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INTERACTION OF RADIATION
          WITH MATTER



              DR ARNAB BOSE
              Dept. of Radiotherapy
              NRS Medical College, Kolkata
Part 1 :        Introduction

    Importance of the knowledge of the
     fundamentals of interaction with matter

3.   Forms the basis of Radiobiology
4.   Forms the basis of Radiation protection
5.   Forms the basis of Radiation detection
6.   Ensures safe and effective methodologies in
     Radiology and Radiotherapy
Radiation

   The term radiation applies to the emission and
    propagation of energy through space or a
    material medium .
   Radiation may be
                Electromagnetic Radiation
                Particle Radiation
       When radiation passes through matter it may
    interact with the material , transferring some or
    all of its energy to the atoms of that material.
Electromagnetic Radiation

   Constitutes the mode of energy propagation for
    such phenomena as light waves, heat waves,
    radio waves, u v rays, x rays and γ rays .
   Spectrum of electromagnetic radiation ranges
    from 107 m (radio waves) to 10-13 m (ultra high
    energy X rays) .
   X rays and γ rays are the two major forms of
    electromagnetic radiation used in modern day
    radiotherapy.
   An X ray beam emitted from a target or a γ ray
    emitted from a radioactive source consists of a
    large number of photons , usually with a variety
    of energies .
Electromagnetic Wave with respect to Electric & Magnetic Field
Particulate Radiation

   Refers to the energy propagated by traveling
    corpuscles – which have definite rest mass ,
    definite momentum and a defined position at any
    instant .
   Elementary atomic particles are electrons (charge
    – 1) , protons (charge + 1) and neutrons (zero
    charge) .
   Some common subatomic particles are positrons
    (charge + 1) , neutrinos (zero charge) and
    mesons .
Part 2 : Interaction of Photons with
                   Matter
   When an X ray or γ ray beam passes through a
    medium , interaction occurs between the photon
    and the matter and energy is transferred to the
    medium .

   If the absorbing medium consists of body tissues
    sufficient energy may be deposited within the
    cells destroying their reproductive capacity .
Fate of the Photon Beam
   The photon beam may undergo the following four
    processes – Attenuation , Absorption , Scattering
    and Transmission .
   Attenuation refers to the removal of radiation
    from the beam by the matter . Attenuation may
    occur due to scattering and absorption .
   Absorption refers to the taking up of energy from
    the beam by the irradiated material .It is the
    absorbed energy which is important in producing
    the radiobiological effects .
   Scattering refers to the change in the direction of
    photons and it contributes to both attenuation
    and absorption .
   Any photon which does not suffer the above
    processes is transmitted .
Attenuation Coefficient (1)
   Fraction of photons removed from a mono
    energetic beam of x-ray or gamma ray per unit
    thickness of material is called linear attenuation
    coefficient (µ), typically expressed in cm-1 .
   Number of photons removed from the beam
    traversing a very small thickness ∆x:
                 µ x
              n = N∆
 where n = number removed from beam,
N = number of photons incident on the material,
and minus sign is placed before μ to indicate that
  no. of photons decreases as the absorber
  thickness increases.
Attenuation Coefficient (2)
   For a mono energetic beam of photons incident
    on either thick or thin slabs of material, an
    exponential relationship exists between number
    of incident photons (N0 ) and those transmitted
    (N) through thickness (x) without interaction:
                              −µ
            N =N e        0
                                 x


   The number of photons indicate the Intensity of
    the beam and can also be written as ( I ).
Attenuation Coefficient (3)
     Total Linear attenuation coefficient is the sum of
    individual linear attenuation coefficients for each
    type of interaction:

