The I nternational L inear C ollider program.
description
Transcript of The I nternational L inear C ollider program.
The International Linear Collider program.
Marcello PiccoloLNF-INFNFrontierScience, Milano Sept. 2005
M.Piccolo, Frontierscience, Milano
Sept. 2005
Agenda
• Brief historical excursus
• The Physics case
• The experimental challenges
• Detector design (s)
• Time scale
• Conclusions
M.Piccolo, Frontierscience, Milano
Sept. 2005
The start of the O(1TeV) L.C.
• It is difficult to set a start date for a program that was in the back of at least 50% of particle physicists mind since at least 25 years.
• I will arbitrarily set the start date at the Saariselka ( Finland ) meeting in September 1991.
• It might be interesting to remember which kind of environment we were living in.
M.Piccolo, Frontierscience, Milano
Sept. 2005
The lepton collider Physics at the end of 1991
• Going back to the summer of 1991 − 106 Z collected at LEP− The Standard Model was capable of
describing everything LEP would turn out.
− E.W. fits were almost perfect− The four LEP detectors were just
turning toward heavy quark Physics.− For the record E.W. fits were giving :
Mtop=120 ± 40 GeV/c2
− CDF had an upper limit on top mass at 91 GeV/c2
M.Piccolo, Frontierscience, Milano
Sept. 2005
The men with vision• Maury Tigner
− The first one to think of it.• Nuovo Cimento 37 (1965) 1228
• Burt Richter− The first one to do it
• SPC SLC
• (Late) Bijorn Wiik− The superconducting RF advocate
• TESLA ILC• His legacy is embedded the actual
program
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Sept. 2005
The study groups• Originally Europe, Japan and USA organized
their own study groups.
• After a while it was realized that a common framework was needed, and the LCWS was organized, with the aim of bringing together the regional groups to share experiences, results and …frustrations
• This in my opinion was the starting of the global character of the effort.
• Now here we are with a programs that carries the word International as a first name.
M.Piccolo, Frontierscience, Milano
Sept. 2005
The Physics program : seeking answers the TeV
Scale
The TeV energy region hold the promise of giving back answers to our quests.
Origin of mass and electro-weak symmetry breaking
Why such a disparity between mweak and mPlanck
What is most of the matter in the Universe made of
and more…
The Tevatron is already at work to open a window into this regime.
LHC will allow a (quasi) complete view on phenomena at the TeV scale!
M.Piccolo, Frontierscience, Milano
Sept. 2005
Will the LHC be enough ?• Although the LHC is the most powerful
research instrument ever built in our field, it does have limitations:
• LHC detectors record about 10-5 of the total cross section
• Analysis will be carried out on 10-10 of the total cross section.
• No events balance visible longitudinal momentum.
• Events with missing neutrals have unknown pt
• High-purity b tagging, any charm tagging and tagging is difficult
• Most LHC analyses rely on a model.
• They are powerful if the underlying assumptions are correct, not so powerful if wrong.
M.Piccolo, Frontierscience, Milano
Sept. 2005
ILC Physics Case
Whatever LHC will find, one CANNOT give up the ILC, that warrants a Physics program which stands on his own feet.
1. If there is a ‘light’ Higgs (consistent with precision EW) proof that it is a particle responsible for giving masses (a)
2. If there is a ‘heavy’ Higgs (inconsistent with precision EW) verify the Higgs mechanism is at work as in (a) understand (in)consistencies with S.M.
3. 1./2. & new states (SUSY, XD, little H, Z’, …) A completely spectroscopy is available to be discovered and measured
4. No Higgs, no new states (inconsistent with precision EW) find out what is wrong with the S.M. look for threshold effects of strong EWSB
(TESLA TDR, Snowmass01, ACFA report, …)
M.Piccolo, Frontierscience, Milano
Sept. 2005
ILC physics case
)( tan dardModelSnewPhysics XXXee
Produce new particles look at deviations
Find new type of states and measure it(cross sections, masses,
BR’s, Quantum numbers)
Look at known processes and find deviations from the expected, through virtual effects.
Needs good experimental work AND good knowledge of what to expect.
Peek deep intomulti-TeV region
ModeldardSee tan
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Sept. 2005
Hadrons cry to loud (B. Toushek ca. 1960)
Electron positron collisions at high energy allow an almost complete
exploration of the phenomena deemed relevant to EWSB.
The initial state is made of individual constituents, and this provide some advantages with respect to protons.
• very well defined (and tunable) centre-of-mass energy
•….and all of it usable.
