introduction: detector tasks
DESCRIPTION
Particle Detectors Tools of High Energy and Nuclear Physics Goal: to detect Individual Particles and reconstruct their 4-vectors Thanks to H. Fenker (Jlab) and B. Surrow (MIT). Introduction: detector tasks. Position measurement: localize hits of a charged particle - PowerPoint PPT PresentationTRANSCRIPT
Particle DetectorsTools of High Energy and Nuclear Physics
Goal: to detect Individual Particlesand reconstruct their 4-vectors
Thanks to H. Fenker (Jlab) and B. Surrow (MIT)
Introduction: detector tasks
• Position measurement: localize hits of a charged particle(eg: wire chambers, segmented scintillators or calorimeters)
• Momentum measurement: by measuring the particle deflection in a magnetic field (eg: magnetic spectrometer)
• Energy measurement: deposition of energy in a localized volume (eg: calorimeters)
• Particle identification: mass and charge of the particle (eg: Cerenkov detectors)
• Triggering: select events of interest• Data acquisition system: readout of an event and storage
after positive decision.
Introduction: detector performances
• Time– Response time: time which is required to produce a signal after the
passage of a particle in the detector (from ~10 ns to ~100 s).– Deadtime: time that must elapse following the passage of a particle
before the detector is ready for the next particle.
• EfficiencyThat is (event registered)/(events emitted by source)The efficiency is the product of at least two quantities:– Intrisic efficiency: (event registered)/(events impinging on detector)– Geometric efficiency: (event impinging on detector)/(event emitted by
source)
• Resolution/Accuracy
Example of position detectors performance
• Avalanche multiplication• Detectors that see the
electrons– Wire chambers
– Time Projection Chamber
– Gas Electron Multiplier
• Detectors that see the light– Scintillators
– Cerenkov Detectors
– Calorimeters
Outline of class Interactions of Particles with Matter
Charged particles
Photons
Using the Interactions:Particle Detectors
Avalanche multiplication
Detectors that sense Charge
Detectors that sense light
Aside: magnetic spectrometers
Putting it all together
Interaction of particles with matter
Charged particles:Energy and trajectories get
degraded as they pass through matter:
• Ionization• Bremsstrahlung• Cherenkov radiation
Photons:Flux gets decreased as they go
through matter. All or nothing interactions
• Photo-electric effects• Compton scattering• Pair production
Outline of class Interactions of Particles with Matter
Charged particle
Photons
Using the Interactions:Particle Detectors
Avalanche multiplication
Detectors that sense Charge
Detectors that sense light
Aside: magnetic spectrometers
Putting it all together
Charged particles- Ionization
Atomic electron is knocked free from the atom.
The remaining atom is now an ion or left in an excited state (will decay by emitting a photon)
ChargedParticle
Free Electron
Electric Field
IonIonization
Ionization: Bethe-Bloch formula
where , , relate to particle speed, z is the particle’s charge..
The other factors describe the medium (Z/A, I, ), or are physical constants.
dE/dx units is MeV cm2/g
E= dE/dx * x /
A value to keep in mind is 2 MeV.g-1.cm2
Charged Particles: Bremsstrahlung
Radiation of real photons in the Coulomb field of a nuclei of the absorber.
Electron
Nucleus
Photon
Define X0 the radiation length: length during which the particle looses a fraction e of its initial energy
Critical energy (Ec) is the energy at which Bremstrahlung loss equal ionization loss
Ec(e- Cu)=20 MeV
Ec(- Cu)=800 GeV
Charged particles: Multiple Coulomb Scattering(both for ionization and radiation)
Detectors scatter particles even without much energy loss…
MCS theory is a statistical description of the scattering angle arising from many small interactions with atomic electrons.
MCS alters the direction of the particle in average.
Most important at low energy.
is particle speed,
z is its charge,
X0 is the material’s Radiation Length.
