Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 61
Day2: Physics at TESLADay2: Physics at TESLA
• Origin of Electroweak Symmetry Breaking as one
great Motivation for a Linear Collider
• The TESLA project
• Higgs Precision Physics at TESLA
• Leaving the Standard Model Behind…
• Precision tests
• Summary
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 62
ElectroElectro--Weak Symmetry BreakingWeak Symmetry Breaking
Quantum Field Theory with massive Quanta fails at high Energies:
Cross section:σ∼ sViolates unitarity at
(if forces remain weak)
TeVs 2.1~
“if nothing happens, something must happen…”
The SM solution:(rescue of the beautiful gauge principle) Introduction of a new scalar field with non-zero field strength In the vacuum: the Higgs Field.
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 63
The Higgs MechanismThe Higgs Mechanism
21 2
2222
vgMwhereMq
=−
Paradigm:All (elementary) particles are massless (per se)
gauge principle worksrenormalizable theory (finite cross sections)
permanent interaction with the Higgs field acts as if particles hada mass (effective mass)
2q1gv 2
2
24
2
2q1gv
2q1
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 64
Where is the Where is the HiggsHiggs Boson?Boson?
Theory:Upper bound: perturbativity (λ<1)Lower bound: vacuum stabilityModels: minimal SUSY: m<135 GeV
GUT’s : m<180 GeV
Experiment:Precision measurements (LEP,SLC,Tevatron) are sensitive tovirtual corrections:
m<200 GeV (95% CL)
The Higgs Boson is probably “light”!
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 65
Higgs Search at TevatronHiggs Search at Tevatron
Maybe…
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 66
Higgs Search at the LHCHiggs Search at the LHC
Production processes:
For m=120 GeV: σ ~ 25 pb 2.5 million Higgs/yearLHC = Higgs factory ?
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 67
Higgs Search at the LHCHiggs Search at the LHC
Gigantic backgrounds!
look for rare but wellmeasureable final states
!hopelessisbbHgg →→
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 68
Higgs Search at the LHC (m<150 GeV)Higgs Search at the LHC (m<150 GeV)
Loop induced decay:
Backgrounds:γγ production 2pb/GeV need σ(m)/m ~ 1%γ + jet, jet-jet production (reducibel) need 10 γ/πsuppression -3 0
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 69
Up to m<600 GeV:Standalone discoverywith 30Above: ZZ llνν andWW lνqq needed
Higgs Search at the LHC: m> 150 GeVHiggs Search at the LHC: m> 150 GeV
ATLAS clear 4-lepton signature,almost background free
1−fb
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 70
Higgs Search at the LHCHiggs Search at the LHC
Discovery potential:
Single channels: Combined channel + expts:
With 10 fb : 5σ discovery in the whole mass range!
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 71
Higgs at the LHC after discovery: Measurements?Higgs at the LHC after discovery: Measurements?
In the SM, all properties of the Higgs boson are predicted, onceits mass is known crucial test of EW symmetry breaking
Absolute measurements are difficult at hadron machines, due touncertainties in production cross sections (QCD,structure functions)and background modelling
Some first measurements can be done:
•Mass: 0.1 – 0.4%•Total Width: 10-20%, model dependent•Production rates: 10-20%•Ratios of couplings: W/Z, W/t, W/τ: 10-20%
To really establish the Higgs mechanism, higher precision and less model depence is needed: Linear Collider!
