Concept:
From Einstein’s photoelectric equation, the maximum kinetic energy of the emitted electrons depends solely on the \textit{frequency} of the incident radiation and is independent of its intensity.
\[
K_{\max} = h\nu - \phi
\]
When radiation contains more than one frequency component, the maximum kinetic energy is governed by the \textit{highest frequency} present in the incident electromagnetic wave.
Step 1: Determine frequencies from the given electric field
The electric field is expressed as:
\[
E = 60[\sin(3 \times 10^{14} t) + \sin(12 \times 10^{14} t)]
\]
Hence, the angular frequencies are:
\[
\omega_1 = 3 \times 10^{14}, \quad \omega_2 = 12 \times 10^{14}
\]
The maximum angular frequency is:
\[
\omega_{\max} = 12 \times 10^{14}
\]
Step 2: Convert angular frequency to ordinary frequency
\[
\nu = \frac{\omega}{2\pi}
\]
\[
\nu_{\max} = \frac{12 \times 10^{14}}{2\pi}
\]
Step 3: Compute the photon energy
Using Planck’s constant $h = 4.14 \times 10^{-15}$ eV·s:
\[
E_{\max} = h\nu_{\max} = \frac{4.14 \times 10^{-15} \times 12 \times 10^{14}}{2\pi}
\]
\[
E_{\max} \approx 4.96 \text{ eV}
\]
Step 4: Apply Einstein’s photoelectric equation
Given the work function:
\[
\phi = 2.8 \text{ eV}
\]
\[
K_{\max} = E_{\max} - \phi = 4.96 - 2.8
\]
\[
K_{\max} = 2.16 \text{ eV}
\]
Conclusion:
\[
\boxed{K_{\max} = 2.16 \text{ eV}}
\]