Radioactivity, Nuclear Physics and its Medical Applications

122 Fission

Learning Objectives

  • Define nuclear fission and explain why it releases energy.
  • Describe how neutron-induced fission occurs and identify the products of a typical fission reaction.
  • Explain the difference between controlled and uncontrolled nuclear chain reactions and describe how chain reactions are sustained.

Nuclear fission is a nuclear reaction in which a heavy atomic nucleus splits into two smaller nuclei. Along with the daughter nuclei, the reaction typically produces several free neutrons and a large amount of energy. This energy comes from the conversion of a small amount of mass into energy according to Einstein's equation, [latex]E=\Delta mc^2[/latex]. Because heavy nuclei are less tightly bound than the medium-mass nuclei produced during fission, the products have a greater binding energy per nucleon and therefore a lower total mass.

Unlike nuclear fusion, which combines light nuclei, fission breaks apart heavy nuclei such as uranium or plutonium. Controlled nuclear fission has been used for decades to generate electricity in commercial nuclear power plants around the world. These facilities provide a significant fraction of the world's low-carbon electrical energy and play an important role in the energy mix of many countries. Advances in reactor design continue to improve safety, efficiency, and waste management while reducing greenhouse gas emissions associated with electricity generation.

A commercial nuclear power plant with cooling towers and the reactor containment building located nearby. Homes and surrounding land illustrate that nuclear power stations operate within populated communities under strict safety regulations.
Figure 122.1: Commercial nuclear power plants generate electricity by carefully controlling nuclear fission reactions inside a reactor. The large cooling towers release water vapor—not smoke—and are used to remove excess heat from the plant. The reactor itself is housed inside the reinforced containment building to the left of the cooling towers. (Credit: Kalmthouts)

Fission releases energy because the nuclei produced are more tightly bound than the original heavy nucleus. As discussed in the previous section on binding energy, energy is released whenever a nuclear reaction produces nuclei with a larger binding energy per nucleon, [latex]\mathrm{BE}/A[/latex], than the starting nucleus.

Heavy nuclei with mass numbers near [latex]A\approx240[/latex] have binding energies of approximately 7.6 MeV per nucleon, whereas medium-mass nuclei near [latex]A\approx120[/latex] have binding energies closer to 8.6 MeV per nucleon. When a heavy nucleus splits into two medium-mass nuclei, the increase of about 1 MeV per nucleon corresponds to a total energy release of roughly 200–240 MeV for a single fission event. This is an enormous amount of energy compared with ordinary chemical reactions, which typically involve only a few electron volts per atom.

The energy released during fission appears primarily as the kinetic energy of the two fission fragments, with smaller amounts carried away by emitted neutrons and gamma rays. These neutrons are especially important because they can induce additional fission events in neighboring nuclei. If enough neutrons continue to produce new fissions, a chain reaction develops. The ability to control this chain reaction is what allows nuclear reactors to generate electricity safely and continuously.

Physics in Healthcare

Although nuclear fission is primarily associated with electricity generation, it also supports many healthcare technologies. Research reactors produce medical isotopes such as molybdenum-99, which decays into technetium-99m—the most widely used radioisotope for diagnostic imaging. Reactors are also used to manufacture isotopes for cancer therapy, sterilize medical equipment, and provide neutron beams for specialized cancer treatments and scientific research.

Example 122.1: Calculating the Energy Released by Fission

Calculate the energy released in the following spontaneous fission reaction:

[latex]{}^{238}\mathrm{U} \rightarrow {}^{95}\mathrm{Sr} + {}^{140}\mathrm{Xe} + 3n[/latex]

The relevant atomic masses are

[latex]m\left({}^{238}\mathrm{U}\right)=238.050784~\mathrm{u},[/latex]
[latex]m\left({}^{95}\mathrm{Sr}\right)=94.919388~\mathrm{u},[/latex]
[latex]m\left({}^{140}\mathrm{Xe}\right)=139.921610~\mathrm{u},[/latex]
[latex]m_n=1.008665~\mathrm{u}.[/latex]

Strategy

The energy released in a nuclear reaction is determined from the decrease in total mass. First calculate the combined mass of the fission products. Then subtract this value from the mass of the original uranium-238 nucleus to obtain the mass defect, [latex]\Delta m[/latex]. Finally, use

[latex]E=\Delta mc^2[/latex]

and the conversion

[latex]1~\mathrm{u}=931.5~\mathrm{MeV}/c^2.[/latex]

