beam instrumentation tests for the linear collider
DESCRIPTION
Beam Instrumentation Tests for the Linear Collider. SLAC EPAC Meeting Nov. 14, 2003. M. Woods, SLAC. Luminosity, Energy and Polarization measurements at the Linear Collider (LC-LEP measurements) SLAC A-Line and End Station A Facility Beam Characteristics and Comparison with NLC Beam - PowerPoint PPT PresentationTRANSCRIPT
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Beam Instrumentation Tests Beam Instrumentation Tests for the Linear Colliderfor the Linear Collider
SLAC EPAC MeetingNov. 14, 2003 M. Woods, SLAC
Luminosity, Energy and Polarization measurements at the Linear Collider(LC-LEP measurements)
SLAC A-Line and End Station A FacilityBeam Characteristics and Comparison with NLC BeamBeam Diagnostics
LC-LEP Beam Tests at SLAC
Request to EPAC
M. Woods (SLAC)
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Beam Instrumentation Tests for the Linear ColliderBeam Instrumentation Tests for the Linear Colliderusing the SLAC A-Line and End Station Ausing the SLAC A-Line and End Station A
SLAC-LOI-2003.2Y. KolomenskyUniversity of California, Berkeley
J. Hauptman, O. AtramentovIowa State University
E. Gulmez,† E. Norbeck, Y. Onel, A. Penzo*University of Iowa
D. J. MillerUniversity College London
R. Arnold, S. Hertzbach, S. RockUniversity of Massachussets
M. HildrethUniversity of Notre Dame
E. TorrenceUniversity of Oregon
J. Clendenin, F.-J. Decker, R. Erickson, J. Frisch, L. Keller, T. Markiewicz, T. Maruyama, K. Moffeit, M. Ross, J. Turner, M. Woods
SLAC
W. OliverTufts University
G. Bonvicini, D. CinabroWayne State University
†also Bogazici University, Istanbul, Turkey*also INFN Trieste, Italy
27 physicists10 institutions
http://www.slac.stanford.edu/grp/rd/epac/LOI/LOI-2003.2.pdf
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Luminosity, Energy and Polarization Luminosity, Energy and Polarization measurements at the Linear Collidermeasurements at the Linear Collider
(LC-LEP measurements)(LC-LEP measurements)
M. Woods (SLAC)
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WG Scope Beam Instrumentation required for LC Physics
PrincipleTopics (L,E,P)• Luminosity, luminosity spectrum (dL/dE) • Energy scale and width• Polarization
IP Beam InstrumentationIP Beam Instrumentation
ALCPG Working GroupALCPG Working Group
Also• Instrumentation for optimizing Luminosity
- IP BPMs for fast feedback and feedforward- detectors for pairs, beamstrahlung, radiative Bhabhas
M. Woods (SLAC)
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Energy
• Top mass: 200 ppm (35 MeV)• Higgs mass: 200 ppm (25 MeV for 120 GeV Higgs)• W mass: 50 ppm (4 MeV) ??• ‘Giga’-Z ALR: 200 ppm (20 MeV) (comparable to ~0.25% polarimetry)
50 ppm (5 MeV) (for sub-0.1% polarimetry with e+ pol) ??
LC-LEP Measurement GoalsLC-LEP Measurement Goals
Luminosity, Luminosity Spectrum
• Total cross sections: absolute L/L to ~0.1%• Z-pole calibration scan for Giga-Zrelative LLto ~0.02%• threshold scans (ex. top mass): relative LLto 1%
+L(E) spectrum: core width to <0.1% andtail population to <1%
Polarization
• Standard Model asymmetries: < 0.5%• ‘Giga’-Z ALR: < 0.25%
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disrupted beam(w/ beamstrahlung radiation
effect included)
radiative Bhabhasfrom pair production
Energy spectrum of electrons in extraction line after IPat NLC-500
Beamstrahlung at the Linear ColliderBeamstrahlung at the Linear Collider
~7% of the beam energygets radiated into photons due to beamstrahlung(at SLC this was 0.1%)
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PP
EEwtlum
wtlum
How well the luminosity-weighted quantities can be determineddepends on the beam parameters at the IP, as well as on the intrinsic capabilities of the polarimeter and the energy spectrometers.
