Nuclear Medicine Flashcards

1
Q

Structure of the atomic nucleus

A
  • Protons + Neutrons
  • Similar mass
  • Mass number is P + N
  • Atomic number is only P
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2
Q

Alpha decay

A
  • Atomic nucleus emits an alpha particle (Helium)
  • Decays into different atomic nucleus
  • Mass number reduced by 4
  • Atomic number reduced by 2
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3
Q

Energy spectra of alpha, beta and gamma radiations

A
  • Alpha spectrum: Line, all excess energy goes to alpha particle that releases from unstable nucleus.
  • Beta spectrum: Continuous, because emitted particles are electron/positron and neutrino/antineutrino.
  • Gamma spectrum: Line, because gamma radiation is packed in quanta
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4
Q

Stability of the atomic nucleus

A
  • Depends on Proton/Neutron ratio
  • Isotopes can be stable or unstable
  • Unstable atoms will decay until they are stable
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5
Q

Beta negative decay

A

Unstable nuclei convert a neutron into a proton, electron and antineutrino

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6
Q

Production of isotopes

A
  • Some isotopes are unstable, so emit radiation
  • Radiation can be harvested for medical use
  • Isotopes produced in nuclear reactors by bombardment of stable nuclei with high energy particles.
  • Tc generator can be used specifically when gamma radiation isotope of short half life is required.
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7
Q

Definition and types of isotopes

A

Two or more atoms that have the same atomic number but different atomic mass (dif. Number of neutrons)

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8
Q

Beta positive decay

A
  • Positron and antineutrino are emitted.
  • Proton in nucleus becomes a neutron
  • Daughter nucleus will have a smaller atomic number but same mass number.
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9
Q

Types of radioactive decay

A
  • Alpha
  • Beta +/-
  • Gamma
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10
Q

Gamma decay

A
  • Product of excited nucleus that tried to achieve stable state.
  • Products of either alpha/beta decay or of some other nuclear process.
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11
Q

Activity

A

Rate of decaying atoms per unit time. (Becquerel)
1Bq = 1 decay/second

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12
Q

Interaction of alpha radiation with matter

A
  • Linear Ion density: Amount of ions produced over a certain length decreases after the particle loses its energy.
  • Effective range: Distance covered by particle until energy is lost. (Mass and charge influence this)
  • Beta particle is much smaller so it has a higher effective range, but much lower linear ion density.
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13
Q

Interaction of gamma radiation with matter I: photoeffect

A
  • Gamma-photon removes an electron from the inner shell of an atom while being absorbed.
  • K.E of electron = incident photon energy
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14
Q

Interaction of gamma radiation with matter II: Compton-scatter

A

Gamma-Photon removes electron from outer shell “Compton electron” and a photon is emitted.

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15
Q

Interaction of gamma radiation with matter III: pair production

A

High energy gamma-photon is absorbed near the nucleus and electron and positron are created.
Process called annihilation where 2 gamma photons will release.

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16
Q

Differential and integral forms of the decay law

A

Integral: N/T (1/s) (Bq)
Differential: N(t) = N^-(1/s)*t

17
Q

Interaction of beta negative radiation with matter

A
  • Directly ionizing atoms by coulomb’s force
  • Scatter on electrons resulting in zigzag path
  • Braking radiation (X-ray)
  • More penetration compared to alpha (Lower mass and charge)
18
Q

Half-life and average lifetime of an isotope

A

Average life: time required for number of undeclared nuclei to decrease to 1/e of initial amount.
Half life: Amount of time taken for undecayed nuclei to decrease to 1/2 of initial amount.

19
Q

Interaction of beta positive radiation with matter

A
  • Radiative particle is positron
  • Collides with electron in annihilation, emitting 2 gamma rays
20
Q

Neutron radiation, proton radiation, the Bragg-peak

A
  • Neutron radiation: Excited nucleus expels a neutron. Neutron does not ionize directly so it collides and energy exchanges to atom. (Elastic scatter, inelastic collision, neutron capture)
  • Proton radiation: Acts similar to alpha particle. (Large mass, shorter effective range)
  • Bragg peak: Relationship between penetration depth and amount of radiation deposited.
21
Q

Scintillation counter I.: the scintillation crystal

A
  • NaI crystal (thallium activated by dropping)
  • Has to be transparent to emission wavelength
  • Absorbs energy of radiation
22
Q

Scintillation counter II.: the photomultiplier tube

A

A tube with a photocathode, converting scintillations from crystal to electrons (photoeffect).
- Electrons multiplied by dynodes before reaching anode.
- Electrons accelerated by a voltage through the tube
-Every collision with dynode produces secondary electrons
- Multiplication factor corresponds to number of secondary electrons.