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Detecting Massive Scalar Particles Detecting Massive Scalar Particles at Proton at Proton Colliders Colliders Darin Acosta University of Florida

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Page 1: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalar Particles Detecting Massive Scalar Particles at Proton at Proton CollidersColliders

Darin AcostaUniversity of Florida

Page 2: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta2

OutlineOutlineMotivation for scalar particles in particle theories

The Higgs particleSupersymmetry

Hints of scalar particlesThe Tevatron collider and the CDF experiment

Review of Run 1 searches for Higgs and SUSYStatus of Run 2 and search prospects

The Large Hadron Collider and the CMS experimentConstruction progress and search prospects

Page 3: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta3

Why Not Scalars?Why Not Scalars?So far, all known matter is composed of spin-½ fermions

electrons, protons, neutrons, …Thus, atomic and nuclear structure obeys the Pauli-Exclusion principleScalar objects do exist, but actually they are composites

e.g. 4He, π+

In fact, all nuclear particles are composed of spin-½ quarksp = u u dn = u d d π+ = u d

Additionally, three of the fundamental forces are propagated by spin-1 bosons

Electromagnetism: Photons (γ)Weak nuclear force: W+, W-, Z bosonsStrong nuclear force: gluons (g)

Quantum gravity would be propagated by a spin-2 boson

unified into one electro-weak theory

Page 4: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta4

Elementary ParticlesElementary Particles

mu,d ~ 5 MeVmγ = 0

mt = 174 GeV

mg = 0

mZ = 91.188 GeVmν ≠ 0 ?

me = 0.511 MeV mW = 80.4 GeV

1 eV = 1.6 × 10–19 J

Page 5: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta5

The Higgs MechanismThe Higgs MechanismThe electro-weak theory is described by the SU(2)×U(1) Weinberg-Salam ModelThe quantum field theory of the strong force is described by Quantum ChromodynamicsCollectively, they are referred to as the “Standard Model”However, all masses are zero unless we introduce a scalar field, and this scalar field must obtain a non-zero vacuum expectation value through spontaneous symmetry breaking

Generates mass for the vector bosonsGenerates mass for the fermionsGenerates a massive neutral scalar

Page 6: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta6

Theoretical Higgs Mass ConstraintsTheoretical Higgs Mass Constraints

Self consistency of the Standard Model places upper and lower bounds on the Higgs mass

Wide mass range up to ~1 TeV allowed if new physics comes in at scale of 1 TeV

Narrow mass range if new physics doesn’t enter until Grand Unification scale

200 400 600 8000MH (GeV)

103

106

109

1012

1015

1018

Mas

s sc

ale

for n

ew p

hysi

cs (G

eV)

ExcludedExcl

uded

Page 7: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta7

Indirect Experimental ConstraintsIndirect Experimental ConstraintsDirect mW, mtmeasurementsIndirect from electro-weak parameters

SM predictions

PDG, 2002

Page 8: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta8

Direct Higgs Search at eDirect Higgs Search at e++ee-- CollidersCollidersThe Large Electron Positron (LEP) collider at CERN ran from 1989 until 2000

In depth studies of the Z-boson resonance at 91 GeVSteadily increased energy to 209 GeV to study W

production and to search for the Higgs Shut down to allow construction of the Large Hadron

Collider

Possible hint of the Higgs ?

Lower bound on Higgs mass assuming no signal is 114 GeV at the 95% CL

Nobs = 4Nexp = 1.25

⇒ P = 3%

Page 9: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta9

SupersymmetrySupersymmetry: : another source of scalarsanother source of scalarsWhy is all matter spin-½ ?Antimatter is the charge conjugation of normal matter

C |e-⟩ = |e+⟩Predicted by P.A.M. Dirac in 1928, observed in 1932

Is there a spin conjugation as well?Q |fermion⟩ = |boson⟩

Such “Supersymmetry” generalizes space-time symmetryPredicts partners to all known particles with opposite spin statistics

Not so good for a theory, which ought to reduce the number of free parameters (28 for the Standard Model) !