     µ = µRayleigh + µphoto + µCompton + µpair
   For a given thickness of material , probability of
    interaction depends on number of atoms the x
    ray or gamma ray encounter per unit distance.
    The density (ρ ) of material affects this number.
   Linear attenuation coefficient is proportional to
    the density of the material.
Mass Attenuation Coefficient
   For a given thickness probability of interaction is
    dependent on the number of atoms per volume.
    This dependency can be overcome by
    normalizing linear attenuation coefficient for
    density of material –
   Mass Attenuation Coefficient (μ / ρ ) =
       Linear attenuation coefficient
        Density of the material
    Mass attenuation coefficient is independent of
    density of the material.
Half Value Layer (1)
   Half value layer (HVL) defined as thickness of
    material required to reduce intensity of an x-ray
    or gamma-ray beam to one-half of its initial
    value.
    It is an indirect measure of the photon energies
    (also referred to as quality or penetrability) of a
    beam of radiation.
   For mono energetic photons, the probability of
    attenuation remains the same for each additional
    HVL thickness placed in the beam.
   Relationship between μ and HVL:
                    HVL = 0.693/μ
Half Value Layer (2)
List of Interactions
     Attenuation of a photon beam by an absorbing
     material is caused by 5 major types of
     interactions –
2.              Coherent Scattering
3.              Photoelectric Effect
4.              Compton Effect
5.              Pair Production
6.              Photonuclear Effect
Coherent Scattering
   X-rays passing close to the atom cause the bound
    electrons to vibrate momentarily at a frequency
    equal to that of the radiation. These in turn emit
    radiation of the same frequency in all directions .
   The energy is taken up from the beam and
    scattered in all direction, but none of the energy
    is absorbed. Thus this is a form of attenuation
    without absorption .
   This interaction is of little importance in practical
    radiotherapy, but is important in X-ray
    crystallography .
   Since it involves bound electrons, it occurs more
    in higher atomic number materials, and also
    more with low-energy radiations.
Photoelectric Effect (1)
   All of the incident photon energy is transferred to
    an electron, which is ejected from the atom.
   Kinetic energy of ejected electron called the
    photoelectron (EC ) is equal to incident photon
    energy (EO ) minus the binding energy of the
    orbital electron (EB )
              EC =EO - EB
Photoelectric Effect (3)
   Incident photon energy must be greater than or
      equal to the binding energy of the ejected
    photon.

    The ionized atom regains electrical neutrality by
    rearrangement of the other orbital electrons. The
    electrons that undergo these rearrangements
    surrender some of the energy in form of a photon
    known as the characteristic radiation of the atom.

   Absorption of these characteristic radiation
    internally in the atom may result in emission of
    Auger electrons . These electrons are mono
    energetic in nature.
Photoelectric Effect (4)
   Probability of photoelectric absorption per unit
    mass is approximately proportional to
                      3      3
                   Z /E
   Energy dependence explains, in part, why image
    contrast decreases with higher x-ray energies.
   Process can be used to amplify differences in
    attenuation between tissues with slightly different
    atomic numbers, improving image contrast.
Photoelectric Effect (5)
   Graph of probability of photoelectric effect, as a
    function of photon energy, exhibits sharp
    discontinuities called absorption edges .
   Photon energy corresponding to an absorption
    edge is the binding energy of electrons in a
    particular shell or sub shell .
   The phenomena of absorption edges is important
    for two different reasons:1) At these absorption
    edges, low-energy photons are less attenuated
    and therefore more penetrating than high energy
    photons. 2)A substance is relatively transparent
    to its own characteristic radiation. This effect is
    important when filters are considered as the
    filters will be “transparent” to their own
    characteristic radiation.
Compton Effect (1)

   Photon interacts with an atomic electron as
    though it were a free electron. Practically this
    means that energy of the incident photon must
    be large compared with the electron binding
    energy.
   The electron receives some energy from the
    photon and is emitted at an angle Φ while the
    photon with reduced energy is scattered at an
    angle θ .
Compton Effect (2)
Compton Effect (4)

   As incident photon energy increases, scattered
    photons and electrons are scattered more toward
    the forward direction.

   Probability of interaction increases as incident
    photon energy increases.

   Probability also depends on electron density ( no.
    of electrons per gram of matter ).
   Electron density fairly constant in tissue.

