INTERACTIONS OF IONIZING RADIATION WITH MATTER
absorbed dose - energy deposited per unit mass of medium
em radiations: x rays and gamma rays
particulate radiations: electrons, protons, alpha particles, heavy charged particles
charged particles - directly ionizing radiation
em radiations, neutrons - indirectly ionizing radiation
E<13.6eV are non-ionizing
average energy to produce an ion pair in air is 33.85eV (W)
specific ionization is the number of ion pairs produced per unit track length (SI)
linear energy transfer is the average loss in energy per unit length of path of the incident radiation (units of kV/m) (LET)
LET = SI * W
narrow beam attenuation: N = N_0*exp(-mu*x) — multiply by B(x, hv, A, L) for broad beam
mu is linear attenuation coefficient - fraction of photons that interact per unit thickness of attenuator (units 1/cm)
thickness that attenuates beam to 50% is HVL
HVL = ln2 / mu
N = N_0 * 2^(-x / x_h)
TVL = ln10 / mu — use in radiation protection shielding calculations
N = N_0×10^(-x / x_t)
only mono-energetic beams can be characterized by a single value of HVL, but linac is mono
fraction “g” of energy is lost, especially in MeV range — E_ab = E_tr * (1 - g)
photons are absorbed by photoelectric effect, compton scattering, pair production, photonuclear itneractions, coherent scattering
charged particles interact through coulomb force of atom or nuclear (soft and hard collisions, nuclear interactions of heavy charged particles)
neutrons interact with nuclei of atoms
photoelectric effect - collision between photon and atom results in ejection of a bound electron
photon disappears and is replaced by an electron efected from the atom with kinetic energy KE = hv - E_b
highest probability if the photon energy is just above the binding energy of the electron
additional energy may be deposited locally by auger electrons and/or fluorescence photons
electron tends to be ejected at 90 degrees for low energy, goes to 0 as energy increases
interaction probability = Z³/(hv)³
coherent scattering
no energy is converted to KE, all is scattered
bnroadens the angular width of beam slightly
negligibly small for energies greater than 100keV in low atomic number materials
photon is scattered by combined action of whole atom
photons do not lose energy, just get redirected through small angle
compton scattering
interaction between photon and electron, independent of Z, increases with E
some energy scattered, some transferred to electron, depending on angle of emission of scattered photon and energy
in soft tissue it is most important for photons in 100keV to 10MeV range
inelastic scattering - energy and momentum are conserved
pair production
photon is absorbed giving rise to electron and positron
threshold energy is 1.022 MeV
can get triplet production at 2.044 MeV
energy transferred is KH = hv - 1.022
attenuation coefficient per unit mass depends on Z
photonuclear reaction
energy of a photon incident on a target atom is greater than the nucleon binding energy, typically 8-10MeV, depends on atomic number and incident beam energy
PLEASE MEMORIZE THE ENERGY VS Z GRAPH FOR WHICH PROCESS IS MOST LIKELY - goes in order of photoelectric, compton, pair production
photoelectric provides high contrast at low imaging energies
interactions of neutrons
elastic collisions with hydrogen nuclei account for most of energy deposited in tissue by neutrons with KE<10MeV
for neutrons with KE>10MeV, inelastic scattering with nuclei other than hydrogen also contributes to energy lost in tissue
energetic charged particles (protons/alpha particles) are often ejected from nuclei excited by inelastic interactions with neutrons
neutron fields can be fast (E>10keV), intermediate (0.5eV<E<10keV), or thermal (E<0.5eV)
thermal neutron interactions in tissue
neutron capture by nitrogen and neutron capture by hydrogen are most important
thermal neutrons have a larger probability of capture by hydrogen atoms in muscle because there are 41 times more H atoms than N atoms in tissue
BPE used to capture neutron in treatment bunker door
MEMORIZE TYPICAL NEUTRON ABSORPTION CROSS SECTION GRAPH
interactions by intermediate and fast neutrons
dominated below 100eV by (n,p) reactions, mostly in nitrogen
resonance peaks occur when the binding energy of a neutron plus the KE of the neutron are equal to the amount required to raise a compound nucleus from its ground state to one of quantum levels
above 100eV elastic scattering of hydrogen nuclei contributes nearly all of the kerma
charged particle interactions
all charged particles lose kinetic energy through Coulomb field interactions with charged particles (electrons or nuclei) of the medium
in each interaction typically only a small amount of particle’s KE is lost
typically undergo very large number of interactions, therefore can be roughly characterized by a common path length in a specific medium
charged particles are characterized by a range - a finite distance which can be calculated from stopping power in continuous slowing down approximation
