Upload
others
View
2
Download
0
Embed Size (px)
Citation preview
February 7, 2020
SiD and the International Linear Collider
Jim BrauUniversity of Oregon
The International Linear Collider❖ The International Linear Collider (ILC) is a proposed linear
particle accelerator. ❖ ILC will collide electrons with positrons at collision energies
of hundreds of GeV.❖ Proposed to be built in the USA, Europe and Japan, but now
the active site being considered is in northern Japan.❖ It would be about ten times as long as SLAC.
2J. Brau - 7 February 2020SiD and the International Linear Collider
Marty’s Impact on ILC❖ Broad and Deep!
❖ First Linear Collider & Detector - SLC and SLD
❖ SiD general concept❖ SiD subdetectors
- silicon tracking, silicon-tungsten ECal, HCal, silicon vertex detector, magnet, …
❖ SiD integration❖ SiD costs❖ ILC machine detector interface❖ …and more…
3J. Brau - 7 February 2020SiD and the International Linear Collider
Marty and Chris Damerell
credit: Cornell 2003
SLC and SLDThe First Linear Collider
❖ SLC built in 1980’s on existing SLAC linac.
❖ Marty led SLD as co-spokesman with Charlie Baltay.
❖ SLD operated 91-98.❖ Alr=0.15056 ± 0.00239✝.❖ Stringent Higgs mass bound:
mh < 147 GeV, 95% CL✝.✝..❖ Established many ILC concepts.❖ Marty contributed significantly
to development of SLC, itself.
4J. Brau - 7 February 2020SiD and the International Linear Collider
✝. PRL 84 5945✝.✝.http://www-sldnt.slac.stanford.edu/alr/
SLD
Early ILC Contribution During SLC
5J. Brau - 7 February 2020SiD and the International Linear Collider
Marty and John O’Fallon
credit: Fred Harris
Marty, Bill Ash & Bob Messner
credit: Fred Harris
Second International Workshop on Physics & Experiments @ Linear e+e- Colliders
University of Hawaii. April, 1993
2001 Motivation for Linear Collider❖ As the 20th century ended, after SLC/SLD’s successful physics
program, motivation for a “next” linear collider was clear.
❖ Paraphrasing “Linear Collider Physics Resource Book for Snowmass 2001,” SLAC-R-570:
❖ All evidence on EW interactions consistent with Standard Model (SM) with symmetry breaking due to Higgs field, ❖ generates masses of W & Z bosons and quarks & leptons.
❖ The Higgs field is an ad hoc addition to the SM, added "by hand".❖ Quark & lepton masses from arbitrary couplings to Higgs field. ❖ To explain these (and other) features, it’s necessary to extend SM. ❖ These extensions, in turn, predict new particles and phenomena.
❖ Higgs boson not yet discovered; SLD suggested low mass.
6J. Brau - 7 February 2020SiD and the International Linear Collider
Y2K - Linear Collider Concepts
NLC & JLC❖ SLAC and KEK❖ X-Band (11.4 GHz)-warm❖ 70 MeV/m
7J. Brau - 7 February 2020SiD and the International Linear Collider
TESLA❖ DESY❖ SuperC RF (1.3 GHz)❖ 35 MeV/m
As the 21st Century began, there were two competingconcepts on world stage for a “next” Linear Collider
NLC ZDRSLAC-R-571 August 2001
TESLA TDRDESY-2001-011 March 2001
Linear Collider Design Evolution❖ Marty’s early work focussed on NLC, the SLAC-led
proposal.
❖ NLC based on warm X-band technology competed with SCRF approach, favored at DESY for TESLA.
8J. Brau - 7 February 2020SiD and the International Linear Collider
2000 Ground Motion Workshop, SLAC
Marty and Andrei Seryi
Linear Collider Design Evolution❖ February 2003 - ICFA’s Technical Review Committee (ILC-TRC, chaired by
Greg Loew) reported on assessment of technical maturity of the technologies.
❖ Both X-Band (SLAC/KEK) and SCRF (DESY) are technically mature.
❖ In 2003 ICFA commissioned a panel (ITRP chaired by B. Barish) to recommend preferred technology, in order to consolidate global effort.
❖ 2004 - After thorough review by ITRP, with several meetings for presentations by advocates, SLAC-favored warm technology lost out to SCRF.
❖ After receiving news with great disappointment, Marty and SLAC colleagues began intense effort on this technology shift to SCRF.
9J. Brau - 7 February 2020SiD and the International Linear Collider
NLC/JLC
TESLA
International Linear Collider
The Silicon Detector (SiD)❖ Marty was leading conception of a new detector capitalizing on
the opportunities offered by the Linear Collider environment. ❖ SiD concept first presented at the ECFA/DESY Workshop on
Linear Colliders in Amsterdam, April, 2003.❖ SLAC-PUB-11413
• Conceived as high performance NLC detector.• Reasonably uncompromised performance.• But, Constrained & Rational cost.
