particle detectors günther dissertori cern-ep cern teachers seminar july 2001

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PARTICLE DETECTORSPARTICLE DETECTORS

Günther DissertoriCERN-EP

CERN Teachers Seminar

July 2001

OutlookOutlook

IntroductionWhat to measure, why?Basic Principles

Tracking Calorimetry Particle Identification

Large detector systemsConclusions

IntroductionIntroductionHE physics experiments study interaction of

particles by scattering of particles on other particles

Results of these interactions are change in flight direction/energy/momentum of

original particles

production of new particles

Introduction...Introduction...These interactions are produced in

1 2

p2 = 0

GoalGoal : measure as many as possible of the resulting particles from the interaction put detector “around” the interaction point

p1 = -p21 2

Detector elements

What to measure, why?What to measure, why?

If we have an “ideal” detector, we can reconstruct the interaction, ie. obtain all possible information on it. This is then compared to theoretical predictions and ultimately leads to a better understanding of the interaction/properties of particles

If we have an “ideal” detector, we can reconstruct the interaction, ie. obtain all possible information on it. This is then compared to theoretical predictions and ultimately leads to a better understanding of the interaction/properties of particles

“Ideal detector” measures all produced particles their energy, momentum type (mass, charge, life time, Spin, decays)

“Ideal detector” measures all produced particles their energy, momentum type (mass, charge, life time, Spin, decays)

Measured quantitiesMeasured quantities

The creation/passage of a particle ( --> type)Electronic equipment

eg. Geiger counter

Its four-momentum Energymomentum in x-dirmomentum in y-dirmomentum in z-dir

E

p=

Its velocity = v/c

px

p = py

pz

Derived propertiesDerived properties

Mass in principle, if E and p measured: E2 = m2 c4 + p2c2

if v and p measured: p = m v / (1 - 2)

from E and p of decay products: m2 c4 = (E1+E2)2 - (cp1+ cp2)2

m

E1,p1

E2,p2

Further properties...Further properties...

The charge (at least the sign…) from curvature in a magnetic field

The lifetime from flight path before decay

Magnetic field, pointingout of the plane

Negative charge

positive charge

length

So, how measure the four-momentum?So, how measure the four-momentum?

Energy : from “calorimetercalorimeter” (see later)

Momentum : from “magnetic spectrometer+tracking detectormagnetic spectrometer+tracking detector”

Magnetic field, pointingout of the plane

Negative charge

positive chargeR1R2

p2

p1

p1<p2 R1 < R2 p1<p2 R1 < R2

q v B = m v2/R

q B R = m v = p

Lorentz-force

velocity : time of flight time of flight oror Cherenkov radiation Cherenkov radiation (see later)(see later)

Lv t = L

Principles of a measurementPrinciples of a measurementMeasurement occurs via the interaction (again…)

of a particle with the detector(material) creation of a measureable signal

IonisationIonisation

Excitation/ScintillationExcitation/Scintillation

Change of the particle trajectoryChange of the particle trajectory• curving in a magnetic field, energy loss• scattering, change of direction, absorption

p

e-

p

e-

pp

Detected ParticlesDetected Particles

Charged particles e-, e+, p (protons), , K (mesons), (muons)

Neutral particles (photons), n (neutrons), K0 (mesons), neutrinos, very difficult)

Different particle types interact differently with matter (detector) (eg. photons do not feel a magnetic field)

need different types of detectors to measure different types of particles

Typical detector conceptTypical detector concept

Combine different detector types/technologies into one large detector system

Interaction point

Precision vertex detector

trackingdetector

Magneticspectrometer

Electro

mag

netic calo

rime

ter

Had

ron

ic calo

rimeter

Mu

on

detecto

rs

Trac

king

sys

tem

Ele

ctro

mag

netic

calo

rim

eter

Had

roni

c ca

lori

met

er

Muo

n de

tect

or

syst

em

Electron e-

Photon

Hadron, eg.

proton p

Muon -

Meson K0

Tracking DetectorsTracking Detectors

Basic goalBasic goal: make the passage of particles through

matter visible --> measure the tracks

ReconstructReconstruct from the measured space points the flight path

Extract information on the momentummomentum (see previous transparencies)

NOTE: the particle should not be too much affected by the detector: No dense materials No dense materials !

This is achieved byThis is achieved by

Detectors where Ionisation signals are recorded

Geiger-Müller counterMWPC (Multi-Wire Proportional Chambers)TPC (Time Projection Chamber)silicon detectors

Bubble chambers (see separate lecture)

Scintillation light is producedeg. scintillating fibers

Principle of gaseous countersPrinciple of gaseous counters

+ HV

signal

cathode

Anode Wire

Gas-filled tubeGas-filled tube

---

--

+++

++ t = 0

- ---

-

+ +++

+

t = t1

Track ionises gas atoms electrons drift towards anode, ions towards cathode around anode electrons are accelerated (increasing field strength) further ionisation --> signal enhancement --> signal induced on wire

Principle of gaseous counters...Principle of gaseous counters...

gas filling

Now : TrackingNow : Tracking

Basic idea : put many counters close to each other

Realization:Realization:wire chamberwire chamber

(MWPC)(MWPC)Nobel prize: G.Charpak, 1992Nobel prize: G.Charpak, 1992

Anode wiresAnode wires

Cathode: pads or wiresCathode: pads or wires

x

y

Tracking: MWPCTracking: MWPC

ITC (ALEPH)Inner Tracking Chamber

Further development:Further development:Time Projection Chambers (TPC)Time Projection Chambers (TPC)

Gas-filled cylinderGas-filled cylinder

Anode Wires

MWPC

gives r,

MWPC

gives r,

E

B

- -- - - - -- -

--

--

++

+

+

++

z = vdrift tz = vdrift t

TPCTPC

LimitationsLimitations Precision limited by wire distance

Error on space point d cannot be reduced arbitrarily!

