To determine the relationship between the energy of Lyman series lines (L$_1$) and Balmer series lines (B$_1$) in the hydrogen spectrum, we utilize the formula for the energy of a photon emitted due to an electron transition:
E = hν = 13.6 eV (1/n$_1^2$ - 1/n$_2^2$), where $n_1$ and $n_2$ are principal quantum numbers with $n_2 > n_1$.
The transition in Lyman series is from $n_2$ to $n_1 = 1$, and for L$_1$, $n_2 = 2$. For Balmer series, the transition is from $n_2$ to $n_1 = 2$, and for B$_1$, $n_2 = 3$.
Calculating the energy difference for L$_1$:
E$_{L_1}$ = 13.6 eV (1/1² - 1/2²) = 13.6 eV (1 - 1/4) = 13.6 eV × 3/4 = 10.2 eV.
Calculating the energy difference for B$_1$:
E$_{B_1}$ = 13.6 eV (1/2² - 1/3²) = 13.6 eV (1/4 - 1/9).
Simplifying:
E$_{B_1}$ = 13.6 eV × (5/36) = 1.89 eV.
Now, find $x$:
$x = \frac{E_{L_1}}{E_{B_1}} = \frac{10.2}{1.89} ≈ 5.40$.
The required answer is $x \space \times \space 10^{-1} = 54$ (nearest integer).
The wavelength of spectral line obtained in the spectrum of Li$^{2+}$ ion, when the transition takes place between two levels whose sum is 4 and difference is 2, is
Spherical node shown in figure-1 is best represented by which point in figure-2. 