Step 1: Understanding the concept.
The electrostatic potential energy of a system of charges is the sum of the potential energies for all distinct pairs of charges. For two point charges \(q_1\) and \(q_2\) separated by a distance \(r\), the potential energy is
\[
U = \frac{1}{4\pi \varepsilon_0} \frac{q_1 q_2}{r}
\]
Step 2: Apply to the given system.
In an equilateral triangle, all three sides are equal to \(L\).
There are 3 distinct pairs of charges: (1,2), (2,3), and (3,1).
Hence, the total potential energy is the sum of potential energies of these three pairs:
\[
U = 3 \times \frac{1}{4\pi \varepsilon_0} \frac{q^2}{L}
\]
Step 3: Simplify the expression.
\[
U = \frac{3}{4\pi \varepsilon_0} \frac{q^2}{L}
\]
Step 4: Conclusion.
The electrostatic potential energy of three identical charges at the vertices of an equilateral triangle is \(\dfrac{3q^2}{4\pi \varepsilon_0 L}\).

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.)