The refractive index is given by:
\(n(\lambda) = n_0 + \frac{a}{\lambda^2} - \frac{b}{\lambda^4}\)
The phase velocity (\(v_p\)) is given by:
\(v_p = \frac{c}{n(\lambda)}\)
The group velocity (\(v_g\)) is given by:
\(v_g = \frac{d\omega}{dk}\)
Using the relation \(v_g = c / (n - \lambda \frac{dn}{d\lambda})\), we compute \(\frac{dn}{d\lambda}\):
\(\frac{dn}{d\lambda} = -\frac{2a}{\lambda^3} + \frac{4b}{\lambda^5}\)
Equating \(v_g = v_p\), we find:
\(n(\lambda) = n(\lambda) - \lambda \frac{dn}{d\lambda}\)
Simplifying gives:
\(-\lambda \frac{dn}{d\lambda} = 0\)
Substitute \(\frac{dn}{d\lambda}\):
\(-\lambda \left(-\frac{2a}{\lambda^3} + \frac{4b}{\lambda^5}\right) = 0\)
Simplify further:
\(\frac{2a}{\lambda^2} = \frac{2a}{\lambda^2}\)
Therefore, we find:
\(\lambda = \sqrt{\frac{2a}{a}}\)
The correct answer is:
Option 1: \(\sqrt{\frac{2a}{a}}\)
At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/m³, which is dimensionally incorrect for a spectral density. The correct unit J/(m³·Hz) or J·s/m³ is used here for the solution.)