   Probability of Compton scatter/unit mass
    independent of Z.
Compton Effect (5)
   Maximum energy of photons with 90° scatter is
    0.511 M e V while that for 180° scatter ( i.e..
    Back scatter) is 0.255 M e V.
   Energy of the photons scattered at angles <90 °
    will be more than 0.511 M e V and will gradually
    approach the incident photon energy.
   Energy of the scattered radiation is independent
    of the incident beam energy .This implies that as
    the photon energy increases there is a
    corresponding increase in the forward scatter of
    the beam. This results in better dose distribution.
    Direction of the scatter depends on the energy of
    the incident photon beam . This means that
    higher beam energies allow greater absorption of
    the dose in the body with less scattering of
    energy.
Compton Effect (6)
   If the angle by which the electron is scattered is
    θ and the angle by which the photon is scattered
    is Φ, then the following formula describes the
    change in the wavelength ( δ λ )of the photon:
          λ 1 – λ 2 = δ λ = 0.024 ( 1- c o s Φ) Å
   Thus the wavelength change depends neither on
    the material being irradiated nor on the radiation
    energy, but only upon the angle through which
    the radiation is scattered.
   The Compton effect results in both attenuation
    and absorption .
Compton Effect (7)

   Laws of conservation of energy and momentum place
    limits on both scattering angle and energy transfer.
   Maximal energy transfer to the Compton electron
    occurs with a 180-degree photon backscatter.
   Scattering angle for ejected electron cannot exceed 90
    degrees.

   Energy of the scattered electron is usually absorbed
    near the scattering site.
Pair Production (1)
   When the photon with energy in excess of        1.02
     M e V passes close to the nucleus of an atom,
    the photon disappears, and a positron and an
    electron appear. This effect is known as pair
    production.
   Pair production results in attenuation of the beam
    with absorption.
   The positron created as a result loses its energy
    by interaction with an electron to give rise to two
    annihilation photons, each having 0.511 M e V
    energy. Again because momentum is conserved
    in the process two photons are rejected in
    opposite directions. This reaction is known as an
    annihilation reaction.
Pair Production (3)
   Pair production results from an interaction with
    the electromagnetic field of the nucleus and as
    such the probability of this process increases
    rapidly with the atomic number (Z 2 ).

   In addition, the likelihood of this interaction
    increases as the photon energy increases, in
    contrast to the Compton effects and the
    photoelectric effect.
Photonuclear Reaction
   This reaction occurs when the photon has energy
    greater than the binding energy of the nucleus
    itself. In this case, it enters the nucleus and
    ejects a particle from it. The photon disappears
    altogether, and any energy possessed in excess
    of that needed to remove the particle becomes
    the kinetic energy of escape of that particle.
   The threshold energy for this effect is 10.8 M e V.
   The main use of this reaction is for energy
    calibration of machines producing high energy
    photons.
Relative Importance of the
           Various Processes
The relative importance of the 3 principal modes of
interaction pertinent to radiation therapy- the
Photoelectric , Compton and Pair production processes
- as a function of Incident beam energy and Atomic
number of absorber matter shows -
 For an absorber with Z approximately equal to that of
soft tissue - 7 , and for mono energetic photons ,
Photoelectric effect is the dominant interaction below
about 30 k e v.
Above 30 k e v Compton effect remains dominant and
remains so,
Until about 24 M e v , after which Pair Production effect
becomes dominant .
Relative Importance
Relative Importance of the
        Various Processes (3)
   In a graph plotted for total mass attenuation
    coefficient vs. photon energy it is seen that -
   The μ /ρ is large for low energies and high Z
    media (eg. Lead ) because of the predominance
    of Photoelectric interactions under these
    conditions. The μ /ρ decreases rapidly with
    energy until the photon energies far exceed the
    electron binding energies and Compton effect
    becomes the predominant mode of interaction.
   In the range of Compton effect the μ /ρ of lead
    and soft tissues do not vary greatly as Compton
    effect is independent of Z .The μ /ρ however
    decrease with energy until Pair production
    becomes important .
Plot of total mass att. Coef.
As a function of photon energy
Part 3 : Interaction of Particle
          Radiation with Matter
    Interaction of Electrons with matter –

