Using Stefan-Boltzmann law, the power radiated by a body is given by:
\[
E = \sigma A T^4
\]
where \( \sigma \) is the Stefan-Boltzmann constant, \( A \) is the surface area, and \( T \) is the temperature.
1. Surface Area of the Sphere:
The total surface area of the sphere is:
\[
A_{\text{sphere}} = 4\pi R^2
\]
The energy radiated per second by the sphere:
\[
E_{\text{sphere}} = \sigma (4\pi R^2) T^4
\]
2. Surface Area of One Hemisphere:
Each hemisphere consists of:
- A curved surface of area \( 2\pi R^2 \)
- A flat circular base of area \( \pi R^2 \)
So, the total surface area of one hemisphere is:
\[
A_{\text{hemisphere}} = 2\pi R^2 + \pi R^2 = 3\pi R^2
\]
The energy radiated per second by one hemisphere:
\[
E_{\text{hemisphere}} = \sigma (3\pi R^2) T^4
\]
3. Ratio of Energies:
\[
\frac{E_{\text{hemisphere}}}{E_{\text{sphere}}} = \frac{3\pi R^2}{4\pi R^2} = \frac{3}{4}
\]
Hence, the required ratio is \( 3:4 \).
Thus, the correct answer is \(\boxed{3:4}\).