lecture powerpoint chapter 31 physics: principles with

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© 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their courses and assessing student learning. Dissemination or sale of any part of this work (including on the World Wide Web) will destroy the integrity of the work and is not permitted. The work and materials from it should never be made available to students except by instructors using the accompanying text in their classes. All recipients of this work are expected to abide by these restrictions and to honor the intended pedagogical purposes and the needs of other instructors who rely on these materials. Lecture PowerPoint Chapter 31 Physics: Principles with Applications, 6 th edition Giancoli

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Page 1: Lecture PowerPoint Chapter 31 Physics: Principles with

© 2005 Pearson Prentice Hall

This work is protected by United States copyright laws and is provided solely for

the use of instructors in teaching their courses and assessing student learning.

Dissemination or sale of any part of this work (including on the World Wide Web)

will destroy the integrity of the work and is not permitted. The work and materials

from it should never be made available to students except by instructors using

the accompanying text in their classes. All recipients of this work are expected to

abide by these restrictions and to honor the intended pedagogical purposes and

the needs of other instructors who rely on these materials.

Lecture PowerPoint

Chapter 31

Physics: Principles with

Applications, 6th edition

Giancoli

Page 2: Lecture PowerPoint Chapter 31 Physics: Principles with

Chapter 31

Nuclear Energy; Effects and

Uses of Radiation

Page 3: Lecture PowerPoint Chapter 31 Physics: Principles with

Units of Chapter 31

• Nuclear Reactions and the Transmutation of

Elements

• Nuclear Fission; Nuclear Reactors

• Nuclear Fusion

• Passage of Radiation through Matter;

Radiation Damage

• Measurement of Radiation – Dosimetry

Page 4: Lecture PowerPoint Chapter 31 Physics: Principles with

Units of Chapter 31

• Radiation Therapy

• Tracers and Imaging in Research and Medicine

• Emission Tomography

• Nuclear Magnetic Resonance (NMR) and

Magnetic Resonance Imaging (MRI)

Page 5: Lecture PowerPoint Chapter 31 Physics: Principles with

31.1 Nuclear Reactions and the

Transmutation of Elements

A nuclear reaction takes place when a nucleus

is struck by another nucleus or particle.

If the original nucleus is transformed into

another, this is called transmutation.

An example:

Page 6: Lecture PowerPoint Chapter 31 Physics: Principles with

31.1 Nuclear Reactions and the

Transmutation of Elements

Energy and momentum must be conserved in

nuclear reactions.

Generic reaction:

The reaction energy, or Q-value, is the sum

of the initial masses less the sum of the

final masses, multiplied by c2:

Page 7: Lecture PowerPoint Chapter 31 Physics: Principles with

31.1 Nuclear Reactions and the

Transmutation of Elements

If Q is positive, the reaction is exothermic, and

will occur no matter how small the initial kinetic

energy is.

If Q is negative, there is a minimum initial kinetic

energy that must be available before the reaction

can take place.

Page 8: Lecture PowerPoint Chapter 31 Physics: Principles with

31.1 Nuclear Reactions and the

Transmutation of Elements

Neutrons are very

effective in nuclear

reactions, as they nave

no charge and therefore

are not repelled by the

nucleus.

Page 9: Lecture PowerPoint Chapter 31 Physics: Principles with

31.2 Nuclear Fission; Nuclear Reactors

After absorbing a neutron, a

uranium-235 nucleus will split

into two roughly equal parts.

One way to visualize this is to

view the nucleus as a kind of

liquid drop.

Page 10: Lecture PowerPoint Chapter 31 Physics: Principles with

31.2 Nuclear Fission; Nuclear Reactors

The mass distribution of the fragments shows

that the two pieces are large, but usually

unequal.

Page 11: Lecture PowerPoint Chapter 31 Physics: Principles with

31.2 Nuclear Fission; Nuclear Reactors

The energy release in a fission reaction is quite

large. Also, since smaller nuclei are stable with

fewer neutrons, several neutrons emerge from

each fission as well.

These neutrons

can be used to

induce fission in

other nuclei,

causing a chain

reaction.

Page 12: Lecture PowerPoint Chapter 31 Physics: Principles with

31.2 Nuclear Fission; Nuclear Reactors

In order to make a nuclear reactor, the chain

reaction needs to be self-sustaining – it will

continue indefinitely – but controlled.