– Marty’s parametric cost analysis.Assume excellent energy flow calorimetry required,
explore optimization of a W-Si ECal,and implications for the detector architecture…
10J. Brau - 7 February 2020SiD and the International Linear Collider
Quadrant View
0.000
1.000
2.000
3.000
4.000
5.000
6.000
7.000
8.000
0.000 2.000 4.000 6.000 8.000
m
m
Beam PipeEcalHcalCoilMTEndcapEndcap_HcalEndcap_EcalVXDTrack AngleEndcap_Trkr_1Endcap_Trkr_2Endcap_Trkr_3Endcap_Trkr_4Endcap_Trkr_5Trkr_2Trkr_3Trkr_4Trkr_5Trkr_1
Coil
2003 SiD Images
❖ After technology decision, GDE formed to develop ILC design under ICFA Mandate.
❖ GDE participants met in Snowmass, CO, in 2005
Barry BarishGDE Director
Global Design Effort (GDE)
11J. Brau - 7 February 2020SiD and the International Linear Collider
Snowmass 2005
❖ After technology decision, GDE formed to develop ILC design under ICFA Mandate.
❖ GDE participants met in Snowmass, CO, in 2005
Barry BarishGDE Director
Global Design Effort (GDE)
11J. Brau - 7 February 2020SiD and the International Linear Collider
Snowmass 2005
❖ After technology decision, GDE formed to develop ILC design under ICFA Mandate.
❖ GDE participants met in Snowmass, CO, in 2005
Barry BarishGDE Director
Global Design Effort (GDE)
11J. Brau - 7 February 2020SiD and the International Linear Collider
Snowmass 2005
ILC Experimental AdvantagesAs the ILC machine was being designed, Marty’s thinking about
experimenting at the ILC was evolving and maturing.❖ Radiation damage mostly not an issue (except very forward).
❖ collisions dominated by electroweak processes - very different from LHC.❖ Trigger-less operation - record every interaction (<6Gb/sec).❖ Bunch train structure allows pulse power w/ gas cooling.
❖ Relatively low event rates.❖ Elementary interactions at known Ecm.
❖ (e.g. e+e- → Z H)❖ Democratic Cross sections.
❖ (e.g. [e+e - → ZH] ~ 1/2 [e+e - → dd] ) ❖ Highly Polarized Electron Beam.
❖ (~ 80% - & positron pol. 30%)❖ Tunable center-of-mass energy.
❖ OPTIMIZE DETECTOR FOR ULTRA-PRECISE MEASUREMENTS12J. Brau - 7 February 2020SiD and the International Linear Collider
2000 Ground Motion Workshop, SLAC
1312 bunches (0.73 ms)
ILC250
J. Brau - 7 February 2020SiD and the International Linear Collider
16 August 2005 SiD Snowmass 05 M. Breidenbach1
SiDExpectations from the Design Study
– Motivation– What We Need!– Technical efforts– Status
Marty on SiD at Snowmass 2005
J. Brau - 7 February 2020SiD and the International Linear Collider
16 August 2005 SiD Snowmass 05 M. Breidenbach1
SiDExpectations from the Design Study
– Motivation– What We Need!– Technical efforts– Status
16 August 2005 SiD Snowmass 05 M. Breidenbach2
SiD Motivation
• SiD is an attempt to interest the international HEP community in the experimental challenges of a LC.
• SiD represents an attempt to design a comprehensive LC detector, aggressive in performance but constrained in cost.
• SiD attempts to optimize the integrated physics performance capabilities of its subsystems.
• The design study should evolve the present concept of SiDtowards a more complete and optimized design.
16 August 2005 SiD Snowmass 05 M. Breidenbach3
Nominal SiD Detector Requirements
– a) Two-jet mass resolution comparable to the natural widths of W and Z for an unambiguous identification of the final states.
– b) Excellent flavor-tagging efficiency and purity (for both b- and c-quarks, and hopefully also for s-quarks).
– c) Momentum resolution capable of reconstructing the recoil-mass to di-muons in Higgs-strahlungwith resolution better than beam-energy spread .
– d) Hermeticity (both crack-less and coverage to very forward angles) to precisely determine the missing momentum.
– e) Timing resolution capable of tagging bunch-crossings to suppress backgrounds in calorimeter and tracker.
– f) Very forward calorimetry that resolves each bunch in the train for veto capability.
– This is the standard doctrine – is it correct and complete?
16 August 2005 SiD Snowmass 05 M. Breidenbach4
SiD
• Conceived as a high performance detector for the LC• Reasonably uncompromised performance
But• Constrained & Rational cost
– Detectors will get about 10%– of the LC budget: 2 detectors, – so perhaps $600 M each
• Accept the notion that excellent energy flow calorimetry is required, and explore optimization of a Tungsten-Silicon EMCal and the implications for the detector architecture…
This is the monster assumption of SiD
16 August 2005 SiD Snowmass 05 M. Breidenbach5
SiD Costs - as of Aug 05
Summary
VXD 6.0
Tracker 19.9
EMCal 74.7
Hcal 74.2
Muon System 26.0
Electronics 37.5
Magnet 164.1
Installation 9.6
Management 9.4
Escalation 140.2
Indirects 38.5
Total 600.2
SiD Costs by category
VXD
Tracker
EMCal
Hcal
Muon System
Electronics
Magnet
Installation
Management
Escalation
Indirects
16 August 2005 SiD Snowmass 05 M. Breidenbach6
Crude Cost Trends
Fixed B, Vary R_Trkr
0
100
200
300
400
500
600
700
800
0 0.5 1 1.5 2
R_Trkr (m)
M$ cost
d$/dR
BR^2 Fixed, Vary R_Trkr
-600
-400
-200
0
200
400
600
800
1000
0.00 0.50 1.00 1.50 2.00 2.50
R_Trkr (m)
M$ R_Trkr
d$/dR
16 August 2005 SiD Snowmass 05 M. Breidenbach7
Architecture arguments
• Calorimeter (and tracker) Silicon is expensive, so limit area by limiting radius (and length)
• Maintain BR2 by pushing B (~5T)• Exquisite tracking resolution by using silicon strips• Buy safety margin for VXD with the 5T B-field.• Do track finding by using 5 VXD space points to determine track – tracker measures
sagitta. Exploit tracking capability of EMCal for Vees.