Solution

The total mass of the products is

[latex]\begin{aligned} m_{\mathrm{products}} &= m\left({}^{95}\mathrm{Sr}\right) + m\left({}^{140}\mathrm{Xe}\right) + 3m_n \\ &= 94.919388~\mathrm{u} + 139.921610~\mathrm{u} + 3\left(1.008665~\mathrm{u}\right) \\ &= 237.866993~\mathrm{u}. \end{aligned}[/latex]

The mass defect is therefore

[latex]\begin{aligned} \Delta m &= m\left({}^{238}\mathrm{U}\right) - m_{\mathrm{products}} \\ &= 238.050784~\mathrm{u} - 237.866993~\mathrm{u} \\ &= 0.183791~\mathrm{u}. \end{aligned}[/latex]

The energy released is

[latex]\begin{aligned} E &= \Delta mc^2 \\ &= \left(0.183791~\mathrm{u}\right) \left( \frac{931.5~\mathrm{MeV}/c^2}{\mathrm{u}} \right)c^2 \\ &= 171.2~\mathrm{MeV}. \end{aligned}[/latex]

Thus, the spontaneous fission reaction releases approximately

[latex]\boxed{E=171~\mathrm{MeV}}.[/latex]

Discussion

An energy release of 171 MeV from a single nucleus is extremely large compared with the energy released in chemical reactions. It is somewhat smaller than the rough estimate of 240 MeV obtained by assuming that the nucleus splits into two equal fragments and gains approximately 1 MeV of binding energy per nucleon.

The difference arises because actual fission reactions do not usually divide a nucleus into two equal pieces. In this reaction, the fragments have different mass numbers, and three free neutrons are also produced. Some of the available energy is associated with the masses and motion of these neutrons and with excited states of the fission fragments.

Fission is a statistical process. A particular nuclide such as uranium-238 can split into many different combinations of daughter nuclei, each with its own probability and energy release. The number of emitted neutrons also varies from one event to another.

The production of free neutrons is one of the most important features of fission. Because neutrons carry no electric charge, they can enter nearby nuclei without being repelled by the positive charge of the nucleus. These neutrons may therefore induce additional fission reactions, making a self-sustaining nuclear chain reaction possible.

Neutron-Induced Fission and Nuclear Chain Reactions

Although some heavy nuclei undergo spontaneous fission, this is usually a relatively rare decay mode. For example, uranium-238 can split spontaneously, but it is far more likely to decay by emitting an alpha particle. In practice, most nuclear reactors rely on neutron-induced fission, in which an incoming neutron is absorbed by a heavy nucleus and causes it to split.

Neutrons are especially effective at initiating fission because they carry no electric charge. Unlike positively charged particles, they are not repelled by the positively charged nucleus. Even slow-moving neutrons can approach a heavy nucleus closely enough for the attractive strong nuclear force to capture them.

A useful way to visualize this process is the liquid drop model of the nucleus. In this model, a large nucleus behaves somewhat like a vibrating liquid droplet. When a neutron is absorbed, it deposits energy into the nucleus, causing it to oscillate and become distorted. As the nucleus stretches, it develops a narrow "neck" between two larger regions. At this point, the attractive strong nuclear force holding the nucleus together weakens, while the electrostatic repulsion between the many protons becomes increasingly important. If the deformation becomes large enough, the nucleus separates into two smaller nuclei, releasing additional neutrons and a large amount of energy.

A general neutron-induced fission reaction can be written as

[latex]n+{}^{A}X \rightarrow \mathrm{FF}_1 + \mathrm{FF}_2 + xn,[/latex]

where [latex]\mathrm{FF}_1[/latex] and [latex]\mathrm{FF}_2[/latex] are the two fission fragments, and [latex]x[/latex] is the number of neutrons emitted. The two fragments usually have different masses rather than splitting exactly in half. Most of the released energy appears as the kinetic energy of the fission fragments, while the remainder is carried by the emitted neutrons and gamma rays.

The emitted neutrons are particularly important because they can trigger additional fission events. If each fission produces, on average, more than one neutron that successfully induces another fission, a self-sustaining chain reaction becomes possible.