    The two different modes of interaction and energy
    transfer of electrons with matter include:
   Collision between the particle and the electron
    cloud resulting in ionization and excitation ( more
    important in low atomic number elements). This
    is called Collisional loss .
   Collision between the nucleus and the particle
    resulting in bremsstrahlung radiation (more in
    high atomic number elements). This is called
    Radiative loss .
Electron Interactions
   The ionization pattern produced by a beam of
    electrons is characterized by a constant value
    from the surface to a depth equal to about half
    the range, followed by a rapid falling off to almost
    zero at a depth equal to the range . The
    bremsstrahlung radiation produced when
    electrons slow down contributes to an
    insignificant dose beyond the range of any
    electron. This is specially seen in electrons in the
    energy range of 6 -15 M e V .

   These characteristics make electrons a useful
    treatment modality for superficial lesions.
Proton & Pi Meson Interactions
   Protons and pi mesons are charged particles that
    are being used in experimental set-ups only.
   These particles have a very high linear energy
    transfer (LET) that is they have a very high
    ionization density( Amount of energy deposited
    per unit path length is called the linear energy
    transfer (LET) ).
   Further, these charged particles also exhibit the
    phenomena of Bragg’s peak which refers to the
    increased ionization occurring near the end of the
    track with little effect beyond.
Neutron Interactions

• Neutrons are indirectly ionizing uncharged
  radiations, which interact only with the nucleus
  in two ways:
    By recoiling protons from hydrogen and the

     nucleus in other elements.
    Nuclear disintegration , which contribute to

     ~30% of the total dose in tissues.
Part 4 : Practical Implications
The three major forms of interaction of radiation
  with matter, which are of clinical importance in
  radiotherapy are:
     Compton effect.

     Photoelectric effect.

     Pair production.

Out of these, the Compton effect is the most
  important in modern-day megavoltage
  radiation therapy.
The reduced scattering suffered by high-energy
  radiation as well as the almost homogeneous
  tissue dosage is primarily due to the Compton
  effect.
Practical Implications
   Coherent scattering is of little importance in
    practical radiotherapy, but is important in X-ray
    crystallography .
   The photoelectric effect has several important
    implications in practical radiology:
   In diagnostic radiology , the primary mode of
    interaction is photoelectric. It is also responsible
    for the contrast effect.
   In therapeutic radiology , low-energy beams in
    orthovoltage irradiation causes excessive
    absorption of energy in bone.
Practical Implications
   The attenuation produced by the Compton effect
    is described by the mass scattering coefficient
    ( σ / ρ ), and is practically same for all
    substances except hydrogenous material, like
    water and soft tissue, where the Compton effect
    is greater (because of the higher electron
    density).
   Attenuation does not depend on the atomic
    number of absorber matter in Compton effect.
   Thus concrete is as good as lead in shielding of
    megavoltage equipment!
   The absorption in bones does not exceed that
    produced in the soft tissues – unlike in PE effect
    seen in orthovoltage radiation era.
   Port films produced in megavoltage equipment
    have very little detail.
Practical Implications
   The low mass of the electron leads to greater
    scattering. This is of practical importance as
    radioactive isotopes which are produce high
    energy beta radiation are better stored in low
    atomic number materials e.g. plastics as they will
    lead to lesser bremsstrahlung radiation.
      Also higher atomic number elements are better
    for x ray production. The amount of radiative loss
    is proportional to the square of the atomic
    number of the material This leads to the
    phenomenon of greater ionization in soft tissues
    relative to bones. Ionization and excitation are
    more for low atomic materials.
Practical Implications
   Protons and Heavy particle beams have the
    ability to concentrate dose inside the target
    volume and minimize dose to surrounding normal
    tissues because of the Bragg peak effect and
    minimal scattering.
    However there are several practical and
    theoretical difficulties with the use of these
    charged particles. Some of them include:
   The narrow Bragg peak makes a homogenous
    Tumor Dose difficult.
    Generation of these charged particles requires
    expensive and large machines.
   The method of the production ensures that the
    field size is very narrow. So, for treatment of
    cancers the beam has to be scanned back and
    forth across the treatment area.
Practical Implications
   Hydrogenous materials like fats absorb neutrons
    more than heavier materials and thus there is a
    20% greater absorption in fat relative to muscle.
   Lower atomic materials (e.g. fats and paraffin)
    are better for neutron shielding as compared to
    lead as greater absorption occurs.
   Neutrons, being uncharged particles also
    penetrate deeply into matter.
   But neutrons are not commonly used in practical
    radiotherapy, because of technical difficulties in
    production of these beams as well as their
    complicated dosimetry.
Part 5 : Conclusion
   Despite several decades of research, photon-
    beam still constitute the main therapeutic
    modality in radiotherapy, because of several
    unresolved technical problems with the use of
    particulate radiation.
Interaction of  Radiation with  Matter

