CBSE 12th Standard Physics Subject Nuclei Chapter Case Study Questions With Solution 2021
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CBSE 12th Standard Physics Subject Nuclei Case Study Questions With Solution 2021
12th Standard CBSE
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Reg.No. :
Physics
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In the year 1939, German scientist Otto Hahn and Strassmann discovered that when an uranium isotope was bombarded with a neutron, it breaks into two intermediate mass fragments. It was observed that, the sum of the masses of new fragments formed were less than the mass of the original nuclei. This difference in the mass appeared as the energy released in the process. Thus, the phenomenon of splitting of a heavy nucleus (usually A> 230) into two or more lighter nuclei by the bombardment of proton, neutron, a-particle, etc with liberation of energy is called nuclear fission.
\({ }_{92} \mathrm{U}^{235}+{ }_{0} n^{1} \rightarrow \quad{ }_{92} \mathrm{U}^{236} \rightarrow{ }_{56} \mathrm{Ba}^{144}+{ }_{36} \mathrm{Kr}^{89}+3{ }_{0} n^{1}+Q\)
Unstable nucleus
(i) Nuclear fission can be explained on the basis of(a) Millikan's oil drop method (b) Liquid. drop model (c) Shell model (d) Bohr's model (ii) For sustaining the nuclear fission chain reaction in a sample (of small size) \({ }_{92}^{235} \mathrm{U}\), it is desirable to slow down fast neutrons by
(a) friction (b) elastic damping/scattering (c) absorption (d) none of these (iii) Which of the following is/are fission reaction(s)?
\(\text {(I) }{ }_{0}^{1} n+{ }_{92}^{235} \mathrm{U} \rightarrow{ }_{92}^{236} \mathrm{U} \rightarrow{ }_{51}^{133} \mathrm{Sb}+{ }_{41}^{99} \mathrm{Nb}+4_{0}^{1} n\)
\(\text {(II) }{ }_{0}^{1} n+{ }_{92}^{235} \mathrm{U} \rightarrow{ }_{54}^{1.40} \mathrm{Xe}+{ }_{38}^{94} \mathrm{Sr}+2{ }_{0}^{1} n\)
\((\mathrm{III}){ }_{1}^{2} \mathrm{H}+{ }_{1}^{2} \mathrm{H} \rightarrow{ }_{2}^{3} \mathrm{He}+{ }_{0}^{1} n\)(a) Both II and III (b) Both I and III (c) Only II (d) Both I and II (iv) On an average, the number of neutrons and the energy of a neutron released per fission of a uranium atom are respectively
(a) 2.5 and 2 keV (b) 3 and 1 keV (c) 2.5 and 2 MeV (d) 2 and 2 keV (v) In any fission process, ratio of mass of daughter nucleus to mass of parent nucleus is
(a) less than 1 (b) greater than 1 (c) equal to 1 (d) depends 0 the mass of parent nucleus (a) -
The nucleus was first discovered in 1911 by Lord Rutherford and his associates by experiments on scattering of a-particles by atoms. He found that the scattering results could be explained, if atoms consist of a small, central, massive and positive core surrounded by orbiting electrons. The experimental results indicated that the size of the nucleus is of the order of 10-14m and is thus 10000 times smaller than the size of atom.
(i) Ratio of mass of nucleus with mass of atom is approximately(a) 1 (b) 10 (c) 103 (d) 1010 (ii) Masses of nuclei of hydrogen, deuterium and tritium are in ratio
(a) 1:2:3 (b) 1:1:1 (c) 1:1:2 (d) 1:2:4 (iii) Nuclides with same neutron number but different atomic number are
(a) isobars (b) isotopes (c) isotones (d) none of these (iv) If R is the radius and A is the mass number, then log R versus log A graph will be
(a) a straight line (b) aparabola (c) anellipse (d) none of these (v) The ratio of the nuclear radii of the gold isotope \({ }_{79}^{197} \mathrm{Au}\) and silver isotope \({ }_{47}^{107} \mathrm{Au}\) is
(a) 1.23 (b) 0.216 (c) 2.13 (d) 3.46 (a) -
A heavy nucleus breaks into comparatively lighter nuclei which are more stable compared to the original heavy nucleus. When a heavy nucleus like uranium is bombarded by slow moving neutrons, it splits into two parts releasing large amount of energy. The typical fission reaction of \({ }_{92} \mathrm{U}^{235}\).
