CBSE · NCERT · Class 12 Physics · Chapter 13

NCERT Solutions: Class 12 Physics Chapter 13 - Nuclei

10 textbook Q&A10 verifiedFree Content

Chapter-wise NCERT intext questions and exercise answers for Nuclei, grounded in the official textbook.

Questions are taken verbatim from the NCERT textbook; answers were grounded against the chapter's content during generation. Items needing review are marked.
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Exercises 10
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1Exercises10 questions
Q.13.1Obtain the binding energy (in MeV) of a nitrogen nucleus ( ) 14 7 N , given m ( ) 14 7 N =14.00307 uv
Solution

For atomic masses, use $\Delta m=Zm_H+(A-Z)m_n-M_{\text{atom}}$, since electron masses cancel. For $^{14}_{7}\text{N}$, $Z=7$ and $A-Z=7$. Thus $\Delta m=7(1.007825)+7(1.008665)-14.00307=0.11236\,\text{u}$. Binding energy $E_b=\Delta m(931.5\,\text{MeV})=0.11236(931.5)=104.7\,\text{MeV}$.

Answer:

$1.05\times10^2\,\text{MeV}$, approximately $104.7\,\text{MeV}$.

Q.13.2Obtain the binding energy of the nuclei 56 26Fe and 20983 Bi in units of MeV from the following data: m ( 56 26Fe ) = 55.934939 u m ( 20983 Bi ) = 208.980388 uv
Solution

For $^{56}_{26}\text{Fe}$, $Z=26$ and $N=30$. Thus $\Delta m=26(1.007825)+30(1.008665)-55.934939=0.528461\,\text{u}$, so $E_b=0.528461(931.5)=492\,\text{MeV}$. For $^{209}_{83}\text{Bi}$, $Z=83$ and $N=126$. Thus $\Delta m=83(1.007825)+126(1.008665)-208.980388=1.760877\,\text{u}$, so $E_b=1.760877(931.5)=1.64\times10^3\,\text{MeV}$.

Answer:

$E_b(^{56}_{26}\text{Fe})\approx492\,\text{MeV}$ and $E_b(^{209}_{83}\text{Bi})\approx1.64\times10^3\,\text{MeV}$.

Q.13.3A given coin has a mass of 3.0 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 63 29Cu atoms (of mass 62.92960 u).v
Solution

For $^{63}_{29}\text{Cu}$, $Z=29$ and $N=34$. Its mass defect is $\Delta m=29(1.007825)+34(1.008665)-62.92960=0.591935\,\text{u}$. Binding energy per nucleus is $0.591935(931.5)=551\,\text{MeV}$. The number of copper atoms in $3.0\,\text{g}$ is $(3.0/62.92960)(6.023\times10^{23})=2.87\times10^{22}$. Total energy required is $(2.87\times10^{22})(551)=1.6\times10^{25}\,\text{MeV}=2.5\times10^{12}\,\text{J}$.

Answer:

$1.6\times10^{25}\,\text{MeV}$, or about $2.5\times10^{12}\,\text{J}$.

Q.13.4Obtain approximately the ratio of the nuclear radii of the gold isotope 197 79 Au and the silver isotope 10747 Ag .v
Solution

Nuclear radius follows $R=R_0A^{1/3}$. Therefore $R_{\text{Au}}/R_{\text{Ag}}=(197/107)^{1/3}=1.23$.

Answer:

$R_{\text{Au}}/R_{\text{Ag}}\approx1.23$.

Q.13.5The Q value of a nuclear reaction A + b ® C + d is defined by Q = [ mA + mb – mC – md]c 2 where the masses refer to the respective nuclei. Determine from the given data the Q-value of the following reactions and state whether the reactions are exothermic or endothermic. (i) 1 3 2 2 1 1 1 1 H+ H H+ H → (ii) 12 12 20 4 6 6 10 2 C+ C Ne+ He → Atomic masses are given to be m ( 2 1 H ) = 2.014102 u m ( 3 1 H ) = 3.016049 u m ( 12 6 C ) = 12.000000 u m ( 20 10 Ne ) = 19.992439 uv
Solution

For (i), using atomic masses, $Q=[m(^1\text{H})+m(^3\text{H})-2m(^2\text{H})]c^2=[1.007825+3.016049-2(2.014102)](931.5)=-4.03\,\text{MeV}$, so the reaction is endothermic. For (ii), $Q=[2m(^{12}\text{C})-m(^{20}\text{Ne})-m(^4\text{He})]c^2=[24.000000-19.992439-4.002603](931.5)=+4.62\,\text{MeV}$, so the reaction is exothermic.