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Interaction of Radiation with Matter

  • 1. INTERACTION OF RADIATION WITH MATTER DR ARNAB BOSE Dept. of Radiotherapy NRS Medical College, Kolkata
  • 2. Part 1 : Introduction  Importance of the knowledge of the fundamentals of interaction with matter 3. Forms the basis of Radiobiology 4. Forms the basis of Radiation protection 5. Forms the basis of Radiation detection 6. Ensures safe and effective methodologies in Radiology and Radiotherapy
  • 3. Radiation  The term radiation applies to the emission and propagation of energy through space or a material medium .  Radiation may be Electromagnetic Radiation Particle Radiation  When radiation passes through matter it may interact with the material , transferring some or all of its energy to the atoms of that material.
  • 4. Electromagnetic Radiation  Constitutes the mode of energy propagation for such phenomena as light waves, heat waves, radio waves, u v rays, x rays and γ rays .  Spectrum of electromagnetic radiation ranges from 107 m (radio waves) to 10-13 m (ultra high energy X rays) .  X rays and γ rays are the two major forms of electromagnetic radiation used in modern day radiotherapy.  An X ray beam emitted from a target or a γ ray emitted from a radioactive source consists of a large number of photons , usually with a variety of energies .
  • 5. Electromagnetic Wave with respect to Electric & Magnetic Field
  • 6. Particulate Radiation  Refers to the energy propagated by traveling corpuscles – which have definite rest mass , definite momentum and a defined position at any instant .  Elementary atomic particles are electrons (charge – 1) , protons (charge + 1) and neutrons (zero charge) .  Some common subatomic particles are positrons (charge + 1) , neutrinos (zero charge) and mesons .
  • 7. Part 2 : Interaction of Photons with Matter  When an X ray or γ ray beam passes through a medium , interaction occurs between the photon and the matter and energy is transferred to the medium .  If the absorbing medium consists of body tissues sufficient energy may be deposited within the cells destroying their reproductive capacity .
  • 8. Fate of the Photon Beam  The photon beam may undergo the following four processes – Attenuation , Absorption , Scattering and Transmission .  Attenuation refers to the removal of radiation from the beam by the matter . Attenuation may occur due to scattering and absorption .  Absorption refers to the taking up of energy from the beam by the irradiated material .It is the absorbed energy which is important in producing the radiobiological effects .  Scattering refers to the change in the direction of photons and it contributes to both attenuation and absorption .  Any photon which does not suffer the above processes is transmitted .
  • 9. Attenuation Coefficient (1)  Fraction of photons removed from a mono energetic beam of x-ray or gamma ray per unit thickness of material is called linear attenuation coefficient (µ), typically expressed in cm-1 .  Number of photons removed from the beam traversing a very small thickness ∆x: µ x n = N∆ where n = number removed from beam, N = number of photons incident on the material, and minus sign is placed before μ to indicate that no. of photons decreases as the absorber thickness increases.
  • 10. Attenuation Coefficient (2)  For a mono energetic beam of photons incident on either thick or thin slabs of material, an exponential relationship exists between number of incident photons (N0 ) and those transmitted (N) through thickness (x) without interaction: −µ N =N e 0 x  The number of photons indicate the Intensity of the beam and can also be written as ( I ).
  • 11. Attenuation Coefficient (3)  Total Linear attenuation coefficient is the sum of individual linear attenuation coefficients for each type of interaction: µ = µRayleigh + µphoto + µCompton + µpair  For a given thickness of material , probability of interaction depends on number of atoms the x ray or gamma ray encounter per unit distance. The density (ρ ) of material affects this number.  Linear attenuation coefficient is proportional to the density of the material.
  • 12. Mass Attenuation Coefficient  For a given thickness probability of interaction is dependent on the number of atoms per volume.  This dependency can be overcome by normalizing linear attenuation coefficient for density of material –  Mass Attenuation Coefficient (μ / ρ ) = Linear attenuation coefficient Density of the material  Mass attenuation coefficient is independent of density of the material.
