Problem 20
Question
Light of wavelength \(488 \mathrm{~nm}\) is produced by an argon laser, which is used in the photoelectric effect. When light from this spectral line is incident on the emitter, the stopping (cut-off) potential of photoelectrons is \(0.38 \mathrm{~V}\). Find the work function of the material from which the emitter is made. (a) \(2.2 \mathrm{eV}\) (b) \(3.7 \mathrm{eV}\) (c) \(1.6 \mathrm{eV}\) (d) \(4.2 \mathrm{eV}\)
Step-by-Step Solution
Verified Answer
The work function is (a) 2.2 eV.
1Step 1: Convert Wavelength to Frequency
First, we need to calculate the frequency of the light using its wavelength. The speed of light \(c\) is \(3 \times 10^8 \text{ m/s}\), and the wavelength \(\lambda\) is given as \(488\text{ nm}\). Convert the wavelength to meters: \(488\text{ nm} = 488 \times 10^{-9}\text{ m}\). The formula for frequency \(f\) is \(f = \frac{c}{\lambda}\). Substituting the known values,\[f = \frac{3 \times 10^8 \text{ m/s}}{488 \times 10^{-9} \text{ m}} = 6.15 \times 10^{14} \text{ Hz}\]
2Step 2: Calculate the Photon Energy
Using the frequency calculated in the previous step, we find the energy of one photon using Planck's constant \(h = 6.626 \times 10^{-34} \text{ J s}\). The formula for energy \(E\) is \(E = hf\). Thus,\[E = (6.626 \times 10^{-34} \text{ J s})(6.15 \times 10^{14} \text{ Hz}) = 4.075 \times 10^{-19} \text{ J}\]Convert this energy into electronvolts (1 eV = \(1.602 \times 10^{-19}\) J):\[E = \frac{4.075 \times 10^{-19} \text{ J}}{1.602 \times 10^{-19} \text{ J/eV}} = 2.54 \text{ eV}\]
3Step 3: Use the Photoelectric Equation
The photoelectric equation is given by:\[E_{photon} = \text{Work Function (}\phi\text{)} + eV_{stop}\]where \(e\) is the charge of an electron \(1.602 \times 10^{-19} \text{ C}\), and \(V_{stop}\) is the stopping potential \(0.38\text{ V}\). So \(eV_{stop}\) in eV is simply \(0.38 \text{ eV}\) because \(1 V \cdot e = 1 eV\). From the equation:\[2.54 = \phi + 0.38\]
4Step 4: Solve for Work Function
Rearrange the equation to find the work function (\(\phi\)):\[\phi = 2.54 - 0.38 = 2.16 \text{ eV}\]Which rounds to \(2.2 \text{ eV}\).
5Step 5: Match the Answer with Choices
The calculated work function \(2.16 \text{ eV}\) rounds to \(2.2 \text{ eV}\), matching option (a). Therefore, the work function of the material is \(2.2 \text{ eV}\).
Key Concepts
Wavelength ConversionPhoton Energy CalculationWork Function Determination
Wavelength Conversion
Understanding wavelength conversion is a fundamental step in many physics problems involving light. Wavelength is typically measured in nanometers (nm) when dealing with visible light, as it is in the original exercise where we have a wavelength of 488 nm. However, to perform calculations involving speed and frequency, it is necessary to convert this measurement into meters. This is because the speed of light, denoted as \( c \), is given in meters per second (\( m/s \)). The conversion is straightforward: multiply the wavelength in nanometers by \( 10^{-9} \) to convert to meters.
- In our example: \( 488 \text{ nm} = 488 \times 10^{-9} \text{ m} \).
Photon Energy Calculation
Once the frequency \( f \) of light is known, the next step is to determine the energy possessed by each photon of that light. This is done using Planck's formula, \( E = hf \), where \( h \) is Planck's constant \( (6.626 \times 10^{-34} \text{ Js}) \). Calculate this energy in Joules first because that's the standard SI unit.
- For our frequency: \( E = (6.626 \times 10^{-34} \text{ J s})(6.15 \times 10^{14} \text{ Hz}) = 4.075 \times 10^{-19} \text{ J} \).
- \( E = \frac{4.075 \times 10^{-19} \text{ J}}{1.602 \times 10^{-19} \text{ J/eV}} = 2.54 \text{ eV} \).
Work Function Determination
The work function of a material is the minimum energy required to eject an electron from its surface due to the absorption of a photon. This is essential for understanding the photoelectric effect because only photons with energy exceeding this threshold will release electrons. The equation at the heart of this is the photoelectric equation: \( E_{photon} = \text{Work Function (}\phi\text{)} + eV_{stop} \), where \( eV_{stop} \) is the energy equivalent of the stopping potential.
- Given that we have already calculated the photon energy \( E_{photon} \) as 2.54 eV and \( eV_{stop} \) as 0.38 eV (since \( 1 V \cdot e = 1 eV \)), substituting these values in gives: \[ 2.54 = \phi + 0.38 \].
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