16 August 2005 SiD Snowmass 05 M. Breidenbach8
Knees
• During the SSC era, the SSC PAC asked the detector collaborations to justify their design choices – where possible by understanding the quality of detector performance as a function of a critical detector parameter. Ideally, quantities like overall errors on an important physics process would flatten out as a function of, say, calorimeter resolution, and there would be a rational argument for how good the resolution should be.
• We need similar analyses for the major parameters of SiD –EMCal radius and B are probably at the top of the list, along with justifying E-Flow calorimetry.
• We need to select physics processes for this study.• We are not constrained to design detector around these
knees, but we should know where they are!
16 August 2005 SiD Snowmass 05 M. Breidenbach9
SiD Configuration
Quadrant View
0.000
1.000
2.000
3.000
4.000
5.000
6.000
7.000
8.000
0.000 2.000 4.000 6.000 8.000
m
m
Beam PipeEcalHcalCoilMTEndcapEndcap_HcalEndcap_EcalVXDTrack AngleEndcap_Trkr_1Endcap_Trkr_2Endcap_Trkr_3Endcap_Trkr_4Endcap_Trkr_5Trkr_2Trkr_3Trkr_4Trkr_5Trkr_1
Scale of EMCal& Vertex Detector
16 August 2005 SiD Snowmass 05 M. Breidenbach10
full train (56 events)454 GeV detected energy100 detected charged tracks
1 bunch crossing
Yellow = muons Red = electrons Green = charged pionsDashed Blue = photons with E > 100 MeV
Illustration of bunch timing tag
T. Barklow16 August 2005 SiD Snowmass 05 M. Breidenbach
11
VXD Questions
• What is the VXD technology? • What is the optimal geometry, considering readout
electronics, cables, and cooling?
16 August 2005 SiD Snowmass 05 M. Breidenbach12
Momenter Questions
• Are there any serious problems with track finding (using VXD & EMCal)? (Barrel is 5 axial layers, segmented ~13 cm.)
• Is the 1.25 m radius optimal? What about the length?• Is 5 T B optimal?• Is there motivation to try to go thinner? Is there a knee in
the physics performance vs multiple scattering?
16 August 2005 SiD Snowmass 05 M. Breidenbach13
EMCal Questions
• Is an (expensive) Si-W tracking EMCal justified by the physics? Does E-Flow really work? It gives good but not great energy resolution – what about an EMCal with crystals with superb energy resolution? Crystals with somelongitudinal segmentation?
• Is there a useful Figure of Merit for E-Flow calorimetry? (My present favorite is BR2/{(σm
eff⊕σpixel)2x(σmeff ⊕δr
samp)}• Is radius of 1.25 m optimal? Is 5T B optimal? Same question as before!• Are there E-Flow performance issues in the forward direction? Are the end
EMCals far enough from the IP?
16 August 2005 SiD Snowmass 05 M. Breidenbach14
• Understanding of the HCal (in simulation and perhaps requiring beamtests) may well be necessary for serious development of the PFA.
• Gaseous detectors probably are less expensive and will have better segmentation than scintillator, but scintillator is a better detector for soft γ’s and neutrons. Is this important? Should an R&D attempt be made to make the gaseous detectors more sensitive – e.g. plastic walls?
• What should HCal radiator be – Tungsten? Stainless? Tungsten costs more but brings overall detector cost down (HCal ∆r is less, moving in coil). Is 4 Λenough?
• The HCal detector gap should be small – costs and shower spreading. Does this affect a detector choice?
• Note that HCal is inside coil. This seems to have gone away as a question.
HCal Assumptions and Questions
16 August 2005 SiD Snowmass 05 M. Breidenbach15
• Solenoid field is 5T – 3 times the field from detector coils that have been used in the detectors. - CMS will be 4T.
• Coil concept based on CMS 4T design. 5 layers of superconductor about 72 x 22 mm, with pure aluminum stabilizer and aluminum alloy structure. The aluminum alloy structural strips are beefed up relative to CMS.
• Coil Δr about 85 cm• Stored energy about 1.5 GJ (for Tracker Cone design, R_Trkr=1.25m, cosθbarrel=0.8).