0
Charged particles- Cerenkov radiationThe electric field of a particle has a long-range interaction with material as it passes
through a continuous medium. It does create a shock wave that causes the material to emit light when it’s speed is large
enough
v = c > c/n where n is the index of refraction of the material
Also the light is emitted at the angle = cos-1 (1/n)
Photon energy ~ few eV (UV to visible) (not an efficient way to loose energy)
1/n1/n
Cerenkov light produced by fuel elements of a nuclear power plant.
Outline of class Interactions of Particles with Matter
Charged particle
Photons
Using the Interactions:Particle Detectors
Avalanche multiplication
Detectors that sense Charge
Detectors that sense light
Aside: magnetic spectrometers
Putting it all together
Interaction of photon with matterPhoto-electric effect
Compton scattering
Pair production
Interaction of photon with matter
Total probability for interaction:
Probability per unit length or total absorption coefficient
Such that the flux of photon is
Absorption length=(absorption coeff)-1
Interactions of Particles with Matter - Summary
When particles pass through matter they usually produce either free electric charges (ionization) or light (photoemission).
Most “particle” detectors actually detect the light or the charge that a particle leaves behind.
In all cases we finally need an electronic signal to record.
Outline of class Interactions of Particles with Matter
Charged particle
Photons
Using the Interactions:Particle Detectors
Aside: Avalanche multiplication
Detectors that sense Charge
Detectors that sense light
Aside: magnetic spectrometers
Putting it all together
Particle Detectors… Avalanche Multiplication
When a particle passes through matter, it creates just a fewelectrons/ions or photons
But the best we can do is to detect signals of the order of nV in a 100 Ohm resistor which
correspond toI= U/R= 10-9 /100 = 10-11 A = 108 electrons. s-1
Which means: The detectors need to amplify the charge produced by particles going through matter. By giving
the charges a push, we can make them move fast enough so that they ionize other atoms when they collide. After this has happened several times we have a sizeable free charge that can be sensed by an electronic circuit.
Particle Detectors: amplification with the photo multiplier
PMTs are commercially produced and very sensitive.•One photon --> up to 108 electrons!•Fast! …down to ~ few x 10-9 seconds.
Photoelectric Effect: A photon liberates a single electron
Secondary Emission
Energetic electrons striking some surfaces can liberate MORE electrons. Those, in turn, can be accelerated onto another surface … so on.
• V is the voltage• rc radius of the outer cathode plane• ra radius of the inner anode
Close to the wire the E field is veryIntense, the charged particle is Accelerated and as a result creates secondaryParticles.
Particle Detectors: amplification with the E-Field
Particle Detectors… Gas Electron Multiplier (GEM)
Gas Ionization and Avalanche Multiplication again, but…
… a different way to get an intense electric field,
… without dealing with fragile tiny wires
http://gdd.web.cern.ch/GDD/
--V
~400v0.002”
GEM
To computer
Dense Material => Lots of Charge. Typically no Amplification
Noble LiquidLiquid Argon Calorimeter
Signals toComputer
Electrons are knocked loose in the silicon and drift throughit to electronics.
Readout strips maybe VERY NARROW
0.001”
0.012”
SemiconductorSilicon
Diamond
StripsPixelsDrift
Particle Detectors: bypassing the amplification (new methods)
Particle detectors
• Avalanche multiplication• Detectors that see the
electrons– Wire chambers
– Time Projection Chamber
• Detectors that see the light– Scintillators
– Cerenkov Detectors
– Calorimeters
Particle Detectors: Gas Filled Wire Chamber
Let’s use Ionization and Avalanche Multiplication to build a detector…
Make a Box. Fill it with some gas: noble gases are more likely to ionize than
others. Use Argon. Insert conducting surfaces to make an intense electric field: The
field at the surface of a small wire gets extremely high, so use tiny wires.
Attach electronics and apply high voltage. We’re done!!
