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Interactions of Radiation With Matter Modified by D. Gamal Mahrous
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Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Jan 11, 2016

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Page 1: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Interactions of Radiation With Matter

Modified by D. Gamal Mahrous

Page 2: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Ionizing radiation is radiation that has sufficient energy to remove electrons from atoms, creating ions.

Ionizing radiation can be classified into two groups: photons (gamma and X-rays) and particles (alpha, beta, and neutrons(

Page 3: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Basic Concepts Of Interaction

Three possible occurrences when x or gamma photons in the primary beam pass through matter: No interaction at all

Known as transmission Absorption Scatter

The latter two are methods of attenuation

Page 4: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Attenuation

The reduction of gamma or x-ray photons as they pass through matterPrimary radiation – attenuation = remnant or exit radiation

Page 5: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Attenuation Of An X-Ray Photon

Page 6: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

The Five Interactions Of X and Gamma Rays With Matter

Photoelectric effect Very important in diagnostic radiology

Compton scatter Very important in diagnostic radiology

Coherent scatter Not important in diagnostic or therapeutic radiology

Pair production Very important in therapeutic&diagnostic radiology

Photodisintegration Very important in therapeutic radiology

Page 7: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Interaction probability

linear attenuation coefficient, μ,The probability of an interaction per unit distance traveledDimensions of inverse length (cm-1). N=No e- μ x

• The coefficient μ depends on photon energy and on the material being traversed.

Page 8: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Photoelectric Effect

All of the energy of the incoming photon is totally transferred to the atom Following interaction, the photon ceases to

exist

The incoming photon interacts with an orbital electron in an inner shell – usually KThe orbital electron is dislodgedTo dislodge the electron, the energy of the incoming photon must be equal to, or greater than the electron’s energy

Page 9: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Photoelectric Effect

The incoming photon gives up all its energy, and ceases to existThe ejected electron is now a photoelectronThis photoelectron now contains the energy of the incoming photon minus the binding energy of the electron shellThis photoelectron can interact with other atoms until all its energy is spentThese interactions result in increased patient dose, contributing to biological damage

Page 10: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Photoelectric Effect

Page 11: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Photoelectric Effect

A vacancy now exists in the inner shellTo fill this gap, an electron from an outer shell drops down to fill the gapOnce the gap is filled, the electron releases its energy in the form of a characteristic photonThis process continues, with each electron emitting characteristic photons, until the atom is stableThe characteristic photon produces relatively low energies and is generally absorbed in tissue

Page 12: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Photoelectric absorption (I-131)

Page 13: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

The Byproducts of the Photoelectric Effect

PhotoelectronsCharacteristic photons

Page 14: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

The Probability of Occurrence

Depends on the following: The energy of the incident photon The atomic number of the irradiated object It increases as the photon energy decreases, and

the atomic number of the irradiated object increases

When the electron is more tightly bound in its orbit When the incident photon’s energy is more or

close to the binding energy of the orbital electron This type of interaction is prevalent in the

diagnostic keV range – 30 - 150

Page 15: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

The Probability of Occurrence

The probability of photoelectric absorption, symbolized (tau), is

roughly proportional to (Z/E)3

Page 16: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

What Does This All Mean?

Bones are more likely to absorb radiation This is why they appear white on the film

Soft tissue allows more radiation to pass through than bone These structures will appear gray on the film

Air-containing structures allow more radiation to pass through These structures will appear black on the film

Page 17: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Compton Scattering

An incoming photon is partially absorbed in an outer shell electronThe electron absorbs enough energy to break the binding energy, and is ejectedThe ejected electron is now a Compton electronNot much energy is needed to eject an electron from an outer shellThe incoming photon, continues on a different path with less energy as scattered radiation

Page 18: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Compton Scatter

Page 19: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.
Page 20: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Byproducts Of Compton Scatter

Compton scattered electron Possesses kinetic energy and is capable of

ionizing atoms Finally recombines with an atom that has an

electron deficiency

Scattered x-ray photon with lower energy Continues on its way, but in a different

direction It can interact with other atoms, either by

photoelectric or Compton scattering It may emerge from the patient as scatter

Page 21: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Probability Of Compton Scatter Occurring

Increases as the incoming photon energy increases up to certain limit then decreases as the photon energy increases.The Compton process is most important for energy absorption for soft tissues in the range from 100 keV to 10MeV.Results:Most of the scattered radiation produced during a radiographic procedure

Page 22: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Coherent Scatter

Occurs at low energies – below 30 keVAn incoming photon interacts with an atomThe atom vibrates momentarilyEnergy is released in the form of an electromagnetic waveA combination of these waves form a scatter waveThe photon changes its direction, but no energy is transferredMay result in radiographic film fog

