Practice MCQs for JEE Physics Modern Physics
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Multiple Choice Questions
(a) 2
(b) 3
(c) 4
(d) 5
Show Answer & Explanation
Answer: (b) 3
Explanation:
1. \( 13.6 - 12.1 = 1.5 \) eV, so the atom reaches \( n = 3 \).
2. Number of lines \( = 3\times2/2 = 3 \).
Teacher's Note:
1. Count transitions down from \( n = 3 \).
(a) \( 1.09\times10^6 \) m/s
(b) \( 0.73\times10^6 \) m/s
(c) \( 3.0\times10^8 \) m/s
(d) \( 2.92\times10^6 \) m/s
Show Answer & Explanation
Answer: (a) \( 1.09\times10^6 \) m/s
Explanation:
1. \( v = 2\pi KZe^2/(nh) = 2.18\times10^6\times Z/n m/s \).
2. \( v = 2.18\times10^6\times2/4 = 1.09\times10^6 m/s \).
Teacher's Note:
1. Speed grows with \( Z \) and falls with \( n \).
(a) \( 0.025\times10^4 \) m⁻¹
(b) \( 0.5\times10^7 \) m⁻¹
(c) \( 10^7 \) m⁻¹
(d) \( 2.5\times10^7 \) m⁻¹
Show Answer & Explanation
Answer: (c) \( 10^7 \) m⁻¹
Explanation:
1. The last line corresponds to \( n\to\infty \): \( \bar\nu = R(1 - 0) = R \).
2. The wave number is \( 10^7 m^{-1} \).
Teacher's Note:
1. The series limit gives the largest wave number.
(a) 1 : 1
(b) 1 : −1
(c) 2 : −1
(d) 1 : −2
Show Answer & Explanation
Answer: (b) 1 : −1
Explanation:
1. \( K = -E \) for an electron in a Bohr orbit.
2. The ratio is 1 : −1.
Teacher's Note:
1. Total energy is negative of the kinetic energy.
(a) hydrogen is a gas
(b) hydrogen is very light
(c) energy difference in energy levels of hydrogen is much less
(d) energy difference in energy levels of hydrogen is much high
Show Answer & Explanation
Answer: (c) energy difference in energy levels of hydrogen is much less
Explanation:
1. Characteristic X-rays need transitions between inner shells with energy differences of keV.
2. In hydrogen the energy differences are only a few eV.
Teacher's Note:
1. Characteristic X-rays come from inner-shell vacancies of heavy atoms.
(a) the wavelength is higher
(b) the intensity is higher
(c) the frequency is higher
(d) the photon energy is lower
Show Answer & Explanation
Answer: (c) the frequency is higher
Explanation:
1. Harder X-rays have higher photon energy, so they have higher frequency and a shorter wavelength.
Teacher's Note:
1. Hard means more penetrating.
(a) 0 to ∞
(b) \( \lambda_{min} \) to ∞, where \( \lambda_{min}>0 \)
(c) 0 to \( \lambda_{max} \), where \( \lambda_{max}<\infty \)
(d) \( \lambda_{min} \) to \( \lambda_{max} \), where \( 0<\lambda_{min}<\lambda_{max}<\infty \)
Show Answer & Explanation
Answer: (b) \( \lambda_{min} \) to ∞, where \( \lambda_{min}>0 \)
Explanation:
1. The maximum photon energy is eV, so there is a minimum wavelength \( \lambda_{min} = hc/eV > 0 \).
2. There is no limit on the lower energy, so the wavelength extends to \( \infty \).
Teacher's Note:
1. The cut-off is only at the short wavelength end.
(a) 0.3443 Å
(b) 0.6887 Å
(c) 1.3982 Å
(d) 4.78 Å
Show Answer & Explanation
Answer: (b) 0.6887 Å
Explanation:
1. \( \Delta E = 18 \) keV.
2. \( \lambda = 12.4/18 = 0.689 \) Å.
Teacher's Note:
1. Use λ(Å) = 12.4/E(keV).
(a) 0.27 Å
(b) 0.32 Å
(c) 0.39 Å
(d) 0.2 Å
Show Answer & Explanation
Answer: (a) 0.27 Å
Explanation:
1. \( K\beta \) comes from the \( M \) to \( K \) transition, which has a larger energy than \( L \) to \( K \).
