Welcome Guestlogin to KGsePGregister at KGsePG email | FAQs

Detection And Dosimetry Of Ionising Radiation

download

    1 of 123

    Detection And Dosimetry Of Ionising Radiation



    Detection And Dosimetry Of Ionising Radiation - Transcript


    MSc-REP Regan Dosimetry 1
    Detection and Dosimetry of
    Ionising Radiation
    MSc-REP Lecture Notes
    Paddy Regan
    p.regan@surrey.ac.uk
    http://www.ph.surrey.ac.uk/~phs1pr/lecture_notes
    MSc-REP Regan Dosimetry 2
    Course text book,
    Radiation Biophysics
    by
    E.L. Alpen, Academic Press
    2nd Edition, (1990)
    Important chapters for this course,
    Chapter 1: Quantities and Units
    Chapter 4: Radiation/Matter interactions.
    Chapter 5: Energy Transfer Processes
    Chapter 16: Dose, Dose Equivalent
    Also, refer to Radiation Detection and
    Measurement, G.F.Knoll, 2nd Edition.
    Introduction to Health Physics, H. Cember and
    T.E. Johnson, 4th Edition (McGraw Hill)
    MSc-REP Regan Dosimetry 3
    Some Useful Web Pages
    Dosimetry definitions etc.
    • http://www.physics.isu.edu/radinf/terms.htm
    • http://www.hps.org/publicinformation/radfactsheets/
    Also, good notes on basic dosimetry terms etc. can be found at
    • http://www.physics.mtsu.edu/~phys2020/index.html (chapter 11)
    •http://www.physics.isu.edu/radinf/index.html
    International Commission in Radiation Protection (ICRP) web site
    • http://www.icrp.org/
    Stopping powers, attenuation coeffs of x-rays, e-s, ps & ?s
    from the USA National Institute for Standards and Technology
    • http://physics.nist.gov/PhysRefData/contents-radi.html
    • http://physics.nist.gov/PhysRefData/XrayMassCoeff/
    (see also Seltzer Radiation Research 136 (1993) p147)
    • http://www.nist.gov/physlab/data/xcom/index.cfm
    •http://www.srim.org/ (for charged particles)
    MSc-REP Regan Dosimetry 4
    Relationship Between Detectors
    and Dosimetry
    – Physical and Chemical Effects of Ionising
    Radiation.
    – General Concepts and Units.
    – Radiation Quantities and Definitions
    – Absolute Methods of Dosimetry
    MSc-REP Regan Dosimetry 5
    Physical and Chemical Effects of
    Ionising Radiation
    Incident ionising radiation can cause the following effects on matter
    (which can, therefore conversely be used to measure the amount of
    radiation imparted):
    • Ionisation (i.e., electrons removed from atoms)
    • Excitation (atoms/molecules raised to excited states)
    • Chemical effects (changes in the structure of molecules which
    can lead to molecular disassociation resulting in biological changes).
    • Radiation damage to the crystalline structure in solids.
    • Thermal effects (radiation causes increase in temperature)
    • Nuclear excitations and/or transmutations.
    MSc-REP Regan Dosimetry 6
    Radiation Damage in Biological Systems
    • In biological organisms, radiation damage occurs due to the
    ionisation of atoms and molecules in cells.
    • The production of ions can result in chemical reactions which break
    molecular bonds in proteins and other important biological molecules.
    • Typically 1-> 40 eV of energy is needed to ionize a molecule or
    atom, thus radiations such as ?, ? and ?, which can have energies in
    the 100keV to few MeV range, can individually result in the
    ionisation of thousands of atoms or molecules.
    • Biological damage can subsequently result either by cells being
    killed or mutating (which can result in cancer). A large enough dose
    will destroy sufficient numbers of cells to kill the organism.
    MSc-REP Regan Dosimetry 7
    There are 2 main types of radiation damage in biological systems:
    Somatic Damage (also known as ‘radiation sickness’): This refers
    to damage to cells which are not associated with reproduction.
    The degree of somatic damage depends on the organ exposed and the
    age of the individual (younger = more susceptible to somatic damage).
    Effects of somatic damage include:
    • reddening of the skin,
    • hair loss,
    • ulceration,
    • reduction of white blood cells,
    • cataracts in the eyes,
    • fibrosis of the lungs.
    Genetic Damage: This refers to damage to cells associated with
    reproduction which can lead to genetic mutations in the offspring.
    MSc-REP Regan Dosimetry 8
    Some Terms Related to Dose
    • Chronic Dose: dose received over an extended period of time.
    • Acute Dose: dose received in a short period of time.
    • Somatic Effects: effects seen in an individual exposed to the dose.
    • Genetic Effects: effects in the offspring of the individual exposed
    to the radiation due to a pre-conception exposure of the offspring.
    • Teratogenic Effects: are effects in the offspring of the individual
    who experienced the dose during gestation.
    • Stochastic Effects: are effects which occur on a random basis.
    Such effects have no effective threshold, but the chances of such
    an effect are increased with dose. Cancer is a stochastic effect.
    • Non-Stochastic Effects: can be directly related to the size of the
    dose received. They often have a dose threshold below which the
    effect does not occur. Skin burning from radiation is a non-
    stochastic effect.
    MSc-REP Regan Dosimetry 9
    Basis of Detector/Dosimetry Systems
    Dosimetry/radiation detection systems can then be designed and
    operated using these effects. Basic systems include,
    • Calorimetry, based of thermal effects and increases in temperature.
    This provides the most basic and accurate ‘primary standard’.
    • Chemical dosimeters, based on chemical effects and molecular
    changes, a good and accurate, ‘secondary standard’
    • Ionisation chambers - electronic ionisation.
    • Proportional Counters/Geiger-Mueller detectors - electronic
    ionisation and atomic/molecular excitation in a gas medium.
    • Semiconductor detectors (silicon, germanium, CdTe) - ionisation
    MSc-REP Regan Dosimetry 10
    Basis of Detector/Dosimetry Systems (cont.)
    • Scintillation counters (e.g., NaI(Tl), BaF2) - scintillation light emitted
    following molecular excitations. (see Knoll p221, p231)
    • Solid state integrating dosimeters - radiation damage in solids
    • Photographic methods - radiation damage in solids
    • Solid state track detectors - radiation damage in solids
    • Activation detectors - nuclear transmutation (for neutrons usually
    via (n,?), (n,p) or (n,?) reactions).
    Slow (thermal) neutrons detection can use (see Knoll p483ff & 707 ff)
    10B(n,?) 7Li (Q=2.310, 94%, E(7Li) = 0.84 MeV, E(?) = 1.47 MeV).
    6Li(n,?)3H (Q=4.78 MeV, E(3H) = 2.73 MeV, E(?) = 2.05 MeV)
    55Mn(n,?)56Mn T1/2=2.6h ; 59Co(n,?)60Co T1/2=10.4min & 5.3y ;
    109Ag(n,?)110Ag, T1/2=24secs; 164Dy(n,?)165mDy, T1/2=1.3mins .
    Threshold activation detectors (for fast neutrons) include
    59Co(n,?)56Mn, T1/2=2.56h ; 23Na(n,?)20F (in a NaI(Tl) detector)
    MSc-REP Regan Dosimetry 11
    FromKnoll p707
    MSc-REP Regan Dosimetry 12
    From Knoll p708
    MSc-REP Regan Dosimetry 13
    From Knoll p709
    MSc-REP Regan Dosimetry 14
    Definitions, Quantities and Units (Alpen p5ff)
    Exposure (X): The exposure is defined as the ratio of the charge
    (of one sign) ?Q produced in a medium when all the electrons
    liberated by photons in the volume element of the medium with mass
    ?m, are completely stopped in the volume. Thus
    The (old) unit of exposure is the Roentgen (R) .
    The natural SI unit for exposure would be C/Kg
    but is never used. 1 Roentgen = 2.58x10-4 C/Kg (see later, ‘KERMA’)
    m
    QX
    ?
    ?
    =
    The Roentgen was originally defined at a 1928 conference as
    ‘ …the quantity of X-radiation which, when secondary electrons are
    fully utilised and the wall effect of the chamber is avoided, produces
    in 1cm3 of atmospheric air at 0oC and 76cm of mercury pressure
    such a degree of conductivity that 1 electrostatic charge is measured
    at saturation current’. (Air was chosen as a standard medium since
    air/gold leaf ionisation chambers were standard equipment).
    Exposure only applies to X- and ?-rays, not p, ?, n, e- etc.
    MSc-REP Regan Dosimetry 15
    The W-value for electrons in air (i.e., average incident energy required
    to produce a single effect) is 33.7eV per ion pair, (= 33.7 J/C).
    The absorbed dose in air at normal STP which is subjected to
    an exposure of 1 roentgen is 87 erg per gram.
    In soft tissue, 1 roentgen = 98 erg per gram i.e. approximately 1 rad
    This is true for most low -Z (atomic number) materials such as
    air, soft biological tissue, plastics etc.
    The definition of exposure is only for X and ? rays. The more
    general use of absorbed dose is a more useful concept.
    Exposure measurements when used have units of ‘air-KERMA’
    from Kinetic Energy Release in Medium (A), see later.
    MSc-REP Regan Dosimetry 16
    Dose and Absorbed Dose (D): is the energy deposited,
    ?ED by ionising radiation to a mass, ?m of matter
    in a given volume element. m
    ED D
    ?
    ?
    =
    The standard unit of absorbed dose was the rad (plural also is rad),
    where 1 rad = 100 erg per gram.
    The SI unit for absorbed dose is the gray (Gy) , 1 Gy = 1Joule / kg.