\({ }_{92} \mathrm{U}^{235}+{ }_{0} n^{1} \rightarrow{ }_{56} \mathrm{Ba}^{141}+{ }_{36} \mathrm{Kr}^{92}+3{ }_{0} n^{1}+200 \mathrm{MeV}\)
The fission of 92U235approximately released 200 MeV of energy.
(i) If 200 MeV energy is released in the fission of a single nucleus of \({ }_{92}^{235} \mathrm{U}\),the fissions which are required to produce a power of 1kW is(a) 3.125 x 1013 (b) 1.52 x 106 (c) 3.125 x 1012 (d) 3.125 x 1014 (ii) The release in energy in nuclear fission is consistent with the fact that uranium has
(a) more mass per nucleon than either ofthe two fragments (b) more mass per nucleon as the two fragment (c) exactly the same mass per nucleon as the two fragments (d) less mass per nucleon than either of two fragments. (iii) When 92U235undergoes fission, about 0.1% of the original mass is converted into energy. The energy released when 1 kg of 92U235undergoes fission is
(a) 9 x 1011J (b) 9 x 1013J (c) 9 x 1015J (d) 9 x 1018J (iv) A nuclear fission is said to be critical when multiplication factor or K
(a) K= 1 (b) K> 1 (c) K< 1 (d) K=0 (v) Einstein's mass-energy conversion relation E = mc2 is illustrated by
(a) nuclear fission (b) \(\beta\)-decay (c) rocket propulsion (d) steam engine (a) -
Neutrons and protons are identical particle in the sense that their masses are nearly the same and the force, called nuclear force, does into distinguish them. Nuclear force is the strongest force. Stability of nucleus is determined by the neutron proton ratio or mass defect or packing fraction. Shape of nucleus is calculated by quadrupole moment and spin of nucleus depends on even or odd mass number. Volume of nucleus depends on the mass number. Whole mass of the atom (nearly 99%) is centred at the nucleus.
(i) The correct statements about the nuclear force is/are(a) change independent (b) short range force (c) non-conservative force (d) all of these. (ii) The range of nuclear force is the order of
(a) 2 x 10-10 m (b) 1.5 x 10-20 m (c) 1.2 x 10-4 m (d) 1.4 x 10-15 m (iii) A force between two protons is same as the force between proton and neutron. The nature of the force is
(a) electrical force (b) weak nuclear force (c) gravitational force (d) strong nuclear force. (iv) Two protons are kept at a separation of 40 \(\dot A\). Fn is the nuclear force and Fe is the electrostatic force between them. Then
(a) Fn << Fe (b) Fn = Fe (c) Fn >> Fe (d) Fn \(\approx \) Fe (v) All the nucleons in an atom are held by
(a) nuclear forces (b) van der Waal's forces (c) tensor forces (d) coulomb forces (a) -
The density of nuclear matter is the ratio of the mass of a nucleus to its volume. As the volume of a nucleus is directly proportional to its mass number A, so the density of nuclear matter is independent of the size of the nucleus. Thus, the nuclear matter behaves like a liquid of constant density. Different nuclei are like drops of this liquid, of different sizes but of same density.
Let A be the mass number and R be the radius of a nucleus. If m is the average mass of a nucleon, then
Mass of nucleus = mA
\(\text { Volume of nucleus }=\frac{4}{3} \pi R^{3}=\frac{4}{3} \pi\left(R_{0} A^{1 / 3}\right)^{3}=\frac{4}{3} \pi R_{0}^{3} A\)
\(\text { Nuclear density, } \rho_{\mathrm{nu}}=\frac{\text { Mass of nucleus }}{\text { Volume of nucleus }} \text { or } \rho_{\mathrm{nu}}=\frac{m A}{\frac{4}{3} \pi R_{0}^{3} A}=\frac{3 m}{4 \pi R_{0}^{3}}\)
Clearly, nuclear density is independent of mass number A or the size of the nucleus. The nuclear mass density is of the order 1017 kg m-3. This density is very large as compared to the density of ordinary matter, say water, for which p = 1.0 x 103 kg m-3.
(i) The nuclear radius of \({ }_{8}^{16} \mathrm{O}\) is 3 X 10-15 m. The density of nuclear matter is(a) 2.9 x 1034 kg m-3 (b) 1.2 x 1017kg m-3 (c) 16 x 1027kg m-3 (d) 2.4 x 1017kg m-3 (ii) What is the density of hydrogen nucleus in SI units? Given Ro = 1.1 fermi and mp = 1.007825 amu
(a) 2.98 x 1017kg m-3 (b) 3.0 x 1034 kg m-3 (c) 1.99 x 1011 kg m-3 (d) 7.85 x 1017kg m-3 (iii) Density of a nucleus is
(a) more for lighter elements and less for heavier elements. (b) more for heavier elements and less for lighter elements (c) very less compared to ordinary matter (d) a constant (iv) The nuclear mass of \({ }_{26}^{56} \mathrm{Fe}\) is 55.85 amu. The its nuclear density is
(a) 5.0 x 1019kg m-3. (b) 1.5 x 1019kg m-3 (c) 2.9 x 1017kg m-3 (d) 9.2 x 1026kg m-3 (v) If the nucleus of \({ }_{13}^{27} \mathrm{Al}\) has a nuclear radius of about 3.6 fm, then \({ }_{52}^{125} \mathrm{Te}\) would have its radius approximately as
(a) 9.6 fm (b) 12 fm (c) 4.8 fm (d) 6 fm (a) -
When subatomic particles undergo reactions, energy is conserved, but mass is not necessarily conserved.However, a particle's mass "contributes" to its total energy, in accordance with Einstein's famous equation, E = mc2, In this equation, E denotes the energy carried by a particle because of its mass. The particle can also have additional energy due to its motion and its interactions with other particles. Consider a neutron at rest and well separated from other particles. It decays into a proton, an electron and an undetected third particle as given here: Neutron \(\rightarrow\) proton + electron + ???
The given table summarizes some data from a single neutron decay. Electron volt is a unit of energy. Column 2 shows the rest mass of the particle times the speed of light squared.Particle Mass x c2 (Me V) Kinetic energy (MeV) Neutron 940.97 0.00 Proton 939.67 0.01 Electron 0.51 0.39 (i) From the given table, which properties of the undetected third particle can be calculate?
(a) Total energy, but not kinetic energy (b) Kinetic energy, but not total energy (c) Both total energy and kinetic energy (d) Neither total energy nor kinetic energy (ii) Assuming the table contains no major errors, what can we conclude about the (mass x c2) of the undetected third particle?
(a) It is 0.79 MeV (b) It is 0.39 MeV (c) It is less than or equal to 0.79 MeV; but we cannot be more precise. (d) It is less than or equal to 0.40 MeV; but we cannot be more precise. (iii) Could this reaction occur?
Proton \(\rightarrow\) neutron + other particles(a) Yes, if the other particles have much more kinetic energy than mass energy. (b) Yes, but only if the proton has potential energy (due to interactions with other particles). (c) No, because a neutron is more massive than a proton. (d) No, because a proton is positively charged while a neutron is electrically neutral. (iv) How much mass has to be converted into energy to produce electric power of 500 MW for one hour?
(a) 2 x 10-5 kg (b) 1 x 10-5 kg (c) 3 X 10-5 kg (d) 4 x 10-5 kg (v) The equivalent energy of 1 g of substance is
(a) 9 x 1013J (b) 6 x 1012J (c) 3 x 1013J (d) 6 x 1013J (a)
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CBSE 12th Standard Physics Subject Nuclei Case Study Questions With Solution 2021 Answer Keys
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(i) (b)
(ii) (b): Fast neutrons are slowed down by elastic scattering with light nuclei as each collision takes away nearly 50% of energy.
