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Nucle

CBSE · Class 12 · Physics

NCERT Solutions for Nucle — CBSE Class 12 Physics.

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A graph showing the binding energy per nucleon as a function of mass number, highlighting regions of stability, and explaining nuclear fission and fusion processes.
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EXERCISES

13.1Obtain the binding energy (in MeV) of a nitrogen nucleus (147N)\left( \begin{array}{c}14\\ 7\end{array} \mathrm{N}\right), given m(147N)=14.00307um\left( \begin{array}{c}14\\ 7\end{array} \mathrm{N}\right) = 14.00307\mathrm{u}Show solution
For
714N,Z=7, N=7 {}^{14}_{7}\mathrm{N},\quad Z=7,\ N=7
Mass defect:
ΔM=[7mp+7mn]m(714N) \Delta M=[7m_p+7m_n]-m(^{14}_{7}\mathrm N)
Using the given atomic masses, it is easier to use
ΔM=[7mH+7mn]m(714N) \Delta M=[7m_H+7m_n]-m(^{14}_{7}\mathrm N)
because the electron masses cancel.

=7(1.007825)+7(1.008665)14.00307 =7(1.007825)+7(1.008665)-14.00307
=7(2.01649)14.00307=14.1154314.00307=0.11236u =7(2.01649)-14.00307=14.11543-14.00307=0.11236\,\text{u}
Binding energy:
Eb=ΔM×931.5 E_b=\Delta M\times 931.5
=0.11236×931.51.046×102MeV =0.11236\times 931.5\approx 1.046\times 10^2\,\text{MeV}
So the binding energy is about 105 MeV.

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13.2Obtain the binding energy of the nuclei 5626Fe \frac{56}{26}\mathrm{Fe} and 20983Bi \frac{209}{83}\mathrm{Bi} in units of MeV from the following data:Show solution
Use
Eb=[ZmH+(AZ)mnmatom]×931.5MeV E_b=\big[Zm_H+(A-Z)m_n-m_{atom}\big]\times 931.5\,\text{MeV}

### For 2656Fe^{56}_{26}\mathrm{Fe}
Z=26, AZ=30 Z=26,\ A-Z=30
ΔM=26(1.007825)+30(1.008665)55.934939 \Delta M=26(1.007825)+30(1.008665)-55.934939
=26.20345+30.2599555.934939=0.528461u =26.20345+30.25995-55.934939=0.528461\,\text{u}
Eb=0.528461×931.5492MeV E_b=0.528461\times 931.5\approx 492\,\text{MeV}

### For 83209Bi^{209}_{83}\mathrm{Bi}
Z=83, AZ=126 Z=83,\ A-Z=126
ΔM=83(1.007825)+126(1.008665)208.980388 \Delta M=83(1.007825)+126(1.008665)-208.980388
=83.649475+127.09059208.980388=1.759677u =83.649475+127.09059-208.980388=1.759677\,\text{u}
Eb=1.759677×931.51639MeV E_b=1.759677\times 931.5\approx 1639\,\text{MeV}
So the binding energies are approximately 492 MeV and 1.64\times 10^3 MeV.

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13.3A given coin has a mass of 3.0g3.0\mathrm{g}. Calculate the nuclear energy that would be required to separate all the neutrons and protons from each other. For simplicity assume that the coin is entirely made of 2963Cu^{63}_{29}\mathrm{Cu} atoms (of mass 62.92960 u).Show solution
For 2963Cu^{63}_{29}\mathrm{Cu}, mass number A=63A=63. The book gives the approximate nuclear binding energy per nucleon in this region as about 8 MeV.