    The conversion between grays and rad is 1 Gy = 100 rad
    Thus, 1 rad =0.01Gy = 1cGy (‘centrigray’) which is also used.
    10Gy would constitute a lethal whole body dose in a human.

    MSc-REP Regan Dosimetry 17
    Energy Imparted (?ED): is the difference between the sum of the
    energies of all the directly and indirectly ionising particles which
    have entered a volume element of mass ?m, given by ?EE and the
    sum of the energies of all those which have left the volume (corrected
    for any changes in rest mass, ?ER, which have taken place due to
    nuclear reactions within the volume element).
    RLED EEEE ?????=?
    The SI unit for the energy imparted is the gray (Gy).
    MSc-REP Regan Dosimetry 18
    Equivalent Dose ( HT )
    The human equivalent dose, HT measures the biological damage to a
    human due to exposure to a particular type of radiation.
    It is defined by HT = WR x DT , where T represents a specific tissue or
    part of the body. H is also called the ‘radiation-weighted dose’
    The SI unit for human-equivalent dose is the sievert (Sv).
    1 Sv = 1 gray x WR
    The traditional unit for human-equivalent dose is the rem, where
    1 rem = ‘Roentgen Equivalent Man’ = dose in rad x Q = 0.01 Sv.
    Typical values are (milli-rems and 10s of micro-sieverts.
    Often the body can be exposed to different types and energies of
    radiation at the same time. Then the human-dose equivalent is given
    by
    the weighted sum of absorbed doses of
    radiation of type R, resulting in the
    observed biological damage to tissue/organ, T.
    RT
    R
    RT DWH ,×= ?
    MSc-REP Regan Dosimetry 19
    Quality/Weighting (‘Q/WR’) Radiation Factors,
    ICRP radiation weighting (W) factors.
    MSc-REP Regan Dosimetry 20
    Example
    A patient has a chest x-ray. The area of the chest exposed to the x-ray
    beam is approximately 500 cm2 and the intensity of the x-ray beam is
    0.3 W/m2. The patient is exposed for 0.2 seconds. Hospital regulations
    state that the absorbed dose must be kept below 0.0020 Gy.
    a) What is the power of the beam to which the patient is exposed ?
    b) What is the maximum human-equivalent dose for the patient ?
    ( )
    public). for the ICRP by thelimit annual drecommende the twice(i.e.
    2mSv0.002Sv dose equivalenthuman max. thusrays,-for x 1Q (iii)
    0.002Gykg0.003J/1.5 senergy/mas Dose (ii)
    Kg5.10.002Gy
    0.2s0.015W mass min. mass min.
    s 0.2 W 0.15 0.002Gy
    Gy 0.002 below dose absorbed keep to tissueof mass Minimum (i)
    0.003JJ 0.2 x 0.015 mepower x ti beamby impartedEnergy b)
    0.015W Power 0.0001mm)01.0(1cm
    0.05m3.0cm5003.0 )area(m )W/mIntensity( (J/s)Power a)
    2222
    2222
    ===
    ===
    =
    ×
    =?
    ×
    =
    ===
    =?==
    ×=×=×=
    MSc-REP Regan Dosimetry 21
    Relative Biological Effectiveness (RBE): The RBE of a particular
    radiation is the ratio of the absorbed dose of a reference radiation DR
    (which is often taken to be gamma-rays from a 60Co source or 250kV
    X-rays) to the absorbed dose of the particular radiation which is begin
    examined, DX, in order to attain the same level of biological effect.
    X
    R
    X D
    DRBE =
    RBE is related (but not identical) to the quality factor, Q (which is
    equivalent in most cases to WR) in the measurement of dose equivalent.
    MSc-REP Regan Dosimetry 22
    Effective Dose (HE)
    The same size of dose can cause different degrees of biological
    damage depending on which part/organ of the body is exposed.

    In order to account for this, the ICRP (publication number 60, 1990)
    provided a list of Tissue Weighting Factors, (WT) for the organs and
    tissues which are susceptible to the main biological radiation damage.
    ? ×=
    T
    TTE HWH
    The Effective Dose (HE) is a way of determining the
    whole-body biological damage due to radiation exposure of different
    types to different types of the body. This is given by the weighted
    sum of the equivalent dose for that type of radiation, multiplied by the
    tissue weighting factors for that particular area of the body, HT.
    Thus
    Note HE and HT both have SI units of sieverts (Sv).
    MSc-REP Regan Dosimetry 23
    The total sum of weighting factors = 1.00
    MSc-REP Regan Dosimetry 24
    The weighting factor, WT
    for an organ is given by
    the risk to that organ
    divided by the total risk.
    The weighting factors are
    given by the lifetime risk
    coefficient divided by the
    total risk.
    Thus, the weighting factor for
    fatal gonad cancer would
    be 1.33/7.25 = 0.18 in the
    general population and
    0.80/5.53= 0.14 for
    occupational radiation workers.
    Alpen p430
    MSc-REP Regan Dosimetry 25
    ICRP Recommended Annual Dose Limits
    Body Part Occupational General Public
    Whole body
    (HE)
    20mSv 1mSv
    Eye lens (HT) 150mSv 15mSv
    Skin (HT) 500mSv 50mSv
    Hands & Feet
    (HT)
    500mSv ---------
    Note these recommended limits EXCLUDE any medical or natural
    background radiation doses.
    MSc-REP Regan Dosimetry 26
    Some More Definitions…
    Particle Fluence (? ): is the number of particles, ?N which enter a
    sphere of cross-sectional area a, such that ?=?N/?a.
    ? has units of particles/m2.
    Particle Fluence rate (?) : is the rate of particle fluence with respect
    to time. ? = ?? / ?t and thus ? has units of particle/m2s.
    Energy Fluence (? ): is related to the particle fluence. It is defined
    by ? = ?Ef / ?a, where ?Ef is the sum of the particle energies
    which enter a cross-sectional area, ?a. Units are Joules/m2
    Energy Fluence Rate (?): is the quotient of the energy fluence with
    respect to time, i.e., ?= ?? / ?t . Units are Joules/m2s.
    MSc-REP Regan Dosimetry 27
    KERMA (Alpen p8, p90)
    Typically, when radiation (x-rays, ? rays and charged particles)
    interact with their environment, they transfer kinetic energy to
    the medium in which they are interacting.
    It is possible however, that not all of the transferred kinetic energy
    remains in the volume of interest. This can be due to radiative
    losses (bremsstrahlung) and kinetic energy losses associated with
    secondary particles produced.
    KERMA is the Kinetic Energy Release in the Medium (A is added!)
    Kerma, (K) accounts for the energy transferred to
    the volume (without correcting for energy losses
    after interaction). It is defined by the expression,
    where ?EK is the sum of initial kinetic energies of all the charged
    particles liberated by ionising particles or photons in a volume
    element of a specific material. Kerma is thus reflects the energy
    RELEASED in a medium. Kerma has the SI unit of the gray (Gy)
    m
    EK K
    ?
    ?
    =
    MSc-REP Regan Dosimetry 28
    Charged Particle Equilibrium (CPE) : Charged particle equilibrium
    is said to exist at a point p, centred in a volume V, if each charged
    particle carrying out a certain energy from this volume is replaced
    by another identical particle which carrying the same energy into the
    volume.
    If CPE exists at a point, the dose = kerma (D = K) at that point
    (provided that the secondary radiation losses by the charged
    particles such as bremsstrahlung are negligible).
    Dose is the energy absorbed in the unit volume,
    while
    kerma is the energy transferred from the original particle (or photon)
    in the same unit volume.
    MSc-REP Regan Dosimetry 29
    Absolute Methods of Dosimetry
    Absolute methods of dosimetry can provide measurements for the
    absorbed dose without the instrument (‘dosemeter’) being calibrated
    in a known radiation field. (Most instruments give measurements
    relative to calibrated primary or secondary standards).
    It is however possible to calibrate certain detector media which
    can then be placed inside the sensitive volume of specific dosemeters.
    These instruments then posses an effective ‘internal calibration’ and
    as such can be described as absolute dosemeters.
    For any radiation phenomenon (e.g., gammas neutrons etc.) to be used
    for radiation dosimetry, we need to know
    1) the fraction (?) of the absorbed dose (D) which is channelled into
    a given effect, and
    2) the average energy (H) needed to produce a given effect (e.g.,
    ionisation, chemical changes, nuclear reactions etc.)
    MSc-REP Regan Dosimetry 30
    Thus, the energy per unit mass going to any specific effect = ?D.
    If this causes Ne subsequent effects per unit mass, and the average
    energy required to produce the unit effect is H, then the total energy
    required is the product of Ne and H, ie. Ne.H = ?D
    Thus, since D = (H/?).Ne, ,, if (H / ?) is a constant and known, the
    number of effects induced by the radiation (Ne) is proportional to the
    absorbed dose. Thus the dose can be obtained by measuring Ne.
    Consider a charged particle of energy E, coming rest inside a medium.
    If a fraction ?i of the particle’s kinetic energy produces ionisation
    in the medium, assuming that the energy required to cause ionisation
    by radiation induced collisions is Hi, we have ?iE=Ni Hi and the
    number of ions produced is Ni=(?i.E)/Hi .
    Now, (E / Ni)=(Hi / ?I) is the average energy required to produce one
    electron-ion pair, which is known as the W-value.
    (NOTE, This is NOT the same as WR mentioned earlier).
    MSc-REP Regan Dosimetry 31
    Therefore, ii
    i
    i
    i
    i
    i
    NNHHN .WD W
    E
    =???
    ?
    ???
    ?
    =?== ??
    Thus, if we know W, we have the calibration factor (Hi / ?i) without
    having to know Hi or ?i individually.
    In the case of dosimetry based on calorimetry, Ht is the energy required
    to raise the temperature of a unit mass of the radiation absorber by 1K,
    which is also the definition of the specific heat, S of the material.
    Here the ‘measured effect’ is the temperature rise in degrees kelvin
    which is caused by the induced radiation.
    ( )
    energy. absorbed theof 13% is energy) thermal
    -(nonoutput light thesince 87.0 NaI(Tl)For .1 cases,most In
    energy. thermalinto converted is which dose theoffraction
    theis and massunit per input energy thermal theis where
    D D and Thus,
    tt =?
    ??
    ?×???
    ?
    ???
    ?
    =???×=??=?=
    ??
    ?
    ??
    t
    t
    te
    mQ
    TSTSmQTN
    MSc-REP Regan Dosimetry 32
    Radiation Equilibrium
    C
    V V’(?m)
    A
    B
    C
    P
    d
    Consider a volume, V, uniformly filled with radioactive material.
    Inside this volume, V, is a smaller secondary volume, V’ (containing
    mass, ?m) which surrounds the point P. The shortest distance between
    the boundaries of V and V’ is given by d.
    The radiation coming from points
    in and around V’ must be in one
    of three categories:
    i) Type A tracks: spend all their
    energy (their entire ‘life history’)
    inside V’.
    ii) Type B tracks: originate inside V’
    but give up part of their energy outside; &
    iii) Type C tracks: start outside V’ but give up some energy inside.
    MSc-REP Regan Dosimetry 33
    If the distance d, is
    larger than the maximum range
    of the ionising radiation being
    considered (neutrinos are usually
    neglected), then there is a
    complete symmetry in the region V’.
    This means, on average (i.e. for
    large numbers of radiation tracks),
    the tracks of type B and C will
    balance out and the energy removed
    from V’ by type B tracks will be
    compensated by the energy deposited into V’ by tracks of type C.
    In these conditions, RADIATION EQUILIBRIUM is said to exit in V’.
    C
    V V’(?m)
    A
    B
    C
    P
    d
    MSc-REP Regan Dosimetry 34
    A more complete definition of absorbed dose is given in Radiation
    Dosimetry volume 1 (1968) pp 32-33, edited by Attix and Roesch.
    ‘ The energy imparted to matter by ionising radiation per unit mass
    is called the absorbed dose. By energy imparted to matter, we mean
    that which appears as ionisation or excitation, increase in chemical
    energy or crystal lattice energy etc. in the material. The energy that
    goes into changes in rest mass of the material or in the radiation itself
    (pair production) is excluded by definition; in some cases this energy
    can be comparable with absorbed dose, but does not produce
    important extra-nuclear effects .’
    Thus, the energy absorbed can be split into 2 components, causing:
    1) changes in atomic/molecular/lattice energy states and
    2) changes in the rest mass.
    MSc-REP Regan Dosimetry 35
    Thus, by conservation of mass energy, the energy imparted to matter
    in the volume element V’ is given by ?ED = ?EE - ?EL - ?ER
    If there is RADIATION EQUILIBRIUM then ?EE = ?EL and
    so,
    ?ED = - ?ER and thus the absorbed dose, D = ?ED / ?m
    The dose imparted to V’ thus arises from the reduction in the rest mass
    of the radionuclides within V’ following their decay to create the
    ionising decay products. (The energy removed by neutrinos following
    ?-decay is excluded since their absorption is vanishingly small).
    C
    V V’(?m)
    A
    BC P
    d
    Consider the point, P, within the volume V’.
    ?EE is the sum of the total energies of all
    the ionising radiations entering V’.
    ?EL is the sum of the total energies
    of ionising radiations leaving V’; and
    ?ER is the increase in rest mass inside V’.
    MSc-REP Regan Dosimetry 36
    [ ] [ ]
    [ ] [ ]intint
    int
    intintint
    int
    , thereforeand
    then exists, mequilibriuradiation If

