Detecting Massive Scalar Particles at Proton Colliders University of Florida

advertisement
Detecting Massive Scalar Particles
at Proton Colliders
Darin Acosta
University of Florida
Outline
Motivation for scalar particles in particle theories
‡ The Higgs particle
‡ Supersymmetry
Î Hints of scalar particles
Î The Tevatron collider and the CDF experiment
‡ Review of Run 1 searches for Higgs and SUSY
‡ Status of Run 2 and search prospects
Î The Large Hadron Collider and the CMS experiment
‡ Construction progress and search prospects
Î
Detecting Massive Scalars
2
Darin Acosta
Why Not Scalars?
So far, all known matter is composed of spin-½ fermions
Î
electrons, protons, neutrons, …
Thus, atomic and nuclear structure obeys the Pauli-Exclusion
principle
Scalar objects do exist, but actually they are composites
Î
e.g. 4He, π+
In fact, all nuclear particles are composed of spin-½ quarks
Î
Î
Î
p = u u d
n = u d d
π+ = u d
Additionally, three of the fundamental forces are propagated by
spin-1 bosons
unified into one
Î Electromagnetism: Photons (γ)
electro-weak theory
Î Weak nuclear force: W+, W-, Z bosons
Î
Strong nuclear force: gluons (g)
Quantum gravity would be propagated by a spin-2 boson
Detecting Massive Scalars
3
Darin Acosta
Elementary Particles
mu,d ~ 5 MeV
mγ = 0
mt = 174 GeV
mg = 0
mν ≠ 0 ?
mZ = 91.188 GeV
me = 0.511 MeV
mW = 80.4 GeV
1 eV = 1.6 × 10–19 J
Detecting Massive Scalars
4
Darin Acosta
The Higgs Mechanism
The electro-weak theory is described by the
SU(2)×U(1) Weinberg-Salam Model
The quantum field theory of the strong force is
described by Quantum Chromodynamics
Collectively, 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 bosons
Î Generates mass for the fermions
Î Generates a massive neutral scalar
Î
Detecting Massive Scalars
5
Darin Acosta
Self consistency of
the Standard Model
places upper and lower
bounds on the Higgs
mass
1018
Î
1015
Excluded
Mass scale for new physics (GeV)
Theoretical Higgs Mass Constraints
1012
Wide mass range up
to ~1 TeV allowed if
new physics comes in
at scale of 1 TeV
Î
Excluded
109
Narrow mass range
if new physics doesn’t
enter until Grand
Unification scale
Î
106
103
0
200
400
800
600
MH (GeV)
Detecting Massive Scalars
6
Darin Acosta
Indirect Experimental Constraints
Direct mW, mt
measurements
Indirect from
electro-weak
parameters
SM predictions
PDG, 2002
Detecting Massive Scalars
7
Darin Acosta
Direct Higgs Search at e+e- Colliders
The Large Electron Positron (LEP) collider at CERN
ran from 1989 until 2000
In depth studies of the Z-boson resonance at 91 GeV
Î Steadily increased energy to 209 GeV to study W
production and to search for the Higgs
Î Shut down to allow construction of the Large Hadron
Collider
Î
Possible hint of the Higgs ?
Nobs = 4
Nexp = 1.25
⇒ P = 3%
Lower bound on Higgs mass
assuming no signal is 114 GeV
at the 95% CL
Detecting Massive Scalars
8
Darin Acosta
Supersymmetry: another source of scalars
Why is all matter spin-½ ?
Antimatter is the charge conjugation of normal matter
Î
Î
C |e-⟩ = |e+⟩
Predicted by P.A.M. Dirac in 1928, observed in 1932
Is there a spin conjugation as well?
Î
Q |fermion⟩ = |boson⟩
Such “Supersymmetry” generalizes space-time
symmetry
Predicts 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) !