• clean, fully reconstructable events (no unknown pl )
• polarized beams.
• moderate backgrounds
• Unfortunately chronical lack of counting rate.
p pe+ e-
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Sept. 2005
The ILC
• Center-of-Mass Energy ~ 90 – 1000 GeV
Time Structure : 5 (10?) Bunch-trains/s Time between collisions: ~ 300 (150) ns
950 µs 199 ms 950 µs
2820 bunches
• Baseline Luminosity :2x1034 cm-2s-1
(>1000xLEP
e+e-qq ~100/hr e+e-W+W- ~1000/hr e+e-tt ~50/hr e+e-HX ~10/hr
e+e-qq ~0.1 /Bunch Train e+e-X ~200 /Bunch Train ~500 hits/BX in Vertex det. ~5 tracks/BX in TPC
• `Backgrounds‘ (depends on ILC parameters)
ILC baseline parameters currently being discussed
e.g. TESLA TDR
Event rates modest – small compared to LHC
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Sept. 2005
Configuration Parameter Space
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Sept. 2005
Impact on Detector Design
Radiation hardness not a big concern. Time structure of the machine not demanding. Worst type of Physics background Angle crossing to be studied in detail.
Final focus lenses (L* ) have big effect on backgrounds
The detector design dictated by Physics
MDI + crossing-angle important : might place constraint on design
M.Piccolo, Frontierscience, Milano
Sept. 2005
Physics processes
• To asses the capabilities of the ILC, I will go over few individual reactions:− Higgs Physics− Super symmetry studies− Gauge bosons− Top
M.Piccolo, Frontierscience, Milano
Sept. 2005
Higgs Physics
• If can use Higgstrahlung, model
independent observation.
• mass measurements
• absolute branching ratios
• total width
• spin, CP
• top Yukawa coupling
• self coupling
Garcia-Abia et al
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Sept. 2005
Higgs at LHC
• LHC will discover some Higgs, if it is there within three years (2011?)
• Will a discovery be enough ? I doubt it.
• Let us suppose to discover H , and to see, as a cross check a final state ttH.
• Technipion? Scalar or pseudo-scalar? Does it couple with W/Z?
M.Piccolo, Frontierscience, Milano
Sept. 2005
Legitimate questions • Was the Higgs boson discovered ?
− Is it the particle responsible for mass ?− Does it have the correct spin parity
assignment 0+?− Is it really the condensate that fills the
Universe ?
• To prove that it is indeed what gives mass to particles− Spin/Parity− Couplings− Vacuum expectation value− Branching Ratios− Self coupling
M.Piccolo, Frontierscience, Milano
Sept. 2005
Higgs Boson at LC• Angular distributions
in e+e–ZX depend on X=h, A, V
is it a 0+?
M.Piccolo, Frontierscience, Milano
Sept. 2005
Higgs Boson at LC
• Branching Fractions prove couplings mass.
The Higgs is responsible for masses. (Battaglia)
M.Piccolo, Frontierscience, Milano
Sept. 2005
Higgs Boson at LC
• Final state ZH
• ALR is proof that is produced by s-channel Z-exchange
• If Z gauge boson, H scalar boson only two vertices possible
• A VEV is needed to have a ZZH vertex.
• Measurement of gZ will prove that Z mass is (partly) due to the scalar.
H. Murayama LBL-38891
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Sept. 2005
Precision Higgs physics
SM
2HDM/MSSM
Yamashita et alZivkovic et al
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Sept. 2005
Now, we have the Higgs and we know is the one that generates masses……
• The S.M. assumes a negative Why ?
• Yes, there is a condensate that shields the weak force.
• Why do we have something that condenses ?
Why the condensation scale ~TeV<<MPl
M.Piccolo, Frontierscience, Milano
Sept. 2005
Possible (model) solutions• Super symmetry
− Crisis with the electron self energy: ….introduction of antimatter
− Double # particles + boson to fermion and viceversa
• Cooper pair mechanism − Cooper pairs: two electrons bond together− Higgs as a fermion antifermion pair
Technicolor
• Physics ends @ TeV scale− Ultimate scale: quantum gravity− Gravitational effects @ ~TeV
hidden dimensions
M.Piccolo, Frontierscience, Milano
Sept. 2005
If it is there LHC will discover super symmetry; however many hard questions will be still unanswered or partially answered:
• is it really SUSY? (measurement of quantum numbers)
• how is it realized? (MSSM, NMSSM, …)
• how is it broken?
ILC will be able to provide answers to these questions!
