ENTC 4390 MEDICAL IMAGING - PowerPoint PPT Presentation

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ENTC 4390 MEDICAL IMAGING

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Only a few of the many different nuclear emanations are used ... An older, less-preferred unit of activity is the curie (Ci), defined as. 1 Ci = 3.7 x 1010 dps ... – PowerPoint PPT presentation

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Title: ENTC 4390 MEDICAL IMAGING


1
ENTC 4390MEDICAL IMAGING
  • RADIOACTIVE DECAY

2
Nuclear Particles Radiation
  • Only a few of the many different nuclear
    emanations are used in medicine.
  • In order of importance, the entities are
  • x-rays
  • Electromagnetic waves of very short wavelength
    that behave in many ways like particles.
  • Gamma (g) rays
  • Electromagnetic waves similar to x-rays, but of
    even shorter wavelength.
  • Neutrons
  • Actual particles that are produced during the
    decay of certain radioacitve materials.

3
Radioactivity
Dont be confused by this picture! A single
radioactive source does not emit all three types
a, b and g.
4
3 Types of Radioactivity
a particles helium nuclei
Easily Stopped
b particles electrons
Stopped by metal
g photons (more energetic than x-rays)
penetrate!
5
  • The nucleus of an atom consists of neutrons and
    protons, referred to collectively as nucleons.
  • In a popular model of the nucleus (the shell
    model), the neutrons and protons reside in
    specific levels with different binding energies.

6
Materials Science Fundamentals
  • The structure of an atom

7
Materials Science Fundamentals
  • 2. Elements/Atomic Number (Z) Atomic Masses
  • Key Chemical Behavior Determined by Z and
    Ionization

8
Materials Science Fundamentals
  • Atomic Number of Protons
  • Mass Number of Protons and Neutrons
  • Atomic Weight Total Mass of Atom

9
  • If a vacancy exists at a lower energy level, a
    neutron or proton in a higher level may fall to
    fill the vacancy
  • This transition releases energy and yields a more
    stable nucleus.
  • The amount of energy released is related to the
    difference in binding energy between the higher
    and lower levels.
  • The binding energy is much greater for neutrons
    and protons inside the nucleus than for electrons
    outside the nucleus.
  • Hence, energy released during nuclear transitions
    is much greater than that released during
    electron transitions.

10
  • If a nucleus gains stability by transition of a
    neutron between neutron energy levels, or a
    proton between proton energy levels, the process
    is termed an isometric transition.
  • In an isomeric transition, the nucleus releases
    energy without a change in its number of protons
    (Z) or neutrons (N).
  • The initial and final energy states of the
    nucleus are said to be isomers.
  • A common form of isomeric transition is gamma
    decay (g) in which the energy is released as a
    packet of energy (a quantum or photon) termed a
    gamma (g) ray
  • An isomeric transition that competes with gamma
    decay is internal conversion, in which an
    electron from an extranuclear shell carries the
    energy out of the atom.

11
  • It is also possible for a neutron to fall to a
    lower energy level reserved for protons, in which
    case the neutron becomes a proton.
  • It is also possible for a proton to fall to a
    lower energy level reserved for neurons, in which
    case the proton becomes a neuron.
  • In these situations, referred to collectively as
    beta (b) decay, the Z and N of the nucleus
    change, and the nucleus transmutes from one
    element to another.
  • In beta (b) decay, the nucleus loses energy and
    gains stability.

12
  • In any radioactive process the mass number of the
    decaying (parent) nucleus equals the sum of the
    mass numbers of the product (progeny) nucleus and
    the ejected particle.
  • That is, mass number A is conserved in
    radioactive decay

13
  • In alpha (a) decay, an alpha particle (two
    protons and two neutrons tightly bound as a
    nucleus of helium ) is ejected from the
    unstable nucleus.
  • The alpha particle is a relatively massive,
    poorly penetrating type of radiation that can be
    stopped by a sheet of paper.

14
  • An example of alpha decay is

15
ENTC 4390MEDICAL IMAGING
  • DECAY SCHEMES

16
  • A decay scheme depicts the decay processes
    specific for a nuclide (nuclide is a generic term
    for any nuclear form).
  • Energy on the y axis, plotted against the
  • Atomic number of the nuclide on the x axis.

17
  • Given a generic nuclide, there are four
    possible routes of radioactive decay.
  • a decay to the progeny nuclide by emission of a
    nucleus.
  • (a) b (positron) decay to progeny nuclide
    by emission of positive electron from the
    nucleus.
  • (b) b- (negatron) decay to progeny nuclide by
    emission of negative electron from the nucleus.
  • g decay reshuffles the nucleons releasing a
    packet of energy with no change in Z (or N or
    A).

18
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Atomic Number
19
ENTC 4390
  • BETA DECAY

20
  • Nuclei tend to be most stable if they contain
    even numbers of protons and neutrons and least
    stable if they contain an odd number of both.
  • Nuclei are extraordinarily stable if they contain
    2, 8 ,14, 20, 28, 50, 82, or 126 protons.
  • These are termed nuclear magic numbers and
  • Reflect full occupancy of nuclear shells.

21
  • The number of neutrons is about equal to the
    number of protons in low-Z stable nuclei.
  • As Z increases, the number of neutrons increases
    more rapidly than the number of protons in stable
    nuclei.

22
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23
  • Can get 4 nucleons in each energy level-
  • lowest energy will favor NZ,
  • But protons repel one another (Coulomb Force) and
    when Z is large it becomes harder to put more
    protons into a nucleus without adding even more
    neutrons to provide more of the Strong Force.
  • For this reason, in heavier nuclei NgtZ.

24
ENTC 4390
  • ISOMERIC TRANSITIONS

25
  • Isomeric transitions are always preceded by
    either electron capture or emission of an a or b
    ( or -) particle.
  • Sometimes one or more of the excited states of a
    progeny nuclide may exist for a finite lifetime.
  • An excited state is termed a metastable state if
    its half-life exceeds 10-6 seconds.

26
  • An isometric transition can also occur by
    interaction of the nucleus with an electron in
    one of the electron shells.
  • This process is called internal conversion.
  • The electron is ejected with kinetic energy Ek
    equal to the energy Eg released by the nucleus,
    reduced by the binding energy Eb of the electron
  • The ejected electron is accompanied by x rays and
    Auger electrons as the extranuclear structure of
    the atom resumes a stable configuration.

27
  • The rate of decay of a radioactive sample depends
    on the number N of radioactive atoms in the
    sample.
  • This concept can be stated as
  • where DN/Dt is the rate of decay, and the
    constant l is called the decay constant.

28
  • The decay constant has units of time .
  • It has a characteristic value for each nuclide.
  • It also reflects the nuclides degree of
    instability
  • a larger decay constant connotes a more unstable
    nuclide
  • i.e., one that decays more rapidly.
  • The rate of decay is a measure of a samples
    activity.

29
  • The activity of a sample depends on the number of
    radioactive atoms in the sample and the decay
    constant of the atoms.
  • A sample may have a high activity because it
    contains a few highly unstable (large decay
    constant) atoms, or
  • because it contains many atoms that are only
    moderately unstable (small decay constant).

30
  • The SI unit of activity is the becquerel (Bq.)
    defined as
  • 1 Bq 1 disintegration per second (dps)
  • An older, less-preferred unit of activity is the
    curie (Ci), defined as
  • 1 Ci 3.7 x 1010 dps

31
Example
a. has a decay constant of 9.49 x 10-3 hr
-1. Find the activity in becquerels of a sample
containing 1010 atoms.
32
Example
  • How many atoms of with a decay constant
    of 2.08 hr -1 would be required to obtain the
    same activity in the previous problem.
  • More atoms of than of are required to
    obtain the same activity because of the
    difference in decay constants.

33
  • Note that the equation
  • can be written as

34
  • Rearranging and solving for N,
  • where No is the number of atoms at time to .

natural log format
35
  • The physical half-life, T1/2, of a radioactive
    nuclide is the time required for decay of half of
    the atoms in a sample of the nuclide.

36
Example
  • The half-life is 1.7 hours for 113mIn (Indium).
  • A sample of 113mIn has a mass of 2mg.

37
ENTC 4390MEDICAL IMAGING
  • DECAY SCHEMES

38
X-Rays
  • Strong or high energy x-rays can penetrate deeply
    into the body.
  • Weak or soft x-rays are used if only limited
    penetration is needed
  • The energy of x-rays, as well as other nuclear
    particles is measured in
  • electron-volts (ev)
  • thousands of electron-volts (kev)
  • millions of electron-volts (Mev)

39
  • The diagnostic use of x-ray depends on the fact
    that various types of absorbs x-rays to a greater
    or lesser degree.
  • Absorption by bone is quite high,
  • Absorption by fatty tissue is low.
  • This allows the use of the x-ray beam for
    delineating the details of body structure.

40
Gamma Rays
  • X-rays are generally produced electrically.
  • g_rays are the result of a radioactive transition
    in a substance that has been activated in a
    nuclear reactor.
  • Once again, energy is measured in
  • electron-volts (ev)
  • thousands of electron-volts (kev)
  • millions of electron-volts (Mev)

41
  • The higher energy g-rays penetrate all human
    tissue quite easily.
  • g-rays are used in conjunction with scanning
    systems to detect anomalies due to disease or
    neoplastic growth.

42
Neutrons
  • Neutron applications in medicine are limited.
  • Again, energy is measured in
  • electron-volts (ev)
  • thousands of electron-volts (kev)
  • millions of electron-volts (Mev)

43
Preflight - Gamma Ray Emission
  • Gamma rays are emitted due to electrons making
    transitions to nuclear energy levels.
  • true
  • false

No, gamma rays are high energy photons emitted
when nucleons make transitions between their
allowed quantum states.
44
Preflight - Nuclear Beta Decay
  • Beta rays are produced when the atom
    spontaneously repels all its electrons from its
    orbits.
  • true
  • false

Beta particles are electrons. However, the atom
does not emit its atomic electrons.
Beta electrons are emitted by a nucleus along
with a neutral weakly interacting particle called
the neutrino when one of the neutrons in the
nucleus decays.
Free neutrons are unstable - they decay.
Sometimes in atoms with large numbers of
neutrons, one of its neutrons may be loosely
bound - spontaneous decay!
45
Preflight - Positrons
  • Beta particles are
  • Always negatively charged.
  • Always positively charged.
  • Some beta decays could produce positively charged
    particles with properties similar to those of
    electrons.

Some radioactive elements emit a positively
charged particle which is in all other respects
similar to an electron! Anti-matter!! Positrons!!!
46
Preflight - Alpha Particles
  • Alpha particles are
  • Electrons
  • Protons.
  • Nuclei of Helium atoms
  • Nuclei of Argon atoms

Some nuclei have lots of protons and many more
protons. Lowest energy bound-states require about
equal numbers of protons and neutrons. Those
nuclei emit most tightly bound nuclear matter,
i.e., Helium nuclei with two protons and two
nuclei.
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