The beam diagnostics measure <E>, <P>. The beam diagnostics measure <E>, <P>. For physics we need to know <E>For physics we need to know <E>lum-wtlum-wt, <P>, <P>lum-wtlum-wt . .
Strategy is to use a combination of beam diagnostics andphysics-based detector measurements. Need to understand L(E) spectrumand how it is affected from beamstrahlung and energy spread,as well as from initial state radiation.
100-200 ppm physics goal for determining <E><E>lum-wtlum-wt
<< 3000ppm energy spread <<< 70,000 ppm energy loss due to beamstrahlung!
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LC Detector Measurements of L(E), LC Detector Measurements of L(E), <E><E>lum-wtlum-wt, <P>, <P>lum-wtlum-wt
Luminosity Spectrum, L(E) Bhabha Acolinearity: 1
2
z-axis
p1
p2
sin
21
21
A
beam
A
p
p
ppp
<P>lum-wt
Asymmetry in forward W-pairs
<E>lum-wt
Radiative return to Z events W-pair events
These techniques don’t replace the need for real-time beam-based measurements.Want complementary and/or combined analyses with beam-based measurements.
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Example of Lum-wted Energy BiasExample of Lum-wted Energy Biasrelated to Beam Energy Spread at NLC-500related to Beam Energy Spread at NLC-500
Head
Tail
For this study, turn off ISR and beamstrahlung and only consider beam energy spread.
Incident beam Incident beam
ppm500GeV 500
GeV 500'
s
Ewtlum
cm
Lum-wted ECM
Bhabha acolinearity analysis alonewon’t help resolve this bias.
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Instrumentation for Luminosity, Luminosity SpectraInstrumentation for Luminosity, Luminosity Spectraand Luminosity Tuningand Luminosity Tuning
Luminosity Bhabha LuMon detector from 40-120 mrad
Luminosity SpectrumBhabha acolinearity measurements using forward tracking
and calorimetry from 120-400 mrad+ additional input from beam energy, energy spread and energy spectrum
measurements
Luminosity TuningPair LuMon detector from 5-40 mradBeamstrahlung detector from 1-2 mrad (further downstream)IP BPMs
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-0.5
-0.4
-0.3
-0.2
-0.1
0
0.1
0.2
0.3
0.4
0.5
0 0.5 1 1.5 2 2.5 3 3.5 4
QD0
HCAL
ECAL
YOKE
Tungsten
46mrad
113mrad
Support Tube
Pair LuMon
BeamPipeLowZ Mask Exit radius 2cm
@ 3.5mTungsten
incoming e+
outgoing e-
z (meters from IP)
Forward Tracking, Calorimetry and MaskingForward Tracking, Calorimetry and Masking(for NLC Silicon Detector)(for NLC Silicon Detector)
Bhabha LuMon
IP BPMs for fast feedback and feed forward @ ~z = 3.5 meters
y (m
eter
s)
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Using Pairs and Beamstrahlung forUsing Pairs and Beamstrahlung forLuminosity TuningLuminosity Tuning
1. Angular distributions of low energy e+e- pairs from 2-photon processesT. Tauchi and K. Yokoya, Phys. Rev. E51 (1995) 6119-6126.