Î
Points the way to a larger theory
When Supersymmetry is required to be a local symmetry, it
can incorporate gravity (Supergravity)
Î Supersymmetry is a prerequisite for string theories
Î Allows for Grand Unification
Î
Detecting Massive Scalars
9
Darin Acosta
Grand Unification
Coupling “constants” vary with the energy scale
Î Minimal Supersymmetric models allow for the unification of
3 forces at one energy scale (would miss otherwise)
Î
1 / coupling
EM
137
128
Gravity
Weak
Strong
102 GeV
Detecting Massive Scalars
1016 GeV
10
Darin Acosta
MPlanck =
1019 GeV
Supersymmetry is Broken
If Supersymmetry exists, there should be scalar
partners to the fermions
Î
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
Detecting Massive Scalars
11
Darin Acosta
Leptoquarks: also a source of scalars
There 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
Î
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
Î
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
Detecting Massive Scalars
12
e
LQ
q
Darin Acosta
Cosmological Implications of Scalars
In the Minimal Supersymmetric Standard Model
the lightest supersymmetric particle is stable
Generally a neutral, weakly interacting particle (neutralino)
Î Good candidate for Cold Dark Matter
Î
Scalar particles can obtain a non-zero vacuum
expectation value (vacuum energy)
Î
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)
Î ΩΛ ≈ 0.7, Ωm ≈ 0.3
Î
Ωm = Ωb + ΩCDM ; Ωb ≈ 0.04
Î
Detecting Massive Scalars
13
Darin Acosta
The Fermi National Accelerator
Laboratory
Batavia, Illinois
The Tevatron
CDF
Proton-Antiproton collider
Ebeam = 1 TeV
R = 1 km
D∅
In operation since 1985
Major upgrade completed
in 1999
Main injector
Detecting Massive Scalars
15
Darin Acosta
The Collider Detector at Fermilab
Run 1: 1992 – 1996
L=120 pb-1
Beam
direction
A very large, general purpose
“microscope” to study the structure
of matter
Hundreds of researchers participate
Detecting Massive Scalars
16
Darin Acosta
Discovery of the Top Quark in 1995
b
e
Relatively
long-lived
b
t t → b b W+ W- → b b q q’ e ν
Detecting Massive Scalars
17
Mtop = 174 ± 5 GeV
Darin Acosta
CDF Heavy Flavor Tagging
Bottom 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 mm
ÎThis is still within the beam pipe,
not in the detectors, so we must
extrapolate a precisely measured
track
Î
An important signature of the
decay of heavier particles…
Detecting Massive Scalars
18
primary
vertex
jet
Darin Acosta
L
Branching Ratios for Higgs Decay
Î
BR (H →bb) ~ 1
Î
BR (H →WW →2µ)
~ 0.01
Î
BR (H →ZZ →4µ)
~ 3x10-4
Î
BR (H →γγ) ~ 10-3
Tagging b quarks is important to discover a light Higgs
Detecting Massive Scalars
19
Darin Acosta
Higgs Production
p
p
Note:
σ = scattering cross section
1 pb = 10–36 cm2
L·σ = N (number of events)
L = 120 pb–1 for Run 1
Detecting Massive Scalars
20
Darin Acosta
Relative Yields at the Tevatron
1 fb = 10–3 pb
Background
Higgs
1 pb
Signal
(one in a billion
collisions!)
Detecting Massive Scalars
21
Darin Acosta
SM Higgs Search in Run 1
WH, ZH
production
Observed events agree well with
background expectations
Require 10–100X more data to be
sensitive to SM Higgs production
No anomalous production
Detecting Massive Scalars
22
Darin Acosta
Signatures of Supersymmetry
Larger cross sections for the production of scalar
quarks and gluons rather than leptons at a proton
collider because of the strong force couplings
Examples:
pp → q~q~, q~g~, g~g~
~~ ~~
pp → GGg, GGq
~~
pp → ~
t1~
t1, b1b1
~
q~, g~, G ⇒ E/ T + jets
~~
t ,b ⇒ E/ T + HF jets
Signatures:
Î
Î
Jets (from the hadronization of quarks and gluons)
Missing energy (from undetected lightest SUSY particle)
Backgrounds:
Î
Î
Î
QCD jets
W/Z production
top quarks
Orders of magnitude larger
Review just one search of many here
Detecting Massive Scalars
23
Darin Acosta
Scalar Top Quark Search
The 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
Î
Thus, the “stop” could be the lightest scalar quark
Search for the pair production
