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NCERT Solutions · Class 12 Physics Atoms

9 exercises · 3 still being checked

Exercises 12.1–12.9

  1. Exercise 12.1

    Choose the correct alternative from the clues given at the end of the each statement:
    (a)
    The size of the atom in Thomson’s model is .......... the atomic size in Rutherford’s model. (much greater than/no different from/much less than.)
    (b)
    In the ground state of .......... electrons are in stable equilibrium, while in .......... electrons always experience a net force. (Thomson’s model/ Rutherford’s model.)
    (c)
    A classical atom based on .......... is doomed to collapse. (Thomson’s model/ Rutherford’s model.)
    (d)
    An atom has a nearly continuous mass distribution in a .......... but has a highly non-uniform mass distribution in .......... (Thomson’s model/ Rutherford’s model.)
    (e)
    The positively charged part of the atom possesses most of the mass in .......... (Rutherford’s model/both the models.)

    Not cross-checked

    NCERT prints no numerical answer for this exercise, so this working has not been cross-checked against the book.

    NCERT’s answer
    (a)
    No different from (b) Thomson’s model; Rutherford’s model (c) Rutherford’s model (d) Thomson’s model; Rutherford’s model (e) Both the models
    NCERT_Solution_Class12_Physics_Ch12_Q12-1
    Compare the two models directly.
    (a)
    The size of the atom in Thomson's model is no different from the atomic size in Rutherford's model — Thomson's model too gives an atom of radius \(\displaystyle \sim 10^{-10}\,\mathrm{m}\); what differs is the mass/charge distribution inside that volume, not the volume itself.
    (b)
    In the ground state of Thomson's model, electrons sit in stable equilibrium (embedded in the uniform positive sphere, restoring force present). In Rutherford's model, electrons orbiting a point nucleus always experience a net (centripetal) force — there is no static equilibrium position.
    (c)
    A classical atom based on Rutherford's model is doomed to collapse: an orbiting (hence accelerating) electron must radiate energy continuously by classical electromagnetism, spiralling into the nucleus.
    (d)
    An atom has a nearly continuous mass distribution in Thomson's model (positive charge/mass spread over the whole sphere), but a highly non-uniform mass distribution in Rutherford's model (almost all mass concentrated in the tiny central nucleus).
    (e)
    The positively charged part of the atom possesses most of the mass in both the models — in Thomson's model the massive positive sphere carries the charge, and in Rutherford's model the massive nucleus carries the positive charge; in each case the light electrons contribute negligible mass.
  2. Exercise 12.2

    Suppose you are given a chance to repeat the alpha-particle scattering experiment using a thin sheet of solid hydrogen in place of the gold foil. (Hydrogen is a solid at temperatures below $\displaystyle 14$ K.) What results do you expect?

    Disagrees with the book

    This working does not reach the answer printed in NCERT. One of the two is wrong and it has not yet been settled which — check it before you rely on it.

    NCERT’s answer
    The nucleus of a hydrogen atom is a proton. The mass of it is $\displaystyle 1.67$ × \(\displaystyle 10^{-27}\) kg, whereas the mass of an incident α-particle is $\displaystyle 6.64$ × \(\displaystyle 10^{-27}\) kg. Because the scattering particle is more massive than the target nuclei (proton), the α-particle won’t bounce back in even in a head-on collision. It is similar to a football colliding with a tenis ball at rest. Thus, there would be no large-angle scattering.
    NCERT_Solution_Class12_Physics_Ch12_Q12-2In Rutherford scattering, the projectile (\(\displaystyle \alpha\)-particle, mass \(\displaystyle \approx 4\,\mathrm{u}\)) is being fired at a target nucleus. For a fixed target that is lighter than the projectile, conservation of momentum caps the maximum possible deflection angle \(\displaystyle \theta_{\max}\), given by \[\sin\theta_{\max}=\frac{m_{\text{target}}}{m_{\text{projectile}}} \]For a hydrogen target, \(\displaystyle m_{\text{target}}\approx 1\,\mathrm{u}\) and \(\displaystyle m_{\text{projectile}}\approx 4\,\mathrm{u}\) (an \(\displaystyle \alpha\)-particle), so \[\sin\theta_{\max}=\frac{1}{4}=0.25 \;\Rightarrow\; \theta_{\max}\approx 14.5^{\circ} \]So, unlike gold (mass \(\displaystyle \approx 197\,\mathrm{u}\), much heavier than the \(\displaystyle \alpha\)-particle), which can send an \(\displaystyle \alpha\)-particle back at large angles including near \(\displaystyle 180^{\circ}\), a solid-hydrogen target — being lighter than the \(\displaystyle \alpha\)-particle — cannot produce any large-angle or back-scattering at all. The alpha particles would pass through the hydrogen sheet with only small deflections (at most \(\displaystyle \sim 14.5^{\circ}\)); no large-angle scattering would be seen, and this experiment could not be used to establish the existence of a small, massive nucleus in hydrogen the way the gold-foil experiment did.
  3. Exercise 12.3