(iii) (d): Reactions I and II represent fission of uranium isotope \({ }_{92}^{235} \mathrm{U}\), when bombarded with neutrons that breaks it into two intermediate mass nuclear fragments. However, reaction III represents two deuterons fuses together to from the light isotope of helium.
(iv) (c): On an average 2.5 neutrons are released per fission of the uranium atom.
The energy of the neutron released per fission of the uranium atom is 2 MeV.
(v) (a): In fission process, when a parent nucleus breaks. into daughter products, the some mass is lost in the form of energy. Thus,mass of fission products < mass of parent nucleus.
\(\Rightarrow \frac{\text { Mass of fission products }}{\text { Mass of parent nucleus }}<1\) -
(i) (a) : As nearly 99.9% mass of atom is in nucleus.
\(\therefore \quad \frac{\text { Mass of nucleus }}{\text { Mass of atom }}=\frac{99.9}{100}=0.99 \approx 1\)
(ii) (a): Since, the nuclei of deuterium and tritium are isotopes of hydrogen, they must contain only one proton each. But the masses of the nuclei of hydrogen, deuterium and tritium are in the ration of 1 : 2 : 3,because of presence of neutral matter in deuterium and tritium nuclei.
(iii) (c)
(iv) (a) : \(R=R_{0} A^{1 / 3}\)
\(\log R=\log R_{0}+\frac{1}{3} \log A\)
On comparing the above equation of straight line; y = mx + c. So, the graph between log A and log R is a straight line also.
(v) (a): Here, A1 = 197 and A2 = 107
\(\therefore \quad \frac{R_{1}}{R_{2}}=\left(\frac{A_{1}}{A_{2}}\right)^{1 / 3}=\left(\frac{197}{107}\right)^{1 / 3}=1.225 \simeq 1.23\) -
(i) (a) : Let the number of fissions per second be n. Energy released per second
\(=n \times 200 \mathrm{MeV}=n \times 200 \times 1.6 \times 10^{-13} \mathrm{~J}\)
Energy required per second = power x time
\(=1 \mathrm{~kW} \times 1 \mathrm{~s}=1000 \mathrm{~J}\)
\(\therefore \quad n \times 200 \times 1.6 \times 10^{-13}=1000\)
\(\text { or } \quad n=\frac{1000}{3.2 \times 10^{-11}}=\frac{10}{3.2} \times 10^{13}=3.125 \times 10^{13}\)
(ii) (a)
(iii) (b): As only 0.1% of the original mass is converted into energy, hence out of 1 kg mass 1 g is converted into energy.
\(\therefore\) Energy released during fission, \(E=\Delta m c^{2}\)
\(=1 \mathrm{~g} \times\left(3 \times 10^{8} \mathrm{~m} \mathrm{~s}^{-1}\right)^{2}=10^{-3} \times 9 \times 10^{16} \mathrm{~J}=9 \times 10^{13} \mathrm{~J}\)
(iv) (a)
(v) (a) -
(i) (d) : All options are basic properties of nuclear forces. So, all options are correct.
(ii) (d) : The nuclear force is of short range and the range of nuclear force is the order of 1.4 x 10-15 m
Now, volume \(\propto R^{3} \propto A\)
(iii) (d)
(iv) (a) : Nuclear force is much stronger than the electrostatic force inside the nucleus i.e., at distances of the order of fermi. At 40 \(\dot A\), nuclear force is ineffective and only electrostatic force of repulsion is present.This is very high at this distance because nuclear force is not acting now and the gravitational force is very feeble.Fnuclear<< Felectrostatiinc this case.
