2 X-ray Interactions Flashcards
The number of electrons each shell
–The number of electrons each shell can contain is 2n2.
The electron density of a substance
–The electron density of a substance is ρ N0(Z/A) electrons/cm3, where ρ is the density measured in grams per cubic centimeter (g/cm3) and N0 is Avogadro’s number.
Z/A is equal to
–For most atoms making up tissues (e.g., oxygen, carbon, nitrogen, calcium), Z/A is equal to 0.5.
The electron binding energy
–The energy required to completely remove an electron from an atom.
Characteristic x-ray
–Electrons moving from an outer shell to an inner shell may emit excess energy as electromagnetic radiation.
Auger electron
–The excess energy may be transferred to an Auger electron, which then leaves the atom.
–Auger electron energy is the characteristic x-ray energy minus the binding energy of the outer shell electron.
Ionization
–Ionization occurs when an electron is ejected from a neutral atom, leaving behind a positive ion.
Directly ionizing
–Radiation is directly ionizing when it is in the form of charged particles.
–Electrons and protons are both directly ionizing radiations.
Excitations
–Energy lost from energetic particles can eject electrons from atoms or raise atomic electrons to more distant atomic shells.
Indirectly ionizing
–Uncharged particles are indirectly ionizing.
–Neutrons are indirectly ionizing radiations that interact with matter by first transferring energy to protons.
–Indirectly ionizing radiations include x-rays, and gamma rays.
Three ways that diagnostic energy x-rays interact with matter
–Three ways that diagnostic energy x-rays interact with matter are (i) coherent scatter, (ii) photoelectric (PE) effect, and (iii) Compton scatter.
Coherent scatter
–Coherent scatter occurs when a low-energy x-ray photon is scattered from an atom without any energy loss.
–The wavelength of the scattered photon is the same as the wavelength of the incident photon.
–Coherent scatter is referred to as Rayleigh or classical scatter.
Photoelectric effect
–This occurs between tightly bound (inner shell) electrons and incident x-ray photons.
–The x-ray photon is totally absorbed by an inner shell electron and that electron is ejected from the atom.
–X-ray photons absorbed in PE interaction therefore “disappear”.
–As a result of the photoelectric interaction, a photoelectron is emitted and a positive atomic ion is left behind.
–The energy of the emitted photoelectron equals the difference between the incident photon energy and the electron binding energy.
–The photoelectron loses energy by ionizing other atoms in the tissue and contributes to patient dose.
Auger electron
–Outer shell electrons fill the inner shell electron vacancies, with the excess energy emitted as a characteristic x-ray or Auger electron.
–Auger electron energy is slightly lower than the characteristic x-ray energy.
Photoelectric effect probability
–Above the K-edge, photoelectric interactions are proportional to 1/E3.
–The probability of photoelectric absorption increases with atomic number and is proportional to Z3.
Compton scatter
–Incident photons interact with outer shell electrons.
–A Compton interaction results in a scattered photon that has less energy than the incident photon and generally travels in a different direction.
–A scattered (ejected or recoil) electron carries the energy lost by the incident photon as kinetic energy.
Compton interaction probability
–Electron density.
–Physical density.
–(1/E).
The linear attenuation coefficient (μ)
–The fraction of incident photons removed from the beam in traveling unit distance.
–Expressed in inverse centimeters (cm−1).