Fission 2 5 0 5

1. Fission 2 5 0 5 Equals
2. Fission 2 5 0 52
3. Fission 2 5 0 5 Equation
4. Fission 2 5 0 5 X 4

Fission track dating d. Some australopithecines are referred to as a 'robust' because: a. They were much taller than their ancestors. Fission 2.5.0 破解版 (好用的音乐裁切编辑工具). Fission releases energy when heavy nuclei are split into medium-mass nuclei. Self-sustained fission is possible, because neutron-induced fission also produces neutrons that can induce other fissions, n + A X → FF 1 + FF 2 + xn, where FF 1 and FF 2 are the two daughter nuclei, or fission fragments, and x is the number of neutrons produced. Fission operates on just the code: Docker and Kubernetes are abstracted away under normal operation, though you can use both to extend Fission if you want to. Fission is extensible to any language; the core is written in Go, and language-specific parts are isolated in something called environments (more below).

Spontaneous fission (SF) is a form of radioactive decay that is found only in very heavy chemical elements. The nuclear binding energy of the elements reaches its maximum at an atomic mass number of about 56; spontaneous breakdown into smaller nuclei and a few isolated nuclear particles becomes possible at greater atomic mass numbers.

Fission 2.5.0 macOS 10.7 MB Crop and trim audio, paste in or join files, or just rapidly split one long file into many. Fission is streamlined for fast editing. Plus, it works without the quality loss caused by other editors, so you can get perfect quality audio even when editing MP3 and AAC files.

History[edit]

By 1908, the process of alpha decay was known to consist of the ejection of helium nuclei from the decaying atom;^[1] however, as with cluster decay, alpha decay is not typically categorized as a process of fission.^[2]

The first nuclear fission process discovered was fission induced by neutrons. Because cosmic rays produce some neutrons, it was difficult to distinguish between induced and spontaneous events. Cosmic rays can be reliably shielded by a thick layer of rock or water. Spontaneous fission was identified in 1940 by Soviet physicists Georgy Flyorov and Konstantin Petrzhak^[3][4] by their observations of uranium in the Moscow MetroDinamo station, 60 metres (200 ft) underground.^[5]

Cluster decay was shown to be a superasymmetric spontaneous fission process.^[6]

Feasibility[edit]

Elemental[edit]

Spontaneous fission is feasible over practical observation times only for atomic masses of 232 amu or more. These are elements at least as heavy as thorium-232 – which has a half-life somewhat longer than the age of the universe. ²³²Th, ²³⁵U, and ²³⁸U are primordial nuclides and have left evidence of undergoing spontaneous fission in their minerals.

The known elements most susceptible to spontaneous fission are the synthetic high-atomic-number actinides and transactinides with atomic numbers from 100 onwards.

For naturally occurring thorium-232, uranium-235, and uranium-238, spontaneous fission does occur rarely, but in the vast majority of the radioactive decay of these atoms, alpha decay or beta decay occurs instead. Hence, the spontaneous fission of these isotopes is usually negligible, except in using the exact branching ratios when finding the radioactivity of a sample of these elements.

Mathematical[edit]

The liquid drop model predicts approximately that spontaneous fission can occur in a time short enough to be observed by present methods when

Z2A≥47.{displaystyle {frac {Z^{2}}{A}}geq 47.}^[7]

where Z is the atomic number and A is the mass number (e.g., Z²/A = 36 for uranium-235). However, all known nuclides which undergo spontaneous fission as their main decay mode do not reach this value of 47, as the liquid drop model is not very accurate for the heaviest known nuclei due to strong shell effects.

Spontaneous fission rates[edit]

In practice, ²³⁹
Pu
will invariably contain a certain amount of ²⁴⁰
Pu
due to the tendency of ²³⁹
Pu
to absorb an additional neutron during production. ²⁴⁰
Pu
's high rate of spontaneous fission events makes it an undesirable contaminant. Weapons-grade plutonium contains no more than 7.0% ²⁴⁰
Pu
.

The rarely used gun-type atomic bomb has a critical insertion time of about one millisecond, and the probability of a fission during this time interval should be small. Therefore, only ²³⁵
U
is suitable. Almost all nuclear bombs use some kind of implosion method.

Spontaneous fission can occur much more rapidly when the nucleus of an atom undergoes superdeformation.