A typical neutron-induced fission reaction is

[latex]n + {}^{235}_{92}\mathrm{U} \rightarrow {}^{142}_{56}\mathrm{Ba} + {}^{91}_{36}\mathrm{Kr} + 3n.[/latex]

As with every nuclear reaction, both electric charge and nucleon number are conserved. In this example, the total charge remains

[latex]92+0=56+36,[/latex]

and the total number of nucleons is also conserved:

[latex]1+235=142+91+3.[/latex]

Although these whole numbers balance exactly, the total mass of the products is slightly smaller than the mass of the reactants. This small mass difference is converted into the large amount of energy released during fission.

Illustration of neutron-induced fission. A neutron is absorbed by a heavy nucleus, causing it to deform into an elongated shape before splitting into two smaller nuclei and several free neutrons.
Figure 122.2: A neutron absorbed by a heavy nucleus deposits energy that causes the nucleus to deform. As the attractive nuclear force becomes less effective across the stretched nucleus, electrostatic repulsion between protons causes the nucleus to split into two fission fragments while releasing additional neutrons and energy.
Illustration of a nuclear chain reaction in which neutrons released from one fission event trigger additional fission reactions in neighboring uranium nuclei.
Figure 122.3: A nuclear chain reaction occurs when neutrons released during one fission event induce additional fission reactions in nearby nuclei. If enough neutrons continue the process, the reaction becomes self-sustaining.

Critical Mass and Fission Fuels

Not every neutron released during fission causes another nucleus to split. Some neutrons escape from the material, while others are absorbed without producing fission. For a chain reaction to continue, enough neutrons must remain available to trigger additional fission events.

The smallest quantity of fissile material capable of sustaining a chain reaction is called the critical mass. Below the critical mass, too many neutrons escape and the reaction quickly dies out. Above the critical mass, enough neutrons remain inside the material for the chain reaction to continue.

Different isotopes require different critical masses because they differ in both the number of neutrons emitted during fission and the probability that an incoming neutron will produce another fission event. For example, plutonium-239 generally releases slightly more neutrons per fission than uranium-235 and therefore requires a smaller critical mass.

The isotopes [latex]{}^{235}\mathrm{U}[/latex] and [latex]{}^{239}\mathrm{Pu}[/latex] are much easier to fission than the much more abundant [latex]{}^{238}\mathrm{U}[/latex]. One reason is related to the number of neutrons in the nucleus. Uranium-235 and plutonium-239 each contain an odd number of neutrons, whereas uranium-238 contains an even number. When an additional neutron is absorbed by a nucleus with an odd number of neutrons, the resulting even-neutron nucleus gains extra binding energy, making it easier for the nucleus to deform and undergo fission.

Naturally occurring uranium contains about 99.3% uranium-238 but only about 0.7% uranium-235. Because uranium-235 is the isotope most useful for sustaining a chain reaction, reactor fuel is usually enriched to increase its concentration before use. Modern enrichment methods primarily use gas centrifuges, which are significantly more energy-efficient than the older gaseous diffusion process.

Another important property of uranium-235 is that it fissions most readily after absorbing slow (thermal) neutrons. However, the neutrons produced by fission are fast, with energies of roughly 1 MeV or more. Nuclear reactors therefore include a moderator, usually ordinary water, which slows the neutrons through repeated collisions with hydrogen nuclei. Once slowed, these thermal neutrons are much more likely to induce additional fission events in uranium-235, allowing a controlled chain reaction to continue.

Diagram of a pressurized water reactor. Fuel rods and control rods are located in a reactor vessel filled with pressurized water. Heat from the reactor is transferred to a separate water loop that produces steam, which drives a turbine and electrical generator. The steam is then condensed and returned to the system.
Figure 122.4: In a pressurized water reactor, fission heats water in a closed primary loop. Because this water is maintained at high pressure, it remains liquid and transfers thermal energy to a separate secondary loop. Steam produced in the secondary loop turns a turbine connected to an electrical generator. Control rods regulate the neutron population and maintain a steady chain reaction.

Controlling Fission in a Nuclear Reactor

Nuclear reactors use control rods made from materials that readily absorb neutrons. By inserting or withdrawing these rods from the reactor core, operators adjust the number of neutrons available to produce additional fission reactions. This makes it possible to increase, decrease, or maintain the reactor's power output.

A reactor operates normally in a condition called criticality. In this state, each fission event causes, on average, one additional fission, so the reaction rate and power output remain approximately constant. The term critical does not mean that the reactor is in danger; it describes a stable, self-sustaining chain reaction.