    A difference of $\displaystyle 2.3$ eV separates two energy levels in an atom. What is the frequency of radiation emitted when the atom make a transition from the upper level to the lower level?
    NCERT’s answer
    5.$\displaystyle 6$ × \(\displaystyle 10^{14}\) Hz
    Photon energy equals the level spacing: \(\displaystyle \Delta E = h\nu\).\[\Delta E = 2.3\,\mathrm{eV} = 2.3 \times 1.6\times10^{-19}\,\mathrm{J} = 3.68\times10^{-19}\,\mathrm{J} \]\[\nu = \frac{\Delta E}{h} = \frac{3.68\times10^{-19}\,\mathrm{J}}{6.63\times10^{-34}\,\mathrm{J\,s}} \]\(\displaystyle \nu \approx 5.55\times10^{14}\,\mathrm{Hz}\), emitted as the atom drops from the upper to the lower level.
  4. Exercise 12.4

    The ground state energy of hydrogen atom is -$\displaystyle 13.6$ eV. What are the kinetic and potential energies of the electron in this state?
    NCERT’s answer
    13.$\displaystyle 6$ eV; -$\displaystyle 27.2$ eV
    For an electron bound by the Coulomb (inverse-square) force, the virial theorem gives \(\displaystyle PE = -2\,KE\), so the total energy \(\displaystyle E = KE + PE = KE - 2KE = -KE\).Given \(\displaystyle E = -13.6\,\mathrm{eV}\):\[KE = -E = -(-13.6\,\mathrm{eV}) = 13.6\,\mathrm{eV} \] \[PE = 2E = 2(-13.6\,\mathrm{eV}) = -27.2\,\mathrm{eV} \]Kinetic energy \(\displaystyle = +13.6\,\mathrm{eV}\), Potential energy \(\displaystyle = -27.2\,\mathrm{eV}\) (their sum reproduces \(\displaystyle E=-13.6\,\mathrm{eV}\)).
  5. Exercise 12.5

    A hydrogen atom initially in the ground level absorbs a photon, which excites it to the n = $\displaystyle 4$ level. Determine the wavelength and frequency of photon.

    Disagrees with the book

    This working does not reach the answer printed in NCERT. One of the two is wrong and it has not yet been settled which — check it before you rely on it.

    NCERT’s answer
    9.$\displaystyle 7$ × $\displaystyle 10$ - $\displaystyle 8$ m; $\displaystyle 3.1$ × \(\displaystyle 10^{15}\) Hz.
    Hydrogen energy levels: \(\displaystyle E_n = -\dfrac{13.6}{n^2}\,\mathrm{eV}\).\[E_1 = -13.6\,\mathrm{eV}, \qquad E_4 = -\frac{13.6}{16} = -0.85\,\mathrm{eV} \]Energy absorbed by the photon: \[\Delta E = E_4 - E_1 = -0.85-(-13.6) = 12.75\,\mathrm{eV} = 12.75\times1.6\times10^{-19}\,\mathrm{J} = 2.04\times10^{-18}\,\mathrm{J} \]Wavelength, from \(\displaystyle \Delta E = hc/\lambda\): \[\lambda = \frac{hc}{\Delta E} = \frac{(6.63\times10^{-34})(3\times10^{8})}{2.04\times10^{-18}\,\mathrm{J}} = 9.75\times10^{-8}\,\mathrm{m} \]Frequency: \[\nu = \frac{c}{\lambda} = \frac{3\times10^{8}}{9.75\times10^{-8}} \]\(\displaystyle \lambda \approx 97.5\,\mathrm{nm}\) (in the ultraviolet), \(\displaystyle \nu \approx 3.08\times10^{15}\,\mathrm{Hz}\).
  6. Exercise 12.6