(TESLA is about 2.4 GJ) [Aleph is largest existing coil at 130 MJ]• Is 5T right? And is it buildable? We need a “pre-conceptual” design!
Coil and Iron
Br Bz
16 August 2005 SiD Snowmass 05 M. Breidenbach16
Coil/Flux Return/Muon Tracker
• Previous questions as to the viability of a 5T coil seem to have gone away. Concept based on 6 layers of the CMS conductor is evolving.
• Iron “baseline” is 10 cm slabs with 1.5 cm gaps for detectors. Any muon identification concerns?
16 August 2005 SiD Snowmass 05 M. Breidenbach17
~ Not Worried about yet
• Small angle systems – forward tracking & calorimetry, Luminosity monitor
• Vibration Control & quad supports• Crossing angle correctors• And many others!
• All are important, and must be done “right” but unlikely to be design drivers in the class with E-Flow, B, Rcal.
16 August 2005 SiD Snowmass 05 M. Breidenbach18
Timing Analysis!
• We need answers to these questions to get to a credible conceptual design in 2006!
• We need answers to these questions to compare performance with the TPC based detectors!
SiD - Expectations from the Design StudyMarty at Snowmass 2005
J. Brau - 7 February 2020SiD and the International Linear Collider
16 August 2005 SiD Snowmass 05 M. Breidenbach1
SiDExpectations from the Design Study
– Motivation– What We Need!– Technical efforts– Status
16 August 2005 SiD Snowmass 05 M. Breidenbach2
SiD Motivation
• SiD is an attempt to interest the international HEP community in the experimental challenges of a LC.
• SiD represents an attempt to design a comprehensive LC detector, aggressive in performance but constrained in cost.
• SiD attempts to optimize the integrated physics performance capabilities of its subsystems.
• The design study should evolve the present concept of SiDtowards a more complete and optimized design.
16 August 2005 SiD Snowmass 05 M. Breidenbach3
Nominal SiD Detector Requirements
– a) Two-jet mass resolution comparable to the natural widths of W and Z for an unambiguous identification of the final states.
– b) Excellent flavor-tagging efficiency and purity (for both b- and c-quarks, and hopefully also for s-quarks).
– c) Momentum resolution capable of reconstructing the recoil-mass to di-muons in Higgs-strahlungwith resolution better than beam-energy spread .
– d) Hermeticity (both crack-less and coverage to very forward angles) to precisely determine the missing momentum.
– e) Timing resolution capable of tagging bunch-crossings to suppress backgrounds in calorimeter and tracker.
– f) Very forward calorimetry that resolves each bunch in the train for veto capability.
– This is the standard doctrine – is it correct and complete?
16 August 2005 SiD Snowmass 05 M. Breidenbach4
SiD
• Conceived as a high performance detector for the LC• Reasonably uncompromised performance
But• Constrained & Rational cost
– Detectors will get about 10%– of the LC budget: 2 detectors, – so perhaps $600 M each
• Accept the notion that excellent energy flow calorimetry is required, and explore optimization of a Tungsten-Silicon EMCal and the implications for the detector architecture…
This is the monster assumption of SiD
16 August 2005 SiD Snowmass 05 M. Breidenbach5
SiD Costs - as of Aug 05
Summary
VXD 6.0
Tracker 19.9
EMCal 74.7
Hcal 74.2
Muon System 26.0
Electronics 37.5
Magnet 164.1
Installation 9.6
Management 9.4
Escalation 140.2
Indirects 38.5
Total 600.2
SiD Costs by category
VXD
Tracker
EMCal
Hcal
Muon System
Electronics
Magnet
Installation
Management
Escalation
Indirects
16 August 2005 SiD Snowmass 05 M. Breidenbach6
Crude Cost Trends
Fixed B, Vary R_Trkr
0
100
200
300
400
500
600
700
800
0 0.5 1 1.5 2
R_Trkr (m)
M$ cost
d$/dR
BR^2 Fixed, Vary R_Trkr
-600
-400
-200
0
200
400
600
800
1000
0.00 0.50 1.00 1.50 2.00 2.50
R_Trkr (m)
M$ R_Trkr
d$/dR
16 August 2005 SiD Snowmass 05 M. Breidenbach7
Architecture arguments
• Calorimeter (and tracker) Silicon is expensive, so limit area by limiting radius (and length)
• Maintain BR2 by pushing B (~5T)• Exquisite tracking resolution by using silicon strips• Buy safety margin for VXD with the 5T B-field.• Do track finding by using 5 VXD space points to determine track – tracker measures
sagitta. Exploit tracking capability of EMCal for Vees.
16 August 2005 SiD Snowmass 05 M. Breidenbach8
Knees
• During the SSC era, the SSC PAC asked the detector collaborations to justify their design choices – where possible by understanding the quality of detector performance as a function of a critical detector parameter. Ideally, quantities like overall errors on an important physics process would flatten out as a function of, say, calorimeter resolution, and there would be a rational argument for how good the resolution should be.
• We need similar analyses for the major parameters of SiD –EMCal radius and B are probably at the top of the list, along with justifying E-Flow calorimetry.
• We need to select physics processes for this study.• We are not constrained to design detector around these
knees, but we should know where they are!