Uncertainties on space points Uncertainties on track origin andmomentum

Step forward:Step forward:Silicon Microstrip DetectorsSilicon Microstrip Detectors

Now precision limited by strip distance 10 - 100 m

Now precision limited by strip distance 10 - 100 m

Creation of electron-hole pairs by ionising particle

Creation of electron-hole pairs by ionising particle

Same principle as gas counters

Silicon wafers, doped

0.2 - 0.3 mm

Silicon microstrip detectors...Silicon microstrip detectors...

Silicon Microstrip detectors...Silicon Microstrip detectors...

ALEPH VDET

OPAL VDET

Future ATLAS tracking detector

Increase in precisionIncrease in precision

0 1cmx

=Beam crossing point

Mean Lifetime of tau =290 x 10-15 sec !! --> c = 87 m !?

Scintillating fibersScintillating fibers Certain materials emit scintillation light after particle

passage (plastic scintillators, aromatic polymers, silicate glass hosts….)

Photomultiplier: converts light into electronic signal

Scintillatingmaterial

Scintillatingmaterial

PM

Total reflection

Put many fibers close to each other--> make track visible

Scintillating fibers...Scintillating fibers...

CalorimetryCalorimetry

Basic principle: In the interaction of a particle with dense

material all/most of its energy is converted into secondary particles and/or heatsecondary particles and/or heat.

These secondary particles are recordedeg. Number, energy, density of secondariesthis is proportional toproportional to the initial energy

NOTE: last year calorimetry was discussed in detail in talks prepared by teachers

NOTE: last year calorimetry was discussed in detail in talks prepared by teachers

Electromagnetic showersElectromagnetic showers

Interactions of electrons and photons with matter:

Matterblock, eg.

lead

Lead atom

Shower partially or completely absorbed

How to measure the secondaries?How to measure the secondaries?

1. With sampling calorimeterssampling calorimeters:

Dense blocks, such as leadDetectors, such as wire chambers,

or scintillators

Sandwich structure !

Total amount of signalsregistered is proportionalto incident energy.

But has to be calibrated with beams of known energy!

Sandwich structure !

Total amount of signalsregistered is proportionalto incident energy.

But has to be calibrated with beams of known energy!

Sampling CalorimetersSampling Calorimeters

e+

e-

ALEPH ECAL

pions electron

muonsphotons

How to measure the secondaries?How to measure the secondaries?

2. With homogenous calorimetershomogenous calorimeters, such as, such as crystal crystal calorimeterscalorimeters:

signal

photons

Note : these crystals are also used in other fields (eg. Medical imaging, PET)Note : these crystals are also used in other fields (eg. Medical imaging, PET)

Photo diode

Crystal (BGO, PbWO4,…)

CMSCMS

L3L3

Hadronic calorimetersHadronic calorimeters Hadronic particles (protons, neutrons, pions) can traverse

the electromagnetic calorimeters. They can also interact via nuclear reactions !

Usually: Put again a sampling calorimeter after the ECAL

Dense blocks, such as iron, uraniumDetectors, such as wire chambers,

or scintillators

Sandwich structure !

Total amount of signalsregistered is proportionalto incident energy. Same energy lost in nuclear excitations!

Has to be calibrated with beams of known energy!

Sandwich structure !

Total amount of signalsregistered is proportionalto incident energy. Same energy lost in nuclear excitations!

Has to be calibrated with beams of known energy!

ALEPH ALEPH

iron

Particle IdentificationParticle Identification

Basic principles: via different interaction with matter (see previous

transparencies)

by measuring the mass from the decay products

by measuring the velocity and independently (!)independently (!) the momentum

Observables sensitive to velocity are

mean energy loss

Cherenkov radiation

Mean energy lossMean energy loss Particles which traverse a gas loose energy, eg. by by

ionizationionization

Elost / path length = func( particle-velocity v/c )

Elost / path length = func( particle-velocity v/c ) Bethe-Bloch formula

Elost amount of ionization size of signals on wires

Note : if plotted as a functionof v and not p all the bands would lie on top of each other!

Note : if plotted as a functionof v and not p all the bands would lie on top of each other!

Cherenkov radiationCherenkov radiation

Particles which in a medium travel faster than the faster than the speed of light in that mediumspeed of light in that medium emit a radiation

--> Cherenkov radiationCherenkov radiation

v

1

nvsin 0cc

v

1

nvsin 0cc

c0 = speed of light in vacuum

Cherenkovlight

wavefront

Compare : shock wave of supersonic airplanes

See http://webphysics.davidson.edu/applets/applets.html for a nice illustration

Large detector systemsLarge detector systems

All these concepts have been put together and realized in large detector systems

Examples at LEP ALEPH , OPAL , L3 , DELPHIALEPH , OPAL , L3 , DELPHI

Fixed Target NA48NA48

Future experiments at LHC ATLAS, CMS, LHCb, ALICEATLAS, CMS, LHCb, ALICE

ATLASATLAS

See http://pdg.lbl.gov/atlas/index.html

See http://cmsinfo.cern.ch/Welcome.html/

SummarySummary I have tried to explain

what what are the things we want to measure in HEP experiments

how how we do it (tracking, calorimetry, particle identification)

This is an enormously large field, of course many things have been left out DAQ (data acquisition) other detector technologies applications in particle astrophysics (cosmic rays, neutrinos,…)

applications outside HEP

I invite you to study these points

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