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 72
•Superconducting e e linear collider
•Phase 1: 500 GeV •Phase 2: 800++ GeV•Luminosity: 3-5x10 cm s•300 – 500 fb / year•Polarized beams•Running options: γγ, eγ, e e ,Giga-Z•Integrated X-Ray Free Electron Laser
The TESLA ProjectThe TESLA Project
+ -
-1
34 -12
- -
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 73
BeamstrahlungBeamstrahlung
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 74
BeamstrahlungBeamstrahlung
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 75
A Detector for TESLAA Detector for TESLA
Detector optimized forprecision physics
Design driven by Higgsphysics in many cases:
-Vertex detector (b/c separation)-Momentum resolution( )-Energy flow: jet reconstruction
Broad R&D programCurrently starting
0Z + −→
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 76
CalorimetryCalorimetry
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 77
CalorimetryCalorimetry
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 78
MaskMask
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 79
Physics Program at TESLAPhysics Program at TESLA
Highlights:
• Origin of Elctroweak symmetry breaking: precision Higgs physics
• Breakdown of the Standard Model
• Supersymmetry
• Extra Space Dimensions
• New Gauge Bosons
• Flavour physics: top quark
• (SM?) Precision measurements
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 80
After the discovery of a Higgs boson, the key task is to establish the Higgs mechanism in all elements as responsiblefor EW symmetry breaking
Electron-Positron Linear Colliders (NLC,JLC,TESLA) withenergies up to 1 TeV and high (300-500 fb /year) are
1. Technologically within reach2. The ideal tool for precision Higgs physics
Precision Measurements should comprise:• Mass• Total Width• Quantum numbers J (Spin 0 ?)• Higgs-Fermion couplings (~ mass ?)• Higgs-Gauge-Boson couplings (W/Z masses)• Higgs self coupling (spontaneous symmetry breaking)
Measurements should be precise enough to distinguish betweendifferent models (e.g. SM/MSSM, extra dimensional effects, …)
Precision Higgs Physics at a Linear ColliderPrecision Higgs Physics at a Linear Collider
-1
PC
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 81
The Higgs Boson Profile at TESLAThe Higgs Boson Profile at TESLA
decay-mode independent Higgs tag:
• select di-lepton eventsconsistent with Z ll
• calculate recoil mass
∆σ ~ 3%model independentmeasurement!
∆m ~ 50 MeVMass measurement:
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 82
The Higgs Boson Profile at TESLAThe Higgs Boson Profile at TESLA
Key issue: momentum resolution:
“Lep”-like resolution Goal with TESLA TPC+Si
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 83
The Higgs Boson Profile at TESLAThe Higgs Boson Profile at TESLA
large cross section atlarge
model independent handleon total width, when combinedwith BR(H WW):
s
)WWH(BRWW
tot →Γ
=Γ
%tot 5≅∆Γ
WW-fusion process:
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 84
The Higgs Boson Profile at TESLAThe Higgs Boson Profile at TESLA
Higgs field responsible for particle masses Couplings must be proportional to the particle masses
Decisive Test: precision analysis of the Higgs branching ratios:
Decay Precision
for 500 fb , m=120 GeV-1
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 85
Separation ofand
The Higgs Boson Profile at TESLAThe Higgs Boson Profile at TESLA
bbH →ccH → Needs high resolution vertex dector:
First layer at 1.5 cm from interaction point!
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 86
The Higgs Boson Profile at TESLAThe Higgs Boson Profile at TESLA
b- and c-tagging efficiencies:
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 87
The Higgs Boson Profile at TESLAThe Higgs Boson Profile at TESLA
Higgs Quantum Numbers: Is it really a Higgs?
Spin from threshold scan:
10 fb /point-1
CP quantum numbers from:
-Angular distribution of H and Z
-Transverse polarisation correlations in H ττ
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 88
The Higgs Boson Profile at TESLAThe Higgs Boson Profile at TESLA
Top quark Yukawa coupling:
-need highest energy-heaviest quark surprises?-small cross section-complicated final state
achievable precision:
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 89
The Higgs Boson Profile at TESLAThe Higgs Boson Profile at TESLA
Global fit of Higgs couplings (HFITTER):
Measurements precise enough to obatain sensitivity beyond cms energy!
