the physics case for clic
DESCRIPTION
The Physics Case for CLIC. Outline of the CLIC project Why an e + e - collider with E CM = 3 TeV? A significant step beyond the LHC/ILC for precision measurements at high energies Complete study of the Higgs boson(s)? Supersymmetric spectra? Deeper probes of extra dimensions? - PowerPoint PPT PresentationTRANSCRIPT
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The Physics Case for CLIC
• Outline of the CLIC project
• Why an e+ e- collider with ECM = 3 TeV?
• A significant step beyond the LHC/ILC for precision measurements at high energies– Complete study of the Higgs boson(s)?
– Supersymmetric spectra?
– Deeper probes of extra dimensions?
– New gauge bosons, excited quarks,leptons?
• More to add, whatever the LHC offers
CLIC Physics Studies 1987 -
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World-Wide CLIC Collaboration
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The Conceptual Layout of CLIC
Power from
low-energy, high-intensity beam
drives
high-energy, low intensity beam
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Nominal CLIC Parameters
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CLIC Accelerating Structure
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Nominal Performance Demonstrated
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Possible CLIC Timeline
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Physics at the CLIC Multi-TeVLinear Collider
E. Accomando (INFN, Torino), E. Ateser (Kafkas Univ.), D. Bardin (JINR, Dubna), M. Battaglia (LBL and UC Berkeley), T. Barklow (SLAC), S. Berge (Univ. of Hamburg), G. Blair (Royal Holloway College, Univ. of London), E.Boos (INP, Moscow), F. Boudjema (LAPP, Annecy), H. Braun (CERN), H.Burkhardt (CERN), M.Cacciari (Univ. Parma), O. Çakir (Univ. of Ankara), S. De Curtis (INFN and Univ. of Florence), A. De Roeck (CERN), M. Diehl (DESY), A. Djouadi (Montpellier), D. Dominici (Univ. of Florence), J. Ellis (CERN), A. Ferrari (Uppsala Univ.), A. Frey (CERN), G. Giudice (CERN), R. Godbole (Bangalore), M. Gruwe (CERN), G. Guignard (CERN), S. Heinemeyer (CERN), C. Heusch (UC Santa Cruz), J. Hewett (SLAC), S. Jadach (INP, Krakow), P. Jarron (CERN), M. Klasen (Univ. of Hamburg), Z. Kirca (Univ. of Meselik), M. Kraemer (Univ. of Edinburgh), S. Kraml (CERN), G. Landsberg (Brown Univ.), K. Matchev (Univ. of Florida), G. Moortgat-Pick (Univ. of Durham), M.Muehlleitner (PSI, Villigen), O. Nachtmann (Univ. of Heidelberg), F. Nagel (Univ. of Heidelberg), K.Olive (Univ. of Minnesota), G.Pancheri (LNF, Frascati), L. Pape (CERN), M. Piccolo (LNF, Frascati), W. Porod (Univ. of Zurich), P. Richardson (Univ. of Durham), T. Rizzo (SLAC), M. Ronan (LBL, Berkeley), C. Royon (CEA, Saclay), L. Salmi (HIP, Helsinki), R. Settles (MPI, Munich), D. Schulte (CERN), T.Sjöstrand (Lund Univ.), M. Spira (PSI, Villigen), S. Sultansoy (Univ. of Ankara), V. Telnov (Novosibirsk, IYF), D. Treille (CERN), C. Verzegnassi (Univ. of Trieste), J. Weng (CERN, Univ. of Karlsruhe), T.Wengler (CERN), A. Werthenbach (CERN), G. Wilson (Univ. of Kansas), I. Wilson (CERN), F. Zimmermann (CERN)
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Waiting for the Higgs boson
How soon will the Higgs be found? …
Higgs probability distribution:
combining direct,
indirect informationThe Tevatron or LHC may soon say the Higgs cannot have anintermediate mass: must be either LIGHT, or HEAVY …?
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If there is a light Higgs boson …
• Large cross section @ CLIC• Measure rare Higgs decays unobservable at
LHC or a lower-energy e+ e- collider• CLIC could measure the effective potential
with 10% precision• CLIC could search indirectly for
accompanying new physics up to 100 TeV• CLIC could identify any heavier partners
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Large Cross Section @ CLIC
Can measure rare decay modes …
H bb
Δg/g = 4% Δg/g = 2%
mH = 120 GeV mH = 180 GeV
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Measure Effective Higgs Potential
Large cross section
for HH pair production
Accuracy in measurement of HHH coupling
MH = 240 GeV
180 GeV
140 GeV
120 GeV
11%
9%
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If the Higgs is light …
There must be new physics
below 1000 TeV …
… and CLIC has a
good chance to find it
in contact interactions
LEP ?