slower moving particle (lower KE) transfers more energy in heavy charged particle interactions
mass collision stopping power - energy loss per unit track length in producing ionization in the absorbing medium
radiative stopping power - energy loss due to bremsstrahlung
no bremsstrahlung for heavy charged particles, only electrons
MEMORIZE PERCENT DEPTH DOSE GRAPH
MEMORIZE STOPPING POWER GRAPH
energy loss by radiation increases with atomic number and energy
ratio of radiation energy loss to energy lost by excitation and ionization is approximately E_k * Z / 820
in slowing down an electron may transfer all its energy in radiative recombination, resulting in a continuous spectrum with max energy equal to the electron kinetic energy
MEMORIZE BRAGG PEAK
slower moving charged particle (lower KE) transfers more energy, resulting in bragg peak at the end of its track
bragg peak is never observed for electrons due to their low lass, electrons constantly change direction as they slow down
MRI
earth’s magnetic field is 0.5 gauss
scanners are 1.5T or 3T
1T=10,000 gauss
MRI is based on imaging H2O molecule
source of signal in MRI is the nuclei of H atoms
a spinning hydrogen nucleus (proton) has magnetic field
billions of single-proton magnets in body in random directions cancel out
net magnetization in body normally is 0
under strong magnetic field, spins split about 50/50 parallel and antiparallel, with a few more parallel, making a small net magnetization M0
three features of M0:
M0 is spinning around the direction of main magnet B0
has T1 relaxation time
has T2 relaxation time
resonance is maximum transfer of energy from RF pulse to the net M0 when frequency of RF pulse equals the frequency of the M0
the z direction is the direction of the main uniform magnetic field B0
relaxation times are unique to each tissue
T1 is the time taken for spinning protons to realign with the external magnetic field
net magnetization is returning to equilibrium value through exponential process called T1 relaxation
T2 is the time taken for spinning protons to lose coherence among nuclei spinning perpendicular to the main field
net magnetization is dephasing (micromagnets repelling each other) through T2 relaxation process
each MRI voxel contains unique net magnetization
the intensity in each MR image voxel is proportional to proton density within that voxel
the intensity in each CT image voxel is proportional to electron density within that voxel
all net magnetizations for all tissues have the same spinning frequency
TE is echo time
TR is repetition time
MRI signal depends on T1, T2, proton density, TE, TR
CT
each tissue has unique attenuation coefficient
relationship between emitted x ray intensity and the attenuated intensity is exponential based on the attenuation coefficient
CT is based on the synchronization of xray tube and detector movement
scanning time now is 3s with image matrix 512
detector width less than 0.5mm
mu (probability of interaction of x ray photons with material) is linearly proportional to electron density
HU represent the different electron density levels of tissues relative to water electron density
water has 0HU, air is -1000HU
HU = 1000 * (mu - mu_water)/(mu_water) where mu is the attenuation coefficient
CT image is a gray scale presentation of HU of numerically solved mu of all materials within selected slice
x ray image is a projected image
CT image is a reconstructed image
window width determines image contrast
contrast detectability is the ability of the imaging system to resolve different objects from the noisy background when the difference in x ray attenuation between the objects and the background is small compared to noise
NUCMED
radioactivity is the process through which an unstable nucleus loses energy by emitting nuclear particles or ionizing radiation (gamma ray)
equation of radioactive decay: N = N_0 * exp(ln2 * t / T_1/2)
nuclear medicine imaging is a functional and quantitative
Tc99m → Tc99 + 140.5keVgamma
usually use parallel-hole collimator, pin-hole for thyroid and heart, converging for brain and heart
the collimator is mounted in the front of the camera crystal
collimators are made from lead
primary function of the collimator in gamma cameras is for accurate spatial localization
the signal in nuclear medicine imaging is the electrical current (output of the PMT)
use windowing to exclude lower energy photons
XRAY
xrays use 20keV-160keV for diagnostic imaging
kV: 25-140kV
tube current: 50-400mA
exposure time: 10-1000ms
xray tube focal spot: 0.1-1.2mm
x ray imaging is based on differential attenuation of xray photons
image spatial: display details of an object
S/N: not noisy image
image contrast: differentiate between objects
image artifacts: no image distortions
smaller focal spot improves image spatial
image radiographic contrast is the density different between neighboring regions on a plain xray radiographic image
lower kVp improves image contrast
increasing mA improves S/N
for optimal image, select options that allow for highest differential attenuation