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02/21/2003 Physics at DZERO 1
Exploring the Microscopic Structure of the University with
DZero??
02/21/2003 Physics at DZERO 2
Exploring the Microscopic Structure of the Universe with
DZero
Jerry BlazeyNorthern Illinois University
02/21/2003 Physics at DZERO 3
The Standard Model
• Simple: “Bits of matter stick together by exchanging stuff.”
• The crowning achievement of particle physics is a model that describes all particles and particle interactions. The model includes:– 6 quarks (those little fellows in the nucleus) and
their antiparticles.– 6 leptons (of which the electron is an example) and
their antiparticles– 4 force carrier particles
• More Precise: “All known matter is composed of composites of quarks and leptons which interact by exchanging force carriers.”
02/21/2003 Physics at DZERO 4
The Quarks*• Three pairs of quarks.• The up and down are
the constituents of protons (= uud) and neutrons (= udd), and make up most matter.
• The other particles are produced in energetic subatomic collisions from cosmic rays or in accelerators, where they are also studied.*The name comes from James’s Joyce’s Finnegan’s Wake,
“Three quarks for Muster Mark!”
02/21/2003 Physics at DZERO 5
Leptons*• Leptons are generally lighter
particles and are most commonly observed in radioactive decays.
• The best example is neutron decay into a proton, an electron, and a neutrino:
*Greek for “small mass”
02/21/2003 Physics at DZERO 6
Periodic Table of Fundamental ParticlesAll point-like (down to
10-18 m) spin-1/2Fermions
Families reflectincreasing mass and
a theoreticalorganization
u, d, , e are “normal matter”
These all interact by exchanging spin 1
bosons…
-1
+2/3
-1/3
0
Mass
02/21/2003 Physics at DZERO 7
SM Interactions• Electroweak interaction
– Photons, W, and Z: all spin-1 bosons
• Strong interaction (QCD)– Gluons: all spin-1 bosons
• Three lepton generations (e,,,’s) – feel electroweak interaction only
• Three quark generations (u,d,s,c,t,b)– feel electroweak, strong interactions
02/21/2003 Physics at DZERO 8
We could stop here but…..
Explained by Standard Model10-37 weakerthan EM, not
explained
02/21/2003 Physics at DZERO 9
Two Compelling Unsolved Questions
(there are many others)
•How do particles get mass?
•How does gravity fit into all of this?
02/21/2003 Physics at DZERO 10
The Higgs Particle• The electroweak unification postulates the existence
of the Higgs field. (Named after a Scottish physicist who first hypothesized its existence.)
• This field interacts with all other particles to impart mass - think of walking through molasses.
• The Higgs field is a microscopic property of space-time, but at least one real particle will result.
• The experimental program at Fermilab, the Large Hadron Collider in Europe, and the next Linear Collider are dedicated, in part, to the search for this particle.
• It’s discovery would be an achievement of the highest order - an understanding of the origins of mass!
02/21/2003 Physics at DZERO 11
Beyond That?• Even with the Higgs, the Standard
Model requires fine tuning of parameters to avoid infinite Higgs masses from quantum corrections – the theory is “ugly.”
• Leads to strong belief that the SM is merely a low energy or effective theory valid up to some scale, where additional physics will appear.
• Most popular theoretical option:
Supersymmetry or SUSY.
02/21/2003 Physics at DZERO 12
SUSY• In SUSY every particle and force
carrier has a massive partner: Squarks, slectrons, gluinos…
• Since they are massive they’ve not been produced in current machines.
• The discovery requires more energetic accelerators – something which is being enthusiastically pursued.
02/21/2003 Physics at DZERO 13
Or…Extra Dimensions!?• Amazingly enough an 11 dimensional world
(time, 3-D & 7 very small less than 1mm in size) can accommodate a theory with all four forces.
• Only gravity can communicate with/to other dimensions, it’s “strength” is diluted in ours. That is, the graviton, or gravity carrier can spread it’s influence among all 10 spatial dimensions.
• Experiments are underway searching for signals of these dimensions.The “other”
dimensions
“Our World”
qgraviton
02/21/2003 Physics at DZERO 14
How do we test these theories?
02/21/2003 Physics at DZERO 15
The Two Basic Ideas: – Find a source of particles with
high kinetic energy.– Study the debris resulting from
collisions inside detectors.