Make full use of the flexibilityof the machine:
- tunable energy
- polarized beams
- possibly e-e- and collisions
Supersymmetry
500200 1000 3000
Sobloher
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Sept. 2005
Super symmetry at LC
• To prove : effective super-partners− Spins differ by 1/2− Same quantum
numbers SU(3)SU(2)U(1)
− Super symmetric couplings
Spin 0?
M.Piccolo, Frontierscience, Milano
Sept. 2005
Supersymmetry at LC (cont.)
Two methods to obtain absolute sparticle masses:
in the continuum: at the kinematic threshold:
many more observables than just masses:
- angular distributions, FB-asymmetries- cross sections- LR-asymmetries- ratios of branching ratios
possibility to determine SUSY parameters without many model assumptions
FreitasMartyn
M.Piccolo, Frontierscience, Milano
Sept. 2005
Supersymmetry LC + LHC
A LHC/LC joint effort:
errors of a 19-parameter fit using ILC+LHC:
allows for model-independent investigation of GUT/Planck scale features of the theory:
Bechtle et al
Porod et al
The overall results on SS data fitting:
It is clear that neither of the two
programs would have such an analyzing
Power.
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Sept. 2005
DM/DM main sensitivity
bulk 3.5%
focus 1.9%
co-ann. 6.5%
funnel 3.1%
01 R R 1,e , ,
0 0 0 0 0 01 2 1 3 1 1 1 1 1, , , , ( )
0 01 1 1,
0 01 1A , ,
The Cosmic ConnectionSUSY provides excellent candidate for dark matter (LSP)
(Other models provide TeV-scale WIMPs too)
Sensitivity for DM search at accelerators of the same order
as astrophysics searches…. ALCPG study/prel.
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Sept. 2005
And if no Higgs comes around ?
Cross section for weak vector boson scattering violates unitarity at ~1.2 TeV, and no new resonances appear
Birkedal et al.Krstonosic et al.
ILC sensitivity deep into multi-TeV region from VB final stateseff. Lagrangian parametersof strong EWSB:
Higgsless model: new resonancein WZWZ
Coupling structure from ILC if resonance seen by LHC
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Sept. 2005
Top
Hoang et al
We know that is there.Threshold scan provides remarkable improvement on mass measurementTheory (NNLL) controls mt(MS) to 100 MeV
Heinemeyer et al
very precise mtop vital
- improved SM fits- MSSM (mh prediction)- DM-density in mSugra- …
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Sept. 2005
Detector Design for the ILC
Optimize the detector so thatevery bit of luminosity counts
In e+e- colliders we always fight with
small cross sections.
Limit systematic errors
Requirements differentfrom LHC detectors
Overall detector concept
R&D on key components
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Sept. 2005
A detector with Particle flow
To exploit to the fullest the ILC environment one seeks complete
reconstruction of complex final states (multi-jets, tau’s)
often accompanied by missing-E
How can we achieve the very best
energy resolution for jets ?
Generally accepted paradigm:
Particle flow
Particle flow is:
- a detector concept
- and an algorithm
M.Piccolo, Frontierscience, Milano
Sept. 2005
The Particle Flow AlgorithmBasic idea: reconstruct every single particle in the event
for each particle type exploit the detector subsystem which cando that best!
~60% charged tracker
~30% photons (from 0) ECAL
~10% neut. hadrons HCAL
sounds reasonablechallenge: cluster mixing/double counting
Separate
charged from neutral: B field, R, trans. granularity, material
EM from HAD: trans. + long. granularity (“shower tracking”)
Goal : E/E = 30%/E0.5
M.Piccolo, Frontierscience, Milano
Sept. 2005
The Particle Flow Algorithm (cont.)
HadHadmemepE EKEKpKjet
2...
2..
42
Resolution terms relevant: hadronicenergy and wrong clustering
Build the best hadronic calorimeterMinimize wrong clustering
Granularity
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Sept. 2005
Detector concept studies
3 different incarnations of a PF detector studied
They have a lot in common:
- both ECAL+HCAL inside coil- highly-granular calorimeter- precision pixel vertex detector- common R&D on components!
concepts, but no closed ‘collaboration’
They differ in:
choice of tracking: TPC vs. Si
magnetic field 3 – 5 T
inner radius of ECAL
choice of ECAL readout Si vs Sc
www-sid.slac.stanford.edu
www.ilcldc.org
ilcphys.kek.jp/gld/
SiD
LDC
GLD
M.Piccolo, Frontierscience, Milano
Sept. 2005
A different detector concept
• At the Snowmass meeting in August a new detector concept was presented:
• The main difference with respect to the traditional PFA detectors is that the calorimeter system on which is based can, by construction, separate e.m. energy, e.m. + hadronic energy and may be the binding energy of nuclear components …..