    dose, totalThe
    R
    ext
    RE
    L
    ext
    L
    ext
    E
    RLE
    ext
    R
    ext
    L
    ext
    E
    D
    ext
    D
    EEED
    EEE
    EEEEEED
    EED
    ?+???=
    ?+?=?
    ???????????=?
    ?+?=
    True radiation equilibrium only occurs in the
    highly symmetric case (as described above), but
    it can be useful to consider some approximations.
    If we consider flows of radiation energy into
    and out of a unit mass from both internal
    and external radiation sources, then
    i.e the Dose (D) is the
    energy from the loss in rest mass following radioactive decay minus
    any increase in rest mass from external & internal radiation interactions,
    or put another way
    Dose = [decrease in rest mass] - [Increase in rest mass]
    ext
    EE?
    ext
    LE?
    ext
    DE?extRE?
    int
    EE?
    int
    RE?
    int
    DE?
    ext
    LE?
    MSc-REP Regan Dosimetry 37
    [ ] [ ]
    [ ]
    achieved.not is mequilibriuradiation perfect and absorbed isradiation
    incident theofpart only since positive bemust where


    ext
    L
    ext
    E
    ext
    R
    ext
    L
    ext
    E
    EE
    EEED
    ?+?
    ???+?=
    Therefore, the absorbed dose equals the net reduction in rest mass
    (neglecting neutrino energy) per unit mass of material.

    If there are no internal sources of energy, (for example, if the material
    is only irradiated by external sources), then
    Note that for photon energies less than 1.022 MeV (the e+e- production
    threshold), there are essentially NO CHANGES in REST MASS and
    thus .
    In this case, the absorbed dose arises from the difference between the
    energy entering the volume and that leaving it.
    0=? extRE
    MSc-REP Regan Dosimetry 38
    Charged Particle Equilibrium
    X-ray and ?-ray photons, and neutrons are uncharged. As such, they
    are described as INDIRECTLY IONISING RADIATIONS since
    they deposit their absorbed dose in matter by a 2-step process:
    1) Kinetic energy is transferred to charged particles (e.g., via recoil
    electrons for photons or nuclear reactions products for neutrons).
    2) These charged particles subsequently deposit energy in the medium.
    If each charged particle carrying energy out of V’ is balanced by
    an identical particle carrying the same amount of energy into the
    same volume element, CHARGED PARTICLE EQUILIBRIUM
    is said to exist inside V’.
    MSc-REP Regan Dosimetry 39
    ( ) ( )[ ] ( ) ( ) ( )[ ]uRuLuEcLcED EEEEEE ?????+???=?
    ( ) ( ) ( ) ( )[ ]
    ( ) ( ) ( )[ ]uRuLuED
    c
    L
    c
    E
    c
    L
    c
    E
    EEEE
    EEEE
    ?????=?
    =????=?

    giving 0 , thus
    If a volume element is irradiated by an external source, considering the
    energy carried in to and out of V’ by
    (i) charged (c) (e.g., electrons, positrons, alphas, fission fragments; and
    (ii) uncharged (u) particles (mainly photons and neutrons), then:
    Note that there is no ‘rest mass’ term (?ER) in the first square bracket
    about since electrons and photons cause virtually no rest mass changes
    in the normal expected energy ranges for these radiations.
    If CHARGED PARTICLE EQUILIBRIUM (CPE) exists, then
    Thus, in effect, for CPE, the dose is delivered by the
    UNCHARGED FLUX, and is equal to the net energy left inside
    in the absorber, minus any changes in the rest mass.
    MSc-REP Regan Dosimetry 40
    If the mass of the material encompassed by the volume element V’ is
    given by ?m, then D = (?ED / ?m) = (?EK / ?m) = K,
    where K = KERMA, the energy released per unit mass.
    Thus, in CPE, D=K, i.e. DOSE = KERMA
    It is now common practice to refer to kinetic energy transfer to charged
    particles and to replace ?EK with ?Etr .
    CPE is always present when radiation equilibrium occurs, but in
    many practical cases, CPE is closely attained, even though radiation
    equilibrium is not. For electrons we speak of ‘electronic equilibrium’.
    Then under Charged Particle Equilibrium (CPE) conditions, ?ED=?EK
    ( ) ( ) ( )[ ]uRuLuED EEEE ?????=?
    ( ) ( ) ( ) ( ) ( ) ( )uRuLuEKuRKuLuE EEEEEEEE ?+???=?????=???
    This result can be interpreted alternatively as:
    The net energy brought into the medium by uncharged radiations
    supplies kinetic energy (?EK) to charged interaction products, and
    also any accompanying rest mass changes. Thus we can write,
    Recalling (p40) that
    MSc-REP Regan Dosimetry 41
    Consider the case of a broad,
    parallel beam of photons
    which travel through vacuum,
    perpendicular to the surface of
    an ‘infinite’ absorptive medium.
    As the photons interact in
    successively deeper layers of
    the absorptive medium
    progressively further from the
    surface, the overlapping tracks of the recoil electrons will deliver an
    increasing dose to the material.
    This dose build up continues to a depth that can just be reached by
    those electrons which are emitted from the surface radiation
    interactions and thus the width of this ‘build-up region’ is equal to the
    maximum range of the recoil electrons in the medium.
    MSc-REP Regan Dosimetry 42
    The absorbed dose falls off slowly with depth from
    the surface as the photon flux is absorbed in the
    medium. There is also a finite dose from recoil
    electrons and backscattered photons originating
    from inside the medium.
    The primary flux transferred to kinetic energy
    of recoil electrons is maximised at the SURFACE,
    thus the KERMA is also maximised at this point.
    • Beyond the build-up region, the KERMA and DOSE curves lie close together since
    electronic equilibrium can be closely approximated in this region.
    • The D (dose) curve is shifted slightly ‘downstream’ relative to the K (kerma)
    curve by about the average recoil electron range, since their kinetic energy delivers
    dose to the medium along their tracks as they slow down.
    • There is an opposing effect due to the emission of bremsstrahlung by the electrons as
    they slow down in the medium (in low-Z stoppers, this is a small effect). However, the
    longer range of the bremsstrahlung photons compared to the e- s means that they often
    escape the region of interest and do not contribute to the local dose. Bremsstrahlung
    effects are usually neglected in the detailed definition of exposure in air.
    • The contemporary replacement for ‘exposure’ is ‘air-kerma’ which is almost equal
    to the dose in air under CPE conditions. The air dose can be measured directly from
    the output of an air-walled ion chamber.
    MSc-REP Regan Dosimetry 43
    ( ) ( )
    event.n interactioper nsferredenergy tra average theis
    andevent n interactioper absorbedenergy average theis
    material.absorber theofdensity theis andt coefficienn attenuatio total theis
    fluence, particle theis where, and
    trav
    abav
    travabav
    E
    E
    a
    NEKED

