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(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.

Short Answer

Expert verified

(a) The energy released in the reaction\(n{ + ^{239}}Pu{ \to ^{96}}Sr{ + ^{140}}Ba + 4n\)is\(E = 180.55MeV\).

(b) It is confirmed that the total number of nucleons and total charge are conserved in \(n{ + ^{239}}Pu{ \to ^{96}}Sr{ + ^{140}}Ba + 4n\) reaction.

Step by step solution

01

Concept Introduction

The power kept in the centre of an atom is known as nuclear energy. All stuff in the cosmos is made up of tiny particles called atoms. The centre of an atom's nucleus is typically where most of its mass is concentrated. Neutrons and protons are the two subatomic particles that make up the nucleus. Atomic bonds that hold them together carry a lot of energy.

02

Energy calculation

The energy release is happening due to the different total mass of nuclei before and after the nuclear reaction. Energydifference can be calculated by the free mass-energy formula –

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

To get these mass differences take parent nuclei and subtract from them daughter nuclei and masses of all otherby-products of the nuclear reaction. Since all atomic masses will be expressed with the unified atomic unit, remember how to convert it to \(eV\) –

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

Now analyse the reaction –

\(n{ + ^{239}}Pu{ \to ^{96}}Sr{ + ^{140}}Ba + 4n\)

Looking in the Appendix for the atomic masses the following is obtained–

\(\begin{align}{}^{96}Sr & = 95.921750{\rm{ }}u\\^{140}Ba & = 139.910581{\rm{ }}u\\^{239}Pu & = 239.052157{\rm{ }}u\\n & = 1.008665{\rm{ }}u\end{align}\)

Expression for mass difference will be –

\(\Delta m = ({m_n} + m\left( {^{239}Pu} \right) - \{ m\left( {^{96}Sr} \right) + m\left( {^{140}Ba} \right) + 4{m_n})\} \)

Plugging in the values –

\(\begin{align}{}\Delta m & = 1.008665{\rm{ }}u + 239.052157{\rm{ }}u - \{ 95.921750{\rm{ }}u + 139.910581{\rm{ }}u + 4 \times 1.008665{\rm{ }}u\} \\\Delta m & = 0.193831{\rm{ }}u\end{align}\)

So, from the energy relation it is obtained that –

\(\begin{align}{}E & = \Delta m{c^2}\\ & = 0.193831 \times \frac{{931.5MeV}}{{{c^2}}} \times {c^2}\\E & = 180.55MeV\end{align}\)

Therefore, the energy value for the reaction is obtained as \(E = 180.55MeV\).

03

Step 3:Number of nucleons and charge

To check that everything is conserved we carefully analyse nuclear reaction –

\(_0^1{n_1} + { - ^{239}}Pul \to _{38}^{96}Sr + _{56}^{140}56 + 4_0^1{n_1}\)

For the nucleon number, we got: \(1 + 239\) on the left side, and \(96 + 140 + 4\) on the right side, both ofthem gives \(240\), which confirms that it is conserved.

For the charge number neutron have zero charges, so on the left, we got \(94\), and on the right, wehave \(56\) and \(38\), which also gives \(94\), which confirms charge conservation.

Therefore, all the quantities are conserved.

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Most popular questions from this chapter

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 \(m\left( {{\rm{ }}239{\rm{ U}}} \right){\rm{ }} = {\rm{ }}239.054289{\rm{ u }},{\rm{ }}m\left( {{\rm{ }}239{\rm{ Np}}} \right){\rm{ }} = {\rm{ }}239.052932{\rm{ u }},{\rm{ and }}m\left( {{\rm{ }}239{\rm{ Pu}}} \right){\rm{ }} = {\rm{ }}239.052157{\rm{ u}}\)

The power output of the Sun is \(4 \times {10^{26}}{\rm{ }}W\).

(a) If \(90\% \) of this is supplied by the proton-proton cycle, how many protons are consumed per second?

(b) How many neutrinos per second should there be per square meter at the Earth from this process? This huge number is indicative of how rarely a neutrino interacts, since large detectors observe very few per day.

(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.

(a) Calculate the number of grams of deuterium in a \(80,000 - L\) swimming pool, given deuterium is \(0.0150\% \) of natural hydrogen.

(b) Find the energy released in joules if this deuterium is fused via the reaction\(^2H{ + ^2}H{ \to ^3}He + n\).

(c) Could the neutrons be used to create more energy?

(d) Discuss the amount of this type of energy in a swimming pool as compared to that in, say, a gallon of gasoline, also taking into consideration that water is far more abundant.

(a) Neutron activation of sodium, which is \({\rm{100\% }}\,{\,^{{\rm{23}}}}{\rm{Na}}\), produces\(^{{\rm{24}}}{\rm{Na}}\), which is used in some heart scans, as seen in Table 32.1. The equation for the reaction is \(^{23}Na + n{ \to ^{24}}Na + \gamma \). Find its energy output, given the mass of \(^{{\rm{24}}}{\rm{Na}}\) is \(23.990962\,u\).

(b) What mass of \(^{{\rm{24}}}{\rm{Na}}\) produces the needed \(5.0\)-mCi activity, given its half-life is \(15.0\,\;h\) ?

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