Concept:
•Photoelectric equation:
\[
E = \phi + K_{\text{max}}
\]
•Motion in magnetic field:
\[
r = \frac{mv}{eB} \Rightarrow v = \frac{eBr}{m}
\]
•Kinetic energy:
\[
K = \frac{1}{2}mv^2 = \frac{e^2 B^2 r^2}{2m}
\]
Step 1: Given data
\[
\lambda = 2475\,\text{\AA}, \quad r = 1\,\text{m}
\]
\[
B = \frac{1}{\sqrt{17}} \times 10^{-5}\,\text{T}, \quad \frac{e}{m} = 1.7 \times 10^{11}
\]
Step 2: Kinetic energy (in eV)
\[
K(\text{eV}) = \frac{1}{2} \cdot \frac{e}{m} \cdot B^2 r^2
\]
\[
B^2 = \frac{1}{17} \times 10^{-10}
\]
\[
K = \frac{1}{2} \times 1.7 \times 10^{11} \times \frac{1}{17} \times 10^{-10}
\]
\[
= \frac{1}{2} \times 0.1 \times 10 = 0.5\,\text{eV}
\]
Step 3: Photon energy
\[
E = \frac{12400}{\lambda(\text{\AA})}
= \frac{12400}{2475} \approx 5\,\text{eV}
\]
Step 4: Work function
\[
\phi = E - K = 5 - 0.5 = 4.5\,\text{eV}
\]
Final: 4.5 eV