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Sept. 2005
Dual-Readout Module (DREAM)
“Unit cell”
M.Piccolo, Frontierscience, Milano
Sept. 2005
Design Issues and Detector R&D
Detector integral part of ILC Design – meet schedule of GDE
Concept optimisation & R&D to be carried out ….since yesterday!Key components:
1. Vertex Detector
2. Charged Particle Tracking
3. Calorimetry
4. Muon system
5. Trigger
6. Forward Region
7. Machine Detector Interface
https://wiki.lepp.cornell.edu/wws/
R&D review Panel established by world-wide LC study to promote and coordinate detector R&D for the ILC
Keeps tabs of R&D activities around the world at:
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Sept. 2005
do
Vertex Detector ( the GLD preliminary optimization)
Want to prove gHff~mf
O(%) measurements of the branching ratios Hbb,cc,gg
Important for many physics analysese.g. couplings of a low mass Higgs
We like to be better than before
a: point resolution, b : multiple scattering
heavy flavour tagging is a tool of choice
d0 ~ a b/[p(GeV)sin3/2Goal: a=5m, b=10m
M.Piccolo, Frontierscience, Milano
Sept. 2005
Inner radius: ~20 mm for impact parameter resolution the smaller the betterLayer Thickness: as thin as possible minimize conversions, reduce M.S.
Main design considerations:
Constraints: Inner radius constrained by e+e- pair depends on the f.f. details + B field Layer thickness depends on Si technology
T. Maruyama
B=5 T
In the end, design driven by machine + technology !
GLD Baseline design:Fine pixel CCDs (FPCCDs)Point resolution : 5 m Inner radius : 20 mmOuter radius : 50 mmPolar angle coverage : |cos|<0.9
BUT ultimate design depends on worldwide detector R&D
GLD Baseline
M.Piccolo, Frontierscience, Milano
Sept. 2005
Backgrounds in GLD VTX
Assuming to be able to bear 0.5% occupancy, set the radius of the first layer accordingly How much of a disadvantage is B = 3T ?
3 T 4 T 5 T
GLD VTX Forced to a slightly larger inner radius : 2mm ? Will depend on ILC parameters/MDI !
This is a disadvantage of lower B-field in GLD concept How much does the larger inner radius matter ?
Sugimoto
M.Piccolo, Frontierscience, Milano
Sept. 2005
T.KuhlRinner = 26mm Rinner = 15mm
Here charm-tagging efficiency for 70 % purity decreases from 45 % 30 % as Rinner increased from 15 mm 26 mm
NOTE: not completely fair comparison as different wafer thickness
Main impact – charm tagging, e.g.
3 Tesla field not helpful from point of view of charm-tagging BUT probably not a big concern
Tesla study
M.Piccolo, Frontierscience, Milano
Sept. 2005
Vertex Detector
Many technologies under study – very active field
CCD DEPFET MAPSand many others…
750 x 400 pixels20 m pitch
CPR1 CPR1
1 MPixel
CCD with column par. r/o
DEPFET Mimosa 9 (MAPS)
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Sept. 2005
Central Tracking
4 1t(1/ p ) 2.8 10 GeV
4 1t(1/ p ) 0.7 10 GeV
Driving Physics: Particle Flow: efficiency (kinks , high dE/dx), resolution less importantHiggs recoil mass, SUSY di-lepton endpoints: momentum resolution
Two options: Gaseous or Silicon tracker?
