+ All Categories
Home > Documents > 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

Date post: 24-Jan-2016
Category:
View: 220 times
Download: 0 times
Share this document with a friend
Popular Tags:
46
02/21/2003 Physics at DZERO 1 Exploring the Microscopic Structure of the University with DZero??
Transcript
Page 1: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

02/21/2003 Physics at DZERO 1

Exploring the Microscopic Structure of the University with

DZero??

Page 2: 02/21/2003Physics at DZERO1 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

Page 3: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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.”

Page 4: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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!”

Page 5: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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”

Page 6: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 7: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 8: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

02/21/2003 Physics at DZERO 8

We could stop here but…..

Explained by Standard Model10-37 weakerthan EM, not

explained

Page 9: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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?

Page 10: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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!

Page 11: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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.

Page 12: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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.

Page 13: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 14: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

02/21/2003 Physics at DZERO 14

How do we test these theories?

Page 15: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 16: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

02/21/2003 Physics at DZERO 16

Fermilab Proton-Antiproton Collider

Main Injector & Recycler

Tevatron

Booster

p p

DØDØ

p source

Batavia, Illinois Chicago

1)Hydrogen Bottle2)Linear Accelerator3)Booster4)Main/Injector5)Tevatron

You are here

Page 17: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 18: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 19: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 20: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

02/21/2003 Physics at DZERO 20

Any resemblance betweenDZero and the Borg Home ship is purely a coincidence.

Page 21: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

02/21/2003 Physics at DZERO 21

Calorimeters Tracker

Muon System

Beamline Shielding

Electronics

protons antiprotons

20 m

Page 22: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

02/21/2003 Physics at DZERO 22

International

• 18 countries• 77 institutions• 650+ physicists

Page 23: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 24: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 25: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 26: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 27: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 28: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 29: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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.

Page 30: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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.

Page 31: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

02/21/2003 Physics at DZERO 31

Sample Run II Event: Ze+e- p

pZ

qq’

l

l

Page 32: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 33: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 34: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 35: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 36: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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.

Page 37: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 38: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 39: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

02/21/2003 Physics at DZERO 39

Well actually… there’s at least

one Higgs!

Page 40: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 41: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 42: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

Page 43: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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

qq

p

Page 44: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

02/21/2003 Physics at DZERO 44

New York Times

Page 45: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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!”

Page 46: 02/21/2003Physics at DZERO1 Exploring the Microscopic Structure of the University with DZero??

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


Recommended