Interactive Transcript
0:01
X-ray interactions with matter can be understood as the following.
0:05
There are four major interactions which are very critical for diagnostic
0:09
radiology and nuclear medicine. Among the four interaction,
0:13
the classical scattering, also called as Rayleigh or elastic scattering,
0:18
Compton scattering, photoelectric effect, and pair
0:21
production.
0:23
Among these four, the main area of interest are the
0:26
Compton scattering and photoelectric effect because these two
0:30
type of interaction are the dominant way of creation of the
0:34
images in diagnostic radiology and nuclear medicine.
0:38
I'm not going to talk much about classical scattering because they're
0:42
usually at a very low energy interaction, and they
0:45
don't penetrate through the body. They just absorb the surface of the body.
0:50
Because of that, we try to remove those low energy X-ray
0:54
beam, which I'm going to explain later.
0:56
So therefore, classical scattering is not of interest for our discussion.
1:01
Similarly, pair production only occurs when the energy is
1:04
higher than the one MeV, which is not, again, of our interest.
1:09
We are going to focus on these two, Compton scattering and photoelectric effect.
1:14
What is photoelectric effect?
1:16
The photoelectric effect is an interaction of incident radiation or
1:21
photon with inner shells of electrons of any matter.
1:25
When this interaction occurs, when the external radiation
1:29
can knock off an electron, or by transferring all its
1:33
energy, it can eject an electron, and that is called
1:37
ejected photoelectron
1:39
as that is equal to the kinetic energy and minus
1:43
the binding energy. So it can show in this image down here,
1:47
an 100 kV incident photon is interacting with matter,
1:51
and this particular atomic structure, the energy is sufficient to knock
1:55
off an electron, and the electron moves out with certain
1:59
energy. There's a difference between the binding energy and the
2:03
energy incident, and that is called the photoelectron.
2:07
More importantly, when this particular electron is knocked off, there is a
2:11
remaining empty shell. In nature, what happen is the electron from
2:15
a higher shell will jump into the lower
2:18
shell. By doing so, there releases a difference in the energy
2:22
called characteristic X-ray. So we're going to see that the empty
2:26
shell immediately filled with electron from outer orbital,
2:30
resulting in emission of characteristic X-rays.
2:33
And those energies are very unique.
2:35
For example, in a iodine matter, when radiation interaction, the
2:39
K-shell energy is about 34 keV, L-shell electron is
2:43
about 5 keV, and M-shell is 0.6 keV.
2:47
I'm going to bring this together when we do the radiography on how the X-ray
2:51
imagings are formed.
2:54
One of the fundamental relationship is the energy of the
2:58
binding energy is proportional to the atomic number squared,
3:02
Z squared. So the photoelectric effect leads
3:06
to either characteristic X-ray and/or auger
3:10
electron. Why is this important? We're going to discuss later when we
3:14
discuss mammography physics.
3:16
The probability of the photoelectric absorption is given
3:20
as follows. It is proportional to Z cube, that is the
3:24
atomic numbers cube, divided by
3:28
energy cube. Means greater the energy of the
3:32
incident radiation, lesser the chances of act-- happening with
3:36
the photoelectric effect. Whereas the lesser energy
3:40
means there is lar-- more chances of having this photoelectric absorption
3:43
probability.
3:45
This explains why contrast decreases as
3:49
higher energy X-rays are used in imaging process.
3:53
Again, I'm going to bring this tie it up together with image contrast
3:56
later. But the photoelectric absorption is important to
4:00
understand. It is one of the key interaction mechanism of radiation
4:04
with matter, and especially when the atomic number of the
4:08
interaction material are small and the energy is low, the
4:12
chances are much higher. And that also brings back to the
4:15
contrast agents we use, like iodine contrast and so forth thereforth.
4:20
If you look here, the photoelectric effect of tissues, on the
4:24
left-hand side, the x-axis is X-ray energy, on
4:28
the y-axis is mass attenuation coefficient.
4:31
If you look through, for a tissue, the absorption is very
4:34
high at the low energy and goes down
4:38
dramatically.