Poisson process[edit]

Spontaneous fission gives much the same result as induced nuclear fission. However, like other forms of radioactive decay, it occurs due to quantum tunneling, without the atom having been struck by a neutron or other particle as in induced nuclear fission. Spontaneous fissions release neutrons as all fissions do, so if a critical mass is present, a spontaneous fission can initiate a self-sustaining chain reaction. Radioisotopes for which spontaneous fission is not negligible can be used as neutron sources. For example, californium-252 (half-life 2.645 years, SF branch ratio about 3.1 percent) can be used for this purpose. 4ukey – password manager 1 0 1 2 3. The neutrons released can be used to inspect airline luggage for hidden explosives, to gauge the moisture content of soil in highway and building construction, or to measure the moisture of materials stored in silos, for example.

As long as the spontaneous fission gives a negligible reduction of the number of nuclei that can undergo such fission, this process can be approximated closely as a Poisson process. In this situation, for short time intervals the probability of a spontaneous fission is directly proportional to the length of time.

The spontaneous fission of uranium-238 and uranium-235 does leave trails of damage in the crystal structure of uranium-containing minerals when the fission fragments recoil through them. These trails, or fission tracks, are the foundation of the radiometric dating method called fission track dating.

See also[edit]

Notes[edit]

1. ^Rutherford, E.; Royds, T. (1908). 'XXIV.Spectrum of the radium emanation'. Philosophical Magazine. series 6. 16 (92): 313–317. doi:10.1080/14786440808636511.
2. ^Santhosh, K P; Biju, R K (1 January 2009). 'Alpha decay, cluster decay and spontaneous fission in (294–326)122 isotopes'. Journal of Physics G: Nuclear and Particle Physics. 36 (1): 015107. Bibcode:2009JPhG..36a5107S. doi:10.1088/0954-3899/36/1/015107.
3. ^G. Scharff-Goldhaber and G. S. Klaiber (1946). 'Spontaneous Emission of Neutrons from Uranium'. Phys. Rev. 70 (3–4): 229. Bibcode:1946PhRv..70.229S. doi:10.1103/PhysRev.70.229.2.
4. ^Igor Sutyagin: The role of nuclear weapons and its possible future missions
5. ^Petrzhak, Konstantin. 'How the spontaneous fission was discovered' (in Russian).
6. ^Dorin N Poenaru; et al. (1984). 'Spontaneous emission of heavy clusters'. Journal of Physics G: Nuclear Physics. 10 (8): L183–L189. Bibcode:1984JPhG..10L.183P. doi:10.1088/0305-4616/10/8/004.
7. ^Krane, Kenneth S. (1988). Introductory Nuclear Physics. John Wiley & Sons. pp. 483–484 (Equation 13.3). ISBN978-0-471-80553-3.
8. ^Shultis, J. Kenneth; Richard E. Faw (2008). Fundamentals of Nuclear Science and Engineering. CRC Press. pp. 141 (table 6.2). ISBN978-1-4200-5135-3.
9. ^Entry at periodictable.com
10. ^Entry at periodictable.com

External links[edit]

• The LIVEChart of Nuclides - IAEA with filter on spontaneous fission decay

LEARNING OBJECTIVES

By the end of this section, you will be able to:

• Define nuclear fission.
• Discuss how fission fuel reacts and describe what it produces.
• Describe controlled and uncontrolled chain reactions.

Nuclear fission is a reaction in which a nucleus is split (or fissured). Controlled fission is a reality, whereas controlled fusion is a hope for the future. Hundreds of nuclear fission power plants around the world attest to the fact that controlled fission is practical and, at least in the short term, economical, as seen in Figure 1. Whereas nuclear power was of little interest for decades following TMI and Chernobyl (and now Fukushima Daiichi), growing concerns over global warming has brought nuclear power back on the table as a viable energy alternative. By the end of 2009, there were 442 reactors operating in 30 countries, providing 15% of the world's electricity. France provides over 75% of its electricity with nuclear power, while the US has 104 operating reactors providing 20% of its electricity. Australia and New Zealand have none. China is building nuclear power plants at the rate of one start every month.

