Physics Objective Questions and Answers: Atoms
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Multiple Choice Questions
(a) \( \dfrac{4\pi^2m}{h^3} \)
(b) \( \dfrac{h^2}{4\pi^2mr} \)
(c) \( \dfrac{h^2}{4\pi^2m^2r^3} \)
(d) \( \dfrac{m^2h^2}{4\pi^2r^3} \)
Show Answer & Explanation
Answer: (c) \( \dfrac{h^2}{4\pi^2m^2r^3} \)
Explanation:
1. Bohr's condition: \( mvr=\dfrac{h}{2\pi}\Rightarrow v=\dfrac{h}{2\pi mr} \). Then \( a=\dfrac{v^2}{r}=\dfrac{h^2}{4\pi^2m^2r^3} \).
Teacher's Note:
1. Centripetal acceleration is \( v^2/r \).
(a) 10.2 eV
(b) 12.1 eV
(c) 12.5 eV
(d) none of these
Show Answer & Explanation
Answer: (b) 12.1 eV
Explanation:
1. The atom gains \( E_3-E_1=-1.51-(-13.6)=12.1 \) eV.
Teacher's Note:
1. Energy absorbed equals the level gap.
(a) \( evr \)
(b) \( evr/2 \)
(c) \( \pi r^2ev \)
(d) \( 2\pi rev \)
Show Answer & Explanation
Answer: (b) \( evr/2 \)
Explanation:
1. \( I=\dfrac{ev}{2\pi r} \), \( M=IA=\dfrac{ev}{2\pi r}\pi r^2=\dfrac{evr}{2} \).
Teacher's Note:
1. Magnetic moment is current times area.
(a) \( n^3 \)
(b) \( n^{-3} \)
(c) \( n \)
(d) \( n^0 \)
Show Answer & Explanation
Answer: (b) \( n^{-3} \)
Explanation:
1. \( f=\dfrac{v}{2\pi r} \) with \( v\propto\dfrac1n \) and \( r\propto n^2 \), so \( f\propto n^{-3} \).
Teacher's Note:
1. Combine the n-dependence of v and r.
(a) 0
(b) 1
(c) \( -2 \)
(d) 2
Show Answer & Explanation
Answer: (a) 0
Explanation:
1. \( p\,L=(mv)(mvr)=m^2v^2r \). With \( v\propto n^{-1} \), \( r\propto n^2 \): \( v^2r\propto n^0 \), so \( x=0 \).
Teacher's Note:
1. Use \( v\propto1/n \) and \( r\propto n^2 \).
(a) \( n=2 \) to \( n=1 \)
(b) \( n=6 \) to \( n=1 \)
(c) \( n=3 \) to \( n=2 \)
(d) \( n=6 \) to \( n=2 \)
Show Answer & Explanation
Answer: (c) \( n=3 \) to \( n=2 \)
Explanation:
1. Balmer lines end on \( n=2 \); the longest wavelength is the smallest energy gap, \( 3\to2 \).
Teacher's Note:
1. Options (a) and (b) are not Balmer transitions.
(a) \( \tfrac12 \)
(b) \( \tfrac21 \)
(c) \( \tfrac54 \)
(d) \( \tfrac34 \)
Show Answer & Explanation
Answer: (d) \( \tfrac34 \)
Explanation:
1. \( \dfrac{n(n-1)}{2}=6\Rightarrow n=4 \); \( =3\Rightarrow n=3 \). Since \( v\propto\dfrac1n \), \( \dfrac{v_4}{v_3}=\dfrac34 \).
Teacher's Note:
1. Count the transitions from the top orbit.
(a) \( \nu_1-\nu_2=\nu_3 \)
(b) \( \nu_1=\nu_2-\nu_3 \)
(c) \( \dfrac1{\nu_2}=\dfrac1{\nu_1}+\dfrac1{\nu_3} \)
(d) \( \dfrac1{\nu_1}=\dfrac1{\nu_2}+\dfrac1{\nu_3} \)
Show Answer & Explanation
Answer: (a) \( \nu_1-\nu_2=\nu_3 \)
Explanation:
1. \( \nu_1=Rc \), \( \nu_2=\tfrac34Rc \), \( \nu_3=\tfrac14Rc \). So \( \nu_1-\nu_2=\tfrac14Rc=\nu_3 \).
