Introduction to Fission Physics Notes | EduRev

Modern Physics for IIT JAM

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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 . 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.
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.


Introduction to Fission Physics Notes | EduRev


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.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 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 αβ, or γ decay.


Calculating Energy Released by Fission
Q.1 Calculate the energy released in the following spontaneous fission reaction:Introduction to Fission Physics Notes | EduRev
given the atomic masses to be Introduction to Fission Physics Notes | EduRev,
Introduction to Fission Physics Notes | EduRev,
Introduction to Fission Physics Notes | EduRev, andIntroduction to Fission Physics Notes | EduRev.

Strategy:
As always, the energy released is equal to the mass destroyed times Introduction to Fission Physics Notes | EduRev, so we must find the difference in mass between the parent Introduction to Fission Physics Notes | EduRevand the fission products.

Solution:

The products have a total mass of
Introduction to Fission Physics Notes | EduRev
The mass lost is the mass of Introduction to Fission Physics Notes | EduRevminus Introduction to Fission Physics Notes | EduRev, or

Introduction to Fission Physics Notes | EduRev

so the energy released is

Introduction to Fission Physics Notes | EduRev
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 Introduction to Fission Physics Notes | EduRev, 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 [link]. 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
Introduction to Fission Physics Notes | EduRev
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 ---> FF+ FF+ xn ,
An example of a typical neutron-induced fission reaction is
Introduction to Fission Physics Notes | EduRev
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.
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.

Introduction to Fission Physics Notes | EduRev

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.

Introduction to Fission Physics Notes | EduRev

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 Introduction to Fission Physics Notes | EduRev.
Additionally, some nuclides are easier to make fission than others. In particular, 235U and 239Pu are easier to fission than the much more abundant 238Pu.
Both factors affect critical mass, which is smallest for 238Pu.
The reason Introduction to Fission Physics Notes | EduRevand 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 Introduction to Fission Physics Notes | EduRevhas 143 neutrons, and Introduction to Fission Physics Notes | EduRevhas 145 neutrons, whereas Introduction to Fission Physics Notes | EduRev 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 Introduction to Fission Physics Notes | EduRevare superior fission fuels. The isotope Introduction to Fission Physics Notes | EduRevis 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 Introduction to Fission Physics Notes | EduRevat some expense. This is called enrichment. The most common separation method is gaseous diffusion of uranium hexafluoride (UF6) through membranes. Since Introduction to Fission Physics Notes | EduRevhas 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. A schematic of a reactor design, called the pressurized water reactor.
A pressurized water reactor is cleverly designed to control the fission of large amounts of Introduction to Fission Physics Notes | EduRev, 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.

Introduction to Fission Physics Notes | EduRev

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 Introduction to Fission Physics Notes | EduRev, 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.
Q.1 Calculating Energy from a Kilogram of Fissionable Fuel
Q.2 Calculate the amount of energy produced by the fission of 1.00 kg of Introduction to Fission Physics Notes | EduRev, given the average fission reaction of Introduction to Fission Physics Notes | EduRevproduces 200 MeV.
Strategy:
The total energy produced is the number of Introduction to Fission Physics Notes | EduRevatoms times the given energy per Introduction to Fission Physics Notes | EduRevfission. We should therefore find the number of Introduction to Fission Physics Notes | EduRevatoms in 1.00 kg.
Solution:
The number of Introduction to Fission Physics Notes | EduRevatoms in 1.00 kg is Avogadro’s number times the number of moles. One mole of Introduction to Fission Physics Notes | EduRevhas a mass of 235.04 g; thus, there are Introduction to Fission Physics Notes | EduRev. The number of Introduction to Fission Physics Notes | EduRevatoms is therefore,
Introduction to Fission Physics Notes | EduRev
So the total energy released is
Introduction to Fission Physics Notes | EduRev
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 [link]. 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 Introduction to Fission Physics Notes | EduRevis readily usable.
One nuclide already mentioned is Introduction to Fission Physics Notes | EduRev, which has a 24,120-y half-life and does not exist in nature. Plutonium-239 is manufactured from Introduction to Fission Physics Notes | EduRevin 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 Introduction to Fission Physics Notes | EduRev. Breeding begins with neutron capture by Introduction to Fission Physics Notes | EduRev:
Introduction to Fission Physics Notes | EduRev
Uranium-239 then Introduction to Fission Physics Notes | EduRev decays:
Introduction to Fission Physics Notes | EduRev
Neptunium-239 also Introduction to Fission Physics Notes | EduRev decays:
Introduction to Fission Physics Notes | EduRev
Plutonium-239 builds up in reactor fuel at a rate that depends on the probability of neutron capture by Introduction to Fission Physics Notes | EduRev(all reactor fuel contains more Introduction to Fission Physics Notes | EduRevthan Introduction to Fission Physics Notes | EduRev). 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 Introduction to Fission Physics Notes | EduRevas 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 Introduction to Fission Physics Notes | EduRevhas a particularly small critical mass, an advantage for nuclear weapons.

Section Summary
1. Nuclear fission is a reaction in which a nucleus is split.
2. Fission releases energy when heavy nuclei are split into medium-mass nuclei.
3. Self-sustained fission is possible, because neutron-induced fission also produces neutrons that can induce other fissions, Introduction to Fission Physics Notes | EduRev, where Introduction to Fission Physics Notes | EduRev and Introduction to Fission Physics Notes | EduRev are the two daughter nuclei, or fission fragments, and x is the number of neutrons produced.
4. A minimum mass, called the critical mass, should be present to achieve criticality.
5. More than a critical mass can produce supercriticality.
6. The production of new or different isotopes (especially Introduction to Fission Physics Notes | EduRev) by nuclear transformation is called breeding, and reactors designed for this purpose are called breeder reactors.
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