Points the way to a larger theoryWhen Supersymmetry is required to be a local symmetry, it

can incorporate gravity (Supergravity)Supersymmetry is a prerequisite for string theoriesAllows for Grand Unification

Page 10: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta10

Grand UnificationGrand UnificationCoupling “constants” vary with the energy scaleMinimal Supersymmetric models allow for the unification of

3 forces at one energy scale (would miss otherwise)

Gravity137

128

EM

Weak

1 / c

oupl

ing

Strong

1016 GeVMPlanck = 1019 GeV102 GeV

Page 11: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta11

Supersymmetry Supersymmetry is Brokenis BrokenIf Supersymmetry exists, there should be scalar partners to the fermions

e.g. scalar electrons, which would not obey the Pauli-Exclusion Principle in atoms

So far, no such particles are observed at low energy

Supersymmetry cannot be an exact symmetry, and must spontaneously break at some energy scale

Particle masses should be less than about 1 TeV

Lightest Higgs boson (there are at least 5 of them) must have mass < 135 GeV

Page 12: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta12

LeptoquarksLeptoquarks: also a source of scalars: also a source of scalarsThere is no explanation in the Standard Model for why atoms are electrically neutral

Specifically, the relationships between quark and lepton electroweak charges exactly cancel triangle anomalies in the Standard Model

Makes the Standard Model a renormalizable theory

Leptoquarks arise in Grand Unification models, “technicolor”, Supersymmetry, and compositeness

Connects the lepton sector to the quark sector, which otherwise are just ad hoc ingredients to the SM

LQs are color triplet bosons (scalar or vector) with lepton number and fractional electric charge

Hint of leptoquarks in data taken by the HERA electron-proton collider in 1997, but no longer seems likely

eLQ

q

Page 13: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta13

Cosmological Implications of ScalarsCosmological Implications of ScalarsIn the Minimal Supersymmetric Standard Model the lightest supersymmetric particle is stable

Generally a neutral, weakly interacting particle (neutralino)Good candidate for Cold Dark Matter

Scalar particles can obtain a non-zero vacuum expectation value (vacuum energy)

May give rise to a cosmological constant

Current consensus among cosmologists from measurements of the cosmic microwave background, supernovae, Big Bang nucleosynthesis, clusters of galaxies,…

Ω ≈ 1 (flat universe)ΩΛ ≈ 0.7, Ωm ≈ 0.3

Ωm = Ωb + ΩCDM ; Ωb ≈ 0.04

Page 14: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

The The Fermi Fermi National AcceleratorNational Accelerator

LaboratoryLaboratory

Batavia, Illinois

Page 15: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta15

The The TevatronTevatronProton-Antiproton collider

Ebeam = 1 TeVR = 1 km

In operation since 1985Major upgrade completed in 1999

CDF D∅

Main injector

Page 16: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta16

The The Collider Collider Detector at Detector at FermilabFermilab

Beam direction

Run 1: 1992 – 1996 L=120 pb-1

A very large, general purpose “microscope” to study the structure of matter Hundreds of researchers participate

Page 17: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta17

Discovery of the Top Quark in 1995Discovery of the Top Quark in 1995

t t → b b W+ W- → b b q q’ e ν

b

b

eRelatively long-lived

Mtop = 174 ± 5 GeV

Page 18: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta18

CDF Heavy Flavor TaggingCDF Heavy Flavor TaggingBottom quarks and charm quarks have a lifetime of about 1 ps

Tag bottom and charm quarks by reconstructing the secondary vertex of their decay products

Measure the flight distance (L)Typically several hundred microns,

extending up to a few mmThis is still within the beam pipe, not in the detectors, so we must extrapolate a precisely measured track

An important signature of the decay of heavier particles…

Lprimary vertex

jet

Page 19: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta19

Branching Ratios for Higgs Decay Branching Ratios for Higgs Decay

BR (H →bb) ~ 1

BR (H →WW →2µ)

~ 0.01

BR (H →ZZ →4µ)

~ 3x10-4

BR (H →γγ) ~ 10-3

Tagging b quarks is important to discover a light Higgs

Page 20: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta20

Higgs ProductionHiggs Production

p

p

Note:σ = scattering cross section1 pb = 10–36 cm2

L·σ = N (number of events)L = 120 pb–1 for Run 1

Page 21: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta21

Relative Yields at the Relative Yields at the TevatronTevatron

Higgs Signal

(one in a billion collisions!)