16 August 2005 SiD Snowmass 05 M. Breidenbach9
SiD Configuration
Quadrant View
0.000
1.000
2.000
3.000
4.000
5.000
6.000
7.000
8.000
0.000 2.000 4.000 6.000 8.000
m
m
Beam PipeEcalHcalCoilMTEndcapEndcap_HcalEndcap_EcalVXDTrack AngleEndcap_Trkr_1Endcap_Trkr_2Endcap_Trkr_3Endcap_Trkr_4Endcap_Trkr_5Trkr_2Trkr_3Trkr_4Trkr_5Trkr_1
Scale of EMCal& Vertex Detector
16 August 2005 SiD Snowmass 05 M. Breidenbach10
full train (56 events)454 GeV detected energy100 detected charged tracks
1 bunch crossing
Yellow = muons Red = electrons Green = charged pionsDashed Blue = photons with E > 100 MeV
Illustration of bunch timing tag
T. Barklow
16 August 2005 SiD Snowmass 05 M. Breidenbach11
VXD Questions
• What is the VXD technology? • What is the optimal geometry, considering readout
electronics, cables, and cooling?
16 August 2005 SiD Snowmass 05 M. Breidenbach12
Momenter Questions
• Are there any serious problems with track finding (using VXD & EMCal)? (Barrel is 5 axial layers, segmented ~13 cm.)
• Is the 1.25 m radius optimal? What about the length?• Is 5 T B optimal?• Is there motivation to try to go thinner? Is there a knee in
the physics performance vs multiple scattering?
16 August 2005 SiD Snowmass 05 M. Breidenbach13
EMCal Questions
• Is an (expensive) Si-W tracking EMCal justified by the physics? Does E-Flow really work? It gives good but not great energy resolution – what about an EMCal with crystals with superb energy resolution? Crystals with somelongitudinal segmentation?
• Is there a useful Figure of Merit for E-Flow calorimetry? (My present favorite is BR2/{(σm
eff⊕σpixel)2x(σmeff ⊕δr
samp)}• Is radius of 1.25 m optimal? Is 5T B optimal? Same question as before!• Are there E-Flow performance issues in the forward direction? Are the end
EMCals far enough from the IP?
16 August 2005 SiD Snowmass 05 M. Breidenbach14
• Understanding of the HCal (in simulation and perhaps requiring beamtests) may well be necessary for serious development of the PFA.
• Gaseous detectors probably are less expensive and will have better segmentation than scintillator, but scintillator is a better detector for soft γ’s and neutrons. Is this important? Should an R&D attempt be made to make the gaseous detectors more sensitive – e.g. plastic walls?
• What should HCal radiator be – Tungsten? Stainless? Tungsten costs more but brings overall detector cost down (HCal ∆r is less, moving in coil). Is 4 Λenough?
• The HCal detector gap should be small – costs and shower spreading. Does this affect a detector choice?
• Note that HCal is inside coil. This seems to have gone away as a question.
HCal Assumptions and Questions
16 August 2005 SiD Snowmass 05 M. Breidenbach15
• Solenoid field is 5T – 3 times the field from detector coils that have been used in the detectors. - CMS will be 4T.
• Coil concept based on CMS 4T design. 5 layers of superconductor about 72 x 22 mm, with pure aluminum stabilizer and aluminum alloy structure. The aluminum alloy structural strips are beefed up relative to CMS.
• Coil Δr about 85 cm• Stored energy about 1.5 GJ (for Tracker Cone design, R_Trkr=1.25m, cosθbarrel=0.8).
(TESLA is about 2.4 GJ) [Aleph is largest existing coil at 130 MJ]• Is 5T right? And is it buildable? We need a “pre-conceptual” design!
Coil and Iron
Br Bz
16 August 2005 SiD Snowmass 05 M. Breidenbach16
Coil/Flux Return/Muon Tracker
• Previous questions as to the viability of a 5T coil seem to have gone away. Concept based on 6 layers of the CMS conductor is evolving.
• Iron “baseline” is 10 cm slabs with 1.5 cm gaps for detectors. Any muon identification concerns?
16 August 2005 SiD Snowmass 05 M. Breidenbach17
~ Not Worried about yet
• Small angle systems – forward tracking & calorimetry, Luminosity monitor
• Vibration Control & quad supports• Crossing angle correctors• And many others!
• All are important, and must be done “right” but unlikely to be design drivers in the class with E-Flow, B, Rcal.
16 August 2005 SiD Snowmass 05 M. Breidenbach18
Timing Analysis!
• We need answers to these questions to get to a credible conceptual design in 2006!
• We need answers to these questions to compare performance with the TPC based detectors!
Marty on SiD at Snowmass 2005
SiDExpectations from the Design StudySiD MotivationNominal SiD Detector Requirements SiDSiD Costs - as of Aug 05Crude Cost TrendsArchitectural argumentsKneesSiD ConfigurationIllustration of bunch timing tagVXD QuestionsMomenter QuestionsEMCal QuestionsHCal Assumptions and QuestionsCoil and IronCoil/Flux Return/Muon Tracker~Not Worried about yetTiming Analysis!
SiD Exec Board - December 2005Near Fermilab
Marty was focussed on the key issues to advance the SiD design,
and led the intellectual effort.