of stop quarks
Look for the decays:
~
±
Î t → bχ 1
Î
g
t
g
t
24
t
g
t
g
t
q
t
g
t
q
t
~
~ 0 (if first closed)
t →cχ
1
Detecting Massive Scalars
g
Darin Acosta
Scalar Top Quark Search (Jets + MET)
~
M ( χ~1± ) > M (ν~ ) > M ( t )
ƒ Use Missing transverse
energy data sample
2 or 3 jets, ET ≥ 15 GeV and | η |≤ 2
No jets with 7 ≤ ET ≤ 15 GeV and | η |≥ 3.6
• Cuts on jet-MET, jet-jet angles
• No l with PT > 10 GeV
~
t
χ~1±*
W*
χ~10
Main Backgrounds:
• MET > 40 GeV
W → τν + 1( 2,3,...) jet
Z → νν~ +2(3,4,...) jet
Require ≥ 1 charm quark tag
Expect 14.5 ± 4.2 events
QCD
Observe 11
Published: PRL, 84,5704(2000)
Detecting Massive Scalars
c
b*
25
Darin Acosta
90
M(t∼1) = M(b) + M(ν∼ )
→ b l ν)=100%
55
∼
M(
1
χ 0)
∼
CDF - 88 pb
95% CL
40
-1
1
60
50
(χ∼0
)
(hep-ph/9611232)
OPAL
√s=189 GeV
+M
65 θstop=0
60
W)
[σNLO: µ=m(t∼1),CTEQ3M]
c)+
√s=189 GeV
M(
CDF Excluded
Region_ ≡
_
∼∼
σ95%CL(t1t1) <σNLO(t∼1∼t1)
70 ALEPH
70
∼
75
80
± ∼
∼
t1 )=
BR(t∼1
2
80
∼
BR (t1 → c + χ01) = 100%
θ∼t = 0.0
M(
85
M(χ01) (GeV/c )
50
∼
CDF - 88 pb
95% CL Excluded
80
90
100
Detecting Massive Scalars
110
D0/
7.4 pb-1
10
LEP1 excluded
40
t1 )=
20
-1
45
M(
b)+
M(
30
120
0
130
M(t∼1) (GeV)
26
M(
M(ν∼ ) (GeV)
Scalar Top Quark Limits
0
20
40
60∼
80
100
2
M(t1) (GeV/c )
Darin Acosta
120
140
CDF II Detector
Goal:
Run 2a: 2001 – 2004
(2000 – 4000 pb-1)
Run 2b: 2004 – 2007+
(15000 pb-1)
Completely new electronics
New plug calorimeter
New muon chambers
New central tracker
New silicon vertex detector
Detecting Massive Scalars
27
Darin Acosta
Silicon Vertex Detector
Radius: inner = 1.35 cm, outer = 29 cm
Length: 90 cm
strip pitch: 60µm
Double-sided layers for r–φ,
New
stereo r–φ, r–z
$20M
Detecting Massive Scalars
28
Darin Acosta
CDF-II Rolling into the Collision Hall
March 2001
Detecting Massive Scalars
29
Darin Acosta
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
Detecting Massive Scalars
30
Darin Acosta
W Boson Measurement from Electrons
W cross section measurement
from W Æ e ν
σ(W)*BR(WÆeν) (nb) =
2.60±0.07stat±0.11syst ±0.26lum
Î
Consistent with Run 1 results
rescaled for higher collision
energy:
2.72±0.02stat±0.08syst ±0.09lum
Î
Detecting Massive Scalars
31
Darin Acosta
Observation of Z Bosons
Clear evidence of ZÆ µ+µ–
Signal shown for opposite
sign muons detected in both
inner and outer muon
chambers
Î
µ1
µ2
-57 candidate events in
66<Minv<116 range
Detecting Massive Scalars
32
Darin Acosta
Tagged Muon in CDF
Muon
Contained in
a jet with ET
= 9 GeV
Note: B mesons decay into soft leptons about 10% of the time
Detecting Massive Scalars
33
Darin Acosta
Secondary Vertices in CDF II
Zoom-in of previous event:
Event : 63457 Run : 138046 EventType : DATA | Unpresc: 33,7,13,21,53,23,55,27 Presc: 33,27 Myron mode: 0
PV
muon
SV
Jets containing soft
muons exhibit low
probability of coming
from the primary vertex
Event was tagged by the “Jet Probability” algorithm we are
developing at UF for tagging bottom and charm jets
Detecting Massive Scalars
34
Darin Acosta
SM Higgs Search in Run II
LEP limit
Run II Higgs WG
Detecting Massive Scalars
35
Darin Acosta
Scalar Top Quark Search in Run II
(χ∼0
1)
)+M
1
∼
(W
M(
+M
L=20 fb-1
(b)
M( ∼
t1 )=
M
M( ∼
t1 )=
M
(c)+
ECM=2.0 TeV
∼
→ c χ01
χ 0)
∼
t1
L=4 fb-1
L=2 fb-1
Run 1
LEP χ01 limit
D.Tsybychev’s
thesis topic
Detecting Massive Scalars
36
Darin Acosta
Scalar Leptoquark Prospects
A.Moorhead,
2002 REU project
β
Charged lepton branching ratio
First Generation Limits
1
0.9
0.8
0.7
D0 Scalar
0.6
CDF Scalar eejj
0.5
CDF Scalar νν
0.4
Existing Run 1
limits
Projected limit
for 2 fb–1
0.3
0.2
Same topology
as for scalar top
quark search
0.1
0
50
100
Detecting Massive Scalars
150
200 250 300 350 400
Leptoquark Mass (GeV/c*c)
37
Darin Acosta
The CERN Laboratory
Geneva, Switzerland
The Large Hadron Collider
CERN
R = 4.5 km
E = 7 TeV
L=100 fb-1/year
Point 5 – CMS
2 proton rings housed
in same tunnel as LEP
Completion: mid 2007
Detecting Massive Scalars
39
Darin Acosta
The Compact Muon Solenoid Expt.