Page 13: Lecture PowerPoint Chapter 31 Physics: Principles with

31.2 Nuclear Fission; Nuclear Reactors

A moderator is needed to slow the neutrons;

otherwise their probability of interacting is too

small. Common moderators are heavy water and

graphite.

Unless the moderator is heavy water, the fraction

of fissionable nuclei in natural uranium is too

small to sustain a chain reaction, about 0.7%. It

needs to be enriched to about 2-3%.

Page 14: Lecture PowerPoint Chapter 31 Physics: Principles with

Neutrons that escape from

the uranium do not

contribute to fission. There

is a critical mass below

which a chain reaction will

not occur because too

many neutrons escape.

31.2 Nuclear Fission; Nuclear Reactors

Page 15: Lecture PowerPoint Chapter 31 Physics: Principles with

31.2 Nuclear Fission; Nuclear Reactors Finally, there are control rods, usually cadmium or boron,

that absorb neutrons and can be used for fine control of

the reaction, to keep it critical but just barely.

Page 16: Lecture PowerPoint Chapter 31 Physics: Principles with

31.2 Nuclear Fission; Nuclear Reactors

Some problems associated with nuclear reactors

include the disposal of radioactive waste and the

possibility of accidental release of radiation.

Page 17: Lecture PowerPoint Chapter 31 Physics: Principles with

31.2 Nuclear Fission; Nuclear Reactors

An atomic bomb also uses fission, but the core is

deliberately designed to undergo a massive

uncontrolled chain reaction when the uranium is

formed into a critical mass during the detonation

process.

Page 18: Lecture PowerPoint Chapter 31 Physics: Principles with

31.3 Nuclear Fusion

The lightest nuclei can fuse to form heavier

nuclei, releasing energy in the process. An

example is the sequence of fusion processes

that change hydrogen into helium in the Sun.

They are listed here with the energy released in

each:

Page 19: Lecture PowerPoint Chapter 31 Physics: Principles with

31.3 Nuclear Fusion

The net effect is to transform four protons into a

helium nucleus plus two positrons, two

neutrinos, and two gamma rays.

(31-7)

More massive stars can fuse heavier

elements in their cores, all the way up to iron,

the most stable nucleus.

Page 20: Lecture PowerPoint Chapter 31 Physics: Principles with

31.3 Nuclear Fusion

There are three fusion reactions that are being

considered for power reactors:

These reactions use very common fuels –

deuterium or tritium – and release much more

energy per nucleon than fission does.

Page 21: Lecture PowerPoint Chapter 31 Physics: Principles with

31.3 Nuclear Fusion

A successful fusion reactor has not yet been

achieved, but fusion, or thermonuclear, bombs

have been built.

Page 22: Lecture PowerPoint Chapter 31 Physics: Principles with

31.3 Nuclear Fusion

Several geometries for the containment of the

incredibly hot plasma that must exist in a fusion

reactor have been developed – the tokamak,

which is a torus; or inertial confinement, which

is tiny pellets of deuterium ignited by powerful

lasers.

Page 23: Lecture PowerPoint Chapter 31 Physics: Principles with

31.4 Passage of Radiation Through Matter;

Radiation Damage

Radiation includes alpha, beta, and gamma rays;

X rays; and protons, neutrons, pions, and other

particles.

All these forms of radiation are called ionizing

radiation, because they ionize material that they

go through.

This ionization can cause damage to materials,

including biological tissue.

Page 24: Lecture PowerPoint Chapter 31 Physics: Principles with

31.5 Measurement of Radiation – Dosimetry

Radiation damages biological tissue, but it can

also be used to treat cancer and other diseases.

It is important to be able to measure the amount,

or dose, of radiation received. The source activity

is the number of disintegrations per second, often

measured in curies, Ci.

The SI unit for source activity is the

becquerel (Bq):

Page 25: Lecture PowerPoint Chapter 31 Physics: Principles with

31.5 Measurement of Radiation – Dosimetry

Another measurement is the absorbed dose

– the effect the radiation has on the

absorbing material.

The rad, a unit of dosage, is the amount of

radiation that deposits energy at a rate of

1.00 x 10-2 J/kg in any material.

The SI unit for dose is the gray, Gy:

1 Gy = 1 J/kg = 100 rad

Page 26: Lecture PowerPoint Chapter 31 Physics: Principles with

31.5 Measurement of Radiation – Dosimetry

The effect on tissue of different types of

radiation varies, alpha rays being the most

damaging. To get the effective dose, the dose is

multiplied by a quality factor.

