Transcript No Slide Title
Scintillation Counters and Photomultiplier Tubes
Learning Objectives
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Understand the basic operation of CROP scintillation counters and photomultiplier tubes (PMTs) and their use in measuring cosmic ray air showers
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Understand how light is generated in a scintillator
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Understand how light is transmitted to a PMT
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Understand how a PMT generates an electric signal
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Be able to hook up a scintillation counter to its high voltage and an oscilloscope for viewing signals
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Be able to identify light leaks in a scintillation counter
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Be able to observe scintillation counter signals using an oscilloscope and identify cosmic ray muons
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Be able to discuss scintillation counter performance in terms of gain, efficiency and attenuation length
Scintillation Counters and Photomultiplier Tubes
Outline
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Introduction
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Light Generation in Scintillators
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Light Collection
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Optical Interfaces and Connections
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Photodetectors and photomultiplier tubes
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Performance and Exercises
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References
Scintillation Counters and Photomultiplier Tubes
Introduction
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Scintillation counters are multi-purpose particle detectors used in many experimental physics applications
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Used for charged particle detection (positive or negative), but also neutral particles (photons, neutrons), although light-generation mechanisms are different for charged and neutral particles
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Basic sequence -- light generation by particle passing through scintillator material, light collection, photodetector turns light into electric signal
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Scintillation Counter Properties Fast time response -- light generated almost immediately after particle passes through scintillator, photodetectors give fast electric signal
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Can count number of particles using pulse height.
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The larger the signal size, the greater the number of particles
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Position information
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Based on size of active scintillator material
Scintillation Counters and Photomultiplier Tubes Basic principles of operation Passage of charged particle generates light in scintillator Charged particle Light guide transmits light to photodetector Photomultiplier tube (PM or PMT) generates electric signal
Scintillation Counters and Photomultiplier Tubes
Introduction
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Examples from High Energy Physics experiments at particle accelerators
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Hodoscope -- an array of several counters covering a large area
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Veto counters -- for particles you don’t want to measure
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Calorimetry -- measuring a particle’s total energy Triggering -- a fast signal which indicates an interesting event to record Examples from cosmic ray experiments
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CASA KASCADE
Scintillation counters in High-Energy Physics Experiments
Fermilab, Batavia, Illinois Protons Anti-protons CERN, Geneva, Switzerland
Scintillation Counters and Photomultiplier Tubes
Scintillation counter hodoscope
Photomultiplier tube Scintillator wedge Foil wrapping Counters arranged as pizza slices
Chicago Air Shower Array (CASA) Dugway Proving Grounds, Utah
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University of Chicago and University of Utah collaboration to study extended cosmic ray air showers
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1089 boxes in a rectangular grid, 15 meter spacing, each with
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4 scintillator planes and 4 photomultplier tubes
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1 low voltage and 1 high voltage supply
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1 electronics card for data triggering and data acquisition
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CASA collected data in the 1990’s and is now complete
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CROP will use retired scintillation counters recovered from CASA
Scintillation Counters and Photomultiplier Tubes Contents of a CASA detector station Electronics card Weatherproof box top 4 scintillators and PMTs Box bottom
The KASCADE experiment in Karlsruhe, Germany
KASCADE = KA rlsruhe S hower C ore and A rray DE tector
• 252 detector stations • Rectangular grid with 13 m spacing • Array of 200 x 200 m
2
The KASCADE experiment
Scintillation Counters and Photomultiplier Tubes
Introduction
Other uses of scintillation counters -- biological research, medical applications (PET scans)
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Use of scintillation counters in CROP Several counters firing at once indicates extended air shower -- on one school or inter-school
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Pulse heights related to number of particles in shower and energy of primary cosmic ray
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Relative arrival times related to primary cosmic ray incident direction