Figure 1. The people living near this nuclear power plant have no measurable exposure to radiation that is traceable to the plant. About 16% of the world's electrical power is generated by controlled nuclear fission in such plants. The cooling towers are the most prominent features but are not unique to nuclear power. The reactor is in the small domed building to the left of the towers. (credit: Kalmthouts)

Fission is the opposite of fusion and releases energy only when heavy nuclei are split. As noted in Fusion, energy is released if the products of a nuclear reaction have a greater binding energy per nucleon (BE/A) than the parent nuclei. Figure 2 shows that BE/A is greater for medium-mass nuclei than heavy nuclei, implying that when a heavy nucleus is split, the products have less mass per nucleon, so that mass is destroyed and energy is released in the reaction. The amount of energy per fission reaction can be large, even by nuclear standards. The graph in Figure 2 shows BE/A to be about 7.6 MeV/nucleon for the heaviest nuclei (A about 240), while BE/A is about 8.6 MeV/nucleon for nuclei having A about 120. Thus, if a heavy nucleus splits in half, then about 1 MeV per nucleon, or approximately 240 MeV per fission, is released. This is about 10 times the energy per fusion reaction, and about 100 times the energy of the average α, β, or γ decay.

Example 1. Calculating Energy Released by Fission

Calculate the energy released in the following spontaneous fission reaction:

²³⁸U → ⁹⁵Sr + ¹⁴⁰Xe + 3n

given the atomic masses to be m(²³⁸U) = 238.050784 u, m(⁹⁵Sr) = 94.919388 u, m(¹⁴⁰Xe) = 139.921610 u, and m(n) =1.008665 u.

Strategy

As always, the energy released is equal to the mass destroyed times c², so we must find the difference in mass between the parent ²³⁸U and the fission products.

Solution

The products have a total mass of

[latex]begin{array}{lll}{m}_{text{products}}& =& 94.919388text{ u}+139.921610 text{ u}+3left(1.008665text{ u}right) & =& 237.866993text{ u}end{array}[/latex]

The mass lost is the mass of ²³⁸U minus m_products, or

so the energy released is

[latex]begin{array}{lll}E& =& left(Delta mright){c}^{2} & =& left(0.183791text{ u}right)frac{931.5text{ Me}text{V/}{c}^{2}}{text{u}}{c}^{2}=171.2text{ MeV}end{array}[/latex]

Discussion

A number of important things arise in this example. The 171-MeV energy released is large, but a little less than the earlier estimated 240 MeV. This is because this fission reaction produces neutrons and does not split the nucleus into two equal parts. Fission of a given nuclide, such as ²³⁸U , does not always produce the same products. Fission is a statistical process in which an entire range of products are produced with various probabilities. Most fission produces neutrons, although the number varies with each fission. This is an extremely important aspect of fission, because neutrons can induce more fission, enabling self-sustaining chain reactions.

Spontaneous fission can occur, but this is usually not the most common decay mode for a given nuclide. For example, ²³⁸U can spontaneously fission, but it decays mostly by α emission. Neutron-induced fission is crucial as seen in Figure 2. Being chargeless, even low-energy neutrons can strike a nucleus and be absorbed once they feel the attractive nuclear force. Large nuclei are described by a liquid drop model with surface tension and oscillation modes, because the large number of nucleons act like atoms in a drop. The neutron is attracted and thus, deposits energy, causing the nucleus to deform as a liquid drop. If stretched enough, the nucleus narrows in the middle. The number of nucleons in contact and the strength of the nuclear force binding the nucleus together are reduced. Coulomb repulsion between the two ends then succeeds in fissioning the nucleus, which pops like a water drop into two large pieces and a few neutrons. Neutron-induced fission can be written as

n + ^AX → FF₁ + FF₂ + xn,

where FF₁ and FF₂ are the two daughter nuclei, called fission fragments, and x is the number of neutrons produced. Most often, the masses of the fission fragments are not the same. Most of the released energy goes into the kinetic energy of the fission fragments, with the remainder going into the neutrons and excited states of the fragments. Since neutrons can induce fission, a self-sustaining chain reaction is possible, provided more than one neutron is produced on average — that is, if x>1 in n + ^AX → FF₁ + FF₂ + xn. This can also be seen in Figure 3. An example of a typical neutron-induced fission reaction is

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

Note that in this equation, the total charge remains the same (is conserved): 92 + 0 = 56 + 36. Also, as far as whole numbers are concerned, the mass is constant: 1 + 235 = 142 + 91 + 3. This is not true when we consider the masses out to 6 or 7 significant places, as in the previous example.

Figure 2. Neutron-induced fission is shown. First, energy is put into this large nucleus when it absorbs a neutron. Acting like a struck liquid drop, the nucleus deforms and begins to narrow in the middle. Since fewer nucleons are in contact, the repulsive Coulomb force is able to break the nucleus into two parts with some neutrons also flying away.

Figure 3. A chain reaction can produce self-sustained fission if each fission produces enough neutrons to induce at least one more fission. This depends on several factors, including how many neutrons are produced in an average fission and how easy it is to make a particular type of nuclide fission.