If too few neutrons cause further fissions, the reactor is subcritical, and the chain reaction decreases. If more than one neutron from each fission produces another fission, the system is supercritical, and the reaction rate increases. Controlled changes in reactivity are part of routine reactor operation, but a rapid or unintended increase must be prevented.

In many reactors, water serves two important purposes. First, it acts as a moderator, slowing fast fission neutrons so that they are more likely to induce fission in uranium-235. Second, it acts as a coolant, carrying thermal energy away from the reactor core. Changes in the temperature and density of the water can also influence the rate of the chain reaction, providing an important form of feedback.

Stopping the fission chain reaction does not immediately eliminate all heat production. The fission fragments created during reactor operation are radioactive and continue to decay after the control rods have been inserted. This decay heat decreases with time but can initially remain large enough to damage the fuel if cooling is lost. For this reason, reactors include emergency cooling systems, backup power supplies, reinforced containment structures, and other safety systems designed to remove residual heat during a shutdown or loss-of-coolant accident.

Example 122.2: Calculating the Energy from One Kilogram of Fissionable Fuel

Calculate the energy produced if 1.00 kg of [latex]{}^{235}\mathrm{U}[/latex] undergoes fission. Assume that each fission event releases an average energy of 200 MeV.

Strategy

The total energy is equal to the number of uranium-235 nuclei multiplied by the energy released per fission. We therefore need to:

  1. Convert the mass of uranium-235 into moles.
  2. Use Avogadro's number to determine the number of nuclei.
  3. Multiply by 200 MeV per fission.
  4. Convert the resulting energy from mega-electron volts to joules.

Solution

The molar mass of uranium-235 is approximately 235.04 g/mol. The number of moles in 1.00 kg is

[latex]n = \frac{1000~\mathrm{g}}{235.04~\mathrm{g/mol}} = 4.25~\mathrm{mol}.[/latex]

The number of uranium-235 nuclei is therefore

[latex]\begin{aligned} N &= \left(4.25~\mathrm{mol}\right) \left(6.02\times10^{23}~\mathrm{nuclei/mol}\right) \\ &= 2.56\times10^{24}~\mathrm{nuclei}. \end{aligned}[/latex]

If every nucleus undergoes fission, the total energy released is

[latex]\begin{aligned} E &= \left(2.56\times10^{24}~\mathrm{fissions}\right) \left(\frac{200~\mathrm{MeV}}{\mathrm{fission}}\right) \left(\frac{1.60\times10^{-13}~\mathrm{J}}{\mathrm{MeV}}\right) \\ &= 8.21\times10^{13}~\mathrm{J}. \end{aligned}[/latex]

Thus, the complete fission of 1.00 kg of uranium-235 would release approximately

[latex]\boxed{E=8.21\times10^{13}~\mathrm{J}}.[/latex]

Discussion

This is an enormous amount of energy for such a small mass of fuel. It is equivalent to the energy released by burning millions of liters of gasoline. The comparison illustrates why nuclear fuels have a much greater energy density than chemical fuels: nuclear reactions involve changes in nuclear binding energy, whereas combustion involves much smaller changes in the electromagnetic energy of atoms and molecules.

Although a single fission event releases more energy than a single fusion reaction, the energy released per kilogram of fuel can be larger for certain fusion fuels. Heavy uranium nuclei have a large mass, so one kilogram contains fewer nuclei than one kilogram of light fusion fuel contains reacting nuclei.

The calculated value also represents an ideal maximum in which every uranium-235 nucleus undergoes fission and all released energy is captured. In an operating power plant, not all fuel nuclei fission, and only part of the thermal energy is converted into electrical energy.

Breeding Fissionable Fuel

Plutonium-239 is another important fissile isotope. It has a half-life of approximately 24,100 years and is produced artificially from uranium-238 inside nuclear reactors. This process makes it possible to convert a nuclide that does not readily undergo fission with thermal neutrons into one that can serve as reactor fuel.

The production of a fissile nuclide from another nuclide is called breeding. The production of plutonium-239 begins when uranium-238 captures a neutron:

[latex]{}^{238}\mathrm{U} + n \rightarrow {}^{239}\mathrm{U} + \gamma.[/latex]

The uranium-239 nucleus is radioactive and undergoes beta-minus decay:

[latex]{}^{239}\mathrm{U} \rightarrow {}^{239}\mathrm{Np} + \beta^- + \overline{\nu}_e, \qquad t_{1/2}\approx23~\mathrm{min}.[/latex]

During beta-minus decay, a neutron in the nucleus changes into a proton, so the atomic number increases from 92 to 93 while the mass number remains 239. The resulting nucleus is neptunium-239.

