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Atomic and Molecular Physics Questions and Answers

1.

Different spectral lines of the Balmer series (transitions \(n \rightarrow 2\), with \(n\) being the principal quantum number) fall one at a time on a Young’s double slit apparatus. The separation between the slits is \(d\) and the screen is placed at a constant distance from the slits. What factor should \(d\) be multiplied by to maintain a constant fringe width for various lines, as \(n\) takes different allowed values?

Exam Year(s)

GATE Physics - 2023,

Answer: C

The factor is \(\frac{4n^{2}}{n^{2} - 4}\), up to a constant.

The fringe width is \(\beta = \lambda D/d\). With the screen distance fixed, keeping \(\beta\) constant requires \(d \propto \lambda\). For the Balmer series,

\[ \begin{aligned} \frac{1}{\lambda} &= R\left(\frac{1}{4} - \frac{1}{n^{2}}\right) = R\,\frac{n^{2} - 4}{4n^{2}} \\ \lambda &= \frac{1}{R} \cdot \frac{4n^{2}}{n^{2} - 4} \end{aligned} \]

so \(d\) must be scaled by \(4n^{2}/(n^{2} - 4)\). The option \((n^{2} - 4)/4n^{2}\) is proportional to \(1/\lambda\), the inverse of what is needed, and the forms with \(n^{2} + 4\) do not come from the Rydberg formula.

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2.

The screened nuclear charge of neutral Helium atom is given as \(1.7 e\), where \(e\) is the magnitude of the electronic charge. Assuming the Bohr model of the atom for which the energy levels are \(E_{n} = -\frac{Z^{2}}{2}\frac{1}{n^{2}}\) atomic units (\(Z\) is the atomic number), the first ionization potential of Helium in atomic units is

Exam Year(s)

GATE Physics - 2025,

Answer: A

The first ionization potential is 0.89 atomic units.

In neutral helium each electron sees the screened charge \(Z = 1.7\), so with both in \(n = 1\) the atom's energy is

\[ \begin{aligned} E_{\text{He}} &= 2 \times \left(-\frac{1.7^{2}}{2}\right) \\ &= -2.89 \end{aligned} \]

After one electron is removed, the remaining electron in He+ sees the full nuclear charge \(Z = 2\):

\[ \begin{aligned} E_{\text{He}^{+}} &= -\frac{2^{2}}{2} = -2 \\ \text{IP} &= -2 - (-2.89) = 0.89 \end{aligned} \]

0.89 a.u. is about 24.2 eV, close to the measured 24.6 eV. 1.78 doubles the answer, and 1.445 (\(1.7^{2}/2\)) would be the result of removing one screened electron without letting the other relax, which is not offered.

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3.

The shortest wavelength observed in Paschen back series of hydrogen spectra is (RH = 10967757·6 m−1)

Exam Year(s)

MH SET - 2018, SET Exam - 2018,

Answer: D

The shortest wavelength is 8205 Å (the paper's 'Paschen back series' means the Paschen series).

Paschen lines end on \( n = 3 \). The shortest wavelength is the series limit, an electron falling from \( n = \infty \):

\[ \begin{aligned} \frac{1}{\lambda} &= R_{H}\left(\frac{1}{3^{2}} - 0\right) \\ \lambda &= \frac{9}{10967757.6}\ \text{m} \approx 8206\ \text{\AA} \end{aligned} \]

The option gives this limit as 8205 Å. 7800 Å and 7349 Å are shorter than the limit, so they cannot be Paschen lines at all, and 9546 Å, longer than the limit, belongs to a transition from a finite upper level, not the shortest line.

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Tags: Hydrogen Atom Spectra Questions and Answers