    (a)
    Using the Bohr’s model calculate the speed of the electron in a hydrogen atom in the n = $\displaystyle 1$, $\displaystyle 2$, and $\displaystyle 3$ levels.
    (b)
    Calculate the orbital period in each of these levels.
    NCERT’s answer
    (a)
    2.$\displaystyle 18$ × \(\displaystyle 10^{6}\) m/s; $\displaystyle 1.09$ × \(\displaystyle 10^{6}\) m/s; $\displaystyle 7.27$ × \(\displaystyle 10^{5}\) m/s (b) $\displaystyle 1.52$ × \(\displaystyle 10^{-16}\) s; $\displaystyle 1.22$ × \(\displaystyle 10^{-15}\) s; $\displaystyle 4.11$ × \(\displaystyle 10^{-15}\) s.
    (a) Orbital speed. Equate the Coulomb force to the centripetal requirement, \(\displaystyle \dfrac{e^2}{4\pi\epsilon_0 r^2}=\dfrac{mv^2}{r}\), together with Bohr's quantization \(\displaystyle mvr=\dfrac{nh}{2\pi}\). Eliminating \(\displaystyle r\) gives \[v_n = \frac{e^2}{2\epsilon_0 h}\cdot\frac{1}{n} \]\[v_n=\frac{(1.6\times10^{-19})^2}{2(8.854\times10^{-12})(6.63\times10^{-34})}\cdot\frac{1}{n}=\frac{2.18\times10^{6}}{n}\ \mathrm{m/s} \]\[v_1 \approx 2.18\times10^{6}\,\mathrm{m/s},\quad v_2 \approx 1.09\times10^{6}\,\mathrm{m/s},\quad v_3 \approx 7.27\times10^{5}\,\mathrm{m/s} \](b) Orbital period. The Bohr radius is \(\displaystyle r_n = n^2 a_0\) with \[a_0=\frac{\epsilon_0 h^2}{\pi m_e e^2}=\frac{(8.854\times10^{-12})(6.63\times10^{-34})^2}{\pi(9.11\times10^{-31})(1.6\times10^{-19})^2}\approx 5.3\times10^{-11}\,\mathrm{m} \] so \(\displaystyle r_1=5.3\times10^{-11}\,\mathrm{m}\), \(\displaystyle r_2=4r_1=2.12\times10^{-10}\,\mathrm{m}\), \(\displaystyle r_3=9r_1=4.77\times10^{-10}\,\mathrm{m}\).Period \(\displaystyle T_n = \dfrac{2\pi r_n}{v_n}\). Since \(\displaystyle r_n\propto n^2\) and \(\displaystyle v_n\propto 1/n\), \(\displaystyle T_n \propto n^3\), so it suffices to get \(\displaystyle T_1\) and scale: \[T_1=\frac{2\pi(5.3\times10^{-11})}{2.18\times10^{6}}\approx1.53\times10^{-16}\,\mathrm{s} \]\(\displaystyle T_1\approx1.53\times10^{-16}\,\mathrm{s}\), \(\displaystyle T_2=8T_1\approx1.22\times10^{-15}\,\mathrm{s}\), \(\displaystyle T_3=27T_1\approx4.13\times10^{-15}\,\mathrm{s}\).
  7. Exercise 12.7

    The radius of the innermost electron orbit of a hydrogen atom is $\displaystyle 5.3$×\(\displaystyle 10^{-11}\) m. What are the radii of the n = $\displaystyle 2$ and n =$\displaystyle 3$ orbits?
    NCERT’s answer
    2.$\displaystyle 12$×\(\displaystyle 10^{-10}\) m; $\displaystyle 4.77$ × \(\displaystyle 10^{-10}\) m
    Bohr radii scale as \(\displaystyle r_n = n^2 r_1\), with \(\displaystyle r_1 = 5.3\times10^{-11}\,\mathrm{m}\) given.\[r_2 = 2^2 r_1 = 4(5.3\times10^{-11}\,\mathrm{m}) = 2.12\times10^{-10}\,\mathrm{m} \] \[r_3 = 3^2 r_1 = 9(5.3\times10^{-11}\,\mathrm{m}) = 4.77\times10^{-10}\,\mathrm{m} \]\(\displaystyle r_2 \approx 2.12\times10^{-10}\,\mathrm{m}\), \(\displaystyle r_3 \approx 4.77\times10^{-10}\,\mathrm{m}\).
  8. Exercise 12.8

