| 1. | \(\dfrac{1}{\sqrt{m}}\) | 2. | \(\dfrac{1}{m^{2}}\) |
| 3. | \(m\) | 4. | \(\dfrac{1}{m}\) |
In the spectrum of hydrogen, the ratio of the longest wavelength in the Lyman series to the longest wavelength in the Balmer series is:
| 1. | \(\frac{4}{9}\) | 2. | \(\frac{9}{4}\) |
| 3. | \(\frac{27}{5}\) | 4. | \(\frac{5}{27}\) |
Consider \(3^{\text{rd}}\) orbit of \(He^{+}\) (Helium). Using a non-relativistic approach, the speed of the electron in this orbit will be: (given \(Z=2\) and \(h\) (Planck's constant)\(= 6.6\times10^{-34}~\text{J-s}\))
1. \(2.92\times 10^{6}~\text{m/s}\)
2. \(1.46\times 10^{6}~\text{m/s}\)
3. \(0.73\times 10^{6}~\text{m/s}\)
4. \(3.0\times 10^{8}~\text{m/s}\)
The hydrogen gas with its atoms in the ground state is excited by monochromatic radiation of \(\lambda = 975~\mathring{{A}}.\) The number of spectral lines in the resulting spectrum emitted will be:
1. \(3\)
2. \(2\)
3. \(6\)
4. \(10\)
| 1. | \(\dfrac{3}{23}\) | 2. | \(\dfrac{7}{29}\) |
| 3. | \(\dfrac{9}{31}\) | 4. | \(\dfrac{5}{27}\) |
| 1. | \(\dfrac{7}{5}\) | 2. | \(\dfrac{20}{7}\) |
| 3. | \(\dfrac{27}{5}\) | 4. | \(\dfrac{27}{20}\) |
| 1. | \(\dfrac{24m}{25hR}\) | 2. | \(\dfrac{25hR}{24m}\) |
| 3. | \(\dfrac{25m}{24hR}\) | 4. | \(\dfrac{24hR}{25m}\) |
The energy of a hydrogen atom in the ground state is \(-13.6\) eV. The energy of a \(\mathrm{He}^{+}\) ion in the first excited state will be:
1. \(-13.6\) eV
2. \(-27.2\) eV
3. \(-54.4\) eV
4. \(-6.8\) eV
| 1. | \(\frac{1}{Ze} \) | 2. | \(v^2 \) |
| 3. | \(\frac{1}{m} \) | 4. | \(\frac{1}{v^4}\) |