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Identify Heavier Partner Higgses
Charged …
… or neutral
1%
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Theorists getting Cold Feet
• Little Higgs modelsextra ‘Top’, gauge bosons, ‘Higgses’
• Interpretation of EW data?consistency of measurements? heavier Higgs?
• Higgs + higher-dimensional operators?corridors to higher Higgs masses?
• Higgsless modelsstrong WW scattering, extra D?
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Generic LittleHiggs Spectrum
Loop cancellation mechanisms
Supersymmetry Little Higgs
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Heretical Interpretation of EW Data
Do all the data tell the same story?e.g., AL vs AH
What attitude towards LEP, NuTeV?
What mostof us think
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Higgs + Higher-Order Operators
Precision EW data suggest they are small: why?
But conspiraciesare possible: mH
could be large, even if believeEW data …?
Do not discard possibility of heavy Higgs
Corridor toheavy Higgs?
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If the Higgs boson is heavier …
Can establish its existencebeyond any doubt if < 1 TeV:
ee H ee
Find resonance in strongWW scattering if > 1 TeV:
ee H νν
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If there is no Higgs boson …
• The LHC might find a hint of strong WW scattering
• The new physics might be invisible at a lower-energy e+ e- collider
• CLIC could study strong WW scattering with high statistics and precision
• CLIC best placed to see/understand scenarios with composite Higgs/quarks/leptons
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Why Supersymmetry (Susy)?
• Intrinsic beauty• Hierarchy/naturalness problem • Unification of the gauge couplings• Predict light Higgs < 150 GeV
– As suggested by precision electroweak data
• Cold dark matter• Essential ingredient in string theory (?)
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Current Constraints on the CMSSM
Excluded because stau LSP
Excluded by b s gamma
Favoured (?) by latest g - 2
assuming neutralino LSP
WMAP constraint on relic density
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Implications of LHC Search for LC
In CMSSM
LHC will tell LCwhere to look
1 ‘year’ @ 10341 ‘year’ @ 1033‘month’ @ 1033‘month’ @ 1032
LHC gluinomass reach
Corresponding sparticle thresholds @ LC
Blaising, JE et al: 2006
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Sparticles may not be very light
FullModel
samples
Detectable@ LHC
ProvideDark Matter
Dark MatterDetectable
Directly
Lightest visible sparticle →
← S
econd lightest visible sparticle
CLIC3 TeV
ILC1 TeV
JE + Olive + Santoso + Spanos
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LHC and CLICScapabilities … and OtherAccelerators
LHC almost
‘guaranteed’
to discover
supersymmetry
if it is relevant
to the mass problem
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Sparticles at Lower-Energy LC
Complementary to LHC: weakly-interacting sparticles
CMSSM
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Sparticle Visibility at CLIC
3 TeV 5 TeV
See ‘all’ sparticles: measure heavier ones better than LHC
CMSSM
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How Soon Might the CMSSM be Detected?
O.Buchmueller et al
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How Soon Might the NUHM1 be Detected?
O.Buchmueller et al
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• NUHM1
Best-Fit Spectra
• CMSSM
O.Buchmueller et al
AccessibleTo ILC 500
Accessibleto ILC 1000
AccessibleTo CLIC
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• b s
Sensitivity to Uncertainties
• g - 2
O.Buchmueller et al
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Example of CLIC Sparticle Search
Dilepton spectrum in neutralino decay
Reach in parameter space
2%
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Measure Heavy Sleptons @ CLIC
Can measure smuon
decay spectrum
Can measure
sparticle masses
2.5%
.
3%
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If the LHC discovers supersymmetry …
• CLIC could complete the spectrum
• CLIC would make many novel, detailed measurements
• Cast light on mechanism of supersymmetry breaking?
• Open a window on string physics?
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Sparticle MassUnification ?
Can test unification
of sparticle masses –
probe of string models?