2. Measuring polarization of the beamstrahlung emitted at angles of (1-2) mrad.G. Bonvicini, N. Powell (2003) hep-ex/0304004; submitted to Phys.Rev.E
2 promising detector techniques for determining beam offsets and individual beamsizes:
7 degrees-of-freedom for colliding bunches:• individual spotsizes (4)• relative offset (2)• relative tilt of bunches (1)
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NLC e+e-
TESLA e+e-NLC e+e-
TESLA e+e-
Using IP BPMs for Luminosity TuningUsing IP BPMs for Luminosity Tuning
Luminosity vs vertical offsetDeflection angle vs vertical offset
Slow (inter-train) and fast (ns-timescale intra-train) feedbacksare planned
Two of the highest risk factors for achieving LC design luminosity are:i) reliance on IP feedbacks and ii) effects of backgrounds (beam-beam and other) on detectors
and beam instrumentation
Fast IP Beam diagnostics must work as planned and be robust against backgrounds
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Instrumentation for Energy, Energy SpreadInstrumentation for Energy, Energy Spreadand disrupted Energy Spectrumand disrupted Energy Spectrum
EnergyBPM spectrometer (upstream of IP)Synchrotron Stripe spectrometer (in extraction line)
Energy SpreadSynchrotron Stripe spectrometer (in extraction line)Wire scanner at high dispersion point in extraction line chicane
Disrupted Energy SpectrumSynchrotron Stripe spectrometer (in extraction line)Wire scanner at high dispersion point in extraction line chicane
Proposed BPM spectrometer at NLCSynchrotron Stripe Spectrometer
at SLC
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Instrumentation for PolarimetryInstrumentation for Polarimetry
Compton Polarimeter in Extraction Line
2mrad
Thin Radiator
Compton IP
Pair SpectrometerElectron Detector
Pair SpectrometerPositron Detector
Back Scattered Photons
Input Laser Light 11.5 mrad
Ken Moffeit
107 GeV
125 Gev
Electron beam
93.8 GeV positrons
100 GeV electrons
4 cm
Beam Stay Clear 1 mrad from IP
Beam Stay Clear 1 mrad from IP
2 cm
30 Meters
13
cm1
2 cm
25 GeV
electron
37.5 GeV
7 cm
Compton ElectronDetector
Chicane bend magnets
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M. Woods (SLAC)
LCRD and UCLCLCRD and UCLC
FY04 R&D Proposals to DOE and NSFFY04 R&D Proposals to DOE and NSF
LuminosityFast Gas Cherenkov Calorimeter (Iowa St.)Parallel Plate Avalanche, Secondary Emission Detectors (Iowa)Large Angle Beamstrahlung Monitor (Wayne St.)3d Si Detector for Pair Monitor (Hawaii)
EnergySynchrotron Stripe Spectrometer (Oregon, UMass)rf BPM Spectrometer (Notre Dame, UC Berkeley)
PolarizationQuartz Fiber Calorimeter; W-pair asymmetry (Iowa)Background study (Tufts)Quartz Fiber Detector; transverse polarization (Tennessee)
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SLAC A-Line and End Station A Facility SLAC A-Line and End Station A Facility for LC-LEP measurementsfor LC-LEP measurements
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SLAC A-Line and End Station A FacilitySLAC A-Line and End Station A Facility• Beam Characteristics and Comparison with NLC Beam
• Beam Diagnostics
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Beam Parameters for SLAC E-158 and NLC-500Beam Parameters for SLAC E-158 and NLC-500
Parameter SLAC E-158 NLC-500
Charge/Train 6 x 1011 14.4 x 1011
Repetition Rate 120 Hz 120 Hz
Energy 45 GeV 250 GeV
e- Polarization 85% 85%
Train Length 270ns 267ns
Microbunch spacing 0.3ns 1.4ns
Beam Loading 13% 22%
Energy Spread 0.15% 0.3%
Intensity Jitter 0.5% rms 0.5% rms
Energy Jitter 0.03% rms 0.3% rms
Transverse Jitter 5% of spotsize (x or y) 22% of x spotsize,
50% of y spotsize
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Use 178.5MHz SHB cavity
BPM electrode signal
LI30 201X
But, beam in LINAC is unstable. - some evidence for beam breakup - needs further study
NLC Bunching StudyNLC Bunching Study
Bunch Train with • 5.6ns spacing• ~1010 bunch charge
PPRC is starting a new R&D project to achieve 714MHz modulation(1.4ns bunch spacing) of the Long Pulse laser used for the Source
- will use an electro-optic modulator driven with 714MHz rf- will experiment both with intra-cavity modulation and an
external modulator
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Beam Diagnostics for SLAC E-158Beam Diagnostics for SLAC E-158
energy ~1 MeV
Agreement (MeV)
BPM
24
X (
MeV
)
BPM12 X (MeV)
toroid ~30 ppm BPM ~2 microns
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A-Line Synchrotron Light Monitor (SLM)A-Line Synchrotron Light Monitor (SLM)
