Step 1: Radioactive decay relation.
The number of parent nuclei remaining after time \(t\) is given by:
\[
N = N_0 e^{-\lambda t}
\]
and the number of daughter nuclei formed is:
\[
N_D = N_0 - N = N_0 (1 - e^{-\lambda t})
\]
Given isotopic ratio:
\[
\frac{N}{N_D} = 50 $\Rightarrow$ \frac{e^{-\lambda t}}{1 - e^{-\lambda t}} = 50
\]
Step 2: Solve for decay constant term.
\[
e^{-\lambda t} = 50 - 50 e^{-\lambda t} $\Rightarrow$ 51 e^{-\lambda t} = 50 $\Rightarrow$ e^{-\lambda t} = \frac{50}{51}
\]
Step 3: Decay constant.
\[
\lambda = \frac{\ln 2}{t_{1/2}} = \frac{0.693}{1.25 \times 10^9} = 5.544 \times 10^{-10}\, \text{yr}^{-1}
\]
Step 4: Substitute to find \(t\).
\[
-\lambda t = \ln{\frac{50}{51}} = -0.0198 $\Rightarrow$ t = \frac{0.0198}{5.544 \times 10^{-10}} = 3.57 \times 10^7\, \text{years}
\]
\[
m = 3.57
\]
Step 5: Conclusion.
Hence, the age of the rock is \(3.57 \times 10^7\, \text{years}\), i.e., \(m = 3.57.\)
The half-life of a radioactive nucleus is 5 years. The fraction of the original sample that would decay in 15 years is:

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.)