Interactions of Radiation and Matter Flashcards

1
Q

What three (general) processes occur when an x-ray beam interacts with a patient, and what do they cause?

A

Transmission - Forms image
Scattering - Staff Dose
Absorption - Patient Dose

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2
Q

State and explain the equation for Exposure (X).

A

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

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3
Q

State and explain the equation for Absorbed Dose (D).

A

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.

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4
Q

Explain how to go from Exposure to Dose in Air.

A

X = Q/m
X/e = No. Ion pairs produced
W - average energy to produce 1 ion pair.
E = W(X/e)

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5
Q

What two assumptions are needed to equate KERMA to absorbed dose-in-air?

A
  • Negligible Bremsstrahlung

- Short electron ranges

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6
Q

How is dose in air converted to dose in another medium?

A

D(m)/D(a) = u/p/u/p
u - mass attenuation coefficient for the medium
p - density of the medium

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7
Q

Explain the photoelectric effect.

A

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.

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8
Q

How does the photoelectric effect change with increasing atomic number?

A

Proportional to Z^3

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9
Q

How does the photoelectric effect change with increasing energy?

A

Proportional to 1/E^3

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10
Q

What is the name of an outer shell electron emitted instead of the photon through the photoelectric effect?

A

Auger Electron

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11
Q

What is the equation for fluorescent yield (probability of no Auger Electrons)?

A

w = no of k x-ray photons/no of k shell vacancies

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12
Q

Explain compton scattering.

A

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.

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13
Q

What is the change in wavelength from compton scatter?

A

Δλ = (h/mc)*(1-cosθ)

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14
Q

What is the change in energy from compton scatter?

A
ΔE = E(0)*[α(1-cosθ)/(1 + α(1-cosθ))]
α = E(0) (in MeV)/0.511
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15
Q

How does compton scatter change with increasing energy?

A

Constant (below 100keV)

Proportional to 1/E (above 100keV)

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16
Q

How does compton scatter change with increasing Z

A

Independent of Z.

17
Q

Explain elastic scattering.

A

Whole atom absorbs recoil
Bound electrons vibrate at frequency of photons
Electrons re-radiate energy at same frequency as photon
Scattering in forward radiation
Less than 10% of interaction - of little practical importance
Proportional to (Z^2)/E

18
Q

Explain pair procuction.

A

High energy (>1.02MeV) photon produces an electron-positron pair.
Positron annihilates with a local free electron.
Produces two photons (0.511MeV) in opposite directions.
Proportional to E-1.02 and Z

19
Q

Explain how k edge matching is used in X-Ray imaging

A

Match detector/contrast material with k-edge at peak of x-ray spectrum.
Maximises absorption, (k-shell electrons can now be emitted) for fewer photons.
Lower dose to patient for same image quality.