Download JEE MCQs for JEE Physics: Nuclei
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Chapter-wise Objective Questions: Nuclei
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Multiple Choice Questions
(a) M < (N·Mn + Z·Mp)
(b) M > (N·Mn + Z·Mp)
(c) M = (N·Mn + Z·Mp)
(d) M = N(Mn + Mp)
Show Answer & Explanation
Answer: (a) M < (N·Mn + Z·Mp)
Explanation:
1. The nucleus is a bound system, and some mass is converted to binding energy
2. Hence the nuclear mass is less than the sum of the masses of its free nucleons (mass defect).
Teacher's Note:
1. Mass defect Δm = (N Mn + Z Mp) − M > 0.
2. Binding energy = Δm c².
(a) (a) and (c)
(b) (a) and (b)
(c) (a) and (d)
(d) all of them
Show Answer & Explanation
Answer: (b) (a) and (b)
Explanation:
1. The fragments are more tightly bound, so their total binding energy exceeds that of the parent
2. The extra binding energy corresponds to a small mass defect converted to energy, so (a) and (b) are correct.
Teacher's Note:
1. Fission and fusion both increase the total binding energy.
2. The released energy equals the gain in binding energy.
(a) nuclear fusion
(b) nuclear fission
(c) combination of hydrogen atoms
(d) combination of electrons and protons
Show Answer & Explanation
Answer: (b) nuclear fission
Explanation:
1. An atom bomb is an uncontrolled chain reaction of fission of U-235 or Pu-239.
Teacher's Note:
1. A hydrogen bomb uses fusion, triggered by a fission bomb.
2. Super-critical mass gives K > 1 and an explosion.
(a) 3.125 × 10¹³
(b) 3.125 × 10¹⁴
(c) 3.125 × 10¹⁵
(d) 3.125 × 10¹⁶
Show Answer & Explanation
Answer: (a) 3.125 × 10¹³
Explanation:
1. Energy per fission = 200 × 1.6 × 10⁻¹³ = 3.2 × 10⁻¹¹ J
2. Number per second = 1000 / 3.2 × 10⁻¹¹ = 3.125 × 10¹³.
Teacher's Note:
1. Rate = power / energy per fission.
2. 1 MeV = 1.6 × 10⁻¹³ J.
(a) 139 MeV/c²
(b) 39 MeV/c²
(c) 93 MeV/c²
(d) 931 MeV/c²
Show Answer & Explanation
Answer: (d) 931 MeV/c²
Explanation:
1. E = mc² = 1.66 × 10⁻²⁷ × (3 × 10⁸)² = 1.49 × 10⁻¹⁰ J = 931 MeV
2. So 1 u = 931 MeV/c².
Teacher's Note:
1. This conversion factor is used in every mass defect problem.
2. Remember 931.5 MeV/c² for more accuracy.
(a) 0.1%
(b) 1%
(c) 10%
(d) 0.01%
Show Answer & Explanation
Answer: (a) 0.1%
Explanation:
1. The mass defect in fission is about 0.1% of the mass of the fissioned nucleus (about 200 MeV out of 235 × 931 MeV).
Teacher's Note:
1. Check: 200 / (235 × 931) ≈ 0.09%.
2. In fusion of hydrogen the figure is about 0.7%.
(a) light nuclei
(b) heavy nuclei
(c) elements lying in the middle of the periodic table
(d) middle elements lying on the binding energy curve
Show Answer & Explanation
Answer: (a) light nuclei
Explanation:
1. Fusion of light nuclei increases the binding energy per nucleon and so releases energy
2. Middle elements are already near the maximum of the curve and heavy nuclei undergo fission instead.
Teacher's Note:
1. Fusion lies on the rising left-hand part of the binding energy curve.
2. Fission lies on the falling right-hand part.
(a) α-particle
(b) electron
(c) proton
(d) neutron
Show Answer & Explanation
Answer: (d) neutron
Explanation:
1. A free neutron decays into a proton, an electron and an anti-neutrino with a half-life of about 10 minutes
2. The other three are stable.
Teacher's Note:
1. A free proton cannot decay because it is lighter than a neutron.
2. Inside a nucleus, a neutron can be stable.
(a) gravitational force
(b) electric force
(c) magnetic force
(d) nuclear force
Show Answer & Explanation
Answer: (a) gravitational force
Explanation:
1. The gravitational force is by far the weakest of the four fundamental forces.
Teacher's Note:
1. Order of strength: nuclear > electromagnetic > weak > gravitational.
2. Gravity matters only because masses are large.
(a) 10¹
(b) 10⁵
(c) 10¹⁰
(d) 10¹⁵
Show Answer & Explanation
Answer: (d) 10¹⁵
Explanation:
1. Atomic radius is about 10⁻¹⁰ m and nuclear radius about 10⁻¹⁵ m, a ratio of 10⁵
2. Volume scales as radius cubed, giving (10⁵)³ = 10¹⁵.
Teacher's Note:
1. Atoms are mostly empty space.
2. The volume ratio is the cube of the radius ratio.
(a) 0.0305 J
(b) 0.0305 erg
(c) 28.4 MeV
(d) 0.061 u
Show Answer & Explanation
Answer: (c) 28.4 MeV
Explanation:
1. Mass of 2 protons and 2 neutrons = 2(1.0073) + 2(1.0087) = 4.0320 u
2. Mass defect = 4.0320 − 4.0015 = 0.0305 u
3. Binding energy = 0.0305 × 931 = 28.4 MeV.
Teacher's Note:
1. Binding energy is expressed in MeV, not in u; u is a unit of mass.
2. Divide by 4 to get 7.1 MeV per nucleon.
(a) always less than its atomic number
(b) always more than its atomic number
(c) may be equal to its atomic number
(d) sometimes less and sometimes more than its atomic number
Show Answer & Explanation
Answer: (c) may be equal to its atomic number
Explanation:
1. A = Z + N, with N ≥ 0
2. For ordinary hydrogen (A = 1, Z = 1) there is no neutron, so A = Z there; for all others A > Z
3. So A may equal Z but is never less.
Teacher's Note:
1. A ≥ Z for every nucleus.
2. The equality holds only for the hydrogen nucleus (protium).
(a) an electron
(b) a positron
(c) an alpha particle
(d) a proton
Show Answer & Explanation
Answer: (c) an alpha particle
Explanation:
1. Mass number: 40 + A = 43 + 1, so A = 4
2. Charge: 20 + Z = 21 + 1, so Z = 2
3. A = 4, Z = 2 is an α-particle.
Teacher's Note:
1. Balance mass number and charge on both sides.
2. Such bombardment reactions are used to make new nuclides.
(a) only between light nuclei
(b) only between heavy nuclei
(c) between both light and heavy nuclei
(d) only between nuclei which are stable against β-decay
Show Answer & Explanation
Answer: (a) only between light nuclei
Explanation:
1. Fusion releases energy only when the nuclei are light (mass number below about 56), so that the product has a higher binding energy per nucleon.
Teacher's Note:
1. Fusion of heavy nuclei would absorb energy.
2. The Coulomb barrier is lowest for hydrogen isotopes.
(a) 10¹³ kg/m³
(b) 10¹⁵ kg/m³
(c) 10¹⁷ kg/m³
(d) 10¹⁹ kg/m³
Show Answer & Explanation
Answer: (c) 10¹⁷ kg/m³
Explanation:
1. Density ≈ 1.66 × 10⁻²⁷ A / [(4/3)π(1.2 × 10⁻¹⁵)³ A] ≈ 2.3 × 10¹⁷ kg/m³.
Teacher's Note:
1. This is the same for all nuclei.
2. A teaspoon of nuclear matter would weigh about a billion tonnes.
(a) m₃ equals the difference m₁ − m₂
(b) m₃ < (m₁ + m₂)
(c) m₃ > (m₁ + m₂)
(d) m₃ = m₁ + m₂
Show Answer & Explanation
Answer: (b) m₃ < (m₁ + m₂)
Explanation:
1. The product is more tightly bound, so some mass is converted into released energy
2. Hence m₃ is less than m₁ + m₂.
Teacher's Note:
1. Mass defect in fusion = (m₁ + m₂) − m₃ > 0.
2. Energy released = Δm × 931 MeV.
(a) Z protons and A − Z neutrons
(b) Z protons and A neutrons
(c) A protons and Z − A neutrons
(d) Z neutrons and A − Z protons
Show Answer & Explanation
Answer: (a) Z protons and A − Z neutrons
Explanation:
1. Z is the atomic number (number of protons) and A is the mass number (protons + neutrons), so neutrons = A − Z.
Teacher's Note:
1. The number of electrons in the neutral atom equals Z.
2. Isotopes have the same Z but different A.
(a) M(N, Z) = N·Mn + Z·Mp + Bc²
(b) M(N, Z) = N·Mn + Z·Mp − B/c²
(c) M(N, Z) = N·Mn + Z·Mp + B/c²
(d) M(N, Z) = N·Mn + Z·Mp − Bc²
Show Answer & Explanation
Answer: (b) M(N, Z) = N·Mn + Z·Mp − B/c²
Explanation:
1. Binding energy B = Δm c² where Δm = (N Mn + Z Mp) − M
2. So M = N Mn + Z Mp − B/c².
Teacher's Note:
1. Dimension check: B/c² has the dimensions of mass, but Bc² does not.
2. The nucleus is lighter than its separate nucleons.
(a) 6.02 × 10⁻²⁷ kg
(b) 1.66 × 10⁻²⁷ kg
(c) 16.66 × 10⁻²⁶ kg
(d) 6.02 × 10⁻²⁶ kg
Show Answer & Explanation
Answer: (b) 1.66 × 10⁻²⁷ kg
Explanation:
1. 931 MeV = 931 × 1.6 × 10⁻¹³ = 1.49 × 10⁻¹⁰ J
2. m = E/c² = 1.49 × 10⁻¹⁰ / 9 × 10¹⁶ = 1.66 × 10⁻²⁷ kg (one atomic mass unit).
Teacher's Note:
1. 931 MeV corresponds to exactly 1 u.