1 fb = 10–3 pb

1 pb

Background

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Detecting Massive Scalars Darin Acosta22

Observed events agree well with background expectations

Require 10–100X more data to be sensitive to SM Higgs production

No anomalous production

WH, ZHproduction

SM Higgs Search in Run 1SM Higgs Search in Run 1

Page 23: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta23

Signatures of Signatures of SupersymmetrySupersymmetryLarger cross sections for the production of scalar quarks and gluons rather than leptons at a proton collider because of the strong force couplings

Examples:

Signatures:Jets (from the hadronization of quarks and gluons)Missing energy (from undetected lightest SUSY particle)

Backgrounds:QCD jetsW/Z productiontop quarks

Review just one search of many here

gggqqqpp ~~,~~,~~→ jetsEGgq T +/⇒~,~,~

HF jetsE b,t T ~~ +/⇒qGGgGGpp ~~,~~→

1111~~,~~ bbttpp →

Orders of magnitude larger

Page 24: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta24

Scalar Top Quark SearchScalar Top Quark SearchThe heavy top quark mass gives rise to a large mixing between the left- and right-handed scalar top eigenstates

Results in a large mass splitting between the two mass eignenstates

Thus, the “stop” could be the lightest scalar quark

Search for the pair production of stop quarks

Look for the decays:

(if first closed)

q

q

t

t

g

g

t

t

g

g

t

t

g

g

t

t

~t b→ ±χ1

~ ~t c→ χ10

Page 25: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta25

Scalar Top Quark Search (Jets + MET)Scalar Top Quark Search (Jets + MET)

)>>± tMMM ~()~()~( 1 νχ

t~

*1

~±χ

*b c01

~χ*W3.6|| and GeV 157 withjets No

2|| and GeV 15 jets, 3or 2T

T≥≤≤

≤≥η

ηE

E

Use Missing transverse energy data sample

• Cuts on jet-MET, jet-jet angles• No l with PT > 10 GeV

Main Backgrounds:• MET > 40 GeV

jet~ 2(3,4,...)+ → ννZjet ,...)3,2(1+→τνW

QCD

quark tag charm 1 Require ≥

events 4.214.5Expect ±Observe 11

Published: PRL, 84,5704(2000)

Page 26: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta26

40

45

50

55

60

65

70

75

80

85

80 90 100 110 120 130M(t∼ 1) (GeV)

M(ν∼ )

(GeV

)

M(t∼ 1) = M(b) + M(ν∼ )

ALEPH√s=189 GeVθstop=0

CDF - 88 pb- 1

95% CL Excluded

BR(t∼ 1 → b l± ν∼ )=100%

CDF Excluded Region ≡σ95%CL(t∼ 1t

∼_

1) <σNLO(t∼ 1t∼_

1)[σNLO: µ=m(t∼ 1),CTEQ3M]

(hep-ph/9611232)

LEP1 excluded0

10

20

30

40

50

60

70

80

90

0 20 40 60 80 100 120 140

BR (t∼1 → c + χ

∼10) = 100%

θt∼ = 0.0

D0/7.4 pb-1

OPAL√s=189 GeV

M(t

∼ 1)=

M(c

)+M

(χ∼ 10 )

M(t

∼ 1)=

M(b

)+M

(W)+

M(χ

∼ 10 )CDF - 88 pb-1

95% CL

M(t∼1) (GeV/c2)

M(χ∼

10 ) (G

eV/c

2 )

Scalar Top Quark LimitsScalar Top Quark Limits

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Detecting Massive Scalars Darin Acosta27

CDF II DetectorCDF II DetectorGoal:

