2 X-ray Interactions Flashcards

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1
Q

The number of electrons each shell

A

–The number of electrons each shell can contain is 2n2.

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2
Q

The electron density of a substance

A

–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.

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3
Q

Z/A is equal to

A

–For most atoms making up tissues (e.g., oxygen, carbon, nitrogen, calcium), Z/A is equal to 0.5.

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4
Q

The electron binding energy

A

–The energy required to completely remove an electron from an atom.

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5
Q

Characteristic x-ray

A

–Electrons moving from an outer shell to an inner shell may emit excess energy as electromagnetic radiation.

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6
Q

Auger electron

A

–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.

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7
Q

Ionization

A

–Ionization occurs when an electron is ejected from a neutral atom, leaving behind a positive ion.

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8
Q

Directly ionizing

A

–Radiation is directly ionizing when it is in the form of charged particles.
–Electrons and protons are both directly ionizing radiations.

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9
Q

Excitations

A

–Energy lost from energetic particles can eject electrons from atoms or raise atomic electrons to more distant atomic shells.

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10
Q

Indirectly ionizing

A

–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.

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11
Q

Three ways that diagnostic energy x-rays interact with matter

A

–Three ways that diagnostic energy x-rays interact with matter are (i) coherent scatter, (ii) photoelectric (PE) effect, and (iii) Compton scatter.

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12
Q

Coherent scatter

A

–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.

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13
Q

Photoelectric effect

A

–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.

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14
Q

Auger electron

A

–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.

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15
Q

Photoelectric effect probability

A

–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.

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16
Q

Compton scatter

A

–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.

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17
Q

Compton interaction probability

A

–Electron density.
–Physical density.
–(1/E).

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18
Q

The linear attenuation coefficient (μ)

A

–The fraction of incident photons removed from the beam in traveling unit distance.
–Expressed in inverse centimeters (cm−1).

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19
Q

The linear attenuation coefficient (μ) affected by

A

–Increases with increasing physical density.
–Increase with increasing atomic number.
–Attenuation decreases with increasing photon energy.

20
Q

The mass attenuation coefficient

A

–The linear attenuation coefficient (μ) divided by the density (ρ).
–Mass attenuation coefficient (μ/ρ) is independent of physical density.

21
Q

Half-Value Layer

A

–The HVL is the thickness of material that attenuates an x-ray beam by 50%.
–HVL increases with increasing photon energy and decreases with increasing atomic number.

22
Q

Filters

A

–Filters are added to the x-ray tube window to preferentially absorb low-energy photons.
–Filtration does not affect the maximum energy of the x-ray beam spectrum.
–Filtration always reduces the x-ray tube output.

23
Q

Beam hardening

A

–The effect of a filter on a polychromatic x-ray beam containing a range of x-ray photon energies.
–Adding filters changes the x-ray spectrum.
–The x-ray beam intensity (i.e., output) is decreased with increased filtration, but the average x-ray energy is increased.
–Hard beams are produced at high voltages using heavy filtration.
–Soft beams are produced at low voltages using less filtration.

24
Q

X-ray beam quality

A

–The ability of an x-ray beam to penetrate the patient.

25
Q

Heel effect

A

–This attenuation is greater in the anode direction than in the cathode direction because of differences in the path length within the target.
–results in higher x-ray intensity at the cathode end and lower x-ray intensity at the anode end of the beam.

26
Q

To reduce the heel effect

A

–The anode angle should be increased, SID increased, and field size decreased.

27
Q

Air gaps and scatter

A

–Air gaps between the patient and cassette reduce scatter.

28
Q

Antiscatter grids

A

–Antiscatter grids are made up of many narrow parallel bars of lead or other highly attenuating material.
–Antiscatter grids are used to removing scatter in diagnostic radiology.

29
Q

The grid ratio

A

–The grid ratio is the ratio of the strip height (h) along the x-ray beam direction to the gap (D) between the lead strips, so the grid ratio is h/D.
–Grid ratios typically range from 4 to 16.

30
Q

The strip line density

A

–1/(D+d) lines per unit length, where d is the strip thickness.
–Strip line densities range from 25 to 60 lines per centimeter.

31
Q

Primary transmission

A

–The percentage of incident primary radiation (i.e., not scattered) that passes through the grid.

32
Q

The Bucky factor

A

– The ratio of radiation incident on the grid to the transmitted radiation.
–The Bucky factor is the increase in patient dose due to the use of a grid.
–Typical values for the Bucky factor range between 2 and 6.

33
Q

The contrast improvement factor

A

– The ratio of contrast with a grid to contrast without a grid.
–Contrast improvement factors are ∼2.

34
Q

Grid ratio

A

–Grid ratios may be increased either by increasing the height of the lead strips or reducing the space between the lead strips.
–Increasing the grid ratio increases x-ray tube loading and patient exposure.
–Increasing the grid ratio increases image contrast.

35
Q

Primary transmission

A

–The percentage of incident primary radiation (i.e., not scattered) that passes through the grid.

36
Q

The Bucky factor

A

–The ratio of radiation incident on the grid to the transmitted radiation.
–The increase in patient dose due to the use of a grid.
–Typical values for the Bucky factor range between 2 and 6.

37
Q

The contrast improvement factor

A

– The ratio of contrast with a grid to contrast without a grid.

38
Q

Air kerma

A

–It is a source-related term used to quantify the x-ray beam intensity.
–Air kerma stands for the Kinetic energy released per unit mass.
–Air kerma is the kinetic energy transferred from uncharged particles (e.g., photons) to charged particles (i.e., electrons).
–The unit of air kerma is joules per kilogram (J/kg), where 1 J/kg is 1 gray (Gy).

39
Q

Intensity

A

–Intensity is the amount of radiation, and is directly related to the number of x-ray photons.

40
Q

Exposure

A

–The total charge of electrons liberated per unit mass of air by the x-ray photons.
–Exposure is measured in coulombs per kilogram (C/kg) in the SI system or in roentgens (R) in non-SI units.
–1 R = 2.58 × 10−4 C/kg

41
Q

Absorbed dose (D)

A

–Absorbed dose (D) measures the amount of radiation energy (E) absorbed per unit mass (M) of a medium: D = E/M.
–Absorbed dose is specified in gray (Gy) in the SI system.
–One gray is equal to 1 J of energy deposited per kilogram.

42
Q

The relation between absorbed dose (D) and air kerma (K)

A

–D = R × K.

–R depends on the characteristics of the medium irradiated, primarily the atomic number (Z) of the absorbing medium.

43
Q

The outer shell binding energy is

A

∼5 eV (i.e., 0.005 keV).

44
Q

It takes 30 eV or so to produce

A

One ionization.

45
Q

Coherent scatter never accounts for

A

More than 5% of all interactions in diagnostic radiology.

46
Q

In bone, Compton and photoelectric interactions are equally probable at

A

40 keV.