In the hydrogen atom, the energy of the electron in the \( n^{th} \) orbit is given by: \[ E_n = - \frac{13.6}{n^2} \text{ eV} \] The wavelength of the emitted photon when the electron transitions from an upper orbit \( n_2 \) to a lower orbit \( n_1 \) can be found using the relation: \[ E_{\text{photon}} = E_{n_2} - E_{n_1} \] The energy of the photon is related to the wavelength \( \lambda \) by the equation: \[ E_{\text{photon}} = \frac{hc}{\lambda} \] where \( h \) is Planck's constant and \( c \) is the speed of light. For the transition from the 3rd orbit to the 2nd orbit, the energy difference is: \[ \Delta E_{3 \rightarrow 2} = E_3 - E_2 = - \frac{13.6}{9} - \left( - \frac{13.6}{4} \right) = \frac{13.6}{4} - \frac{13.6}{9} \] The wavelength of the emitted photon for this transition is: \[ \lambda = \frac{hc}{\Delta E_{3 \rightarrow 2}} = \frac{5}{27} \cdot \lambda \] For the transition from the 2nd orbit to the 1st orbit, the energy difference is: \[ \Delta E_{2 \rightarrow 1} = E_2 - E_1 = - \frac{13.6}{4} - \left( - \frac{13.6}{1} \right) = \frac{13.6}{1} - \frac{13.6}{4} \] The wavelength of the emitted photon for this transition is: \[ \lambda_{\text{new}} = \frac{hc}{\Delta E_{2 \rightarrow 1}} = \frac{5}{27} \cdot \lambda \]
Thus, the wavelength of the photon emitted when the electron jumps from the second to the first orbit is \( \frac{5\lambda}{27} \).
List I (Spectral Lines of Hydrogen for transitions from) | List II (Wavelength (nm)) | ||
A. | n2 = 3 to n1 = 2 | I. | 410.2 |
B. | n2 = 4 to n1 = 2 | II. | 434.1 |
C. | n2 = 5 to n1 = 2 | III. | 656.3 |
D. | n2 = 6 to n1 = 2 | IV. | 486.1 |
The angular momentum of an electron in a stationary state of \(Li^{2+}\) (\(Z=3\)) is \( \frac{3h}{\pi} \). The radius and energy of that stationary state are respectively.
If the ratio of lengths, radii and Young's Moduli of steel and brass wires in the figure are $ a $, $ b $, and $ c $ respectively, then the corresponding ratio of increase in their lengths would be: