Step 1: Write down given data.
\[
V_{CC} = 20\,V, V_{CE} = 14\,V, V_{BE} = 0.7\,V, \beta = 100
\]
\[
R_C = 2\,k\Omega, R_E = 1\,k\Omega
\]
Step 2: Apply KVL to the collector-emitter loop.
\[
V_{CC} = I_C R_C + V_{CE} + I_E R_E
\]
Since \(I_E \approx I_C\):
\[
20 = I_C(2 + 1) \times 10^3 + 14
\]
\[
I_C = \frac{20 - 14}{3000} = 2\,mA
\]
Step 3: Calculate base current.
\[
I_B = \frac{I_C}{\beta} = \frac{2 \times 10^{-3}}{100} = 20\,\mu A
\]
Step 4: Apply KVL to base circuit.
\[
V_{CC} = I_B R_B + V_{BE} + I_E R_E
\]
\[
20 = 20 \times 10^{-6} R_B + 0.7 + 2 \times 10^{-3} \times 10^3
\]
\[
20 = 20 \times 10^{-6} R_B + 0.7 + 2
\]
\[
R_B = \frac{17.3}{20 \times 10^{-6}} = 865 \times 10^3 = 865\,k\Omega
\]
Hence, approximately \(R_B = 865\,k\Omega\).
Step 5: Conclusion.
The required base resistor is \(R_B = 865\,k\Omega\).

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.)