The coefficient of restitution, \( e \), is the ratio of velocities after and before the collision. For a ball dropped from a height \( h \), the time between successive bounces is proportional to \( \sqrt{h} \).
The total time \( T \) is proportional to:
\[ T \propto \sum_{n=0}^\infty e^n = \frac{1}{1 - e}, \quad \text{for } 0 < e < 1 \]
When adding the effect of the initial drop time and the bounce heights, the proportionality constant includes \( 1 + e \) in the numerator and \( 1 - e \) in the denominator:
\[ T \propto \frac{1 + e}{1 - e} \]
Thus, the total time taken by the ball to stop bouncing is proportional to \( \frac{1 + e}{1 - e} \).
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/mΒ³, which is dimensionally incorrect for a spectral density. The correct unit J/(mΒ³Β·Hz) or JΒ·s/mΒ³ is used here for the solution.)