Page 23: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Rayleigh Scattering

Page 24: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Pair Production

Incoming photon must have an energy of at least 1.02 MeVThis process is a conversion of energy into matter and then matter back into energyTwo electrons are produced in this interaction

Page 25: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Pair Production

An incoming photon of 1.02 MeV or greater interacts with the nucleus of an atomThe incoming photon disappearsThe transformation of energy results in the formation of two particlesNegatron Possesses negative charge

Positron Possesses a positive charge

Page 26: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Pair Production

Page 27: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

PositronsConsidered antimatterDo not exist freely in natureCannot exist near matterWill interact with the first electron they encounterAn electron and the positron destroy each other during interaction Known as the annihilation reaction

This converts matter back into energyBoth the positron and electron disappearTwo gamma photons are released with an energy of .51 MeV

Page 28: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Pair Production

The produced gamma photons may interact with matter through pair production or Compton scatterPair production is used for positron emission tomography, a nuclear medicine imaging procedureIt is also used in radiation therapy

Page 29: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Pair production probability, symbolized (kappa),· Increases with increasing photon energy· Increases with atomic number approximately as Z2

Page 30: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Photoelectric effect dominant

Pair production dominant

Compton effect dominant

0.01 0.1

1

10

100

Z of absorber

Photon Energy, in Mev

Page 31: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Photodisintegration

Occurs at above 10 MeVA high energy photon is absorbed by the nucleusThe nucleus becomes excited and becomes radioactiveTo become stable, the nucleus emits negatrons, protons, alpha particles, clusters of fragments, or gamma raysThese high energy photons are found in radiation therapy

Page 32: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Photodisintegration

Page 33: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Gamma Knife

Page 34: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Interactions Of Particulate Radiation With Matter

Alpha radiation is monoenergeticBeta particles and positrons are also monoenergeticThese particles lose energy in the form of ion pairsAs they pass near or through a neutral atom, they remove energy through the force of attraction or repulsion

Page 35: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Interactions Of Particulate Radiation With Matter

Alpha particles ionize by attracting an electron from an atomBeta particles ionize by repelling an electron from an atom

Page 36: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Particle interactions

Energetic charged particles interact with matter by electrical forces and lose kinetic energy via:Excitation IonizationRadiative losses

Page 37: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Charged Particle Tracks

Electrons follow tortuous paths in matter as the result of multiple scattering events Ionization track is sparse and nonuniform

Larger mass of heavy charged particle results in dense and usually linear ionization trackPath length is actual distance particle travels; range is actual depth of penetration in matter

Page 38: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Path lengths vs. ranges

Page 39: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Linear Energy Transfer

Amount of energy deposited per unit path length is called the linear energy transfer (LET)Expressed in units of eV/cmLET of a charged particle is proportional to the square of the charge and inversely proportional to its kinetic energy(velocity)High LET radiations (alpha particles, protons, etc.) are more damaging to tissue than low LET radiations (electrons, gamma and x-rays)

Page 40: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Specific Ionization

Number of primary and secondary ion pairs produced per unit length of charged particle’s path is called specific ionization Expressed in ion pairs (IP)/mm

Increases with electrical charge of particleDecreases with increase incident particle velocity

Page 41: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Specific ionization for 7.69 MeV alpha particle from polonium 214

Page 42: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Bremsstrahlung

Probability of bremsstrahlung production per atom is proportional to the square of Z of the absorberEnergy emission via bremsstrahlung varies inversely with the square of the mass of the incident particle Protons and alpha particles produce less

than one-millionth the amount of bremsstrahlung radiation as electrons of the same energy

Page 43: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

Bremsstrahlung

Page 44: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

DIFFERENT DEGREES OF DECCELERATION

X-RAYS

HEAT

Page 45: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

X-rays are one of the main diagnostical tools in medicine X-rays are one of the main diagnostical tools in medicine since its discovery by Wilhelm Roentgen in 1895. since its discovery by Wilhelm Roentgen in 1895.

Current estimates show that there are approximately 650 Current estimates show that there are approximately 650 medical and dental X-ray examinations per 1000 patients per year. medical and dental X-ray examinations per 1000 patients per year.

X-rays are produced when high energetic electrons X-rays are produced when high energetic electrons interact with matter. interact with matter.

The kinetic energy of the electrons is converted into The kinetic energy of the electrons is converted into electromagnetic energy by atomic interactions (see chapter 7.1.)electromagnetic energy by atomic interactions (see chapter 7.1.)

Page 46: Interactions of Radiation With Matter Modified by D. Gamal Mahrous.

The X-ray tube provides an environment for X-The X-ray tube provides an environment for X-ray production via ray production via bremsstrahlungbremsstrahlung and characteristic and characteristic radiation mechanisms. radiation mechanisms.

electron source electron source

electron acceleration potential electron acceleration potential

target for X-ray production target for X-ray production

The classical X-ray tube requires:The classical X-ray tube requires: