Title: ENTC 4390 MEDICAL IMAGING
1ENTC 4390MEDICAL IMAGING
2Nuclear 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.
3Radioactivity
Dont be confused by this picture! A single
radioactive source does not emit all three types
a, b and g.
43 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.
6Materials Science Fundamentals
7Materials Science Fundamentals
- 2. Elements/Atomic Number (Z) Atomic Masses
- Key Chemical Behavior Determined by Z and
Ionization
8Materials 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
15ENTC 4390MEDICAL IMAGING
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).
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Atomic Number
19ENTC 4390
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(No Transcript)
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.
24ENTC 4390
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
31Example
a. has a decay constant of 9.49 x 10-3 hr
-1. Find the activity in becquerels of a sample
containing 1010 atoms.
32Example
- 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.
36Example
- The half-life is 1.7 hours for 113mIn (Indium).
- A sample of 113mIn has a mass of 2mg.
37ENTC 4390MEDICAL IMAGING
38X-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.
40Gamma 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.
42Neutrons
- Neutron applications in medicine are limited.
- Again, energy is measured in
- electron-volts (ev)
- thousands of electron-volts (kev)
- millions of electron-volts (Mev)
43Preflight - 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.
44Preflight - 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!
45Preflight - 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!!!
46Preflight - 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.