PHYS 3446, Fall 2006 - PowerPoint PPT Presentation

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PHYS 3446, Fall 2006

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its time of flight (t) for reaching some scintillation counter at a distance L ... is called nuclear interaction lengths and is substantially larger than that ... – PowerPoint PPT presentation

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Title: PHYS 3446, Fall 2006


1
PHYS 3446 Lecture 13
Monday, Oct. 23, 2006 Dr. Jae Yu
  • Particle Detection
  • Scintillation Counters
  • Time of Flight
  • Cerenkov Counter
  • Calorimeters
  • 2. Particle Accelerators
  • Electrostatic Accelerators

2
Announcements
  • Research Day tomorrow Rio Grande
  • 9am 4pm poster presentations
  • Our cloud chamber prototype will be in display
    from noon 4pm
  • Need presenters to operate the chamber and man
    the poster
  • Next LPCC Workshop
  • Preparation work
  • Lists of goals and items to purchase?
  • 10am 5pm, Saturday, Nov. 4
  • CPB303 and HEP experimental areas
  • Quiz results
  • Class average 68.5
  • Top score96/90
  • Assignments
  • Derive Eq. 7.10
  • Carry out computations for Eq. 7.14 and 7.17
  • Due for these assignments is Monday, Oct. 30

3
Paper Template
4
Scintillation Counters
  • Two types of scintillators
  • Organic or plastic
  • Tend to emit ultra-violate
  • Wavelength shifters are needed to reduce
    attenuation
  • Faster decay time (10-8s)
  • More appropriate for high flux environment
  • Inorganic or crystalline (NaI or CsI)
  • Doped with activators that can be excited by
    electron-hole pairs produced by charged particles
    in the crystal lattice
  • These dopants can then be de-excited through
    photon emission
  • Decay time of order 10-6sec
  • Used in low energy detection

5
Scintillation Counters Photo-multiplier Tube
  • The light produced by scintillators are usually
    too weak to see
  • Photon signal needs amplification through
    photomultiplier tubes
  • Gets the light from scintillator directly or
    through light guide
  • Photocathode Made of material in which valence
    electrons are loosely bound and are easy to cause
    photo-electric effect (2 12 cm diameter)
  • Series of multiple dynodes that are made of
    material with relatively low work-function
  • Operating at an increasing potential difference
    (100 200 V) difference between dynodes

6
Scintillation Counters Photo-multiplier Tube
  • The dynodes accelerate the electrons to the next
    stage, amplifying the signal to a factor of 104
    107
  • Quantum conversion efficiency of photocathode is
    typically on the order of 0.25
  • Output signal is proportional to the amount of
    the incident light except for the statistical
    fluctuation
  • Takes only a few nano-seconds for signal
    processing
  • Used in as trigger or in an environment that
    requires fast response
  • ScintillatorPMT good detector for charged
    particles or photons or neutrons

7
Some PMTs
Super-Kamiokande detector
8
Scintillation Detector Structure
HV PS
Scintillation Counter
Light Guide/ Wavelength Shifter
PMT
Readout Electronics
Scope
9
Time of Flight
  • Scintillator PMT can provide time resolution of
    0.1 ns.
  • What position resolution does this corresponds
    to?
  • 3cm
  • Array of scintillation counters can be used to
    measure the time of flight (TOF) of particles and
    obtain their velocities
  • What can this be used for?
  • Can use this to distinguish particles with about
    the same momentum but with different mass
  • How?
  • Measure
  • the momentum (p) of a particle in the magnetic
    field
  • its time of flight (t) for reaching some
    scintillation counter at a distance L from the
    point of origin of the particle
  • Determine the velocity of the particle and its
    mass

10
Time of Flight (TOF)
  • TOF is the distance traveled divided by the speed
    of the particle, tL/v.
  • Thus Dt in flight time of the two particle with
    m1 and m2 is
  • For known momentum, p,
  • Since
  • In non-relativistic limit,
  • Mass resolution of 1 is achievable for low
    energies

11
Cerenkov Detectors
  • What is the Cerenkov radiation?
  • Emission of coherent radiation from the
    excitation of atoms and molecules
  • When does this occur?
  • If a charged particle enters a dielectric medium
    with a speed faster than light in the medium
  • How is this possible?
  • Since the speed of light is c/n in a medium with
    index of refraction n, if the particles bgt1/n,
    its speed is larger than the speed of light
  • Cerenkov light has various frequencies but blue
    and ultraviolet band are most interesting
  • Blue can be directly detected w/ standard PMTs
  • Ultraviolet can be converted to electrons using
    photosensitive molecules mixed in with some gas
    in an ionization chamber