Teacher's Note:
1. Write each in terms of \( Rc \).
(a) line emission spectrum
(b) continuous emission spectrum
(c) line absorption spectrum
(d) band emission spectrum
Show Answer & Explanation
Answer: (b) continuous emission spectrum
Explanation:
1. A hot incandescent flame with solid particles emits a continuous spectrum.
Teacher's Note:
1. Hot solids and liquids give continuous spectra.
(a) \( 6.95\times10^{14} \) Hz
(b) \( 3.68\times10^{15} \) Hz
(c) \( 5.5\times10^{14} \) Hz
(d) \( 9.11\times10^{15} \) Hz
Show Answer & Explanation
Answer: (c) \( 5.5\times10^{14} \) Hz
Explanation:
1. \( \nu=\dfrac{E}{h}=\dfrac{2.3\times1.6\times10^{-19}}{6.63\times10^{-34}}=5.5\times10^{14} \) Hz.
Teacher's Note:
1. Convert eV to joule.
(a) \( n=1 \) to \( n=2 \)
(b) \( n=2 \) to \( n=1 \)
(c) \( n=3 \) to \( n=10 \)
(d) \( n=10 \) to \( n=3 \)
Show Answer & Explanation
Answer: (b) \( n=2 \) to \( n=1 \)
Explanation:
1. Emission means falling to a lower level, so (a) and (c) are out. \( 2\to1 \) releases 10.2 eV and \( 10\to3 \) only about 1.4 eV.
Teacher's Note:
1. Highest frequency means largest energy released.
(a) \( n\pi \)
(b) \( 2\pi h \)
(c) \( \dfrac{2h}{\pi} \)
(d) \( \dfrac h\pi \)
Show Answer & Explanation
Answer: (d) \( \dfrac h\pi \)
Explanation:
1. The moment of linear momentum is angular momentum \( \dfrac{nh}{2\pi}=\dfrac{2h}{2\pi}=\dfrac h\pi \).
Teacher's Note:
1. Angular momentum is quantised.
(a) 13.6 eV
(b) 27.2 eV
(c) 54.4 eV
(d) 68.0 eV
Show Answer & Explanation
Answer: (c) 54.4 eV
Explanation:
1. \( E=13.6\,Z^2/n^2 \) with \( Z=2 \), \( n=1 \): 54.4 eV.
Teacher's Note:
1. The minimum position is the ground state.
(a) \( n=2\) to \( n=1 \)
(b) \( n=3\) to \( n=1 \)
(c) \( n=3\) to \( n=2 \)
(d) \( n=4\) to \( n=3 \)
Show Answer & Explanation
Answer: (d) \( n=4\) to \( n=3 \)
Explanation:
1. Gap sizes: 10.2, 12.1, 1.89 and 0.66 eV respectively, so \( 4\to3 \) is smallest.
Teacher's Note:
1. Minimum frequency needs the smallest energy gap.
(a) \( \dfrac{16}{25}\lambda_0 \)
(b) \( \dfrac{20}{27}\lambda_0 \)
(c) \( \dfrac{27}{20}\lambda_0 \)
(d) \( \dfrac{25}{16}\lambda_0 \)
Show Answer & Explanation
Answer: (b) \( \dfrac{20}{27}\lambda_0 \)
Explanation:
1. \( \dfrac1{\lambda_0}=R\left(\tfrac14-\tfrac19\right)=\dfrac{5R}{36} \), \( \dfrac1{\lambda}=R\left(\tfrac14-\tfrac1{16}\right)=\dfrac{3R}{16} \). \( \dfrac{\lambda}{\lambda_0}=\dfrac{5/36}{3/16}=\dfrac{20}{27} \).
Teacher's Note:
1. Use the Rydberg formula for both jumps.
(a) \( \dfrac n{2\pi} \)
(b) \( \dfrac{n^2}{2\pi} \)
(c) \( \dfrac1{2\pi n} \)
(d) \( \dfrac1{2\pi n^2} \)
Show Answer & Explanation
Answer: (a) \( \dfrac n{2\pi} \)
Explanation:
1. Bohr's condition gives \( 2\pi r=n\lambda \), so \( \dfrac r\lambda=\dfrac n{2\pi} \).
Teacher's Note:
1. The orbit holds n de Broglie wavelengths.
(a) I, III, IV are correct
(b) only I is correct
(c) I and II are correct
(d) only III is correct
Show Answer & Explanation
Answer: (a) I, III, IV are correct
Explanation:
1. \( v\propto1/n \) (I true), \( r\propto n^2 \) (II false), \( KE\propto1/n^2 \) (III true), \( L=nh/2\pi \) (IV true).