Neptunium-239 then undergoes another beta-minus decay:

[latex]{}^{239}\mathrm{Np} \rightarrow {}^{239}\mathrm{Pu} + \beta^- + \overline{\nu}_e, \qquad t_{1/2}\approx2.4~\mathrm{d}.[/latex]

This second decay increases the atomic number from 93 to 94, producing plutonium-239. The complete breeding sequence can therefore be summarized as

[latex]{}^{238}\mathrm{U} \xrightarrow{\,n,\gamma\,} {}^{239}\mathrm{U} \xrightarrow{\,\beta^-\,} {}^{239}\mathrm{Np} \xrightarrow{\,\beta^-\,} {}^{239}\mathrm{Pu}.[/latex]

Plutonium-239 accumulates in uranium-based reactor fuel because uranium-238 nuclei absorb some of the neutrons produced during fission. Some of the resulting plutonium-239 later undergoes fission and contributes to the reactor's energy output.

A breeder reactor is designed to produce fissile material from more abundant nonfissile, or fertile, isotopes. In principle, breeding can make more efficient use of natural uranium because uranium-238 represents nearly all naturally occurring uranium. Breeder systems, however, require careful fuel processing, reactor control, waste management, and safeguards because they produce and handle materials with significant radiological and security concerns.

Plutonium-239 has several properties that make it useful as a reactor fuel. It can undergo fission after absorbing a thermal neutron, and each fission releases enough neutrons to support a chain reaction. It is also chemically different from uranium, which allows the two elements to be separated through chemical processing of used reactor fuel.

Radiation Protection and Reactor Medicine

The radioactive fission products remaining in used reactor fuel continue to emit beta particles, gamma rays, and other radiation long after the reactor is shut down. The same principles used in healthcare radiation protection—time, distance, shielding, contamination control, and careful dose monitoring—are also essential in nuclear facilities. However, reactor fuel contains much larger activities and requires heavily shielded systems, remote handling, continuous cooling, and long-term waste management.

Interactive Exploration: Nuclear Fission

Nuclear fission occurs when a heavy nucleus absorbs a neutron and splits into two smaller nuclei. This process releases a large amount of energy along with two or three additional neutrons. If these neutrons induce fission in nearby nuclei, the process can continue as a chain reaction. Whether the reaction dies out, remains steady, or grows rapidly depends on how many neutrons continue to produce additional fission events.

In this interactive simulation, you will investigate how chain reactions begin, why a critical amount of fuel is required, and how nuclear reactors safely regulate fission. You will also explore the effects of neutron-absorbing control rods and non-fissionable materials on the behavior of the chain reaction.

Figure 122.X. Explore how neutron-induced fission creates chain reactions and how control rods regulate the neutron population in a nuclear reactor using the PhET Nuclear Fission simulation.

Guided Exploration

As you work through the simulation, consider the following questions:

  1. Begin with a single neutron striking a uranium nucleus. What particles are produced during the fission event, and where does the released energy appear?
  2. Observe the neutrons emitted during fission. How do these neutrons initiate additional fission reactions?
  3. Create a self-sustaining chain reaction. What conditions are necessary for the reaction to continue without dying out?
  4. Experiment with different amounts of fissile material. How does the amount of fuel affect whether the reaction is subcritical, critical, or supercritical?
  5. Insert and remove the control rods. How do they change the number of neutrons available to produce additional fission reactions?
  6. Replace some fissile nuclei with non-fissionable isotopes. How does this influence the likelihood of maintaining a chain reaction?
  7. Based on your observations, explain how nuclear reactors maintain a controlled chain reaction while preventing the rapid increase in power associated with an uncontrolled reaction.

After completing the simulation, compare your observations with the concepts presented in this chapter. Every fission event converts a small amount of mass into energy according to

[latex]E=\Delta mc^2.[/latex]

Because fission also releases additional neutrons, one reaction can trigger many others. A reactor operates safely by maintaining criticality, in which each fission event produces, on average, one additional fission. Control rods and the moderator regulate the neutron population, allowing electrical energy to be generated steadily without an uncontrolled chain reaction.