electron beamvisible SR
visible SR
imaging telescope
gated ccdcamera
Energy and Energy spread (in MeV) in 60-ns time slicesalong the 300ns train for 45 GeV beam
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Target chamber
Dipoles
Beam Monitors
Detector Cart
Drift pipe
Quadrupoles
LuminosityMonitor
Concrete Shielding
60 m
End Station AEnd Station A configured for E-158configured for E-158
Target Station
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LC-LEP Beam Tests at SLAC LC-LEP Beam Tests at SLAC
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BPM TestsBPM Tests(Energy Spectrometer BPMs and IP BPMs)(Energy Spectrometer BPMs and IP BPMs)
1. Characterize performance of LC BPMsTemporal response and resolution; comparewith existing high resolution diagnostics(SLM at high dispersion point and wire arrayat target)
A-Line 45 GeV
Beams can have temporal ‘banana’ shape in position, angle, energy
2. Mimick ‘beamstrahlung and disruption’for IP bpms using a thick target in ESA;compare LC bpm measurement 4 meters downstreamof target with precision upstream bpms
NLC-500ESA-25GeV (w/ 10% X0 Carbon target)
<5mrad production angle
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NLC-500 ESA
(SLAC)
NLCTA
(SLAC)
FFTB
(SLAC)
ATF
(KEK)
Beam Energy 250 GeV 25 GeV 65 MeV 25 GeV 1.3 GeV
Bunch charge per 1.4ns 0.75 x 1010 0.25 x 1010 109 1010 109
Bunch spacing 1.4ns 0.36ns* 0.09 - 2.8 ns
bunches per train 190 830 1900 1 20
Train length 267 ns 300 ns 170 ns - 60 ns †
IP BPM type Stripline Stripline Button Stripline rf cavity
Accelerator Facilities for LC BPM TestsAccelerator Facilities for LC BPM Tests
*new PPRC project is attempting to produce 714MHz modulation of long pulse beam†ATF will attempt 3-train operation with 60-ns gaps between trains for 300-ns train length
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NLC-500 ESA
Beam Energy 250 GeV 25 GeV
Incoming beam divergence (x,y) 3 rad; 3 rad 40 rad; 30 rad
Outgoing beam divergence (x,y) 170 rad; 170 rad 240 rad; 100 rad
RMS spotsize at IP,Target (x,y) 500 m; 500 m 0.24 m; 0.003 m
RMS spotsize @ z=3.5m (x,y) 710 m; 710 m 840 m; 350 m
Comparison of Beam Spotsizes and Divergences at NLC-500Comparison of Beam Spotsizes and Divergences at NLC-500and ESA and ESA (w/ 10% X0 target)
Similar divergences and spotsizes at IP BPM location
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NLC-500 ESA-25GeV
Photon Distributions downstream of IP(Target)Photon Distributions downstream of IP(Target)
ESA-25 GeV
NLC-500
Beam Energy 25 GeV 250 GeV
#photons/electron 1.34 1.60
<E>/Ebeam 0.068 0.041
E/Ebeam 0.092 0.066
<E> 1.7 GeV 10.3 GeV
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Beam Tests for Pair detectorsBeam Tests for Pair detectors
Test performance of high rate pair detector - use thinner target to match rates and hit density- test temporal response over 300ns train
NLC-500 (per colliding bunch)ESA-25GeV (per 20K incident electrons on 10% X0 target)
Electron Spectra
NLC-500 (per colliding bunch)ESA-25GeV (per 20K incident electrons on 10% X0 target)
Positron Spectra
>5mrad production angle
>5mrad production angle
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Beam Tests for Synchrotron DetectorsBeam Tests for Synchrotron Detectors(for energy spectrometer, possibly for beamstrahlung detector)
Improve instrumentation for existing SLM in A-Line
Commission new synchrotron stripe detectors in ESA• Mirrors and ccds for visible SR• Quartz fibers w/ multi-anode PMT readout for ~MeV SR• test capability for resolving beam energy spread and hard edge at
NLC-500 (w/ energy spread) ESA-25GeV (w/o energy spread,
w/ 10% X0 target)
incomingbeamEE
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Implement both BPM and synchrotron stripe energy spectrometers. • Compare their performance directly, including capabilities for resolving energy
variations along 300-ns train• Compare energy jitter and energy temporal profile with existing instrumentation
using BPMs and the SLM at high dispersion points in the A-Line
24.5-degree A-line bend angle gives 180-degree spin precession every “3.237” GeV• Use energy scans across 2 or 3 zero-crossings of the polarization, where the beam
longitudinal polarization is measured with a Moller or Compton polarimeter. Compare new energy spectrometer results with polarization results. (Can also check comparison with A-line flip coil and power supply currents.) 10-3 accuracy from spin precession should be possible; whether 100-200 ppm is feasible needs study.