12
Cerenkov Detectors
  • The angle of emission is given by
  • The intensity of the produced radiation per unit
    length of the radiator is proportional to sin2qc.
  • For bngt1, light can be emitted while for bnlt1, no
    light can be observed.
  • Thus, Cerenkov effect provides a means for
    distinguishing particles with the same momentum
  • One can use multiple chambers of various indices
    of refraction to detect Cerenkov radiation from
    particles of different mass but with the same
    momentum

13
Cerenkov Detectors
  • Threshold counters
  • Particles with the same momentum but with
    different mass will start emitting Cerenkov light
    when the index of refraction is above a certain
    threshold
  • These counters have one type of gas but could
    vary the pressure in the chamber to change the
    index of refraction to distinguish particles
  • Large proton decay experiments use Cerenkov
    detector to detect the final state particles,
    such as p ? ep0
  • Differential counters
  • Measure the angle of emission for the given index
    of refraction since the emission angle for
    lighter particles will be larger than heavier ones

14
Super Kamiokande A Differential Water Cerenkov
Detector
  • Kamioka zinc mine, Japan
  • 1000m underground
  • 40 m (d) x 40m(h) SS
  • 50,000 tons of ultra pure H2O
  • 11200(inner)1800(outer) 50cm PMTs
  • Originally for proton decay experiment
  • Accident in Nov. 2001, destroyed 7000 PMTs
  • Dec. 2002 resumed data taking

15
Super-K Event Displays
16
Cerenkov Detectors
  • Ring-imaging Cerenkov Counters (RICH)
  • Use UV emissions
  • An energetic charged particle can produce
    multiple UV distributed about the direction of
    the particle
  • These UV photons can then be put through a
    photo-sensitive medium creating a ring of
    electrons
  • These electrons then can be detected in an
    ionization chamber forming a ring
  • Babar experiment at SLAC uses this detector

17
Semiconductor Detectors
  • Semiconductors can produce large signal
    (electron-hole pairs) for relatively small energy
    deposit (3eV)
  • Advantageous in measuring low energy at high
    resolution
  • Silicon strip and pixel detectors are widely used
    for high precision position measurements
  • Due to large electron-hole pair production, thin
    layers (200 300 mm) of wafers sufficient for
    measurements
  • Output signal proportional to the ionization loss
  • Low bias voltages sufficient to operate
  • Can be deposit in thin stripes (20 50 mm) on
    thin electrode
  • High position resolution achievable
  • Can be used to distinguish particles in multiple
    detector configurations
  • So what is the catch?
  • Very expensive ? On the order of 30k/m2

18
DØ Silicon Vertex Detector
19
Calorimeters
  • Magnetic measurement of momentum is not
    sufficient for physics, why?
  • The precision for angular measurements gets worse
    as particles momenta increases
  • Increasing magnetic field or increasing precision
    of the tracking device will help but will be
    expensive
  • Cannot measure neutral particle momenta
  • How do we solve this problem?
  • Use a device that measures kinetic energies of
    particles
  • Calorimeter
  • A device that absorbs full kinetic energy of a
    particle
  • Provides signal proportional to deposited energy

20
Calorimeters
  • Large scale calorimeter were developed during
    1960s
  • For energetic cosmic rays
  • For particles produced in accelerator experiments
  • How do high energy EM (photons and electrons) and
    Hadronic particles deposit their energies?
  • Electrons via bremsstrahlung
  • Photons via electron-positron conversion,
    followed by bremsstrahlung of electrons and
    positrons
  • These processes continue occurring in the
    secondary particles causing an electromagnetic
    shower losing all of its energy

21
Electron Shower Process
Photon, g
22
Calorimeters
  • Hadrons are massive thus their energy deposit via
    brem is small
  • They lose their energies through multiple nuclear
    collisions
  • Incident hadron produces multiple pions and other
    secondary hadrons in the first collision
  • The secondary hadrons then successively undergo
    nuclear collisions
  • Mean free path for nuclear collisions is called
    nuclear interaction lengths and is substantially
    larger than that of EM particles
  • Hadronic shower processes are therefore more
    erratic than EM shower processes

23
Sampling Calorimeters
  • High energy particles require large calorimeters
    to absorb all of their energies and measure them
    fully in the device (called total absorption
    calorimeters)
  • Since the number of shower particles is
    proportional to the energy of the incident
    particles
  • One can deduce the total energy of the particle
    by measuring only the fraction of their energy,
    as long as the fraction is known ? Called
    sampling calorimeters
  • Most the high energy experiments use sampling
    calorimeters

24
How particle showers look in detectors
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