Download JEE MCQs for JEE Physics: Dual Nature Of Radiation and Matter
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Chapter-wise Objective Questions: Dual Nature Of Radiation and Matter
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Multiple Choice Questions
(a) 1.8 eV
(b) 1.1 eV
(c) 0.8 eV
(d) 1.6 eV
Show Answer & Explanation
Answer: (b) 1.1 eV
Explanation:
1. Photon energy \( =13.6\left(\frac14-\frac19\right)=1.89\ \text{eV} \).
2. Fastest electron: \( p=eBr=1.6\times10^{-19}\times3\times10^{-4}\times10^{-2}=4.8\times10^{-25} \), so \( K=\frac{p^2}{2m}=1.27\times10^{-19}\ \text{J}=0.79\ \text{eV} \).
3. Work function \( =1.89-0.79\approx1.1\ \text{eV} \)
Teacher's Note:
1. The largest radius belongs to the electrons of maximum kinetic energy.
(a) \( \lambda/4 \)
(b) \( \lambda/6 \)
(c) \( 6\lambda \)
(d) \( 4\lambda \)
Show Answer & Explanation
Answer: (d) \( 4\lambda \)
Explanation:
1. \( 3eV_0=\frac{hc}\lambda-W,\quad eV_0=\frac{hc}{2\lambda}-W \); subtract: \( 2eV_0=\frac{hc}{2\lambda}\Rightarrow eV_0=\frac{hc}{4\lambda} \).
2. \( W=\frac{hc}{2\lambda}-\frac{hc}{4\lambda}=\frac{hc}{4\lambda}\Rightarrow\lambda_0=\frac{hc}{W}=4\lambda \)
Teacher's Note:
1. Eliminate the work function between the two equations to get it in terms of lambda.
Assertion (A): A metallic surface is irradiated by monochromatic light of frequency greater than the threshold frequency. The maximum kinetic energy and the stopping potential are \( K_{max} \) and \( V_0 \). If the frequency of the incident light is doubled, both \( K_{max} \) and \( V_0 \) are also doubled.
Reason (R): The maximum kinetic energy and stopping potential of photoelectrons emitted from a surface are linearly dependent on the frequency of the incident light.
(a) Both A and R are true, and R is the correct explanation of A.
(b) Both A and R are true, but R is not the correct explanation of A.
(c) A is true, but R is false.
(d) A is false, but R is true.
Show Answer & Explanation
Answer: (d) A is false, but R is true.
Explanation:
1. \( K_{max}=h\nu-W \) is linear in frequency but has an intercept, so it is not proportional to it.
2. Doubling the frequency gives \( 2h\nu-W\neq2(h\nu-W) \), so A is false; R is true.
Teacher's Note:
1. A linear relation with a non-zero intercept is not a proportion.
(a) 3.09 eV
(b) 1.42 eV
(c) 151 eV
(d) 1.68 eV
Show Answer & Explanation
Answer: (b) 1.42 eV
Explanation:
1. Photon energy \( =\frac{1240}{400}=3.10\ \text{eV} \).
2. \( W=3.10-1.68=1.42\ \text{eV} \)
Teacher's Note:
1. Work function equals photon energy minus the maximum kinetic energy.
(a) \( \frac{B^2}{2VE^2} \)
(b) \( \frac{2VB^2}{E^2} \)
(c) \( \frac{2VE^2}{B^2} \)
(d) \( \frac{E^2}{2VB^2} \)
Show Answer & Explanation
Answer: (d) \( \frac{E^2}{2VB^2} \)
Explanation:
1. No deflection: \( eE=evB\Rightarrow v=\frac EB \).
2. \( eV=\frac12mv^2\Rightarrow\frac em=\frac{v^2}{2V}=\frac{E^2}{2VB^2} \)
Teacher's Note:
1. Use the velocity selector condition together with energy gained in the accelerating potential.
(a) \( 5\times10^{16} \)
(b) \( 5\times10^{17} \)
(c) \( 5\times10^{14} \)
(d) \( 5\times10^{15} \)
Show Answer & Explanation
Answer: (d) \( 5\times10^{15} \)
Explanation:
1. \( n=\frac{P}{h\nu}=\frac{2\times10^{-3}}{6.63\times10^{-34}\times6\times10^{14}}\approx5\times10^{15} \)
Teacher's Note:
1. Photons per second equal the power divided by the energy of one photon.
(a) \( 2\times10^7 \) m/s
(b) \( 2\times10^6 \) m/s
(c) \( 8\times10^6 \) m/s
(d) \( 8\times10^5 \) m/s
Show Answer & Explanation
Answer: (c) \( 8\times10^6 \) m/s
Explanation:
1. First case: \( K_1=2h\nu_0-h\nu_0=h\nu_0 \); second: \( K_2=5h\nu_0-h\nu_0=4h\nu_0 \).
2. \( v\propto\sqrt K\Rightarrow v_2=2v_1=8\times10^6\ \text{m/s} \)
Teacher's Note:
1. Velocity scales as the square root of the maximum kinetic energy.
(a) less than \( v\sqrt{4/3} \)
(b) \( v\sqrt{3/4} \)
(c) \( v\sqrt{4/3} \)
(d) greater than \( v\sqrt{4/3} \)
Show Answer & Explanation
Answer: (d) greater than \( v\sqrt{4/3} \)
Explanation:
1. \( \frac12mv^2=\frac{hc}\lambda-W \); \( \frac12mv'^2=\frac{4hc}{3\lambda}-W=\frac43\cdot\frac12mv^2+\frac W3 \).
2. Since W > 0, \( v'^2>\frac43v^2 \), i.e. \( v'>v\sqrt{4/3} \).
Teacher's Note:
1. The work function does not scale with the photon energy, so the kinetic energy grows by more than the factor 4/3.
(a) Depends on the nature of the metal used
(b) Depends on the intensity of the radiation
(c) Depends both on the intensity of the radiation and the metal used
(d) Is the same for all metals and independent of the intensity of the radiation
Show Answer & Explanation
Answer: (d) Is the same for all metals and independent of the intensity of the radiation
Explanation:
1. \( K=h\nu-W \): slope = h, a universal constant.
Teacher's Note:
1. Different metals only shift the intercept.
(a) \( \sqrt{\frac{2eV}{m}} \)
(b) \( \sqrt{\frac{eV}{m}} \)
(c) \( \frac{eV}{2m} \)
(d) \( \frac{eV}{m} \)
Show Answer & Explanation
Answer: (a) \( \sqrt{\frac{2eV}{m}} \)
Explanation:
1. \( eV=\frac12mv^2\Rightarrow v=\sqrt{\frac{2eV}{m}} \)
Teacher's Note:
1. Work done by the field becomes kinetic energy.
(a) \( \lambda\frac Mm \)
(b) \( \lambda\frac mM \)
(c) \( \lambda\sqrt{\frac Mm} \)
(d) \( \lambda\sqrt{\frac mM} \)
Show Answer & Explanation
Answer: (d) \( \lambda\sqrt{\frac mM} \)
Explanation:
1. \( \lambda=\frac{h}{\sqrt{2mqV}}\propto\frac1{\sqrt m} \) for equal charge and voltage.
2. \( \lambda_p=\lambda\sqrt{\frac mM} \)
Teacher's Note:
1. Same charge and voltage give the same kinetic energy, so wavelength falls with the root of mass.
(a) \( 1.24\times10^{15} \)
(b) \( 2.4\times10^{20} \)
(c) \( 1.24\times10^{18} \)
(d) \( 2.4\times10^{23} \)
Show Answer & Explanation
Answer: (b) \( 2.4\times10^{20} \)
Explanation:
1. \( \nu=\frac Eh=\frac{10^6\times1.6\times10^{-19}}{6.63\times10^{-34}}\approx2.4\times10^{20}\ \text{Hz} \)
Teacher's Note:
1. Frequency is directly proportional to photon energy.
(a) 540 nm
(b) 400 nm
(c) 310 nm
(d) 220 nm
Show Answer & Explanation
Answer: (c) 310 nm
Explanation:
1. \( \lambda_{max}=\frac{1240}{4.0}=310\ \text{nm} \)
Teacher's Note:
1. The threshold wavelength is hc divided by the work function.
(a) 0.2 m
(b) 0.148 m
(c) 0.048 m
(d) 0.418 m
Show Answer & Explanation
Answer: (b) 0.148 m
Explanation:
1. Photon energy \( =\frac{1240}{180}=6.89\ \text{eV} \), so \( K=4.89\ \text{eV} \).
2. \( p=\sqrt{2mK}=1.19\times10^{-24} \), \( r=\frac{p}{eB}=\frac{1.19\times10^{-24}}{1.6\times10^{-19}\times5\times10^{-5}}\approx0.148\ \text{m} \)
Teacher's Note:
1. The electron moves perpendicular to the field, so it follows a circle of radius p/(eB).
(a) \( \frac h{mv} \)
(b) \( hmv \)
(c) \( \frac{mh}{v} \)
(d) \( \frac m{hv} \)
Show Answer & Explanation
Answer: (a) \( \frac h{mv} \)
Explanation:
1. \( \lambda=\frac hp=\frac h{mv} \)
Teacher's Note:
1. The de Broglie relation links wavelength and momentum.
(a) Ultra-violet region
(b) Infra-red region
(c) Visible region
(d) X-ray region
Show Answer & Explanation
Answer: (a) Ultra-violet region
Explanation:
1. Photon energy \( =6.2+5=11.2\ \text{eV} \).
2. \( \lambda=\frac{1240}{11.2}\approx110\ \text{nm} \), which lies in the ultraviolet.
Teacher's Note:
1. Add the stopping energy to the work function to get the photon energy.
(a) \( \frac{hc}{e}\left[\frac1{\lambda_3}+\frac1{\lambda_2}-\frac1{\lambda_1}\right] \)
(b) \( \frac{hc}{e}\left[\frac1{\lambda_3}+\frac1{2\lambda_2}-\frac1{\lambda_1}\right] \)
(c) \( \frac{hc}{e}\left[\frac1{\lambda_3}-\frac1{\lambda_2}-\frac1{\lambda_1}\right] \)
(d) \( \frac{hc}{e}\left[\frac1{\lambda_3}+\frac1{2\lambda_2}-\frac3{2\lambda_1}\right] \)
Show Answer & Explanation
Answer: (d) \( \frac{hc}{e}\left[\frac1{\lambda_3}+\frac1{2\lambda_2}-\frac3{2\lambda_1}\right] \)
Explanation:
1. \( eV=\frac{hc}{\lambda_1}-W,\ 3eV=\frac{hc}{\lambda_2}-W\Rightarrow eV=\frac{hc}2\left(\frac1{\lambda_2}-\frac1{\lambda_1}\right) \)
2. \( W=\frac{hc}{\lambda_1}-eV=hc\left(\frac3{2\lambda_1}-\frac1{2\lambda_2}\right) \)
3. \( V_3=\frac{hc}{e}\left[\frac1{\lambda_3}-\frac3{2\lambda_1}+\frac1{2\lambda_2}\right] \)
Teacher's Note:
1. Find the work function from the first two stopping potentials, then apply the equation to lambda 3.
(a) 0.5 angstrom
(b) 1.2 angstrom
(c) 1.7 angstrom
(d) 2.4 angstrom
Show Answer & Explanation
Answer: (c) 1.7 angstrom
Explanation:
1. \( \lambda=\frac{12.27}{\sqrt{50}}\ \text{angstrom}\approx1.7\ \text{angstrom} \)
Teacher's Note:
1. Use lambda = 12.27 / sqrt(V) angstrom for electrons.
(a) 1.0
(b) 1.6
(c) 2.8
(d) 4.1
Show Answer & Explanation
Answer: (b) 1.6
Explanation:
1. Photon energy \( =\frac{1240}{436}=2.84\ \text{eV} \).
2. Stopping potential \( =2.84-1.24=1.6\ \text{V} \)
Teacher's Note:
1. Stopping potential in volts equals the maximum kinetic energy in electron-volts.
(a) 1
(b) 2
(c) 3
(d) 4
Show Answer & Explanation
Answer: (b) 2
Explanation:
1. Kinetic energies: \( 1-0.5=0.5\ \text{eV} \) and \( 2.5-0.5=2\ \text{eV} \).
2. \( \frac{v_1}{v_2}=\sqrt{\frac{0.5}{2}}=\frac12 \), so n = 2.
Teacher's Note:
1. Speed varies as the square root of kinetic energy.
(a) 100
(b) 150
(c) 200
(d) 250
Show Answer & Explanation
Answer: (b) 150
Explanation:
1. \( \lambda=\frac{h}{\sqrt{2meV}}=\frac{12.27}{\sqrt V}\ \text{angstrom} \), so \( n=12.27^2\approx150 \)
Teacher's Note:
1. Square the numerical constant 12.27.
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