Energy Spectrometer Beam TestsEnergy Spectrometer Beam Tests
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Install a Compton polarimeter• Reuse hardware from SLD Compton polarimeter• Commission new detectors and make independent asymmetry measurements with
complementary detectors to evaluate systematics- compare electron and photon measurements- compare counting mode versus integrating mode
• Measure temporal dependence of polarization along the 300-ns train• With chicane for polarimeter downstream of target, can commission measurement
in presence of bremsstrahlung mimicking the beamstrahlung
Polarimetry Beam TestsPolarimetry Beam Tests
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Extraction Line Instrumentation (after IP)
• More flexibility to implement optimized beam optics for the instrumentation.No constraint to avoid emittance degradation. (Ex: can have x10 larger bendangles for the energy spectrometer)
• Can measure beam-beam effects (luminosity, disruption, beamstrahlung, depolarization)
• Can still measure undisrupted beam parameters, by requiring ~2% of pulses to besingle beam (no collisions)
• Energy spectrometer and polarimeter can be closer to the IP.
LC luminosity and LC physics capabilities
• Any beam or detector instrumentation that cannot be commissioned until the LC is built have very high risk factors. Do beam tests early!
General CommentsGeneral Comments
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Impact on LC Design
• There’s a close interplay between machine parameters and beam optics design with themeasurements discussed here. What we learn from these LC-LEP beam tests and simulation studies can impact the machine design.
Co-ordination with European and Asian Activities
• The UK Linear Collider group is focusing on the beam delivery system, includingsome of the beam instrumentation discussed in this LOI. They have recentlybeen awarded ~$8M Euros (over 3 years) from PPARC for their LC activities on theAccelerator. One of the UK groups (UC London; David Miller) has alreadyjoined this LOI.
• The LCRD proposal for a pair detector involves a collaboration with Tohoku U. inJapan and we would hope to test this detector in the ESA beam tests.
• The beam-beam simulation codes in use are GUINEA-PIG (European code) andCAIN (Japan and US code). Further checks of these codes with both simulationsand experiment are very desirable, in particular for understanding the tails of thedisrupted beam distributions and the PT spectrum of the pairs. Comparisons withbeam distributions from a thin fixed target, both with EGS simulation and experimentalmeasurements may be useful.
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Requests to EPACRequests to EPAC
1. Recognize importance of SLAC’s Polarized Electron Source, A-Line and End Station A facilities for LC-LEP beam tests. (Currently there are noapproved physics experiments at SLAC requiring a polarized beam or a high power long-pulse beam.)
2. Recommend that SLAC take into consideration LC-LEP beam tests, whenmodifying the A-Line and ESA beamlines, or the Polarized Source.(Also need compatibility with Linac modifications for LCLS.)
3. Encourage the development of (full technical) proposals for LC-LEPbeam tests.
4. Recommend that SLAC allow for a 1-week beam test in FY05 and 1-2 week beam tests in FY06 and FY07 in the long-range accelerator planning.
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ConclusionsConclusions
We have presented a description of LC-LEP measurements that are required by the LC physics program, as well as critical instrumentation that is needed forrealizing the LC luminosity goals.
The long pulse polarized beam to End Station A reflects many of the beam characteristics for the NLC beam at a 500-GeV collider. We have described howthe existing beam and beam diagnostics can be utilized for LC-LEP beam tests.
We have presented an overview of LC-LEP beam tests that can be carried out atSLAC’s ESA to demonstrate the stringent requirements for the detectors and techniques to be employed at the Linear Collider. There is much work to do to carefully design meaningful and cost-effective beam tests. We can be ready for first beam tests in FY05.