Scintillation Counters and Photomultiplier Tubes
PET Scans (Positron Emission Tomography)
Scintillating crystal detector and photomultiplier Cross Section 3-D image
Scintillation Counters and Photomultiplier Tubes
2. Light generation in scintillators
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Different scintillator materials
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Plastic scintillator -- good for large areas
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Sodium Iodide (NaI)
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BGO (Bi 4 Ge 2 O 12 ) Lead Tungstanate (PbWO 4 ) Inorganic crystals
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Focus on plastic scintillator
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Composition
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Polystyrene (plexiglass)
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Doped with small admixture of a fluor
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Fluor is organic macro-molecule like POPOP: 1,4-Bis-[2-(5-phenyloxazolyl)]-benzene C 24 H 16 N 2 O 2
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Light generated by fluorescence process
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One of energy loss mechanisms when charged particles pass through matter
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Similar to television screen or computer monitor Quantum mechanical process Light (photons) emitted isotropically
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Emission spectrum from typical scintillator
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Relation to visible light spectrum
Energy absorption and emission diagram Electrons excited to higher energy levels when a charged particle passes, absorbing part of its energy Electron ground state Electrons drop back to ground state, emitting fluorescence or scintillation light
Scintillation Counters and Photomultiplier Tubes
Typical plastic scintillator emission spectrum
Wavelength of emitted light
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1 nm = 1 nanometer = 1
10 -9 meter For reference, 1 nm = 10 Angstroms, where 1 Angstrom is approximate size of an atom
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Maximum emission at about 425 nm
Scintillation Counters and Photomultiplier Tubes The wavelengths of visible light
Scintillation Counters and Photomultiplier Tubes
Scintillation Counters and Photomultiplier Tubes
3. Light Collection
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Purpose -- Direct as much generated light as possible to the photodetector
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Need for making counters light tight
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Light transmission within scintillator
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Reflections from surfaces, total internal reflection
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Transmission through surfaces
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Critical angle Importance of smooth polished surfaces Use of reflective coverings (foil, white paint, white paper, black paper)
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Multiple bounces (many!) Ray-tracing simulation programs
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Attenuation of light in scintillator
Scintillation Counters and Photomultiplier Tubes
Light transmission within scintillator
Charged particle passes through here Scintillator Light rays Photomultiplier tubes
Scintillation Counters and Photomultiplier Tubes
Reflection and transmission at surfaces
Air Scintillator material Light totally internally reflected for incident angle greater than
critical which depends on optical properties of scintillator and air Scintillator Air Refraction (i.e. transmission) outside scintillator for incident angle less than
critical
Scintillation Counters and Photomultiplier Tubes
3. Light Collection
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Different light collection schemes
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Different types of plastic light guides
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Air light guides (KASCADE)
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CASA scheme
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Not optimal, PMT glued onto surface
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Wavelength-shifting side bars
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Embedded wavelength-shifting optical fibers
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Connected to clear optical fibers
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Can transport light over long distance
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Other fiber optics applications
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Laproscopic surgery Telecommunications
Scintillation Counters and Photomultiplier Tubes
Laproscopic surgery
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Optical fibers transmit image to surgeon Less instrusive technique
Light collection in the KASCADE experiment Electron and photon detector Photomultiplier 33 kg of liquid scintillator Argon-filled space (better light transmission than air) Light emitted from scintillator is guided by conical reflecting surfaces to photomultiplier tube above
Light collection in the KASCADE experiment Muon detector Wavelength-shifting bars around perimeter of planes guide light to photomultiplier tubes 4 plastic scintillator planes
Scintillation Counters and Photomultiplier Tubes
Optical Fibers
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Fiber core and cladding optimized to prevent leakage of light out of the fiber
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95% transmission over 1 km
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If this were true for ocean water, you could clearly see ocean bottom Transmission modes within optical fibers
Scintillation Counters and Photomultiplier Tubes
What’s wrong with this picture?
