Interactions of Radiation and Matter Flashcards
What three (general) processes occur when an x-ray beam interacts with a patient, and what do they cause?
Transmission - Forms image
Scattering - Staff Dose
Absorption - Patient Dose
State and explain the equation for Exposure (X).
X = dQ/dm
X - The amount of radiation that produces, in air, ion of either sign equal to 1C/kg
dQ - The sum of all the charges (of all ions of one sign) produced when all electrons produced in a volume (dV) are stopped in air.
dm - The mass of air in volume dV
State and explain the equation for Absorbed Dose (D).
D = dE/dm
the energy absorbed per unit mass, measured in Gy (J/kg), need to specify the material in which the energy is absorbed.
Explain how to go from Exposure to Dose in Air.
X = Q/m
X/e = No. Ion pairs produced
W - average energy to produce 1 ion pair.
E = W(X/e)
What two assumptions are needed to equate KERMA to absorbed dose-in-air?
- Negligible Bremsstrahlung
- Short electron ranges
How is dose in air converted to dose in another medium?
D(m)/D(a) = {uen/p}(m) / {uen/p}(a)
uen - mass energy absorption coefficient for the medium
p - density of the medium
Explain the photoelectric effect.
X-Ray photon transfers all energy to inner (k) shell electron
Electron liberated with energy of photon - binding energy
Vacancy in k-shell filled by outer electron
Characteristic X-ray emitted (may be absorbed locally in low z material)
Dominant at lower energies.
How does the photoelectric effect change with increasing atomic number?
Proportional to Z^3
How does the photoelectric effect change with increasing energy?
Proportional to 1/E^3
What is the name of an outer shell electron emitted instead of the photon through the photoelectric effect?
Auger Electron
What is the equation for fluorescent yield (probability of no Auger Electrons)?
w = no of k x-ray photons/no of k shell vacancies
Explain compton scattering.
Photon incident on “free” electron
Photon scatters at reduced energy
Electron recoils from collision
Change in photon energy depends on initial energy and angle of scatter.
What is the change in wavelength from compton scatter?
Δλ = (h/mc)*(1-cosθ)
What is the change in energy from compton scatter?
ΔE = E(0)*[α(1-cosθ)/(1 + α(1-cosθ))] α = E(0) (in MeV)/0.511
How does compton scatter change with increasing energy?
Constant (below 100keV)
Proportional to 1/E (above 100keV)