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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 32.4. The pertinent masses are \(m\left( {{\rm{ }}239{\rm{ U}}} \right){\rm{ }} = {\rm{ }}239.054289{\rm{ u }},{\rm{ }}m\left( {{\rm{ }}239{\rm{ Np}}} \right){\rm{ }} = {\rm{ }}239.052932{\rm{ u }},{\rm{ and }}m\left( {{\rm{ }}239{\rm{ Pu}}} \right){\rm{ }} = {\rm{ }}239.052157{\rm{ u}}\)

Short Answer

Expert verified

The energy produced in each of the reaction listed for plutonium breeding is:

(a)\(E = 4.78\,{\rm{MeV}}\)

(b)\(E = 1.26\,{\rm{MeV}}\)

(c)\(E = 0.722\,{\rm{MeV}}\)

Step by step solution

01

Definition of breeding plutonium

Amount of plutonium produced to the amount of uranium-235 needed this process is called plutonium breeding.

02

Calculate the energy produce in each of the reaction

In this problem, we will calculate the energy released in the plutonium breeding cycle:

\(^{238}{\rm{U}} + n{ \to ^{239}}{\rm{U}} + \gamma \)

We are to find the energy released in this neutron-induced reaction. The energy release is happening due to the different total mass of nuclei before and after the nuclear reaction. Energy difference can be calculated by the free mass-energy formula:

\(E = \Delta m{c^2}\)

To get these mass differences we take parent nuclei and subtract from them daughter nuclei and masses of all other byproducts of the nuclear reaction. Since all atomic masses will be expressed with the unified atomic unit we should remember how to convert it to\({\rm{eV}}\):

\(lu = \frac{{931.5\,{\rm{MeV}}}}{{{c^2}}}\)

03

Finding the mass

To find the mass difference we subtract the atomic masses of parent and daughter nuclei. Trough Appendix A we can find the needed atomic masses:

\(\begin{array}{c}{\rm{Neutron }} = 1.008665\,{\rm{u}}\\^{238}{\rm{U}} = 238.05078\,{\rm{u}}\\^{239}{\rm{U}} = 239.054289\,{\rm{u}}\end{array}\)

So our expression for the mass difference will be:

\(\Delta m = m(n) + m\left( {^{238}{\rm{U}}} \right) - m\left( {^{238}{\rm{U}}} \right)\)

Putting in all of the numbers we got:

\(\begin{array}{l}\Delta m = 1.008645\,{\rm{u}} + 238.05078\,{\rm{u}} - 239.054289\,{\rm{u}}\\\Delta m = 0.005136{\rm{u}}\end{array}\)

From the mass-energy equivalence relation we have:

\(E = \Delta m{c^2} = \left( {0.005136 \times \frac{{931.5\,{\rm{MeV}}}}{{{c^2}}}} \right)\left( {{c^2}} \right)\)

And we get the result of:

\(E = \Delta m{c^2} = 4.78\,{\rm{MeV}}\)

For the second reaction we have\(\beta \)decay of uranium:

\(^{239}{\rm{U}}{ \to ^{239}}\;{\rm{Np}} + {\beta ^ - } + {v_e}\)

We just subtract the mass of neptunium from the mass of the uranium:

\(\Delta m = m(n) + m\left( {^{238}{\rm{U}}} \right) - m\left( {^{239}\;{\rm{Np}}} \right)\)

From the Appendix we can find the masses, so when we put in the numbers we got:

\(\Delta m = m(n) + m\left( {^{238}{\rm{U}}} \right) - m\left( {^{239}\;{\rm{Np}}} \right)\)

Which gives the result of:

\(\Delta m = 0.001357\,{\rm{u}}\)

To get the energy we follow the same procedure as for the first reaction:

\(E = \Delta m{c^2} = \left( {0.001357 \times \frac{{931.5\,{\rm{MeV}}}}{{{c^2}}}} \right) \times {c^2}\)

And we get the result of:

\(E = \Delta m{c^2} = 1.26\,{\rm{MeV}}\)

For the last reaction were plutonium is made we have:

\(^{239}\;{\rm{Np}}{ \to ^{239}}{\rm{Pu}} + {\beta ^ - } + {v_e}\)

For the mass difference we got:

\(\Delta m = m\left( {^{239}{\rm{Np}}} \right) - m\left( {^{239}{\rm{Pu}}} \right)\)

Putting in the numbers we have:

\(\Delta m = 239.052932\,{\rm{u}} - 239.052157\,{\rm{u}}\)

Which gives the result of:

\(\Delta m = 0.000775\,{\rm{u}}\)

To get the energy we follow the same procedure as for the first reaction:

\(E = \Delta m{c^2} = \left( {0.000775 \times \frac{{931.5\,{\rm{MeV}}}}{{{c^2}}}} \right)\left( {{c^2}} \right)\)

And we get the result of:

\(E = \Delta m{c^2} = 0.722\,{\rm{MeV}}\)

(a)\(E = 4.78\,{\rm{MeV}}\)

(b)\(E = 1.26\,{\rm{MeV}}\)

(c) \(E = 0.722\,{\rm{MeV}}\)

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Most popular questions from this chapter

Are some types of cancer more sensitive to radiation than others? If so, what makes them more sensitive?

(a) Estimate the years that the deuterium fuel in the oceans could supply the energy needs of the world. Assume world energy consumption to be ten times that of the United States which is \(8 \times {10^9}J/y\) and that the deuterium in the oceans could be converted to energy with an efficiency of \(32\% \). You must estimate or look up the amount of water in the oceans and take the deuterium content to be \(0.015\% \) of natural hydrogen to find the mass of deuterium available. Note that approximate energy yield of deuterium is \(3.37 \times {10^{14}}J/kg\).

(b) Comment on how much time this is by any human measure. (It is not an unreasonable result, only an impressive one.)

How many kilograms of water are needed to obtain the \(198.8{\rm{ }}mol\) of deuterium, assuming that deuterium is \(0.01500\% \) (by number) of natural hydrogen?

The naturally occurring radioactive isotope \(^{{\rm{232}}}{\rm{Th}}\) 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 \(^{{\rm{238}}}{\rm{U}}\) is bred into\(^{239}P\)).

(a) What are Z and N for\(^{{\rm{232}}}{\rm{Th}}\)?

(b) Write the reaction equation for neutron captured by \(^{{\rm{232}}}{\rm{Th}}\) and identify the nuclide \(^AX\)produced in\(n{ + ^{232}}Th{ \to ^A}X + \gamma \).

(c) The product nucleus \({\beta ^ - }\)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.

(a) Calculate the energy released in the neutron-induced fission (similar to the spontaneous fission in Example\(32.3\)) \(n{ + ^{238}}U{ \to ^{96}}Sr{ + ^{140}}Xe + 3n\), given \(m{(^{96}}Sr) = 95.921750{\rm{ }}u\) and \(m{(^{140}}Xe) = 139.92164{\rm{ }}u\).

(b) This result is about \(6{\rm{ }}MeV\) greater than the result for spontaneous fission. Why?

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

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