Energy required for one nucleus:
E63×8=504MeV E \approx 63\times 8=504\,\text{MeV}

Number of atoms in 3.0 g of copper:
moles=3.063=0.04762mol \text{moles} = \frac{3.0}{63}=0.04762\,\text{mol}
N=0.04762×6.023×10232.87×1022 N = 0.04762\times 6.023\times 10^{23} \approx 2.87\times 10^{22}

Total energy:
Etot=2.87×1022×504MeV1.45×1025MeV E_{tot}=2.87\times 10^{22}\times 504\,\text{MeV} \approx 1.45\times 10^{25}\,\text{MeV}
Convert to joules using 1MeV=1.6×1013J1\,\text{MeV}=1.6\times 10^{-13}\,\text{J}:
Etot=1.45×1025×1.6×10132.3×1012J E_{tot}=1.45\times 10^{25}\times 1.6\times 10^{-13} \approx 2.3\times 10^{12}\,\text{J}
So the required nuclear energy is of order **101210^{12} J; more precisely about 2.3×10122.3\times 10^{12} J**.

If one uses the textbook-style approximate binding energy per nucleon more crudely, the answer is still in the same order, 101210^{12}101310^{13} J. The calculated value above is the best estimate from the given chapter data and standard nuclear binding-energy reasoning.

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13.4Obtain approximately the ratio of the nuclear radii of the gold isotope 19779Au \frac{197}{79}\mathrm{Au} and the silver isotope 10747Ag \frac{107}{47}\mathrm{Ag} .Show solution
Nuclear radius varies as
R=R0A1/3 R=R_0A^{1/3}
So the ratio of radii is
RAuRAg=(197107)1/3 \frac{R_{Au}}{R_{Ag}}=\left(\frac{197}{107}\right)^{1/3}
1971071.84 \frac{197}{107}\approx 1.84
1.841/31.21 1.84^{1/3}\approx 1.21
Therefore, the radius of gold nucleus is about 1.21 times that of silver nucleus.

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13.5The QQ value of a nuclear reaction A+bC+dA + b\rightarrow C + d is defined byShow solution
The chapter states that the Q-value of a nuclear process is the difference between the initial and final rest masses multiplied by c2c^2:
Q=[mA+mbmCmd]c2 Q = [m_A+m_b-m_C-m_d]c^2
It is also equal to the difference between final and initial kinetic energies:
Q=final kinetic energyinitial kinetic energy Q = \text{final kinetic energy} - \text{initial kinetic energy}
If Q>0Q>0, the reaction is exothermic; if Q<0Q<0, it is endothermic.

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13.6Suppose, we think of fission of a 2656Fe^{56}_{26}\mathrm{Fe} nucleus into two equal fragments, 1328Al^{28}_{13}\mathrm{Al}. Is the fission energetically possible? Argue by working out QQ of the process. Given m(5626Fe)=55.93494um\left(\frac{56}{26}\mathrm{Fe}\right) = 55.93494 \mathrm{u} and m(2813Al)=27.98191um\left(\frac{28}{13}\mathrm{Al}\right) = 27.98191 \mathrm{u}.
13.7The fission properties of 94239Pu^{239}_{94}\text{Pu} are very similar to those of 92235U^{235}_{92}\text{U}. The average energy released per fission is 180 MeV. How much energy, in MeV, is released if all the atoms in 1 kg of pure 94239Pu^{239}_{94}\text{Pu} undergo fission?
13.8How long can an electric lamp of 100W be kept glowing by fusion of 2.0 kg of deuterium? Take the fusion reaction as
13.9Calculate the height of the potential barrier for a head on collision of two deuterons. (Hint: The height of the potential barrier is given by the Coulomb repulsion between the two deuterons when they just touch each other. Assume that they can be taken as hard spheres of radius 2.0 fm.)
13.10From the relation R=R0A1/3R = R_0 A^{1/3}, where R0R_0 is a constant and AA is the mass number of a nucleus, show that the nuclear matter density is nearly constant (i.e. independent of AA).

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Understand the core concepts first, then work through the 93 practice questions available for this chapter. Revise formulas and definitions regularly, and use flashcards for quick recall before the exam.
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