    ?
    µ
    ?
    µ
    ?
    ?
    =??=?=
    (from Alpen p 91)
    For fast electrons, D and K can also be defined in terms of the incident fluence
    MSc-REP Regan Dosimetry 44
    A radiation energy fluence E, (in units of Jm-2) of photons passing
    through an absorber falls off exponentially with increasing depth,
    (after build-up to CPE). That is E(x)=Eoexp(-µenx) - (1), where
    µen is the linear energy absorption coefficient, and x is the depth
    (or linear distance through the medium).
    ( )
    absorber. theof surface thefrom Similarly,
    maximum. buildup dose thebeyondregion CPE in the
    ,mass
    energy
    length
    1
    length
    Joules
    mass
    length of dimensions has 1
    .1 gives, density massabsorber by the gMultiplyin
    1- exp (1), atingDifferenti
    2
    3
    0
    EK
    ED
    Ddosedx
    dE
    E
    dx
    dE
    Edx
    dEExEdx
    dE
    tr
    en
    en
    enenenen
    ?=
    ?=?
    ?=????
    ???
    ?
    =??
    ???
    ?
    ?
    ?=??=??=
    ?
    µ
    ?
    µ
    ?
    ?
    µ
    ?
    ?
    µµµµ
    Mass Energy Absorption Coefficients
    MSc-REP Regan Dosimetry 45
    ( ) ( )xIxIIdx
    dI µµ ?=???= exp 1 0
    Note µen/? = mass energy absorption coefficient [units of cm2.g-1]
    and µtr/? = mass energy transfer coefficient [units of m2.kg-1]
    The two coefficients can be
    obtained from the slopes of the
    dose-depth and kerma-depth
    curves respectively, and are both
    very closely related (but not
    identical!) to the underlying mass
    attenuation coefficient.
    For a photon fluence I, which enters a small absorber element of
    thickness dx in which the fluence is reduced by an amount dI, the
    LINEAR ATTENUATION COEFFICIENT (µ) is given by
    The mass attenuation coefficient is defined by (µ /? ) ,
    where ? is the density of the absorber material
    MSc-REP Regan Dosimetry 46
    Edx
    dE?Idx
    dI?
    I
    dI
    E
    dEE
    EdIdEEIE
    ?
    1 n,subsitutioby 1 Since
    . ,for ngsubstituti Thus,
    ating,differenti ,
    ??=??=
    ?=?
    ×=×= ??
    The energy fluence carried by the photon beam given by the photon
    fluence multiplied by the photon energy, ie.
    This look very similar to the definition of the linear energy absorption
    coefficient µen (see p45), but while µ describes photons (and the
    energy which they carry) which are removed from the primary photon
    beam, µen describes the energy absorbed in the medium.
    µen is always smaller than µ since there are other effects which can
    remove photons in the beam which do not necessarily impart energy
    (e.g., bremsstrahlung, fluorescence, X-rays, Compton scattered photons
    and pair production/ annihilation radiation.).
    MSc-REP Regan Dosimetry 47
    ( )
    ( ) ( )gg
    (g)
    E
    cm
    f
    E
    cm?-f?E
    ???
    tr
    tr
    ?
    s
    ?
    ppsc
    ?
    petr
    ppc
    ?=?=
    =
    =
    ???
    ?
    ???
    ?
    ?++???
    ?
    ???
    ?
    ?=
    ++=
    +
    1 and 1 thus,
    further coeff. absorptionenergy thereduces This dose. local the tocontribute
    not does and lungbremsstrah of form in the radiated-re is electrons recoil
    toed transferrisch energy whi kinetic theof fraction, small) (typicallyA
    radiation. eeby en energy takincident theoffraction )MeV022.1(2
    photons scattered by the taken collisionsCompton in fraction energy theis
    ; rays-X sticcharacteri theofenergy mean theis where
    2111 t,coefficiennsfer energy tralinear
    theeach term, torelatedradiation secondary escapefor allow weIf
    by given ist coefficienn attenuatiolinear The
    en
    en
    -
    2
    0
    2
    0
    pe
    ?
    µ
    ?
    µµµ
    ?
    µµµµ
    The linear attenuation coefficient can be reduced to allow for the escape
    processes to give an expression for the LINEAR ENERGY TRANSFER
    MSc-REP Regan Dosimetry 48
    Mass energy absorption
    coefficients
    µen < µ
    511keV
    Pair-Production
    e-
    e+
    brem
    brem
    511keV
    brem
    Compton scattering
    e-
    Compton scatter
    Photo-electric effect
    e-
    brem
    K? etc
    brem = bremsstrahlung
    MSc-REP Regan Dosimetry 49
    Mass attenuation coefficients for (A) Lead and (B) Water.
    Taken from Alpen, p81-82.
    MSc-REP Regan Dosimetry 50
    Relationship between air-kerma, exposure & absorbed dose in air
    Consider an electron of K.E. Te, induced in air by photon interactions, which is
    brought to rest inside unit mass of air. A fraction, g, of this energy escapes from the
    sample in the form of bremsstrahlung radiation.
    Hence the energy absorbed in unit mass of air, (i.e. absorbed dose) is given by:
    Dair = (1 - g)Te.
    This produces Ni ion pairs in this unit mass and an additional gNi ion pairs externally due to
    absorption of the escaping bremsstrahlung, giving a total of (1 + g)Ni ion pairs at a total
    energy cost of Te.
    Therefore, from the definition of W-value, we can write We = Te/(1 + g)Ni and thus:
    Te = WeNi(1 + g).
    Substituting for Te in the expression for the dose given above:
     
    Dair = (1 - g).WeNi(1 + g) = WeNi(1 - g2)
    Since Te = WeNi(1 + g) and remembering that air-kerma, Kair, is defined as the initial kinetic
    energy transferred per unit mass of air then
    Kair = Te = WeNi(1 + g) and thus Kair = Dair/(1 - g).
    MSc-REP Regan Dosimetry 51
    The relative importance of the three major types of gamma-ray
    interaction. The lines show regions of gamma-ray energy and the Z
    (atomic number) of the absorber material for which the two
    neighbouring effects are equal. Taken from Knoll p. 54
    MSc-REP Regan Dosimetry 52
    Worked Example:
    A 8 MeV photon penetrates into a 200g mass of tissue and
    undergoes a single, pair production interaction.
    Both the e+ and e- particles created in this interaction dissipate all
    their kinetic energy within the mass through secondary ionisation
    and bremsstrahlung production.
    Two bremsstrahlung photons of energy 1.1 and 2 MeV
    respectively are produced and escape from the mass without further
    interaction.
    The positron, after expending all its kinetic energy
    interacts with an ambient electron within the mass and they mutually
    annihilate.
    Both photons created in the annihilation radiation escape the mass
    before further interaction.
    Calculate
    (i) the kerma and
    (ii) absorbed dose the tissue receives from these interactions.
    MSc-REP Regan Dosimetry 53
    ANSWER:
    Kerma is the sum of initial kinetic energies per unit mass of all charged
    particles produced by the radiation.
    In this case, this is the kinetic energy of the e+e- pair released, which is 6.978
    MeV
    (i.e. 8MeV- the rest masses of the electron and positron created (1.022 MeV)).
    This is split evenly between the two particles such that they each have 3.489
    MeV.
    This is the sum of the initial kinetic energies.
    The Kerma = KE released / mass of the tissue volume, and thus
    GykgJkgg
    J
    dm
    KEreleasedKerma 1212
    13
    106.5/106.52.0200
    106.1978.6
    ??
    ?
    ×=×=
    =
    ××
    ==
    MSc-REP Regan Dosimetry 54
    Absorbed Dose is defined as the energy absorbed per unit mass.
    In this case, from the 8 MeV photon, an initial 6.978MeV of Kinetic Energy is
    released
    in the medium by the initial pair production interaction.
    This is followed by losses from the material of 1.1+2=3.1 MeV from the
    bremsstrahlung interactions of the electron formed in the pair production
    interaction.
    and 2 annihilation photons (1.022 MeV), all which escaped from the mass.
    Thus of the initial energy interacting with the mass of 8 MeV, 4.122 MeV is not
    absorbed in this tissue volume and thus, including the change in rest mass of the
    tissue
    volume (from the creation of the e+e- pair = 1.022 MeV), the absorbed dose is
    given by ( ) Gykg
    J
    kg
    MeVMeV
    dm
    dEDose 12
    13
    101.32.0
    106.1878.3
    2.0
    122.48
    ?
    ?
    ×=
    ××
    =
    ?
    ==
    Answer (cont).
    MSc-REP Regan Dosimetry 55
    Mass energy absorption
    coefficients
    A photon source placed between two semi-infinite
    absorbers
    S
    1 2
    CPECPE
    MSc-REP Regan Dosimetry 56
    Mass energy absorption
    coefficients
    The energy fluence, E, passing through both absorbers is the
    same ( ) ED en ?= 11 / ?µ ( ) ED en ?= 22 / ?µ
    ( )
    ( ) 11
    22 /
    / DD
    en
    en
    ?=