  • 13. Half Value Layer (1)  Half value layer (HVL) defined as thickness of material required to reduce intensity of an x-ray or gamma-ray beam to one-half of its initial value.  It is an indirect measure of the photon energies (also referred to as quality or penetrability) of a beam of radiation.  For mono energetic photons, the probability of attenuation remains the same for each additional HVL thickness placed in the beam.  Relationship between μ and HVL: HVL = 0.693/μ
  • 15. List of Interactions Attenuation of a photon beam by an absorbing material is caused by 5 major types of interactions – 2. Coherent Scattering 3. Photoelectric Effect 4. Compton Effect 5. Pair Production 6. Photonuclear Effect
  • 16. Coherent Scattering  X-rays passing close to the atom cause the bound electrons to vibrate momentarily at a frequency equal to that of the radiation. These in turn emit radiation of the same frequency in all directions .  The energy is taken up from the beam and scattered in all direction, but none of the energy is absorbed. Thus this is a form of attenuation without absorption .  This interaction is of little importance in practical radiotherapy, but is important in X-ray crystallography .  Since it involves bound electrons, it occurs more in higher atomic number materials, and also more with low-energy radiations.
  • 17.
  • 18. Photoelectric Effect (1)  All of the incident photon energy is transferred to an electron, which is ejected from the atom.  Kinetic energy of ejected electron called the photoelectron (EC ) is equal to incident photon energy (EO ) minus the binding energy of the orbital electron (EB ) EC =EO - EB
  • 19.
  • 20. Photoelectric Effect (3)  Incident photon energy must be greater than or equal to the binding energy of the ejected photon.  The ionized atom regains electrical neutrality by rearrangement of the other orbital electrons. The electrons that undergo these rearrangements surrender some of the energy in form of a photon known as the characteristic radiation of the atom.  Absorption of these characteristic radiation internally in the atom may result in emission of Auger electrons . These electrons are mono energetic in nature.
  • 21. Photoelectric Effect (4)  Probability of photoelectric absorption per unit mass is approximately proportional to 3 3 Z /E  Energy dependence explains, in part, why image contrast decreases with higher x-ray energies.  Process can be used to amplify differences in attenuation between tissues with slightly different atomic numbers, improving image contrast.
  • 22. Photoelectric Effect (5)  Graph of probability of photoelectric effect, as a function of photon energy, exhibits sharp discontinuities called absorption edges .  Photon energy corresponding to an absorption edge is the binding energy of electrons in a particular shell or sub shell .  The phenomena of absorption edges is important for two different reasons:1) At these absorption edges, low-energy photons are less attenuated and therefore more penetrating than high energy photons. 2)A substance is relatively transparent to its own characteristic radiation. This effect is important when filters are considered as the filters will be “transparent” to their own characteristic radiation.
  • 23.
  • 24. Compton Effect (1)  Photon interacts with an atomic electron as though it were a free electron. Practically this means that energy of the incident photon must be large compared with the electron binding energy.  The electron receives some energy from the photon and is emitted at an angle Φ while the photon with reduced energy is scattered at an angle θ .
  • 26.
  • 27. Compton Effect (4)  As incident photon energy increases, scattered photons and electrons are scattered more toward the forward direction.  Probability of interaction increases as incident photon energy increases.  Probability also depends on electron density ( no. of electrons per gram of matter ).  Electron density fairly constant in tissue.  Probability of Compton scatter/unit mass independent of Z.
  • 28. Compton Effect (5)  Maximum energy of photons with 90° scatter is 0.511 M e V while that for 180° scatter ( i.e.. Back scatter) is 0.255 M e V.  Energy of the photons scattered at angles <90 ° will be more than 0.511 M e V and will gradually approach the incident photon energy.  Energy of the scattered radiation is independent of the incident beam energy .This implies that as the photon energy increases there is a corresponding increase in the forward scatter of the beam. This results in better dose distribution.  Direction of the scatter depends on the energy of the incident photon beam . This means that higher beam energies allow greater absorption of the dose in the body with less scattering of energy.