Scintillation Counters and Photomultiplier Tubes
Several scintillators tied together optically with optical fibers
To photo-detector Wavelehgth-shifting optical fiber Scintillator planes
Scintillation Counters and Photomultiplier Tubes
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Advantages and limitations of each type of light read-out scheme
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Definition of
efficiency of light collection
Number of photons arriving at the photo-detector Number of photons generated by charged particle
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About 10% for light guide attached to side
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A few percent for CASA counters
Scintillation Counters and Photomultiplier Tubes
4. Optical Interfaces and Connections
Purpose -- transmit light with high efficiency, sometimes provide mechanical stability of detector as well (should decouple the two tasks if possible)
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Interface between scintillator material and
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Light guide
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Optical fiber
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Wavelength-shifting bar
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Interface between light guide or fiber and photodetector
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Commonly used
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Optical cements and epoxies
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Optical grease
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Air gap
Scintillation Counters and Photomultiplier Tubes
5. Photodetectors and Photomultiplier Tubes
Purpose -- transform light into electric signal for further processing of particle information
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Examples
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Photomultiplier tube (CROP focus)
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Photodiode
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Charged-coupled device
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Avalanche photodiode (APD) Visible Light Photon Counter (cryogenics)
Photomultiplier tube details
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Entrance window
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Must be transparent for light wavelengths which need to enter tube
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Common: glass Fused silicate -- transmits ultraviolet as well
Scintillation Counters and Photomultiplier Tubes Schematic drawing of a photomultiplier tube (from scintillator) Photocathode Photons eject electrons via photoelectric effect Each incident electron ejects about 4 new electrons at each dynode stage “Multiplied” signal comes out here Vacuum inside tube An applied voltage difference between dynodes makes electrons accelerate from stage to stage
Scintillation Counters and Photomultiplier Tubes Different types of dynode chain geometries
Scintillation Counters and Photomultiplier Tubes
Definition of
Photomultiplier Tube Gain
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= average number of electrons generated at each dynode stage
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Typically,
= 4 , but this depends on dynode material and the voltage difference between dynodes
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n = number of multiplication stages
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Photomultiplier tube gain =
n
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For n = 10 stages and
= 4 ,
gain = 4 10 = 1
10 7
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This means that one electron emitted from the photocathode (these are called “photoelectrons”) yields 1
10 7 electrons at the signal output
Scintillation Counters and Photomultiplier Tubes
The Photocathode
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Incoming photons expel electrons from the metallic surface of the photocathode via the photoelectric effect.
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The effect was discovered by Heinrich Hertz in 1887 and explained by Albert Einstein in 1905.
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According to Einstein's theory, light is composed of discrete particles of energy, or quanta, called PHOTONS . When photons with enough energy strike the photocathode, they liberate electrons that have a kinetic energy equal to the energy of the photons less the “work function” (the energy required to free the electrons from a particular material).
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Einstein received the Nobel Prize for his 1905 paper explaining the photoelectric effect. What were the other two famous Einstein papers from 1905?
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Theory of special relativity
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Explanation of Brownian motion
Scintillation Counters and Photomultiplier Tubes
The Photocathode
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Photocathode composition
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Semiconductor material made of antimony (Sb) and one or more alkalai metals (Cs, Na, K)
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Thin, so ejected electrons can escape
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Definition of
photocathode quantum efficiency,
h(l) h(l)
=
Number of photoelectrons released Number of incident photons (
l
) on cathode
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Typical photocathode quantum efficiency is 10 - 30%
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Photocathode response spectrum
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Need for matching scintillator light output spectrum with photocathode response spectrum
Scintillation Counters and Photomultiplier Tubes Typical photocathode response curve 200 nm Wavelength of light 1 nm = 1 nanometer = 1
10 -9 meter Note: Quantum efficiency > 20% in range 300 - 475 nm Peak response for light wavelengths near 400 nm 700 nm
Scintillation Counters and Photomultiplier Tubes
The dynode chain
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High voltage applied to dynodes creates electric fields which guide electrons between from stage to stage
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Process of
secondary emission
yields more electrons at each stage
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This is the “multiplication” in “photomultiplier”
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Process is similar to photoelectric effect, with incident photon replaced by incident electron
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Composition of dynodes
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Ag - Mg
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Cu - Be Deposited in thin layer on
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Cs - Sb conducting support
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Sensitivity to earth’s magnetic field
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Earth’s magnetic field is typically 0.5 - 1.0 Gauss
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Trajectories of charged particles moving in a magnetic field will curve, depending on field orientation
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Can cause photoelectrons and secondary-emitted electrons not to reach next stage
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First few stages, when there are few electrons, most vulnerable
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Use of magnetic shields
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Should extend shield beyond front of tube
Scintillation Counters and Photomultiplier Tubes
The phototube base and high voltage supply
Purpose -- provide an electric field between
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photocathode and first dynode
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successive dynodes to accelerate electrons from stage to stage
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About 100 V voltage difference needed between stages
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Chain of resistors forms voltage divider to split up high voltage into small steps
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Capacitors store readily-available charge for electron multiplication
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Typical base draws 1 - 2 milliamperes of current
Scintillation Counters and Photomultiplier Tubes The electric field between successive dynodes A simplified view 100 Volts
+
Represents a dynode
- - - - -
Electric field between plates
+ + + + + +
Represents the next dynode An electron (negative charge) released from the negative plate will be accelerated toward the positive plate
Photocathode Dynodes Tube body Scintillation Counters and Photomultiplier Tubes Typical phototube base schematic Output signal to oscilloscope Ground Positive High voltage supply Capacitors (which store charge) needed for final stages when there are many electrons Output signal flows out of tube Current flows through resistor chain for voltage division
Scintillation Counters and Photomultiplier Tubes
A simple voltage divider
Current, I (amperes) Greek omega for resistance unit, Ohms 4
W =
R
1
Battery V batt = 9 Volts
+ -
a 2
W =
R
2
Voltmeter here b
Ohm' s law :
V
=
I
R
or
I
=
V R
Current in V
across
R
2 =
I
circuit
R
2 =
:
I
( 1
=
.