TPC:
>200 3D space pointswith ‘gas type’ point-res O(100µm)(LDC, GLD)
Si:
5 (pix) + 5 (strips)high-res pointspoint-res o(few µm)(SiD)
M.Piccolo, Frontierscience, Milano
Sept. 2005
Use Micro Pattern Gas Detectors (GEMs, MicroMegas) for gas amplification
- native 2D structure- ion-feedback suppression built in
-- thin end-plates
R&D topics:
-stable operation on large scale- optimize resolution/pad geometry- operation in magnetic field- field cage design
TPC R&D
Significant effort worldwideLC-TPC collaboration
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Sept. 2005
Central Tracking: Silicon Tracker
SiLC collaboration
R&D:
long ladders (Reduce M.S.)long shaping time: low noise
develop r/o chipspattern recognition use VTX as seed
FE prototype ASICmomentum resolution: simulation
GOAL: testbeam in 2006
M.Piccolo, Frontierscience, Milano
Sept. 2005
Calorimetry
Driving physics: Jet energy resolution in multi-jet (6,8,..) events tau reconstruction non-pointing photons
E.G. : Strong EW symmetry breakingdistinguish W and Z in their hadronic
decays w/o kinematic constraints
E%30E%60
ALEPH like resolution ILC goal
M.Piccolo, Frontierscience, Milano
Sept. 2005
The H self coupling
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Sept. 2005
Calorimeter and Particle Flow algorithm are a real challenge
Present technologies under study:EM calorimeter: Si W (SiD,LDC), Sc W (GLD)HAD calorimeter: scintillating tiles (‘analog’) RPC, GEM, tiles (‘digital’)
addressed by a world-wide R&D efforte.g. CALICE: 26 Institutes, 9 Countriesin 3 Regions
ECAL1st testbeamat DESY
Calorimetry
2 electrons, ~3cm apart
Testbeam data!
M.Piccolo, Frontierscience, Milano
Sept. 2005
HCALHCAL issues:
active medium gaseous or scintillator?
Understand hadron showers
Scintillator: new possibilities with
small photo-sensors (“SiPMs”)
Prototype construction under way
Scintillator plane with SiPM r/oMinical prototype at DESY
Detail of SiPM
Fluctuations of hadronic showersSimulation of same 6 GeV pion:
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Sept. 2005
ECAL+HCAL joint testbeam
Tail Catcher
ECALECAL
HCALHCAL
Electronic Racks
Beam
1m3 prototype testbeam planned for 2006detailed understanding of el-mag and hadronic showers ina highly-granular Calorimeter
M.Piccolo, Frontierscience, Milano
Sept. 2005
Radiator choice for Had.Cal.• Lately W was looked
at as a possible radiator for the Had-cal.
• Detailed evaluation ongoing.
• Material cost could be offset by smaller radius….
• S.C. Coil could cost much less.
M.Piccolo, Frontierscience, Milano
Sept. 2005
Simulation of cal. overall performances
• Simulation results with the two had.cal. options for the LGD
M.Piccolo, Frontierscience, Milano
Sept. 2005
Trigger and DAQ• The common wisdom is that there is
no need for triggering.
• The idea, as of now, is to use commercial hardware to pipeline the data during the beam crossing (~ 1 msec.) and build the event during the intra-beam time (~200 msec.)
• Individual detectors might tag “interesting bunch crossings”
• Really a no-bias trigger.
M.Piccolo, Frontierscience, Milano
Sept. 2005
Program development
Aug. 2005 (Snowmass) - optimize detector parameters. Prepare inputs to machine.
End 2005 - A detector R&D document to go withthe machine baseline configuration document.
End 2006 - Detector Concept Report (one document with multiple concepts, costed) to go with the machine reference design report.
2008 Detector Concept will be part of: ILC Technical Design report
…let me now borrow GDE director transparencies from his Snowmass presentation:
M.Piccolo, Frontierscience, Milano
Sept. 2005
Approach to ILC R&D Program
• Proposal-driven R&D in support of the baseline design. − Technical developments, demonstration
experiments, industrialization, etc.
• Proposal-driven R&D in support of alternatives to the baseline− Proposals for potential improvements to the baseline,
resources required, time scale, etc.
• Develop a prioritized DETECTOR R&D program aimed at technical developments needed to reach combined design performance goals
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Sept. 2005
GDE – Near Term Plan
• Schedule• Begin define Configuration (Snowmass Aug 05) • Baseline Configuration Document by end of 2005-----------------------------------------------------------------------• Put Baseline under Configuration Control (Jan 06) • Develop Reference Design Report by end of 2006
• Three volumes -- 1) Reference Design Report; 2) Shorter glossy version for non-experts and policy makers ; 3) Detector Concept Report
The GDE Plan and Schedule
2005 2006 2007 2008 2009 2010
Global Design Effort Project
Baseline configuration
Reference Design
ILC R&D Program
Technical Design
Bids to Host; Site Selection;
International Mgmt
LHCPhysics
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Sept. 2005
Conclusions
• ILC Physics program is compelling; it does stand on its own.
• LHC and ILC are two remarkable instruments that will help us make the big step forward in understanding our Universe.
•In my opinion, there will be a big positive interference between the LHC and ILC programs.
• Development of the detectors is considered an integral part
of the GDE.
• The schedule for the technical reports/designs is ambitious. 2008 is close: plenty of possibilities to come and contribute to the startup of this program.