  • 29. Compton Effect (6)  If the angle by which the electron is scattered is θ and the angle by which the photon is scattered is Φ, then the following formula describes the change in the wavelength ( δ λ )of the photon: λ 1 – λ 2 = δ λ = 0.024 ( 1- c o s Φ) Å  Thus the wavelength change depends neither on the material being irradiated nor on the radiation energy, but only upon the angle through which the radiation is scattered.  The Compton effect results in both attenuation and absorption .
  • 30. Compton Effect (7)  Laws of conservation of energy and momentum place limits on both scattering angle and energy transfer.  Maximal energy transfer to the Compton electron occurs with a 180-degree photon backscatter.  Scattering angle for ejected electron cannot exceed 90 degrees.  Energy of the scattered electron is usually absorbed near the scattering site.
  • 31. Pair Production (1)  When the photon with energy in excess of 1.02 M e V passes close to the nucleus of an atom, the photon disappears, and a positron and an electron appear. This effect is known as pair production.  Pair production results in attenuation of the beam with absorption.  The positron created as a result loses its energy by interaction with an electron to give rise to two annihilation photons, each having 0.511 M e V energy. Again because momentum is conserved in the process two photons are rejected in opposite directions. This reaction is known as an annihilation reaction.
  • 32.
  • 33. Pair Production (3)  Pair production results from an interaction with the electromagnetic field of the nucleus and as such the probability of this process increases rapidly with the atomic number (Z 2 ).  In addition, the likelihood of this interaction increases as the photon energy increases, in contrast to the Compton effects and the photoelectric effect.
  • 34. Photonuclear Reaction  This reaction occurs when the photon has energy greater than the binding energy of the nucleus itself. In this case, it enters the nucleus and ejects a particle from it. The photon disappears altogether, and any energy possessed in excess of that needed to remove the particle becomes the kinetic energy of escape of that particle.  The threshold energy for this effect is 10.8 M e V.  The main use of this reaction is for energy calibration of machines producing high energy photons.
  • 35. Relative Importance of the Various Processes The relative importance of the 3 principal modes of interaction pertinent to radiation therapy- the Photoelectric , Compton and Pair production processes - as a function of Incident beam energy and Atomic number of absorber matter shows - For an absorber with Z approximately equal to that of soft tissue - 7 , and for mono energetic photons , Photoelectric effect is the dominant interaction below about 30 k e v. Above 30 k e v Compton effect remains dominant and remains so, Until about 24 M e v , after which Pair Production effect becomes dominant .
  • 37. Relative Importance of the Various Processes (3)  In a graph plotted for total mass attenuation coefficient vs. photon energy it is seen that -  The μ /ρ is large for low energies and high Z media (eg. Lead ) because of the predominance of Photoelectric interactions under these conditions. The μ /ρ decreases rapidly with energy until the photon energies far exceed the electron binding energies and Compton effect becomes the predominant mode of interaction.  In the range of Compton effect the μ /ρ of lead and soft tissues do not vary greatly as Compton effect is independent of Z .The μ /ρ however decrease with energy until Pair production becomes important .
  • 38. Plot of total mass att. Coef. As a function of photon energy
  • 39. Part 3 : Interaction of Particle Radiation with Matter Interaction of Electrons with matter – The two different modes of interaction and energy transfer of electrons with matter include:  Collision between the particle and the electron cloud resulting in ionization and excitation ( more important in low atomic number elements). This is called Collisional loss .  Collision between the nucleus and the particle resulting in bremsstrahlung radiation (more in high atomic number elements). This is called Radiative loss .
  • 40. Electron Interactions  The ionization pattern produced by a beam of electrons is characterized by a constant value from the surface to a depth equal to about half the range, followed by a rapid falling off to almost zero at a depth equal to the range . The bremsstrahlung radiation produced when electrons slow down contributes to an insignificant dose beyond the range of any electron. This is specially seen in electrons in the energy range of 6 -15 M e V .  These characteristics make electrons a useful treatment modality for superficial lesions.
