
for
redundancy
(+ polarized
e- source)
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Polarized Positrons at FFTB
•
•
•
•
•
50 GeV, low emittance electron beam
2.4 mm period, K=0.17 helical undulator
10 MeV polarized photons
0.5 r.l. converter target
51%-54% positron polarization
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E-166 vs LC
E-166 is a demonstration of undulator-based production
of polarized positrons for linear colliders (next slide):
• Photons are produced in the same energy range and
polarization characteristics as in LC
• Same target thickness and material
• Polarization of the produced positrons is in the same
range as at LC
• Simulation tools, diagnostics: same as those being used
for LC polarized positron source
• But: the intensity per pulse is low by a factor of 2000.
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LC / E-166 Parameter Comparison
Table 1: TESLA, NLC/USLCSG, E-166 Polarized Positron Parameters
Parameter
Units
TESLA*
NLC
E-166
GeV
150-250
150
50
Beam Energy, Ee
10
9
3x10
8x10
1x1010
Ne/bunch
2820
190
1
Nbunch/pulse
Hz
5
120
30
Pulses/s
planar
helical
helical
Undulator Type
1
1
0.17
Undulator Parameter, K
cm
1.4
1.0
0.24
Undulator Period u
st
MeV
9-25
11
9.6
1 Harmonic Cutoff, Ec10
photons/m/e
1
2.6
0.37
dN /dL
m
135
132
1
Undulator Length, L
Ti-alloy Ti-alloy Ti-alloy, W
Target Material
r.l.
0.4
0.5
0.5
Target Thickness
%
1-5
1.8†
0.5
Yield
%
25
20
Capture Efficiency
12
12
8.5x10
1.5x10
2x107
N+/pulse
3x1010
8x109
2x107
N+/bunch
%
40-70
40-70
Positron Polarization
*TESLA baseline design; TESLA polarized e+ parameters (undulator and
polarization) are the same as for the NLC/USLCSG
† Including the effect of photon collimation at = 1.414.
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Helical Undulator l=2.4 mm,
K=0.17
Table 3: FFTB Helical Undulator System Parameters
Parameter
Number of Undulators
Length
Inner Diameter
Period
Field
Undulator Parameter, K
Current
Peak Voltage
Pulse Width
Inductance
Wire Type
Wire Diameter
Resistance
Repetition Rate
Power Dissipation
T/pulse
Energy
Units
m
mm
mm
kG
Amps
Volts
s
H
mm
ohms
Hz
W
0
C
Value
1
1.0
0.89
2.4
7.6
0.17
2300
540
30
0.9x10-6
Cu
0.6
0.110
30
260
2.7
Polarization
30.6 K 2
photons
/
m
/
e
0.37
photons
/
e
dL u mm 1 K 2
dN
Ec10 24 MeV
E
e
50 GeV
2
u mm 1 K 2
9.6 MeV
Alexander A. Mikhailichenko,
Pulsed Helical
Undulator….CBN 02-10, LCC-106
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Circ. γ -> long. e+ polarization
N(e+)
P(e
+)
P(e+)
Olsen & Maximon, 1959
0.5 r.l. Ti Alloy target; 0.5% yield, P(e+)=54% averaged over full spectrum
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Polarimeter Overview
4 x 109
4 x 107
1 x 1010 e 4 x 109
4 x 109
2 x 107 e+
2 x 107 e+
4 x 105 e+
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4 x 105 e+
1 x 103
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Photon Transmission Polarimetry
M. Goldhaber et al. Phys. Rev. 106 (1957) 826.
comp
phot comp pair
0 P Pe P
Pe 0.07
Pe / Pe 0.05
For photons of undulator spectrum, use number- or energy-weighted integral.
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Expected Photon
Polarimeter Performance
Si-W Calorimeter
Expected measured energy asymmetry δ = (E+-E-)/(E++E-)
and energy-weighted analyzing power AE
by analytic integration and, with good agreement, from polarized
GEANT simulation:
0.0266
Pe 0.07
AE 0.62
Energy-weighted Mean
Aerogel Cerenkov
will measure P for E > 5 MeV;
1% stat. measurements very fast (~ minutes),
main syst. error of ΔP /P ~ 0.05 from Pe
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Polarimetry of Positrons
2-step Process:
• re-convert e+ via brems/annihilation process
– polarization transfer from e+ to well-known
• measure polarization of re-converted photons with photon transmission
– infer P(e+) from measured photon polarization
Experimental Challenges:
• large angular distribution of the positrons at production target:
– e+ collection & transport efficiency; - background rejection issues
• angular distribution of the re-converted photons
– detected signal includes large fraction of Compton scattered photons
– requires simulations to determine effective Analyzing Power
14-20%
Formal Procedure:
Stat. Error (~108 photons /15 minutes) δ(P) ~ 2 – 4 %
Expected systematic Error of δ(P)/P ~5% dominated by eff. Magnetization of iron
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Polarimetry Summary
• Transmission polarimetry is well-suited for photon and
positron beam measurements in E166
• Analyzing power determined from simulations
is sufficiently large and robust
• Measurements will be very fast with negligible statistical
errors
• Expect systematic errors of ΔP/P ~ 0.05
from magnetization of iron
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E-166 Outlook
•
•
•
•
Experiment approved mid-June 2003;
…with proviso: should study backgrounds first;
Installation under way now (Aug.2004)
Will run Oct.2004, Jan 2005 (….before end of
2005, after which FFTB will become LCLS)
• Hope to blaze the way for polarised positrons at
a future LC!
For References, details see:
http://www.slac.stanford.edu/exp/e166
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Backup Slides
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Positron Polarimeter Layout
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Photon Detectors
For Photons:
Threshold Cerenkov (AeroGel)
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Si-W Calorimeter
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Positron Transport System
e+
transmission
(%) through
spectrometer
photon
background
fraction
reaching
CsIdetector
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CsI Calorimeter Detector
Crystals:
Number of crystals:
Typical front face of one crystal:
Typical backface of one crystal:
Typical length:
Density:
Rad. Length
Mean free path (5 MeV):
No. of interaction lengths (5 MeV):
Long. Leakage (5 MeV):
from BaBar Experiment
4 x 4 = 16
4.7 cm x 4.7 cm
6 cm x 6 cm
30 cm
4.53 g/cm³
8.39 g/cm² = 1.85 cm
27.6 g/cm² = 6.1 cm
4.92
0.73 %
Photodiode Readout (2 per crystal):
Hamamatsu S2744-08
with preamps
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Expected Positron
Polarimeter Performance
Expected systematic Error of δ(P)/P ~5% dominated by eff. Magnetization of iron
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