Run 2a: 2001 – 2004 (2000 – 4000 pb-1)

Run 2b: 2004 – 2007+(15000 pb-1)

Completely new electronicsNew plug calorimeterNew muon chambersNew central trackerNew silicon vertex detector

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Detecting Massive Scalars Darin Acosta28

Silicon Vertex DetectorSilicon Vertex DetectorRadius: inner = 1.35 cm, outer = 29 cm Length: 90 cmstrip pitch: 60µmDouble-sided layers for r–φ, stereo r–φ, r–z New

$20M

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Detecting Massive Scalars Darin Acosta29

March 2001CDFCDF--II Rolling into the Collision HallII Rolling into the Collision Hall

Page 30: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta30

Run 2 Integrated Luminosity (CDF)Run 2 Integrated Luminosity (CDF)

≈70 pb–1 delivered

≈50 pb–1 recorded

Best instantaneous luminosity: 2.8×1031 cm–2 s–1

Design goal: 8.6×1031 cm–2 s–1

Expect 100–200 pb-1 delivered by end of year

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Detecting Massive Scalars Darin Acosta31

W Boson Measurement from ElectronsW Boson Measurement from Electrons

W cross section measurement from W e ν

σ(W)*BR(W eν) (nb) =2.60±0.07stat±0.11syst ±0.26lum

Consistent with Run 1 results rescaled for higher collision energy: 2.72±0.02stat±0.08syst ±0.09lum

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Detecting Massive Scalars Darin Acosta32

Observation of Z BosonsObservation of Z Bosons

-57 candidate events in 66<Minv<116 range

µ1

µ2

Clear evidence of Z µ+µ–

Signal shown for opposite sign muons detected in both inner and outer muon chambers

Page 33: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta33

Tagged Muon in CDF Tagged Muon in CDF

Note: B mesons decay into soft leptons about 10% of the time

Muon

Contained in a jet with ET= 9 GeV

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Detecting Massive Scalars Darin Acosta34

Secondary Vertices in CDF IISecondary Vertices in CDF II

Event : 63457 Run : 138046 EventType : DATA | Unpresc: 33,7,13,21,53,23,55,27 Presc: 33,27 Myron mode: 0

PV

SV muon

Zoom-in of previous event:

Event was tagged by the “Jet Probability” algorithm we are developing at UF for tagging bottom and charm jets

Jets containing soft muons exhibit low probability of coming from the primary vertex

Page 35: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta35

SM Higgs Search in Run IISM Higgs Search in Run II

Run II Higgs WGLEP limit

Page 36: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta36

LEP χ01 limit

ECM=2.0 TeV

L=20 fb-1

L=4 fb-1

L=2 fb-1

M(t

∼ 1)=

M(c

)+M

(χ∼ 10 )

M(t

∼ 1)=

M(b

)+M

(W)+

M(χ

∼ 10 )

t∼1 → c χ

∼10

Run 1

Scalar Top Quark Search in Run IIScalar Top Quark Search in Run II

D.Tsybychev’sthesis topic

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Detecting Massive Scalars Darin Acosta37

Scalar Scalar Leptoquark Leptoquark ProspectsProspects

Leptoquark Mass (GeV/c*c)50 100 150 200 250 300 350 400

β

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1First Generation Limits

D0 Scalar

CDF Scalar eejj

ννCDF Scalar Projected limit for 2 fb–1

A.Moorhead, 2002 REU project

Existing Run 1 limits

Same topology as for scalar top quark search

Cha

rged

lept

on b

ranc

hing

ratio

Page 38: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

The CERN LaboratoryThe CERN LaboratoryGeneva, Switzerland

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Detecting Massive Scalars Darin Acosta39

The LargeThe Large Hadron ColliderHadron Collider

CERN

R = 4.5 kmE = 7 TeVL=100 fb-1/year

Point 5 – CMS

2 proton rings housed in same tunnel as LEP

Completion: mid 2007

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Detecting Massive Scalars Darin Acosta40

The Compact Muon Solenoid The Compact Muon Solenoid ExptExpt..