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 90
The Higgs Boson Profile at TESLAThe Higgs Boson Profile at TESLA
Higgs self-coupling (‘the holy grail’):
Close connection to the shape of the Higgs potentialessential test of the mechanism of spontaneous symmetry breaking
Tiny cross sectionComplicated multi-jet final state
detector design: energy flow
Need highest luminosityPrecision for 1 ab :
%20≅∆λ
λ
-1
LEP TESLA
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 91
divergent W W W W amplitude
new strong interaction at
spontaneously broken chiral symmetry
Goldstone bosons (“Pions”) = W states (“technicolor”)
no calculable theory until today in agreement with precision data
Experimental consequences: deviations in triple and quartic gauge
couplings:
No Higgs Boson?No Higgs Boson?
L L L L
L
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 92
Triple Gauge CouplingsTriple Gauge Couplings
TGC’s are a universalprecision test fornew physics
Sensitivity to new physicsscale Λ:
At 500 GeV, 500 fb -1
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 93
Quartic Gauge CouplingsQuartic Gauge Couplings
Sensitivity to new physicsscale Λ:
- complicated final state- need to separate WW 4q and ZZ 4qenergy flow!
complete threshold regionof new strong interactioncovered
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 94
Physics beyond the Standard ModelPhysics beyond the Standard Model
SM cannot be the ultimate theory!
Why???
• Hierarchy problem
• Gravity
• Many free parameters
• Cold dark matter
• Baryon asymmetry
• Connection between quarks and leptons? Q(proton) = Q(positron)
• Connection between the families: ‘flavour physics’
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 95
The Hierarchy problemThe Hierarchy problem
In Nature, there are two largely different mass scales:
1. The electroweak scale: v = 246 GeV
2. The Planck scale:
The particle masses (especially the Higgs mass) recieve largescale dependent corrections, e.g.
19PlanckM =10 GeV
2 2Mδ Λ∼ Λ is the scale up to whichThe SM should be valid
⇒ If it is hard to believe that the correctionGets compensated by a bare mass which is alsoTo yield a physical Higgs massSomething should “protect” the Higgs mass!
2 2PlanckM Mδ ∼
2Planck(M )o
2(v )o
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 96
SupersymmetrySupersymmetry
is one of the most attractiveextensions to the SM!
Simple Idea:
Symmetry betweenBosons and Fermions
each SM particle has aSUSY partner with sameQuantum numbers andSpin differing by ½.
But where are the SUSYPartners? Must be heavy
SUSY must be broken!
Why is it so attractive, then?
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 97
Why is SUSY so attractive?Why is SUSY so attractive?
1. It solves the Hierarchy problem:
The divergency in the Higgs mass corrections if cancelled exactlyFor unbroken SUSY.
If it is not broken too heavily (i.e. if the SUSY partners are at<~ 1 TeV), there is no fine tuning necessary.
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 98
Why is SUSY so attractive?Why is SUSY so attractive?
2. It shows a path to Grand unification:
This is achieved for
Experiment:
2 SUSYWsin θ = 0.2335(17)
2 exp.Wsin θ = 0.2315(2)
Minimal SUSY prediction:
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 99
Why is SUSY so attractive?Why is SUSY so attractive?
3. Cold Dark Matter:
The lightest SUSY partner particle might well be stable andAn excellent candidate for the observed cold dark matter
4. Link to Gravity:
SUSY offers the theoretical link to incorporate gravity. Most stringmodels are supersymmetric.
5. Light Higgs Boson:
SUSY predicts a light (< 135 GeV) Higgs boson as favoured byElectro-weak precision data from LEP and Tevatron.
