Ionizing Radiation: Particle Interaction Flashcards
What are some examples of charged and uncharged particles?
Alpha particles (α2+ or He2+), protons (p+), beta particles (β−), positrons (β+), and electrons (e−) are some examples of charged particles. Photons (ie, X-ray and gamma-ray), neutrons, and neutrinos are some examples of uncharged particles.
What are the three types of interactions that a charged particle can have with the matter?
There are excitation, ionization, and bremsstrahlung. Excitation and ionization are interactions of the charged particle with the orbital electrons. Bremsstrahlung is an interaction of the charged particle with the nucleus.
What is the difference between excitation and ionization?
The main difference between excitation and ionization is whether an orbital electron is ejected from the atom. In excitation, the transferred energy does not exceed the binding energy of the electron, so the electron is raised to a higher energy level without actual ejection. In ionization, the transferred energy exceeds the binding energy of the electron, so the electron is ejected from the atom.
What are some examples of ionizing and nonionizing radiations?
X-rays, gamma-rays, electrons, protons, alpha particles, and neutrons are some examples of ionizing radiation. Microwaves, radio waves, and optical photons are some examples of nonionizing radiation.
What are the differences between directly and indirectly ionizing radiation?
Directly ionizing radiation comes from charged particles (eg, protons, electrons, and alpha particles) and indirectly ionizing radiation from uncharged particles (eg, photons and neutrons).
What are delta rays?
Delta rays are secondary electrons with sufficient energy to travel a significant distance away from the primary radiation beam and produce further ionization (ie, secondary ionization).
What is specific ionization (SI)?
The average number of primary and secondary ion pairs produced per unit length of the charged particle’s path is called the SI. SI is often expressed in units of ion pairs per mm (IP/mm).
What is the Bragg peak?
As a charged particle travels through matter, it loses velocity causing its specific ionization (SI) to increase to a maximum (called the Bragg peak) when it stops. The SI drops off rapidly after the proton has deposited its energy.
What is the difference between the path length and range of a particle?
The path length of a particle is the distance that the particle travels, while the range of a particle is the depth of penetration of the particle in matter. The path length of an individual electron almost always exceeds its range, while the path length of a heavy charged particle (eg, alpha particles) is essentially equal to its range.
What is the linear energy transfer (LET)?
the average amount of energy deposited locally in matter per unit path length. LET is often expressed in units of keV per μm (keV/μm).
What is the dependence of linear energy transfer (LET) on the charge (Q) and kinetic energy (Ek) of the incident charged particle?
The LET of a charged particle increases with Q^2 and decreases with E . Thus, LET ∝ Q^2/E .
What are some examples of high linear energy transfer (LET) and low LET radiation?
Alpha particles, protons, and neutrons are examples of high LET radiation. Electrons, X-rays, and gamma-rays are examples of low LET.
What is a bremsstrahlung X-ray?
As an electron interacts with an atomic nucleus, it is deflected and decelerated by the positively charged nucleus, with a loss of kinetic energy as emission of bremsstrahlung X-rays. Bremsstrahlung is a German word meaning “braking radiation.”
What is the dependence of bremsstrahlung on the atomic number (Z) of the absorber and the mass (m) of the incident particle?
Total bremsstrahlung emission per atom increases with Z^2 and decreases with m^2. Thus, bremsstrahlung ∝ Z^2/m^2.
What is positron annihilation?
A positron interacts with an electron at the end of its range, resulting in the annihilation of the electron–positron pair and the conversion of their rest mass to energy in the form of two oppositely directed 0.511 MeV photons.