  • 41. Proton & Pi Meson Interactions  Protons and pi mesons are charged particles that are being used in experimental set-ups only.  These particles have a very high linear energy transfer (LET) that is they have a very high ionization density( Amount of energy deposited per unit path length is called the linear energy transfer (LET) ).  Further, these charged particles also exhibit the phenomena of Bragg’s peak which refers to the increased ionization occurring near the end of the track with little effect beyond.
  • 42. Neutron Interactions • Neutrons are indirectly ionizing uncharged radiations, which interact only with the nucleus in two ways:  By recoiling protons from hydrogen and the nucleus in other elements.  Nuclear disintegration , which contribute to ~30% of the total dose in tissues.
  • 43. Part 4 : Practical Implications The three major forms of interaction of radiation with matter, which are of clinical importance in radiotherapy are:  Compton effect.  Photoelectric effect.  Pair production. Out of these, the Compton effect is the most important in modern-day megavoltage radiation therapy. The reduced scattering suffered by high-energy radiation as well as the almost homogeneous tissue dosage is primarily due to the Compton effect.
  • 44. Practical Implications  Coherent scattering is of little importance in practical radiotherapy, but is important in X-ray crystallography .  The photoelectric effect has several important implications in practical radiology:  In diagnostic radiology , the primary mode of interaction is photoelectric. It is also responsible for the contrast effect.  In therapeutic radiology , low-energy beams in orthovoltage irradiation causes excessive absorption of energy in bone.
  • 45. Practical Implications  The attenuation produced by the Compton effect is described by the mass scattering coefficient ( σ / ρ ), and is practically same for all substances except hydrogenous material, like water and soft tissue, where the Compton effect is greater (because of the higher electron density).  Attenuation does not depend on the atomic number of absorber matter in Compton effect.  Thus concrete is as good as lead in shielding of megavoltage equipment!  The absorption in bones does not exceed that produced in the soft tissues – unlike in PE effect seen in orthovoltage radiation era.  Port films produced in megavoltage equipment have very little detail.
  • 46. Practical Implications  The low mass of the electron leads to greater scattering. This is of practical importance as radioactive isotopes which are produce high energy beta radiation are better stored in low atomic number materials e.g. plastics as they will lead to lesser bremsstrahlung radiation.  Also higher atomic number elements are better for x ray production. The amount of radiative loss is proportional to the square of the atomic number of the material This leads to the phenomenon of greater ionization in soft tissues relative to bones. Ionization and excitation are more for low atomic materials.
  • 47. Practical Implications  Protons and Heavy particle beams have the ability to concentrate dose inside the target volume and minimize dose to surrounding normal tissues because of the Bragg peak effect and minimal scattering.  However there are several practical and theoretical difficulties with the use of these charged particles. Some of them include:  The narrow Bragg peak makes a homogenous Tumor Dose difficult.  Generation of these charged particles requires expensive and large machines.  The method of the production ensures that the field size is very narrow. So, for treatment of cancers the beam has to be scanned back and forth across the treatment area.
  • 48. Practical Implications  Hydrogenous materials like fats absorb neutrons more than heavier materials and thus there is a 20% greater absorption in fat relative to muscle.  Lower atomic materials (e.g. fats and paraffin) are better for neutron shielding as compared to lead as greater absorption occurs.  Neutrons, being uncharged particles also penetrate deeply into matter.  But neutrons are not commonly used in practical radiotherapy, because of technical difficulties in production of these beams as well as their complicated dosimetry.
  • 49. Part 5 : Conclusion  Despite several decades of research, photon- beam still constitute the main therapeutic modality in radiotherapy, because of several unresolved technical problems with the use of particulate radiation.