4T magnet
Muon chambers
Silicon Tracker
PbWO4 Crystals
Hadronic calorimeter
γ / e detection
Jets, missing E (ν)
Detecting Massive Scalars
40
Darin Acosta
“There’s no scale”
The inner vacuum tank of the magnet cryostat
Detecting Massive Scalars
41
Darin Acosta
Endcap Muon System
Iron disk of endcap muon system
One of 540 chambers to be
mounted
System will have 0.5 million electronic channels
Detecting Massive Scalars
42
Darin Acosta
CMS DAQ Architecture
CMS has a multi-tiered trigger system:
40 MHz BX rate
⇒ 1 GHz of
collisions
Î L1 reduces rate from 40 MHz to 75 kHz
‡ Custom hardware processes calorimeter and muon data to
select electrons, photons, jets, muons, ET above threshold
Î
L2, L3,… (HLT) reduces rate from 75 kHz to 100 Hz
‡ Commercial CPU farm runs online programs to select
physics channels
40 TB/s
Large telecomm
switch (500 Gbit/s)
~1000 node PC
cluster
100 MB/s
Detecting Massive Scalars
43
Darin Acosta
UF Muon Trigger Prototype
Final Selection Unit
Extrapolation Units
XCV150BG352
XCV400BG560
Programmable
logic performs
massively
parallel
computation to
reconstruct
muons in
real-time
3 GB/s
input
100 billion
operations
per second
Assignment Units Track Assemblers Bunch Crossing
256k x 16 SRAM
XCV50BG256 &
Analyzer
2M x 8 SRAM
Detecting Massive Scalars
Successfully
tested in 2000
XCV50BG256
44
Darin Acosta
The Next Generation
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
From
CCB
To Muon
Sorter
To/From
Barrel
Detecting Massive Scalars
45
Darin Acosta
SM Higgs – Intermediate Mass
H→ZZ→l+l– l+l– (l =e,µ)
ÎVery
clean
‡ Resolution: ~ 1 GeV
ÎWorks for the mass range
130<MH<500 GeV/c2
Detecting Massive Scalars
46
Darin Acosta
SM Higgs – Low Mass
H → bb via
ttH → ttbb →lνb+bjj+bb
Î
CMS 30fb-1
S=38 B=52
Use likelihood for top quark
decays & event kinematics
‡ S/B ≈ 0.8
H→γγ: decay is rare (B~10-3)
Îgood
resolution essential
Îreason for PbWO4 crystals
Îat 100 GeV, σ≈1GeV
‡ S/B ≈ 1:20
Detecting Massive Scalars
CMS
100fb-1
K=1.6, S/B ~4%
47
Darin Acosta
SM Higgs Prospects at CMS
H → ZZ → 4l covers widest
mass range
Î
Good muon coverage
H → γγ important at low
mass
Î
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
Detecting Massive Scalars
48
Darin Acosta
Conclusion
Scalar particles are the key to understanding the
nature of the fundamental forces and space-time
Higgs
‡ Strong indirect evidence of its existence, though no direct
measurement yet. Last particle to be discovered in SM
Î Supersymmetry
‡ Compelling theoretical framework, but no experimental
evidence
Î Leptoquarks
‡ Stranger things could happen…
Î
CDF II is operating well, but data coming slowly
Î
Î
Î
Expect 100–200 pb-1 delivered by end of year (≈ Run 1)
Goal is to collect ~15000 pb-1 of data by 2007
Good 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
Detecting Massive Scalars
49
Darin Acosta
Download