Physics Objective Questions and Answers: Nuclei
Access targeted multiple-choice questions for Nuclei designed to align with the latest JEE academic syllabus for JEE Physics. These objective practice sets help students evaluate their conceptual understanding and improve exam readiness.
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Multiple Choice Questions
(a) X and Y are isotopes
(b) X and Z are isobars
(c) X and Y are isobars
(d) X and Z are isotopes
Show Answer & Explanation
Answer: (d) X and Z are isotopes
Explanation:
1. Alpha emission lowers Z by 2 and A by 4. Two beta-minus emissions raise Z by 2 and leave A unchanged.
2. So Z has the same atomic number as X but mass number 4 less: X and Z are isotopes.
Teacher's Note:
1. Isotopes share atomic number, isobars share mass number. Track Z and A separately for each step.
(a) 6 and 8
(b) 6 and 6
(c) 8 and 8
(d) 8 and 6
Show Answer & Explanation
Answer: (d) 8 and 6
Explanation:
1. Mass number falls by 32, and each alpha removes 4: \( 32/4=8 \) alpha particles.
2. Eight alphas lower Z by 16 but Z falls only by 10, so 6 beta-minus particles (each raises Z by 1) are emitted.
Teacher's Note:
1. First find alphas from the change in mass number. Betas then correct the atomic number.
(a) Electrons
(b) Electromagnetic radiation
(c) Helium nuclei
(d) Neutrons
Show Answer & Explanation
Answer: (d) Neutrons
Explanation:
1. Natural radioactivity emits alpha (helium nuclei), beta (electrons) and gamma (electromagnetic) radiation.
2. Neutrons are not emitted in natural radioactive decay.
Teacher's Note:
1. Memorise the three natural emissions: alpha, beta and gamma. Neutron emission occurs in nuclear reactions.
(a) pair annihilation takes place
(b) energy is released due to conversion of a neutron into a proton
(c) energy is released due to de-excitation of a nucleus
(d) none of these
Show Answer & Explanation
Answer: (c) energy is released due to de-excitation of a nucleus
Explanation:
1. A nucleus left in an excited state after alpha or beta decay drops to a lower level.
2. The energy difference leaves as a gamma photon.
Teacher's Note:
1. Gamma rays come from nuclear energy level transitions, just as visible light comes from atomic ones. The proton number and mass number do not change.
(a) \( {}^{0}_{-1}e \)
(b) \( {}^{1}_{1}\text{H} \)
(c) \( {}^{4}_{2}\text{He} \)
(d) \( {}^{1}_{0}n \)
Show Answer & Explanation
Answer: (d) \( {}^{1}_{0}n \)
Explanation:
1. Mass number: 27 + 4 = 30 + A, so A = 1.
2. Charge: 13 + 2 = 15 + Z, so Z = 0.
3. A particle with A = 1 and Z = 0 is a neutron.
Teacher's Note:
1. Balance both the mass number and the charge. This was the reaction in which artificial radioactivity was discovered.
(a) \( 1\times10^5 \)
(b) \( 2\times10^5 \)
(c) \( 7\times10^5 \)
(d) \( 11\times10^5 \)
Show Answer & Explanation
Answer: (c) \( 7\times10^5 \)
Explanation:
1. \( N=N_0\left(\tfrac12\right)^{t/T}=10^6\times2^{-1/2} \).
2. \( =10^6\times0.707\approx7\times10^5 \).
Teacher's Note:
1. Half the time of a half-life leaves about 71 percent. It is the reciprocal of root 2.
(a) 0.5
(b) 2.0
(c) 1.0
(d) 3.0
Show Answer & Explanation
Answer: (a) 0.5
Explanation:
1. In 30 minutes P completes 3 half-lives: fraction \( (1/2)^3=1/8 \).
2. Q completes 2 half-lives: fraction \( (1/2)^2=1/4 \).
3. Ratio = (1/8)/(1/4) = 0.5.
Teacher's Note:
1. Count the number of half-lives for each isotope separately. Then compare the surviving fractions.
(a) e
(b) \( 1/e \)
(c) \( \dfrac{e-1}{e} \)
(d) \( \dfrac{e}{e-1} \)
Show Answer & Explanation
Answer: (c) \( \dfrac{e-1}{e} \)
Explanation:
1. After one mean life \( t=1/\lambda \), \( N=N_0e^{-1} \).
2. Fraction decayed = \( 1-\dfrac1e=\dfrac{e-1}{e} \) (about 63 percent).
Teacher's Note:
1. In one mean life the sample falls to 1/e of its original size. About 63 percent has decayed by then.
(a) \( \dfrac1{10\lambda} \)
(b) \( \dfrac1{11\lambda} \)
(c) \( \dfrac{11}{10\lambda} \)
(d) \( \dfrac1{9\lambda} \)
Show Answer & Explanation
Answer: (d) \( \dfrac1{9\lambda} \)
Explanation:
1. \( \dfrac{N_1}{N_2}=\dfrac{e^{-10\lambda t}}{e^{-\lambda t}}=e^{-9\lambda t} \).