Not every neutron produced by fission induces fission. Some neutrons escape the fissionable material, while others interact with a nucleus without making it fission. We can enhance the number of fissions produced by neutrons by having a large amount of fissionable material. The minimum amount necessary for self-sustained fission of a given nuclide is called its critical mass. Some nuclides, such as ²³⁹Pu, produce more neutrons per fission than others, such as ²³⁵U . Additionally, some nuclides are easier to make fission than others. In particular, ²³⁵U and ²³⁹Pu, are easier to fission than the much more abundant ²³⁸U . Both factors affect critical mass, which is smallest for ²³⁹Pu.

The reason ²³⁵U and ²³⁹Pu are easier to fission than ²³⁸U is that the nuclear force is more attractive for an even number of neutrons in a nucleus than for an odd number. Consider that [latex]{}_{text{92}}^{text{235}}{text{U}}_{text{143}}[/latex] has 143 neutrons, and [latex]{}_{text{94}}^{text{239}}{text{P}}_{text{145}}[/latex] has 145 neutrons, whereas [latex]{}_{text{92}}^{text{238}}{text{U}}_{text{146}}[/latex] has 146. When a neutron encounters a nucleus with an odd number of neutrons, the nuclear force is more attractive, because the additional neutron will make the number even. About 2-MeV more energy is deposited in the resulting nucleus than would be the case if the number of neutrons was already even. This extra energy produces greater deformation, making fission more likely. Thus, ²³⁵U and ²³⁹Pu are superior fission fuels. The isotope ²³⁵U is only 0.72 % of natural uranium, while ²³⁸U is 99.27%, and ²³⁹Pu does not exist in nature. Australia has the largest deposits of uranium in the world, standing at 28% of the total. This is followed by Kazakhstan and Canada. The US has only 3% of global reserves.

Most fission reactors utilize ²³⁵U , which is separated from ²³⁸U at some expense. This is called enrichment. The most common separation method is gaseous diffusion of uranium hexafluoride (UF₆) through membranes. Since ²³⁵U has less mass than ²³⁸U , its UF₆ molecules have higher average velocity at the same temperature and diffuse faster. Another interesting characteristic of ²³⁵U is that it preferentially absorbs very slow moving neutrons (with energies a fraction of an eV), whereas fission reactions produce fast neutrons with energies in the order of an MeV. To make a self-sustained fission reactor with ²³⁵U , it is thus necessary to slow down ('thermalize') the neutrons. Water is very effective, since neutrons collide with protons in water molecules and lose energy. Figure 4 shows a schematic of a reactor design, called the pressurized water reactor.

Figure 4. A pressurized water reactor is cleverly designed to control the fission of large amounts of ²³⁵U , while using the heat produced in the fission reaction to create steam for generating electrical energy. Control rods adjust neutron flux so that criticality is obtained, but not exceeded. In case the reactor overheats and boils the water away, the chain reaction terminates, because water is needed to thermalize the neutrons. This inherent safety feature can be overwhelmed in extreme circumstances.

Control rods containing nuclides that very strongly absorb neutrons are used to adjust neutron flux. To produce large power, reactors contain hundreds to thousands of critical masses, and the chain reaction easily becomes self-sustaining, a condition called criticality. Neutron flux should be carefully regulated to avoid an exponential increase in fissions, a condition called supercriticality. Control rods help prevent overheating, perhaps even a meltdown or explosive disassembly. The water that is used to thermalize neutrons, necessary to get them to induce fission in ²³⁵U, and achieve criticality, provides a negative feedback for temperature increases. In case the reactor overheats and boils the water to steam or is breached, the absence of water kills the chain reaction. Considerable heat, however, can still be generated by the reactor's radioactive fission products. Other safety features, thus, need to be incorporated in the event of a loss of coolant accident, including auxiliary cooling water and pumps.

Example 2. Calculating Energy from a Kilogram of Fissionable Fuel

Calculate the amount of energy produced by the fission of 1.00 kg of ²³⁵U , given the average fission reaction of ²³⁵U produces 200 MeV.

Strategy

The total energy produced is the number of ²³⁵U atoms times the given energy per ²³⁵ U fission. We should therefore find the number of ²³⁵U atoms in 1.00 kg.

Solution

The number of ²³⁵U atoms in 1.00 kg is Avogadro's number times the number of moles. One mole of ²³⁵U has a mass of 235.04 g; thus, there are (1000 g)/(235.04 g/mol) = 4.25 mol. The number of ²³⁵U atoms is therefore,

[latex]left(4.25 text{ mol}right)left(6.02times {10}^{23}{}^{{235}text{U/mol}right)=2.56times{10}^{24}{}^text{ 235}text{U}[/latex].