    ( )
    ( ) 1
    221 /
    /


    en
    enS =? D2 = 1S2.D1 where
    MSc-REP Regan Dosimetry 57
    1
    22
    11
    2
    11
    1
    2
    2
    2
    2
    1
    1
    where , thereforeand
    and regions, CPE In the
    ???
    ????
    ?
    ???
    ????
    ?
    ==?
    ???
    ????
    ?
    ???
    ????
    ?
    =
    ????
    ????
    ?
    =????
    ????
    ?
    =
    ?
    µ
    ?
    µ
    ?
    µ
    ?
    µ
    ?
    µ
    ?
    µ
    en
    en
    en
    en
    enen
    SDSDD
    EDED
    PConsider a photon source placed
    midway between 2 ‘infinite’ absorbers.
    The energy fluence E (in Jm -2), passing
    through both absorbers must be the same, and thus we can write,
    Thus, in a given radiation field, the dose in one medium (such as
    biological tissue) can be derived from measurement in a second, more
    practical medium (e.g., air), if the ratio of their mass energy
    absorption coefficients is known (and if CPE is attained in both).
    D1
    (µen /? )1
    D2
    (µen /? )2
    MSc-REP Regan Dosimetry 58
    • A special case if an air-filled ion chamber is used.
    • The W-value in air is 33.7eV/ion pair.
    • Using this the absorbed dose in air corresponding to an exposure of
    X = 1 roentgen can be calculated to be 87erg.g-1 (= 0.87 rad).
    Thus, the relation to dose in ANY MEDIUM of type m, situated at
    a point where the exposure is 1 roentgen can be found using the relation:
    Dm = airSm.Dair
    Thus, Dair=0.87.airSm rad.
    More generally, for an exposure of X roentgens, the dose in rads is given
    by Dm=0.87.airSm.X rad
    or written another way, Dm=f.X rad where f = 0.87.airSm
    f is called the ‘rad per roentgen factor’.
    For photons of E?=10 keV -> 3 MeV in soft tissues (made of H,C,O
    and other low-Z elements), f = 0.92-0.97. Water has f = 0.90-0.96.
    Bone (calcium, Z=20) has f = 3.6 for 10 keV and 0.92 @ 1MeV
    MSc-REP Regan Dosimetry 59
    The dose in higher Z materials is much larger than in air (and other low-Z materials)
    for lower X-ray energies due to the strong Z-dependence of the photoelectric effect
    cross-section (?pe~Zn/E?4-5)
    The photon attenuation coefficients, and the related energy absorption coefficients
    are complex functions of E? and atomic no.(Z), but over a RESTRICTED RANGE
    of these two parameters, it is possible to represent the dosimetric behaviour of a
    mixture of elements (such as in biological tissue) with the use of a single
    parameter, called the EFFECTIVE ATOMIC NUMBER, Zeff.
    For soft tissues over the range of diagnostic X-rays ( E=10-250 keV, Zeff=7.8).
    This concept can be useful for estimating the degree of equivalence (or ‘matching’)
    between real biological tissue and possible dosimetric media.
    Although PERFECT MATCHING (i.e., 1S2=1.0) is only true for identical atomic
    compositions, approximate matching is often good enough for radiation protection
    purposes.
    For example, tissue-equivalent gas mixtures can be used inside tissue-equivalent and
    used inside natural body apertures to accurate dose measurements in radiotherapy.
    Effective Atomic Numbers and’ Matching’
    MSc-REP Regan Dosimetry 60
    Cavity Detectors
    Consider a volume of gas contained in a cavity inside a solid material which
    itself is surrounded by a third material. When CPE is attained in the cavity gas
    and in the medium surrounding the ion chamber:
    Dm = gSm Dg
    If the absorbed dose gives rise to Jg (C.kg-1) of ionisation in the gas then the
    dose in the gas is:
    Dg (J.kg-1) = Jg (C.kg-1) x wg (J.C-1)
     
    ? Dm = gSm Jg wg (Gy)
     
    In this way the dose rate in the medium of interest can be derived from the
    ion chamber current.
    If the cavity wall, the cavity gas and the surrounding medium are all well
    matched we have the homogeneous ion chamber case and gSm = 1.0.
    MSc-REP Regan Dosimetry 61
    Relationship between air-kerma, exposure and
    absorbed dose in air
    Air-dose, Dair, is derived directly from the output of an air-walled ion chamber by
    collecting all of the ionisation in the sensitive volume, dividing by the mass of air
    it contains and multiplying by We. The ionisation per unit mass is simply the
    exposure, X, so we can also write:
     
    Dair = X . We .
     
    However in SI units we express exposure not in ion pairs per unit mass but in
    coulombs per kilogram. (recall, The energy needed to produce an ion pair in air is
    33.7eV ? 33.7JC-1 (1eV = 1J * 1.6x10-19C-1)
    Thus air-dose is related to exposure by air-dose (J.kg-1) = exposure (C.kg-1) x
    We/e(J.C-1) where We is expressed in joules per ion pair and e, the electronic
    charge, is in coulombs.
     
    ? and
     
    so again kerma is slightly larger than absorbed dose in this case.
    /eWXD eair ?= ( )g
    e
    ?
    ?
    = 1
    /WXK eair
    MSc-REP Regan Dosimetry 62
    The Bragg-Gray principle says that the amount of ionization
    produced in a small gas-filled volume cavity surrounded by
    a larger, solid absorbing medium is directly proportional to
    the radiation energy absorbed by the solid.
    The gas cavity must be small enough relative to the mass of the
    solid absorber to leave the angular and velocity distributions of
    the primary electrons unchanged.
    The cavity must be surrounded of a solid with sufficient thickness to
    achieve electronic equilibrium.
    MSc-REP Regan Dosimetry 63
    Bragg-Gray Cavity Relation
    Consider a cavity of unit area and width ?x; and let the energy lost inside the
    cavity medium by an electron crossing it at right angles to the long side be ?E.
    ?xdx
    dT?E
    c
    g
    ???
    ???
    ?
    =
    electron track
    gas
    ?E
    ?xunit area ( ) xxm gg ?=?=? ??.1
    c
    gg
    g dx
    dT
    ?
    1
    ?m
    ?ED ??
    ???
    ?
    ==
    c
    gg dx
    dT
    ?
    1 ??
    ???
    ? is the mass stopping
    power for electrons.
    MSc-REP Regan Dosimetry 64
    By taking the ratio of these two expressions we find that,
    where gsm is the ratio of mass stopping powers of the medium and the cavity
    gas respectively. By measuring the ionisation per unit mass in the cavity, Jg:
    Bragg-Gray Cavity Relation
    Dg ? mass stopping power, and for the same electron fluence in the
    surrounding medium we have. c
    mm
    m dx
    dT
    ?
    1D ??
    ???
    ?
    ?
     