ILC Parameters• 2006 - Parameters Subcommittee of the International Linear
Collider Steering Committee (chair, Rolf Heuer)• “The machine should allow for an energy range for physics
between 200 GeV and 500 GeV, with operation at any energy value as dictated by the physics (e.g. at the maximum of the Higgs production cross section).”
• Question in 2006 - what is the value of the Higgs mass?
14J. Brau - 7 February 2020SiD and the International Linear Collider
2009 - Letter of IntentarXiv:0911.0006
SiD Path to Validation2004 - led by Spokespersons J.Jaros & H.Weerts
2006 - Detector Outline Documenthttps://web.archive.org/web/20101117023030/http://hep.uchicago.edu/~oreglia/siddod.pdf
2007 - Reference Design ReportarXiv:0712.2356
15J. Brau - 7 February 2020SiD and the International Linear Collider
August, 2009, the IDAG (M.Davier, chair) validated two concepts.One was SiD. Next challenge: the TDR!
After Validation, the TDR
ILC Technical Design Report complete in 2012,and delivered to ICFA in three continent event in 2013.
16J. Brau - 7 February 2020SiD and the International Linear Collider
Five volumesVol 4 - Detectors
FermilabCERNTokyo
Parameter TDR
C.M.Energy(GeV) 500Upgradeableto1TeV
Length(km) 31
Luminosity(x1034) 1.8
Repetition(Hz) 5
BeamPulsePeriod(ms) 0.73
BeamCurrent(mAinpulse)
5.8
Beamsize(y)atFF(nm) 5.9
SRFCavityGr(MV/m),Q0
31.5,1x1010
SitePower(MW) 163main linacbunch
compressor
dampingring
source
pre-accelerator
collimation
final focus
IP
extraction& dump
KeV
few GeV
few GeVfew GeV
250-500 GeV
Nano-beamTechnology
SRFAcceleratingTechnology
KeyTechnologies
PhysicsDetectors
based on S. Michizono, 8 Nov 2017
ILC TDR is 5-volumes, published 12 June 2013
Polarized electrons (± 80%) and positrons (± 30%)
Design resulting from two decades of dedicated R&D
ILCTDR
17
31 km
Parameter TDR
C.M.Energy(GeV) 500Upgradeableto1TeV
Length(km) 31
Luminosity(x1034) 1.8
Repetition(Hz) 5
BeamPulsePeriod(ms) 0.73
BeamCurrent(mAinpulse)
5.8
Beamsize(y)atFF(nm) 5.9
SRFCavityGr(MV/m),Q0
31.5,1x1010
SitePower(MW) 163main linacbunch
compressor
dampingring
source
pre-accelerator
collimation
final focus
IP
extraction& dump
KeV
few GeV
few GeVfew GeV
250-500 GeV
Nano-beamTechnology
SRFAcceleratingTechnology
KeyTechnologies
PhysicsDetectors
based on S. Michizono, 8 Nov 2017
ILC TDR is 5-volumes, published 12 June 2013
Polarized electrons (± 80%) and positrons (± 30%)
Design resulting from two decades of dedicated R&D
ILCTDR
17
31 km
Higgs Boson Discovery❖ As ILC TDR was being completed.❖ Announced July 4, 2012. Mass = 125 GeV (light)
18J. Brau - 7 February 2020SiD and the International Linear Collider
Higgs Boson Cross Section
19J. Brau - 7 February 2020SiD and the International Linear Collider
(GeV)s200 250 300 350 400 450 500
Cro
ss s
ectio
n (fb
)
0
100
200
300
400=125 GeV
h)=(-0.8, 0.3), M+, e-P(e
hfSM all fZhWW fusionZZ fusion
=125 GeVh
)=(-0.8, 0.3), M+, e-P(e
WW fusionrising with
center-of-massenergy
Higgs-strahlungpeaks and falls with
center-of-massenergy
Higgs Boson Cross Section
19J. Brau - 7 February 2020SiD and the International Linear Collider
(GeV)s200 250 300 350 400 450 500
Cro
ss s
ectio
n (fb
)
0
100
200
300
400=125 GeV
h)=(-0.8, 0.3), M+, e-P(e
hfSM all fZhWW fusionZZ fusion
=125 GeVh
)=(-0.8, 0.3), M+, e-P(e
WW fusionrising with
center-of-massenergy
Higgs-strahlungpeaks and falls with
center-of-massenergy
Parameters Committee Report:
• “…operation at any energy value as dictated by the physics (e.g. at the maximum of the Higgs production cross section).”