(v) (a). -
(i) (d) : Here R = 3 X 10-15 m
Nuclear mass = 16 amu = 16 x 1.66 x 10-27 kg
\(\rho_{\mathrm{nu}}=\frac{\text { Nuclear mass }}{\text { Nuclear volume }}=\frac{16 \times 1.66 \times 10^{-27}}{\frac{4}{3} \pi\left(3 \times 10^{-15}\right)^{3}}\)
\(=2.359 \times 10^{17} \mathrm{~kg} \mathrm{~m}^{-3} \simeq 2.4 \times 10^{17} \mathrm{~kg} \mathrm{~m}^{-3}\)
(ii) (a): Density,
\(\rho=\frac{3 m_{p}}{4 \pi R_{0}^{3}}=\frac{3 \times 1.007825 \times 1.66 \times 10^{-27}}{4 \times \frac{22}{7} \times\left(1.1 \times 10^{-15}\right)^{3}}\)
\(=2.98 \times 10^{17} \mathrm{~kg} \mathrm{~m}^{-3}\)
(iii) (d) : \(\text { Density }=\frac{\text { Mass }}{\text { Volume }}=\frac{A m_{p}}{\frac{4}{3} \pi\left(R_{o} A^{1 / 3}\right)}\)
\(=\frac{m_{p}}{\frac{4}{3} \pi R_{0}^{3}}\)
\(\text { where } m_{P}=1.6 \times 10^{-27} \mathrm{~kg}^{3}\)
\(=2.3 \times 10^{17} \mathrm{~kg} \mathrm{~m}^{-3} \text {, which is a constant }\)
(iv) (c): Given, mass of mFe = 55.85 amu
= 55.85 x 1.66 x 10-27 kg = 9.27 x 10-26 kg
Nuclear radius = \(R_{0} A^{1 / 3}=1.1 \times 10^{-15} \times(56)^{1 / 3} \mathrm{~m}\)
\(\rho_{\mathrm{nu}}=\frac{\text { Nuclear mass }}{\text { Nuclear volume }}=\frac{m_{\mathrm{Fe}}}{\frac{4}{3} \pi R^{3}}\) \([\because A=56]\)
\(=\frac{9.27 \times 10^{-26}}{\frac{4 \pi}{3} \times\left(1.1 \times 10^{-15}\right)^{3} \times 56}=2.9 \times 10^{17} \mathrm{~kg} \mathrm{~m}^{-3}\)
(v) (d): Here, A1 = 27, A2 = 125, R1 = 3.6 fm
\(\text { As, } \frac{R_{2}}{R_{1}}=\left(\frac{A_{2}}{A_{1}}\right)^{1 / 3}=\left(\frac{125}{27}\right)^{1 / 3}=\frac{5}{3}\)
\(\therefore \quad R_{2}=\frac{5}{3} R_{1}=\frac{5}{3} \times 3.6=6 \mathrm{fm}\) -
(i) (a) : As just shown, energy conservation allows us to calculate the third particle's total energy.But we do not know what percentage of that total is mass energy.
(ii) (d): According to the passage, subatomic reactions do not conserve mass. So, we cannot find the third particle's mass by setting mneutronequal to mproton+ melectron+ mthirdparticle
The neutron has energy 940.97 MeV. The proton has energy 939.67 MeV + 0.01 MeV = 939.69 MeV. The electron has energy 0.51 MeV + 0.39 MeV = 0.90 MeV.
Therefore, the third particle has energy
\(E_{\text {third particle }}=E_{\text {neutron }}-E_{\text {proton }}-\mathrm{E}_{\text {Electron }}\)
= 940.97 - 939.67 - 0.90 = 0.40 MeV
We just found the third particle's total energy, the sum of its mass energy and kinetic energy. Without more information, we cannot figure out how much of that energy is mass energy.
(iii) (b)
(iv) (a): Here, P = 500 MW = 5 x 108 W,
t = 1 h = 3600 s
Energy produced, E = P x t = 5 x 108 x 3600
= 18 x 1011 J
\(\text { As } E=\Delta m c^{2}\)
\(\therefore \quad \Delta m=\frac{E}{c^{2}}=\frac{18 \times 10^{11}}{\left(3 \times 10^{8}\right)^{2}}=\frac{18 \times 10^{11}}{9 \times 10^{16}}=2 \times 10^{-5} \mathrm{~kg}\)
(v) (a): Using, E = mc2
Here, \(m=1 \mathrm{~g}=1 \times 10^{-3} \mathrm{~kg}, c=3 \times 10^{8} \mathrm{~m} \mathrm{~s}^{-1}\)
\(\therefore E=10^{-3} \times 9 \times 10^{16}=9 \times 10^{13} \mathrm{~J}\)