     
    g
    m
    gm DsD =
    gg
    m
    gm wJsD =
    MSc-REP Regan Dosimetry 65
    If a cavity ionization chamber is built with a wall material
    whose radiation absorption properties are similar to those
    of tissue, then the energy absorbed per unit mass of the wall
    material, dEm/dMm is related to the energy absorbed per
    unit mass of gas in the cavity gas, dEg/dMg by the relation:
    JwdM
    dE
    S
    S
    dM
    dE
    m
    m
    g
    g
    m
    m
    m ××=×= ?
    where Sm is the mass stopping power of the wall material and Sg is the
    mass stopping power of the cavity gas and their ratio can be written by
    m
    g
    m
    S
    S ?=
    w is the mean energy dissipated in the production of the ion-pair in the gas
    and J = number of ions pairs created per unit mass in the gas.
    MSc-REP Regan Dosimetry 66
    Example Question:
    Calculate the absorbed dose measured in a tissue-equivalent chamber
    with a 1cm3 air filled cavity within the chamber which is exposed to a
    source of 60Co gamma rays for 10 minutes.
    A total of 2.25x109 electrons are collected from the chamber as a result
    of ionization events in this period and the average mass stopping
    power ratio of tissue to air is given by:
    137.1=
    g
    m
    S
    S for 60Co gamma rays
    USEFUL INFORMATION:
    Average energy required to form an e--ion pair in air at STP = 34eV.
    1eV = 1.6x10-19J ; the density of air at STP,
    ?air = 1.293x10-6kg/cm3
    ( ) ( ) ( ) Gycmcmkg
    ionseVJeVJwdM
    dE
    m
    m
    m 0108.01/293.1
    1025.2/106.134137.1 33
    9
    19
    =
    ×
    ×
    ××××=××= ??
    SOLUTION:
    MSc-REP Regan Dosimetry 67
    Calorimetry
    1. Temperature rise ?T in a mass ?m of a material (whose
    specific heat S is known) is measured ? ?Q = ?m.S.?T
    (?m.S is the heat capacity)
    2. Null method: a measured amount of electrical energy is
    supplied to an identical "dummy" absorber to maintain it at the
    same temperature as the irradiated sample; this obviates the
    need for differential heating/cooling corrections.
    3. Latent heat method; the mass of a substance undergoing a
    change of state at constant temperature due to absorption of
    radiation energy is measured (e.g. melting of ice).
    MSc-REP Regan Dosimetry 68
    Calorimetry
    Low Temperature Calorimetry
    Calorimetry can be used for absolute calibration of the
    disintegration rate of radioactive sources. For a monoenergetic
    alpha emitter it is easy to ensure all the disintegration energy is
    contained inside the calorimeter. The rate of heat input to the
    calorimeter is equal to the energy output rate from the source.
    ?Q/?t = ?N/?t x Eav
    where ?N/?t is the disintegration rate and Eav is the average energy
    per disintegration of charged reaction products.
    MSc-REP Regan Dosimetry 69
    Calorimetry
    Example Question
    310.5 kBq of Ra-226 in 30 ml of water gave a
    temperature increase of 0.076 mK in 11 hours;
    assuming no heat losses and ignoring escaping gamma
    radiation show this corresponds to a mean
    disintegration energy of approximately 4.87 MeV, given
    the specific heat capacity of water is 4.18 kJkg-1K-1.
    MSc-REP Regan Dosimetry 70
    Example Answer
    310.5 kBq of Ra-226 emits an alpha 100% of ?N times in 11 hours:
    ?N = 310.5 x 103 x 11 x 60 x 60
    = 1.23x1010
    The total energy released is:
    ?Q = ?m S ?T
    = 0.03kg x 4.18x103Jkg-1K-1 x 7.6x10-5K
    = 0.00958J
    The energy of each emission is therefore:

    E = ?Q / ?N
    = 0.00958 / 1.23x1010
    = 7.79x10-13J
    = 7.79x10-13J / 1.6x10-19 eVJ-1
    = 4.87 MeV
    MSc-REP Regan Dosimetry 71
    Calorimetry
    Thermometry
    Semiconductors (thermistors) have temperature coefficients of
    resistance of ~ -2 to -4 % per K.
    Platinum resistance thermometers are more stable and
    reproducible but are less sensitive (~ +0.4 % per degree).
    Using thermistors, in order to measure ?T ? 10-3 K to ~ 1 % we
    need to measure resistance changes of ~ 100 parts per billion
    using a sensitive Wheatstone bridge.
    Alternatively thermocouples such as copper/constantan with ?V =
    50 µV per K can be employed and the output voltage measured
    with a potentiometer; several thermocouples in series generate a
    larger potential difference.
    MSc-REP Regan Dosimetry 72
    Calorimetry
    Low Temperature Calorimetry
    (1) Heat transfer by radiation (?T4) is reduced so that thermal
    isolation of the calorimeter from its surroundings is easier to attain.
     
    (2) Specific heat capacity decreases to give a much larger
    temperature change for a given radiation dose.
     
    (3) Thermistor sensitivity increases to ~ 10 % per K.
    In combination these improvements in sensitivity enable dose rates
    as low as ~30 mGy per minute to be measured to an accuracy
    of ?25 % in a one hour run.
    MSc-REP Regan Dosimetry 73
    Solid State Integrating Detectors
    In alkali halides, such as LiF, NaI, etc (which form simple cubic lattices) the
    outer shell electron in the alkali is donated to the halide to produce an inert
    gas like in both atoms, and produces an insulator.
    In the lattice F-centres and H-centres are regions of positive and negative
    charge which can bind to wandering electrons and holes respectively.
    Impurity (activator) atoms can be added to the lattice in interstitial positions
    to create trapping centres.
    Ionising radiation can damage the lattice if they are very energetic (recoil
    energy of ~10-20 eV is needed) or may give rise to free charges which can
    become semi-permanently trapped.
    The number of trapped charges represents some measure of the absorbed
    dose, this phenomenon is used in (a) RadioPhotoLuminescence and (b)
    ThermoLuminescence.
    MSc-REP Regan Dosimetry 74
    Radiophotoluminescence Dosimetry
    Unirradiated radiophotoluminescence (RPL) solids are not luminecence
    until they absorb ionising radiation.
    The trapped charges in RPL devices are detected and quantified by
    irradiating the dosemeter with UV light. This excites the trapped electrons
    into higher quantum states, as they fall back to the ground state they emit
    visible light. This light can then be measured with a PMT and standardised
    by calibration in a known radiation field.
    Valence band
    Conduction band
    Electron
    Trap
    Hole
    Trap
    UV light
    Visible light
    Formation Readout
    MSc-REP Regan Dosimetry 75
    Radiophotoluminescence Dosimetry
    Typical optical absorption/emission curves for an RPL glass is shown
    below.
    MSc-REP Regan Dosimetry 76
    Radiophotoluminescence Dosimetry
    The apparatus used to readout RPL glasses which are used for
    intermediate doses (10?Gy to 104Gy) is shown below.
    There are two types of RPL glass (1) high-Z barium [enhances low energy
    photon response (2) low-Z lithium or aluminium phosphate which is more
    tissue equivalent.
    RPL dosemeters are easily read-out and can be read out many times.
    RPL Glass
    PMT
    Optical filter
    (removes visible)
    UV lampUV
    Luminscence
    and UV scatter
    UV filter (removes
    scattered UV)
    MSc-REP Regan Dosimetry 77
    Thermoluminescence Dosimetry
    Thermoluminescence Dosemeters (TLD) are similar to RPLs in the way
    electrons are created and trapped. They differ in the way they are readout.
    Electron
    Trap
    Hole
    Trap
    Conduction band
    Valence band
    Formation Readout
    Mg
    Ti
    TLD
    photons
    The trapped electrons and holes (Mg sites) in TLDs are
    recombined by heating the material promoting the electrons back
    into the conduction band before recombination (Ti sites).
    MSc-REP Regan Dosimetry 78
    Thermoluminescence Dosimetry
    TLDs are readout by systems which essentially consists of a heating and
    light measurement system.
    MCS
    Current
    Integrator
    DC
    amp PM
    T
    HV
    supply
    Optical
    IR } filters
    N2 flushing gas
    Heater
    MSc-REP Regan Dosimetry 79
    Thermoluminescence Dosimetry
    As the TLD material is heated light is emitted as a series of “glow-peaks”
    A) CaSO4:Mn ;B) LiF:Mg,Ti ;C) CaF2 ;and D) CaF2:Mn. As the temperature
    rises above 200°C “black body” radiation increases. Peaks about 200°C
    are favoured.
    MSc-REP Regan Dosimetry 80
    Thermoluminescence Dosimetry
    Randall-Wilkins theory of glow curves: The probablity per unit time of an
    electron being detrapped (i.e. freed) by thermal energy is (this is the
    probablity the electron energy is in the Maxwell-Boltzman tail above the
    trap depth Et), ??
    ???
    ? ?
    = kT
    ESyprobabilit texp, ?
    ??
    ???
    ? ?
    =? kT
    EnSdt
    dnrate texp,
    where Et = depth of energy trap, S = constant, k = Boltzmann’s constant
    and T = temperature.
    The rate at which electrons escape from a trap of energy Et is,
    where n = number of electrons in a trap. Et and S can be determined
    experimentally. For example LiF:Mg,Ti has several dominant traps
    ranging from 1 to 2eV, with S values of 1012 to 1020 s-1. This implies the
    mean lifetime in shallow traps will be a few minutes, whilst in deeper traps
    the mean lifetime is around 80 years. This results in a natural “fading” of
    TL signal with time.
    MSc-REP Regan Dosimetry 81
    Additional revision slides,examples
    and additional material
    MSc-REP Regan Dosimetry 82
    Internal Dosimetry and Effective Half-Life
    The effective elimination rate constant is the sum of the probability of
    radioactive
    decay, ?R and the biological elimination constant, ?B, such that ?E=?R+?B.
    The effective half-life is the time for the quantity of radioactive material in
    an organ to fall to a half of its original value, i.e for Q0 to decay to Q0/2.
    TE=ln2/?E=0.693/?E.
    For 1st order kinetics
    ( ) ( ) [ ]( ) ( ) ???
    ?
    ???
    ?
    ?=?=+?=???=
    E
    EBRBR T
    tQtQtQttQtQ 693.0expexpexpexpexp)( 0000 ?????
    MSc-REP Regan Dosimetry 83
    From the general expression for the activity, ANdt
    dN
    =?= ?
    we can solve and substitiute to get:
    ( ) { } ( )tdt
    dNtAtAdt
    dN ?? ?=?== expexp 00
    ( )dttdt
    dNdN ??= exp0
    The expression for imparted dose rate will have a similar form since the dose rate
    is directly proportional to the activity of the sample. Thus we have the initial
    expression
    ( )dttdt
    dDdD E??×= exp0
    Since dD0/dt = a constant (i.e. initial dose rate at time t=0),
    then
    ( ) ( )dttdt
    dDdttdt
    dDdD ttt E
    tt
    t E ??? ==== ?=?×= 000 0 expexp ??
    MSc-REP Regan Dosimetry 84
    ( ) ( )
    tt
    t
    E
    E
    tdt
    dDtD
    =
    =
    ??
    ???
    ?
    ??=?
    0
    0 exp1 ?
    ?
    ( ) ( ) ( ) ??
    ???
    ?
    ???
    ?
    ???
    ?
    +??=??
    ???
    ?
    ???
    ?
    ???
    ?
    ????=?
    E
    E
    EE
    E
    E
    tdt
    dDtdt
    dDtD
    ?
    ?
    ??
    ?
    ?
    1exp11exp1 00
    ( ) ( ) ??
    ???
    ?
    ???=? tdt
    dDtD E
    E
    ?
    ?
    exp110
    Integrating gives the total imparted dose time t after the initial internal
    contamination D(t)
    MSc-REP Regan Dosimetry 85
    Worked Example Question
    MSc-REP Regan Dosimetry 86
    Worked Example
    MSc-REP Regan Dosimetry 87
    Example examination question (2009):
    MSc-REP Regan Dosimetry 88
    (2009)
    Exam
    question
    MSc-REP Regan Dosimetry 89
    Example exam question (2009)
    MSc-REP Regan Dosimetry 90
    Example exam question (2009)
    MSc-REP Regan Dosimetry 91
    Example exam question (2009)
    MSc-REP Regan Dosimetry 92
    Exposure Rate Constants
    Example Question
     Using the expression dX/dt = ?? A/d2, where dX/dt is the
    exposure rate, A the activity and d the distance,
    Show that ?? = 3.2 R.cm2.hr-1.mCi-1 for Caesium-137 given the
    following information:
    The gamma-ray branching ratio for the 662 keV decay
    following the 137Cs decay is 85%.
     