So the total energy released is

[latex]begin{array}{lll}E & =& left(2.56times {10}^{24}{}^{235}text{U}right)left(frac{200text{ MeV}}{{}^{text{235}}text{U}}right)left(frac{1.60times {10}^{-13}text{ J}}{text{MeV}}right) & =& 8.21times {10}^{13}text{ J}end{array}[/latex].

Discussion

This is another impressively large amount of energy, equivalent to about 14,000 barrels of crude oil or 600,000 gallons of gasoline. But, it is only one-fourth the energy produced by the fusion of a kilogram mixture of deuterium and tritium as seen in Example 1. Calculating Energy and Power from Fusion. Even though each fission reaction yields about ten times the energy of a fusion reaction, the energy per kilogram of fission fuel is less, because there are far fewer moles per kilogram of the heavy nuclides. Fission fuel is also much more scarce than fusion fuel, and less than 1% of uranium (the ²³⁵U) is readily usable.

One nuclide already mentioned is ²³⁹Pu, which has a 24,120-y half-life and does not exist in nature. Plutonium-239 is manufactured from ²³⁸U in reactors, and it provides an opportunity to utilize the other 99% of natural uranium as an energy source. The following reaction sequence, called breeding, produces ²³⁹Pu. Breeding begins with neutron capture by ²³⁸U :

Uranium-239 then β^– decays:

²³⁹U →²³⁹Np + β⁻ +v_e(t_1/2 = 23 min).

Neptunium-239 also β^– decays:

²³⁹Np → ²³⁹Pu + β⁻ + v_e(t_1/2 = 2.4 d).

Plutonium-239 builds up in reactor fuel at a rate that depends on the probability of neutron capture by ²³⁸U (all reactor fuel contains more ²³⁸U than ²³⁵U). Reactors designed specifically to make plutonium are called breeder reactors. They seem to be inherently more hazardous than conventional reactors, but it remains unknown whether their hazards can be made economically acceptable. The four reactors at Chernobyl, including the one that was destroyed, were built to breed plutonium and produce electricity. These reactors had a design that was significantly different from the pressurized water reactor illustrated above. Plutonium-239 has advantages over ²³⁵U as a reactor fuel — it produces more neutrons per fission on average, and it is easier for a thermal neutron to cause it to fission. It is also chemically different from uranium, so it is inherently easier to separate from uranium ore. This means ²³⁹Pu has a particularly small critical mass, an advantage for nuclear weapons.

PhET Explorations: Nuclear Fission

Section Summary

• Nuclear fission is a reaction in which a nucleus is split.
• Fission releases energy when heavy nuclei are split into medium-mass nuclei.
• Self-sustained fission is possible, because neutron-induced fission also produces neutrons that can induce other fissions, n + ^AX → FF₁ + FF₂ + xn, where FF₁ and FF₂ are the two daughter nuclei, or fission fragments, and x is the number of neutrons produced.
• A minimum mass, called the critical mass, should be present to achieve criticality.
• More than a critical mass can produce supercriticality.
• The production of new or different isotopes (especially ²³⁹Pu) by nuclear transformation is called breeding, and reactors designed for this purpose are called breeder reactors.

Conceptual Questions

1. Explain why the fission of heavy nuclei releases energy. Similarly, why is it that energy input is required to fission light nuclei?
2. Explain, in terms of conservation of momentum and energy, why collisions of neutrons with protons will thermalize neutrons better than collisions with oxygen.
3. The ruins of the Chernobyl reactor are enclosed in a huge concrete structure built around it after the accident. Some rain penetrates the building in winter, and radioactivity from the building increases. What does this imply is happening inside?
4. Since the uranium or plutonium nucleus fissions into several fission fragments whose mass distribution covers a wide range of pieces, would you expect more residual radioactivity from fission than fusion? Explain.
5. The core of a nuclear reactor generates a large amount of thermal energy from the decay of fission products, even when the power-producing fission chain reaction is turned off. Would this residual heat be greatest after the reactor has run for a long time or short time? What if the reactor has been shut down for months?
6. How can a nuclear reactor contain many critical masses and not go supercritical? What methods are used to control the fission in the reactor?
7. Why can heavy nuclei with odd numbers of neutrons be induced to fission with thermal neutrons, whereas those with even numbers of neutrons require more energy input to induce fission?
8. Why is a conventional fission nuclear reactor not able to explode as a bomb?

