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

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

This problem gives some idea of the magnitude of the energy yield of a small tactical bomb. Assume that half the energy of a 1.00 - kT nuclear depth charge set off under an aircraft carrier goes into lifting it out of the water—that is, into gravitational potential energy. How high is the carrier lifted if its mass is 90,000 tons?

The energy produced by the fusion of a \(1.00 - kg\) mixture of deuterium and tritium was found in Example Calculating Energy and Power from Fusion. Approximately how many kilograms would be required to supply the annual energy use in the United States?

Calculate the energy output in each of the fusion reactions in the proton-proton cycle, and verify the values given in the above summary.

(a) Calculate the energy released in the neutron-induced fission reaction\(n{ + ^{239}}Pu{ \to ^{96}}Sr{ + ^{140}}Ba + 4n\), given \(m{(^{96}}Sr) = 95.921750{\rm{ }}u\)

And

\(m{(^{140}}Ba) = 139.910581{\rm{ }}u\).

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

Another set of reactions that result in the fusing of hydrogen into helium in the Sun and especially in hotter stars is called the carbon cycle. It is

\(\begin{array}{*{20}{l}}{^{12}C{ + ^1}H}&{{ \to ^{13}}N + \gamma ,}\\{^{13}N}&{{ \to ^{13}}C + {e^ + } + {v_e},}\\{^{13}C{ + ^1}H}&{{ \to ^{14}}N + \gamma ,}\\{^{14}N{ + ^1}H}&{{ \to ^{15}}O + \gamma ,}\\{^{15}O}&{{ \to ^{15}}N + {e^ + } + {v_e},}\\{^{15}N{ + ^1}H}&{{ \to ^{12}}C{ + ^4}He.}\end{array}\)

Write down the overall effect of the carbon cycle (as was done for the proton-proton cycle in \(2{e^ - } + {4^1}H{ \to ^4}He + 2{v_e} + 6\gamma \)). Note the number of protons (\(^1H\)) required and assume that the positrons (\({e^ + }\)) annihilate electrons to form more \(\gamma \) rays.

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free