4:40
Now, if you add a contrast material, you see this type of a
4:44
spectrum. And in this type of a spectrum means around
4:48
this area, it's called the K-edges, the energy is
4:52
more absorbed, therefore, the signal spikes up, increases,
4:56
and that's why you use contrast agent, to enhance the image
4:59
quality. And the two commonly used contrast
5:03
agents in X-ray imaging is barium contrast and
5:07
iodine contrast. It's pretty same for fluoroscopy,
5:11
radiography, and CT. And this is the reason why,
5:14
because they have a K-edge around in a convenient
5:18
area, which is in the area in between the dynamic range we use.
5:23
On the right-hand side, if you'll see, again, this thick is listed in
5:27
the keV energy, and on the y-axis is the
5:31
percent of photoelectric absorption
5:33
and also the percent Compton scattering on the right-hand side.
5:37
If you look here, for most of the diagnostic energy range,
5:41
this is the range between 10 to 100 keV.
5:44
In fact, we generally go up to 60, 70 keV, that's all.
5:48
In this case, the majority is this Compton scattering is
5:52
very high in the low energy and decreases as we go
5:56
along. But there is a Compton energy comes into-- Compton
6:00
scattering comes later. But these things, the sodium iodide and
6:04
lead, are discussed in nuclear medicine.
6:06
I'm not going to discuss here, but this is the range of interest we are interested
6:10
in photoelectric effect for tissue.
6:13
So if you look in the attenuation coefficient, soft tissues
6:17
or bone, what happens here is trying to match
6:21
with respect to the absorption, the type of
6:25
interaction of the radiation with the tissue, and how does
6:29
that translate to imaging. This is an image of a chest X-ray, and
6:33
this is an imaging of a mammography.
6:35
In mammography, it is all soft tissue.
6:38
There is no bony structure. So a lot of this is done in the
6:42
photoelectric range here.
6:45
Whereas a chest X-ray range includes both a wide range of
6:49
tissues from bone to soft tissue to air.
6:52
We work in the range of the Compton area.
6:55
So for most of the energies which we use in imaging,
6:59
the predominant interaction is photoelectric absorption or
7:03
Compton scattering.
7:06
How do we make an image? This is showing a lateral
7:10
X-ray of a knee, and the way it can be done
7:14
is the detector can be placed according to the patient, wherever you want,
7:18
and then the X-ray tube is automatically positioned to get an image.
7:22
You can see there is a contrast between the bony structure and the
7:26
soft tissue structure, but within the soft tissue structure, you don't see the
7:29
difference between muscle and soft tissue and so forth.
7:33
Just to give you an idea. Therefore, we
7:36
need to get an image for diagnosis.
7:39
We want tissue contrast.
7:41
There are four major categories of materials and tissues
7:46
that produce tissue contrast in radiography.
7:49
The four major categories are air, adipose or
7:53
fat tissue, soft tissue, and bone.
7:56
So the image contrast depends on the radiographic technique we used.
8:00
What technique we use will determine the tissue contrast.
8:04
As you can see here, this is a complex image.
8:07
The chest X-ray is one of the complex imaging technique because it has to
8:11
balance between the bony structure, the lung air,
8:15
and also the other soft tissue. So it should accommodate
8:19
all these things when it does the imaging.
8:22
Whereas in mammography, we're typically imaging the fatty
8:26
tissue and glandular tissue or the soft tissue, so there are no bony
8:30
structure, and that makes a determination of what type of technique we are
8:34
going to use.
8:35
This is the basic radiography system component.
8:39
Typically, this is a tabletop X-ray system, radiography system.
8:43
The basic component are the X-ray tube,
8:47
and we have aluminum filters for the reason I'm going to explain later.
8:51
We have a collimator, which will adjust the X-ray field
8:54
size to the anatomy of interest we are imaging.
8:58
Underneath the patient, we have what is called an antiscatter
9:02
grid.
9:03
We also have a photocell, which will automatically adjust
9:07
the technique based on what it is seeing, the patient
9:11
thickness, and it's called as automatic exposure control.
9:15
Then we have a detector. We have detectors from film screen,
9:19
older days, to digital detector, and I'm going to discuss all these
9:22
things as we go along. So we have source on one
9:26
side, detector on the other side. Typically, for a
9:30
tabletop radiograph, the distance between the source to the
9:34
detector is about 100 centimeter or approximately 40
9:38
inches. That's a typical distance for the basic
9:42
X-ray of the abdomen or any of the body part
9:46
when the patient is lying on a tabletop.