The Sources:– Cosmic Rays– Accelerators – The higher the energy the more
numerous the number and types of particles.
The Detectors:– A series of special purpose devices that
track and identify collision products
p p
02/21/2003 Physics at DZERO 16
Fermilab Proton-Antiproton Collider
Main Injector & Recycler
Tevatron
Booster
p p
DØ
DØDØ
p source
Batavia, Illinois Chicago
1)Hydrogen Bottle2)Linear Accelerator3)Booster4)Main/Injector5)Tevatron
You are here
02/21/2003 Physics at DZERO 17
Physics Goals of a Detector
Precise study of the known quanta of the Standard ModelWeak bosons, top quark, QCD, b-quark
Search for particles and forces beyond those knownHiggs, supersymmetry, extra dimensions, other new phenomena
Driven by these goals, A detector emphasizes– Electron,
muon and tau identification
– Jets (q and g) and missing transverse energy
– Flavor tagging through displaced vertices and leptons
02/21/2003 Physics at DZERO 18
A Schematic detector
Hadronic
layers
Tracking system Magnetized volume
CalorimeterInduces shower
in dense material
Innermost tracking layers
use silicon
Muon detector
Interactionpoint
Absorber material
Bend angle momentum
Electron
Experimental signature of a quark or gluon
Muon
Jet: q or g
“Missing transverse energy”
Signature of a non-interacting (or weaklyinteracting) particle like a neutrino
EM layersfine sampling
p p
02/21/2003 Physics at DZERO 19
A Real Detector: D0muon system
electronics
• Proposed 1982
• First Data: 1992-1995
1.8 TeV• Upgrade:
1996-2001• Run II:
2002-2008 2.0 TeV
02/21/2003 Physics at DZERO 20
Any resemblance betweenDZero and the Borg Home ship is purely a coincidence.
02/21/2003 Physics at DZERO 21
Calorimeters Tracker
Muon System
Beamline Shielding
Electronics
protons antiprotons
20 m
02/21/2003 Physics at DZERO 22
International
• 18 countries• 77 institutions• 650+ physicists
02/21/2003 Physics at DZERO 23
Run I (1992-6) Results
• 140+ reviewed articles– Discovery of the top quark– Precision measurements of particle
masses and cross sections– Limits on new physics
• 100/year presentations• 100+ Ph.D./Master’s Students each
with an separate data stream, topic, and analysis
02/21/2003 Physics at DZERO 24
About the Detector: Silicon Microstrip Tracker
• 1M Channels• Four barrel layers• Axial and stereo
layers• Disks for
Forward/Backward Coverage
02/21/2003 Physics at DZERO 25
Scintillating Fiber Tracker
• 100k Channels in eight layers
• Scintillating Fiber
• Clear Fiber• Solid State
Visible Light Photon Counters at 9 Kelvin
02/21/2003 Physics at DZERO 26
Fiber Tracker Readout3-FRONT
4-FRONT
D3
-G4
B 1
5A 5B
E 3
R99.000
A2
-G5
A 2
G 5
C 3
E 4
C3
-E4
A 1
H 5
A1
-H5
B 2
F 4
123
ONE HALF CONNECTOR IN SECTOR 3 ONLY WITH FULL SHAREDCONNECTORS AT SECTORS 1 & 2, AND SECTORS 4 & 5.
4 5
B2
-F4
274
296
232
135
177
SECTORS 1 THRU 5 (5 SPLIT)CABLE ROUTES3/4 DIA. BUNDLES HELD AT R58 AND
CONTINUING ON TO THE TOP OF THE NOTCHES575eith3card.dwg
SCALE: 1/8(LOOKING AT SOUTH FACE OF CC)
B 3
H 6
B3
-H6
D4
-F5
D 4
F 5
B 5
B5
-H1
1
F 9
G 1 0
H 1 1
F9
-G1
0
D 7
E 8
D7
-E8
C 6
H 1 0
B1
-E3
C 2
F 3
H 4
D 2
C2
-H4
D2
-F3
D 3
G 4
C6
-H1
0
G 9
A 4
A4
-G9
E 7
G 3
H 3
G3
-H3
E2
-F2
E 2
F 2
F 8
E7
-F8
D 6
H 9
D6
-H9
C 5
G 8
C5
-G8
E 6
F 7
E6
-F7
B 4
H 8
B4
-H8
G 7
D 5
D5
-G7
A 3
F 6
A3
-F6
C 4
H 7
C4
-H7
E 5
G 6
E5
-G6
C1
-D1
C 1
D 1
E 1
F 1
G 1
H 1
H 2
G 2
E1
-G1
F1
-H2
G1
-H1
C.P.S
.
