To solve the problem, we will use the photoelectric equation:
E_{k} = h \nu - h \nu_0
where:
First, we need to calculate the threshold frequency \nu_0 and the frequency \nu of the incident light using the formula:
\nu = \frac{c}{\lambda}
Given:
Step 1: Calculate \nu_0
\nu_0 = \frac{c}{\lambda_0} = \frac{3 \times 10^8}{3250 \times 10^{-10}} = \frac{3}{32.5} \times 10^{15} \approx 0.0923 \times 10^{15} Hz
Step 2: Calculate \nu
\nu = \frac{c}{\lambda} = \frac{3 \times 10^8}{2536 \times 10^{-10}} = \frac{3}{25.36} \times 10^{15} \approx 0.1183 \times 10^{15} Hz
Step 3: Calculate the kinetic energy E_{k}
E_{k} = h(\nu - \nu_0) = 4.14 \times 10^{-15} \times (0.1183 - 0.0923) \times 10^{15} eV
E_{k} = 4.14 \times 10^{-15} \times 0.026 \times 10^{15} = 0.10764 eV
Step 4: Convert the kinetic energy into velocity:
Using the relation E_{k} = \frac{1}{2} m v^2, where m = 9.11 \times 10^{-31} kg (mass of electron), we get:
0.10764 \, eV = \frac{1}{2} \times 9.11 \times 10^{-31} \times v^2
Convert E_{k} from eV to Joules:
0.10764 \, eV = 0.10764 \times 1.6 \times 10^{-19} \, J
v^2 = \frac{2 \times 0.10764 \times 1.6 \times 10^{-19}}{9.11 \times 10^{-31}}
Calculate v:
v = \sqrt{\frac{2 \times 0.10764 \times 1.6 \times 10^{-19}}{9.11 \times 10^{-31}}} = \sqrt{3.778 \times 10^{11}} \approx 6.14 \times 10^5 \, ms^{-1}
The closest option is \approx 6 \times 10^5 \, ms^{-1}.