Section Summary

  • Nuclear fission is a nuclear reaction in which a heavy nucleus splits into two smaller nuclei while releasing energy and additional neutrons.
  • Fission releases energy because the products have a greater [latex]\mathrm{BE}/A[/latex] than the original heavy nucleus, resulting in a decrease in mass that is converted into energy.
  • Most practical reactors rely on neutron-induced fission, which can be represented by
    [latex]n+{}^{A}X \rightarrow \mathrm{FF}_1 + \mathrm{FF}_2 + xn,[/latex]

    where [latex]\mathrm{FF}_1[/latex] and [latex]\mathrm{FF}_2[/latex] are the fission fragments and [latex]x[/latex] is the number of neutrons emitted.

  • A chain reaction becomes self-sustaining when enough of the emitted neutrons produce additional fission events.
  • The minimum quantity of fissile material required to sustain a chain reaction is called the critical mass. Below this amount the reaction dies out, while above it the reaction can become self-sustaining.
  • A reactor operating at criticality maintains a steady chain reaction. If the reaction rate increases uncontrollably, the reactor becomes supercritical.
  • Control rods, moderators, and cooling systems work together to regulate the neutron population, remove heat from the reactor core, and maintain safe operation.
  • Breeding is the production of new fissile isotopes, such as plutonium-239, from fertile materials like uranium-238. Reactors designed to maximize this process are known as breeder reactors.

Conceptual Questions

  1. Explain why the fission of heavy nuclei releases energy. Similarly, why is an input of energy required to fission light nuclei?
  2. Using conservation of momentum and energy, explain why collisions with protons thermalize neutrons more effectively than collisions with oxygen nuclei.
  3. The remains of the damaged Chernobyl reactor were enclosed within large protective structures after the accident. At times, water entered the original structure and increases in neutron activity were observed. What does this suggest may have been occurring inside the reactor material?
  4. A uranium or plutonium nucleus can fission into many different combinations of fragments whose masses cover a wide range. Would you expect fission to produce more residual radioactivity than fusion? Explain.
  5. The core of a nuclear reactor continues to generate thermal energy from the radioactive decay of fission products even after the power-producing chain reaction has been stopped. Would this residual heat be greater after the reactor has operated for a long time or for a short time? What happens to the residual heat after the reactor has been shut down for several months?
  6. How can a nuclear reactor contain many critical masses of fissile material without becoming dangerously supercritical? What methods are used to control the fission rate?
  7. Why can heavy nuclei containing an odd number of neutrons be induced to fission by thermal neutrons, whereas nuclei containing an even number of neutrons generally require a greater input of energy?
  8. Why is a conventional nuclear fission reactor unable to explode in the same manner as a nuclear weapon?

Problems

  1. (a) Calculate the energy released in the following neutron-induced fission reaction, which is similar to the spontaneous fission reaction examined in Example 122.1:
    [latex]n+{}^{238}\mathrm{U} \rightarrow {}^{96}\mathrm{Sr} + {}^{140}\mathrm{Xe} + 3n.[/latex]

    Use

    [latex]m\left({}^{96}\mathrm{Sr}\right)=95.921750~\mathrm{u}[/latex]

    and

    [latex]m\left({}^{140}\mathrm{Xe}\right)=139.92164~\mathrm{u}.[/latex]

    (b) This result is approximately 6 MeV greater than the result obtained for spontaneous fission in Example 122.1. Explain why.

    (c) Confirm that the total number of nucleons and the total electric charge are conserved in this reaction.

  2. (a) Calculate the energy released in the following neutron-induced fission reaction:
    [latex]n+{}^{235}\mathrm{U} \rightarrow {}^{92}\mathrm{Kr} + {}^{142}\mathrm{Ba} + 2n.[/latex]

    Use

    [latex]m\left({}^{92}\mathrm{Kr}\right)=91.926269~\mathrm{u}[/latex]

    and

    [latex]m\left({}^{142}\mathrm{Ba}\right)=141.916361~\mathrm{u}.[/latex]

    (b) Confirm that the total number of nucleons and the total electric charge are conserved in this reaction.

  3. (a) Calculate the energy released in the following neutron-induced fission reaction:
    [latex]n+{}^{239}\mathrm{Pu} \rightarrow {}^{96}\mathrm{Sr} + {}^{140}\mathrm{Ba} + 4n.[/latex]

    Use

    [latex]m\left({}^{96}\mathrm{Sr}\right)=95.921750~\mathrm{u}[/latex]

    and

    [latex]m\left({}^{140}\mathrm{Ba}\right)=139.910581~\mathrm{u}.[/latex]

    (b) Confirm that the total number of nucleons and the total electric charge are conserved in this reaction.

