A curve is given by $\vec{r}(t)=t\hat{i}+t^{2}\hat{j}+t^{3}\hat{k}$. The unit vector of the tangent at $t=1$ is
Step 1: Find the tangent vector.
$\vec{r}'(t) = \frac{d}{dt}(t, t^{2}, t^{3}) = (1, 2t, 3t^{2})$.
Step 2: Evaluate at $t=1$.
$\vec{r}'(1) = (1,2,3)$.
Step 3: Convert to unit vector.
Magnitude $= \sqrt{1^{2}+2^{2}+3^{2}}=\sqrt{14}$.
Unit tangent $= \dfrac{1}{\sqrt{14}}(1,2,3)$.
Step 4: Conclusion.
The required unit tangent vector is $\dfrac{\hat{i}+2\hat{j}+3\hat{k}}{\sqrt{14}}$.

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.)