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Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit...

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Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is no interaction The radiation interacts almost continuously giving up a small amount of its energy at each interaction. N E l θ E o Incident Beam
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Page 1: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Types of Radiation Interactions

All or Nothing Many Small

There is a finite probability per unit length that the radiation is absorbed. If not, there is no interaction

The radiation interacts almost continuously giving up a small amount of its energy at each interaction.

N

E

l

θ

Eo

Incident Beam

Page 2: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Types of Radiation Interactions

N

E

N

E

N

l

N

l

NN

θ

θ0

Eo

Eo

0

The energy provides a marker for those photons of interest

Attenuation tells us the depth.

Angular spread of beam is maintained, thus well defined projection direction

Output beam

Page 3: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Types of Interactions We Want

y

x

detector

Thus, the reduction in the beam intensity should be a property of the object along the line.

−dII

= μdx

Where is the linear attenuation coefficient and in general is a function of x and y -

μ

μ x,y( )

Page 4: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Types of Interactions We Want

Integrate along the path for a uniform material of length, x.

I = Ioe−μx

In general,

Idx,y( ) = I

oe

− μ x ,y( ) dx∫

thickness of absorber

tran

smis

sio n

Page 5: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Some details of photon interactions

1. “good” geometry - all photons that interact leave the measurement beam.

3 approaches

1) Restrict geometry to a narrow beam system. Collimator, place detector at infinity

2) Limit interaction to photo-electric (usually safe to assume that characteristic photons do not leave the sample)

3)Energy select detected photons

Can define a build up factor to account for the additional photons at the detector or even in the sample itself.

Page 6: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Some details of photon interactions

Consider a sample geometry with only a collimator at the output side

This volume element only sees the normal beam intensity .

This volume element also sees the excess intensity from the buildup factor.

SourceCollimator

Detector

So the buildup factor can contribute to the signal as well as the noise.

Io

Page 7: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Attenuation Mechanisms (Simple Scatter)

(a) Simple Scatter (Rayleigh Scattering)

The incindent photon energy is much less than the binding energy of the electron in an atom. The photon is scattered without change of energy. Low energy relatively unimportant.

Page 8: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Attenuation Mechanisms (Photoelectric Effect)

The photon, slightly greater than gives up all of its energy to an inner shell electron, thereby ejecting it from the atom. The excited atom retains to the ground state with the emission of characteristic photons. Most of these are of relatively low energy and are absorbed by the material.

(b) Photoelectric effect

E

Eb

Page 9: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Attenuation Mechanisms (Compton Scattering)

The photon energy is much greater than , and only part of this is given up during the interaction with an outer valence electron (the binding of valence electrons is relatively weak, hence the “free”). The photon is scattered with reduced energy and the energy of the electron is dissipated through ionizations.

(c) Compton Scattering

Eb

Page 10: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Attenuation Mechanisms (Pair Production)

A very high energy photon interacts with a nucleus to create an electron/positron pair. The mass of each particle is 9.11 x 10^-31 kg. So the minimum photon energy is:

(d) Pair Production

Both the electron and the positron lose energy via ionization until an anihilation event takes place yielding two photons of 0.51 MeV moving in oppoiste directions.€

Emin

= 2 × 9.11×10−31kg× 3×108 msec( )

2

=1.64 ×10−13J

=1.02 MeV

Page 11: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Tissue Transparency

1 m 100 m 1cm 1m 100m

Ultrasound

X-ray Radio-frequency

1 100 1 m 100 m 1cm 1m 100m

damaging harmlessC-Hbond energy

Windows of transparency in imaging via sound and electromagnetic radiation. The vertical scale measures absorption in tissue.

Page 12: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Attenuation Mechanisms

μ dependenceMechanism E Z Energy Range in

Soft Tissue

simple scatter

photoelectric

Compton

pair production rises slowly with E

falls slowly with E

1/E3

1/E Z2

Z3

independent

Z2 above 20 MeV

30 keV-20 MeV

1-30 keV

1-20 keV

Page 13: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Attenuation Mechanisms 2

Attenuation mechanisms in water

The optimum photon energy is about 30 keV (tube voltage 80-100 kV) where the photoelectric effect dominates. The Z3 dependence leads to good contrast:

Zfat 5.9Zmuscles 7.4Zbone 13.9

Photoelectric attenuation from bone is about 11x that due to soft tissue, which is dominated by Compton scattering.