Straw Tube Tracker for the COSY-TOF Experiment Julich Institute (Germany)
Central Drift Chamber (Hall D Jlab)
Straw chambers: better resolution
2D solution:
The wire touched gives X position info
The time of transit between the two amplis gives the Y position info
X
y
Multi-Wire Gas Chamber
start
stop
Best 1D solution:
-Use an external trigger to start a clock
-Measure the time it takes for the electron to drift from the initial ionization to the wire.
Resolution ~ 10 m
TPC: 3D position information.
Cathode Anode(gain)
Readoutelectrodes
Time Projection Chamber (TPC): Drift through a VolumeJust a box of gas with
Electric Field andReadout Electrodes
Readout elements only on one surface.Ionization Electrons drift to Surface for
AmplificationCharge Collection
Readout Electrode Position gives (x,y)Time of Arrival gives (z).
Particletrack
X
Y
Z
Particle detectors
• Avalanche multiplication• Detectors that see the
electrons– Wire chambers
– Time Projection Chamber
• Detectors that see the light– Scintillators
– Cerenkov Detectors
– Calorimeters
Particle Detectors… Cerenkov Counter
If =v/c > 1/n, there will be light.If not, there won’t.
Can be used for trigger systemIf you know the momentum of the particle: can be used for PID
Cerenkov Counters – sensitive to
TRD Counters – sensitive to
= (1- 2)-1/2 = E/m
= v/c = p/E
Momentum (GeV/c)
Rich detector : Ring imaging Cherenkov
Light is emitted at the angle
= cos-1 (1/n)
Scintillators
Scintillation Counters are probably the most widely used detectors in Nuclear and High Energy Physics.
Scintillator material are special material that
-emit light when traversed by energetic particles and
-can shift the wavelength of this light
to be harnessed by PMTs
They can be solid, liquid (even gas)
They can be molded in all kind of shapes
Solids
Liquid
Saint Gobin Inc
Sample experimentMIT/Bates
Detecting scintillationIn Air.
Particle Detectors: Calorimeter
Used to measure energy.
Based on Bremsstrahlung effect
Suppose an initial photon of energy E0
After t radiation lengths, the average energy of secondary is:
The number of secondaries is
The shower stops when
EM (or hadronic) calorimeters are used because:- They can detect charged or neutral particle- They produce a really fast signal (10-100 ns) that is ideal for making trigger decision
The energy resolution of the calorimeter therefore goes as
Alice’s ZDC calorimeterCERN
Hall A/DVCS calorimeter(50*30 cm2)JLAB
Outline of class Interactions of Particles with Matter
Charged particle
Photons
Using the Interactions:Particle Detectors
Avalanche multiplication
Detectors that sense Charge
Detectors that sense light
Aside: magnetic spectrometers
Putting it all together
Particle Detectors:aside: magnetic spectrometer
Just as light of different wavelength is bent differently by a prism...
Nature lets us measure the Momentum of a chargedparticle by seeing how much its path is deflected bya magnet.
(x1,y1)(x2,y2)
Magnet
MAMI (Germany)
Four quantities measured in the IN frame and 4 in the OUT/VDC frame.The best is to design the magnet to be insensitive to xIN and with <x|> as the main coefficient
Central trajectory
OUT frame usually equipped with a Vertical Drift Chamber (VDC)
IN frameUsually a“short” target
Outline of class Interactions of Particles with Matter
Charged particle
Photons
Using the Interactions:Particle Detectors
Avalanche multiplication
Detectors that sense Charge
Detectors that sense light
Aside: magnetic spectrometers
Putting it all together
Putting it all Together: A Detector SystemHall C/JLAB
Putting it all Together: A Detector System
QWEAK: conceptual overview
• Elastic e-p scattering on liquid hydrogen target• Toroidal magnet to provide momentum dispersion• Collimator system to select elastic events only• Lower energy inelastic events bent outside of the detector acceptance
Outline of class Interactions of Particles with Matter
Charged particle
Photons
Using the Interactions:Particle Detectors
Avalanche multiplication
Detectors that sense Charge
Detectors that sense light
Aside: magnetic spectrometers
Putting it all together