C.P.S
.
H 1 2
H 1 3
H 1 4
H 1 5
H 1 6
H 1 7
G 1 1
G 1 2
G 1 3
G 1 4
G 1 5
F 1 0
F 1 1
F 1 2
F 1 3
F 1 4
E 9
E 1 0
E 1 1
E 1 2
D 8
D 9
D 1 0
D 1 1
C 7
C 8
C 9
B 6
B 7
B 8
A 5
A 6
H 1 8
H 1 9
H 2 0
H 2 1
H 2 2
G 1 6
G 1 7
G 1 8
G 1 9
G 2 0
G 2 1G 2 2
F 1 5
F 1 6
F 1 7
F 1 8
F 1 9
F 2 0
E 1 3
E 1 4
E 1 5
E 1 6
E 1 7 E 1 8
D 1 2
D 1 3
D 1 4
D 1 5
D 1 6
C 1 0
C 1 1
C 1 2
C 1 3
C 1 3
B 9
B 1 0
B 1 1B 1 2
A 7
A 8
A 9
A 1 0
B 1 3
C 1 4
C 1 5
D 1 7
D 1 8
E 1 9
E 2 0
F 2 1
F 2 2
F 2 3
G 2 3
G 2 4
G 2 5
H 2 3
H 2 4 H 2 5
H 2 6
H 2 7
H 2 8
B6
-C8
-F1
0-H
12
E9
-G1
1
Readout under detector
Photoelectron peaks 1 pe ~ 7 fC
02/21/2003 Physics at DZERO 27
Liquid Argon Calorimeter
Z
y
x
p
p
69.0GeV, 472
69.0GeV, 47522
11
T
T
E
E
Highest ET jet event in Run 1
• 50k Channels• Liquid argon
sampling with Ur absorber
02/21/2003 Physics at DZERO 28
Muon System
Connect tracks
J/ +-
scintillator
Match to CFT
tracks = 83 MeV
Resolutions ~ 20% better in MC than data
shielding
02/21/2003 Physics at DZERO 29
Run II: 24/7 Event Collection• Proton-antiprotons collide at 7MHz
or seven million times per second• Tiered electronics pick
successively more interesting events– Level 1 10 kHz– Level 2 1 kHz
• About 100 crates of electronics readout the detectors and send data to a Level 3 farm of 100 CPUs that reconstruct the data
• Per second: 50 events or 300 Mbytes of data to tape.
• Per year: 10 million events or 30 Terabytes of data.
02/21/2003 Physics at DZERO 30
Physics: Event Analysis• Events are “reconstructed”
offline by farms of ~100 CPUs.
• Each detector samples position, energy, or momentum, 1M+ channels
• Then computers build or reconstruct full event characteristics based upon these samples
• Interesting events or signals are culled from the background usually 100’s out of millions.
02/21/2003 Physics at DZERO 31
Sample Run II Event: Ze+e- p
pZ
qq’
l
l
02/21/2003 Physics at DZERO 32
Sample Distributions: Ze+e-
1) Collect events2) Calculate mass for each event3) Plot distributions4) Statistically measure mass or production rate as a function of brightness or luminosity (1pb-1 means 1 event of cross section 1 pb will be produced.)5) Test predictions of Standard Model
02/21/2003 Physics at DZERO 33
Prospects for W mass and width
Current knowledge of mW:• DØ: 80.483 ± .084 GeV• World: 80.451 ± .033 MeV
Run II prospects for mW
• 2 fb-1 ±27 MeV• 15 fb-1 ±15 MeV
To improve measurements will require ~ fb-1 datasets or several years of Tevatron running.
p
pW
qq’
e
02/21/2003 Physics at DZERO 34
Top Mass Measurement
Discovered at Tevatron in 1995
Expected top mass accuracy by the end of Run II : ~ 1.4 GeV
02/21/2003 Physics at DZERO 35
W and Top Measurements
Indirectly constrain mass of The Higgs
Top quark mass (GeV)
W m
ass
(GeV
)
2001
mt 2 GeVmW 15 MeV
Stand
ard
Mod
elSuper
sym
met
ry
02/21/2003 Physics at DZERO 36
114 GeV 193 GeV
Past Searches for the Higgs
Over the last decade, experiments at the CERN e+e–
collider ( European Laboratory for Particle Physics) have been searching for the Higgs– direct searches for Higgs
production exclude mH < 114 GeV.