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 100
The Supersymmetric particle spectrumThe Supersymmetric particle spectrum
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 101
SUSY precision measurements at TESLASUSY precision measurements at TESLA
Typical production in collisions: pair production, e.g.: + -e e
Detector signature:2 Muons + miss.Energy
Muon energies:‘box spectrum’Endpoints contain informationabout masses of Smuon and Neutralino
Reachable precision o(100 MeV)
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 102
SUSY precision measurements at TESLASUSY precision measurements at TESLA
Alternative: mass from threshold scan
0 0 0 0
2 2 1 1e e χ χ χ χ+ − → →
Reachable precision < 100 MeV
Disentangle different states, in caseThere are many SUSY particles
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 103
SUSY precision measurements at TESLASUSY precision measurements at TESLA
Beam Polarisation allows SUSY parameter determination.Example: Neutralino-sector depends on 4 parameters:
2 1tan , , ,M Mβ µ
1M can be obtained from polarisation dependence of cross sectionand FB-Asymmetry
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 104
But maybe more demanding signatures…But maybe more demanding signatures…
In some SUSY scenarios(‘GMSB’) the Neutralinois not stable:
‘non-pointing’ photonsignaturedemanding for calorimetry!
01 Gχ γ→
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 105
Extrpolation to very high scalesExtrpolation to very high scales
• SUSY parameters ‘run’ with energy (like SM coupling constants)
• Running described by Renormaisation Group Equations (RGE’s)
• Precise measurement of SUSY parameters at ‘low’ (i.e. TESLA)allows to extrapolate to very high (e.g. GUT) scales and test thehigh energy behaviour of SUSY
Test of Grand Unification becomes possible
Information about the mechanism which breaks SUSY can be
obtained
“mSUGRA” “GMSB”
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 106
Extra Space Dimensions?Extra Space Dimensions?
• Completely alternative approach to solve the hierarchy problem:‘There is no hierarchy problem’
• Suppose, the SM fields live in ‘normal’ 3+1D space• Gravity lives in 4 + δ Dimensions• δ extra Dimensions are curled to a small volume (radius R):
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 107
Extra Space Dimensions?Extra Space Dimensions?
For r < R, gravity follows Newtons law in 4+δ dimensions:
1( ) SGV rrδ +
=
w( h) itS N SN
G G GV r GR r r Rδ δ= = =
For r > R, gravity follows effectively Newton’s law in 4 dimensions,since the ‘distance’ in the extra dimensions does not rise anymore:
If e.g. R ~ o(100 µm) and δ=2 one obtains ! (1TeV)SM o=
The Planck-Mass only effectively appears
so high at large distances. The true scale of gravity is
2 /Planck NM c G=
2 / /S S NM c G cR Gδ= =
Gravity might become visible in TeV-scale colliders as TESLA!!
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 108
Extra Space Dimensions?Extra Space Dimensions?
Effects from real graviton emission:
measures the numberof extra dimensions!
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 109
Extra Space Dimensions?Extra Space Dimensions?
Effects from virtual graviton exchange:
can prove Spin-2 exchange!
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 110
New Gauge BosonsNew Gauge Bosons
If there is a GUT, the GUT gauge group (e.g. SU(5)) might be brokenin steps e.g. new U(1) at the TeV scale new Z’ boson.TESLA has reach up >10 TeV through interference of Z’ with Z and γ.
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 111
New Gauge BosonsNew Gauge Bosons
If LHC observes at Z’, TESLA can measure itscouplings and pin down the model
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 112
Top Quark precision physicsTop Quark precision physics
∆m(top) ~ 100 MeV
∆Γ(top)/Γ(top) ~ 5%
Threshold scan of e e tt+ − →
study top production anddecay angular distributions
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 113
Return to the Z0: GigaReturn to the Z0: Giga--ZZ
Operate TELSA at the Z-Pole and WW-threshold1 Billion Z0’s in a few months (100xLEP)
• (factor 10 better than LEP) •
2sin 0.000013Wθ∆ =6 MeVWM∆ =
Klaus Desch, Physics at e+e- Colliders, DESY Summer Student Lecture 08/2002 Page 114
SummarySummary
• TESLA physics is fascinating
• Higgs Mechanism can be established in all essential details
• Precision SUSY measurements reconstruct fundamental theory
• Precision is the key sensitivity far beyond collider energy
• World-wide consenus that a Linear Collider should be the next major step in HEP
• This will be YOUR machine!