E L D Q U τ υτ B Q3 T H1 H2
Accuracy in measuring
sparticle masses squared
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Gravitino Dark Matter Scenarios
Scenario with small
gravitino mass
mSUGRA scenario
‘Sweet spot’
For Lithium
Cyburt, JE, Fields, Olive + Spanos
Including
bound-state
effects
with metastable stau as next-to-lightest sparticle
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Cross Section for Stau Production in e+e- Annihilation
Cakir + Turk-Cakir + JE + Kirca
Benchmark in
‘sweet spot’
for LithiumX-sections for
stoppable staus
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Slow-Moving Staus Stop in Detector
Cakir + Turk-Cakir + JE + Kirca
Beam conditions
optimized for
Staus with low
Beam conditions
optimized for total
cross section
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Total Rates for Stoppable Stau Production in e+e- Annihilation
Cakir + Turk-Cakir + JE + Kirca
Including cascade
decays of heavier
sparticles
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If the LHC discovers extra dimensions
Mini-black hole at CLIC
Easily distinguishable from Standard Modelbackground
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CLIC could measure Kaluza-Klein excitations
Direct-channel resonances Angular distribution in graviton decay
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CLIC can measure a Z’
and constrain the triple-gauge
coupling0.00013 @ 3 TeV
Δm = 0.01%
ΔΓ = 0.4%
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Physics
Reaches
Of
Various
Colliders
Squarks 2.5 0.4 3 1.5 2.5
Sleptons 0.34 0.4 1.5 2.5
New gauge boson Z’
5 8 6 22 28
Excited quark q*
6.5 0.8 7.5 3 5
Excited lepton l*
3.4 0.8 3 5
Two extra space dimensions
9 5–8.5
12 20-35
30–55
Strong WLWL
scattering2 - 4 70 90
Triple-gaugeCoupling(TGC) (95%)
.0014
0.0004
0.0006
0.00013
0.00008
14 TeV
0.8 TeV
14 TeV
3 TeV 5 TeV
Scale ofcompositeness
30 100 40 300 400
Process LHC/ILC/SLHC/CLIC 3,5 TeV
Integrated luminosities used are 100 fb–1 for the LHC, 500 fb–1 for the 800 GeV LC, and 1000 fb–1 for the SLHC and CLIC. Most numbers given are TeV, but for strong WLWL scattering the numbers of standard deviations, and pure numbers for the triple gauge coupling (TGC).
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Conclusions
• CLIC will provide unique physics @ energy frontier
• Beamstrahlung and backgrounds not insurmountable problems
• Can exploit fully high c.o.m. energy• Added value for light Higgs, heavy Higgs,
supersymmetry, extra dimensions, …• Whether light or heavy!
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Meta-Conclusions
• The LHC will define the future course of high-energy physics
• All scenarios best explored by a high-energy e+ e- collider
• Should have widest possible technology choice when LHC results appear
• CLIC and ILC are working together• Determine feasibility of CLIC technology
by the end of this decade
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Supersymmetric Benchmark Studies
Specific
benchmark
Points along
WMAP lines
Lines in
susy space
allowed by
accelerators,
WMAP data
Sparticle
detectability
Along one
WMAP line
Calculation
of relic
density at a
benchmark
point
BDEG(M)OP(W)
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The Reach of the LHC for New High-Mass Physics
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Event rates in ATLAS or CMS at L = 1033 cm-2 s-1
Huge Statistics thanks to High Energy and Luminosity
LHC is a factory for anything: top, W/Z, Higgs, SUSY, etc…. mass reach for discovery of new particles up to m ~ 5 TeV
Process Events/s Events per year Total statistics collected at previous machines by 2007
W e 15 108 104 LEP / 107 Tevatron
Z ee 1.5 107 107 LEP
1 107 104 Tevatron
106 1012 – 1013 109 Belle/BaBar ?
gg~~
tt
bb
H m=130 GeV 0.02 105 ?