2. Setting this equal to \( e^{-1} \) gives \( t=\dfrac1{9\lambda} \).
Teacher's Note:
1. Divide the two exponentials and the decay constants subtract. Equate the remaining exponent to minus one.
(a) 16.425
(b) 15.425
(c) 18.725
(d) 1.301
Show Answer & Explanation
Answer: (a) 16.425
Explanation:
1. \( \dfrac{N}{N_0}=\dfrac1{20}=2^{-t/T}\Rightarrow t=T\log_2 20 \).
2. \( \log_220=4.322\Rightarrow t=3.8\times4.322=16.4 \) days.
Teacher's Note:
1. Write the surviving fraction as a power of two. log base 2 of 20 is a little over 4.3.
(a) 28 min
(b) 32 min
(c) 16 min
(d) 40 min
Show Answer & Explanation
Answer: (b) 32 min
Explanation:
1. The rate halves between 4 min and 36 min.
2. So one half-life = 36 - 4 = 32 min.
Teacher's Note:
1. When the count rate halves, exactly one half-life has passed. The elapsed time between the two readings is the half-life.
(a) 20 min
(b) 40 min
(c) 50 min
(d) 10 min
Show Answer & Explanation
Answer: (a) 20 min
Explanation:
1. At 33 percent decay, 67 percent remains. At 67 percent decay, 33 percent remains.
2. The amount has halved (67 to 33.5 is nearly a factor of 2), so the time is about one half-life, 20 min.
Teacher's Note:
1. The two remaining fractions are about 2 : 1. Whenever the ratio is 2, one half-life has elapsed.
(a) 150
(b) 200
(c) 300
(d) 400
Show Answer & Explanation
Answer: (b) 200
Explanation:
1. 1600 to 100 is a factor of 16 = \( 2^4 \), so 4 half-lives in 8 s and \( T=2 \) s.
2. At 6 s, 3 half-lives have passed: \( 1600/2^3=200 \) counts/s.
Teacher's Note:
1. Find the half-life from the total fall first. Then count the half-lives up to the time asked.
(a) \( \dfrac{N_0}{2^8} \)
(b) \( \dfrac{N_0}{2^4} \)
(c) \( \dfrac{N_0}{2^6} \)
(d) \( \dfrac{N_0}{2^5} \)
Show Answer & Explanation
Answer: (a) \( \dfrac{N_0}{2^8} \)
Explanation:
1. 0 to 0.5 hr (A only): one half-life, factor 1/2.
2. 0.5 to 1.5 hr (B only): 1 hr = 4 half-lives of 1/4 hr, factor 1/16.
3. 1.5 to 2 hr (both): decay constants add, so effective half-life \( T=\dfrac{(1/2)(1/4)}{1/2+1/4}=\dfrac16 \) hr; 0.5 hr = 3 half-lives, factor 1/8.
4. Total: \( \tfrac12\cdot\tfrac1{16}\cdot\tfrac18=\dfrac1{256}=2^{-8} \).
Teacher's Note:
1. When two processes act together their decay constants add. Handle each time interval separately and multiply the factors.
(a) 1 : 2 : 3
(b) 2 : 1 : 3
(c) 3 : 2 : 1
(d) 2 : 3 : 1
Show Answer & Explanation
Answer: (a) 1 : 2 : 3
Explanation:
1. All lumps are the same substance, so they have the same decay constant.
2. Activity \( A=A_0e^{-\lambda t} \) falls by the same factor for all, so the ratio stays 1 : 2 : 3.
Teacher's Note:
1. A common decay constant means every sample shrinks by the same factor. Ratios are therefore preserved.
(a) no nucleus will decay before t = 4 days
(b) no nucleus will decay before t = 8 days
(c) all nuclei will decay before t = 16 days
(d) a given nucleus may decay at any time after t = 0
Show Answer & Explanation
Answer: (d) a given nucleus may decay at any time after t = 0
Explanation:
1. Radioactive decay is random; half-life is a statistical property of a large number of nuclei.
2. Any single nucleus may decay at any instant, and some will survive beyond 16 days.
Teacher's Note:
1. Half-life describes the behaviour of a large population, not of one nucleus. A single nucleus has no fixed lifetime.
(a) 4
(b) 2
(c) 0.25
(d) 0.75
Show Answer & Explanation
Answer: (a) 4
Explanation:
1. \( A=\lambda N \). With \( N_1=2N_2 \): \( \lambda_1=\dfrac{A_1}{2N_2},\ \lambda_2=\dfrac{2A_1}{N_2} \).