.01.03

.05 0.1 11.02 30

10

photoelectric

pair

totalCompton

simple scatter

Compton

Photon energy (MeV)(log plot)

Attenuation(log plot)

Page 14: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Beam Energy

So, beam energy is important

Idx,y( ) = I

oε( )e

− μ x ,y ,ε( )dx∫ dε∫

This does not include buildup factor or scattering but does include beam hardening

Page 15: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Beam EnergyAlso need to consider beam energy even if only photoelectric effect, since absorption rate depends on the energy. Thus, low energy photons deliver no useful information.

N

E

N

BConsider contrast agents, add a material to inhance contrast (more attenuation)

k edge, minimal energy needed to have photoelectric effect with k shell electrons.

Increase the contrast, decrease the signal, increase the dose

μ

h20 keV

Page 16: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Heterogeneous Case

Interested in the heterogeneous case

then

I = Ioe− α 1l 1 + α 2l 2 + L + α N l N( )

where li= L

N i =1

N

α1

l1

α2

l2

α3

l3

α4

l4

α5

l5

a line integral over the sample and defined by the ray of interaction

I = Ioe

− αdl0

L

∫1 2 4 3 4

−l nII

o

= αdl0

L

this is theprojection

1 2 3

Thus, in a continuosly varying medium

Page 17: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Heterogeneous Case

P θ ,z( ) = −l nI θ ,z( )I

oθ ,z( )

= α l( )dl0

L

We wish to recontrast th linear attenuation coefficient .

α l( )

In 2D,

P θ ,z( ) = α x,y( )dlL

Page 18: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

X-ray Attenuation Coefficients

50030020015010050403020100.1

0.15

0.2

0.3

0.40.5

1.0

2

2.5

5

FAT

MUSCLE

BONE

PHOTONENERGY

(kev)

μ(cm2/g)

X-ray attenuation coefficients for muscle, fat, and bone, as a function of photon energy.

Page 19: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Photoelectric Effects Predominates

Page 20: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Unknown

Delta ray knocked out electron.

Ionization event.

Electron-electron interactions generates heat. This is the most common.

E − hν€

Bremsstrahlung

Bremsstrahlung

hν = E

Characteristic Radiation

Electron ejected

e−

e−

e−

e−

E

E

Page 21: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Bremsstrahlung - Breaking Radiation

e−

nucleusX-rays

Coulombic interaction between electron and a nuclear charge

For each interaction, the X-ray spectrum is white and the electron loses some energy.

E

E€

EmaxI n

ter a

cti o

n

Inte

nsit

y

“True” Bremsstrahlung Spectrum

Page 22: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

More Details On X-ray Tubes

• electrons are boiled off filament

• accelerated through a high vacuum from the cathode to the anode

• electrons strike the anode, a tungsten target, and create X-rays

• X-rays are emitted in all directions though only a cone is used

• 99% of the electric energy is dissipated a heat into the anode. Typically less than 1% of the energy is converted into useful X-rays.

• X-rays that are diverted into the target are absorbed and contribute to the production of heat.

Page 23: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

The Origins of X-Rays

Page 24: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

The X-Ray Spectrum

Page 25: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Unknown

But interactions filter out low energy

Usually place some material between tube and object to further reduce low X-rays

Need to take care in designing a filter so as not to create low energy charcteristic lines.

Page 26: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

Bremsstrahlung

Page 27: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

The X-Ray Spectrum (Changes in Voltage)

The characteristic lines are a result of electrons ejecting orbital electrons from the innermost shells. When electrons from outer shells fall down to the level of the inner ejected electron, they emit a photon with an energy that is characteristic to the atomic transition.

The continuous spectrum is from electrons decelerating rapidly in the target and transferring their energy to single photons, Bremsstrahlung.

Emax

= eVp

Vp≡ peak voltage across the X − ray tube

Page 28: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

The X-Ray Spectrum (Changes in tube)

Page 29: Types of Radiation Interactions All or Nothing Many Small There is a finite probability per unit length that the radiation is absorbed. If not, there is.

The X-Ray Spectrum (Changes in Target Material)

Increase in Z:

1. Increase in X-ray intensity since greater mass and positive charge of the target nuclei increase the probability of X-ray emission total output intensity of Z

2. Characteristic lines shift to higher energy, K and L electrons are more strongly held

3. No change in

Emax


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