    Air has a mass energy absorption coefficient at this
    gamma-ray energy of 0.0293 cm2.g-1;

    The activity is 1mCi, and the source distance is 1cm.
    MSc-REP Regan Dosimetry 93
    Example Answer
     
    If activity A is 1mCi and the distance is 1cm. Therefore ?? = dX/dt. The Dose per second is given by
    energy photon fluence multiplied by the mass energy absorption coefficient. [remember 1Ci = 3.7x1010
    Bq]

    Dose per second =
     0.85 x 3.7x107 mCi–1 x (0.662)x106 eV x 1.6x10-19 J.eV-1 x 0.0293 cm2.g-1
    4pi x 1s

    = 7.77x10-9 J.s-1.g-1.cm2.mCi-1
     
    in 1 hour (1hr = 3600s)
     
    = 2.80x10-5 J.g-1.cm2.hr-1.mCi-1
     
    for 1 kg (1kg = 1000g)
     
    = 2.80x10-2 J.kg-1.cm2.hr-1.mCi-1 (or in units Gy.cm2.hr-1.mCi-1)
     
    in rads (1Gy = 100rad)
     
    = 2.80 rad.cm2.hr-1.mCi-1
     
    in Roentgen (1R = 0.87 rad)
     
    = 3.2 R.cm2.hr-1.mCi-1
    MSc-REP Regan Dosimetry 94
    Radiation Equilibrium
    P.V’
    A B
    d
    C V
    ?EE = ionising radiation energy entering V'
    ?EL = ionising radiation energy leaving V'
    ?ER = increase in rest mass energy within V'
    C.of.E ? energy imparted to matter in V',
    ?ED = ?EE - ?EL - ?ER
     
    Under conditions of
    radiation equilibrium
    ?EE = ?EL ? ?ED = -?ER
     
    ? Dose = ?ED/?m = - ?ER/?m
    MSc-REP Regan Dosimetry 95
    Radiation Equilibrium
    ?EEext
    ?EEint
    ?ELext
    ?EDext?ERext
    ?ERint
    ?EDint
    ?ELint
    MSc-REP Regan Dosimetry 96
    Total Dose,
    D = ?EDext + ?EDint
    ? D = [?EEext-?ELext-?ERext]+[?EEint-?ELint-?ERint]

    Radiation Equilibrium??EEext = ?ELext + ?Elint
    ? D = [?EEint] - [?ERext + ?ERint]
    ? D = [Decrease in rest mass] - [Increase in rest
    mass]
    If there are no internal sources,
    ? D = [?EEext - ?ELext] - ?ERext
    Radiation Equilibrium
    MSc-REP Regan Dosimetry 97
    Charged Particle Equilibrium
    Uncharged particles impart dose via two-
    steps
    1. Kinetic energy is transferred to
    charged particles
    2. These charged particles deposit
    energy in the medium.
    MSc-REP Regan Dosimetry 98
    Charged Particle Equilibrium
    Uncharged particles impart dose via two-
    steps
    1. Kinetic energy is transferred to
    charged particles
    2. These charged particles deposit
    energy in the medium.
    MSc-REP Regan Dosimetry 99
    Charged Particle Equilibrium
    If each charged particle carrying energy out of
    V' is balanced by an identical particle carrying
    the same amount of energy in, then charged
    particle equilibrium (CPE) is said to exist inside
    V'.
    MSc-REP Regan Dosimetry 100
    Charged Particle Equilibrium
    If a volume is irradiated by an external source,
    the energy carried in and out by charged (c) and
    uncharged particles (u) is,
    ? ?ED = [(?EE)c-(?EL)c]+[(?EE)u-(?EL)u- (?ER)u]
    If CPE exists,
    (?EE)c = (?EL)c
    ? ?ED = [(?EE)u-(?EL)u- (?ER)u]
    MSc-REP Regan Dosimetry 101
    Charged Particle Equilibrium
    Energy from uncharged radiation supplies ?EK to charged particles + rest mass changes,
    (?EE)u - (?EL)u = ?EK + (?ER)u
    ? ?EK = (?EE)u - (?EL)u - (?ER)u
    c.f. ?ED = [(?EE)u-(?EL)u- (?ER)u] from before
    ? ?ED = ?EK
    MSc-REP Regan Dosimetry 102
    Charged Particle Equilibrium
    If the mass of material in the volume is ?m,
    Dose = ?ED /?m
    = ?EK /?m
    = K, kerma
    ? C.P.E. ? D = K
    CPE is always present when radiation equilibrium
    occurs, but in many cases of practical interest CPE is
    closely attained even though complete radiation
    equilibrium is not.
    MSc-REP Regan Dosimetry 103
    Charged Particle Equilibrium
    Vacuum Medium
    Build up
    Region
    Relectron
    Absorbed Dose
    Kerma
    e-
    MSc-REP Regan Dosimetry 104
    Mass energy absorption
    coefficients
    For an air filled ion chamber, the absorbed dose for an
    exposure of 1R = 0.87rad.
    air
    m
    airm DSD ?=
    Hence for an exposure of X roentgen, the dose in rads is,
    XSD mairm ??= 87.0
    This can be written Dm = f.X where f = 0.87.airSm
    which is called the rad per roentgen factor
    X.D air ?= 870
    MSc-REP Regan Dosimetry 105
    Mass energy absorption coefficients
    As radiation energy fluence passes through an
    abosorber it decreases exponentially,
    E = E0exp(-µenx)
    Differentiating gives:
    dE/dx = -µenE0exp(-µenx) = -µenE
    Multiply by 1/?, (? is absorber mass density) to give
    which has units of energy/mass ? dose
    E?
    ?
    dx
    dE
    ?
    1 en
    ?=??
    ???
    ?
    ?
    MSc-REP Regan Dosimetry 106
    Mass energy absorption coefficients
    µen/? = mass energy absorption coefficient
    E?
    ?D dose, en ?=
    E?
    ?K kerma, tr ?=
    µtr/? = mass energy transfer coefficient
    MSc-REP Regan Dosimetry 107
    Mass energy absorption coefficients
    The linear attenuation coefficient is,
    Allowing for escaping radiation,
    Additionally bremsstrahlung reduces this again,
    ( ) ( ) ( )?2oppsc?petr Ec2m1?f1?E?1?? ?+?+?=
    pppe ???? c ++=
    g)(1?
    ?
    ?
    ? and g)(1?? trentren ?=?=?
    MSc-REP Regan Dosimetry 108
    Exposure Rate Constants
    Consider a point source of photons in air of activity A mCi
    situated at distance d from the point of interest where the
    exposure rate is dX/dt R.h-1.
    The exposure rate depends only on the activity of the
    source and the inverse square of the distance from the
    source.
    Hence dX/dt = ??.A/d2 where ?? is called the exposure rate
    constant. Using the above units ?? has units
    R.cm2.h-1.mCi-1.
    MSc-REP Regan Dosimetry 109
    Additional Information on
    Personal Dosimetry / TLDs
    MSc-REP Regan Dosimetry 110
    Thermoluminescence Dosimetry
    Real TLD materials have a dose range of about 0.1?Gy to in excess of
    10Gy. As well as specifically made TLD materials, suitable environmental
    samples (such as the roof tiles in Hiroshima) can also be used.
    TLD measurements though are subject to two types of spurious
    luminescence (1) triboluminescence – arising from trapping of charges
    generated by friction between loose grains, reduced by encapsulating the
    TL crystals in a PFTE binder (2) chemiluminescence – arising from oxygen
    induced surface reactions, reduced by N2 flushing.
    In addition UV light can cause the TLD to prematurely fade and can be
    reduced by keeping the TLD in light-tight packaging.
    There are also two related techniques, Thermally Stimulated Electron
    Emission (TSEE) and Thermally Stimulated Conductivity (TSC) which are
    alternative readout methods.
    MSc-REP Regan Dosimetry 111
    Photographic Emulsion Dosimetry
    The photographic emulsion is a suspension of silver halide crystals in a
    gelatin matrix. The film badge has an emulsion coating on both sides
    but of differing sensitivities, one for a high dose range, and the other for
    low dose ranges.
    When the film is exposed to X-rays, secondary ionisation makes one or
    more of the silver halide ions latent. When developed this produces
    metallic silver which varies spatially according to the amount of dose
    absorbed within the matrix, this forms the photographic negative.
    20µm
    200µm
    protective coating
    base material
    silver halide
    grains in a
    gelatin matrix
    MSc-REP Regan Dosimetry 112
    Photographic Emulsion Dosimetry
    A typical film density versus exposure curve is shown below,
    MSc-REP Regan Dosimetry 113
    Photographic Emulsion Dosimetry
    Despite some of the drawbacks described above photographic
    dosimetry still has some advantages over alternatives like TLD.
    (a) In fine grain emulsions individual particle tracks can be recognised
    under a microscope and the nature and energy of the incident radiation
    can be deduced. In radiation protection this has been used to record
    proton recoil tracks arising in the surrounding gelatin matrix as result of
    fast neutrons passing through the film badge.
    (b) The technique produces a permanent visible record so that
    exposures can be readily rechecked. For example radioactive
    contamination of a film badge can be distinguished from a "normal"
    uniform exposure to more distant radiation sources. The self-indicating
    feature is advantageous if required as legal evidence.
    (c) The technique is relatively "low-tech" compared with TLD for
    example and needs less costly equipment which may make it
    more practicable in some cases. Although it is not as readily
    automated as a TLD system this may not be important if the
    workforce being monitored is fairly small.
    MSc-REP Regan Dosimetry 114
    Personal Dosemeters
    Film Badges and TLDs
    MSc-REP Regan Dosimetry 115
    Personal Dosemeter Badges
    Thermoluminescent dosemeter (a.k.a. “TLD”)