PbWO4 Crystalsγ / e detection

Muon chambers

Silicon Tracker

4T magnet

Hadronic calorimeterJets, missing E (ν)

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Detecting Massive Scalars Darin Acosta41

“There’s no scale”“There’s no scale”

The inner vacuum tank of the magnet cryostat

Page 42: Detecting Massive Scalar Particles at Proton Colliders › ~acosta › scalar_colloq.pdfMotivation for scalar particles in particle theories ... scalar field, and this scalar field

Detecting Massive Scalars Darin Acosta42

Endcap Muon SystemEndcap Muon SystemIron disk of endcap muon systemOne of 540 chambers to be mounted

System will have 0.5 million electronic channels

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Detecting Massive Scalars Darin Acosta43

CMS DAQ ArchitectureCMS DAQ ArchitectureCMS has a multi-tiered trigger system:

L1 reduces rate from 40 MHz to 75 kHzCustom hardware processes calorimeter and muon data to select electrons, photons, jets, muons, ET above threshold

L2, L3,… (HLT) reduces rate from 75 kHz to 100 HzCommercial CPU farm runs online programs to select physics channels 40 TB/s

100 MB/s

Large telecomm switch (500 Gbit/s)

~1000 node PC cluster

40 MHz BX rate ⇒ 1 GHz of collisions

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Detecting Massive Scalars Darin Acosta44

Extrapolation UnitsXCV400BG560

Final Selection UnitXCV150BG352

Bunch Crossing Analyzer

XCV50BG256

Track Assemblers256k x 16 SRAM

UF Muon Trigger PrototypeUF Muon Trigger Prototype

3 GB/s input

100 billion operations per second

Successfully tested in 2000Programmable

logic performs massively parallel computation to reconstruct muons in real-time

Assignment UnitsXCV50BG256 &2M x 8 SRAM

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Detecting Massive Scalars Darin Acosta45

From CCB

To Muon Sorter

To/From Barrel

1 chip contains all logic of previous board!

3 other boards merged

To be tested this winter –

Design/test involves 3 engineers, 1 grad student, 1 undergrad

The Next GenerationThe Next Generation

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Detecting Massive Scalars Darin Acosta46

SM Higgs SM Higgs –– Intermediate MassIntermediate MassH→ZZ→l+l– l+l– (l =e,µ)

Very cleanResolution: ~ 1 GeV

Works for the mass range 130<MH<500 GeV/c2

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Detecting Massive Scalars Darin Acosta47

SM Higgs SM Higgs –– Low MassLow MassH → bb viattH → ttbb →lνb+bjj+bb

Use likelihood for top quark decays & event kinematics

S/B ≈ 0.8

H→γγ: decay is rare (B~10-3)good resolution essentialreason for PbWO4 crystalsat 100 GeV, σ≈1GeV

S/B ≈ 1:20

CMS 30fb-1

S=38 B=52

CMS100fb-1

K=1.6, S/B ~4%

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Detecting Massive Scalars Darin Acosta48

H → ZZ → 4l covers widest mass range

Good muon coverage

H → γγ important at low mass

Good calorimetry

Greater than 5σ discovery potential over full mass range from LEP limit to 1 TeV in 1 year at design luminosity

LEP limit

SM Higgs Prospects at CMSSM Higgs Prospects at CMS

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Detecting Massive Scalars Darin Acosta49

ConclusionConclusionScalar particles are the key to understanding the nature of the fundamental forces and space-time

HiggsStrong indirect evidence of its existence, though no direct measurement yet. Last particle to be discovered in SM

SupersymmetryCompelling theoretical framework, but no experimental evidence

LeptoquarksStranger things could happen…

CDF II is operating well, but data coming slowlyExpect 100–200 pb-1 delivered by end of year (≈ Run 1)Goal is to collect ~15000 pb-1 of data by 2007Good heavy-flavor tagging (b,c quarks) is essential

If not discovered at the Tevatron, the LHC will be capable of discovering the Higgs and ruling in/out Supersymmetry, starting in 2007