    A $\displaystyle 12.5$ eV electron beam is used to bombard gaseous hydrogen at room temperature. What series of wavelengths will be emitted?
    NCERT’s answer
    Lyman series: $\displaystyle 103$ nm and $\displaystyle 122$ nm; Balmer series: $\displaystyle 656$ nm.
    NCERT_Solution_Class12_Physics_Ch12_Q12-8Ground-state hydrogen has \(\displaystyle E_1=-13.6\,\mathrm{eV}\). In an inelastic collision the bombarding electron (energy \(\displaystyle 12.5\,\mathrm{eV}\)) can transfer at most \(\displaystyle 12.5\,\mathrm{eV}\) to the atom. Check which excited levels \(\displaystyle E_n=-13.6/n^2\,\mathrm{eV}\) are reachable, i.e. for which \(\displaystyle E_n-E_1\le 12.5\,\mathrm{eV}\):\[E_2-E_1 = -3.4-(-13.6)=10.2\,\mathrm{eV}\ \ (\text{reachable}) \] \[E_3-E_1 = -1.51-(-13.6)=12.09\,\mathrm{eV}\ \ (\text{reachable, }\le12.5\,\mathrm{eV}) \] \[E_4-E_1 = -0.85-(-13.6)=12.75\,\mathrm{eV}\ \ (\text{NOT reachable, exceeds }12.5\,\mathrm{eV}) \]So the electron beam can excite the atom up to \(\displaystyle n=3\) only. On de-excitation, the atom can emit the three transitions \(\displaystyle 3\to1\), \(\displaystyle 3\to2\), and \(\displaystyle 2\to1\), using \(\displaystyle \lambda = hc/\Delta E\) with \(\displaystyle hc\approx1243\,\mathrm{eV\,nm}\):\[\lambda_{3\to1}=\frac{1243}{12.09}\approx102.8\,\mathrm{nm}\ (\text{Lyman}) \] \[\lambda_{2\to1}=\frac{1243}{10.2}\approx121.9\,\mathrm{nm}\ (\text{Lyman}) \] \[\lambda_{3\to2}=\frac{1243}{1.89}\approx658\,\mathrm{nm}\ (\text{Balmer}) \]Two Lyman-series lines (\(\displaystyle \lambda\approx102.8\,\mathrm{nm}\) and \(\displaystyle 121.9\,\mathrm{nm}\), from \(\displaystyle 3\to1\) and \(\displaystyle 2\to1\)) and one Balmer-series line (\(\displaystyle \lambda\approx658\,\mathrm{nm}\), from \(\displaystyle 3\to2\)) are emitted; transitions to \(\displaystyle n=4\) or beyond do not occur since that would require more than \(\displaystyle 12.5\,\mathrm{eV}\).
  9. Exercise 12.9

    In accordance with the Bohr’s model, find the quantum number that characterises the earth’s revolution around the sun in an orbit of radius $\displaystyle 1.5$ × \(\displaystyle 10^{11}\) m with orbital speed $\displaystyle 3$ × \(\displaystyle 10^{4}\) m/s. (Mass of earth = $\displaystyle 6.0$ × \(\displaystyle 10^{24}\) kg.)
    NCERT’s answer
    2.$\displaystyle 6$ × \(\displaystyle 10^{74}\)
    Bohr's quantization condition: angular momentum \(\displaystyle mvr = \dfrac{nh}{2\pi}\), so \[n=\frac{2\pi m v r}{h} \]With \(\displaystyle m=6.0\times10^{24}\,\mathrm{kg}\), \(\displaystyle v=3\times10^{4}\,\mathrm{m/s}\), \(\displaystyle r=1.5\times10^{11}\,\mathrm{m}\):\[n=\frac{2\pi(6.0\times10^{24})(3\times10^{4})(1.5\times10^{11})}{6.63\times10^{-34}} \]\[n=\frac{1.696\times10^{41}}{6.63\times10^{-34}} \]\(\displaystyle n \approx 2.6\times10^{74}\) — an enormous quantum number, showing why the earth's orbit (a macroscopic, essentially continuous system) shows no observable quantization; Bohr's quantum condition reduces to classical mechanics for such large \(\displaystyle n\) (Bohr's correspondence principle).