                                   
           
    This is a reusable dosemeter which uses lithium fluoride to
    measure radiation dose. It stores dose information until heated to
    over 250°C when it gives out light the amount of which is
    proportional to the dose received. It is environmentally robust and
    excellent for use in all working environments.
    Photographic film dosemeter (a.k.a. “film badge”)

                                  
           
    Film is worn in a holder containing several different filters. When
    developed the film darkens in proportion to the amount of radiation
    energy received. Due to the differing amounts of filtration we can
    gain information on the energy of radiation causing the dose.
    Radioactive contamination of the film can be readily identified.
    Extremity dosemeter (a.k.a. “finger TLD”)

                                    
                           
    This is a miniature TLD which can be supplied in
    different forms to suit your needs (stalls, straps or
    rings). The finger stall is most commonly used and
    is worn like the finger of a glove.
    MSc-REP Regan Dosimetry 116
    A dosemeter often measures two quantities. The first is the personal
    dose equivalent Hp(10), which is often referred to as the “whole body”
    dose which results from penetrating radiation. The second quantity is
    the personal dose equivalent Hp(0.07) which is an assessment of the
    dose equivalent to the skin from both weakly and strongly penetrating
    radiations.
    The “H” of Hp is used generally to signify the Equivalent Dose and is
    in units of Sieverts. The “p” is used to signify it is personal equivalent
    dose.
    The definition of Hp(10) is the dose equivalent at a depth of 10 mm
    into a human body. Similarly Hp(0.07) is 0.07mm into the body.
    Other measurements of equivalent dose may not give accurate values
    of the Hp equivalent dose as it is the absorption and scattering effects
    of the human body throughout the different response to the energy of
    the radiation which give true Hp readings.
    Hp (0.07) and Hp (10)
    MSc-REP Regan Dosimetry 117
    Film Badge Dosemeters
    For many decades the standard method personal dosimetry involved the
    use of photographic emulsions in the form of film badge dosemeters.
    Although they are increasingly being replaced by other methods, they are
    still in use as dosemeters for X-, beta and gamma radiation.
    To cover the required dose range the film incorporates two emulsions, of
    different sensitivities. Additionally the film badge holder has a number of
    different filters to sort out the various components of radiation exposure.
    Detection Gamma rays X-rays Beta particles
    Dose range
    measured
    0.1 mSv to 10 Sv 0.1 mSv to 400
    mSv
    0.1 mSv to 10 Sv
    Energy range
    detected
    10 keV to 7 MeV
    for Hp (0.07)
    20 keV to 7 MeV
    for Hp (10)
    10 keV to 7 MeV
    for Hp (0.07)
    20 keV to 7 MeV
    for Hp (10)
    700 keV to 3.5
    MeV (Emax) for
    Hp (0.07)
    MSc-REP Regan Dosimetry 118
    The variation of response with energy and angle of incidence (mean
    between 0° and 60°) for the quantities Hp(10) [red] and Hp (0.07) [blue]
    is shown for photons in the graph below. This is for the combined film
    emulsions and is normalised to caesium-137 with a value of 0.9.
    The film badge is still found in hospitals and other medical
    establishments where X-rays are used. It is the use of a technology
    with is familiar to the user, that adds an important element of
    confidence that the personal dosemeter is performing its required
    use.
    MSc-REP Regan Dosimetry 119
    Thermoluminescent Dosemeters
    Currently the most common used personal dosemeter. The dosemeter
    consists of two thermoluminescent detectors containing the radiation-
    sensitive material lithium fluoride (LiF). The detectors are located in a plate
    which is identified uniquely by means of an array of holes. The lithium
    fluoride stores the energy it receives from ionising radiations until it is
    heated during processing (in this case to about 250°C) when the energy is
    released as light. The amount of light released is proportional to the
    radiation dose. The plate is supplied to the wearer in a plastic wrapper
    which protects the detectors from light and contaminants.
    LiF inserts
    Current NRPB
    TLD and new
    Harshaw TLD
    MSc-REP Regan Dosimetry 120
    Detection X-rays and Gamma rays Beta particles
    Dose range
    measured
    0.05 mSv to 10 Sv 0.05 mSv to 10 Sv
    Energy range
    detected
    10 keV to 10 MeV for Hp (0.07)
    15 keV to 10 MeV for Hp (10)
    700 keV to 3.5 MeV
    (Emax) for Hp (0.07)
    The Hp(10), “whole body” dose is measured by the detector behind the
    domed part of the holder. The Hp(0.07), “dose equivalent to the skin
    from both weakly and strongly penetrating radiations” is measured by
    the detector behind the circular window.
    MSc-REP Regan Dosimetry 121
    Optically Stimulated
    Luminesence Dosemeters
    Optically Stimulated Luminesence Dosemeters (OSLDs) measures
    radiation through a thin layer of aluminum oxide. During analysis, the
    aluminum oxide is stimulated with selected frequencies of laser light
    causing it to become luminescent in proportion to the amount of
    radiation exposure.
    OSLDs gives accurate readings down to 1 µSv. This degree of
    sensitivity is ideal for employees working in low-radiation environments
    and for pregnant employees.
    The Al203 (aluminum oxide) detector can be restimulated  numerous
    times to confirm the accuracy of a radiation dose measurement. 
    OSLDs be used for up to one year. They are unaffected by heat,
    moisture, and pressure when the clear blister packaging is
    uncompromised.
    OSLD readers do not require heaters or gas flow.
    MSc-REP Regan Dosimetry 122
    Optically Stimulated
    Luminesence Dosemeters
    Measurements Photon
    (X-Ray and Gamma Ray)
    Beta Particle Neutron
    (Optional Neutrak® 144 Detector Inside
    Dosemeter)
    Detector Al203 (Aluminum Oxide) Al203 (Aluminum Oxide) Neutrak 144 allyl diglycol carbonate solid state nuclear track detector
    Analysis
    Method
    Optically Stimulated
    Luminescence (OSL)
    Optically Stimulated
    Luminescence (OSL)
    Chemical etching followed by track
    counting
    Energies
    Detected
    5 keV to in excess of 40
    MeV
    150 keV to in excess of 10
    MeV
    Fast: 40 keV to in excess of 35 MeV
    Thermal: under 0.5 eV
    Dose
    Measurement
    Range
    10 uSv to 0.1 Sv 0.1 mSv to 10 Sv Fast: 0.2 mSv to 0.25 Sv
    Thermal: 0.1 mSv to 50 mSv
    Accreditation Accredited by NVLAP in all categories including VIII when neutron component is added, NVLAP
    Lab Code 100518-0.
    Landauer Luxel® Dosemeter
    MSc-REP Regan Dosimetry 123
    Neutron Dosemeters
    The poly-allyl diglycol carbonate (PADC) neutron dosemeter is designed to
    measure doses from neutron radiation in terms of the radiation quantities
    specified by the Health and Safety Executive (HSE). The PADC neutron
    service is approved by the HSE under Regulation 35 of the Ionising
    Radiations Regulations 1999. The dosemeter is a passive device for the
    detection of thermal, epithermal and fast neutrons. It is insensitive to other
    radiations (gamma, X- and beta), is relatively unaffected by environmental
    factors such as heat and humidity and has a very low radon sensitivity.
    Detection Neutron radiation
    Dose range
    measured
    0.2 mSv to 250 mSv
    Energy range
    detected
    Thermal, epithermal and fast
    (144 keV to 15 MeV)
    neutrons for Hp (10)