Teacher's Note:
1. Radius goes as \( n^2 \), not n.
(a) 1000 \( \text{\AA} \)
(b) 800 \( \text{\AA} \)
(c) 1300 \( \text{\AA} \)
(d) 2100 \( \text{\AA} \)
Show Answer & Explanation
Answer: (a) 1000 \( \text{\AA} \)
Explanation:
1. The shortest wavelength is the Lyman limit: \( \lambda=\dfrac1R=10^{-7} \) m \( =1000 \) \( \text{\AA} \).
Teacher's Note:
1. Series limit of Lyman is \( 1/R \).
(a) \( 1\times10^{-15} \)
(b) \( 1\times10^{-10} \)
(c) \( 1\times10^{-23} \)
(d) \( 1\times10^{-27} \)
Show Answer & Explanation
Answer: (c) \( 1\times10^{-23} \)
Explanation:
1. \( I=ef=1.6\times10^{-19}\times6.6\times10^{15}=1.06\times10^{-3} \) A. \( M=I\pi r^2=1.06\times10^{-3}\times\pi\times(0.528\times10^{-10})^2\approx9\times10^{-24}\approx10^{-23} \) A m\(^2\).
Teacher's Note:
1. Magnetic moment is current times loop area.
(a) \( n=4 \)
(b) \( n=2 \)
(c) \( n=16 \)
(d) \( n=3 \)
Show Answer & Explanation
Answer: (b) \( n=2 \)
Explanation:
1. \( r\propto n^2 \): \( n^2=\dfrac{21.2}{5.3}=4 \Rightarrow n=2 \).
Teacher's Note:
1. Radius scales as \( n^2 \).
(a) \( 2.188\times10^6 \) m s\(^{-1}\)
(b) \( 1.094\times10^6 \) m s\(^{-1}\)
(c) \( 4.376\times10^6 \) m s\(^{-1}\)
(d) \( 1.59\times10^6 \) m s\(^{-1}\)
Show Answer & Explanation
Answer: (d) \( 1.59\times10^6 \) m s\(^{-1}\)
Explanation:
1. The ground orbit has \( r_1=0.529 \) \( \text{\AA} \) and \( v_1=2.188\times10^6 \) m s\(^{-1}\). For Coulomb motion \( v\propto r^{-1/2} \): \( v=2.188\times10^6\sqrt{0.529/1}=1.59\times10^6 \) m s\(^{-1}\).
Teacher's Note:
1. For circular Coulomb orbits \( v^2\propto1/r \).
(a) \( \sqrt{\dfrac{\lambda R}{\lambda R-1}} \)
(b) \( \sqrt{\dfrac{\lambda}{\lambda R-1}} \)
(c) \( \sqrt{\dfrac{\lambda R^2}{\lambda R-1}} \)
(d) \( \sqrt{\dfrac{\lambda R}{\lambda-1}} \)
Show Answer & Explanation
Answer: (a) \( \sqrt{\dfrac{\lambda R}{\lambda R-1}} \)
Explanation:
1. \( \dfrac1\lambda=R\left(1-\dfrac1{n^2}\right)\Rightarrow\dfrac1{n^2}=\dfrac{\lambda R-1}{\lambda R}\Rightarrow n=\sqrt{\dfrac{\lambda R}{\lambda R-1}} \).
Teacher's Note:
1. Solve the Rydberg formula for n.
(a) incandescent electric lamp
(b) mercury vapour lamp
(c) sodium vapour lamp
(d) polyatomic substances
Show Answer & Explanation
Answer: (a) incandescent electric lamp
Explanation:
1. A glowing solid filament emits all wavelengths, a continuous spectrum; vapour lamps give line spectra.
Teacher's Note:
1. Hot solids give continuous spectra.
(a) 4:1
(b) 16:1
(c) 8:1
(d) 2:1
Show Answer & Explanation
Answer: (b) 16:1
Explanation:
1. Area \( \propto r^2\propto n^4 \): \( \dfrac{2^4}{1^4}=16 \).
Teacher's Note:
1. The first excited state has \( n=2 \).
(a) infinite energy
(b) maximum energy
(c) minimum energy
(d) zero energy
Show Answer & Explanation
Answer: (c) minimum energy
Explanation:
1. The \( n=1 \) orbit has the most negative energy (\( -13.6 \) eV), the minimum energy.
Teacher's Note:
1. Energy rises towards zero as n increases.
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FAQs
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