Problems & Exercises

1. (a) Calculate the energy released in the neutron-induced fission (similar to the spontaneous fission in Example 1. Calculating Energy Released by Fission)

given m(⁹⁶Sr) = 95.921750 u and m(¹⁴⁰Xe) = 139.92164. (b) This result is about 6 MeV greater than the result for spontaneous fission. Why? (c) Confirm that the total number of nucleons and total charge are conserved in this reaction.

2. (a) Calculate the energy released in the neutron-induced fission reaction

given m(⁹²Kr) = 91.926269 u and m(¹⁴²Ba) = 141.916361 u.

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

3. (a) Calculate the energy released in the neutron-induced fission reaction

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

Fission 2 5 0 5 Equals

4. Confirm that each of the reactions listed for plutonium breeding just following Example 2. Calculating Energy from a Kilogram of Fissionable Fuel conserves the total number of nucleons, the total charge, and electron family number.

5. Breeding plutonium produces energy even before any plutonium is fissioned. (The primary purpose of the four nuclear reactors at Chernobyl was breeding plutonium for weapons. Electrical power was a by-product used by the civilian population.) Calculate the energy produced in each of the reactions listed for plutonium breeding just following Example 2. Calculating Energy from a Kilogram of Fissionable Fuel. The pertinent masses are m(²³⁹U) = 239.054289 u, m(²³⁹Np) = 239.052932 u, and m(²³⁹Pu) = 239.052157 u.

6. The naturally occurring radioactive isotope ²³²Th does not make good fission fuel, because it has an even number of neutrons; however, it can be bred into a suitable fuel (much as ²³⁸U is bred into ²³⁹P).

(a) What are Z and N for ²³²Th?

(b) Write the reaction equation for neutron captured by ²³²Th and identify the nuclide ^AX produced in n + ²³²Th → ^AX + γ.

(c) The product nucleus β⁻ Neverending nightmares 3 0 22218 download free. decays, as does its daughter. Write the decay equations for each, and identify the final nucleus.

(d) Confirm that the final nucleus has an odd number of neutrons, making it a better fission fuel.

(e) Look up the half-life of the final nucleus to see if it lives long enough to be a useful fuel.

7. The electrical power output of a large nuclear reactor facility is 900 MW. It has a 35.0% efficiency in converting nuclear power to electrical.

(a) What is the thermal nuclear power output in megawatts? Allavsoft video downloader converter 3 22 1 7331 download free.

Fission 2 5 0 52

(b) How many ²³⁵U nuclei fission each second, assuming the average fission produces 200 MeV?

(c) What mass of ²³⁵U is fissioned in one year of full-power operation?

8. A large power reactor that has been in operation for some months is turned off, but residual activity in the core still produces 150 MW of power. If the average energy per decay of the fission products is 1.00 MeV, what is the core activity in curies?

Glossary

breeder reactors:

reactors that are designed specifically to make plutonium

Fission 2 5 0 5 Equation

breeding:

reaction process that produces ²³⁹Pu

criticality:

condition in which a chain reaction easily becomes self-sustaining

Fission 2 5 0 5 X 4

critical mass:

minimum amount necessary for self-sustained fission of a given nuclide

fission fragments:

a daughter nuclei

liquid drop model:

a model of nucleus (only to understand some of its features) in which nucleons in a nucleus act like atoms in a drop

nuclear fission:

reaction in which a nucleus splits

neutron-induced fission:

fission that is initiated after the absorption of neutron

supercriticality:

an exponential increase in fissions

Selected Solutions to Problems & Exercises

1. (a) 177.1 MeV (b) Because the gain of an external neutron yields about 6 MeV, which is the average BE/A for heavy nuclei. (c) A = 1 + 238 = 96 + 140 + 1 + 1 + 1, Z = 92 = 38 + 53, efn = 0 = 0

3. (a) 180.6 MeV (b) A = 1 + 239 = 96 + 140 + 1 + 1 + 1 + 1, Z = 94 = 38 + 56, efn = 0 = 0

5. ²³⁸U + n → ²³⁹U + γ 4.81 MeV

²³⁹U → ²³⁹Np + β⁻ + v_e 0.753 MeV

²³⁹Np → ²³⁹Pu + β⁻ + v_e 0.211 MeV

7. (a) 2.57 × 10³ MW (b) 8.03 × 10¹⁹ fission/s (c) 991 kg