5
R
1
V
batt
R
Amps
2
)(
=
9 2
W
) Volts 6
W = =
1 3 Volts .
5 Amps
Measured with voltmeter between points (a) and (b) You have “divided” the 9 Volt battery: 3 Volts and 6 Volts are now accessible with this circuit.
Scintillation Counters and Photomultiplier Tubes
Vacuum inside tube body
Purpose -- minimize collisions of electrons with gas molecules during transit
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Requires strong tube body Pins for electrical connections pierce through glass at bottom of tube (leak-tight)
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Damage to tube by helium or hydrogen
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“Small” gas molecules can leak into tube, even through glass
Scintillation Counters and Photomultiplier Tubes
Variation of PMT gain with high voltage
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Increasing high voltage increases electron transmission efficiency from stage to stage
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Especially important in first 1-2 dynodes
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Increasing high voltage increases kinetic energy of electrons impacting dynodes
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Increases amplification factor
Scintillation Counters and Photomultiplier Tubes Oscilloscope traces from scintillation counters Plastic scintillator 10 nsec / division Inorganic crystal, NaI 5000 nsec / division (Longer time scale for fluorescence to occur)
Scintillation Counters and Photomultiplier Tubes Close-up of photoelectron trajectories to first dynode
Scintillation Counters and Photomultiplier Tubes
References
1. Introduction to Experimental Particle Physics by Richard Fernow, Cambridge University Press, 1986, ISBN 0-521-30170-7 (paperback), Chapter 7, pages 148-177 (includes exercises) 2. Photomultiplier Manual, Technical Series PT-61, 1970, RCA Corporation 3. Techniques for Nuclear and Particle Physics by W. R. Leo, Springer-Verlag, Germany, 1994, ISBN 3-540-57280-5, Chapters 7-9, pages 157-214 4. Radiation Detection and Measurement, 3rd Edition, by Glenn F.Knoll, Wiley 2000, ISBN 0-417-07338-5, Chapters 8-10, pages 219 - 306
Scintillation Counters and Photomultiplier Tubes
Light transmission through entrance wnidow
Different window materials Wavelength of light 200 nm 700 nm
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Observe:
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20% transmission typical for 400 nm light
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Fused silica extends transmission into lower wavelengths Less than 400 nm is ultraviolet light
Scintillation Counters and Photomultiplier Tubes
Scintillation Counters and Photomultiplier Tubes
6. Performance and exercises
Signal shape, pulse height and duration Pulse height distributions Linearity Attenuation length Oscilloscope examples and exercises with changing high voltage, radioactive source, attenuation length
Scintillation Counters and Photomultiplier Tubes
Development Questions
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Request permission to use figures now
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Specific figures or general release?
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What format to aim for this summer?
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Powerpoint presentation (with embedded figures?)
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Accompanying text
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Accessibility on the web, with “more detail here” links
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Curriculum & Instruction check for level-appropriateness
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Format for field-testing in schools
Scintillation Counters and Photomultiplier Tubes