Step 1: Conservation of momentum.
In a completely inelastic collision, momentum is conserved: \[ \vec{p}_{\text{initial}} = \vec{p}_{\text{final}} \] Final momentum \(= (m + 2m) \cdot \frac{v}{3} = m v\).
Step 2: Initial momentum components.
Magnitude of resultant momentum before collision: \[ |\vec{p}_i| = \sqrt{(mv)^2 + (2m \cdot \frac{v}{2})^2 + 2(mv)(mv)\cos\theta} \] Simplify: \[ m v = m v \sqrt{1 + 1 + 2\cos\theta} \Rightarrow 1 = \sqrt{2(1 + \cos\theta)} \] \[ \Rightarrow 1 = \sqrt{4\cos^2(\theta/2)} \Rightarrow \cos(\theta/2) = \frac{1}{2} \Rightarrow \theta = 120^\circ \]
Step 3: Conclusion.
The angle between their initial velocity vectors is \(120^\circ.\)



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.)