Intro to radiation physics

NHS University Hospitals Coventry and Warwickshire NHS Trust Introduction to Radiation

Page 2:

  • Learning Outcomes:

    • Review atomic & nuclear structure

    • What is radiation

    • Types of radiation

    • Waves and particles

    • Interactions between radiation and matter

Page 4: Atomic Scale

    • Everything is made of atoms

    • Atoms can combine to make molecules in a highly predictable way

Page 5: Atomic Structure

    • Bohr Model of the atom

    • Electrons arranged in shells

    • Size of atom, nucleus, and their ratio

    • Comparison with astronomy

Page 6: Sub-atomic particles

    • Protons: positive charge, mass

    • Neutrons: neutral charge, mass, holds the nucleus together

    • Electrons: negative charge, mass

Page 7:Electron Shells

    • Innermost shell is K shell, can support two electrons

    • Second shell is L, can support eight electrons

    • Third shell is M, can support eight electrons (plus an extra 8)

    • Outermost shell is the valence shell

Page 8: Periodic Table

    • Groups elements with similar chemical properties together

    • Nomenclature: Element, Atomic Number, Mass Number

    • Elements form chemical bonds to create stable molecules

Page 10: Stable Atoms / Molecules

    • A stable atom has a complete outermost electron shell

    • Chemical reactions occur when atoms exchange electrons

    • Elements in column 8 are found naturally, others form chemical bonds

Page 12: Excitation and Ionisation

    • Electrons closest to the nucleus are most tightly bound

    • Excited atom: electron moves to another shell, atom has extra energy

    • Ionisation: electron leaves the atom, atom becomes positively charged

Page 13:

  • Brief summary so far:

    • Quick refresher on atoms and atomic structure

    • Different types of atoms and their differences

    • Atomic stability and the role of electrons

    • How atoms combine to become stable molecules

    • Excitation and Ionisation

Page 14: Radiation

    • Definition of radiation

    • Emission of energy as electromagnetic waves or moving subatomic particles

Page 15:

  • Particles:

    • Moving particles have kinetic energy

    • Faster and heavier particles have more energy

  • Waves:

    • Also carry energy

Page 16 :Electromagnetic Radiation

    • Cell Phone frequencies

    • Non-ionizing and ionizing radiation

Page 17: EM Radiation

    • Electromagnetic waves consist of rapidly oscillating electric and magnetic fields

    • Transverse wave with oscillations at right angles to the direction of motion

    • Wavelength, frequency, and velocity of electromagnetic waves

Page 18: Features of waves

    • Low and high frequency

    • Speed of light is fixed at 300,000 km/s

    • If frequency increases, wavelength decreases

Page 19: Dual Nature of EM radiation

    • EM radiation can be both a wave and a particle

    • Photons are particles of EM radiation

    • Photons have discrete bundles of energy called quanta

    • Photons have no mass and travel at the velocity of light

Page 20: Electromagnetic Radiation - Photons

    • Increasing frequency leads to increasing photon energy

Page 21: Intensity of EM Radiation

    • Intensity is the total energy per second flowing past unit area

    • Inverse Square Law: Energy spreads over an ever-widening area

Page 22: Excitation and Ionisation

    • Excitation and ionization are processes that occur when radiation passes through matter

    • Excitation involves raising electrons to higher energy levels

    • Ionization involves removing electrons from atoms or molecules

Page 23: Attenuation

    • Radiation passing through matter is attenuated (reduced in intensity)

    • Attenuation follows an exponential decay law

    • Equal thicknesses of matter absorb equal fractions of incident radiation

    • Half value layer (HVL) is the thickness of material required to attenuate X-rays by 50%

Page 24: Scatter and Absorption

    • X-ray beams passing through matter are attenuated through absorption and scatter

    • Absorption involves the removal of X-ray photons from the beam and deposition of energy in matter

    • Scatter involves the removal of X-ray photons from the beam and change in direction, with some absorption involved

Page 26:

  • Summary

    • Identified radiation as particles or waves

    • Discussed properties of radiation

    • Discussed interchangeability between particles and waves

    • Discussed spreading of radiation with distance

    • Discussed interactions of waves or particles with matter

P

age 27:

  • Interactions between Photons and Matter

    • No specific details mentioned

Page 28: Coherent or Elastic Scatter

    • Elastic scatter occurs when an incident photon passes close to an electron, causing it to vibrate and absorb the photon

    • The vibrating electron re-radiates the photon in a different direction, resulting in scatter without absorption

    • This process occurs at low photon energies (1-30 keV)

    • Interaction probability is inversely proportional to energy and proportional to the square of the atomic number (Z)

Page 29: Compton Scatter

    • Compton scatter occurs when an incident photon bounces off a free electron, reducing its energy and changing its direction

    • This process results in scatter and absorption

    • Interaction probability gradually decreases with increasing energy

    • Interaction probability depends on electron density, which is similar for most materials and independent of atomic number (Z)

Page 30: Photoelectric Effect

    • The photoelectric effect occurs when an incident photon is totally absorbed by a bound electron, causing ionization

    • This process results in absorption

    • Interaction probability is proportional to the cube of the atomic number (Z) and inversely proportional to energy

Page 31: Pair Production

    • Pair production occurs when a photon turns into an electron and a positron in the presence of a nucleus

    • This process results in absorption

    • Requires high energy (1.02 MeV) incident photons

    • Interaction probability is independent of energy and atomic number (Z)

Page 32: Interaction Probabilities

    • Interactions between photons and matter are random

    • Different conditions favour different interactions, including photon energy and tissue type

    • Rarely, an electron can be fully stopped, releasing all its energy and producing a spectrum of X-ray energies

Page 33: Interaction Probabilities

    • Lead has a K-edge at 88 keV

    • Iodine has a K-edge at 33 keV

Page 34: Interactions between Electrons and Matter

    • Electrons interact with electrons in shells and the nucleus

    • Electrons in shells repel the incident electron

    • Protons in the nucleus attract the incident electron

Page 35:Interactions between Electrons and Matter

    • Electrons are repelled by electrons in the electron cloud, causing deflection and energy transfer

    • This can result in scatter with some absorption

    • Incident electrons can occasionally interact with a nucleus, leading to attraction

Page 36:Bremsstrahlung

    • Bremsstrahlung occurs when an electron is deflected by the electrostatic attraction of a nucleus, resulting in the release of a single X-ray

    • Rarely, the electron is fully stopped, releasing all its energy and producing a spectrum of X-ray energies

Page 37:

  • Overall summary

    • Review of atomic and nuclear structure

    • Radiation is the transfer of energy

    • Types of radiation include waves and particles

    • Dual nature of radiation

    • Interactions between radiation and matter include elastic scatter, Compton scatter, photoelectric effect, pair production, and bremsstrahlung

Page 38:

  • Learning Outcome

    • No specific details mentioned