Page 27: Lecture PowerPoint Chapter 31 Physics: Principles with

31.5 Measurement of Radiation – Dosimetry

If the dose is measured in rad, the effective

dose is in rem; if the dose is grays, the effective

dose is in sieverts, Sv.

Page 28: Lecture PowerPoint Chapter 31 Physics: Principles with

31.5 Measurement of Radiation – Dosimetry

Natural background radiation is about 0.3 rem

per year. The maximum for radiation workers is

5 rem in any one year, and below 2 rem per year

averaged over 5 years.

A short dose of 1000 rem is almost always fatal;

a short dose of 400 rem has about a 50% fatality

rate.

Page 29: Lecture PowerPoint Chapter 31 Physics: Principles with

31.6 Radiation Therapy

Cancer is sometimes treated with radiation

therapy to destroy the cells. In order to minimize

the damage to healthy tissue, the radiation

source is often rotated so it goes through

different parts of the body on its way to the

tumor.

Page 30: Lecture PowerPoint Chapter 31 Physics: Principles with

31.7 Tracers and Imaging in Research and

Medicine

Radioactive isotopes are widely

used in medicine for diagnostic

purposes. They can be used as

non-invasive scans, or tools to

check for unusual

concentrations that could signal

a tumor or other problem. The

radiation is detected with a

gamma-ray detector.

Page 31: Lecture PowerPoint Chapter 31 Physics: Principles with

31.8 Emission Tomography

Radioactive tracers can also be detected using

tomographic techniques, where a three-

dimensional image is gradually built up

through successive scans.

Page 32: Lecture PowerPoint Chapter 31 Physics: Principles with

31.9 Nuclear Magnetic Resonance (NMR)

and Magnetic Resonance Imaging (MRI)

A proton in a magnetic field can have its spin

either parallel or antiparallel to the field.

The field splits the

energy levels slightly;

the energy difference

is proportional to the

field.

Page 33: Lecture PowerPoint Chapter 31 Physics: Principles with

31.9 Nuclear Magnetic Resonance (NMR)

and Magnetic Resonance Imaging (MRI)

The object to be examined is placed in a static

magnetic field, and radio frequency (RF)

electromagnetic radiation is applied.

Page 34: Lecture PowerPoint Chapter 31 Physics: Principles with

31.9 Nuclear Magnetic Resonance (NMR)

and Magnetic Resonance Imaging (MRI)

When the radiation has the right energy to excite

the spin-flip transition, many photons will be

absorbed. This is nuclear magnetic resonance.

The value of the field depends somewhat on the

local molecular neighborhood; this allows

information about the structure of the molecules

to be determined.

Page 35: Lecture PowerPoint Chapter 31 Physics: Principles with

31.9 Nuclear Magnetic Resonance (NMR)

and Magnetic Resonance Imaging (MRI)

Magnetic resonance imaging works the same

way; the transition is excited in hydrogen

atoms, which are the commonest in the human

body.

Page 36: Lecture PowerPoint Chapter 31 Physics: Principles with

31.9 Nuclear Magnetic Resonance (NMR)

and Magnetic Resonance Imaging (MRI)

Giving the field a gradient can contribute to

image accuracy, as it allows determining the

origin of a particular signal.

Page 37: Lecture PowerPoint Chapter 31 Physics: Principles with

31.9 Nuclear Magnetic Resonance (NMR)

and Magnetic Resonance Imaging (MRI)

Here is a summary of the medical imaging

techniques we have discussed.

Page 38: Lecture PowerPoint Chapter 31 Physics: Principles with

Summary of Chapter 31

• Nuclear reaction occurs when nuclei collide

and different nuclei are produced

• Reaction energy or Q-value:

• Fission: heavy nucleus splits into two

intermediate-sized nuclei

• Chain reaction: neutrons emitted in one

fission reaction trigger another, and so on

• Critical mass: minimum needed to sustain

chain reaction

Page 39: Lecture PowerPoint Chapter 31 Physics: Principles with

Summary of Chapter 31

• Moderator: slows neutrons

• Fusion: small nuclei combine to form larger

ones

• Sun’s energy comes from fusion reactions

• Useful fusion reactor has not yet been built

• Radiation damage is measured using dosimetry

• Effect of absorbed dose depends on type of

radiation