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Attenuation is?
The reduction of energy (e.g x-ray) as it passes through a medium or tissue.
Linear attenuation coefficient (μ) is?
The measure of a material’s ability to attenuate an x-ray beam per unit thickness.
Thickness (cm) is a linear quantity
Large μ = high % of attenuation per cm
Low μ = vice versa
The total linear attenuation of coefficient is ?
The fraction of x-ray removed from the beam per unit thickness of the irradiated beam.
Mass attenuation coefficient (μ/p) is?
Linear attenuation coefficient (μ) divided by density of a material (p)
μ measured in cm2 a
p measured in g.
Each x-ray interaction has a linear attenuation coefficient and mass attenuation coefficient
Mass attenuation coefficient for PE, Compton scatter, and pair production
(μ/p)PE, (μ/p)C, (μ/p)PP
What is the total mass attenuation equal to?
(μ/p)TT = (μ/p)PE + (μ/p)C + (μ/p)PP
Photoelectric absorption
x-ray hits inner shell electron (usually k-shell)
X-ray is completely absorbed
When x-ray energy is more than binding energy of electron the electron is ejected from the atom (photo-electron)
Usually followed by characteristic x-ray emission
What increases PE occuring?
High atomic number of absorbing material
Decreases with increased x-ray photon energy.
Compton Scattering interactions explained
x-ray hits outer shell electron
x-ray is scatter and changes direction with less energy, some energy is transferred to electron which recoils
Electron energy = energy loss from x-ray
Scattered photon escapes target material or interacts again (PE or CS)
Compton scatter
X-ray is scattered angled 0-180 degrees
Small energy transfer from x-ray to electron = small scattering angle
Small incident x-ray energy = large scattering angle
Larger incident x-ray energy = smaller scattering angle
What increases probability of CS to occur?
High atomic number
Decreasing photon energy
Pair production
Incident x-ray passes close to the nucleus and interacts with nuclear field
X-ray absorption occurs and energy is converted to electron positron pair (E=mc2)
For PP to occur, x-ray energy must be 2× 0.511 MeV (1.02 MeV) this is the threshold energy
Energy greater than 1.02 MeV given to electron + positron as kinetic energy
Positron will annihilate with an electron and two gamma rays are produced at 180o
Attenuation of x- and y-rays
depends on thickness and type of absorber, I = I 0e-μx I
I = intensity of transmitted beam (W/m2)
I0 = initial intensity (W/m2)
μ = linear attenuation coefficient of absorber material (
x= thickness of absorber (cm)
can be rearranged for -ln (I/I0) = μx
Half value thickness or Layer (HVT/HVL)
Thickness of absorber required to attenuate 50% of incident beam. = HVT = ln2/μ
Tenth value thickness
Thickness of absorber required to attenuate 10% of incident beam.
TVT = ln10/μ
Electron interactions
electrons are charged particles with mass and interact differently to photons (x-rays and gamma rays)
Interact with the electric field (coloumb field) of other charged particles (protons and orbital electrons)
Through these collisions the electrons may lose some kinetic energy or scatter.
Electron interactions with orbital electrons
Inelastic collisions between the incident electron and orbital electron are coulomb interactions that result in
Atomic ionisation - ejection of orbital elctron from the absorber atom
Atomic excitation - the transfer of an atomic orbital electron from one shell) to a higher shell
Atomic ionisation and excitations cause energy loss for incident electron
Electrons lose energy in 1000s of collisions losing small amounts of energy until it is stopped.
Electron interactions with nucleus
THey may pass close to nucleus and experience loss of energy due to electrostatic force
This results in x-ray photon emission (aka bremsstrahlung)
The energy of the -ray photons is distributed over a range (max energy = energy of the incident e-_ and is dependent on how close the e- passes to the atomic nucleus
x-rays electrons and dose
Electrons cause energy to be deposited in a material e.g tissue
X-ray interact through CS, PE, and PP
Results in electron
The electron then travels soem small distance losing energy along its track in multiple energy loss collisions (ionisation or excitation with orbital electrons)
Also radiative losses (bremsstrahlung from the nucleus)