2. Its wavelength is shorter than 0.32 Å, about 0.27 Å (the ratio is \( (1-1/4)/(1-1/9)\approx0.84 \)).
Teacher's Note:
1. A bigger jump gives a shorter wavelength.
(a) the K-series of characteristic X-ray will be emitted by Co only
(b) the K-series of characteristic X-rays will be emitted by Cu and Co only
(c) the K-series of characteristic X-rays will be emitted by Cu, Co and Mo
(d) the minimum wavelength of continuous X-rays emitted by the three metals will not be the same
Show Answer & Explanation
Answer: (b) the K-series of characteristic X-rays will be emitted by Cu and Co only
Explanation:
1. A K-shell vacancy needs electron energy above the \( K \) ionisation energy.
2. The 15 keV electrons exceed 7.8 and 9.0 keV, but not 20.1 keV.
3. So only Co and Cu emit the K-series.
Teacher's Note:
1. Compare the beam energy with the ionisation energy.
(a) 1/4
(b) 1/16
(c) \( 2/\sqrt5 \)
(d) 25/16
Show Answer & Explanation
Answer: (d) 25/16
Explanation:
1. Moseley's law: \( \lambda\propto1/(Z-1)^2 \).
2. \( \lambda_1/\lambda_2 = (79/63)^2\approx1.57\approx25/16 \).
Teacher's Note:
1. Use \( Z - 1 \) rather than \( Z \).
(a) Li⁷
(b) Na²¹
(c) Fe⁵⁶
(d) Na²³
Show Answer & Explanation
Answer: (a) Li⁷
Explanation:
1. \( R\propto A^{1/3} \), so \( A = 189/27 = 7 \).
2. The nucleus is Li⁷.
Teacher's Note:
1. Radius scales as the cube root of \( A \).
(a) 4.8
(b) 3.6
(c) 2.4
(d) 1.2
Show Answer & Explanation
Answer: (a) 4.8
Explanation:
1. \( R = 3.6(64/27)^{1/3} = 3.6\times4/3 \).
2. \( R = 4.8 \) fermi.
Teacher's Note:
1. Use \( R ∝ A^{1/3} \).
(a) F_pp < F_pn = F_nn
(b) F_pp > F_pn = F_nn
(c) F_pp = F_pn = F_nn
(d) F_pp < F_pn < F_nn
Show Answer & Explanation
Answer: (c) F_pp = F_pn = F_nn
Explanation:
1. Nuclear force is charge independent.
2. The three forces are equal at the same separation.
Teacher's Note:
1. Nuclear force does not distinguish protons from neutrons.
(a) E₁ = 2E₂
(b) E₂ = 2E₁
(c) E₁ > E₂
(d) E₂ > E₁
Show Answer & Explanation
Answer: (d) E₂ > E₁
Explanation:
1. In fission energy is released, so the daughter nuclei are more tightly bound.
2. Hence \( E_2 > E_1 \).
Teacher's Note:
1. Higher binding energy per nucleon means more stable.
(a) Both Z and A will decrease, if the process is α decay
(b) Z will decrease but A will not change, if the process is β⁺ decay
(c) Z will decrease but A will not change, if the process is β⁻ decay
(d) Z and A will remain unchanged, if the process is γ decay
Show Answer & Explanation
Answer: (c) Z will decrease but A will not change, if the process is β⁻ decay
Explanation:
1. In β⁻ decay a neutron becomes a proton, so \( Z \) increases by 1, not decreases.
2. The other three statements are right.
Teacher's Note:
1. β⁻ raises \( Z, \beta^{+} \) lowers \( Z \).
(a) M₂ = 2M₁
(b) M₂ > 2M₁
(c) M₂ < 2M₁
(d) M₁ < 10(mₙ + mₚ)
Show Answer & Explanation
Answer: (c) M₂ < 2M₁
Explanation:
1. Ca-40 has a higher binding energy per nucleon than Ne-20, so its mass defect is more than twice that of Ne-20.
2. Therefore \( M_2 < 2M_1 \).
Teacher's Note:
1. Mass defect grows faster than the number of nucleons.
(a) A & B
(b) A & D
(c) B & C
(d) C & D
Show Answer & Explanation
Answer: (b) A & D
Explanation:
1. Fission releases energy, so the rest mass energy of \( U \) is greater than that of the products.
2. \( (A) \) and \( (D) \) state this.
Teacher's Note:
1. Energy released equals the drop in rest mass energy.
(a) A typical fission may be represented by \( ^{235}_{92}U + ^1_0n \to ^{143}_{56}Ba + ^{93}_{36}Kr + \text{energy} \)
(b) Heavy water is used as moderator in preference to ordinary water because H may capture neutrons, while D does not
(c) Cadmium rods increase the reactor power when they go in, decrease when they go outward
(d) Slower neutrons are more effective in causing fission than faster neutrons in case of U²³⁵
Show Answer & Explanation
Answer: (c) Cadmium rods increase the reactor power when they go in, decrease when they go outward
Explanation:
1. Cadmium rods absorb neutrons.
2. Pushing them in decreases the chain reaction and the power, and pulling them out increases it, so statement 3 is reversed.
