Give Einstein's equation for photoelectric emission. The work function of a metal is 4.2 eV. Electrons are emitted due to light of wavelength 2000 Å. Find the stopping potential for the emitted electrons.
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Photon energy \( hc/\lambda = 12400/2000 = 6.2\ \text{eV} \); subtract the 4.2 eV work function, and the stopping potential in volts equals the leftover energy in eV.
Step 1: Set up the energy balance. Einstein's equation says a photon's energy splits into the work function plus the electron's kinetic energy: \(h\nu = W + eV_0\), where \(eV_0\) is the energy needed to stop the fastest electron. Rearranged, \(eV_0 = h\nu - W\).
Step 2: Photon energy in joules. \[E = \frac{hc}{\lambda} = \frac{(6.6\times10^{-34})(3\times10^{8})}{2000\times10^{-10}}\] \[E = \frac{1.98\times10^{-25}}{2\times10^{-7}} = 9.9\times10^{-19}\ \text{J}\]
Step 3: Work function in joules. \[W = 4.2\ \text{eV} = 4.2\times1.6\times10^{-19} = 6.72\times10^{-19}\ \text{J}\]
Step 4: Solve for stopping potential. \[eV_0 = E - W = 9.9\times10^{-19} - 6.72\times10^{-19} = 3.18\times10^{-19}\ \text{J}\] \[V_0 = \frac{3.18\times10^{-19}}{1.6\times10^{-19}} = 1.99\ \text{V} \approx 2.0\ \text{V}\] Working entirely in SI units gives the same result as the electron-volt shortcut.
\[\boxed{V_0 \approx 2.0\ \text{V}}\]
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