m= 1 TeV 0.001 104 ---
Black holes 0.0001 103 ---m > 3 TeV (MD=3 TeV, n=4)
LHC-b
+ Ion Collisions
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Cross Sections at CLIC
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Experimental Issues: Backgrounds
CLIC 3 TeV e+e- collider with a luminosity ~ 1035cm-2s-1 (1 ab-1/year)
To reach this high luminosity: CLIChas to operate in a regime of high beamstrahlung
Expect large backgrounds# of photons/beam particle e+e- pair production events Muon backgrounds Neutrons Synchrotron radiationExpect distorted lumi spectrumReport
Old Values
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Experimental issues: Luminosity Spectrum
Luminosity spectrum not assharply peaked as e.g. at LEPor TESLA/NLC
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New Parameters..See D. Schulte
Same bunch distance (0.6 nsec) 2 x more bunches per train Backgrounds similar or somewhat better
Do not except significant differences with studies in the report
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Example: Resonance ProductionResonance scans, e.g. a Z’
Degenerate resonancese.g. D-BESS model
1 ab-1 M/M ~ 10-4 & / = 3.10-3
Can measure M down to 13 GeV
Smeared lumi spectrum allowsstill for precision measurements
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Physics Case: the light Higgs
Large cross sections Large CLIC luminosityLarge events statistics Keep large statistics also for highest Higgs masses
O(500 K) Higgses/yearAllows to study the decaymodes with BRs ~ 10-4 suchas H and Hbb (>180 GeV) Eg: determine gH to ~4%
Low mass Higgs:400 000 Higgses/
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Physics case: Heavy Higgs (MSSM)
LHC: Plot for 5 discovery
3 TeV CLIC H, A detectable up to ~ 1.2 TeV
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Susy Mass Measurements
Momentum resolutionpt/pt
2 ~ 10-4 GeV-1
adequate for thismeasurement
Mass measurementsto O(1%)
Momentum resolution (G3)
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Physics Case: Extra Dimensions
Universal extra dimensions: Measure all (pair produced) newparticles and see the higher level excitations
RS KK resonances…Scan the different states
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Rare Higgs Decays: H
gH
Not easy to access at a 500 GeV collider
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How `Likely’ are Large Sparticle Masses?
Fine-tuning of EW scale Fine-tuning of relic density
Larger masses require more fine-tuning: but how much is too much?
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CMSSM
How much of Susy Parameter Space Covered by LC?
Scatter plot of twolightest observablesparticles : NSP, NNSP
Reach of 1000 GeV LC
Reach of 500 GeV LC
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Why Supersymmetry (Susy)?
• Hierarchy problem: why is mW << mP ?
(mP ~ 1019 GeV is scale of gravity)• Alternatively, why is
GF = 1/ mW2 >> GN = 1/mP
2 ?• Or, why is
VCoulomb >> VNewton ? e2 >> G m2 = m2 / mP2
• Set by hand? What about loop corrections?
δmH,W2 = O(α/π) Λ2
• Cancel boson loops fermions• Need | mB
2 – mF2| < 1 TeV2
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Other Reasons to like Susy
It enables the gauge couplings to unify
It stabilizes the Higgs potential for low masses
Approved by Fabiola Gianotti
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Current Constraints
on CMSSM
Impact ofHiggsconstraintreducedif larger mt
Focus-pointregion far up
Differenttan βsign of μ
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Exploring the Supersymmetric Parameter Space
Strips allowed by WMAP
and other constraints
Numbers of
sparticle
species
detected
at LHC
along WMAP
strip
Numbers of
sparticle
species
detected
at CLIC
along WMAP
strip
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Density belowWMAP limit
Decays do not affectBBN/CMB agreement
DifferentRegions of
SparticleParameterSpace if
Gravitino LSP
DifferentGravitinomasses
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Effects on GDM parameter Space
Scenario with fixed
gravitino mass
Scenario with varying
gravitino mass
‘Sweet spot’
For LithiumCyburt, JE, Fields, Olive + Spanos
Including
bound-state
effects
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Little Higgs Models
• Embed SM in larger gauge group• Higgs as pseudo-Goldstone boson• Cancel top loop
with new heavy T quark
• New gauge bosons, Higgses• Higgs light, other new
physics heavyMany extra particles accessible to CLIC
MT < 2 TeV (mh / 200 GeV)2
MW’ < 6 TeV (mh / 200 GeV)2
MH++ < 10 TeV
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If the LHC discovers supersymmetry …
• CLIC could complete the spectrum
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If there is a light Higgs boson …
• Large cross section @ CLIC
• Measure rare Higgs decays unobservable at LHC or a lower-energy e+ e- collider
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If there is a light Higgs boson …
• Large cross section @ CLIC
• Measure rare Higgs decays unobservable at LHC or a lower-energy e+ e- collider
• CLIC could measure the effective potential with 10% precision
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Higgsless Models
• Four-dimensional versions:
Strong WW scattering @ TeV, incompatible with precision data?
• Break EW symmetry by boundary conditions in extra dimension:
delay strong WW scattering to ~ 10 TeV?
Kaluza-Klein modes: mKK > 300 GeV?
compatibility with precision data?
• Warped extra dimension + brane kinetic terms?
Lightest KK mode @ 300 GeV, strong WW @ 6-7 TeV
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