250 GeV
Higgs Factory observes Higgs recoiling from a Z, with known CM energy⇓
• powerful channel for unbiassed tagging of Higgs events• measurement of even invisible decays
(⇓ - some beamstrahlung)
Higgstrahlung at 250 GeV
20J. Brau - 7 February 2020SiD and the International Linear Collider
Invisible decays are included
4. MEASURE RECOILAND OBSERVE DECAY
1. KNOWN INTIAL STATE2. MEASURE Z→ l+l−
3. SELECT E(Z boson) = 110 GeV M(recoil) = 125 GeV
l+
l−
)2Recoil Mass (GeV/c110 120 130 140 150
Eve
nts
0
100
200
300
400
+ X @ 250 GeV-µ+µ →
-+e+e
Toy MC Data
Signal+Background
Signal
Background
arXiv:1604.07524, PRD94 (2016) 113002
ILC/HL-LHC Comparison (model-dependent)
Model dependence: 1.) Assume Higgs boson has no decay modes beyond those predicted by SM,
2.) Higgs boson WW & ZZ couplings modified only by rescaling.21J. Brau - 7 February 2020SiD and the International Linear Collider
0
1
2
3
4
5
6
7
Prec
isio
n of
Hig
gs b
oson
cou
plin
gs [%
]
Z W b τ g c γ µ
1/2×
t
1/2×
λ
1/20×
HL-LHC arXiv:1902.00134S1: CMS, S2: ATLAS&CMS
ILC250⊕HL-LHC ILC500⊕ ILC250 ⊕HL-LHC
dark/light: S1/S2
=0 & no anom. hZZ/hWW coupl.)BSM
Γ Fit (κModel Dependent EFT / LCC Physics WG
1 %
arXiv:1903.01629
• S1, current projection• /model-dependent• S2, improved• /model-dependent
(HL-LHC adopted)
ILC Model Independent Higgs precision at 250 GeV
❖ Highly model-independent analysis of EFT: Phys Rev D97, 053003 (2018)
22J. Brau - 7 February 2020SiD and the International Linear Collider
0
0.5
1
1.5
2
2.5
3
3.5
Prec
isio
n of
Hig
gs b
oson
cou
plin
gs [%
]
Z W b τ g c invΓ hΓ γ γZ
1/3×
µ
1/2×
t
1/2×
λ
1/10×
ILC250⊕HL-LHC
ILC500⊕ ILC250 ⊕HL-LHC
dark/light: S1*/S2*
Model Independent EFT Fit LCC Physics WG
“Model-independent”EFT fit
~1 % goal to access
New Physics beyond HL-LHC
direct search
arXiv:1903.01629
Model Discrimination - 250 GeV
23J. Brau - 7 February 2020SiD and the International Linear Collider
arXiv:1710.07621
02468101214161820 σ
mod
el d
iscr
imin
atio
n in
SM pMSSM
2HDM-II2HDM-X
2HDM-YComposite
LHT-6LHT-7
RadionSinglet
Singlet
Radion
LHT-7
LHT-6
Composite
2HDM-Y
2HDM-X
2HDM-II
pMSSM
SM
3.6 6.8 10.5 7.2 12.0 3.5 3.6 5.6 6.2
6.1 9.8 13.7 9.1 14.6 7.0 9.1 6.4
5.4 10.4 15.1 9.0 15.6 2.7 8.3
4.3 5.2 7.7 7.2 10.1 5.9
3.9 8.3 12.6 7.8 13.6
11.3 6.2 7.8 15.7
6.2 10.3 10.7
9.7 6.5
5.8ILC250, S2*
EFT interpretation• S1*, current projection
/model-independent• S2*, improved
/model-independent
Nine(9) models unlikely to be discovered by HL-LHC.
Masses beyond reach.
Model Discriminationimproves @ higher energy,
eg. 500 GeV
e- Source
e+ Main Linac
e+ Source
e- Main Linac
Parameter Initialstage
TDR
C.M.Energy(GeV) 250 500
Length(km) 20 31
Luminosity(x1034) 1.35(2.7,5.4)
1.8
Repetition(Hz) 5(10) 5
BeamPulsePeriod(ms) 0.73 0.73
BeamCurrent(mAinpulse)
5.8 5.8
Beamsize(y)atFF(nm) 7.7 5.9
SRFCavityGr(MV/m),Q0
31.5,1x1010
31.5,1x1010
SitePower(MW) 129 163main linacbunch
compressor
dampingring
source
pre-accelerator
collimation
final focus
IP
extraction& dump
KeV
few GeV
few GeVfew GeV
250-500 GeV
Nano-beamTechnology
SRFAcceleratingTechnology
KeyTechnologies
PhysicsDetectors
Damping Ring
based on S. Michizono, 8 Nov 2017
ILC TDR is 5-volumes, published 12 June 2013
Polarized electrons (± 80%) and positrons (± 30%)
~20km
arXiv:1903.01629arXiv:1711.00568
Design resulting from two decades of dedicated R&D
InitialStage-ILC250
24
e- Source
e+ Main Linac
e+ Source
e- Main Linac
Parameter Initialstage
TDR
C.M.Energy(GeV) 250 500
Length(km) 20 31
Luminosity(x1034) 1.35(2.7,5.4)
1.8
Repetition(Hz) 5(10) 5
BeamPulsePeriod(ms) 0.73 0.73
BeamCurrent(mAinpulse)
5.8 5.8
Beamsize(y)atFF(nm) 7.7 5.9
SRFCavityGr(MV/m),Q0
31.5,1x1010
31.5,1x1010
SitePower(MW) 129 163main linacbunch
compressor
dampingring
source
pre-accelerator
collimation
final focus
IP
extraction& dump
KeV
few GeV
few GeVfew GeV
250-500 GeV
Nano-beamTechnology
SRFAcceleratingTechnology
KeyTechnologies
PhysicsDetectors
Damping Ring
based on S. Michizono, 8 Nov 2017
ILC TDR is 5-volumes, published 12 June 2013
Polarized electrons (± 80%) and positrons (± 30%)
~20km
arXiv:1903.01629arXiv:1711.00568
Design resulting from two decades of dedicated R&D
InitialStage-ILC250
24
Cost (ILC250) ~ 60% Cost (TDR ILC - 500 GeV)
Japan Preparing to Host ILC
Vigorous recent activities in Japanese government to launch
international project.25J. Brau - 7 February 2020SiD and the International Linear Collider
Hitoshi Murayama, 2002 Nobel laureate Masatoshi Koshiba, LCC Director Lyn Evans, PM Shinzo Abe,
and Diet member Takeo Kawamura,
The Silicon Detector (SiD)• High performance ILC detector,
• Reasonably uncompromised performance,
• BUT constrained & Rational cost
• Compact design (R 6m) in a 5 T field.• Robust all-silicon tracking with
excellent momentum resolution.• Time-stamping for single bunch crossings.• Highly granular optimized for Particle Flow.• Integrated design: All parts work in tandem.• Iron flux return/muon identifier self-shields SiD.
