The photoelectric equation is given by:
\[
K.E = h \nu - \phi
\]
where:
- \( K.E \) is the kinetic energy of the emitted electrons,
- \( h \) is Planck's constant,
- \( \nu \) is the frequency of the incident light,
- \( \phi \) is the work function of the metal.
The stopping potential \( V_0 \) is related to the kinetic energy of the emitted electrons by:
\[
K.E = eV_0
\]
When the frequency of light is \( \nu \), the stopping potential is \( V_0 \), and the equation becomes:
\[
eV_0 = h \nu - \phi
\]
When the frequency of light is \( \frac{\nu}{2} \), the stopping potential becomes \( \frac{V_0}{4} \), and the equation becomes:
\[
e\left(\frac{V_0}{4}\right) = h \left(\frac{\nu}{2}\right) - \phi
\]
Simplifying:
\[
\frac{eV_0}{4} = \frac{h\nu}{2} - \phi
\]
Now, solving the two equations:
1. \( eV_0 = h\nu - \phi \)
2. \( \frac{eV_0}{4} = \frac{h\nu}{2} - \phi \)
By comparing these equations, we can find that the threshold frequency \( \nu_0 \), which is the frequency at which the stopping potential is zero, is:
\[
\nu_0 = \frac{\nu}{2}
\]
Thus, the threshold frequency for photoelectric emission is:
\[
\text{(B) } \frac{\nu}{2}
\]