Answer:

(i) $Q=-4.03\,\text{MeV}$, endothermic. (ii) $Q=+4.62\,\text{MeV}$, exothermic.

Q.13.6Suppose, we think of fission of a 56 26Fe nucleus into two equal fragments, 28 13 Al . Is the fission energetically possible? Argue by working out Q of the process. Given m ( 56 26Fe ) = 55.93494 u and m ( 28 13 Al ) = 27.98191 u.v
Solution

For $^{56}_{26}\text{Fe}\to2\,^{28}_{13}\text{Al}$, $Q=[m(^{56}\text{Fe})-2m(^{28}\text{Al})]c^2=[55.93494-2(27.98191)](931.5)=-26.9\,\text{MeV}$. The negative Q-value means the fission is endothermic and is not energetically possible without external energy.

Answer:

No. $Q=-26.9\,\text{MeV}$, so energy must be supplied.

Q.13.7The fission properties of 239 94 Pu are very similar to those of 23592 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 239 94 Pu undergo fission?v
Solution

The number of atoms in $1\,\text{kg}$ of pure $^{239}\text{Pu}$ is $N=(1000/239)(6.023\times10^{23})=2.52\times10^{24}$. With $180\,\text{MeV}$ released per fission, the total energy is $E=N(180)=4.5\times10^{26}\,\text{MeV}$.

Answer:

$4.5\times10^{26}\,\text{MeV}$.

Q.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 2 2 3 1 1 2 H+ H He+n+3.27 MeV →v
Solution

Each fusion reaction consumes two deuterium nuclei and releases $3.27\,\text{MeV}$. In $2.0\,\text{kg}$ of deuterium, the number of deuterium atoms is approximately $(2000/2)(6.023\times10^{23})=6.02\times10^{26}$. Thus the number of reactions is $3.01\times10^{26}$. The energy released is $(3.01\times10^{26})(3.27)=9.85\times10^{26}\,\text{MeV}=1.58\times10^{14}\,\text{J}$. A $100\,\text{W}$ lamp uses $100\,\text{J s}^{-1}$, so the time is $1.58\times10^{14}/100=1.58\times10^{12}\,\text{s}$, about $5.0\times10^4$ years.

Answer:

About $1.6\times10^{12}\,\text{s}$, or $5.0\times10^4$ years.

Q.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.)v
Solution

Each deuteron has charge $+e$. When two deuterons of radius $2.0\,\text{fm}$ just touch, their centre-to-centre separation is $r=4.0\,\text{fm}=4.0\times10^{-15}\,\text{m}$. The Coulomb potential energy is $U=(1/4\pi\epsilon_0)e^2/r=9.0\times10^9(1.6\times10^{-19})^2/(4.0\times10^{-15})=5.8\times10^{-14}\,\text{J}$. In MeV, this is $(5.8\times10^{-14})/(1.6\times10^{-13})=0.36\,\text{MeV}$.

Answer:

$5.8\times10^{-14}\,\text{J}$, or about $0.36\,\text{MeV}$.

Q.13.10From the relation R = R0A 1/3, where R0 is a constant and A is the mass number of a nucleus, show that the nuclear matter density is nearly constant (i.e. independent of A).v
Solution

The nuclear radius is $R=R_0A^{1/3}$, so the nuclear volume is $V=\frac43\pi R^3=\frac43\pi R_0^3A$. The nuclear mass is approximately $M=Am_N$, where $m_N$ is the average nucleon mass. Therefore $\rho=M/V=Am_N/(\frac43\pi R_0^3A)=3m_N/(4\pi R_0^3)$, which contains no $A$. Hence nuclear matter density is nearly constant for all nuclei.

Answer:

Since nuclear mass is proportional to $A$ and nuclear volume is also proportional to $A$, nuclear density is independent of $A$.