2. Use m = E/c² for any energy-to-mass conversion.
(a) 9 J
(b) 9 × 10¹³ J
(c) 9 × 10⁵ J
(d) 9 × 10¹⁰ J
Show Answer & Explanation
Answer: (d) 9 × 10¹⁰ J
Explanation:
1. m = 1 mg = 10⁻⁶ kg
2. E = mc² = 10⁻⁶ × 9 × 10¹⁶ = 9 × 10¹⁰ J.
Teacher's Note:
1. Convert milligram to kilogram first (1 mg = 10⁻⁶ kg).
2. This is enough energy to run a 1 MW power station for about a day.
(a) nuclear force > electric force
(b) electric force > nuclear force
(c) gravitational force > nuclear force
(d) none of the above
Show Answer & Explanation
Answer: (a) nuclear force > electric force
Explanation:
1. Nuclear force is strongest at nuclear distances (about 100 times the Coulomb repulsion), which is why the nucleus is stable
2. Gravity is much weaker than both.
Teacher's Note:
1. Heavy nuclei are unstable because the Coulomb force is long-range while the nuclear force is short-range.
2. The nuclear force is attractive between 0.8 fm and about 3 fm.
(a) graph (a)
(b) graph (b)
(c) graph (c)
(d) graph (d)
Show Answer & Explanation
Answer: (a) graph (a)
Explanation:
1. BN rises steeply for light nuclei, reaches a maximum of about 8.8 MeV at A = 56 (iron) and then falls slowly for heavy nuclei
2. Only graph (a) has this shape with the peak at A = 56.
Teacher's Note:
1. The other graphs have peaks or minima at the wrong place or the wrong shape.
2. The maximum near iron explains why iron is the most stable nucleus.
(a) \({}^{74}_{34}\mathrm{Se}\) and \({}^{71}_{31}\mathrm{Ga}\)
(b) \({}^{84}_{38}\mathrm{Sr}\) and \({}^{86}_{38}\mathrm{Sr}\)
(c) \({}^{92}_{42}\mathrm{Mo}\) and \({}^{92}_{40}\mathrm{Zr}\)
(d) \({}^{40}_{20}\mathrm{Ca}\) and \({}^{32}_{16}\mathrm{S}\)
Show Answer & Explanation
Answer: (a) \({}^{74}_{34}\mathrm{Se}\) and \({}^{71}_{31}\mathrm{Ga}\)
Explanation:
1. Isotones have the same number of neutrons
2. Se-74 has 74 − 34 = 40 neutrons and Ga-71 has 71 − 31 = 40 neutrons
3. The other pairs: isotopes, isobars, and 20 and 16 neutrons respectively.
Teacher's Note:
1. Isotopes: same Z. Isobars: same A. Isotones: same N.
2. Always compute N = A − Z for each nucleus.
(a) \({}^{10}_{5}\mathrm{B}\) + \({}^{4}_{2}\mathrm{He}\) → \({}^{13}_{7}\mathrm{N}\) + \({}^{1}_{1}\mathrm{H}\)
(b) \({}^{23}_{11}\mathrm{Na}\) + \({}^{1}_{1}\mathrm{H}\) → \({}^{22}_{10}\mathrm{Ne}\) + \({}^{4}_{2}\mathrm{He}\)
(c) \({}^{239}_{93}\mathrm{Np}\) → \({}^{239}_{94}\mathrm{Pu}\) + β⁻ + anti-neutrino
(d) \({}^{11}_{7}\mathrm{N}\) + \({}^{1}_{1}\mathrm{H}\) → \({}^{12}_{6}\mathrm{C}\) + β⁺ + ν
Show Answer & Explanation
Answer: (c) \({}^{239}_{93}\mathrm{Np}\) → \({}^{239}_{94}\mathrm{Pu}\) + β⁻ + anti-neutrino
Explanation:
1. Check A and Z on both sides
2. First: A 14 → 14 but Z 7 → 8, no. Second: A 24 → 26, no. Third: A 239 → 239 and Z 93 → 94 − 1 = 93, yes. Fourth: Z 8 → 7 (6 + 1), no.
Teacher's Note:
1. A possible nuclear reaction conserves both mass number and charge.
2. The third is an ordinary β⁻ decay.
(a) a + b + c
(b) c + a − b
(c) c − a − b
(d) a + b − c
Show Answer & Explanation
Answer: (c) c − a − b
Explanation:
1. Energy released = (total binding energy of products) − (total binding energy of reactants)
2. The neutron has no binding energy, so Q = c − (a + b).
Teacher's Note:
1. Binding energy released = gain in binding energy.
2. Free nucleons have zero binding energy.
(a) greater than 1
(b) depends on the mass of the parent nucleus
(c) equal to 1
(d) less than 1
Show Answer & Explanation
Answer: (d) less than 1
Explanation:
1. Some mass is converted into released energy, so the products weigh less than the parent.
Teacher's Note:
1. The mass defect is only about 0.1%, so the ratio is just under 1.
2. Mass and energy together are conserved.
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Multiple Choice Questions (MCQs) for JEE Physics Nuclei
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