– precision measurements of parameters of the W and Z bosons, combined with Fermilab’s Run I top quark mass measurements, set an upper limit of mH ~ 193 GeV.
02/21/2003 Physics at DZERO 37
Higgs Hunting at the Tevatron• For any given Higgs mass,
the production cross section, decays are calculable within the Standard Model Inclusive Higgs cross section ~ 1pb
• A good search bet below ~ 140 GeV is associated production with W or Z– e or decays of W/Z
help give the needed background rejection
– cross section ~ 0.2 pb
p
pW*
qq’
H
W
02/21/2003 Physics at DZERO 38
“The Tevatron’s a Good Bet!”“We find it or eliminate it”
15 fb-1
110-190 GeV
Combined Channel/Experiments Higgs Mass Reach
02/21/2003 Physics at DZERO 39
Well actually… there’s at least
one Higgs!
02/21/2003 Physics at DZERO 40
Supersymmetry
• Postulates a symmetry between bosons and fermions such that all the presently observed particles have new, more massive super-partners (SUSY is a broken symmetry)
• Theoretically attractive:– additional particles cancel divergences in mH
– SUSY closely approximates the standard model at low energies
– allows unification of forces at much higher energies– provides a path to the incorporation of gravity and
string theory: Local Supersymmetry = Supergravity– lightest stable particle cosmic dark matter
candidate• masses depend on unknown parameters, but expected
to be 100 GeV - 1 TeV
02/21/2003 Physics at DZERO 41
Supersymmetry signatures• Squarks and gluinos are the most copiously produced
SUSY particles• As long as the associated new quantum number “R-
parity” is conserved, cannot decay to normal particles • Missing transverse energy from escaping (lightest
supersymmetric particle or LSP)
Possible decay chains always end inthe LSP:
Which leaves missingTransverse Energy in the DetectorSearch region typically > 75 GeV
02/21/2003 Physics at DZERO 42
Past Searches at the Tevatron• In Run I DØ carried out extensive
searches for SUSY
– Squarks/gluinos Missing ET + jets (+ lepton(s))
– Charginos/neutralinos multileptons
– GMSB Missing ET +photon(s)
• Searches for other new phenomena – leptoquarks, dijet resonances,
W’,Z’, massive stable particles, extra dimensions . . .
Now sign of new physics:DØ analysed 32 final states containing electrons, muons, photons, jets, W’s, Z’s and missing ET Find an 89% CL for agreement with the Standard Model (PRD 64 012004)
Run II prospect:gluino mass ~ 400 GeV
Run I excluded
02/21/2003 Physics at DZERO 43
Searches for Extra Dimensions
Standard Model
ExtraDimensions
DATA
Instrumental background (from data)
Extra Dimensions
Run II limits frompp ee,, MS(GRW) > 0.92 TeV (ee/)
MS(GRW) > 0.50 TeV () (first limit from a hadron collider in this channel)less than 1 mm depending on the number of extra dimensions.
p
G
p
02/21/2003 Physics at DZERO 44
New York Times
02/21/2003 Physics at DZERO 45
Closing Comments: Prospects• Over the next several years DZero and the
Tevatron will explore the microscopic universe:– Constrain the SM and place limits on the
Higgs mass or – Discover the Higgs, and perhaps– Discover new physics, extra dimensions….
• It is an exciting, challenging program that asks two of the most fundamental questions: – What is the structure of the universe? – What is the history of the universe?“To the
Microscopic Universe….and beyond!”
02/21/2003 Physics at DZERO 46
Now (15 billion yrs)
Stars form (1 billion yrs)
Atoms form (300,000 yrs)
Nuclei form (180 seconds)
Protons and neutrons (10-10 s)
Quarks differentiate (10-34 s)
Fermilab4×10-12 seconds