Teacher's Note:
1. Control rods absorb neutrons.
(a) 23 MeV
(b) 46 MeV
(c) 7.1 MeV
(d) 28.4 MeV
Show Answer & Explanation
Answer: (c) 7.1 MeV
Explanation:
1. \( B = 0.0305\times931.5 = 28.4 \) MeV.
2. Per nucleon \( = 28.4/4 = 7.1 \) MeV.
Teacher's Note:
1. Divide the total binding energy by \( A \).
(a) \( M(N,Z) = NM_n + ZM_p + Bc^2 \)
(b) \( M(N,Z) = NM_n + ZM_p + B/c^2 \)
(c) \( M(N,Z) = NM_n + ZM_p - B/c^2 \)
(d) \( M(N,Z) = NM_n + ZM_p - Bc^2 \)
Show Answer & Explanation
Answer: (c) \( M(N,Z) = NM_n + ZM_p - B/c^2 \)
Explanation:
1. The nucleus is lighter than its separated nucleons by the mass equivalent of the binding energy.
2. \( M = NM_n + ZM_p - B/c^2 \).
Teacher's Note:
1. Binding energy is released, so mass decreases.
(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. \( Q = (\text{BE of products}) - (\text{BE of reactants}) \).
2. The neutron has no binding energy: \( Q = c - (a + b) \).
Teacher's Note:
1. Energy released is the gain in total binding energy.
(a) neutron
(b) anti neutrino
(c) neutrino
(d) proton
Show Answer & Explanation
Answer: (b) anti neutrino
Explanation:
1. β⁻ decay always emits an antineutrino with the electron, to conserve lepton number and energy.
Teacher's Note:
1. β⁻ is accompanied by an antineutrino.
(a) 4.4 MeV
(b) 5.4 MeV
(c) 5.6 MeV
(d) 6.5 MeV
Show Answer & Explanation
Answer: (b) 5.4 MeV
Explanation:
1. Momentum conservation shares \( Q \) inversely as the masses.
2. \( K_\alpha = Q\times\dfrac{A-4}{A} = 5.5\times\dfrac{216}{220} = 5.4 \) MeV.
Teacher's Note:
1. The lighter particle takes the larger share.
(a) 20 MeV
(b) 16 MeV
(c) 8 MeV
(d) 1.6 MeV
Show Answer & Explanation
Answer: (b) 16 MeV
Explanation:
1. Binding energy of reactants \( = 2(1) + 7(5.5) = 40.5 \) MeV.
2. Products \( = 2\times4\times7 = 56 \) MeV.
3. Energy released \( = 56 - 40.5\approx16 \) MeV.
Teacher's Note:
1. Subtract total binding energies.
(a) \( \dfrac{A-Z-4}{Z-2} \)
(b) \( \dfrac{A-Z-8}{Z-4} \)
(c) \( \dfrac{A-Z-4}{Z-8} \)
(d) \( \dfrac{A-Z-12}{Z-4} \)
Show Answer & Explanation
Answer: (c) \( \dfrac{A-Z-4}{Z-8} \)
Explanation:
1. Mass number becomes \( A - 12 \). Atomic number becomes \( Z - 6 - 2 = Z - 8 \).
2. Neutrons \( = (A-12)-(Z-8) = A-Z-4 \).
3. Ratio \( = (A-Z-4)/(Z-8) \).
Teacher's Note:
1. Each positron lowers \( Z \) by 1.
(a) 120 MeV
(b) 220 MeV
(c) 240 MeV
(d) 180 MeV
Show Answer & Explanation
Answer: (a) 120 MeV
Explanation:
1. \( Q = (100+140)(8.1) - 240(7.6) \).
2. \( = 1944 - 1824 = 120 \) MeV.
Teacher's Note:
1. Gain in total binding energy.
(a) \( ^{89}_{26}Kr \)
(b) \( ^{89}_{36}Kr \)
(c) \( ^{90}_{26}Kr \)
(d) \( ^{89}_{36}Sr \)
Show Answer & Explanation
Answer: (b) \( ^{89}_{36}Kr \)
Explanation:
1. Mass number: \( 236 = 144 + A + 3 \), so \( A = 89 \).
2. Atomic number: \( 92 = 56 + Z \), so \( Z = 36 \), which is krypton.
Teacher's Note:
1. Balance \( A \) and \( Z \) separately.
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