2. \( \lambda_1/\lambda_2=1/4 \), and since \( T\propto1/\lambda \), \( T_1/T_2=4 \).
Teacher's Note:
1. Activity equals decay constant times number of nuclei. Half-life varies inversely with decay constant.
(a) 1.40
(b) 1.50
(c) 2.750
(d) 3.375
Show Answer & Explanation
Answer: (b) 1.50
Explanation:
1. \( R=R_0A^{1/3} \), so \( R_1/R_2=(135/40)^{1/3}=(3.375)^{1/3}=1.5 \).
Teacher's Note:
1. Nuclear radius varies as the cube root of mass number. 135/40 is 27/8, a perfect cube ratio.
(a) \( 2^{1/3}:1 \)
(b) \( 1:2^{1/3} \)
(c) \( 2^{3/2}:1 \)
(d) \( 1:2^{3/2} \)
Show Answer & Explanation
Answer: (b) \( 1:2^{1/3} \)
Explanation:
1. Momentum conservation: \( m_1v_1=m_2v_2 \), so \( m_1:m_2=1:2 \) (the faster part is lighter).
2. Radius \( \propto A^{1/3}\propto m^{1/3} \), so \( R_1:R_2=1:2^{1/3} \).
Teacher's Note:
1. Equal and opposite momenta mean the speeds are inversely proportional to the masses. Mass number is proportional to mass.
(a) Proton and electron
(b) Neutron and electron
(c) Electron and neutron
(d) All of these
Show Answer & Explanation
Answer: (d) All of these
Explanation:
1. Nuclear (strong) force acts between nucleons only: proton-proton, neutron-neutron and proton-neutron.
2. An electron is a lepton and does not feel the strong force, so none of the pairs listed experiences it.
Teacher's Note:
1. The strong force acts on nucleons, not on electrons. Electrons take part in electromagnetic and weak interactions.
(a) \( {}^4\text{He} \)
(b) \( {}^7\text{Li} \)
(c) Equally stable
(d) Cannot be decided
Show Answer & Explanation
Answer: (a) \( {}^4\text{He} \)
Explanation:
1. Stability depends on binding energy per nucleon.
2. He-4: 27.37/4 = 6.84 MeV. Li-7: 39.3/7 = 5.61 MeV.
3. He-4 has the larger value, so it is more stable.
Teacher's Note:
1. Never compare total binding energies of nuclei of different size. Divide by the number of nucleons first.
(a) 8 eV
(b) 8 J
(c) 8 keV
(d) 8 MeV
Show Answer & Explanation
Answer: (d) 8 MeV
Explanation:
1. For most nuclei binding energy per nucleon lies between 7 and 9 MeV, with a maximum near 8.7 MeV for iron.
Teacher's Note:
1. Nuclear energies are millions of times larger than chemical ones. A few eV per atom in chemistry, about 8 MeV per nucleon in nuclei.
(a) \( 2(x_2-x_1) \)
(b) \( 2(x_1+x_2) \)
(c) \( 4(x_1+x_2) \)
(d) \( 4(x_2-x_1) \)
Show Answer & Explanation
Answer: (d) \( 4(x_2-x_1) \)
Explanation:
1. Binding energy of He-4 = \( 4x_2 \); of two deuterons = \( 2\times2x_1=4x_1 \).
2. Q = BE of products - BE of reactants = \( 4x_2-4x_1=4(x_2-x_1) \).
Teacher's Note:
1. Energy released equals the gain in total binding energy. Multiply binding energy per nucleon by the number of nucleons.
(a) \( E_a-3E_b=Q \)
(b) \( 3E_b-E_a=Q \)
(c) \( E_a+3E_b=Q \)
(d) \( E_b+3E_a=Q \)
Show Answer & Explanation
Answer: (a) \( E_a-3E_b=Q \)
Explanation:
1. Energy released = binding energy of the product - binding energy of the reactants.
2. \( Q=E_a-3E_b \).
Teacher's Note:
1. Q equals binding energy after minus binding energy before. Each of the three B nuclei brings its own binding energy.
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Practice MCQs for JEE Physics Nuclei
JEE Physics Nuclei Objective Test Questions
Test your conceptual understanding of Nuclei with these targeted multiple-choice questions. Designed in alignment with the latest JEE curriculum for JEE Physics, these problem sets build accuracy and prepare students for objective exams.
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FAQs
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