• Thanks to Marty and colleagues, SiD well thought out, with initial R&D demonstrating concept, ready for intense engineering phase leading to construction.
≲
26J. Brau - 7 February 2020SiD and the International Linear Collider
SiD Workshop, 2007 Fermilab
SiD
SiD Key Subsystems
27J. Brau - 7 February 2020SiD and the International Linear Collider
OUTER TRACKING
❖ Silicon Tracking (SiD) - strips❖ 5 barrel layers, 4 forward disks❖ 1.2 m outer radius❖ Pixels being considered❖ B = 5T
CALORIMETRY❖ Separate W&Z di-jet events.❖ Resolution 3% for 100 GeV jet.❖ Use particle flow analysis.
≳
σ1pT
!
"#
$
%& ≤ 5×10−5 (GeV −1)
VERTEX DETECTOR
❖ CMOS pixels
σ rϕ ≈σ rz ≈ 5⊕10 / (p sin3/2ϑ ) µm
Chronopixel for Vertex DetectionOregon/YaleCollaboraDon• MonolithicCMOSdesign.
90nmfeaturesize,7µmepitaxiallayer280µmthickchip10ohm⋅cmmanufacturedbyTSMC
• Storeupto2hitsperpixel.
• 6sensordiodeopaonsevaluated.
28J. Brau - 7 February 2020SiD and the International Linear Collider
Chronopixel
Chronopixel prototype 3 development board
N. Sinev et al., PoS VERTEX 2005, 038 (2015)
diodeoption
Capacitance(fF)
μV/e
1 9.0 18
2 6.2 6.3
3 2.7 59
4 4.9 33
5 4.9 33
6 8.9 18
Silicon Tracking w/ Gas Cooling → Low Material
❖ Linkage between readout/mechanics/powering/cooling studies.❖ Maintain low mass construction.❖ Tracking material from SiD design:
29J. Brau - 7 February 2020SiD and the International Linear Collider
SiDvxd+trk SiCfoam,
J.Goldstein
10% X0
Silicon-tungsten ECal - Very High Granularity
SiD ECal Design
• 6 inch silicon wafers• 1024 13 mm2 pixels• KPiX readout and cable are bump-bonded directly to sensor • 1 mm readout gaps -> 13 mm effective Moliere radius•. Tungsten plates thermal bridge to edge cooling •. Feeds Particle Flow (~3% jet resolution at 100 GeV) •. EM resolution: 17%/sqrt(E)❖
30J. Brau - 7 February 2020SiD and the International Linear Collider
KPiX ASIC &sample trace
KPiX
SLD Luminosity Monitor
First Si-W Calorimeter used in a running experiment
Dieter Freytag
KPiX - Key Element
Applications: Si strip tracking, Si-W ECal (possibly RPCs, GEMs, SiPMs)
31J. Brau - 7 February 2020SiD and the International Linear Collider
Dual-KPiX Tracking Sensor
Design Achieves Physics Requirements❖ SiD employs
❖ High granularity❖ Dense integration❖ Super light materials❖ Low power/pulse power❖ Air cooling
❖ Unprecedented performance with clean events and small backgrounds.
❖ Ready for final phase of engineering, (Led now by Spokespersons M. Stanitzki and A. White)followed by ILC launch and SiD construction!
32J. Brau - 7 February 2020SiD and the International Linear Collider
SiD
Built on Excellence - People and Collaboration
33J. Brau - 7 February 2020SiD and the International Linear Collider
Built Friendships
34J. Brau - 7 February 2020SiD and the International Linear Collider
Built Friendships
34J. Brau - 7 February 2020SiD and the International Linear Collider
Thank you, Marty, for your Vision,for your Leadership, and for your Friendship.
Thank you, Marty, for your Vision,for your Leadership, and for your Friendship.
Thank you, Marty, for your Vision,for your Leadership, and for your Friendship.