  4. Confirm that each reaction in the plutonium-239 breeding sequence presented after Example 122.2 conserves all of the following:
    1. the total number of nucleons,
    2. the total electric charge, and
    3. the electron-family lepton number.
  5. The breeding of plutonium releases energy even before any of the plutonium undergoes fission. Calculate the energy released in each reaction of the plutonium-239 breeding sequence presented after Example 122.2.Use the following atomic masses:
    [latex]m\left({}^{239}\mathrm{U}\right)=239.054289~\mathrm{u},[/latex]
    [latex]m\left({}^{239}\mathrm{Np}\right)=239.052932~\mathrm{u},[/latex]
    [latex]m\left({}^{239}\mathrm{Pu}\right)=239.052157~\mathrm{u}.[/latex]

    The first reaction in the sequence is

    [latex]{}^{238}\mathrm{U}+n \rightarrow {}^{239}\mathrm{U}+\gamma.[/latex]

    Check for the first reaction: 4.81 MeV.

  6. The naturally occurring radioactive isotope [latex]{}^{232}\mathrm{Th}[/latex] is not readily fissioned by thermal neutrons because it contains an even number of neutrons. However, it can be converted into a suitable fissile fuel through a breeding process similar to the conversion of uranium-238 into plutonium-239.
    1. Determine the values of [latex]Z[/latex] and [latex]N[/latex] for [latex]{}^{232}\mathrm{Th}[/latex].
    2. Write the reaction equation for neutron capture by thorium-232 and identify the nuclide [latex]{}^{A}X[/latex] produced in
      [latex]n+{}^{232}\mathrm{Th} \rightarrow {}^{A}X+\gamma.[/latex]
    3. The product nucleus undergoes beta-minus decay, and its daughter nucleus also undergoes beta-minus decay. Write both decay equations and identify the final nucleus.
    4. Confirm that the final nucleus has an odd number of neutrons, making it more suitable as a fission fuel.
    5. Look up the half-life of the final nucleus and determine whether it lives long enough to be useful as a reactor fuel.
  7. The electrical power output of a large nuclear power facility is 900 MW. The facility is 35.0% efficient in converting thermal energy from fission into electrical energy.
    1. What is the thermal power generated by the reactor, in megawatts?
    2. How many uranium-235 nuclei undergo fission each second if each fission releases an average of 200 MeV?
    3. What mass of uranium-235 undergoes fission during one year of continuous full-power operation?
  8. A large power reactor that has operated for several months is shut down, but the radioactive decay of fission products in the core continues to produce 150 MW of thermal power. If the average energy released per decay is 1.00 MeV, what is the activity of the reactor core in curies?

Glossary

breeder reactor
A nuclear reactor designed to convert fertile isotopes, such as [latex]{}^{238}\mathrm{U}[/latex], into fissile fuel such as [latex]{}^{239}\mathrm{Pu}[/latex] through neutron capture and subsequent radioactive decay.
breeding
The process of producing a new fissile isotope by nuclear transformation. An important example is the conversion of uranium-238 into plutonium-239 inside a nuclear reactor.
criticality
The operating condition in which a nuclear chain reaction is self-sustaining because each fission event produces, on average, one additional fission.
critical mass
The minimum amount of fissile material required to sustain a nuclear chain reaction under specified conditions.
fission fragments
The two smaller daughter nuclei produced when a heavy nucleus undergoes nuclear fission.
liquid drop model
A simplified model of the atomic nucleus that treats it as a liquid droplet, helping explain phenomena such as nuclear deformation and fission.
nuclear fission
A nuclear reaction in which a heavy atomic nucleus splits into two or more smaller nuclei, releasing energy and usually several neutrons.
neutron-induced fission
A fission reaction initiated when a nucleus absorbs an incoming neutron.
supercriticality
A condition in which more than one neutron from each fission event causes another fission, leading to an increasing rate of nuclear reactions.
definition

License

Icon for the Creative Commons Attribution 4.0 International License

Introductory Physics for the Health and Life Sciences II Copyright © 2012 by OSCRiceUniversity is licensed under a Creative Commons Attribution 4.0 International License, except where otherwise noted.